Version 2

INSPEC search: cPbL Aug 12 2000
 Find AUTHOR INAN, U.S. or AUTHOR INAN, U. S. or AUTHOR INAN,
   U.            

272 citations

CAUTION!!!!!!!!! Inan first-authored two papers in May 1996 in GRL.
One should be called Inan1May96 and the other Inan15May96!!

Also, corrected quotes in "early/fast" title.


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/usr/tmp/citation.tmp.28355
@ARTICLE{SalvatiMar00,
	author={Salvati, M.A. and Inan, U.S. and Rosenberg, T.J. and Weatherwax, A.T.},
	title={
Solar wind control of polar chorus
	},
	journal={Geophysical Research Letters},
	volume={27},
	number={5},
	year={2000},
	month={Mar},
	pages={649-52},
	abstract={
The intensity of chorus as observed at several high latitude ground
stations in the Antarctic is highly correlated with the solar wind dynamic
pressure exerted on the magnetopause boundary. In two different cases,
intense chorus and associated precipitation measured as riometer absorption
were abruptly interrupted by several minutes of deep quieting. Satellite
measurements of solar wind dynamic pressure showed the intensity of chorus
to rapidly respond to magnetospheric compression and relaxation over an
extended region as evidenced by the fact the effect was observed at
multiple sites
	},
	keywords={
		atmospheric radiation
		magnetosphere
		solar wind
		magnetosphere
		radiowave emission
		plasma wave
		polar chorus
		solar wind control
		solar wind interaction
		solar wind magnetosphere interaction
		intensity
		high latitude
		Antarctic
		dynamic pressure
		magnetopause boundary
		intense chorus
		associated precipitation
		deep quieting
		magnetospheric compression
		relaxation
		AD 1997 02 23
		AD 1997 04 11
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PaskoFeb00,
	author={Pasko, V.P. and Inan, U.S. and Bell, T.F.},
	title={
Fractal structure of sprites
	},
	journal={Geophysical Research Letters},
	volume={27},
	number={4},
	year={2000},
	month={Feb},
	pages={497-500},
	abstract={
A large scale model of sprites based on a phenomenological probabilistic
approach to modeling of streamer corona discharges is developed. The model
utilizes the experimentally documented macroscopic properties of positive
and negative streamer coronas in air and allows a realistic determination
of the propagation of multiple breakdown branches in a self-consistent
electric field. The model results reproduce the large scale volumetric
shapes of sprites, agree with the experimentally documented thundercloud
charge moment changes in sprites producing cloud to ground lightning
discharges (CGs), and demonstrate fundamental asymmetries between sprites
generated by CGs of positive and negative polarity
	},
	keywords={
		fractals
		ionospheric disturbances
		lightning
		thunderstorms
		fractal structure
		sprites
		streamer corona discharges
		macroscopic properties
		multiple breakdown branches
		self-consistent electric field
		large scale volumetric shapes
		thundercloud charge moment changes
		cloud to ground lightning discharges
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SampathJan00,
	author={Sampath, H.T. and Inan, U.S. and Johnson, M.P.},
	title={
Recovery signatures and occurrence properties of lightning-associated
subionospheric VLF perturbations
	},
	journal={Journal of Geophysical Research},
	volume={105},
	number={A1},
	year={2000},
	month={Jan},
	pages={183-91},
	abstract={
Subionospheric VLF signatures of lightning-associated ionospheric
disturbances observed at multiple sites in the central United States are
used to investigate the occurrence properties and recovery signatures of
characteristic perturbations exhibiting rapid onset followed by slow
recoveries. The two different types of events, so-called early/fast and
lightning-induced electron precipitation (LEP) [Inan et al., 1996], are
distinguished by the lack of presence of a few hundred millisecond delay
between VLF event onsets and causative lightning discharges, respectively.
Analysis of recovery signatures of the two types of events indicate subtle
but distinct differences in the recovery rates. A majority of early/fast
events were found to exhibit a more rapid initial recovery to pre-event
levels during the first 20 s of recovery, when compared to LEP events. This
experimental evidence indicates that the physical nature of the ionospheric
disturbance involved in the two classes of events are different, consistent
with a theoretical suggestion [Inan et al., 1996]. The occurrence
properties of early/fast events observed by the Holographic Array for
Ionospheric Lighting (HAIL) receivers indicate that ionospheric
disturbances act primarily as forward scatterers
	},
	keywords={
		atmospheric electron precipitation
		atmospherics
		ionospheric disturbances
		lightning
		recovery signatures
		occurrence properties
		lightning-associated subionospheric VLF perturbations
		lightning-associated ionospheric disturbances
		central United States
		lightning-induced electron precipitation
		delay
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{ErgunJan00,
	author={Ergun, R.E. and Larson, D.E. and Phan, T. and Taylor, D. and Bale, S. and Carlson, C.W. and Roth, I. and Angelopoulos, V. and Raeder, J. and Bell, T. and Inan, U.S. and Bougeret, J.-L. and Manning, R.},
	title={
Feasibility of a multisatellite investigation of the Earth's magnetosphere
with radio tomography
	},
	journal={Journal of Geophysical Research},
	volume={105},
	number={A1},
	year={2000},
	month={Jan},
	pages={361-73},
	abstract={
Describes the scientific motivation, basic principles, and feasibility of a
relatively new measurement technique, radio tomography, and shows how it
can be used to investigate the Earth's magnetosphere. The authors
demonstrate that a multisatellite radio tomography experiment can produce
two-dimensional images of plasma density in the Earth's magnetosphere at
sufficient spatial (1/2 R/sub E/) and temporal (À10 s) resolution to
address key problems of magnetospheric physics. The imaging technique
incorporates well-established radio science methods and computed
tomography. Several coplanar satellites are required in orbits that
encompass the imaged area. The authors suggest that the large-scale images
are more valuable when combined with in situ observations, supporting an
unambiguous interpretation of the in situ data and an investigation of the
interdependence of small- and large-scale plasma processes
	},
	keywords={
		atmospheric techniques
		magnetosphere
		magnetospheric electromagnetic wave propagation
		tomography
		Earth magnetosphere
		measurement technique
		multisatellite radio tomography experiment
		magnetospheric physics
		imaging technique
		radio science methods
		coplanar satellites
		large-scale images
		in-situ observations
		plasma processes
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BellJan00,
	author={Bell, T.F. and Inan, U.S. and Helliwell, R.A. and Scudder, J.D.},
	title={
Simultaneous triggered VLF emissions and energetic electron distributions
observed on POLAR with PWI and HYDRA
	},
	journal={Geophysical Research Letters},
	volume={27},
	number={2},
	year={2000},
	month={Jan},
	pages={165-8},
	abstract={
The authors report simultaneous observations of energetic 1-20 keV
electrons and VLF emissions triggered within the plasmasphere by pulses
from ground based VLF transmitters, using the PWI and HYDRA instruments on
the POLAR spacecraft. The 1-20 keV electrons have the correct energy to
interact with the input pulses through gyroresonance. Emissions are
generated by the pulses only when the particle flux is enhanced well above
background and the particle pitch angle distribution is very highly
anisotropic, with the average equatorial pitch angle exceeding À75 degrees
. Because of these high pitch angles, the particles are trapped typically
within 7 degrees of the magnetic equator. Only pulses which propagate
within whistler mode ducts are observed to trigger emissions. The observed
pitch angle anisotropies are much larger than those assumed in present
models of the VLF emission triggering phenomenon, and thus the authors'
observations provide a starting point for understanding the emission
process
	},
	keywords={
		atmospheric radiation
		magnetosphere
		magnetosphere
		radiowave emission
		VLF
		triggered emission
		energetic electron distribution
		POLAR
		PWI
		HYDRA
		plasmasphere
		ground based VLF transmitter
		radiowave excitation
		gyroresonance
		particle pitch angle distribution
		equatorial pitch angle
		whistler mode duct
		pitch angle anisoptropy
		radiowave heating experiment
		AD 1996
		AD 1997
		1 to 20 keV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{Barrington-LeighDec99,
	author={Barrington-Leigh, C.P. and Inan, U.S. and Stanley, M. and Cummer, S.A.},
	title={
Sprites triggered by negative lightning discharges
	},
	journal={Geophysical Research Letters},
	volume={26},
	number={24},
	year={1999},
	month={Dec},
	pages={3605-8},
	abstract={
High altitude air breakdown, manifested as "red sprites", is reported in
close association with negative cloud-to-ground lightning (-CG) on at least
two occasions above an unusual storm on August 29, 1998. Data from high
speed photometry, low-light-level video, and receivers of lightning
electromagnetic signatures in the frequency range 10 Hz to 20 kHz are used
to establish the association and indicate that the causative -CG discharges
effected unusually large vertical charge moment changes ( Delta M/sub Qv/)
of up to 1550 C.km in 5 ms. The existence of sprites caused by -CG events,
rather than the regularly associated +CG events, has immediate implications
for sprite models and observations
	},
	keywords={
		atmospheric electricity
		ionospheric disturbances
		lightning
		photometry
		negative lightning discharges
		sprite triggering
		high altitude air breakdown
		red sprites
		negative cloud-to-ground lightning
		AD 1998 08 29
		high speed photometry
		low-light-level video
		lightning EM signatures
		vertical charge moment changes
		sprite models
		sprite observations
		N Gulf of California
		Mexico
		10 Hz to 20 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{JohnsonDec99,
	author={Johnson, M.P. and Inan, U.S. and Lauben, D.S.},
	title={
Subionospheric VLF signatures of oblique (nonducted) whistler-induced
precipitation
	},
	journal={Geophysical Research Letters},
	volume={26},
	number={23},
	year={1999},
	month={Dec},
	pages={3569-72},
	abstract={
Subionospheric very low frequency (VLF) signal perturbations observed at
multiple sites in association with individual lightning discharges exhibit
onset delays which steadily increase with increasing L-value. The timing of
the onsets and the inferred spatial extent (À1000 km) of the ionospheric
disturbance are consistent with those expected for electron precipitation
induced by obliquely propagating (i.e., nonducted) whistlers
	},
	keywords={
		atmospheric electron precipitation
		ionospheric electromagnetic wave propagation
		magnetospheric electromagnetic wave propagation
		radiation belts
		whistlers
		magnetosphere
		radiation belt
		radiowave propagation
		whistler
		subionospheric signature
		VLF signature
		nonducted whistler-induced precipitation
		oblique whistler-induced precipitation
		trapped particle
		wave particle interaction
		EM wave
		onset delay
		L-value
		spatial extent
		timing
		ionospheric disturbance
		electron precipitation
		obliquely propagating whistler
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{DemirkolDec99,
	author={Demirkol, M.K. and Inan, U.S. and Bell, T.F. and Kanekal, S.G. and Wilkinson, D.C.},
	title={
Ionospheric effects of relativistic electron enhancement events
	},
	journal={Geophysical Research Letters},
	volume={26},
	number={23},
	year={1999},
	month={Dec},
	pages={3557-60},
	abstract={
The relativistic electron population as measured both at geosynchronous
orbit and at low altitudes at subauroral latitudes exhibits pronounced
fluctuations in association with magnetospheric substorm and solar
activity. A ground-satellite correlative study based on amplitude and phase
measurements of VLF signals propagating in the Earth-ionosphere waveguide
indicates that the relativistic electron enhancements are accompanied by
similar enhancements in nighttime ionospheric conductivity produced by
associated enhanced precipitation. VLF signal amplitudes are found to
exhibit >10 dB changes, showing the same 27 day cycle and 2-3 day rise and
fall time pattern as relativistic electron enhancement events recorded by
GOES 7 and SAMPEX, and indicating that the nighttime lower ionospheric
electron density at subauroral latitudes is detectably affected by 27-day
periodicity in solar rotation
	},
	keywords={
		atmospheric electron precipitation
		ionosphere
		ionospheric disturbances
		ionospheric electromagnetic wave propagation
		ionosphere magnetosphere interaction
		ionospheric effect
		relativistic electron enhancement event
		subauroral latitude
		fluctuations
		substorm
		solar activity
		magnetic storm
		ionospheric disturbance
		VLF signal
		Earth-ionosphere waveguide
		night
		nighttime
		electrical conductivity
		enhanced precipitation
		elecron precipitation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanNov99,
	author={Inan, U.S. and Lehtinen, N.G. and Lev-Tov, S.J. and Johnson, M.P. and Bell, T.F. and Hurley, K.},
	title={
Ionization of the lower ionosphere by gamma -rays from a magnetar:
detection of a low energy (3-10 keV) component
	},
	journal={Geophysical Research Letters},
	volume={26},
	number={22},
	year={1999},
	month={Nov},
	pages={3357-60},
	abstract={
A gigantic periodic flare from the soft gamma repeater SGR 1900+14 produced
enhanced ionization at ionospheric altitudes of 30 to 90 km, which was
observed as unusually large amplitude and phase changes of very low
frequency (VLF) signals propagating in the Earth-ionosphere waveguide. The
VLF signals remained perturbed for À5 min and exhibited the 5.16 s
periodicity of the giant flare detected on the Ulysses spacecraft (Hurley
et al., 1999). Quantitative analysis indicates the presence of an intense
initial low energy (3-10 keV) photon component that was not detectable by
the Ulysses instrument
	},
	keywords={
		atmospheric ionisation
		gamma-ray effects
		gamma-ray sources (astronomical)
		ionospheric disturbances
		lower ionosphere ionization
		gamma -rays
		magnetars
		low energy component detection
		gigantic periodic flare
		soft gamma -ray repeater
		enhanced ionization
		ionospheric altitudes
		VLF signals
		low energy photon component
		30 to 90 km
		5.16 s
		3 to 10 keV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{LehtinenNov99,
	author={Lehtinen, N.G. and Bell, T.F. and Inan, U.S.},
	title={
Monte Carlo simulation of runaway MeV electron breakdown with application
to red sprites and terrestrial gamma ray flashes
	},
	journal={Journal of Geophysical Research},
	volume={104},
	number={A11},
	year={1999},
	month={Nov},
	pages={24699-712},
	abstract={
A three-dimensional Monte Carlo model of the uniform relativistic runaway
electron breakdown in air in the presence of static electric and magnetic
fields is used to calculate electron distribution functions, avalanche
rates, and the direction and velocity of avalanche propagation. The authors
also derive the conditions required for an electron with a given momentum
to start an avalanche in the absence of a magnetic field. The results are
compared to previously developed kinetic and analytical models and their
own analytical estimates, and it is concluded that the rates used in many
early models [e.g., Lehtinen et al., 1997; Taranenko and Roussel-Dupre,
1996; Yukhimuk et al., 1998; Roussel-Dupre et al., 1998] are overestimated
by a factor of À10. The Monte Carlo simulation results are applied to a
fluid model of runaway electron beams in the middle atmosphere accelerated
by quasi-electrostatic fields following a positive lightning stroke. In
particular, the authors consider the case of lightning discharges which
drain positive charge from remote regions of a laterally extensive (>100
km) thundercloud, using a Cartesian two-dimensional model. The resulting
optical emission intensities in red sprites associated with the runaway
electrons are found to be negligible compared to the emissions from thermal
electrons heated in the conventional type of breakdown. The calculated
gamma ray flux is of the same order as the terrestrial gamma ray flashes
observed by the Burst and Transient Source Experiment detector on the
Compton Gamma Ray Observatory
	},
	keywords={
		atmospheric electricity
		atmospheric radiation
		gamma-rays
		lightning
		mesosphere
		mesosphere
		middle atmosphere
		electric discharge
		electricity
		electric breakdown
		model
		Monte Carlo simulation
		runaway MeV electron breakdown
		red sprite
		gamma ray flash
		gamma-ray emission
		lightning
		three-dimensional model
		gamma-rays
		relativistic runaway
		electron distribution function
		avalanche rate
		propagation velocity
		propagation direction
		quasi-electrostatic field
		optical emission
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{LaubenAug99,
	author={Lauben, D.S. and Inan, U.S. and Bell, T.F.},
	title={
Poleward-displaced electron precipitation from lightning-generated oblique
whistlers
	},
	journal={Geophysical Research Letters},
	volume={26},
	number={16},
	year={1999},
	month={Aug},
	pages={2633-6},
	abstract={
New simulation results show that obliquely propagating lightning-generated
whistlers which fill vast volumes of the magnetosphere readily induce
significant energetic electron precipitation over large regions of the
ionosphere, depositing appreciable energy flux to the upper atmosphere at
locations substantially poleward of the lightning source. These results
provide a new interpretation for the observed spatial relationships between
lightning discharges and subsequently disturbed ionospheric regions
inferred from subionospheric signal perturbations (i.e. Trimpi-events)
reported in several lightning-induced electron precipitation (LEP) studies
	},
	keywords={
		atmospheric electron precipitation
		magnetospheric electromagnetic wave propagation
		whistlers
		magnetosphere
		radiowave propagation
		poleward displaced electron precipitation
		lightning-generated oblique whistlers
		whistler
		simulation
		obliquely propagating
		oblique propagation
		ionosphere
		poleward displacement
		lightning
		wave particle interaction
		Trimpi-event
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{JohnsonAug99,
	author={Johnson, M.P. and Inan, U.S. and Lev-Tov, S.J. and Bell, T.F.},
	title={
Scattering pattern of lightning-induced ionospheric disturbances associated
with early/fast VLF events
	},
	journal={Geophysical Research Letters},
	volume={26},
	number={15},
	year={1999},
	month={Aug},
	pages={2363-6},
	abstract={
Simultaneous observations of early/fast very low frequency (VLF) events at
nine closely spaced (À65 km) sites are used together with a numerical model
of the propagation and scattering of VLF signals in the Earth-ionosphere
waveguide to directly measure the scattering pattern of associated
ionospheric disturbances. In cases when the causative lightning is within
700 km of the north-south array of observing sites, early/fast VLF events
are typically observed at no more than 2 or 3 sites, which indicates a
narrow beam of the scattered signal in the forward direction. In the
different cases studied, forward scattering patterns exhibit 15 dB
beamwidths of less than 30 degrees consistent with horizontal extent of
90+or-30 km
	},
	keywords={
		atmospherics
		Earth-ionosphere waveguide
		electromagnetic wave scattering
		ionospheric disturbances
		lightning
		scattering pattern
		lightning-induced ionospheric disturbances
		early/fast VLF events
		fast VLF events
		propagation
		scattering
		Earth-ionosphere waveguide
		ionospheric disturbances
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PaskoMay99,
	author={Pasko, V.P. and Inan, U.S. and Bell, T.F.},
	title={
Mesospheric electric field transients due to tropospheric lightning
discharges
	},
	journal={Geophysical Research Letters},
	volume={26},
	number={9},
	year={1999},
	month={May},
	pages={1247-50},
	abstract={
A physical picture and quantitative two-dimensional electromagnetic
modeling of mesospheric electric field transients produced by
cloud-to-ground (CG) lightning discharges with short duration currents
(<0.5 ms) are presented. The range of applicability of existing
quasi-electrostatic models of sprites and the physical conditions under
which relatively weak CG lightning discharges (thundercloud charge moment
changes less than 50 C *10 km) may initiate sprites are discussed in the
context of experimental findings
	},
	keywords={
		atmospheric electricity
		lightning
		mesosphere
		mesospheric electric field transients
		tropospheric lightning discharges
		2D EM modelling
		cloud-to-ground lightning discharges
		short duration currents
		quasi-electrostatic models
		sprites
		thundercloud charge moment changes
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{VeronisJun99,
	author={Veronis, G. and Pasko, V.P. and Inan, U.S.},
	title={
Characteristics of mesospheric optical emissions produced by lightning
discharges
	},
	journal={Journal of Geophysical Research},
	volume={104},
	number={A6},
	year={1999},
	month={Jun},
	pages={12645-56},
	abstract={
A new 2D cylindrically symmetric EM model of the lightning-ionosphere
interaction includes effects of both the lightning radiated EM pulses (EMP)
and the quasi-electrostatic (QE) fields, thus allowing effective studies of
lightning-ionosphere interactions on time scales ranging from several
microseconds to tens of milliseconds. The temporal and spatial evolution of
the electric field, lower ionospheric electron density, and optical
emissions calculated with the new model are used to investigate
theoretically the effects of the lightning return stroke current waveform
and of the observational geometry on the optical signals observed with a
photometer. For typical lightning discharges of À100 mu s duration the
ionospheric response is dominated by the EMP-induced heating leading to the
highly transient and laterally expanding optical flashes known as elves.
The optical signal characteristics are found to be highly sensitive to both
the observational geometry and the current waveform. The onset delay with
respect to the lightning discharge, the duration, and the peak magnitude of
optical emissions are highly dependent on the elevation and azimuth angles
of field of view of individual photometric pixels. The shape of the optical
signal clearly reflects the source current waveform. For a waveshape with
risetime of À50 mu s or longer a double-pulse shape of the photometric
signal is observed. For cloud to ground lightning discharges of À1 ms
duration removing substantial amount of charge, heating and ionization
changes induced by the QE field lead to the mesospheric luminous glows with
lateral extent <100 km, referred to as sprites
	},
	keywords={
		atmospheric radiation
		atmospheric temperature
		electromagnetic pulse
		electron density
		ionospheric disturbances
		lightning
		mesosphere
		mesospheric optical emissions
		lightning discharges
		2D cylindrically symmetric electromagnetic model
		lightning-ionosphere interaction
		EM pulses
		quasi-electrostatic fields
		time scales
		temporal evolution
		spatial evolution
		lower ionospheric electron density
		lightning return stroke current waveform
		observational geometry
		EMP-induced heating
		optical flashes
		elves
		onset delay
		duration
		source current waveform
		risetime
		double-pulse shape
		photometric signal
		ionization changes
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{ReisingApr99,
	author={Reising, S.C. and Inan, U.S. and Bell, T.F.},
	title={
ELF sferic energy as a proxy indicator for sprite occurrence
	},
	journal={Geophysical Research Letters},
	volume={26},
	number={7},
	year={1999},
	month={Apr},
	pages={987-90},
	abstract={
Broadband ELF/VLF measurements of sferics near Ft. Collins, Colorado,
demonstrate that ELF sferic energy is a proxy for sprite occurrence which
can be used to estimate the number of sprites produced by a thunderstorm.
Ultra-long range (À12000 km) measurements at Palmer Station, Antarctica,
confirm the application of this proxy to storms where no video observations
of sprites are available. Comparison with high-resolution photometer
measurements demonstrate the simultaneity of sprite luminosity and an ELF
"second pulse" believed to be radiated by electrical currents within the
sprite body (Cummer et al., 1998). Measurements of the second ELF pulse are
used to identify a quantitative relationship between the current in sprites
and total sprite luminosity
	},
	keywords={
		atmospherics
		thunderstorms
		ELF sferic energy
		proxy indicator
		sprite occurrence
		broadband ELF/VLF measurements
		Ft. Collins
		Colorado
		thunderstorms
		ultra-long range measurements
		Palmer Station
		Antarctica
		high-resolution photometer measurements comparison
		electrical currents
		second ELF pulse
		total sprite luminosity
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{Barrington-LeighMar99,
	author={Barrington-Leigh, C.P. and Inan, U.S.},
	title={
Elves triggered by positive and negative lightning discharges
	},
	journal={Geophysical Research Letters},
	volume={26},
	number={6},
	year={1999},
	month={Mar},
	pages={683-6},
	abstract={
Optical flashes in the lower ionosphere due to the transient heating caused
by lightning electromagnetic pulses (EMP) are unambiguously identified with
the Fly's Eye photometric array. Data from a thunderstorm over Mexico
recorded at Langmuir Laboratory on August 27 1997 demonstrate that
relatively common negative cloud-to-ground lightning is a previously
unrecognized major cause of elves. The spatial extent of the transient
heating is shown optically to be typically at least 200-700 km laterally,
indicating the possibility for accumulation of ionization effects produced
by successive flashes within large nighttime thunderstorm systems. One
especially bright event suggests that temporal fine-structure in the
causative very low frequency EMP can manifest itself in the photometric
record of elves
	},
	keywords={
		ionosphere
		lightning
		mesosphere
		thermosphere
		elf
		elves
		optical emission
		upper atmosphere
		thermosphere
		middle atmosphere
		mesosphere
		lightning triggered
		negative lightning discharge
		positive lightning
		lightning
		electric discharge
		optical flash
		lower ionosphere
		transient heating
		lightning electromagnetic pulse
		EMP
		thunderstorm
		storm
		Mexico
		AD 1997 08 27
		negative cloud-to-ground lightning
		cause
		spatial extent
		ionization effec
		temporal fine-structure
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{CummerNov98,
	author={Cummer, S.A. and Inan, U.S. and Bell, T.F.},
	title={
Ionospheric D region remote sensing using VLF radio atmospherics
	},
	journal={Radio Science},
	volume={33},
	number={6},
	year={1998},
	month={Nov},
	pages={1781-92},
	abstract={
Lightning discharges radiate the bulk of their electromagnetic energy in
the very low frequency (VLF, 3-30 kHz) and extremely low frequency (ELF,
3-3000 Hz) bands. This energy, contained in impulse-like signals called
radio atmospherics or sferics is guided for long distances by multiple
reflections from the ground and lower ionosphere. This suggests that
observed sferic waveforms radiated from lightning and received at long
distances (>1000 km) from the source stroke contain information about the
state of the ionosphere along the propagation path. The focus of this work
is on the extraction of nighttime D region electron densities (in the
altitude range of À70-95 km) from observed VLF sferics. In order to
accurately interpret observed sferic characteristics, we develop a model of
sferic propagation which is based on an existing frequency domain
subionospheric VLF propagation code. The model shows that the spectral
characteristics of VLF sferics depend primarily on the propagation path
averaged ionospheric D region electron density profile, covering the range
of electron densities from À10/sup 0/ to 10/sup 3/ cm/sup -3/. To infer the
D region density from observed VLF sferics, we find the electron density
profile that produces a modeled sferic spectrum that most closely matches
an observed sferic spectrum. In most nighttime cases the quality of the
agreement and the uncertainties involved allow the height of an
exponentially varying electron density profile to be inferred with a
precision of À0.2 km
	},
	keywords={
		atmospherics
		D-region
		electron density
		ionospheric electromagnetic wave propagation
		ionospheric techniques
		radiowave propagation
		remote sensing
		ionospheric D-region remote sensing
		VLF radio atmospherics
		lightning discharges
		electromagnetic energy
		VLF
		ELF
		impulse-like signals
		radio atmospherics
		sferics
		multiple reflections
		propagation path
		nighttime D-region electron densities
		frequency domain subionospheric VLF propagation code
		spectral characteristics
		3 Hz to 30 kHz
		70 to 95 km
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{FosterNov98,
	author={Foster, J.C. and Cummer, S. and Inan, U.S.},
	title={
Midlatitude particle and electric field effects at the onset of the
November 1993 geomagnetic storm
	},
	journal={Journal of Geophysical Research},
	volume={103},
	number={A11},
	year={1998},
	month={Nov},
	pages={26359-66},
	abstract={
Millstone Hill incoherent scatter radar elevation scans across midlatitudes
captured the ionospheric response to storm-induced electric field and
precipitation-induced changes near the equatorward extent of the expanding
auroral region during the early phases of the November 3-4, 1993, magnetic
storm. Solar wind-induced magnetospheric compression was observed at À2307
UT [Borovsky et al.] and a prompt, short-duration (10 min) increase in the
upward plasma velocity to >100 m/s at À2319 UT on November 3, 1993 signaled
the onset of the storm-induced enhancement of the east ward electric field
over Millstone Hill in the premidnight sector at 54 degrees invariant
latitude ( Lambda ). This resulted in an uplifting of the F-region
ionosphere above the site by À80 km by 2330 UT. Formation of a narrow
ionospheric trough poleward of the Millstone site accompanied the auroral
convection enhancement at somewhat later times while plasma sheet
precipitation produced the ionization at altitudes between 200 and 300 km
at Lambda <60 degrees observed by the radar. Strong precipitation of
energetic particles from the outer radiation belt was observed by SAMPEX at
58.5 degrees Lambda , near the equatorward limit of the plasmasheet
precipitation observed by DMSP and Millstone Hill. Amplitude perturbations
of VLF signals propagating in the Earth-ionosphere waveguide serve to
localize the energetic radiation belt precipitation to latitudes between 56
degrees Lambda and 58.5 degrees Lambda and provide accurate timing of
storm-induced energetic precipitation, whose onset was at À2332 UT in the
premidnight sector. A later enhancement of the eastward electric field at
latitudes equatorward of Millstone Hill and the storm-induced trough led to
a perturbation of the midlatitude ionosphere to Lambda <40 degrees and is
the subject of a companion paper
	},
	keywords={
		ionosphere
		ionospheric disturbances
		magnetic storms
		ionosphere magnetosphere interaction
		ionospheric disturbance
		middle latitude
		midlatitude particles
		electric field
		onset
		magnetic storm
		geomagnetic storm
		AD 1993 11 03
		AD 1993 11 04
		ionospheric response
		storm-induced electric field
		precipitation-induced change
		expanding auroral region
		F-region
		ionospheric trough
		convection enhancement
		plasma sheet precipitation
		particle precipitation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SmithOct98,
	author={Smith, A.J. and Engebretson, M.J. and Klatt, E.M. and Inan, U.S. and Arnoldy, R.L. and Fukunishi, H.},
	title={
Periodic and quasiperiodic ELF/VLF emissions observed by an array of
Antarctic stations
	},
	journal={Journal of Geophysical Research},
	volume={103},
	number={A10},
	year={1998},
	month={Oct},
	pages={23611-22},
	abstract={
Describes amplitude modulations in the frequency range 0-500 mHz of ELF/VLF
(0.5-4.0 kHz) radio wave power recorded throughout 1993 and 1995 at Halley
and South Pole stations, Antarctica, which lie in approximately the same
magnetic meridian and at geomagnetic latitudes ( Lambda ) of 61 degrees and
74 degrees , respectively. Data from the intermediate automatic geophysical
observatories P2 and P3 ( Lambda =70 degrees and 72 degrees , respectively)
were also analyzed where available. In agreement with earlier work,
spectrograms have revealed the frequent daytime (typically 0700-1700 MLT)
occurrence of modulations lying almost entirely within the two period
ranges: 10-60 s and 4-6 s. The first range corresponds to quasiperiodic
(QP) emissions, while the latter is typical of the two-hop whistler mode
echo period in the plasma trough, and the events are termed periodic
emissions (PEs). QP occurrence rates higher than some earlier studies (335
station-days out of 667 examined) may be attributable to the sensitive
spectral analysis technique. The type I QPs (i.e. those correlated with
geomagnetic pulsations observed at South Pole and/or P2/P3) were consistent
with an upstream wave driver, controlled by the IMF cone angle. Type II QPs
(uncorrelated with magnetic pulsations) were always accompanied by PEs,
suggesting a link between the two. The authors propose that type II QPs are
driven by field line resonant ULF waves which in turn are generated by
field-aligned currents arising from PE induced electron precipitation
	},
	keywords={
		magnetospheric electromagnetic wave propagation
		radiowave propagation
		periodic ELF emissions
		periodic VLF emissions
		quasiperiodic ELF emissions
		quasiperiodic VLF emissions
		Antarctic stations
		amplitude modulations
		radio wave power
		AD 1993 to 1995
		Halley station
		South Pole station
		Antarctica
		intermediate automatic geophysical observatories
		P2
		P3
		spectrograms
		two-hop whistler mode echo period
		plasma trough
		periodic emissions
		spectral analysis
		geomagnetic pulsations
		South Pole
		IMF cone angle
		field line resonant ULF waves
		field-aligned currents
		electron precipitation
		0.5 to 4 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PaskoMay98,
	author={Pasko, V.P. and Inan, U.S. and Bell, T.F.},
	title={
Ionospheric effects due to electrostatic thundercloud fields
	},
	journal={Journal of Atmospheric and Solar-Terrestrial Physics},
	volume={60},
	number={7-9},
	year={1998},
	month={May},
	pages={863-70},
	abstract={
Electrostatic thundercloud fields are shown to heat lower ionospheric
electrons significantly under night time conditions. The effect is
maximized under conditions of higher altitudes of thundercloud charges,
larger magnitudes of these charges, and larger scale heights of ambient
conductivity profiles. The lower ionospheric conductivity can be modified
as a result of the heating by up to one order of magnitude in regions with
a characteristic lateral extent of À150 to 350 km. The vertical extent of
the heated region is À10 km, at altitudes of À70-80 km, reaching above 85
km in some cases, depending on the ambient night-time conductivity profile.
The electron heating may potentially alter the chemical balance in the
D-region, modify the ambient levels of optical emissions and the magnitude
of electrostatic thundercloud fields which map to higher ionospheric
altitudes
	},
	keywords={
		atmospheric composition
		atmospheric electricity
		atmospheric temperature
		D-region
		ionospheric disturbances
		thunderstorms
		electrostatic thundercloud fields
		ionospheric effects
		lower ionospheric electrons
		night time conditions
		thundercloud charges
		scale height
		vertical extent
		electron heating
		chemical balance
		D-region
		optical emissions
		magnitude
		0 to 100 km
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PaskoSep98,
	author={Pasko, V.P. and Inan, U.S. and Bell, T.F. and Reising, S.C.},
	title={
Mechanism of ELF radiation from sprites
	},
	journal={Geophysical Research Letters},
	volume={25},
	number={18},
	year={1998},
	month={Sep},
	pages={3493-6},
	abstract={
Charge and current systems associated with sprites constitute a part of the
large scale atmospheric electric circuit, providing a context for physical
understanding of recently discovered ELF radiation originating from
currents flowing within the body of sprites. It is shown that the impulse
of the electric current driven in the conducting body of the sprite by
lightning generated transient quasi-electrostatic fields produces
significant electromagnetic radiation in the ELF range of frequencies,
comparable to that radiated by the causative lightning discharge
	},
	keywords={
		atmospheric radiation
		atmospherics
		lightning
		mesosphere
		thermosphere
		thunderstorms
		radiowave emission
		ELF
		ELF radiation
		sprite
		mechanism
		mesosphere
		thermosphere
		ionosphere
		atmospherics
		thunderstorm
		vertical electric current
		vertical current
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{LaBelleSep98,
	author={LaBelle, J. and Weatherwax, A.T. and Perring, J. and Walsh, E. and Trimpi, M.L. and Inan, U.S.},
	title={
Low-frequency impulsive auroral hiss observations at high geomagnetic
latitudes
	},
	journal={Journal of Geophysical Research},
	volume={103},
	number={A9},
	year={1998},
	month={Sep},
	pages={20459-68},
	abstract={
Wave receivers in Antarctic Automatic Geophysical Observatories (AGOs)
measure spectral features of low-frequency impulsive auroral hiss emissions
which cannot be observed at northern hemisphere sites or near manned
Antarctic stations due to man-made interference. From observations at
AGO-P1 (À80 degrees invariant latitude) the authors distinguish two
spectral types of LF impulsive auroral hiss: normal events, in which the
power spectral density is a decreasing function of frequency throughout the
LF band, presumably peaking in the VLF band below the frequency range of
the LF/MF/HF receiver; and LF cutoff events, for which the power spectral
density peaks in the LF band with little or no power at VLF. Out of a large
sample of impulsive auroral hiss events observed at AGO-P1, 64% are the
normal type, 14% are the LF-cutoff type, and 22% are a mixture of both. A
hiss propagation model similar to that of Makita (1979) was used to
evaluate approximately whether the observed occurrence statistics of LF
cutoff auroral hiss are consistent with previous models of auroral hiss
generation and propagation. The results indicate that LF cutoff auroral
hiss can be explained by propagation effects and suggest that the observed
LF cutoff occurrence statistics are consistent with LF impulsive auroral
hiss originating at or ducted to altitudes of 2000-5000 km
	},
	keywords={
		atmospherics
		LF impulsive auroral hiss
		high geomagnetic latitudes
		Antarctic Automatic Geophysical Observatories
		low-frequency impulsive auroral hiss emissions
		wave receivers
		AGO-P1
		normal event
		LF cutoff events
		VLF band
		power spectral density peaks
		hiss propagation model
		auroral hiss generation
		auroral hiss propagation effects
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{LaubenAug98,
	author={Lauben, D.S. and Inan, U.S. and Bell, T.F. and Kirchner, D.L. and Hospodarsky, G.B. and Pickett, J.S.},
	title={
VLF chorus emissions observed by POLAR during the January 10, 1997,
magnetic cloud
	},
	journal={Geophysical Research Letters},
	volume={25},
	number={15},
	year={1998},
	month={Aug},
	pages={2995-8},
	abstract={
VLF chorus emissions occur near the dawn meridian in fast response (<60 s)
to magnetospheric perturbations caused by sudden fluctuations in solar wind
dynamic pressure and southward turnings of the interplanetary magnetic
field (IMF) at the arrival of the January 10, 1997 magnetic cloud.
Raytracing analysis indicates the likely chorus source region to be near
the magnetic equator with rays launched at oblique wave normal angles, for
which likely resonant electron energies are in the range EÀ14-30 keV,
consistent with observed particle data
	},
	keywords={
		atmospheric radiation
		atmospherics
		interplanetary magnetic fields
		magnetospheric electromagnetic wave propagation
		plasma waves
		solar wind
		VLF chorus emissions
		POLAR observations
		AD 1997 01 10
		magnetic cloud
		dawn meridian
		magnetospheric perturbations
		sudden fluctuations
		solar wind dynamic pressure
		southward turning interplanetary magnetic field
		raytracing analysis
		chorus source region
		magnetic equator
		oblique wave normal angles
		resonant electron energies
		particle data
		14 to 30 keV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{VossJun98,
	author={Voss, H.D. and Walt, M. and Imhof, W.L. and Mobilia, J. and Inan, U.S.},
	title={
Satellite observations of lightning-induced electron precipitation
	},
	journal={Journal of Geophysical Research},
	volume={103},
	number={A6},
	year={1998},
	month={Jun},
	pages={11725-44},
	abstract={
Lightning-induced electron precipitation (LEP) from the Earth's radiation
belt has been observed on numerous occasions with detectors on the
low-altitude S81-1/SEEP satellite. A sequence of seven LEP events on
September 9, 1982, and eight events on October 20, 1982, are correlated on
a one-to-one basis with one-hop whistlers at Palmer, Antarctica. The
temporal profile within a LEP burst has a remarkable fine structure. It is
shown to be associated with bunches of magnetically guided and focused
100-to-200 keV electrons that are repeatedly scattered by the atmosphere
and bounce between the northern and southern hemispheres. The delay time
between the lightning sferic and the arrival of the first electron bunch
increases with increasing L as predicted by the first-order order
gyresonance theory. The global distribution of strong LEP events observed
with the SEEP payload correlates with lightning activity and shows a
preferred distribution at 2<L<3. This L shell range corresponds to the slot
region in the electron radiation belt. A single LEP burst in the slot
region is estimated to deplete À0.001% of the particles in the region
covered by the burst magnetic field lines. The evidence supports the
production of structured LEP by ducted rather than nonducted whistlers. It
is found that ducted whistlers can be an important pitch angle diffusion
mechanism for 100-250 keV electrons in the 2<L<3 range although a number of
uncertainties in the various parameters remain to be resolved. It is
suggested that observations of LEP can be a new tool to measure the
presence and transverse dimensions of plasmaspheric whistler mode ducts
	},
	keywords={
		atmospheric electron precipitation
		atmospherics
		lightning
		radiation belts
		whistlers
		satellite observations
		lightning-induced electron precipitation
		LEP
		radiation belt
		S81-1/SEEP satellite data
		September 9 1982
		October 20 1982
		one-hop whistlers
		Palmer
		Antarctica
		temporal profile
		fine structure
		magnetically guided electrons
		focused electrons
		scattering
		bouncing
		delay time
		lightning sferic
		electron bunch
		first-order order gyresonance theory
		global distribution
		SEEP payload data
		slot region
		electron radiation belt
		burst magnetic field lines
		ducted rather than nonducted whistlers
		pitch angle diffusion mechanism
		plasmaspheric whistler mode ducts
		AD 1982 10 20
		AD 1982 09 09
		100 to 250 keV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PaskoJun98,
	author={Pasko, V.P. and Inan, U.S. and Bell, T.F.},
	title={
Spatial structure of sprites
	},
	journal={Geophysical Research Letters},
	volume={25},
	number={12},
	year={1998},
	month={Jun},
	pages={2123-6},
	abstract={
A theory of the electrical breakdown (EB) above thunderstorms is developed.
The streamer type of the EB is proposed for the explanation of observations
of fine spatial structures and bursts of blue optical emissions associated
with sprites
	},
	keywords={
		atmospheric electricity
		lightning
		mesosphere
		thunderstorms
		spatial structure
		sprites
		electrical breakdown
		thunderstorms
		streamer type
		bursts
		blue optical emissions
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{Ristic-DjurovicMay98,
	author={Ristic-Djurovic, J.L. and Bell, T.F. and Inan, U.S.},
	title={
Precipitation of radiation belt electrons by magnetospherically reflected
whistlers
	},
	journal={Journal of Geophysical Research},
	volume={103},
	number={A5},
	year={1998},
	month={May},
	pages={9249-60},
	abstract={
The authors use a test particle simulation model based on gyro-averaged
equations of motion to study the influence of oblique magnetospherically
reflected (MR) whistlers on the near-loss-cone distribution function of
radiation belt electrons. They find that MR whistlers originating in
lightning can resonantly interact with radiation belt electrons over a
broad range of L shells and precipitate higher energy electrons from lower
L shells. Electrons in the energy-range of 1 to 2.6 MeV are precipitated
from L=2, whereas from L=4 the precipitated electron energy range is
150-220 keV. The precipitated differential electron flux, due to this
interaction, is higher for higher L shells, and the maximum value ranges
from Phi E/sub prec/ (1.11 MeV)=5.2*10/sup -4/ electrons cm/sup -2/ s/sup
-1/ keV/sup -1/ at L=2 to Phi E/sub prec/ (173 keV)=4.6*10/sup -1/
electrons cm/sup -2/ s/sup -1/ keV/sup -1/ at L=4. The lifetimes of
radiation belt electrons in a given magnetic flux tube around the L shell
on which the interaction takes place are found to be of the order of
several days, comparable to lifetimes corresponding to electron loss
induced by hiss, which was heretofore assumed to be the dominant loss
mechanism [Lyons et al., 1972]. The minimum electron lifetimes vary from
2.4 days for 1.11 MeV electrons at L=2 to 4.6 days for 173 keV electrons at
L=4
	},
	keywords={
		atmospheric electron precipitation
		radiation belts
		whistlers
		magnetosphere
		electron precipitation
		radiation belt
		radiation belt electrons
		magnetospherically reflected whistler
		test particle simulation mode
		gyro-averaged equations of motion
		oblique whistler
		wave particle interaction
		near-loss-cone distribution function
		dominant loss mechanism
		electron lifetime
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BellApr98,
	author={Bell, T.F. and Reising, S.C. and Inan, U.S.},
	title={
Intense continuing currents following positive cloud-to-ground lightning
associated with red sprites
	},
	journal={Geophysical Research Letters},
	volume={25},
	number={8},
	year={1998},
	month={Apr},
	pages={1285-8},
	abstract={
In July-August, 1996, Stanford University carried out broadband ELF/VLF
measurements of the magnetic field radiated by positive cloud-to-ground
(CG) discharges associated with Red Sprites. The authors report these
measurements for 17 sprite associated discharges that occurred during a 15
minute period on August 1, 1996. The current and charge moments for each of
the events are deduced, and it is found that, in every case, intense
continuing currents of À1 ms duration are responsible for most of the
positive charge transfer to ground that precedes the appearance of the
sprite. The time delay between the causative positive discharge and the
video field in which the sprite first appeared varied from 0 to 15 ms for
the larger events to as much as 100 ms for the smaller events. The authors
suggest that in the smaller events the removal of significant positive
charge during this delay interval is accomplished through a horizontal
intracloud discharge
	},
	keywords={
		atmospheric electricity
		lightning
		thunderstorms
		atmosphere
		stratosphere
		sprite
		intense continuing current
		electric current
		positive cloud-to-ground lightning
		red sprite
		AD 1996 07
		AD 1996 08
		ELF
		VLF
		radiowave emission
		positive cloud-to-ground discharge
		positive charge transfer
		causative positive discharge
		time delay
		horizontal intracloud discharge
		thunderstorm
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{CummerApr98,
	author={Cummer, S.A. and Inan, U.S. and Bell, T.F. and Barrington-Leigh, C.P.},
	title={
ELF radiation produced by electrical currents in sprites
	},
	journal={Geophysical Research Letters},
	volume={25},
	number={8},
	year={1998},
	month={Apr},
	pages={1281-4},
	abstract={
Measurements of ELF-radiating currents associated with sprite-producing
lightning discharges exhibit a second current peak simultaneous in time
with sprite luminosity, suggesting that the observed ELF radiation is
produced by intense electrical currents flowing in the body of the sprite
	},
	keywords={
		atmospheric electricity
		atmospheric radiation
		lightning
		mesosphere
		stratosphere
		thermosphere
		stratosphere
		mesosphere
		thermosphere
		middle atmosphere
		upper atmopshere
		radiowave emission
		ELF radiation
		electric current
		electrical current
		sprite
		lightning discharge
		second current peak
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{LehtinenNov97,
	author={Lehtinen, N.G. and Bell, T.F. and Pasko, V.P. and Inan, U.S.},
	title={
A two-dimensional model of runaway electron beams driven by
quasi-electrostatic thundercloud fields
	},
	journal={Geophysical Research Letters},
	volume={24},
	number={21},
	year={1997},
	month={Nov},
	pages={2639-42},
	abstract={
Intense, transient quasi-electrostatic (QE) fields, which exist above
thunderclouds following a positive cloud-to-ground lightning discharge, can
produce an upward travelling runaway electron (REL) beam. A new
two-dimensional (2D) REL-QE model is developed, expanding the previously
reported 1D model [Bell et al., 1995] and incorporating the QE [Pasko et
al., 1997] and the electrostatic heating (ESH) [Pasko et al., 1997] models.
The new model gives the lateral electron distribution in the beam and
allows us to determine the ionospheric effects and the optical luminosities
resulting from the simultaneous action of the QE fields on the ambient
electrons and the runaway electrons. The model is self-consistent and
includes the changes in space charge and conductivity due to the REL.
Optical emissions and gamma -ray emissions [Lehtinen et al., 1996] are
calculated and compared to experimental observations of sprites and
terrestrial gamma -ray flashes (TGF). It is shown that the structure of the
electric field and the optical emissions can be significantly affected by
the REL
	},
	keywords={
		atmospheric electricity
		atmospheric radiation
		electron beams
		ionospheric disturbances
		mesosphere
		thunderstorms
		two-dimensional model
		runaway electron beams
		quasi-electrostatic thundercloud fields
		transient quasi-electrostatic fields
		thunderclouds
		positive cloud-to-ground lightning discharge
		upward travelling runaway electron beam
		REL-QE model
		electrostatic heating
		lateral electron distribution
		ionospheric effects
		optical luminosities
		space charge
		optical emissions
		gamma -ray emissions
		terrestrial gamma -ray flashes
		sprites
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PicardNov97,
	author={Picard, R.H. and Inan, U.S. and Pasko, V.P. and Winick, J.R. and Wintersteiner, P.P.},
	title={
Infrared glow above thunderstorms?
	},
	journal={Geophysical Research Letters},
	volume={24},
	number={21},
	year={1997},
	month={Nov},
	pages={2635-8},
	abstract={
Sustained heating of lower ionospheric electrons by thundercloud fields, as
suggested by Inan et al. [1996], may lead to the production of enhanced
infrared (IR) emissions, in particular 4.3- mu m CO/sub 2/ emission. The
excitation rate for N/sub 2/(v) via electron collisions is calculated using
a new steady-state two-dimensional electrostatic-heating (ESH) model of the
upward coupling of the thundercloud (TC) electric fields. The vibrational
energy transfer to CO/sub 2/ and 4.3- mu m radiative transfer are then
computed using a line-by-line non-LTE (non-local thermodynamic equilibrium)
radiation model. Limb-viewing radiance profiles at 4.3- mu m and typical
radiance spectra are estimated for five different TC charge distributions
and ambient ionic conductivities. Broadband 4.3- mu m enhancements of
greater than a factor of two above ambient nighttime levels are predicted
for tangent heights (TH) in the range À80 to >130 km for the most perturbed
case with larger enhancements in selected narrower spectral regions. The
predicted IR enhancements should be observable to an orbiting IR sensor
	},
	keywords={
		atmospheric electricity
		atmospheric radiation
		atmospheric temperature
		carbon compounds
		thunderstorms
		infrared glow
		thunderstorms
		heating
		lower ionospheric electrons
		CO/sub 2/ emission
		excitation rate
		electron collisions
		steady-state two-dimensional electrostatic-heating
		upward coupling
		vibrational energy transfer
		line-by-line nonLTE
		limb-viewing radiance profiles
		charge distributions
		ambient ionic conductivities
		tangent heights
		4.3 mum
		N/sub 2/
		CO/sub 2/
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SonwalkarJul97,
	author={Sonwalkar, V.S. and Carpenter, D.L. and Helliwell, R.A. and Walt, M. and Inan, U.S. and Caudle, D.L. and Ikeda, M.},
	title={
Properties of the magnetospheric hot plasma distribution deduced from
whistler mode wave injection at 2400 Hz: ground-based detection of
azimuthal structure in magnetospheric hot plasmas
	},
	journal={Journal of Geophysical Research},
	volume={102},
	number={A7},
	year={1997},
	month={Jul},
	pages={14363-80},
	abstract={
Siple station VLF wave injection experiments aimed at finding the
properties of the magnetospheric hot plasma were conducted for a 9-hour
period between 1705 and 0210 UT on January 23-24, 1988. A special frequency
versus time format, lasting 1 min and transmitted every 5 min, consisted of
a sequence of pulses, frequency ramps, and parabolas, all in a 1-kHz range
centered on 2400 Hz. The transmitted signals, after propagating along a
geomagnetic field-aligned duct were recorded at Lake Mistissini, Canada. At
various times during the 9-hour interval the Siple signals showed features
characteristic of wave-particle interactions, including wave growth,
sidebands, and triggered emissions. On the assumption that gyroresonant
interactions were responsible for the observed wave growth and saturation,
the timescales over which those phenomena varied provide constraints on the
possible energetic electron population within the duct. The authors
conclude that ground-based active and passive wave experiments have
substantial potential for investigating properties of the hot plasma of the
magnetosphere
	},
	keywords={
		magnetosphere
		magnetospheric electromagnetic wave propagation
		magnetospheric hot plasma distribution
		whistler mode wave injection
		ground-based detection
		azimuthal structure
		Siple station VLF wave injection experiments
		AD 1988 01 23 to 24
		geomagnetic field-aligned duct
		Siple signals
		wave-particle interactions
		wave growth
		sidebands
		triggered emissions
		gyroresonant interactions
		energetic electron population
		ground-based active experiments
		passive wave experiments
		2400 Hz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{CarpenterJul97,
	author={Carpenter, D.L. and Sonwalkar, V.S. and Helliwell, R.A. and Walt, M. and Inan, U.S. and Ikeda, M. and Caudle, D.L.},
	title={
Probing properties of the magnetospheric hot plasma distribution by
whistler mode wave injection at multiple frequencies: evidence of spatial
as well as temporal wave growth
	},
	journal={Journal of Geophysical Research},
	volume={102},
	number={A7},
	year={1997},
	month={Jul},
	pages={14355-62},
	abstract={
Discusses and illustrates the use of wave injection at multiple discrete
frequencies to study temporal changes in magnetospheric hot electrons with
parallel (gyroresonant) velocities in various nonoverlapping ranges. The
data studied were acquired during a special 9-hour period of 1.9-2.9 kHz
VLF transmissions from Siple Station, Antarctica, to Lake Mistissini,
Canada, on January 23-24, 1988. The amplitudes of the leading edges of
constant frequency pulses at 1900, 2150, and 2400 Hz were found to vary
independently with time. This is interpreted as evidence of a spatial
amplification process that accompanied the well known and more readily
identifiable phenomena of exponential temporal growth to a saturation
level. Evidence of wave-hot plasma interactions showed a dependence on
df/dt of the input signal frequency versus time format; in general, the
slow frequency ramps showed the highest amplitudes and the fast ramps and
parabolas the lowest, in agreement with past work
	},
	keywords={
		magnetospheric electromagnetic wave propagation
		plasma
		plasma waves
		whistlers
		magnetospheric hot plasma distribution
		whistler mode wave injection
		spatial wave growth
		temporal wave growth
		wave injection
		multiple frequencies
		temporal changes
		magnetospheric hot electrons
		gyroresonant velocities
		VLF transmissions
		Siple Station
		AD 1988 01 23 to 24
		spatial amplification process
		wave-hot plasma interactions
		1.9 to 2.9 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PaskoJul97,
	author={Pasko, V.P. and Inan, U.S. and Bell, T.F.},
	title={
Sprites as evidence of vertical gravity wave structures above mesoscale
thunderstorms
	},
	journal={Geophysical Research Letters},
	volume={24},
	number={14},
	year={1997},
	month={Jul},
	pages={1735-8},
	abstract={
Large area multicell thunderstorms lead to the formation of vertically
oriented cylindrical structures of gravity waves at mesospheric altitudes
closely resembling those observed in optical emissions associated with
transient luminous glows called sprites
	},
	keywords={
		atmospheric movements
		gravity waves
		lightning
		mesosphere
		thunderstorms
		lightning
		mesosphere
		middle atmosphere
		movement
		gravity wave
		vertically oriented cylindrical structure
		sprite
		sprites
		vertical gravity wave structure
		mesoscale thunderstorm
		optical emission
		optical emissions
		transient luminous glow
		model
		penetrative convection
		mesoscale convective complex
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{CummerJul97,
	author={Cummer, S.A. and Inan, U.S.},
	title={
Measurement of charge transfer in sprite-producing lightning using ELF
radio atmospherics
	},
	journal={Geophysical Research Letters},
	volume={24},
	number={14},
	year={1997},
	month={Jul},
	pages={1731-4},
	abstract={
Transient high altitude optical emissions referred to as "sprites" are
believed to occur as a result of the transfer of large amounts of charge
(\100-300 C) from cloud altitudes of 5-10 km to the ground. Using a general
subionospheric ELF propagation model, the authors quantitatively interpret
magnetic field waveforms of ELF radio atmospherics originating in
mid-western U.S. lightning discharges and observed at Stanford (\1800 km
range) to determine the temporal variation of the lightning current and
thereby measure the charge transfer during the stroke. For 6
sprite-producing lightning current waveforms observed on July 24, 1996, the
authors find that 25 to 325 coulombs of charge was transferred during the
first 5 ms of the discharges, assuming a 10 km altitude for the initial
charge
	},
	keywords={
		atmospherics
		clouds
		ionospheric electromagnetic wave propagation
		lightning
		thunderstorms
		atmosphere
		troposphere
		thunderstorm
		thundercloud
		electric current
		electric charge transfer
		sprite-producing lightning
		sprites
		ELF radio atmospherics
		transient high altitude optical emission
		cloud
		subionospheric ELF propagation model
		magnetic field waveform
		United States
		USA
		temporal variation
		lightning current
		AD 1996 07 24
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{CummerApr97,
	author={Cummer, S.A. and Bell, T.F. and Inan, U.S. and Chenette, D.L.},
	title={
VLF remote sensing of high-energy auroral particle precipitation
	},
	journal={Journal of Geophysical Research},
	volume={102},
	number={A4},
	year={1997},
	month={Apr},
	pages={7477-84},
	abstract={
Ground-based measurements of VLF transmitter signals propagating in the
Earth-ionosphere waveguide can be used to determine the location of
nighttime high-energy (>or approximately=100 keV) auroral particle
precipitation. When the region of auroral particle precipitation passes
over a VLF propagation path, disturbances in the D-region of the ionosphere
created by the high-energy particles perturb the amplitude of VLF signals
propagating below in a characteristic manner. Continuous nighttime
observations of the amplitude of the signal from the NLK transmitter (24.8
kHz, Jim Creek, Washington) were made in Gander, Newfoundland, during
November 1993 and January 1994. Simultaneous images of atmospheric X-rays
created by auroral particle precipitation taken by the AXIS instrument on
the UARS satellite were examined for times when large-scale auroral
particle precipitation extended over the NLK-Gander propagation path.
Quantitative characteristics of the precipitation-associated NLK signal
perturbations are established from days which clearly exhibit good
correlation between the AXIS images and VLF data, and a larger data set
from the months of November 1993 and January 1994 is examined statistically
to determine the effectiveness of the VLF technique in capturing particle
precipitation events. The number of particle precipitation onsets seen in
the AXIS images that can be readily identified in the VLF amplitude data is
found to be almost 94%. VLF propagation model calculations show that the
observed VLF amplitude decreases are consistent with propagation under
conditions of enhanced lower ionosphere electron density caused by auroral
electron precipitation and suggest that electrons with energies greater
than 100 keV are responsible for the VLF amplitude perturbations
	},
	keywords={
		atmospheric electron precipitation
		atmospheric ion precipitation
		ionospheric techniques
		ionosphere
		measurement technique
		radiowave propagation
		VLF remote sensing
		high-energy auroral particle precipitation
		electron precipitation
		VLF transmitter signal
		Earth-ionosphere waveguide
		location
		nighttime high-energy precipitation
		D-region
		NLK transmitter
		USA
		Washington
		Newfoundland
		Canada
		Gander
		AD 1993
		AD 1994
		signal perturbation
		VLF technique
		ion precipitation
		24.8 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PaskoMar97,
	author={Pasko, V.P. and Inan, U.S. and Bell, T.F. and Taranenko, Y.N.},
	title={
Sprites produced by quasi-electrostatic heating and ionization in the lower
ionosphere
	},
	journal={Journal of Geophysical Research},
	volume={102},
	number={A3},
	year={1997},
	month={Mar},
	pages={4529-61},
	abstract={
Quasi-electrostatic (QE) fields that temporarily exist at high altitudes
following the sudden removal (e.g., by a lightning discharge) of
thundercloud charge at low altitudes lead to ambient electron heating (up
to \5 eV average energy), ionization of neutrals, and excitation of optical
emissions in the mesosphere/lower ionosphere. Model calculations predict
the possibility of significant (several orders of magnitude) modification
of the lower ionospheric conductivity in the form of depletions of electron
density due to dissociative attachment to O/sub 2/ molecules and/or in the
form of enhancements of electron density due to breakdown ionization.
Results indicate that the optical emission intensities of the 1st positive
band of N/sub 2/ corresponding to fast (\1 ms) removal of 100-300 degrees C
of thundercloud charge from 10 km altitude are in good agreement with
observations of the upper part ("head" and "hair" [Sentman et al., 1995])
of the sprites. The typical region of brightest optical emission has
horizontal and vertical dimensions \10 km, centered at altitudes 70 km and
is interpreted as the head of the sprite. The model also shows the
formation of low intensity glow ("hair") above this region due to the
excitation of optical emissions at altitudes \85 km during \500 mu s at the
initial stage of the lightning discharge. Comparison of the optical
emission intensities of the 1st and 2nd positive bands of N/sub 2/, Meinel
and 1st negative bands of N/sub 2//sup +/ and 1st negative band of O/sub
2//sup +/ demonstrates that the 1st positive band of N/sub 2/ is the
dominating optical emission in the altitude range around \70 km, which
accounts for the observed red color of sprites, in excellent agreement with
recent spectroscopic observations of sprites. Results indicate that the
optical emission levels are predominantly defined by the lightning
discharge duration and the conductivity properties of the atmosphere/lower
ionosphere (i.e., relaxation time of electric
	},
	keywords={
		airglow
		atmospheric ionisation
		ionosphere
		ionospheric disturbances
		lightning
		mesosphere
		stratosphere
		thunderstorms
		thunderstorm
		lightning
		mesosphere
		ionosphere
		optical emission
		airglow
		middle atmosphere
		quasi-electrostatic heating
		sprite
		ionization
		electron heating
		model calculation
		breakdown ionization
		ionospheric disturbance
		thundercloud charge
		head
		hair
		red color
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanMar97,
	author={Inan, U.S. and Barrington-Leigh, C. and Hansen, S. and Glukhov, V.S. and Bell, T.F. and Rairden, R.},
	title={
Rapid lateral expansion of optical luminosity in lightning-induced
ionospheric flashes referred to as elves'
	},
	journal={Geophysical Research Letters},
	volume={24},
	number={5},
	year={1997},
	month={Mar},
	pages={583-6},
	abstract={
Data acquired by a new array of horizontally spaced photometers boresighted
with a low-light-level camera provide the first measurement of the rapid
lateral expansion of optical luminosity in lightning-induced ionospheric
flashes referred to as elves', occurring over time scales substantially
less than 1 ms. The narrow individual fields-of-view of (2.2 degrees *1.1
degrees ) provide a spatial resolution of \20-km at a range of 500 km,
enabling the documentation of expansion occurring over a horizontal range
of 200 km with a time resolution of \30 mu s. The observed dynamic features
of elves are consistent with a model in which the optical output is
produced as a result of heating by the electromagnetic pulse (EMP) from a
lightning discharge
	},
	keywords={
		atmospheric radiation
		atmospheric temperature
		ionospheric disturbances
		lightning
		plasma radiofrequency heating
		rapid lateral expansion
		optical luminosity
		lightning-induced ionospheric flashes
		elves
		dynamic features
		heating
		electromagnetic pulse
		lightning discharge
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{CarpenterJan97,
	author={Carpenter, D.L. and Galand, M. and Bell, T.F. and Sonwalkar, V.S. and Inan, U.S. and LaBelle, J. and Smith, A.J. and Clark, T.D.G. and Rosenberg, T.J.},
	title={
Quasiperiodic \5-60 s fluctuations of VLF signals propagating in the
Earth-ionosphere waveguide: a result of pulsating auroral particle
precipitation?
	},
	journal={Journal of Geophysical Research},
	volume={102},
	number={A1},
	year={1997},
	month={Jan},
	pages={347-61},
	abstract={
Subionospheric very low frequency and low-frequency (VLF/LF) transmitter
signals received at middle-latitude ground stations at nighttime were found
to exhibit pulsating behavior with periods that were typically in the \5-60
s range but sometimes reached \100 s. The amplitude versus time shape of
the pulsations was often triangular or zigzag-like, hence the term "zigzag
effect." Variations in the envelope shape were usually in the direction of
faster development than recovery. Episodes of zigzag activity at Siple,
Antarctica (L\4.3), and Saskatoon, Canada (L\4.2), were found to occur
widely during the predawn hours and were not observed during
geomagnetically quiet periods. The fluctuations appeared to be caused by
ionospheric perturbations at the \85 km nighttime VLF reflection height in
regions poleward of the plasmapause. The authors infer that in the case of
the Saskatoon and Siple data, the perturbations were centered within \500
km of the stations and within \100-200 km of the affected signal paths.
Their horizontal extent is inferred to have been in the range \50-200 km.
The assembled evidence, supported by Corcuff's (1996) research at Kerguelen
(L\3.7), suggests that the underlying cause of the effect was pulsating
auroral precipitation
	},
	keywords={
		atmospheric elementary particle precipitation
		Earth-ionosphere waveguide
		radiowave propagation
		quasiperiodic fluctuations
		VLF signals
		Earth-ionosphere waveguide
		pulsating auroral particle precipitation
		subionospheric LF transmitter signals
		zigzag effect
		envelope shape
		Siple
		Antarctica
		Saskatoon
		Canada
		ionospheric perturbations
		nighttime VLF reflection height
		5 to 60 s
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Grossman96,
	author={Grossman, D.A. and Sweeney, K.J. and Frieder, O.},
	title={
Client/server performance testing: a case study of a personnel application
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={925-34 vol.2},
	abstract={
We present a simulation-based approach to client/server performance
testing. This approach uses the Promark Rhobot/Win testing tool to simulate
execution of and measure performance of a client/server application. We
describe a case study of a large personnel application and address a
variety of complexities unique to the client/server environment
	},
	keywords={
		business data processing
		client-server systems
		distributed databases
		personnel
		program testing
		software performance evaluation
		virtual machines
		client server performance testing
		case study
		personnel application
		simulation-based approach
		Promark Rhobot Win testing tool
		performance evaluation
		distributed database
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Kostin96,
	author={Kostin, A.E.},
	title={
A protocol for distributed scheduling in a processor network
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={915-24 vol.2},
	abstract={
A distributed scheduler is proposed which is based on a special
communication protocol in a processor network. An informal description of
the protocol used by the scheduler is provided. The protocol was
implemented as a model in terms of the extended Petri nets (E-nets). The
results of a simulation study are compared to the behaviour of an ideal,
centralized scheduler
	},
	keywords={
		multiprocessor interconnection networks
		Petri nets
		processor scheduling
		protocols
		virtual machines
		distributed scheduling protocol
		processor network
		communication protocol
		extended Petri nets
		simulation study
		centralized scheduler
		job scheduling
		modeling
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Al-Khayatt96,
	author={Al-Khayatt, S. and Cooling, J.E.},
	title={
Issues in the design of a kernel for distributed, embedded systems
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={901-13 vol.2},
	abstract={
In a number of parallel computations, tasks may be naturally distributed in
a functional partitioning manner. Functionally distributed systems are
often modelled and controlled as a set of communicating, distributed
sub-tasks (processes). The software for such systems invariably reflects
the distributed nature of the application. Moreover, the software design
and support of such a functional distribution of sub-tasks depends on the
degree of interaction of these processes among the different nodes. The
design approach advocated in the paper is particularly appropriate to
real-time applications. Moreover, it should result in the generation of
high quality software which has good run-time performance. This paper is
organised to address two issues: task management in a distributed
environment; and kernel design to support functional partitioning and the
use of distributed variables
	},
	keywords={
		message passing
		network operating systems
		operating system kernels
		real-time systems
		software performance evaluation
		software quality
		systems analysis
		distributed embedded systems kernel design
		parallel computations
		distributed tasks
		functional partitioning
		functionally distributed systems
		communicating processes
		software design
		real-time applications
		high quality software
		run-time performance
		task management
		distributed variables
		message passing
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Chi-Ming-Chung96,
	author={Chi-Ming Chung and Shih, T.K. and Ying-Hong Wang and Ying-Feng Kou and Yuh-Long Shyy},
	title={
Concurrent programming testing and metrics based on task decomposition
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={891-900 vol.2},
	abstract={
Software testing and metrics are two important approaches to assure the
reliability and quality of software. Testing and metrics of sequential
programs have been a fairly sophisticated process, with various
methodologies and tools available for use in building and demonstrating the
correctness of a program being tested. The emergence of concurrent
programming in the recent years, however, introduces new testing problems
and difficulties that cannot be solved by testing techniques of traditional
sequential programs. One of the difficult tasks is that concurrent programs
can have many instances of execution for the same set of input data. Many
concurrent program testing methodologies are proposed to solve controlled
execution and determinism. There are few discussions of concurrent software
testing from the inter-task viewpoints. Yet, the common characteristics of
concurrent programming are explicit identification of the large grain
parallel computation units (tasks), and the explicit inter-task
communication via a rendezvous-style mechanism. We focus the testing view
on concurrent programming through task decomposition. We propose four
testing criteria to test a concurrent program. The programmer can choose an
appropriate testing strategy depending on the properties of concurrent
programs. Associated with the strategies, four equations are provided to
measure the complexity of concurrent programs
	},
	keywords={
		parallel programming
		program testing
		program verification
		software metrics
		software quality
		software reliability
		concurrent programming testing
		software metrics
		task decomposition
		software reliability
		software quality
		sequential programs
		methodologies
		software tools
		program correctness
		controlled execution
		determinism
		large grain parallel computation
		explicit inter-task communication
		rendezvous-style mechanism
		program complexity
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Adda96,
	author={Adda, M. and Dwyer, J. and Bouridane, A.},
	title={
The architecture of a RISC multithread processor
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={877-89 vol.2},
	abstract={
The major concerns for constructing efficient general purpose massively
parallel computers are the programmability and the hardware latency. The
latency, which emanates during local or remote memory accesses or during
concurrent synchronization of operations, tends to leave the processor idle
for several clock cycles and hence deteriorates the performance of the
whole system. We present the architecture of a simple RISC multithread
processor (RISC-MP). When interleaving the execution of several operations
belonging to separate threads, the processor tolerates the local memory,
network and synchronization latencies imposed by the components of the
system. The processor switches between threads every clock cycle, and
allows them to communicate through register banks without necessarily
sharing any memory
	},
	keywords={
		general purpose computers
		multiprogramming
		parallel architectures
		parallel machines
		parallel programming
		performance evaluation
		reduced instruction set computing
		synchronisation
		RISC multithread processor architecture
		general purpose massively parallel computers
		programmability
		hardware latency
		remote memory access
		concurrent synchronization
		clock cycles
		performance
		RISC-MP
		local memory
		synchronization latencies
		register banks
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Cinar96,
	author={Cinar, A. and Arslan, A.},
	title={
Two approaches on blending
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={869-76 vol.2},
	abstract={
Blending is the joining of sharp edges or corners in the intersecting or
nonintersecting region of 2D or 3D objects with smooth surfaces or curves,
or the smoothing of sharp edges or corners of objects. Two different
methods and the relation between these methods are given and blend shapes
are realized with the help of the first method. The first method is the
creation of surfaces with approximation curves based on three points and
the second method is the solution of a parabolic partial differential
equation (PPDE) taking the intersection curves as boundary conditions.
While the first method is well suited for interactive operations, the
second method, which is based on a more detailed mathematical work, needs
much more computational power
	},
	keywords={
		finite difference methods
		parabolic equations
		partial differential equations
		solid modelling
		blending
		sharp edge joining
		sharp corner joining
		intersecting region
		nonintersecting region
		2D objects
		3D objects
		smooth surfaces
		curves
		sharp edge smoothing
		sharp corner smoothing
		blend shapes
		approximation curves
		surface creation
		parabolic partial differential equation
		intersection curves
		boundary conditions
		interactive operations
		solid modelling
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Stemposz96,
	author={Stemposz, E.J. and Rutkowski, A.},
	title={
Determining faces of a 3D object in engineering drawings based on planar
graphs
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={861-8 vol.2},
	abstract={
The authors present a method of determining the set of 3D object faces from
its projections. The main tool is the algorithm enumerating all inner
cycles in a planar undirected simple graph. Since the most time consuming
operation they use is sorting of n-element set the computational complexity
of the method is O(nlgn)
	},
	keywords={
		computational complexity
		edge detection
		engineering graphics
		graph theory
		image reconstruction
		object recognition
		sorting
		stereo image processing
		3D object face determination
		projections
		algorithm
		inner cycle enumeration
		planar undirected simple graph
		engineering drawings
		n-element set sorting
		computational complexity
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Sarukhanyan96,
	author={Sarukhanyan, A.G. and Grigoryan, A.M.},
	title={
Decomposition of the Hadamard matrices by orthogonal vectors. The paired
algorithm for computing of 1-D Hadamard transform
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={851-60 vol.2},
	abstract={
The first part of the paper is devoted to the classical algorithm of the
Walsh-Hadamard fast transform using only nlog/sub 2/n addition operations
where n is a power of two. A problem of decomposition of Hadamard matrices
of arbitrary older n,n identical to O(mod4) by orthogonal (-1, +1)-vectors
of length k is investigated. An algorithm of the Hadamard fast transform
which uses only nlog/sub 2/k+n(n/k-1) addition operations, and in some
cases is more efficient than the classical algorithm, is proposed. In the
second part, the fast algorithm of computation of the one-dimensional
unitary discrete Hadamard transform by means of the paired transform is
given. It is proved that to compute the N-point transform only O(N)
addition-subtraction operations are necessary
	},
	keywords={
		computational complexity
		Hadamard matrices
		Hadamard transforms
		matrix decomposition
		vectors
		Hadamard matrix decomposition
		orthogonal vectors
		paired algorithm
		1D Hadamard transform computation
		classical algorithm
		Walsh-Hadamard fast transform
		addition operations
		1D unitary discrete Hadamard transform
		paired transform
		addition-subtraction operations
		N-point transform
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Atmaca96,
	author={Atmaca, H. and Bulut, M. and Demir, D. and Pazar, S.},
	title={
A new fuzzy Kohonen clustering network based on histogram for image
segmentation
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={845-9 vol.2},
	abstract={
The fuzzy Kohonen clustering network (FKCN) algorithm is proposed for image
segmentation. However, for iterative operations this algorithm takes a very
long time. Therefore, care has been taken in order to make the FKCN
algorithm realistically useful for image segmentation. A new FKCN algorithm
has been developed which is based on an image histogram. Theoretical
analysis and experimental results show that computing time is decreased and
the proposed FKCN is a successful algorithm for image segmentation
	},
	keywords={
		computational complexity
		fuzzy neural nets
		image segmentation
		pattern recognition
		self-organising feature maps
		fuzzy Kohonen clustering network algorithm
		image segmentation
		image histogram
		iterative operations
		computing time
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Babaev96,
	author={Babaev, A. and Guler, B.},
	title={
Adequacy theorems for fuzzy models
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={837-44 vol.2},
	abstract={
Adequacy fuzzy systems for classic logical inference rules are investigated
and necessary conditions are stated. The problem is considered by regarding
input and projection using variations and necessary theorems are proved. An
application of these theorems is discussed
	},
	keywords={
		fuzzy logic
		fuzzy systems
		inference mechanisms
		theorem proving
		adequacy fuzzy systems
		classic logical inference rules
		adequacy theorems
		fuzzy models
		input
		projection
		variations
		theorem proving
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Benslimane96,
	author={Benslimane, A.},
	title={
On the use of reachability graph for protocols analysis
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={827-36 vol.2},
	abstract={
In a complete protocol design process, it is often important to validate
the protocol for general correctness properties such boundedness, deadlock
and unspecified reception freedom. Reachability analysis has proved to be
one of the most effective methods for protocol validation based on the
state transition model. Consequently, many protocol validation tools have
been built based on the technique of reachability analysis. The author
presents the VALIPRO (Validation of Protocols) validation tool for
communication protocols modeled as a number of communicating finite states
machines. It allows a user-friendly and graphic introduction of automata
and proposes four methods of validation. Deadlocks, unspecified receptions,
blocking reception states, and capacity overflow are detected by this tool
	},
	keywords={
		computer graphics
		finite state machines
		formal specification
		formal verification
		protocols
		reachability analysis
		protocol analysis
		reachability graph
		protocol design
		protocol validation
		correctness properties
		boundedness
		deadlock
		unspecified reception freedom
		reachability analysis
		state transition model
		VALIPRO validation tool
		communication protocols
		communicating finite states machine
		automata
		graphical method
		blocking reception states
		capacity overflow
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Korver96,
	author={Korver, H. and Sellink, M.P.A.},
	title={
On automating process algebra proofs
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={815-25 vol.2},
	abstract={
Groote and Springintveld (1995) incorporated several model-oriented
techniques-such as invariants, matching criteria, state mappings-in the
process-algebraic framework of mu CRL for structuring and simplifying
protocol verifications. The authors formalise these extensions in Coq,
which is a proof development tool based on type theory. In the updated
framework, the length of proof constructions is reduced significantly.
Moreover, the new approach allows for more automation (proof generation)
than was possible in the past. The results are illustrated by an example in
which they prove two queue representations equal
	},
	keywords={
		formal verification
		process algebra
		protocols
		queueing theory
		theorem proving
		type theory
		automated process algebra proofs
		model-oriented techniques
		invariants
		matching criteria
		state mappings
		mu CRL
		protocol verification structuring
		protocol verification simplification
		Coq
		proof development tool
		type theory
		proof construction length
		proof generation
		queue representations
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Moreaux96,
	author={Moreaux, P.},
	title={
Combining aggregation and decomposition methods for performance evaluation
of complex systems
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={805-14 vol.2},
	abstract={
To reduce the complexity of computation of performance indices of parallel
systems, the author presents a new exact method combining the aggregation
and decomposition methods of the state space. Aggregation is performed by
the use of the stochastic well-formed net (SWN) Petri net model and
decomposition follows tensor methods initiated by Plateau (1985). The
author generalizes previous work to provide results for asynchronous as
well as synchronous composition of submodels. The author highlights the
problems of such an approach and derives necessary conditions on the
modelled systems that allow for the two methods to be combined. For
parallel systems satisfying these necessary conditions, models with
corresponding algorithms are developed
	},
	keywords={
		Markov processes
		parallel algorithms
		Petri nets
		software performance evaluation
		decomposition methods
		aggregation methods
		performance evaluation
		computational complexity
		performance indices
		parallel systems
		complex systems
		state space
		stochastic well-formed net
		tensor methods
		asynchronous submodel composition
		synchronous submodel composition
		algorithms
		Petri net model
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Abdulla96,
	author={Abdulla, P.A. and Kindahl, M.},
	title={
Using lossy channel systems for the verification of communication protocols
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={793-803 vol.2},
	abstract={
The authors consider the class of finite-state systems communicating
through unbounded but lossy FIFO channels (called lossy channel systems).
These systems have infinite state spaces due to the unboundedness of the
channels. Lossy channel systems are able to model e.g. link protocols such
as the alternating bit protocol, HDLC, and the bounded retransmission
protocol. In an earlier paper, they showed that the problems of checking
reachability, safety properties, and eventuality properties are decidable
for lossy channel systems. The decidability results were obtained under the
assumption that message delivery through a channel may take an arbitrary
amount of time. They consider a variant of lossy channel systems where
message deliveries have zero delays. This new model allows one to analyze
new classes of protocols which are not covered by the original model
	},
	keywords={
		decidability
		formal verification
		losses
		protocols
		safety
		telecommunication channels
		communication protocol verification
		finite-state systems
		lossy FIFO channels
		unbounded FIFO channels
		lossy channel systems
		infinite state spaces
		link protocols
		alternating bit protocol
		HDLC
		bounded retransmission protocol
		reachability
		safety properties
		eventuality properties
		decidability
		message delivery
		zero delays
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Inal96,
	author={Inal, H. and Ersoy, C.},
	title={
A heuristic approach for finding the minimum delay spanning tree in
topological design of interconnected LANs
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={785-91 vol.2},
	abstract={
As the use of local area networks (LANs) increases, the need for
interconnecting LANs has become an important topic. Some of the reasons for
interconnecting LANs are obtaining higher reliability, security, and
performance, and to increase the number of stations supported. Bridges are
data link layer devices that store and forward frames between similar or
dissimilar LANs. The paper describes a heuristic algorithm for finding a
minimum delay spanning tree that is used by transparent bridges to
interconnect LANs. The interconnected network is represented as a graph in
which nodes correspond to LANs to be interconnected. The edges selected in
the graph to form a tree correspond to connections provided by transparent
bridges. In order to measure the quality of the solutions, the authors
found the global minimum for small size problems. The algorithm finds
solutions very close to the global minimum for small size problems. For
larger size problems, they created 5000 trees that satisfy constraints for
15, 20 and 30 nodes to show that the heuristic algorithm will give better
solutions than randomly selected trees. They tested the algorithm for
various size problems to evaluate its time complexity. The time analysis
gave O(n/sup 2/) complexity
	},
	keywords={
		computational complexity
		computer network reliability
		LAN interconnection
		local area networks
		security
		trees (mathematics)
		interconnected LANs
		topological design
		minimum delay spanning tree
		local area networks
		reliability
		security
		performance
		stations
		data link layer devices
		heuristic algorithm
		transparent bridges
		graph
		nodes
		edges
		small sized problems
		global minimum
		constraints
		time complexity
		time analysis
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Billionnet96,
	author={Billionnet, A. and Costa, M.-C. and Wei-Ying Thang},
	title={
Task allocation and computing architecture optimization. An application at
EDF
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={775-84 vol.2},
	abstract={
The purpose of this article is to place the task allocation problem in a
computing architecture design concept. This problem is the main concern of
EDF (Electricite de France) engineers in charge of validating, and even
optimizing, computing architectures by simulation. We describe the design
process and we specify the types of applications and architectures
concerned with our study. Then, we present an application concerning the
design of an electricity control and monitoring system and we propose a
model of the tasks, the databases and the links. We have selected two
criteria to evaluate the quality of an allocation: a balanced distribution
of "loads" between the processors and a limited use of the communication
lines. We associate a mathematical model with the problem and we solve it
using a simulated annealing heuristic
	},
	keywords={
		computerised monitoring
		database management systems
		electricity supply industry
		heuristic programming
		parallel architectures
		power system control
		resource allocation
		simulated annealing
		virtual machines
		task allocation
		computing architecture optimization
		EDF
		simulation
		electricity control
		electricity monitoring system
		databases
		quality
		load balancing
		communication lines
		mathematical model
		simulated annealing heuristic
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Kasapoglu96,
	author={Kasapoglu, H. and Erdogan, N.},
	title={
DRM: distributed raw-data manager
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={771-4 vol.2},
	abstract={
The paper presents the logical implementation of shared memory on a
physically distributed memory system. A collection of workstations
connected by an Ethernet network serves as the platform of implementation.
DRM-distributed raw-data manager-is a software tool that provides the
distributed shared data paradigm at user-level, through run-time library
routines. It combines the general and convenient programming model of
shared memory systems with the computing power of distributed memory
systems, hiding the details of data distribution and communication
management required by the message passing model
	},
	keywords={
		distributed memory systems
		local area networks
		message passing
		parallel programming
		shared memory systems
		workstations
		DRM
		distributed raw-data manager
		shared memory
		physically distributed memory system
		workstations
		Ethernet network
		software tool
		user-level distributed shared data paradigm
		run-time library routines
		programming model
		data distribution
		communication management
		message passing model
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Khan96,
	author={Khan, A.S. and Simonenko, V. and Pham Hong Hanh},
	title={
Theoretical adding for solving problem of maximum matching in distributed
systems
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={759-69 vol.2},
	abstract={
The paper provides a theoretical basis that supports a new approach for
solving the assignment problem in dynamic scheduling in distributed
systems. The key idea of the approach is to divide the process of
scheduling into preliminary analysis of initial data and finding the
solution with the support of the results of this analysis. The analysis
algorithm is built on the principle of step-by-step forming and is called
adaptive multi-analyzing algorithm (AMA). This algorithm is based on
theoretical task assignment. The time complexity of the proposed algorithm
varies from O[Nlog(N)+E] to less. The adding of this algorithm based on
their theoretical system for analyzing initial data allows them to decrease
the whole time complexity for finding the schedule of jobs and resources.
These advances of AMA are shown using the results of experiments in the
simulation of multiprocessing systems as well
	},
	keywords={
		computational complexity
		distributed algorithms
		multiprocessing systems
		processor scheduling
		virtual machines
		maximum matching
		distributed systems
		assignment problem
		dynamic scheduling
		theoretical adding
		initial data analysis
		step-by-step forming
		adaptive multi-analyzing algorithm
		task assignment
		time complexity
		job scheduling
		resource scheduling
		multiprocessing system simulation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Coppa96,
	author={Coppa, F. and Nardelli, E. and Talamo, M.},
	title={
Discrete representation of spatial relations
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={749-58 vol.2},
	abstract={
The authors show how to represent spatial objects in discrete space so that
testing of containment and intersection relations between objects in the
continuum can be done correctly. They characterize containment and
intersection relations between spatial objects in terms of containment and
intersection between sets of points of Z/sup 2/. The model is based on a
mapping from spatial objects in real space to their representations in the
discrete world such that topological relations on spatial objects are
preserved. The mapping makes reference to a suitable topology whose
underlying set is a canonical decomposition of the real plane in square
cells
	},
	keywords={
		database theory
		geographic information systems
		spatial data structures
		topology
		visual databases
		spatial relations
		discrete representation
		spatial object representation
		discrete space
		containment relation testing
		intersection relation testing
		continuum
		containment relations
		intersection relations
		real space
		topological relations
		canonical decomposition
		real plane
		square cells
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Cak96,
	author={Cak, S. and Ersak, A.},
	title={
Fuzzy c-means clustering based color selection in ray tracing
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={745-8 vol.2},
	abstract={
Color selection from a ray tracer output is normally made by using the
output image histogram for finding the frequently used colors in the image.
Although the execution time is short in using the histogram method, the
image quality visually degrades in return. The fuzzy c-means clustering
algorithm can alternatively be used for the color selection in order to
reduce the level of image quality degradation. The study, based on the fact
that dominant peaks of the histogram are almost equal to the fuzzy
centroids of clusters, takes the histogram peaks as iteratively determined
fuzzy centroids of FCM. This reduces the computational burden in FCM and
besides that it improves the overall performance
	},
	keywords={
		colour graphics
		fuzzy set theory
		image colour analysis
		ray tracing
		fuzzy c-means clustering based color selection
		ray tracing
		ray tracer output
		fuzzy c-means clustering algorithm
		image quality degradation
		dominant histogram peaks
		iteratively determined fuzzy centroids
		performance
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Sarfraz96,
	author={Sarfraz, M.},
	title={
An alternative to the NURBS of degree three
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={735-44 vol.2},
	abstract={
A constructive approach is adopted to build a B-spline-like basis for a
rational cubic spline with a cubic numerator and quadratic denominator.
This formulation is quite useful for producing well controlled shape
effects when compared to th NURBS and it does work as an alternative to the
NURBS (the author calls it ANURBS). This ANURBS method is also a C/sup 2/
alternative to the GC/sup 2/ v-splines and the Gamma splines. The method
for evaluating this rational cubic B-spline curve is suggested by a
transformation to Bernstein-Bezier form. A comparative study, regarding the
better shape control as compared to the NURBS, is also made
	},
	keywords={
		CAD
		CAD/CAM
		curve fitting
		engineering graphics
		splines (mathematics)
		degree three NURBS
		B-spline-like basis
		rational cubic spline
		cubic numerator
		quadratic denominator
		shape effects
		ANURBS method
		GC2 v-splines
		Gamma splines
		rational cubic B-spline curve
		Bernstein-Bezier form
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Cuppens96,
	author={Cuppens, F. and Gabillon, A.},
	title={
A query language for a multilevel object-oriented database
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={723-34 vol.2},
	abstract={
The paper proposes a formal model for answering queries in a multilevel
object-oriented database (OODB). The MultiView model is a multilevel
security model for an OOBD. It provides a user cleared at a given security
level with a consistent and complete view of the multilevel OODB
corresponding to her clearance level. The formal definition of the
MultiView model is based on first-order logic. An OODB secured with the
MultiView model is associated with its own logical theory. The authors show
how the first-order language they defined can be used to query a multilevel
OODB secured with the MultiView model
	},
	keywords={
		authorisation
		object-oriented databases
		query languages
		query processing
		multilevel object-oriented database
		formal model
		query answering
		query language
		MultiView model
		multilevel security model
		security level
		clearance level
		first-order logic
		logical theory
		first-order language
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Bayram96,
	author={Bayram, Z.O. and Bryant, B.R. and Altmay, U.},
	title={
ROSE: a practical higher-order functional/logic language
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={713-22 vol.2},
	abstract={
The authors present a higher-order functional/logic language, ROSE. The
programs of ROSE are made up of conditional constructor based term
rewriting systems. The conditions in the rules can optionally be
committing. The operational semantics of the language is conditional
narrowing, augmented to deal with committing conditions. The major
innovation of the language is the use of committing guards and backtracking
to make possible very practical, operationally oriented programs. They show
many practical examples, one of which is the definition of the extra
logical function not, which implements the negation-as-finite-failure rule
in the context of functional/logic programming
	},
	keywords={
		backtracking
		computational linguistics
		functional languages
		functional programming
		logic programming
		logic programming languages
		rewriting systems
		higher-order functional/logic language
		ROSE language
		ROSE programs
		constructor based term rewriting systems
		operational semantics
		conditional narrowing
		committing conditions
		committing guards
		backtracking
		operationally oriented programs
		not logical function
		negation-as-finite-failure rule
		functional/logic programming
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Gaibisso96,
	author={Gaibisso, C. and Nardelli, E. and Proietti, G.},
	title={
Incremental constraints maintenance in concurrent logic programming
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={703-12 vol.2},
	abstract={
The authors consider an algorithmic problem related to the incremental
maintenance of constraints in a context of concurrent constraint logic
programming (CC). They consider CC languages defined on symbolic,
non-structured finite domains, where concurrent agents working on different
sets of constraints define different partitions into equivalence classes
over the universe of feasible values. An equivalence class of a partition
contains the values which are equivalent as far as the satisfaction of the
related set of constraints is concerned. The problem of knowing which are
the equivalence classes with respect to the various agents can be modelled
by means of a variant of the well-known disjoint set union problem. They
introduce a data structure for such a variant which leads to an optimal
worst case cost in dealing with the new defined operation, paying a cost
which is proportional to the size of the returned intersection. They also
provide the conditions under which the introduced data structure has better
performances than the extension of classical approach for the set union
problem
	},
	keywords={
		constraint handling
		data structures
		equivalence classes
		logic programming languages
		parallel languages
		parallel programming
		incremental constraints maintenance
		concurrent constraint logic programming
		algorithmic problem
		concurrent constraint logic programming languages
		symbolic nonstructured finite domains
		concurrent agents
		equivalence classes
		feasible values
		disjoint set union problem
		data structure
		optimal worst case cost
		returned intersection
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Cavusoglu96,
	author={Cavusoglu, A. and Demirer, M. and Cayir, H.},
	title={
A multi-lingual system for teaching programming language constructs
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={699-702 vol.2},
	abstract={
One of the major problems of lecturers is teaching beginners programming
language constructs. To overcome this problem a reconfigurable user
friendly interpreter has been developed. The system allows users to change
the interpreted graphical language which is used to solve maze problems
formed by the user. The user has the freedom to change the language which
is targetted to teach programming constructs similar to Pascal. At the
moment the user can either use Turkish or English (predefined) for
programming. In other cases, the user has to input the keywords for the new
language (i.e. French, German etc.) to match their English equivalents
	},
	keywords={
		computer science education
		program interpreters
		teaching
		visual languages
		multi-lingual system
		programming language construct teaching
		reconfigurable user friendly interpreter
		interpreted graphical language
		maze problems
		Pascal
		Turkish language
		English language
		keywords
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Karaman96,
	author={Karaman, F.S.},
	title={
Building a multimedia Web site by using JAVA and JAVA applets
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={693-8 vol.2},
	abstract={
The answer to the question what makes the World Wide Web so powerful is
that the client-side calculations frees the server from dependence on the
client's operating system. It makes the Web simultaneously system
independent and a minimal consumer of the bandwidth. By creating a standard
way to transmit functions, not just data, over network lines, the
reliability and authority of the server database can be used with the power
of the client computer so that the Web will not be just an information
publishing network-as it was during its short history-but a universal
database. In this study the usage in multimedia environments of one tool
(JAVA), which is well on its way to perform these changes, is examined.
JAVA is a programming language (akin to C++) developed specifically for the
Web by SUN Microsystems. Java applets-small applications built for specific
tasks-are compact and platform independent, or rather dependent only on
whether client's platform's browsers support the language. Web developers
are going to be able to link applets to HTML documents, effectively turning
the browser into an ad hoc application window. So the study covers building
a Web site for a well known local Rock band including multimedia
applications such as using sound (five songs of the band), video (an
interview with the members of the band) and so on using JAVA and JAVA
applets
	},
	keywords={
		Internet
		multimedia systems
		object-oriented languages
		object-oriented programming
		multimedia Web site
		JAVA applets
		World Wide Web
		client-side calculations
		system independent
		server database
		client computer
		information publishing network
		universal database
		multimedia environments
		JAVA programming language
		Web developers
		HTML documents
		browser
		ad hoc application window
		local Rock band
		multimedia applications
		video
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Oyman96,
	author={Oyman, E.I. and Ersoy, C.},
	title={
Multipoint communication in multimedia applications
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={685-91 vol.2},
	abstract={
Choosing a route that minimizes the network cost between multicasting
parties is a decision problem which is closely related with the Steiner
tree problem (STP), and is known to be NP complete. Several heuristics have
been proposed for solving STP that run in polynomial time and result in
reasonable solutions. However, they have the drawback that they are not
designed for multimedia applications which require certain quality of
service (QoS) guarantees. We investigate the success of simulated annealing
(SA) for solving this problem. We experimented with example problems of
different size and obtained promising results
	},
	keywords={
		computational complexity
		minimisation
		multimedia communication
		multimedia computing
		simulated annealing
		trees (mathematics)
		multipoint communication
		multimedia applications
		network cost minimisation
		multicasting parties
		decision problem
		Steiner tree problem
		STP
		NP complete
		polynomial time
		quality of service
		QoS guarantees
		simulated annealing
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Brown96,
	author={Brown, J.C. and Chase, M.R. and Cooper, M.A. and Kirkwood, P.J. and Sadik, A.K.},
	title={
A Postscript document management system
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={675-84 vol.2},
	abstract={
Postscript is an ideal, as yet unexplored storage format for document
management: its advantages are listed in comparison with raster files, and
with text marked up with SGML or HTML. A prototype system is described,
written in 20,000 lines of C and interfacing to the portable Display
Postscript interpreter and X Graphics User Interface. Screen snapshots show
the document catalogue, Boolean query facility on author, title and
document text, the document viewer and automatically generated contents
list and alphabetic index. An interactive graphical reading path solves the
"lost in hyperspace" problem, and a browsable semantic network supports
users, unsure of the exact query terms they seek. Indexing performance data
is presented for a large document. Analysis methods for indexing Postscript
are discussed, and a general method, with acceptable indexing time, is
proposed for Postscript coming from any source. The wider applicability of
these techniques is discussed
	},
	keywords={
		desktop publishing
		indexing
		information retrieval
		page description languages
		Postscript document management system
		storage format
		C
		portable Display Postscript interpreter
		X Graphics User Interface
		document catalogue
		Boolean query facility
		document viewer
		automatically generated contents list
		alphabetic index
		interactive graphical reading path
		lost in hyperspace problem
		browsable semantic network
		query terms
		indexing performance data
		indexing time
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{McNeill96,
	author={McNeill, M.D.J. and White, M. and Lister, P.F.},
	title={
Graphics codesign for multimedia systems
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={667-74 vol.2},
	abstract={
The design of graphics systems for multimedia applications requires a
wealth of considerations regarding hardware/software trade-offs and
price/performance issues. Often a family of architectures is designed to
cover a broad range of performance abilities and provide a clear path for
future products. We present a codesign environment targeted specifically at
the graphics accelerator market. GALADRIEL allows the design, test and
simulation of architectures on the desktop using a library of reusable
components and technology databases. Each functional component has one or
more implementations (in software and/or a high level hardware description
language) and associated performance metrics to permit the investigation of
price/performance issues at a number of stages throughout the design
process. A novel cosimulation technique is employed to verify designs
	},
	keywords={
		computer graphic equipment
		computer graphics
		hardware description languages
		high level synthesis
		multimedia computing
		software reusability
		graphics codesign
		multimedia systems
		graphics systems design
		multimedia applications
		hardware/software trade-offs
		price/performance issues
		performance abilities
		future products
		codesign environment
		graphics accelerator market
		GALADRIEL
		reusable components
		technology databases
		functional component
		high level hardware description language
		performance metrics
		design process
		novel cosimulation technique
		design verification
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Davenport96,
	author={Davenport, D.},
	title={
On computation and its relation to cognition
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={657-66 vol.2},
	abstract={
Many people now view the human mind as a sort of computer, but what exactly
does that entail? The paper examines the general notion of computation and
its relationship to cognition. The necessarily functional perspective that
it presents, is shown to be coherent with the arguments of J. Searle (1990;
1992) and S. Harnad (1995). One interesting consequence of these views is
that the concept of formal symbol systems is seen to be compatible with
computation in general, including connectionism, not just the symbolic view
it is normally associated with
	},
	keywords={
		artificial intelligence
		cognitive systems
		neural nets
		philosophical aspects
		cognition
		human mind
		computation
		functional perspective
		formal symbol systems
		connectionism
		symbolic view
		artificial intelligence
		philosophical foundations
		chinese room
		symbol grounding
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Ucoluk96,
	author={Ucoluk, G.},
	title={
Level of consciousness as an evaluation criteria for natural and artificial
intelligence: a life independent approach
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={651-5 vol.2},
	abstract={
It is argued that a false value assertion is made by referring to Life' as
valuable. Consciousness' is proposed instead. A Life' independent
definition of consciousness' is given and the components for a measure of
the level of consciousness' are introduced. A brief discussion follows on
some ethical problems that arise
	},
	keywords={
		artificial intelligence
		philosophical aspects
		professional aspects
		social aspects of automation
		consciousness level
		evaluation criteria
		artificial intelligence
		natural intelligence
		life independent approach
		false value assertion
		life independent definition
		level of consciousness
		ethical problems
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Cicekli96,
	author={Cicekli, N.},
	title={
A temporal reasoning approach to knowledge-based simulations
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={641-50 vol.2},
	abstract={
A simple logical framework for knowledge based simulation systems is
presented. Special consideration is given to the simulation of systems
which involve discontinuous change. An abbreviated form of R.A. Kowalski
and M. Sergot's (1986) event calculus is introduced as a basis for tackling
the problem and it is extended first with a convention for representing
causal laws, and then to include higher order persistence and potential
events. A logic programming approach to the computational problem is
adopted and a logic program presented which is efficient yet which retains
many of the logical properties of the set of event calculus axioms. It is
hoped that the framework described will serve as a basis of a rule based
simulation system with temporal reasoning facilities
	},
	keywords={
		digital simulation
		knowledge based systems
		knowledge representation
		logic programming
		process algebra
		temporal reasoning
		temporal reasoning approach
		knowledge based simulation systems
		discontinuous change
		causal law representation
		higher order persistence
		potential events
		logic programming approach
		computational problem
		logical properties
		event calculus axioms
		rule based simulation system
		temporal reasoning facilities
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Turhan96,
	author={Turhan, M.},
	title={
A GBML approach to DFA construction and its application to Turkish word
inflection
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={627-40 vol.2},
	abstract={
The construction of the grammar that accepts a given set of strings is a
machine learning problem. In this work it has been shown that genetic based
machine learning (GBML) can successfully be used in the generation of some
grammars. A genetic algorithm (GA) engine is developed and Turkish word
inflection which has an agglutinative nature, is used as the testbed for
the proposed technique. Results for a subset of all word inflections,
namely the noun inflections is presented
	},
	keywords={
		genetic algorithms
		grammars
		learning (artificial intelligence)
		natural languages
		word processing
		GBML approach
		DFA construction
		Turkish word inflection
		grammar generation
		strings
		machine learning problem
		genetic based machine learning
		genetic algorithm engine
		agglutinative nature
		noun inflections
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{El-Den96,
	author={El-Den, J.},
	title={
Suitability of object oriented concepts for computer supported cooperative
work
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={615-26 vol.2},
	abstract={
The paper looks at computer supported cooperative work (CSCW) and how the
object oriented (OO) concepts are introduced to facilitate many of the
concerns that are still under research in CSCW. The paper also looks at an
improved version of a previously presented model for CSCW (J. El-Den,
1995). The paper ends with an example for the model
	},
	keywords={
		abstract data types
		groupware
		object-oriented methods
		object-oriented programming
		object oriented concepts
		computer supported cooperative work
		CSCW
		OO concepts
		groupware
		object classes
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Chi-Ming-Chung96,
	author={Chi-Ming Chung and Shih, T.K. and Shyy, D.Y. and Chun-Chia Wang},
	title={
A graph-theoretical metric for object-oriented software complexity
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={603-14 vol.2},
	abstract={
Software metrics are widely used to measure software complexity and assure
software quality. However, research in the field of the software complexity
of a class hierarchy has not yet been carefully studied. We introduce a
novel factor named URI (Unit Repeated Inheritance) and an important method
named ILT (Inheritance Level Technique) to realize and measure the object
oriented software complexity of a class hierarchy. The approach is based on
the graph theoretical model for measuring the hierarchical complexity in
inheritance relations. The proposed metric shows that inheritance has a
close relation to the object oriented software complexity and reveals that
overuse of repeated (multiple) inheritance will increase software
complexity and be prone to implicit software errors
	},
	keywords={
		graph theory
		inheritance
		object-oriented programming
		software metrics
		software quality
		graph theoretical metric
		object oriented software complexity
		software metrics
		software quality
		class hierarchy
		URI
		Unit Repeated Inheritance
		ILT
		Inheritance Level Technique
		graph theoretical model
		hierarchical complexity
		inheritance relations
		multiple inheritance
		implicit software errors
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Thevenoux96,
	author={Thevenoux, P. and Larouche, G. and Barrat, B.},
	title={
Improving programming re-usability via an object oriented approach in
multi-sensor system evaluation
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={597-601 vol.2},
	abstract={
This paper presents an object-oriented approach used to manage the
performance evaluation of a highly complex multi-sensor system. Emphasis is
placed on the design phase using OMT and the concepts of inheritance and
virtuality are put forward to stress the re-usability factor
	},
	keywords={
		infrared imaging
		inheritance
		object-oriented programming
		performance evaluation
		radar signal processing
		sensor fusion
		software reusability
		software reusability
		object oriented approach
		multisensor system evaluation
		object oriented programming
		performance evaluation
		design phase
		OMT
		inheritance
		virtuality
		radar
		IR camera
		range laser
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Van-Bommel96,
	author={Van Bommel, M.},
	title={
Operations on incremental multiple inheritance hierarchies
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={589-95 vol.2},
	abstract={
Emerging programming and database definition languages permit the
declaration of multiple inheritance hierarchies. The efficient computation
of lattice operations on hierarchies for large software systems is a
difficult problem. Permitting incremental update of the hierarchy further
complicates the issue. Presented is a technique for the efficient encoding
of multiple inheritance hierarchies in an incremental fashion. The encoding
builds a mapping to a Boolean lattice of binary words, leading to almost
constant-time lattice operations. Contrary to earlier works only supporting
subsumption computations, the operations of greatest lower bound (GLB) and
least upper bound (LUB) are also supported
	},
	keywords={
		database languages
		database theory
		inheritance
		object-oriented databases
		object-oriented languages
		incremental multiple inheritance hierarchies
		programming languages
		database definition languages
		lattice operations
		large software systems
		Boolean lattice
		binary words
		constant-time lattice operations
		subsumption computations
		greatest lower bound
		least upper bound
		class hierarchy
		object oriented database
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Van-Der-Schoot96,
	author={Van Der Schoot, H. and Ural, H.},
	title={
Deciding deadlock-freedom of daisy-chain protocols by fair reachability
analysis
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={579-88 vol.2},
	abstract={
A relief strategy called fair reachability analysis (Gouda and Han, 1985)
is extended for the verification of daisy-chain protocols, which are
defined in the communicating finite state machine model as networks of
n>or=2 processes with a bidirectional, serial link structure. Fair
reachability analysis is shown to decide the deadlock detection problem for
daisy-chain protocols whose fair reachable global state space is finite. A
sufficient condition for this finiteness is also given
	},
	keywords={
		concurrency control
		finite state machines
		formal verification
		protocols
		reachability analysis
		deadlock-freedom
		daisy-chain protocols
		fair reachability analysis
		protocol verification
		communicating finite state machine model
		bidirectional serial link structure
		deadlock detection problem
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Antonova96,
	author={Antonova, G.S.},
	title={
MTIE estimations for different SONET/SDH synchronization network topologies
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={575-8 vol.2},
	abstract={
Synchronization is always a problem of different layers in a distributed
system. The essential SONET/SDH features, which are high-speed and pointer
activity, cause problems in applying traditional solutions for clock
synchronization offered for digital networks. This paper introduces the
maximum time interval error (MTIE) estimations for different SONET/SDH
synchronization network topologies. These estimations were done by
experiments with the universal model of the synchronization network,
obtained using a simulation method, which scientists have not applied
before. The model consists of the primary reference source (PRS) model,
slave clock model, represented by phase-locked loop (PLL), and
synchronization link model. MTIE estimations were obtained for four
different synchronization network topologies
	},
	keywords={
		clocks
		errors
		phase locked loops
		SONET
		synchronisation
		synchronous digital hierarchy
		timing
		SONET
		SDH
		synchronization network topologies
		distributed system
		pointer activity
		clock synchronization
		maximum time interval error estimations
		simulation method
		primary reference source model
		slave clock model
		phase-locked loop
		synchronization link model
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Kutlu96,
	author={Kutlu, A. and Ekiz, H. and Baba, M.D. and Powner, E.T.},
	title={
Implementation of "Comb" based wireless access method for control area
network
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={565-73 vol.2},
	abstract={
Wireless communication, within the context of industrial applications, is
an important issue for accessing the sensors and actuators through a
wireless channel. More importantly, the question of interest is to operate
in the broadcast mode, where any node needs to receive the data from any
other node within the coverage area of each other. In this paper, the
"Comb" based wireless access method is implemented for the control area
network (CAN) which is a half duplex, serial data communication protocol
for automotive and industrial applications. In this scheme, the transmitter
node generates a binary sequence-known as a comb-before the actual frame to
solve the contention situation. If the message has a higher priority, it is
transmitted before any other messages without cancelling the transmission.
Following a general description of the control area network, the Comb based
wireless access method is presented. The results obtained from the
simulations are given
	},
	keywords={
		actuators
		binary sequences
		data communication
		industrial control
		protocols
		sensors
		wireless LAN
		Comb
		wireless access method
		control area network
		wireless communication
		industrial applications
		sensors
		actuators
		broadcast mode
		half duplex serial data communication protocol
		automotive applications
		transmitter node
		binary sequence
		simulations
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Calamoneri96,
	author={Calamoneri, T. and Petreschi, R.},
	title={
Visual representations of Trivalent Cayley Interconnection Networks
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={555-64 vol.2},
	abstract={
We deal with Trivalent Cayley Interconnection Networks and we present two
new representations of them emphasizing their geometric characteristics,
both on the three-dimensional space and on the bidimensional grid. Looking
inside these representations, we solve two problems related to them: the
optimal area layout and the shortest routing problem
	},
	keywords={
		geometry
		graph theory
		multiprocessor interconnection networks
		network routing
		optimisation
		visual representations
		Trivalent Cayley Interconnection Networks
		geometric characteristics
		three-dimensional space
		3D space
		bidimensional grid
		optimal area layout
		shortest routing problem
		graph theory
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Altinay96,
	author={Altinay, O. and Tulunay, E. and Tulanay, Y.},
	title={
On data organization, training strategy and network size when using neural
networks for identification purposes
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={551-4 vol.2},
	abstract={
Multilayer perceptrons are employed for nonlinear system identification.
This short communication, which is a product of experience gained in such
identification effort, presents comments on data organization, neural
network training strategy and network complexity. Points discussed lead to
justifiable results in general
	},
	keywords={
		backpropagation
		data handling
		feedforward neural nets
		identification
		multilayer perceptrons
		data organization
		training strategy
		network size
		neural networks
		network complexity
		multilayer perceptrons
		nonlinear system identification
		backpropagation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Birol96,
	author={Birol, I. and Hacinhyan, A. and Ziya Perdahct, N.},
	title={
Choice of time steps in simulating chaotic systems
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={543-9 vol.2},
	abstract={
Overflows caused by the positive Lyapunov exponents of chaotic systems are
the principal source of error in their simulation. In this work, it is
shown that the Wiesel (1993) algorithm for Lyapunov exponent calculation
represents a system which exactly maintains an orthonormal basis for the
tangent flow. The choice of simulation time steps for chaotic systems is
also considered. Suggested bounds for the time step are validated for the
Lorenz (1963) and Rossler (1976) systems
	},
	keywords={
		chaos
		error analysis
		integration
		Lyapunov matrix equations
		simulation
		time steps
		chaotic systems simulation
		positive Lyapunov exponents
		error
		Lyapunov exponent calculation
		orthonormal basis
		tangent flow
		numerical integration
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Genc96,
	author={Genc, I. and Guzelis, C.},
	title={
One-dimensional signal recognition by two-dimensional dynamical arrays
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={535-42 vol.2},
	abstract={
This paper gives a general approach to one-dimensional (1-D) signal
recognition by means of two-dimensional (2-D) arrays of dynamical cells.
The 2-D arrays are used for transforming feature signals obtained in a
feature extraction stage into 2-D feature signals which are easy to be
classified. The motivation of using 2-D dynamical arrays for 1-D signals is
mainly biological. It is known that many biological neural networks in the
cerebral cortex of the brain are indeed 2-D layers of dynamical neurons
interconnected through lateral feedback and that they define some
topological feature maps. Kohonen's phoneme map is such an example
introduced as a simplification of the human auditory cortex. Another
motivation comes from the fact that some 2-D artificial neural networks
such as Kohonen's self organizing feature map are very suitable for
nonlinear data projection to visualize high dimensional data in pattern
recognition. This paper extends the classical recognition systems in two
directions: the proposed 2-D arrays are dynamical as opposed to the
existing algebraic ones allowing time varying signals; feature signals to
be processed are extracted from 1-D signals by a transformation which might
be nonlinear and/or dynamical. As a specific application acoustic alarm
signal classification is presented in the paper, so that discrete wavelet
transformation (DWT) is used for extracting feature signals and cellular
neural networks (CMNs) as 2-D dynamical arrays
	},
	keywords={
		acoustic signal processing
		alarm systems
		arrays
		brain models
		cellular neural nets
		feature extraction
		pattern classification
		self-organising feature maps
		wavelet transforms
		one-dimensional signal recognition
		1D signal recognition
		two-dimensional dynamical arrays
		2D dynamical arrays
		feature signals
		feature extraction
		biological neural networks
		cerebral cortex
		brain
		cellular neural networks
		lateral feedback
		topological feature maps
		phoneme map
		human auditory cortex
		neural networks
		self organizing feature map
		nonlinear data projection
		pattern recognition
		data visualization
		time varying signals
		acoustic alarm signal classification
		discrete wavelet transformation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Gulmezoglu96,
	author={Gulmezoglu, M.B. and Keskin, M. and Barkana, A.},
	title={
Isolated word-recognition with a neural network which extracts personal
differences
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={527-34 vol.2},
	abstract={
A voice signal contains psychological and physiological properties of the
person as well as the dialect differences, the acoustical environment
effects and the phase differences. For these reasons the same word uttered
by different speakers can be very different. In this paper, a neural
network (NN) is developed to extract the common properties of a spoken word
which is represented as a vector. The inputs of the NN are formed from the
Energy+Cepstral (ECEP) parameters which are derived from the time domain
samples. The outputs of the NN are the elements of the common vector and
this vector is used in isolated word recognition. The weights in the NN are
the elements of the orthonormal vectors
	},
	keywords={
		neural nets
		psychology
		speech recognition
		vectors
		isolated word recognition
		neural network
		personal difference
		voice signal
		psychological properties
		physiological properties
		dialect
		acoustical environment
		phase difference
		vector
		time domain samples
		orthogonalization
		weights
		orthonormal vectors
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Sagiroglu96,
	author={Sagiroglu, S.},
	title={
Identification of linear dynamic systems using multi-layered perceptrons
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={517-26 vol.2},
	abstract={
The identification of dynamic systems can be carried out by means of
feedforward neural networks or recurrent neural networks. Multilayered
perceptrons, as feedforward networks, are versatile and relatively simple
to implement. This paper describes the use of multilayered perceptrons to
identify linear dynamic systems. Both the order and parameters of the
systems to be identified are unknown. The structure of a neural network
capable of dealing with systems of up to a given maximum order i is
detailed. Such a network is termed an i-th order network. Results of
computer simulations using a 5th-order network to identify systems of up to
the 5th order are presented
	},
	keywords={
		control system analysis computing
		digital simulation
		feedforward neural nets
		identification
		linear systems
		multilayer perceptrons
		linear dynamic systems identification
		multilayered perceptrons
		feedforward neural networks
		unknown system order
		unknown parameters
		computer simulations
		5th-order network
		backpropagation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Henson96,
	author={Henson, M.C.},
	title={
Vernacular rules for general recursion
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={507-16 vol.2},
	abstract={
We present rules for the informal construction of programs by general
recursion and explore a proof-theoretic interpretation of these
constructions within a non-extensional constructive theory of operations
and types. We present a result (the adequacy theorem) which guarantees that
interpretable constructions are correct. This work contributes to the study
of informal mathematical arguments
	},
	keywords={
		programming theory
		recursive functions
		set theory
		vernacular rules
		general recursion
		informal program construction
		proof-theoretic interpretation
		nonextensional constructive theory
		operations
		types
		adequacy theorem
		interpretable constructions
		correctness guarantee
		informal mathematical arguments
		constructive set theory
		intensional semantics
		program derivation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Godskesen96,
	author={Godskesen, J.C.},
	title={
Telecommunications service validation and interaction detection
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={495-505 vol.2},
	abstract={
The major contribution of this paper is a technique that allows for early
off-line validation of telecommunications services and detection of
unintended interaction between them. The technique utilizes the
standardized specification languages SDL (Specification and Description
Language, MSC (Message Sequence Charts) and TTCN (Tree and Tabular Combined
Notation), and the commercially available specification tools SDT and ITEX.
Telecommunications services have traditionally been validated online by
means of testing at a rather late stage in the development process. With
the technique advocated in this paper, services may, as a supplement to the
traditional approach, be validated and interaction detected already at the
design phase. In the paper, we show how each of the services Call-Waiting
and Call-Forward-on-Busy can be specified as an extension of the core
telecommunications service Basic-Call. We indicate how service validation
and test case generation from the validated service specifications can be
carried out by tool support. Finally, we demonstrate how the derived test
cases can be used for detecting service interaction on a combined
specification of Call-Waiting and Call-Forward-on-Busy
	},
	keywords={
		formal verification
		project support environments
		specification languages
		telecommunication computing
		telecommunication services
		telephony
		telecommunications service validation
		unintended interaction detection
		early off-line validation
		standardized specification languages
		SDL
		MSC
		TTCN
		commercially available specification tools
		SDT
		ITEX
		design phase
		Call-Waiting
		Call-Forward-on-Busy
		Basic-Call service
		test case generation
		Specification and Description Language
		Message Sequence Charts
		Tree and Tabular Combined Notation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Hadj-Rabia96,
	author={Hadj-Rabia, N. and Habrias, H.},
	title={
Formal specification from NIAM model: a bottom up approach
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={483-94 vol.2},
	abstract={
Presents automatic techniques for generating B specifications from a NIAM
(Natural-language Information Analysis Method) model. Specifications
contain not only the data structure of the NIAM model but also some basic
operations according to graphical constraints. We describe a bottom-up
approach to specify the dynamic aspects of an information system. The use
of this approach should help in finding ambiguities and deficiencies in the
requirements specification and/or in the very high-level specification of
transactions. It should contribute to improvements in the quality of the
programs, because many errors can be detected before implementation
(reification). Furthermore, this can considerably reduce the costs of
testing and maintenance. We illustrate our approach with examples which
show how the specification of our information system can be built through
the specification of its subsystems
	},
	keywords={
		data structures
		error detection
		formal specification
		program testing
		software maintenance
		software quality
		transaction processing
		formal specification
		NIAM model
		bottom-up approach
		automatic B specification generation
		Natural-Language Information Analysis Method
		data structure
		basic operations
		graphical constraints
		information system dynamics
		ambiguities
		deficiencies
		requirements specification
		very high-level specification
		transactions
		program quality
		error detection
		reification
		software testing costs
		software maintenance costs
		implementation
		subsystem specification
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Drias96,
	author={Drias, H.},
	title={
Counting and testing satisfiability
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={473-82 vol.2},
	abstract={
In this paper, we propose a new algorithm for computing solutions of
satisfiability. It is then slightly modified to solve the corresponding
decision problem. Probabilistic analyses are performed and show average
polynomial time complexity for both cases. A comparison with algorithm "IS"
proposed by J. Franco (1986) and previous works on SAT show that our
results outperform these other algorithms
	},
	keywords={
		computability
		computational complexity
		decision theory
		probability
		satisfiability testing
		decision problem
		probabilistic analyses
		average polynomial time complexity
		algorithm IS
		algorithm performance
		solution counting
		checking
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Turner96,
	author={Turner, K.J. and McClenaghan, A. and Chan, C.},
	title={
Specification and animation of reactive systems
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={355-64 vol.1},
	abstract={
SOLVE (Specification using an Object-based, LOTOS-defined, Visual language)
is designed to allow formal requirements capture, particularly for reactive
systems. The SOLVE language is object-based, and formally defined using
LOTOS (Language Of Temporal Ordering Specification). SOLVE is supported by
tools that allow direct visual animation of systems specified in this
language. Animation is supported by translating a SOLVE specification
automatically into a LOTOS specification, and then graphically simulating
this. A further application is embodied in the XDILL tool that supports
requirements specification and visual animation of digital logic circuits.
Several illustrative SOLVE examples are given
	},
	keywords={
		computer animation
		data visualisation
		engineering graphics
		formal specification
		logic CAD
		logic circuits
		object-oriented languages
		specification languages
		visual languages
		reactive systems
		formal requirements capture
		specification
		object-based LOTOS-defined visual language
		SOLVE language
		direct visual animation
		automatic SOLVE specification translation
		LOTOS specification
		graphical simulation
		XDILL tool
		visual animation
		digital logic circuits
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Dalkilic96,
	author={Dalkilic, M.E.},
	title={
Register and function unit binding in architecture synthesis
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={225-34 vol.1},
	abstract={
One of the primary jobs in translating a behavioral specification into a
register-transfer level architecture is binding. Typically, binding follows
operation scheduling and is composed of three strongly interrelated NP-hard
subtasks: function unit (FU) binding, register binding, and interconnect
binding. Register binding (assignment of variables to registers) and FU
binding (assignment of operations to function units) problems are
addressed. Register and FU binding algorithms based on a bipartite matching
model are presented. The goal is to find a binding which minimizes the
hardware cost. The FU and register binding algorithms are implemented and
they compare favourably to other approaches
	},
	keywords={
		computer architecture
		logic design
		processor scheduling
		architecture synthesis
		behavioral specification translation
		register-transfer level architecture
		function unit binding
		register unit binding
		operation scheduling
		NP-hard subtasks
		interconnect binding
		binding algorithms
		bipartite matching model
		minimized hardware cost
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Ozer96,
	author={Ozer, E. and Orencik, B. and Akyokus, S.},
	title={
An imprecise interrupt handling scheme in superscalar processors
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={207-12 vol.1},
	abstract={
An imprecise interrupt handling mechanism is proposed for superscalar
processors which employ out-of-order issue and out-of-order execution
policies to achieve high performance. The proposed scheme is based on
inserting shadow latch stacks between stages of processor pipelines to save
processor contexts. This scheme is especially useful to accommodate nested
interrupts
	},
	keywords={
		interrupts
		pipeline processing
		reduced instruction set computing
		imprecise interrupt handling scheme
		superscalar processors
		out-of-order issue policies
		out-of-order execution policies
		high performance system
		shadow latch stacks
		processor pipelines
		processor context saving
		nested interrupts
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Giloi96,
	author={Giloi, W.K. and Lindemann, C. and Pletner, S.},
	title={
Performance modeling of novel node architectures for multiprocessor systems
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={213-23 vol.1},
	abstract={
We analyze the performance of several design alternatives for the node
architecture of two innovative distributed memory parallel architectures:
the 2-processor node of MANNA and the 4-processor node of META. The
analysis is based on the use of deterministic and stochastic Petri nets.
The MANNA node architecture features two processors, the application
processor and the communication processor, which share the node memory via
a bus. The aim of the META design is a node that allows for a
multi-threaded architecture with several threads being executed in
parallel. Therefore, the META node consists of several processors and
several memory units connected through a crossbar. The purpose of the study
is to provide a basis for the node design decisions by providing
quantitative results concerning processor and memory utilization for
several design alternatives. These quantitative results can also be
utilized for the validation of results obtained by a detailed hardware
simulation study
	},
	keywords={
		distributed memory systems
		multiprocessor interconnection networks
		multiprogramming
		parallel architectures
		performance evaluation
		Petri nets
		stochastic processes
		virtual machines
		performance modeling
		novel node architectures
		multiprocessor systems
		distributed memory parallel architectures
		two-processor node
		MANNA
		four-processor node
		META
		deterministic Petri nets
		stochastic Petri nets
		application processor
		communication processor
		bus
		multi-threaded architecture
		memory units
		crossbar
		node design
		validation
		hardware simulation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Kant96,
	author={Kant, M.},
	title={
The twisted d-cube and the folded hypercube, two interesting topologies for
efficient routing
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={197-205 vol.1},
	abstract={
In this paper, the problem of routing messages along a shortest path in the
folded hypercube and the twisted d-cube is considered. Boolean routing
schemes are proposed for them, and two algorithms are presented for the
one-to-one routing on a shortest path between source and destination. The
authors prove that the space complexity for the storage of the
communication information is O(2/sup d/) bits for the twisted d-cube, and
O(2/sup n/(n-s)) bits for the folded hypercube FHC(n)
	},
	keywords={
		Boolean functions
		communication complexity
		distributed algorithms
		graph theory
		hypercube networks
		message passing
		multiprocessor interconnection networks
		network routing
		twisted d-cube
		folded hypercube
		routing topology
		message routing
		shortest path
		Boolean routing schemes
		distributed algorithms
		one-to-one routing
		space complexity
		communication information storage
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Birecik96,
	author={Birecik, S. and Kurugollu, F.},
	title={
Comparison of thresholding methods for morphological edge detection
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={193-6 vol.1},
	abstract={
In this paper, the binary morphological edge detection method is compared
with other well-known edge detection methods in the literature. Different
thresholding methods are used to binarize test images, then morphological
edge detection is performed on the resulting images, and the figure of
merit for measuring the performance of the edge detector is calculated
	},
	keywords={
		edge detection
		mathematical morphology
		software performance evaluation
		thresholding methods
		binary morphological edge detection method
		image binarization
		figure of merit
		edge detector performance measurement
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Starovoitov96,
	author={Starovoitov, V.},
	title={
On qualitative comparison of methods for low-level image processing
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={189-92 vol.1},
	abstract={
A new measure of dissimilarity between grey-scale images is presented. It
may be used for the comparison of algorithms devoted to the same task, like
edge-preserving noise smoothing, restoration, edge detection or
thresholding. We consider the requirements of the measure and propose a
multilevel measure design. Each level of the measure calculation
(pixel-to-pixel, pixel-to-window, window-to-window and image-to-image) is
based on different distance values. Experimental results with real images
illustrate the performance of the proposed measure as a comparator
	},
	keywords={
		image processing
		low-level image processing methods
		image dissimilarity measure
		grey-scale images
		algorithm comparison
		edge-preserving noise smoothing
		image restoration
		edge detection
		thresholding
		multilevel measure design
		pixel-to-pixel level
		pixel-to-window level
		window-to-window level
		image-to-image level
		distance values
		performance
		digital images
		method comparison
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Erdogan96,
	author={Erdogan, A. and Leblebicioglu, K. and Halici, U. and Atalay, V.},
	title={
Extraction of optimal texture features by a genetic algorithm
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={183-8 vol.1},
	abstract={
This paper describes an approach for the supervised segmentation of images.
Optimal local texture features are determined by a genetic algorithm.
Several feature measures, most of which are based on the co-occurrence
matrix, are suggested as basic texture measures. In the training phase,
optimum ranges of these measures are determined on an image containing
known texture regions. The genetic algorithm is of the elitist type and
employs "roulette wheel selection" with fitness scaling
	},
	keywords={
		feature extraction
		genetic algorithms
		image segmentation
		image texture
		matrix algebra
		optimal texture feature extraction
		elitist genetic algorithm
		supervised image segmentation
		local texture features
		feature measures
		cooccurrence matrix
		training phase
		optimum ranges
		known texture regions
		roulette wheel selection
		fitness scaling
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Ozcan96,
	author={Ozcan, E. and Mohan, C.K.},
	title={
Simulated annealing and genetic algorithms for partial shape matching
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={173-81 vol.1},
	abstract={
Partial shape matching may be viewed as an optimization problem, to be
solved using methods such as simulated annealing (SA) and genetic
algorithms (GAs). We apply and compare both these methods for matching
input shapes with model shapes described in terms of features such as line
segments and angles. The quality of matching is gauged using a measure
derived from attributed shape grammars. Current results show that both SA
and GAs succeed in the shape matching task. A GA is faster and yields the
global optimum more often than the versions of SA implemented
	},
	keywords={
		attribute grammars
		genetic algorithms
		image matching
		simulated annealing
		simulated annealing
		genetic algorithms
		partial shape matching
		optimization
		input shape matching
		model shapes
		line segments
		angles
		matching quality
		attributed shape grammars
		global optimum
		pattern recognition
		attributed strings
		evolutionary computing
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Kapus96,
	author={Kapus, T. and Brezocnik, Z.},
	title={
Incorporating real time into a concurrent temporal logic of actions
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={163-72 vol.1},
	abstract={
Although the temporal logic of actions (TLA) is not a real-time temporal
logic by definition, it can be employed for specifying and verifying
real-time properties by interpreting an ordinary variable of the logic as
representing real time. Models of TLA formulae are state (and also action)
sequences. We call a temporal logic, similar to TLA, whose models are some
partially ordered state (and also action) sets, a "concurrent temporal
logic of actions". Due to the structure of its models, an originally
non-real-time concurrent temporal logic of actions cannot express real-time
properties. This paper, however, shows that time can be incorporated into
it by introducing a special variable
	},
	keywords={
		distributed algorithms
		formal specification
		formal verification
		real-time systems
		sequences
		set theory
		temporal logic
		concurrent temporal logic of actions
		real-time properties specification
		real-time properties verification
		state sequences
		action sequences
		partially ordered sets
		posets
		variable
		true concurrency
		partial order runs
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Levin96,
	author={Levin, V. and Bounimova, E. and Basbugoglu, O. and Inan, K.},
	title={
A bilingual specification environment for software/hardware co-design
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={153-62 vol.1},
	abstract={
A new bilingual specification environment consisting of the two languages
SDL and S/R is described. The new design is based on the SDL-to-S/R
compiler that was implemented at a previous phase and introduces the
necessary interface semantics as restrictions on special SDL shell
processes that encapsulate the interfaced S/R modules. The environment can
be used in SW/HW co-design by involving the verification engine COSPAN
geared to the S/R language specification
	},
	keywords={
		formal specification
		formal verification
		logic design
		program compilers
		specification languages
		systems analysis
		bilingual specification environment
		software hardware co-design
		SDL
		S/R
		specification languages
		compiler
		interface semantics
		shell processes
		verification engine
		COSPAN
		Specification and Description Language
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Zamulin96,
	author={Zamulin, A.V.},
	title={
Algebraic specification of an Oberon compiler
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={143-52 vol.1},
	abstract={
A case study of the application of the algebraic specification technique to
the formal definition of a real-world-language compiler has been performed.
The programming language Oberon has been chosen for the purpose. Some
results of the study are presented in the paper. The main attention is
given to the formal definition of compiler data structures and semantic
functions mapping an Oberon program into a term of an abstract target
machine
	},
	keywords={
		algebraic specification
		data structures
		object-oriented languages
		object-oriented programming
		program compilers
		algebraic specification
		Oberon compiler
		formal definition
		programming language
		compiler data structures
		semantic functions
		abstract target machine
		object oriented language
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Varpaaniemi96,
	author={Varpaaniemi, K.},
	title={
Finding small stubborn sets automatically
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={133-42 vol.1},
	abstract={
State space generation is often needed in the analysis of concurrent and
distributed systems. The stubborn set method is one of the techniques that
try to alleviate the state space explosion encountered in state space
generation. An algorithm for finding a stubborn set having as few enabled
transitions as possible is presented. The practicality of the algorithm is
motivated with the aid of examples
	},
	keywords={
		distributed algorithms
		formal verification
		graph theory
		minimisation
		systems analysis
		stubborn set method
		state space generation
		concurrent systems
		distributed systems verification
		systems analysis
		state space explosion
		distributed algorithm
		graph theory
		minimisation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Ping-Kuen-Chen96,
	author={Ping-Kuen Chen and Gwo-Dong Chen and Jorng-Tzong Horng},
	title={
A hierarchical view mechanism for supporting a navigation query in
object-oriented databases
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={123-32 vol.1},
	abstract={
When a manager in a company wants to know what is going on, he always needs
to read the summary reports then goes on to different levels of detail for
interesting areas found in the summary reports. However, managers usually
cannot deal with a complex database schema and a sophisticated query
language. Therefore, a hierarchical view mechanism and navigation query
facilities are required so that a manager can just click buttons and find
the data he wants. Existing database view mechanisms do not support this.
We propose a hierarchical view mechanism for users to navigate and locate
data from levels of summary data to levels of detail
	},
	keywords={
		business data processing
		human factors
		object-oriented databases
		query languages
		query processing
		user interfaces
		hierarchical view mechanism
		navigation query
		object-oriented databases
		manager
		company
		summary reports
		complex database schema
		query language
		database view mechanisms
		levels of detail
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Bostan96,
	author={Bostan, B. and Yazici, A.},
	title={
UDOOM: uncertainty in deductive object-oriented data modeling
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={113-22 vol.1},
	abstract={
Uncertainty modeling and manipulation is required in deductive
object-oriented models to handle complex objects with uncertain properties.
The authors propose a data model called UDOOM for not only representing
complex objects and having deduction capabilities but also for handling
uncertainty
	},
	keywords={
		deductive databases
		object-oriented databases
		uncertainty handling
		uncertainty modeling
		uncertainty manipulation
		deductive object-oriented data modeling
		complex object handling
		uncertain properties
		UDOOM data model
		complex object representation
		deduction capabilities
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Dogac96,
	author={Dogac, A. and Ozhan, G. and Kilic, E. and Ozcan, F. and Nural, S. and Mancuhan, S. and Dengi, C. and Koksal, P. and Halici, U. and Arpinar, B. and Evrendilek, C. and Sadjadi, V.},
	title={
An interoperability infrastructure for developing multidatabase systems
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={103-12 vol.1},
	abstract={
A multidatabase system (MDBS) allows the users to simultaneously access
autonomous, heterogenous databases using a single data model and a query
language. This provides for achieving interoperability among heterogeneous,
federated DBMSs. The authors describe the interoperability infrastructure
of a multidatabase system, namely METU interoperable DBMS (MIND). The
architecture of MIND is based on the OMG distributed object management
model. It is implemented on top of a CORBA compliant ORB, namely,
ObjectBroker. The interface of the generic database object is defined in
CORBA IDL and multiple implementations of this interface, one for each
component DBMSs, namely, Oracle7, Sybase, Adabas D and MOOD (METU
Object-Oriented Database System) are provided. The main components of MIND
which are built on this infrastructure are a global query manager, a global
transaction manager, a schema integrator, interfaces to supported database
systems and a graphical user interface
	},
	keywords={
		distributed databases
		graphical user interfaces
		object-oriented databases
		open systems
		query languages
		query processing
		transaction processing
		multidatabase system development
		interoperability infrastructure
		simultaneous autonomous heterogenous database access
		data model
		query language
		federated DBMS
		METU interoperable DBMS
		architecture
		OMG distributed object management model
		CORBA compliant ORB
		ObjectBroker
		generic database object interface
		CORBA IDL
		interface
		Oracle7
		Sybase
		Adabas D
		MOOD
		global query manager
		global transaction manager
		schema integrator
		graphical user interface
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Aniorte96,
	author={Aniorte, P. and Meyranx, J.},
	title={
Terminological database design: an approach based on the use of conceptual
graphs
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={93-102 vol.1},
	abstract={
A considerable interest in terminological databases is emerging in many
fields of research. Nevertheless, little work has been done on such
databases. The authors' objective is to propose an approach for database
design, based on the conceptual graph theory, which has the ability to
model the semantics of an application domain, and which proves to be
well-suited to the terminologist's approach
	},
	keywords={
		database management systems
		database theory
		graph theory
		nomenclature
		tree data structures
		terminological database design
		conceptual graphs
		semantics modelling
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Gultekin96,
	author={Gultekin, A. and Gokmen, M.},
	title={
Adaptive shape from shading
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={83-92 vol.1},
	abstract={
Extracting surface orientation and surface depth from one or more images is
a classic problem in computer vision. Shape-from-shading (SFS) deals with
the recovery of 3D shape from a single shaded image. The shape is recovered
by minimizing an energy functional involving constraints such as
smoothness. In this constrained problem, although the smoothness constraint
helps to stabilize the minimization process, it pushes the reconstruction
toward a smooth surface. The authors present a new adaptive
shape-from-shading method which reduces this oversmoothing by controlling
the smoothness spatially over the image space. In order to improve the
quality of the reconstruction, they also integrated this adaptive SFS
algorithm and photometric stereo technique to recover shape by using more
than one input image. The new algorithm is robust, data driven and updates
both the gradient field and height map simultaneously. A hierarchical
implementation of the algorithm is used to speed up the iterative scheme.
Typical SFS and photometric stereo results are given to illustrate the
usefulness of the approach
	},
	keywords={
		computer vision
		image reconstruction
		stereo image processing
		surface orientation extraction
		surface depth extraction
		computer vision
		adaptive shape from shading
		3D shape recovery
		shaded image
		minimized energy functional
		constraints
		smoothness
		reconstruction
		oversmoothing
		photometric stereo technique
		adaptive algorithm
		input image
		gradient field updating
		height map updating
		iterative scheme
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Cloppet96,
	author={Cloppet, F. and Stamon, G.},
	title={
Analysis of images of cells with neurites
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={73-81 vol.1},
	abstract={
The study is concerned with segmentation of cytological images and
extraction of cellular entities in order to provide quantitative data about
the number of cells in culture (statistical tests, morphology, model of
evolution, etc....). This quantitative data is useful in biology to
evaluate the consequences of the application of active substances on
morphological changes and cellular viability. The authors have implemented
algorithms to extract cell contours and to split and merge each contour in
order to obtain individual cells at the end of the analysis process
	},
	keywords={
		biology computing
		cellular biophysics
		computational geometry
		edge detection
		image segmentation
		neurites
		cell image analysis
		cytological image segmentation
		cellular entity extraction
		quantitative data
		culture
		biology
		active substance application
		morphological changes
		cellular viability
		algorithms
		cell contour extraction
		contour splitting
		contour merging
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Carkacioglu96,
	author={Carkacioglu, A. and Yarman-Vural, F.T.},
	title={
Markov random fields texture similarity
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={63-72 vol.1},
	abstract={
The paper deals with a class of textures which can be represented by a
Markov random fields (MRF) model. Although the MRF model has been
successfully employed for many texture generation and classification
problems, numerical studies indicate that the success of the results
heavily depends on the texture type. Binary textures are generated by the
MRF model and examined for various texture alphabets. The study introduces
new concepts, namely, base clique, base clique chain and n/sup th/ order
clique chain. These concepts are then used to define mean clique length
(MCL) and clique standard deviation (CSD) as measures of texture. The
association between the appearance of texture and the texture measures is
investigated. The simulation experiments are performed on various texture
alphabets to quantify the data type by using the MCL and CSD texture
measures. The factors that shape the structure of the texture are
investigated
	},
	keywords={
		image classification
		image texture
		Markov processes
		random processes
		Markov random fields model
		texture similarity
		texture generation
		texture classification
		texture type
		binary textures
		texture alphabet
		base clique
		base clique chain
		nth order clique chain
		mean clique length
		clique standard deviation
		texture measures
		simulation
		data type
		image processing
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Ekinci96,
	author={Ekinci, M. and Thomas, B.T.},
	title={
Multi-camera vision-based navigation of autonomous road vehicles in complex
road networks
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={53-62 vol.1},
	abstract={
Presents a computer vision system for an autonomous road vehicle (ARV) that
is capable of negotiating complex road junctions and intersections in real
time. The roads are detected from a sequence of monochromatic images
captured by a multi-video-camera. A model-based object approach is used for
detecting the road junctions in images. In this approach, the results of a
region-growing segmentation process and an edge detection process using
edge segments are fused based on a model voting strategy to locate the road
junction surface. A multi-camera vision-based re-orientation mode has been
used to guide the ARV during the turning process. Results are presented for
real road intersection images and performed on the experimental ARV in real
time
	},
	keywords={
		computerised navigation
		edge detection
		image segmentation
		image sequences
		mobile robots
		real-time systems
		road vehicles
		robot vision
		sensor fusion
		traffic control
		multi-camera vision-based navigation
		autonomous road vehicles
		complex road networks
		computer vision
		complex road junctions
		road intersection images
		real-time computing
		monochromatic image sequence
		road detection
		multi-video-camera
		model-based object approach
		region-growing segmentation process
		edge detection process
		edge segments
		data fusion
		model voting strategy
		road junction surface location
		vision-based reorientation mode
		turning process
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Groote96,
	author={Groote, J.F. and van Maaren, H.},
	title={
Equivalence of the concave optimisation method and d'Agostino's tableaux
for propositional logic
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={41-51 vol.1},
	abstract={
Both d'Agostino's (1992) tableau system and the optimisation of concave
associated functions can be used to determine whether formulas in
propositional logic are contradictory, satisfiable or tautological. Both
systems have very different roots and appear incompatible at first sight:
d'Agostino's tableau system comes from the realm of logic, while concave
optimisation is a typical technique that stems from operations research. We
show that both techniques are computationally equivalent, in the sense that
they simulate each other polynomially regarding proof length and proof
search
	},
	keywords={
		computability
		concave programming
		formal logic
		operations research
		theorem proving
		concave optimisation method
		tableaux
		propositional logic
		concave associated functions
		contradictory formulas
		satisfiable formulas
		tautological formulas
		operations research
		computationally equivalent techniques
		polynomial simulation
		proof length
		proof search
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Evans96,
	author={Evans, A.S.},
	title={
An assertional verification method for Z specifications of concurrent
systems
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={29-39 vol.1},
	abstract={
Presents a a set of inference rules for formally proving safety and
liveness properties of extended Z specifications of concurrent systems. The
rules are based on assertional verification techniques but are implemented
in W, the emerging deductive calculus for Z. Thus, they can be verified by
existing Z proof tools. The techniques presented are suitable for
specifying and verifying properties of a variety of concurrent systems
types, including communication-based systems, as is illustrated by the
simple buffer case study presented in this paper
	},
	keywords={
		calculus
		formal logic
		formal specification
		formal verification
		inference mechanisms
		multiprocessing programs
		multiprocessing systems
		safety
		assertional verification method
		extended Z specifications
		concurrent systems
		inference rules
		formal proof
		safety properties
		liveness properties
		W deductive calculus
		Z proof tools
		communication based systems
		buffer
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Orava96,
	author={Orava, F.},
	title={
Formal analysis of a railway interlocking system
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={17-27 vol.1},
	abstract={
A high-level specification of a railway interlocking system expressed in
CCS is presented. Safety-critical properties are formulated in the modal mu
-calculus and verified using the Concurrency Workbench. The main
functionality of the system is to establish safe paths-train routes-through
a railyard. The properties verified express that the routes established are
indeed safe, and that if the conditions for a safe route are fulfilled,
then that route will eventually be established
	},
	keywords={
		calculus of communicating systems
		formal specification
		formal verification
		railways
		safety
		signalling
		formal analysis
		railway interlocking system
		high-level specification
		CCS
		safety-critical properties verification
		modal mu -calculus
		Concurrency Workbench
		safe path establishment
		train routes
		railyard
		railway signalling
		automatic verification
		model checking
		process algebra
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Klaudel96,
	author={Klaudel, H. and Riemann, R.-C.},
	title={
Consistent equivalence notion for a class of high level Petri nets
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={7-16 vol.1},
	abstract={
This paper presents an equivalence relation and a set of transformation
rules on a class of high-level Petri nets, called M-nets, which are
designed as a compact high-level representation of Petri boxes (Best et
al., 1992). Boxes are equivalence classes of labelled Petri nets. As the
main result, it is shown that the set of transformation rules is complete
with respect to the equivalence relation in the finite case
	},
	keywords={
		equivalence classes
		Petri nets
		consistent equivalence notion
		equivalence relation
		transformation rules
		high-level Petri nets
		M-nets
		compact high-level representation
		Petri boxes
		equivalence classes
		labelled Petri nets
		completeness
		finite case
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
/usr/tmp/citation.tmp.28355
@ARTICLE{ReisingDec96,
	author={Reising, S.C. and Inan, U.S. and Bell, T.F. and Lyons, W.A.},
	title={
Evidence for continuing current in sprite-producing cloud-to-ground
lightning
	},
	journal={Geophysical Research Letters},
	volume={23},
	number={24},
	year={1996},
	month={Dec},
	pages={3639-42},
	abstract={
Radio atmospherics launched by sprite-producing positive cloud-to-ground
lightning flashes and observed at Palmer Station, Antarctica, exhibit large
ELF slow tails following the initial VLF portion, indicating the presence
of continuing currents in the source lightning flashes. One-to-one
correlation of sferics with NLDN lightning data in both time and arrival
azimuth, measured with an accuracy of +or-1 degrees at \12,000 km range,
allows unambiguous identification of lightning flashes originating in the
storm of interest. Slow-tail measurements at Palmer can potentially be used
to measure continuing currents in lightning flashes over nearly half of the
Earth's surface
	},
	keywords={
		atmospherics
		lightning
		thunderstorms
		atmosphere
		troposphere
		electric field
		electric current
		continuing current
		sprite-producing cloud-to-ground lightning
		thunderstorm
		atmospherics
		positive cloud-to-ground lightning flash
		Palmer Station
		Antarctica
		large ELF slow tail
		source lightning flash
		sferics
		NLDN lightning
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Al-Ayyoub96,
	author={Al-Ayyoub, A.-E. and Day, K.},
	title={
The hyperstar interconnection network
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={463-72 vol.1},
	abstract={
A multiprocessor interconnection topology, the hyperstar, based on the
Cartesian product of star graphs, is presented. The basic properties of the
hyperstar are discussed and proved. These include reduced degree and
diameter, hierarchical structure, vertex symmetry, optimal routing, and
shortest path characterization. The hyperstar is shown to be a member of
the Cayley class of symmetric graphs. Embeddings of hypercubes, star
graphs, meshes, and Hamiltonian cycles are discussed. An optimal one-to-all
broadcasting algorithm is obtained and analyzed. Furthermore, a comparative
study between the hyperstar and seven related networks is also conducted.
The comparison is based on scalability, communication cost, link
requirements, cost/performance ratio, and other static parameters such as
degree, diameter, and average diameter
	},
	keywords={
		broadcasting
		graph theory
		multiprocessor interconnection networks
		reconfigurable architectures
		hyperstar interconnection network
		multiprocessor interconnection topology
		Cartesian star graphs
		reduced degree
		reduced diameter
		hierarchical structure
		vertex symmetry
		optimal routing
		shortest path characterization
		Cayley symmetric graphs
		embedded hypercubes
		embedded star graphs
		embedded meshes
		Hamiltonian cycles
		optimal one-to-all broadcasting algorithm
		scalability
		communication cost
		link requirements
		cost/performance ratio
		static parameters
		average diameter
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Akgun96,
	author={Akgun, B.T. and Peksen, E. and Harmanci, A.E.},
	title={
Heterogeneous task migration mechanism in BAG distributed real-time
operating system
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={453-62 vol.1},
	abstract={
The task migration facility of the distributed real time operating system,
BAG, is presented. The SDL model has been selected as the real time
programming model. The task migration mechanism of BAG which is essentially
based on user level states, improves performance and also simplifies
problems related to the continuity of message handling. This mechanism has
been separately deviced for homogeneous and heterogeneous systems. The
heterogeneous migration mechanism is specially emphasized
	},
	keywords={
		electronic messaging
		network operating systems
		programming
		real-time systems
		heterogeneous task migration mechanism
		BAG distributed real time operating system
		task migration facility
		SDL model
		real time programming model
		user level states
		message handling
		heterogeneous systems
		homogeneous systems
		heterogeneous migration mechanism
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Al-Mouhamed96,
	author={Al-Mouhamed, M. and Seiden, S. and Abu-Haimed, H.},
	title={
Minimization of memory and network contention for accessing arbitrary
power-of-2 data patterns
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={443-52 vol.1},
	abstract={
Finding general XOR schemes to minimize memory and network contention for
accessing arrays with arbitrary sets of data templates is presented. A
combined XOR matrix is proposed, together with a necessary and sufficient
condition for conflict free access. We present a new characterization of
the baseline network. Finding an XOR matrix for combined templates is shown
to be an NP complete problem. A heuristic is proposed for finding XOR
matrices by determining the constraints of each template matrix and solving
a set of simultaneous equations for each row. Evaluation shows significant
reduction of memory and network contention compared to interleaving and to
static row-column-diagonals storage
	},
	keywords={
		computational complexity
		matrix algebra
		memory architecture
		minimisation
		storage allocation
		storage management
		network contention
		memory contention minimisation
		arbitrary power-of-2 data pattern access
		XOR schemes
		arbitrary sets
		data templates
		combined XOR matrix
		sufficient condition
		conflict free access
		baseline network
		combined templates
		NP complete problem
		heuristic
		template matrix
		simultaneous equations
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Gul96,
	author={Gul, E.},
	title={
A mathematical model for multiprocessor implementation of an algorithm
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={437-42 vol.1},
	abstract={
A mathematical model is derived for a multiprocessor implementation of a
target tracking algorithm. The practical implementation of this algorithm
confirms the results obtained from the model. This analysis is useful to
predict multiprocessor performance of an algorithm
	},
	keywords={
		military computing
		multiprocessing systems
		parallel algorithms
		target tracking
		mathematical model
		multiprocessor implementation
		target tracking algorithm
		practical implementation
		multiprocessor performance
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Gueaieb96,
	author={Gueaieb, W.},
	title={
The practical significance of simple classification rules
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={427-36 vol.1},
	abstract={
The author adopts the classification algorithm T2, derived by Auer et al.
(1995), to show that simple classification algorithms, with decision trees
of depth 2, usually lead to accuracies which are very close to those
produced by complex ones, such as C4.5. As a consequence, the author
suggests that T2 may be used as a challenging practical metric to evaluate
the accuracies of complex classification algorithms. Furthermore, the
author shows how to take advantage of the cases where decision trees, with
low depth and number of leaves, produce close or higher accuracies than
those with higher depth and number of leaves, by showing how to determine
the relative relevance, and detect any possible redundancies among some of
the attributes of the dataset in use
	},
	keywords={
		decision theory
		learning (artificial intelligence)
		pattern classification
		redundancy
		trees (mathematics)
		simple classification rules
		T2 classification algorithm
		simple classification algorithms
		decision trees
		depth 2 algorithms
		accuracies
		practical metric
		complex classification algorithms
		accuracy evaluation
		leaves
		relative relevance
		redundancies
		dataset
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Matwin96,
	author={Matwin, S. and Rouget, T.},
	title={
Explainable induction with an imperfect qualitative model
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={415-25 vol.1},
	abstract={
The paper addresses the problem of learning concept descriptions that are
interpretable/explainable. Explainability is understood as the ability to
justify the learned concept in terms of the existing background knowledge.
The starting point for the work was an existing system that would induce
only fully explainable rules. The system performed well when the model used
during induction was complete and correct. In practice, however, models are
likely to be imperfect, i.e. incomplete and incorrect. The authors report a
new approach that achieves explainability with imperfect models. The basis
of the system is the standard inductive search driven by an
accuracy-oriented heuristic, biased towards rule explainability. The bias
is abandoned when there is heuristic evidence that a significant loss of
accuracy results from constraining the search to explainable rules only.
The user can express their relative preference for accuracy vs.
explainability. Experiments indicate that, even with a partially incomplete
and/or incorrect model, insisting on explainability results in only a small
loss of accuracy. They also show how the new approach can repair a faulty
model using evidence derived from data during induction
	},
	keywords={
		explanation
		heuristic programming
		knowledge based systems
		learning by example
		search problems
		uncertainty handling
		imperfect qualitative model
		concept description learning
		explainable induction
		interpretability
		explainability
		background knowledge
		standard inductive search
		accuracy-oriented heuristic
		rule explainability
		constrained search
		accuracy
		partially incorrect model
		partially incomplete model
		faulty model repair
		evidence
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Arzu-Sigman96,
	author={Arzu Sigman, N. and Alpaslan, F.N. and Yarman Vural, F.T.},
	title={
An Ottoman-Turkish transcription system
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={405-14 vol.1},
	abstract={
A system for transcribing Ottoman text into modern Turkish alphabet is
described. This system utilizes Ottoman text coded by ASCII characters as
input. It is assumed that all the characters in the Ottoman text are
recognized by an OCR system which outputs the Ottoman characters as
ASCII-coded compound structures (i.e. subwords). All the compound
structures that are obtained from the test documents are stored in a
B+-tree which is named OCST (Ottoman Compound Structure Table). All the
transcriptions are produced by the help of the Ottoman-Turkish dictionary,
which is kept as a tree in the memory. The inner nodes of the tree are
Ottoman compound structures and the leaf nodes are Turkish transcriptions.
The output text composed of Turkish transcriptions is produced by
processing the input
	},
	keywords={
		character sets
		computational linguistics
		linguistics
		optical character recognition
		tree data structures
		Ottoman-Turkish transcription system
		Ottoman text transcription
		modern Turkish alphabet
		ASCII characters
		OCR system
		ASCII-coded compound structures
		B+-tree
		Ottoman Compound Structure Table
		OCST
		Ottoman-Turkish dictionary
		inner tree nodes
		leaf nodes
		output text
		input processing
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Bayram96,
	author={Bayram, Z.O.},
	title={
SSST (State-Space Search Tool): a probabilistic forward-chained expert
system shell with full backtracking
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={395-404 vol.1},
	abstract={
The author describes a probabilistic backtracking forward-chained expert
system shell that performs a best-first search of the state-space
consisting of working memory states. The state space that needs to be
traversed can be narrowed significantly through tactful use of the context
mechanism. Fail conditions detect forbidden working memory states and cause
immediate backtracking. Heuristic information about which rules should have
higher priority are encoded in the rules at the granularity level of
condition elements in the form of importance factors. Facts in the working
memory have associated with them confidence factors, which allows the
representation of uncertain information. The paradigm that results as the
combination of this specific set of features permits declarative
specification of the state space required for the solution of many kinds of
scheduling problems and other kinds of problems requiring intelligent
search of the state space with possible backtracking
	},
	keywords={
		backtracking
		expert system shells
		forward chaining
		heuristic programming
		inference mechanisms
		probabilistic backtracking forward-chained expert system shell
		SSST
		State-Space Search Tool
		best-first state-space search
		working memory states
		context mechanism
		fail conditions
		forbidden working memory state detection
		heuristic information
		rule priority
		condition element granularity level
		importance factors
		confidence factors
		uncertain information
		declarative specification
		scheduling problems
		intelligent state space search
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Levin96,
	author={Levin, V. and Bounimova, E. and Inan, K.},
	title={
An interface implementation using a formal compiler specification method
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={385-94 vol.1},
	abstract={
The paper presents a new formal compiler specification method that has
evolved out of a number of realistic applications including the current
application reported in the paper and describes how it is used as a formal
method tool for compiler design and implementation problems
	},
	keywords={
		application program interfaces
		formal specification
		program compilers
		formal compiler specification method
		formal method tool
		compiler design
		interface implementation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Bernardo96,
	author={Bernardo, M. and Donatiello, L. and Gorrieri, R.},
	title={
A stochastic process algebra model for the analysis of the alternating bit
protocol
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={375-84 vol.1},
	abstract={
The authors illustrate an application of the integrated approach for
modeling and analyzing concurrent systems proposed by the authors in 1995.
The case study concerns the alternating bit protocol. The protocol is
specified by means of a set of terms of the stochastic process algebra
EMPA, and then studied from the functional and the performance point of
view after constructing the semantic models associated with the terms
	},
	keywords={
		parallel processing
		Petri nets
		process algebra
		protocols
		software performance evaluation
		system monitoring
		stochastic process algebra model
		alternating bit protocol analysis
		integrated modeling/analysis method
		concurrent systems
		EMPA stochastic process algebra
		performance
		functional analysis
		semantic models
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Lilius96,
	author={Lilius, J. and Pelz, E.},
	title={
An M-net semantics for B(PN)/sup 2/ with procedures
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={365-74 vol.1},
	abstract={
The authors extend the M-net semantics for the concurrent programming
language B(PN)/sup 2/, a high-level net semantics which is original by its
full compositionality, to B(PN)/sup 2/ with procedures. To this end they
introduce a procedure-box concept for M-nets. A procedure-box is a finite
net with one entry and one exit place that represents a B(PN)/sup 2/
procedure. Procedure call and return is achieved through synchronization
while the distinction between the different instances is done with
structured tokens
	},
	keywords={
		computational linguistics
		parallel languages
		Petri nets
		process algebra
		synchronisation
		M-net semantics
		concurrent programming language
		B(PN)/sup 2/ with procedures
		high-level net semantics
		full compositionality
		procedure-box concept
		finite net
		exit place
		entry place
		procedure call
		synchronization
		structured tokens
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Tianruo-Yang96,
	author={Tianruo Yang},
	title={
Parallel least squares problems on massively distributed memory computers
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={345-54 vol.1},
	abstract={
The author studies the parallel aspects of PCGLS, a basic iterative method,
the main idea of which is to organize the computation of a conjugate
gradient method with pre-conditioner applied to normal equations, and
incomplete modified Gram-Schmidt pre-conditioner for solving least squares
problems on massively parallel distributed memory computers. The
performance of these methods on this kind of architecture is always limited
because of the global communication required for the inner products. The
author describes the parallelization of the PCGLS and IMGS pre-conditioners
using two methods of improvement. One is to assemble the results of a
number of inner products collectively and the other is to create situations
where communication can be overlapped with computation. A theoretical model
of computation and communication phases is presented which allows one to
decide the number of processors that minimizes the runtime. Several
numerical experiments on Parsytec GC/PowerPlus are presented
	},
	keywords={
		conjugate gradient methods
		distributed memory systems
		least squares approximations
		parallel architectures
		parallel machines
		parallel least squares problems
		PCGLS iterative method
		conjugate gradient method
		pre-conditioner
		normal equations
		incomplete modified Gram-Schmidt pre-conditioner
		massively parallel distributed memory computers
		communication
		architecture
		parallelization
		inner products
		computation
		minimized runtime
		Parsytec GC/PowerPlus
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Al-Mouhamed96,
	author={Al-Mouhamed, M. and Al-Maasarani, A.},
	title={
Performance evaluation of scheduling precedence-constrained computations on
message-passing systems
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={337-44 vol.1},
	abstract={
Scheduling precedence graphs with communication times is the theoretical
basis for achieving efficient parallelism in message-passing machines. The
lack of global information on the tasks, due to communication, has lead to
develop local scheduling heuristics such as the earliest-task-first. Using
knowledge on computation, communication, and system topology, a class of
global priority-based scheduling heuristics called generalized list
scheduling (GLS) is proposed. The task-level is evaluated by backward
scheduling the computation over the multiprocessor by using the best local
heuristic. This leads to realistic measurement of the task priority for use
in forward GLS scheduling. Experimental evaluation of local and GLS
heuristics is carried out using extensive random graph generation and
altering over the communication, inherent parallelism, and system topology.
Analysis shows that local heuristics rely on locally maximizing the
processor efficiency and gives acceptable deviations from the best known
solution only when the inherent parallelism is large enough to cover the
effective communication. This leads the local heuristics to achieve bounded
speedup. GLS scheduling is based on combining two strategies: (1)
differentiate critical computation and communications from others by
scheduling critical paths first, and (2) implement effective management of
processor utilization in order to increase the speedup
	},
	keywords={
		message passing
		parallel processing
		performance evaluation
		processor scheduling
		precedence-constrained computation scheduling
		message passing systems
		performance evaluation
		precedence graph scheduling
		communication times
		efficient parallelism
		local scheduling heuristics
		earliest-task-first heuristics
		system topology
		global priority-based scheduling heuristics
		generalized list scheduling
		backward scheduling
		best local heuristic
		multiprocessor
		task priority measurement
		forward scheduling
		random graph generation
		inherent parallelism
		random graph alteration
		locally maximed processor efficiency
		bounded speedup
		critical path scheduling
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Al-Mouhamed96,
	author={Al-Mouhamed, M. and Seiden, S. and Abu-Haimed, H.},
	title={
Array organization in lock-step parallel memories
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={327-36 vol.1},
	abstract={
The serialization of memory accesses is a major limiting factor in high
performance SIMD computers. The data patterns or templates that are
accessed by a program can be perceived by the compiler and therefore, the
design of dynamic storage schemes that minimize conflicts may dramatically
improve performance. The problem of finding storage schemes that minimize
the access time of arbitrary sets of power-of-2 data patterns is proved to
be NP complete. We propose linear address transformations that can be
dynamically applied by each processing element for mapping array references
onto memories. An efficient approach for combining the constraints of
different access patterns into one single linear address transformation is
presented. We prove that finding the transformation that minimizes the
access time is reduceable to N coloring, where N is the number of parallel
memories. Using coloring heuristics, storage schemes that minimize overall
memory access time are heuristically constructed. Evaluation shows that
synthesized storages lead to dramatic reduction of the degree of conflict
and largely outperforms interleaving and row-column-diagonals (STARAN)
storages
	},
	keywords={
		computational complexity
		graph colouring
		memory architecture
		minimisation
		storage allocation
		storage management
		array organization
		lock step parallel memories
		memory access serialization
		high performance SIMD computers
		templates
		dynamic storage schemes
		power-of-2 data patterns
		NP complete
		linear address transformations
		processing element
		array references
		access patterns
		single linear address transformation
		access time minimisation
		N coloring
		coloring heuristics
		storage schemes
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Kant96,
	author={Kant, M.},
	title={
Parallel algorithms for inferring evolutionary trees
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={317-26 vol.1},
	abstract={
Let S=»s/sub 1/,...,s/sub n/À be a set of n species n I, and C=»c/sup
1/,...,c/sup nu /À a set of p characters, p>1. Every character c' may have
k, distinct values (states) c/sub 1/',...,c/sub k1//sup 1/.K/sub 1/>1. We
denote by S', the set of species which have the value c/sub i/' for the
character c/sup 1/, and by I, the set »S/sub 1/'¬1<or=i<or=p,
1<or=t<or=k,À. Let T be a rooted tree with labeled leaves, and x an
internal node of T. We denote by X the set of leaves which are descendant
from x. Given S, C and I we say that T/sub SC/ is a phylogeny if T/sub SC/
is a rooted tree with labeled leaves s/sub 1/,...,S/sub n/ and for every
S/sub 1/' element of I there is a unique x, internal node of T, with
N=S/sub 1/'. The paper addresses two problems in the study of evolution:
the Perfect Phylogeny Problem (given S and C, build a phylogeny T/sub SC/,
PPP, and the Tree Compatibility Problem (given some trees, search for a
supertree T*, so that each given tree can be obtained from T* by pruning
some branches), TCP. It has been shown that PPP is an NP complete problem.
We present two parallel algorithms: TEST and TREE LIKE. TEST solves the PPP
problem for binary characters in polynomial time. TREE LIKE receives as
input a set of constraints on sets of elements, determines whether there
exists a family with tree like structure which satisfies the constraints,
and if so it builds a rooted tree T* which satisfies the constraints. TREE
LIKE may be applied to solve the TCP if the phylogenies are given as sets
of constraints like in (M. Kant and D. Sankoff, 1995). One could also use
this algorithm to verify whether a set of proposed constraints leads to a
rooted tree or not
	},
	keywords={
		genetic algorithms
		parallel algorithms
		tree data structures
		tree searching
		trees (mathematics)
		parallel algorithms
		evolutionary tree inference
		distinct values
		species
		rooted tree
		labeled leaves
		internal node
		Tree Compatibility Problem
		Perfect Phylogeny Problem
		tree searching
		supertree
		pruning
		NP complete problem
		TEST
		TREE LIKE
		PPP problem
		binary characters
		tree like structure
		TCP
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Llorens96,
	author={Llorens, J. and Amescua, A. and Velasco, M.},
	title={
Adapting the information science techniques to the software engineering
area: the application to the Software Thesaurus
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={303-15 vol.1},
	abstract={
So far, information science (IS) has not had a complete application in the
software engineering area. Some of the techniques and theories determined
by IS enhance the classification, storage and retrieval of software
components. We describe a software methodology and repository structure
"Software Thesaurus" (ST) whose main purpose is to develop software using
the reusability of the objects produced previously in other software
projects as much as possible. A tool is defined by a new repository
metamodel which supports the classification and retrieval of the essential
software objects defined in the current object oriented methodologies, 4th
generation languages, and GUI. The article presents both a free text
information system and software indexing system which allows classification
of all the objects necessary to develop a software application. The ST
represents a novel method to achieve the typical software tasks of
analysis, design, and implementation through the combination of software
engineering techniques (reusability) and information science theories
(classification and retrieval structures, thesaurus). The result of using
the Software Thesaurus is a total computer assisted analysis, design and
implementation
	},
	keywords={
		computer aided software engineering
		software reusability
		software tools
		information science techniques
		software engineering
		Software Thesaurus
		software methodology
		repository structure
		object reusability
		software projects
		repository metamodel
		object oriented methodologies
		4th generation languages
		GUI
		free text information system
		software indexing system
		software engineering techniques
		information science theories
		total computer assisted design
		CASE
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Chi-Ming-Chung96,
	author={Chi-Ming Chung and Shih, T.K. and Jich-Yan Tsai},
	title={
Inheritance hierarchy metric
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={295-302 vol.1},
	abstract={
The object oriented (OO) paradigm has a valuable programming technique.
However, very few software metrics have been proposed in the field of the
OO paradigm. Even of those proposed, not many focus on the complexity of an
inheritance hierarchy. We propose a suite of software metrics to measure
the complexity of an inheritance hierarchy and introduce two indicators:
Inheritance Density (ID) and Level Density (LD). These indicators show how
the inheritance hierarchy influences software complexity. Also, we evaluate
our proposed OO metrics by E.J. Weyuker's (1988) software metrics
evaluation criteria
	},
	keywords={
		inheritance
		object-oriented programming
		software metrics
		inheritance hierarchy metric
		object oriented paradigm
		programming technique
		OO paradigm
		software complexity measurement
		Inheritance Density
		Level Density
		software metrics evaluation criteria
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Topaloglu96,
	author={Topaloglu, N.Y. and Dikenelli, O. and Sengonca, H.},
	title={
A four dimensional reuse maturity model
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={285-94 vol.1},
	abstract={
Reusing existing software components as building blocks in developing new
software systems is being considered as a solution to high software
development costs, to low software quality and to the long time needed in
software development. Accomplishing software reuse in a software
development organization requires changes in methodological, technical,
managerial and cultural aspects of the organization. These changes should
be done according to a plan which will result in institutionalization of
software reuse. Reuse maturity models are used to assess a software
development organization's maturity according to reuse. The four
dimensional reuse maturity model (FDRMM) introduced in the paper, assesses
a software development organization's reuse maturity in a dynamic context
from four different dimensions
	},
	keywords={
		software development management
		software quality
		software reusability
		four dimensional reuse maturity model
		software component reuse
		building blocks
		software development costs
		software quality
		software development organization
		institutionalization
		reuse maturity models
		FDRMM
		dynamic context
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Debnath96,
	author={Debnath, N.C.},
	title={
Theoretical framework towards quality software development
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={275-84 vol.1},
	abstract={
The paper deals with the theoretical framework that may help improve the
software development, testing and maintenance processes. Formal definitions
of some commonly used abstract models for representing imperative language
software are included. Algorithms necessary to construct these models for a
given input program are presented. These algorithms will help automatically
generate these software models and measures, and thus can directly be
utilized to design and implement more general automated software
engineering tools. The paper also presents some theoretical developments of
the study of the interfaces between the structure of control flow and data
dependencies in imperative programs. The results of the paper may prove
useful for further research in software development, testing and
maintenance research
	},
	keywords={
		automatic programming
		formal specification
		programming theory
		software maintenance
		software quality
		software tools
		theoretical framework
		quality software development
		maintenance processes
		formal definitions
		abstract models
		imperative language software
		input program
		software models
		general automated software engineering tools
		control flow
		data dependencies
		imperative programs
		software development
		maintenance research
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Yanchun-Zhang96,
	author={Yanchun Zhang and Jie Lu},
	title={
On operation synchronisation in cooperative database processing
environments
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={265-74 vol.1},
	abstract={
In cooperative database processing environments, multiple cooperative users
can operate on the same data at the same time from multiple sites connected
by a communication network. The cooperative database system is different
from other multi user database systems in the sense that each cooperative
participant can read and write others' uncommitted data. Some inconsistency
problems in cooperative database processing environments are identified.
Conflict database operations are classified in cooperative environments and
related theorems are presented. Then a schema of cooperative operation
synchronisation is proposed
	},
	keywords={
		data integrity
		distributed databases
		groupware
		multi-access systems
		synchronisation
		operation synchronisation
		cooperative database processing environments
		multiple cooperative users
		multiple sites
		communication network
		multi user database systems
		cooperative participant
		uncommitted data
		inconsistency problems
		conflict database operations
		cooperative operation synchronisation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Jinli-Cao96,
	author={Jinli Cao and Orlowski, M.W.},
	title={
Transactions classification and a concurrency control algorithm in a
multidatabase system
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={255-64 vol.1},
	abstract={
A multidatabase system (MDBS) interconnects existing database systems in a
bottom up fashion to support the new (global user) and old (local user)
applications accessing the multiple databases concurrently. It is desirable
that the local database system autonomy is preserved and the old local
applications are executable after the local databases joining a MDBS. The
paper considers a multidatabase with various interdatabase dependencies and
proposes a concurrency control approach to support the transparency for the
local user transactions. The old local transactions are allowed to submit
at local site while the system hides various interdatabase dependencies
from the local users. In order to do these we reclassify transactions
according to the data availability and various data dependencies. Different
execution strategies are then investigated and a concurrency control
algorithm is presented in a MDBS environment
	},
	keywords={
		concurrency control
		distributed databases
		transaction processing
		transaction classification
		concurrency control algorithm
		multidatabase system
		global user
		local user
		multiple database access
		local database system autonomy
		old local applications
		interdatabase dependencies
		concurrency control approach
		transparency
		local user transactions
		data availability
		data dependencies
		execution strategies
		MDBS environment
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Amghar96,
	author={Amghar, Y. and El Nemr, G. and Flory, A.},
	title={
Object migration: a constraint-driven approach
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={245-53 vol.1},
	abstract={
The paper deals with the migration of objects within an object oriented
database. In this framework we propose an approach based on the notion of
characteristic function which expresses the conjunction of constraints
linked to a class. The evaluation of such a function is made for a given
object and class. The result belongs to the interval [0,1] meaning that the
object does or does not belong to the class. When the value is lower than 1
and greater than 0, then the object is located at a given distance from the
class. This distance is similar to Hamming distance and defines an
adherence criterium. The approach that we have used to model migration is
based on integrity constraint semantics. The semantic of relationship
between an object and a class is as follows: each object which satisfies
constraints attached to a class, belongs to that class. In addition, an
object which certifies only a part of the constraints is located at a given
distance from the class. Hence, the relationship degree notion is
introduced. The multi relationship between an object and many classes is
then easily represented
	},
	keywords={
		abstract data types
		constraint theory
		object-oriented databases
		object migration
		constraint driven approach
		object oriented database
		characteristic function
		adherence criterium
		integrity constraint semantics
		constraint satisfaction
		relationship degree notion
		multi relationship
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Bayram96,
	author={Bayram, Z.O. and Bryant, B.R. and Hakan Bilgen, F.},
	title={
A deductive declarative object-oriented data model and query language based
on narrowing
	},
	booktitle={Proceedings of the Eleventh International Symposium on Computer andInformation Sciences. ISCIS},
	volume={},
	number={},
	year={1996},
	month={},
	pages={235-44 vol.1},
	abstract={
The pure object oriented data model is not convenient for describing inter
object relationships and can result in very involved and hard to understand
queries. Augmenting the object oriented model with declarative description
of the relationships between objects using conditional rewrite rules is a
convenient way to address the problem. Under this scheme, inter object
relationships are described declaratively using conditional rewrite rules
and queries are posed also declaratively in the form of equations to be
solved. We describe an experimental system written in Smalltalk which
demonstrates the feasibility and appeal of this approach. Various examples
are also given
	},
	keywords={
		deductive databases
		object-oriented databases
		query languages
		query processing
		rewriting systems
		Smalltalk
		deductive declarative object oriented data model
		query language
		narrowing
		declarative description
		conditional rewrite rules
		inter object relationships
		experimental system
		Smalltalk
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{Walt96,
	author={Walt, M. and Inan, U.S. and Voss, H.D.},
	title={
Trapped electron losses by interactions with coherent VLF waves
	},
	journal={AIP Conf. Proc. (USA), AIP Conference Proceedings},
	volume={},
	number={},
	year={1996},
	month={},
	pages={65-70},
	abstract={
VLF whistler waves from lightning enter the magnetosphere and cause the
precipitation of energetic trapped electrons by pitch angle scattering.
These events, known as lightning-induced electron precipitation (LEP) have
been detected by satellite and rocket instruments and by perturbations of
VLF waves traveling in the Earth-ionosphere waveguide. Detailed comparison
of precipitating electron energy spectra and time dependence are in general
agreement with calculations of trapped electron interactions with ducted
whistler waves. In particular the temporal structure of the precipitation
and the dynamic energy spectra of the electrons confirm this interpretation
of the phenomena. There are discrepancies between observed and measured
electron flux intensities and pitch angle distributions, but these
quantities are sensitive to unknown wave intensities and mapped particle
fluxes near the loss cone angle. The overall effect of lightning generated
VLF waves on the lifetime of trapped electrons is still uncertain. The flux
of electrons deflected into the bounce loss cone by a discrete whistler
wave has been measured in a few cases. However, the area of the
precipitation region is not known, and thus the total number of electrons
lost in an LEP event can only be estimated. While the LEP events are
dramatic, more important effects on trapped electrons may arise from the
small but numerous deflections which increase the pitch angle diffusion
rate of the electron population
	},
	keywords={
		atmospheric electron precipitation
		magnetospheric electromagnetic wave propagation
		radiation belts
		radiowave propagation
		whistlers
		trapped electron losses
		coherent VLF waves
		VLF whistler waves
		magnetosphere
		energetic trapped electrons
		pitch angle scattering
		lightning-induced electron precipitation
		Earth-ionosphere waveguide
		energy spectra
		temporal structure
		electron flux intensities
		wave intensities
		bounce loss cone
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{LehtinenSep96,
	author={Lehtinen, N.G. and Walt, M. and Inan, U.S. and Bell, T.F. and Pasko, V.P.},
	title={
gamma -ray emission produced by a relativistic beam of runaway electrons
accelerated by quasi-electrostatic thundercloud fields
	},
	journal={Geophysical Research Letters},
	volume={23},
	number={19},
	year={1996},
	month={Sep},
	pages={2645-8},
	abstract={
In an experiment described by Fishman et al. [1994], high energy photons of
atmospheric origin were detected by the Burst and Transient Source
Experiment (BATSE) detectors, located on the Compton Gamma Ray Observatory
(CGRO). In this paper the authors assess the possibility that the bursts
may be bremsstrahlung produced by relativistic (>1 MeV) runaway electron
beams-accelerated in an avalanche process by quasi-electrostatic
thundercloud fields. They consider the height-dependent density profile of
the relativistic electrons specified as a function of time in the context
of a previously reported runaway model [Bell et al., 1995]. The electron
beam is modeled as a vertical cylinder with radius 10 km, and numerical
estimates are provided of gamma -ray fluxes which would be observed at the
satellite. The predicted fluxes at the satellite altitude and at horizontal
distances of up to 500 km from the source are found to be comparable to the
experimental data
	},
	keywords={
		atmospheric electricity
		atmospheric radiation
		gamma-rays
		lightning
		thunderstorms
		atmosphere
		storm
		thunderstorm
		gamma ray emission
		gamma -ray emission
		relativistic electron beam
		runaway electrons
		quasi-electrostatic field
		electric field
		lightning
		high energy photons
		BATSE
		CGRO
		gamma ray burst
		bremsstrahlung
		avalanche process
		relativistic electrons
		runaway model
		vertical cylinder
		gamma -ray flux
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{FukunishiAug96,
	author={Fukunishi, H. and Takahashi, Y. and Kubota, M. and Sakanoi, K. and Inan, U.S. and Lyons, W.A.},
	title={
Elves: lightning-induced transient luminous events in the lower ionosphere
	},
	journal={Geophysical Research Letters},
	volume={23},
	number={16},
	year={1996},
	month={Aug},
	pages={2157-60},
	abstract={
Observations of optical phenomena at high altitude above thunderstorms
using a multichannel high-speed photometer and image intensified CCD
cameras were carried but at Yucca Ridge Field Station (40 degrees 40' N,
104 degrees 56' W), Colorado as part of the SPRITES'95 campaign from 15
June to August 6, 1995. These new measurements indicate that diffuse
optical flashes with a duration of <1 ms and a horizontal scale of À100-300
km occur at 75-105 km altitude in the lower ionosphere just after the onset
of cloud-to-ground lightning discharges, but preceding the onset of
sprites. Here we designate these events as "elves" to distinguish them from
"red sprites". This finding is consistent with the production of diffuse
optical emissions due to the heating of the lower ionosphere by
electromagnetic pulses generated by lightning discharges as suggested by
several authors
	},
	keywords={
		atmospheric radiation
		atmospheric temperature
		electromagnetic pulse
		ionospheric disturbances
		lightning
		thunderstorms
		lightning-induced transient luminous events
		lower ionosphere
		thunderstorms
		SPRITES'95 campaign
		diffuse optical flashes
		cloud-to-ground lightning discharges
		elves
		heating
		electromagnetic pulses
		AD 1995 06 15 to 08 06
		75 to 105 km
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{GlukhovAug96,
	author={Glukhov, V.S. and Inan, U.S.},
	title={
Particle simulation of the time-dependent interaction with the ionosphere
of rapidly varying lightning EMP
	},
	journal={Geophysical Research Letters},
	volume={23},
	number={16},
	year={1996},
	month={Aug},
	pages={2193-6},
	abstract={
The interaction with the lower ionosphere of rapidly varying
electromagnetic pulses (EMPs) produced by lightning discharges is studied.
The nonlinear heating, ionization and optical emission production are
modeled using the Monte Carlo technique, which allows for consideration of
realistic lightning EMPs with a few mu s rise times. Results indicate that
the electron distribution function is highly anisotropic during the first
few mu s of the interaction, but subsequently develops into a
near-isotropic quasi-stationary state. The peak optical emissions
intensities are found to be highly dependent on the EMP waveform, while the
altitude range at which the emissions occur is relatively independent of
pulse shape. Results of the particle simulation are used to assess the
range of applicability of the quasi-stationary models [Taranenko et al.,
1993; Inan et al., 1996]
	},
	keywords={
		electromagnetic pulse
		ionospheric disturbances
		ionospheric electromagnetic wave propagation
		lightning
		EM pulse
		radiowave propagation
		ionospheric disturbance
		particle simulation
		time-dependent interaction
		ionosphere
		rapidly varying lightning EMP
		rapidly varying electromagnetic pulse
		nonlinear heating
		ionization
		optical emission
		Monte Carlo method
		anisotropic electron distribution function
		EMP waveform
		quasistationary model
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{Lev-TovJul96,
	author={Lev-Tov, S.J. and Inan, U.S. and Smith, A.J. and Clilverd, M.A.},
	title={
Characteristics of localized ionospheric disturbances inferred from VLF
measurements at two closely spaced receivers
	},
	journal={Journal of Geophysical Research},
	volume={101},
	number={A7},
	year={1996},
	month={Jul},
	pages={15737-47},
	abstract={
The very low frequency (VLF) NPM signal from Hawaii was recorded at two
closely spaced (À50 km) receivers (located at Palmer and Faraday stations)
on the Antarctic Peninsula. Measurements of characteristic amplitude and
phase signatures of lightning-induced electron precipitation (LEP) events
were made on three different days in March 1992. Both amplitude and, for
the first time, phase measurements are quantitatively interpreted using a
three-dimensional model of VLF propagation in the Earth-ionosphere
waveguide in the presence of lower ionospheric disturbances. This is the
first time such a study has been undertaken with mirrored precipitation.
Differences between the amplitude and phase changes at the two sites are
accounted for by the location of the LEP ionospheric disturbance transverse
to the VLF signal propagation paths. The change in these differences is
explained by the horizontal movement of the disturbance region and,
therefore, the causative whistler duct footprint across the
transmitter-receiver paths. Trends in the amplitude and phase changes on a
timescale of order 1 hour are found to be encompassed by the modeling of
the passage of the day-night terminator along the paths
	},
	keywords={
		atmospheric electron precipitation
		Earth-ionosphere waveguide
		ionospheric disturbances
		ionosphere
		three-dimensional model
		AD 1992 03
		localized ionospheric disturbance
		VLF
		two closely spaced receivers
		Antarctica
		amplitude
		phase signatures
		lightning-induced electron precipitation
		radiowave propagation
		Earth-ionosphere waveguide
		mirrored precipitation
		causative whistler duct footprint
		transmitter-receiver path
		day-night terminator passage
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{Inan15May96,
	author={Inan, U.S. and Pasko, V.P. and Bell, T.F.},
	title={
Sustained heating of the ionosphere above thunderstorms as evidenced in
``early/fast'' VLF events
	},
	journal={Geophysical Research Letters},
	volume={23},
	number={10},
	year={1996},
	month={May},
	pages={1067-70},
	abstract={
Quasi-electrostatic (QE) thundercloud fields are proposed to maintain the
ionospheric electrons at a persistently heated level well above their
ambient thermal energy. Changes in the thundercloud charge (e.g., in
lightning discharges) lead to heating/cooling above/below this quiescent
level, and are registered as sudden (i.e., fast'<20 ms) subionospheric VLF
signal changes, occurring simultaneously (i.e., early'<20 ms) with
lightning discharges, and referred to as early/fast VLF events [Inan et
al., 1993]
	},
	keywords={
		atmospheric radiation
		atmospheric temperature
		ionospheric disturbances
		lightning
		thunderstorms
		sustained heating
		ionosphere
		thunderstorms
		VLF events
		quasi-electrostatic thundercloud fields
		lightning discharges
		cooling
		subionospheric VLF signal changes
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{Inan1May96,
	author={Inan, U.S. and Reising, S.C. and Fishman, G.J. and Horack, J.M.},
	title={
On the association of terrestrial gamma-ray bursts with lightning and
implications for sprites
	},
	journal={Geophysical Research Letters},
	volume={23},
	number={9},
	year={1996},
	month={May},
	pages={1017-20},
	abstract={
Measurements of ELF/VLF radio atmospherics (sterics) at Palmer Station,
Antarctica, provide evidence of active thunderstorms near the inferred
source regions of two different gamma-ray bursts of terrestrial origin
(Fishman et al., 1994). In one case, a relatively intense steric occurring
within +or-1.5 ms of the time of the gamma-ray burst provides the first
indication of a direct association of this burst with a lightning
discharge. This steric and many others launched by positive cloud-to-ground
(CG) discharges and observed at Palmer during the periods studied exhibit
slow tail' waveforms, indicative of continuing currents in the causative
lightning discharges. The slow tails of these sterics are similar to those
of sterics originating in positive CG discharges that are associated with
sprites
	},
	keywords={
		atmospheric radiation
		atmospherics
		lightning
		thunderstorms
		terrestrial gamma-ray bursts
		CGRO observations
		sprites
		ELF radio atmospherics
		VLF radio atmospherics
		sterics
		Palmer Station
		Antarctica
		active thunderstorms
		source regions
		lightning discharge
		positive cloud-to-ground discharges
		slow tail waveforms
		300 Hz to 20 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PaskoMar96,
	author={Pasko, V.P. and Inan, U.S. and Bell, T.F.},
	title={
Sprites as luminous columns of ionization produced by quasi-electrostatic
thundercloud fields
	},
	journal={Geophysical Research Letters},
	volume={23},
	number={6},
	year={1996},
	month={Mar},
	pages={649-52},
	abstract={
Quasi-electrostatic (QE) fields which exist above thunderclouds after
lightning discharges can lead to the formation of columnar channels of
breakdown ionization and carrot-like vertical luminous structures with
typical transverse dimension À5-10 km spanning an altitude range from À80
km to well below À50 km. The carrot-like forms closely resemble those
observed in sprites. Results indicate that the appearance of optical
emissions can be significantly delayed in time (À1-20 ms) with respect to
the causative lightning discharge
	},
	keywords={
		airglow
		atmospheric electricity
		atmospheric ionisation
		lightning
		mesosphere
		thermosphere
		thunderstorms
		middle atmosphere
		mesosphere
		upper atmosphere
		thermosphere
		stratosphere
		ionisation
		ionization
		sprite
		thunderstorm disturbance
		optical emission
		electric discharge
		luminous column
		quasi-electrostatic field
		electric field
		lightning
		columnar channel
		breakdown ionization
		carrot-like vertical luminous structure
		delay
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{CummerMar96,
	author={Cummer, S.A. and Bell, T.F. and Inan, U.S. and Zanetti, L.J.},
	title={
VLF remote sensing of the auroral electrojet
	},
	journal={Journal of Geophysical Research},
	volume={101},
	number={A3},
	year={1996},
	month={Mar},
	pages={5381-9},
	abstract={
Investigates a new potential technique to determine the position of the
auroral electrojet from ground-based VLF amplitude and phase measurements.
The chief advantage of this technique over conventional ground magnetometer
measurements is that it can provide data on a continental scale with a
small number of receiving stations and with a minimum of data processing.
At the edge of the auroral zone, where the electrojet current system flows,
high-energy (E>300 keV) precipitating electrons cause local electron
density enhancements in the ionosphere which cause phase and amplitude
perturbations in VLF waves propagating in the Earth-ionosphere waveguide.
Continuous measurements of the amplitude and phase of signals from the
Omega North Dakota VLF transmitter were made in Nome, Alaska. Using a
two-dimensional model of VLF propagation which accounts for ionospheric
disturbances caused by the electron precipitation associated with the
electrojet, the amplitude and phase signatures of electrojet incursion
across each propagation path were predicted. Seventeen nights of
simultaneous VLF amplitude and phase data and ground magnetometer data were
examined and catalogued based on the degree of temporal correlation between
the two data sets and the degree to which the VLF events matched the
propagation simulations. Of the nights exhibiting activity, more than 60%
exhibited excellent correlation between the magnetometer and VLF events,
and the majority of these showed good agreement with the model results. An
additional estimate of the electrojet position was provided for one of the
studied sights by field-aligned current measurements from the Freja
satellite. A comparison of these independent means of determining the
electrojet position shows that they are in good agreement for the night
examined
	},
	keywords={
		electrojets
		ionospheric electromagnetic wave propagation
		ionospheric techniques
		ionosphere
		electric current
		measurement technique
		ground based method
		VLF remote sensing
		auroral electrojet
		position
		radiowave amplitude
		phase
		Earth-ionosphere waveguide
		LF propagation
		electron precipitation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanMar96,
	author={Inan, U.S. and Slingeland, A. and Pasko, V.P. and Rodriguez, J.V.},
	title={
VLF and LF signatures of mesospheric/lower ionospheric response to
lightning discharges
	},
	journal={Journal of Geophysical Research},
	volume={101},
	number={A3},
	year={1996},
	month={Mar},
	pages={5219-38},
	abstract={
New evidence is presented of disturbances of the electrical conductivity of
the nighttime mesosphere and the lower ionosphere in association with
lightning discharges. In addition to extensive documentation of the
characteristics of a class of events heretofore referred to as early/fast
VLF events, Inan et al. (1993), the present authors data reveal a new
feature of these events, consisting of a postonset peak that typically
lasts for 1-2 s. They also report the observation of short-duration VLF or
LF perturbations, in which the amplitude of the subionospheric signal
exhibits a sudden change within 20 ms of the causative lightning discharge,
and recovers back to its original level in <3 s. These short-duration
events have characteristics similar to the previously observed rapid onset,
rapid decay VLF signatures, Doulden et al. (1994). Both the typical and
rapidly recovering events are observed primarily when the causative
lightning discharge is within +or-50 km of the VLF or LF great circle
propagation path, indicating that the scattering from the localized
disturbance is highly collimated in the forward direction. The latter in
turn implies that for the parameters in hand, the transverse extent of the
disturbance must be at least À100-150 km. The measured VLF signatures are
compared with the predictions of a three-dimensional model of
subionospheric VLF propagation and scattering in the presence of localized
ionospheric disturbances produced by electromagnetic impulses and
quasi-electrostatic QE fields produced by lightning discharges. The rapidly
recovering or short-duration events are consistent with the heating of the
ambient electrons by quasi-static electric fields, in cases when heating is
not intense enough to exceed-the attachment or ionization thresholds. When
no significant electron density changes occur, the conductivity changes due
to heating alone last only as long as the QE fields, typically less than a
few seconds. When heating is intense enough so t
	},
	keywords={
		atmospheric electricity
		atmospheric electromagnetic wave propagation
		atmospherics
		ionospheric disturbances
		ionospheric electromagnetic wave propagation
		lightning
		mesosphere
		atmospherics
		radiowave emission
		thunderstorm
		VLF signature
		LF signature
		mesosphere
		lower ionosphere response
		middle atmosphere
		ionospheric disturbance
		lightning
		electric discharge
		electrical conductivity
		night
		postonset peak
		short-duration perturbation
		short-duration events
		radiowave propagation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{AlfordJan96,
	author={Alford, J. and Engebretson, M. and Arnoldy, R. and Inan, U.},
	title={
Frequency variations of quasi-periodic ELF-VLF emissions: a possible new
ground-based diagnostic of the outer high-latitude magnetosphere
	},
	journal={Journal of Geophysical Research},
	volume={101},
	number={A1},
	year={1996},
	month={Jan},
	pages={83-97},
	abstract={
Magnetic pulsations and quasi-periodic (QP) amplitude modulations of
ELF-VLF waves at Pc 3-4 frequencies (15-50 mHz) are commonly observed
simultaneously in cusp-latitude data. The naturally occurring ELF-VLF
emissions are believed to be modulated within the magnetosphere by the
compressional component of geomagnetic pulsations formed external to the
magnetosphere. The authors have examined data from South Pole Station
(LÀ14) to determine the occurrence and characteristics of QP emissions. On
the basis of 14 months of data during 1987 and 1988 they found that QP
emissions typically appeared in both the 0.5-1 kHz and 1-2 kHz receiver
channels at South Pole Station and occasionally in the 2-4 kHz channel. The
QP emission frequency appeared to depend on solar wind parameters and
interplanetary magnetic field (IMF) direction, and the months near fall
equinox in both 1987 and 1988 showed a significant increase in the
percentage of QP emissions only in the lowest-frequency channel. They
present a model consistent with these variations in which high-latitude
(nonequatorial) magnetic field minima near the magnetopause play a major
role, because the field magnitude governs both the frequency of ELF-VLF
emissions and the whistler mode propagation cutoffs. Because the field in
these regions will be strongly influenced by solar wind and IMF parameters,
variations in the frequency of such emissions may be useful in providing
ground-based diagnostics of the outer high-latitude magnetosphere
	},
	keywords={
		atmospheric radiation
		atmospheric techniques
		magnetosphere
		micropulsations
		whistlers
		atmosphere
		measurement technique
		outer magnetosphere
		magnetic pulsation
		micropulsation
		radiowave emission
		frequency variation
		quasi-periodic ELF-VLF emission
		quasiperiodic emissions
		ELF
		VLF
		high-latitude magnetosphere
		magnetic pulsations
		amplitude modulation
		Pc 3
		Pc 4
		geomagnetic pulsations
		South Pole Station
		occurrence characteristics
		AD 1987
		AD 1988
		interplanetary magnetic field
		IMF direction
		whistler mode propagation cutoff
		0.5 to 5 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PaskoFeb96,
	author={Pasko, V.P. and Inan, U.S. and Bell, T.F.},
	title={
Blue jets produced by quasi-electrostatic pre-discharge thundercloud fields
	},
	journal={Geophysical Research Letters},
	volume={23},
	number={3},
	year={1996},
	month={Feb},
	pages={301-4},
	abstract={
Pre-discharge quasi-electrostatic fields immediately above the thundercloud
lead to the formation and upward propagation of streamer type ionization
channels with features in good agreement with video observations of blue
jets
	},
	keywords={
		atmospheric electricity
		electric fields
		lightning
		thunderstorms
		blue jets
		quasielectrostatic predischarge thundercloud fields
		upward propagation
		formation
		streamer type ionization channels
		video observations
		sprites
		runaway electrons
		100 km/s
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{Jiunn-Tsair-ChenMar96,
	author={Jiunn-Tsair Chen and Inan, U.S. and Bell, T.F.},
	title={
VLF strip holographic imaging of lightning-associated ionospheric
disturbances
	},
	journal={Radio Science},
	volume={31},
	number={2},
	year={1996},
	month={Mar},
	pages={335-48},
	abstract={
A linear array of very low frequency (VLF) receivers, deployed along a line
roughly perpendicular to the direction of signal propagation, enables the
determination of the size and location of D region disturbances produced by
lightning-induced electron precipitation (LEP) bursts or by
lightning-induced heating in the vicinity of the great circle VLF
propagation paths. The configuration essentially constitutes a strip
hologram so that the width of both the amplitude and phase perturbation of
the signal pattern recorded along the strip are simply related to the size
and location of the disturbance for the range of altitude profiles of
disturbed ionization expected for LEP events. The validity of the approach
is demonstrated both analytically for single waveguide-mode propagation and
also for a realistic propagation path (Annapolis-Stanford) by using a
three-dimensional numerical model of VLF propagation and scattering in the
Earth-ionosphere waveguide. We also discuss the criteria by which the
spacing of discrete elements along the strip can be optimally chosen
	},
	keywords={
		array signal processing
		atmospheric electron precipitation
		atmospheric temperature
		D-region
		Earth-ionosphere waveguide
		geophysical signal processing
		holography
		image processing
		ionospheric disturbances
		ionospheric techniques
		lightning
		radiowave propagation
		VLF strip holographic imaging
		lightning-associated ionospheric disturbances
		size
		location
		D-region disturbances
		electron precipitation
		lightning-induced heating
		great circle VLF propagation paths
		amplitude and phase perturbation
		phase perturbation
		altitude profile
		disturbed ionization
		single waveguide-mode propagation
		Annapolis-Stanford
		three-dimensional numerical model
		VLF propagation
		scattering
		Earth-ionosphere waveguide
		discrete elements
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanJan96,
	author={Inan, U.S. and Sampson, W.A. and Taranenko, Y.N.},
	title={
Space-time structure of optical flashes and ionization changes produced by
lightning-EMP
	},
	journal={Geophysical Research Letters},
	volume={23},
	number={2},
	year={1996},
	month={Jan},
	pages={133-6},
	abstract={
Intense electromagnetic pulses (EMPs) released by lightning discharges
produce bright optical emissions at 80-95 km altitudes emitted in a thin
(À30 km) cylindrical shell expanding to radial distances of up to >150 km,
lasting for À400 mu s, and appearing in limb-view as a thin layer with À400
km lateral extent
	},
	keywords={
		airglow
		atmospheric ionisation
		atmospheric optics
		atmospheric radiation
		lightning
		upper atmosphere
		airglow
		optical emission
		thermosphere
		spatial structure
		temporal structure
		optical flash
		light
		ionization change
		lightning
		EMP
		electromagnetic pulse
		EM pulse
		thin cylindrical shell
		80 to 95 km
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanDec95,
	author={Inan, U.S. and Bell, T.F. and Pasko, V.P. and Sentman, D.D. and Wescott, E.M. and Lyons, W.A.},
	title={
VLF signatures of ionospheric disturbances associated with sprites
	},
	journal={Geophysical Research Letters},
	volume={22},
	number={24},
	year={1995},
	month={Dec},
	pages={3461-4},
	abstract={
VLF perturbations on signals propagating along great-circle-paths (GCP)
through electrically active midwest thunderstorms are associated with
luminous high altitude glows (referred to as sprites) observed from
aircraft or ground. The data constitutes the first evidence that the
physical processes leading to sprites also alter the conductivity of the
lower ionosphere
	},
	keywords={
		airglow
		ionosphere
		ionospheric disturbances
		ionospheric electromagnetic wave propagation
		lightning
		mesosphere
		radiowave propagation
		thermosphere
		thunderstorms
		upper atmosphere
		ionosphere
		mesosphere
		upper atmosphere
		middle atmosphere
		VLF signature
		ionospheric disturbance
		sprite
		lightning
		airglow
		great-circle-path
		electrically active midwest thunderstorm
		United States
		USA
		radiowave propagation
		luminous high altitude glow
		sprites
		lower ionosphere
		electrical conductivity decrease
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{JasnaJun94,
	author={Jasna, D. and Inan, U.S. and Bell, T.F.},
	title={
Precipitation of radiation belt electrons by magnetospherically reflected
(MR) whistlers
	},
	journal={Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika},
	volume={37},
	number={6},
	year={1994},
	month={Jun},
	pages={727-40},
	abstract={
Uses a test particle simulation model based on gyro-averaged equations of
motion to study the influence of oblique magnetospherically reflected (MR)
whistlers on the near-loss-cone distribution function of radiation belt
electrons. The authors find that MR whistlers originating in lightning can
resonantly interact with radiation belt electrons over a broad range of
L-shells and precipitate higher energy electrons from lower L-shells.
Electrons in the energy range of 1-2.6 Me V are precipitated from L=2,
whereas from L=4 the precipitated electron energy range is 150-220 keV. The
precipitated differential electron flux due to this interaction is higher
for higher L-shells, and the maximum value ranges from Phi /sub
E(prec)/(1.11 MeV)=5.2*10/sup -4/ el/cm/sup 2/.s.keV at L=2 to Phi /sub
E(prec)/(173 keV)=4.6*10/sup -1/ el/cm/sup 2/.s.keV at L=4. The lifetimes
of radiation belt electrons in a given magnetic flux tube around the
L-shell on which the interaction takes place are found to be of the order
of several days, comparable to lifetimes corresponding to electron loss
induced by hiss, which was heretofore assumed to be the dominant loss
mechanism. The minimum electron lifetimes vary from 2.47 days for E=1.11
MeV electrons at L=2 to 4.64 days for E=173 keV electrons at L=4
	},
	keywords={
		atmospheric electron precipitation
		radiation belts
		whistlers
		radiation belt electrons
		magnetospherically reflected whistlers
		test particle simulation model
		gyro-averaged equations of motion
		near-loss-cone distribution function
		precipitation
		L-shells
		precipitated differential electron flux
		magnetic flux tube
		electron loss
		hiss
		loss mechanism
		minimum electron lifetimes
		1 to 2.6 MeV
		150 to 220 keV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{Lev-TovNov95,
	author={Lev-Tov, S.J. and Inan, U.S. and Bell, T.F.},
	title={
Altitude profiles of localized D region density disturbances produced in
lightning-induced electron precipitation events
	},
	journal={Journal of Geophysical Research},
	volume={100},
	number={A11},
	year={1995},
	month={Nov},
	pages={21375-83},
	abstract={
A three-dimensional model of very low frequency (VLF) radio wave
propagation in the Earth-ionosphere waveguide in the presence of lower
ionospheric disturbances is used to quantitatively interpret VLF signatures
of lightning-induced electron precipitation (LEP) events observed in two
previously reported cases. One case is that of a 28.5-kHz signal
originating in Puerto Rico and propagating to a receiver in Lake
Mistissini, Quebec. The other case involves a 24.0-kHz signal originating
in Cutler, Maine, and received at Stanford, California. In both cases,
high-resolution measurements of the VLF signals were made to accurately
document characteristic signatures of LEP events. The comparison of the
model calculations with the data yields information about the altitude
profiles of electron density of both the extra ionization produced by the
LEP events and of the ambient ionospheric D-region. The comparisons are
carried out using generally accepted values of the spatial extent of the
disturbed regions and the intensity of the particle flux constituting the
LEP burst
	},
	keywords={
		atmospheric electron precipitation
		D-region
		Earth-ionosphere waveguide
		electron density
		ionospheric disturbances
		lightning
		radiowave propagation
		ionosphere
		localized D-region density disturbances
		lightning-induced electron precipitation events
		altitude profiles
		3D model
		VLF radio wave propagation
		Earth-ionosphere waveguide
		lower ionospheric disturbances
		high-resolution measurements
		LEP events
		electron density
		ionization
		disturbed regions
		particle flux intensity
		28.5 kHz
		24 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BellNov95,
	author={Bell, T.F. and Inan, U.S. and Danielson, M.T. and Cummer, S.A.},
	title={
VLF signatures of ionospheric heating by HIPAS
	},
	journal={Radio Science},
	volume={30},
	number={6},
	year={1995},
	month={Nov},
	pages={1855-67},
	abstract={
The amplitude and phase of subionospherically propagating VLF signals are
known to be sensitive indicators of the electron density and temperature at
D region altitudes. The authors present new observations at a station in
Alaska positioned to provide measurements of VLF signals that have
propagated beneath the ionospheric region heated by the high-power auroral
stimulation (HIPAS) HF heating facility near Fairbanks, Alaska. Analysis of
data from HIPAS campaigns conducted in fall 1992 and spring 1993 has shown
that in roughly 60% of the cases analyzed, the amplitude of the 23.4-kHz
signal from the NPM transmitter in Hawaii as observed in Fort Yukon,
Alaska, exhibited a measurable change in amplitude with the same on/off
modulation pattern as that of the HIPAS HF transmissions at 2.85 MHz. In
almost 70% of the cases analyzed, the same signal exhibited similar
measurable changes in phase. The amplitude changes ranged from -0.2 dB to
+0.5 dB, and the sensitivity of the measurement was approximately +or-0.02
dB. The phase changes ranged from -4.5 degrees to -0.3 degrees , and the
sensitivity of the measurement was typically +or-0.4 degrees . It is
demonstrated that the phase and amplitude changes can be used as diagnostic
tools to determine characteristics of the ambient electron density profile
above the HIPAS facility
	},
	keywords={
		D-region
		electron density
		ionospheric disturbances
		ionospheric electromagnetic wave propagation
		radiowave propagation
		ionospheric heating
		VLF signatures
		amplitude
		phase
		subionospherically propagating VLF signals
		electron density
		temperature
		D region
		HIPAS
		high-power auroral stimulation HF heating facility
		on/off modulation pattern
		AD 1992 to 1993
		23.4 kHz
		2.85 MHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BellAug95,
	author={Bell, T.F. and Pasko, V.P. and Inan, U.S.},
	title={
Runaway electrons as a source of red sprites in the mesosphere
	},
	journal={Geophysical Research Letters},
	volume={22},
	number={16},
	year={1995},
	month={Aug},
	pages={2127-30},
	abstract={
Large quasi-electrostatic (QE) fields above thunderclouds produce an upward
traveling beam of approximately 1 MeV runaway electrons which may
contribute to the production of optical emissions above thunderclouds
referred to as red sprites. Results of a one dimensional computer
simulation model suggest that the runaway electrons can produce optical
emissions similar in intensity and spectra to those observed in red
sprites, but only for large QE fields produced by positive cloud-to-ground
discharges lowering 250 C or more to ground from an altitude of at least 10
km. Differences in predicted optical spectra from that of other mechanisms
suggest that the runaway electron mechanism can be readily tested by high
resolution spectral measurements of red sprites
	},
	keywords={
		atmospheric electricity
		electric fields
		electron beam effects
		mesosphere
		thunderstorms
		source
		red sprites
		mesosphere
		quasielectrostatic fields
		thunderclouds
		upward travelling electron beam
		optical emissions
		1D computer simulation model
		emission intensity
		upward discharges
		positive cloud-to-ground discharges
		predicted optical spectra
		runaway electron mechanism
		20 keV to 20 MeV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SonwalkarMay95,
	author={Sonwalkar, V.S. and Inan, U.S. and Aggson, T.L. and Farrell, W.M. and Pfaff, R.},
	title={
Focusing of nonducted whistlers by the equatorial anomaly
	},
	journal={Journal of Geophysical Research},
	volume={100},
	number={A5},
	year={1995},
	month={May},
	pages={7783-90},
	abstract={
Impulsive ELF/VLF electric field bursts observed by the vector electric
field instrument (VEFI) on the Dynamics Explorer 2 (DE 2) satellite on
almost every crossing of the geomagnetic equator in the evening hours are
interpreted as originating in lightning discharges. These signals that peak
in intensity near the magnetic equator are observed within 5-20 degrees
latitude of the geomagnetic equator at altitudes of 300-500 km with
amplitudes of the order of approximately mV/m in the 512- to 1024-Hz
frequency band of the VEFI instrument. Whistler-mode ELF/VLF wave
propagation through a horizontally stratified ionosphere predicts strong
attenuation of subionospheric signals reaching the equator at low
altitudes. However, ray tracing analysis shows that the presence of the
equatorial density anomaly, commonly observed in the upper ionosphere
during evening hours, leads to the focusing of the wave energy from
lightning near the geomagnetic equator at low altitudes, thus accounting
for all observed aspects of the phenomenon. The observations presented
indicate that during certain hours in the evening, almost all the energy
input from lightning discharges entering the ionosphere at <30 degrees
latitude remains confined to a small region (in altitude and latitude) near
the geomagnetic equator. The net wideband electric field, extrapolated from
the observed electric field values in the 512- to 1024-Hz band, can be
approximately 10 mV/m or higher. These strong electric fields generated in
the ionosphere by lightning at local evening times may be important for the
equatorial electrodynamics of the ionosphere
	},
	keywords={
		F-region
		ionospheric electromagnetic wave propagation
		whistlers
		radiowave propagation
		nonducted whistlers
		whistler
		focusing
		ionosphere
		equatorial electrodynamics
		equatorial anomaly
		impulsive ELF electric field burst
		VLF
		lightning
		F-region
		horizontally stratified ionosphere
		strong attenuation
		300 to 500 km
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PaskoFeb95,
	author={Pasko, V.P. and Inan, U.S. and Taranenko, Y.N. and Bell, T.F.},
	title={
Heating, ionization and upward discharges in the mesosphere due to intense
quasi-electrostatic thundercloud fields
	},
	journal={Geophysical Research Letters},
	volume={22},
	number={4},
	year={1995},
	month={Feb},
	pages={365-8},
	abstract={
Quasi-electrostatic fields that temporarily exist at high altitudes
following the sudden removal (e.g. by a lightning discharge) of
thundercloud charge at low altitudes are found to significantly heat
mesospheric electrons and produce ionization and light. The intensity,
spatial extent, duration and spectra of optical emissions produced are
consistent with the observed features of the red sprite type of upward
discharges
	},
	keywords={
		atmospheric ionisation
		electrons
		electrostatic discharge
		mesosphere
		plasma heating
		thunderstorms
		mesospheric electron heating
		ionization
		upward discharges
		mesosphere
		intense quasielectrostatic thundercloud fields
		lightning discharge
		sudden thundercloud charge removal
		light production
		ionization production
		intensity
		spatial extent
		duration
		spectra
		optical emissions
		red sprites
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SonwalkarFeb95,
	author={Sonwalkar, V.S. and Inan, U.S. and Bell, T.F.},
	title={
An interpretation of a mysterious 3.0- to 4.6-kHz emission band observed on
Voyager 2 near Neptune
	},
	journal={Journal of Geophysical Research},
	volume={100},
	number={A2},
	year={1995},
	month={Feb},
	pages={1795-809},
	abstract={
A whistler mode interpretation is provided for the narrowband signal (f
approximately 3-4.6 kHz, Delta f approximately 200-800 Hz) detected by the
plasma wave instrument on Voyager 2 during its encounter with Neptune. The
analysis indicates that this signal may have been generated in a limited
spatial region and that it propagated to other regions of the Neptunian
magnetosphere in the nonducted whistler mode with wave normal vectors lying
close to the whistler mode resonance cone. The observed frequency variation
of the emission along the Voyager 2 trajectory is consistent with this
interpretation. The source location is estimated to be near the magnetic
equator at L approximately 4 and dipole longitude of 111 degrees W (260
degrees W longitude in Neptune coordinate system). The source frequency and
bandwidth are estimated to be 3.6 kHz and 300 Hz, respectively. The waves
most likely would have been generated by energetic electrons with 2- to
20-keV parallel energy via a gyroresonance mechanism. The interpretation of
the narrowband emissions places the following limits on the Neptunian
thermal plasma density and temperature: (1) N/sub e,min/>0.16 el/cm/sup 3/
for 1.2R/sub N/<R<5R/sub N/,(2)N/sub e,max/=597.5 cm/sup -3/ at R=1.3R/sub
N/,(3)T/sub e,max/<500-1000 K at R approximately 5R/sub N/. It is also
possible that the weak UV aurora observed near Neptune could have been
caused by the precipitation of energetic particles by the narrowband
emission as a result of wave particle interactions
	},
	keywords={
		Neptune
		planetary atmospheres
		Neptune
		Voyager 2 plasma wave instrument
		planetary encounter
		Neptunian magnetosphere
		nonducted whistler mode
		whistler mode resonance cone
		emission frequency variation
		source location
		energetic electrons
		gyroresonance mechanism
		narrowband emissions
		thermal plasma density
		plasma temperature
		UV aurora
		energetic particle precipitation
		VLF
		wave particle interactions
		3 to 4.6 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{RosenbergJan95,
	author={Rosenberg, T.J. and Singh, S. and Wu, C.S. and LaBelle, J. and Treumann, R.A. and Inan, U.S. and Lanzerotti, L.J.},
	title={
Coincident bursts of auroral kilometric radiation and VLF emissions
associated with a type III solar radio noise event
	},
	journal={Journal of Geophysical Research},
	volume={100},
	number={A1},
	year={1995},
	month={Jan},
	pages={281-8},
	abstract={
Examines a magnetospheric VLF/radio noise event that is highly suggestive
of the triggering of auroral kilometric radiation (AKR) by solar type III
radio emission and of a close relation between AKR and broadband hiss. The
solar type III burst was coincident with local dayside VLF/LF noise
emission bursts at South Pole station. It was also coincident with AKR
bursts detected on the AMPTE/IRM satellite, at the same magnetic local time
as South Pole. It is likely that the AKR source was on the dayside and on
field lines near South Pole station. The general level of geomagnetic
activity was very low. However, an isolated magnetic impulse event (MIE)
accompanied by a riometer absorption pulse was in progress when all of the
VLF/radio noise bursts occurred. The very close association of the type III
burst at HF with the AKR is consistent with external stimulation of the AKR
if a different, more immediate, triggering process than that implied by
Calvert (1981) is invoked. It is suggested that some of the HF solar
radiant energy may decay into waves with frequencies comparable to those of
the AKR by parametric excitation or some other process, thus providing the
few background photons required for the generation of AKR by the Wu and Lee
(1979) cyclotron maser instability. The AKR, perhaps by modifying the
magnetospheric electron velocity distribution, might have produced the
observed VLF emissions. Alternatively, the VLF emissions may have arisen
from the same anisotropic and unstable electron distribution function
responsible for the AKR
	},
	keywords={
		atmospheric radiation
		atmospherics
		magnetosphere
		solar radiofrequency radiation
		auroral kilometric radiation
		VLF emissions
		type III solar radio noise
		broadband hiss
		LF noise
		magnetic impulse event
		triggering process
		HF solar radiant energy
		parametric excitation
		cyclotron maser instability
		magnetospheric electron velocity distribution
		electron distribution function
		AD 1984 11 12
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{RodriguezDec94,
	author={Rodriguez, J.V. and Inan, U.S. and Bell, T.F.},
	title={
Heating of the nighttime D region by very low frequency transmitters
	},
	journal={Journal of Geophysical Research},
	volume={99},
	number={A12},
	year={1994},
	month={Dec},
	pages={23329-38},
	abstract={
VLF signals propagating in the Earth-ionosphere waveguide are used to probe
the heated nighttime D-region over three U.S. Navy very low frequency (VLF,
3-30 kHz) transmitters. Ionospheric cooling and heating are observed when a
transmitter turns off and on in the course of normal operations. Heating by
the 24.0-kHz NAA transmitter in Cutler, Maine, (1000 kW radiated power) was
observed by this method in 41 of 52 off/on episodes during December 1992,
increasing the amplitude and retarding the phase of the 21.4-kHz NSS probe
wave propagating from Annapolis, Maryland, to Gander, Newfoundland, by as
much as 0.84 dB and 5.3 degrees , respectively. In six of these 41
episodes, the amplitude of the 28.5-kHz NAU probe wave propagating from
Puerto Rico to Gander was also perturbed by as much as 0.29 dB. The latter
observations were unexpected due to the >770 km distance between NAA and
the NAU-Gander great circle path. Heating by the NSS (21.4 kHz, 265 kW) and
NLK (24.8 kHz, 850 kW) transmitters was observed serendipitously in data
from earlier measurements of the amplitudes of VLF signals propagating in
the Earth-ionosphere waveguide. A three-dimensional model of wave
absorption and electron heating in a magnetized, weakly ionized plasma is
used to calculate the extent and shape of the collision frequency (i.e.
electron temperature) enhancement above a VLF transmitter. The calculated
changes in the D-region conductivity are used in a three-dimensional model
of propagation in the Earth-ionosphere waveguide to predict the effect of
the heated patch on a subionospheric VLF probe wave
	},
	keywords={
		D-region
		Earth-ionosphere waveguide
		ionospheric disturbances
		plasma radiofrequency heating
		radiowave propagation
		heated nighttime D-region
		Earth-ionosphere waveguide
		VLF signals
		ionospheric cooling
		ionospheric heating
		NAA transmitter
		NSS probe wave
		NAU probe wave
		NSS transmitter
		NLK transmitter
		3D propagation model
		wave absorption
		electron heating
		magnetized weakly ionized plasma
		collision frequency
		electron temperature enhancement
		D-region conductivity
		subionospheric VLF probe wave
		24 kHz
		21.4 kHz
		28.5 kHz
		24.8 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BellApr94,
	author={Bell, T.F. and Inan, U.S. and Lauben, D. and Sonwalkar, V.S. and Helliwell, R.A. and Sobolev, Ya.P. and Chmyrev, V.M. and Gonzalez, S.},
	title={
DE-1 and COSMOS 1809 observations of lower hybrid waves excited by VLF
whistler mode waves
	},
	journal={Geophysical Research Letters},
	volume={21},
	number={8},
	year={1994},
	month={Apr},
	pages={653-6},
	abstract={
Past work demonstrates that strong lower hybrid (LH) waves can be excited
by electromagnetic whistler mode waves throughout large regions of the
topside ionosphere and magnetosphere. The effects of the excited LH waves
upon the suprathermal ion population in the topside ionosphere and
magnetosphere depend upon the distribution of LH wave amplitude with
wavelength lambda . The present work reports plasma wave data from the DE-1
and COSMOS 1809 spacecraft which suggests that the excited LH wave spectrum
has components for which lambda <or=3.5 m when excitation occurs at a
frequency roughly equal to the local lower hybrid resonance frequency. This
wavelength limit is a factor of approximately 3 below that reported in past
work and suggests that the excited LH waves can interact with suprathermal
H/sup +/ ions with energy 16 eV. This finding supports recent work
concerning the heating of suprathermal ions above thunderstorm cells
	},
	keywords={
		ionosphere
		magnetosphere
		plasma waves
		whistlers
		ionosphere
		magnetosphere
		satellite observations
		lower hybrid wave
		VLF whistler mode wave
		plasma wave excitation
		electromagnetic whistler
		topside
		excited LH wave
		suprathermal ion population
		plasma wave
		DE-1
		COSMOS 1809
		H/sup +/
		suprathermal ion
		thunderstorm cell
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PaskoSep94,
	author={Pasko, V.P. and Inan, U.S.},
	title={
Recovery signatures of lightning-associated VLF perturbations as a measure
of the lower ionosphere
	},
	journal={Journal of Geophysical Research},
	volume={99},
	number={A9},
	year={1994},
	month={Sep},
	pages={17523-37},
	abstract={
A new model of the physical processes associated with subionospheric VLF
signal perturbations caused by lightning-induced electron precipitation
(LEP) bursts is developed to diagnose the state of the lower ionosphere
(e.g. electron number density and rate coefficients for various chemical
reactions) on the basis of measurements of VLF recovery signatures. The
model accounts for the energy spectrum of the electron bursts precipitated
by lightning-generated whistlers, the chemical relaxation of enhanced
secondary ionization in the nighttime D-region due to LEP bursts, and
quantitatively treats the resultant effects on propagation of the VLF
signal in the Earth-ionosphere waveguide. Application of the model to
experimental data obtained for the VLF propagation path from NPM station
(Hawaii) to Palmer station (Antarctica) indicates that effective electron
detachment rate gamma , enhanced secondary ionization profile (e.g. energy
content of LEP bursts), as well as the ambient electron density
distribution, may be estimated using observed subionospheric VLF recovery
signatures. The effective detachment rate was identified as approximately
10/sup -18/ N s/sup -1/, where N is total number density of neutrals. The
model indicates in particular that the attachment-detachment processes play
the dominant role in recovery of subionospheric VLF signal perturbations on
timescales approximately 100 s, and that the observed perturbations of the
NPM-Palmer signal correspond to the LEP bursts consisting of relatively
soft (<250 keV) electrons
	},
	keywords={
		ionospheric electromagnetic wave propagation
		lightning
		radiowave propagation
		whistlers
		lightning-associated VLF perturbations
		lower ionosphere
		model
		subionospheric VLF signal perturbations
		lightning-induced electron precipitation bursts
		electron number density
		rate coefficients
		chemical reactions
		VLF recovery signatures
		energy spectrum
		lightning-generated whistlers
		chemical relaxation
		enhanced secondary ionization
		nighttime D-region
		Earth-ionosphere waveguide
		effective electron detachment rate
		enhanced secondary ionization profile
		NPM Hawaii-Palmer signal propagation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SonwalkarSep94,
	author={Sonwalkar, V.S. and Inan, U.S. and Bell, T.F. and Helliwell, R.A. and Chmyrev, V.M. and Sobolev, Ya.P. and Ovcharenko, O.Ya. and Selegej, V.},
	title={
Simultaneous observations of VLF ground transmitter signals on the DE 1 and
COSMOS 1809 satellites: detection of a magnetospheric caustic and a duct
	},
	journal={Journal of Geophysical Research},
	volume={99},
	number={A9},
	year={1994},
	month={Sep},
	pages={17511-22},
	abstract={
Khabarovsk transmitter signals (15.0 kHz, 48 degrees N, 135 degrees E) were
observed on the high-altitude ( approximately 15000 km) Dynamic Explorer 1
(DE 1) and the low-altitude ( approximately 960) km COSMOS 1809 satellites
during a 9-day period in August 1989. On 7 out of 9 days the linear wave
receiver (LWR) on the DE 1 satellite detected signals from the Khabarovsk
transmitter. In addition, the DE 1 satellite also detected signals from the
Alpha transmitter (11.9-15.6 kHz) in Russia and an Omega transmitter
(10.2-13.6 kHz) in Australia, as well as natural VLF emissions such as
hiss, chorus, whistlers, and wideband impulsive signals. On two days,
August 23 and 27, observations of the Khabarovsk transmitter signals were
simultaneously carried out at high altitude on the DE 1 satellite and at
low altitude on the COSMOS 1809 satellite. Analysis of data from these 2
days has led to several new results on the propagation of whistler mode
signals in the Earth's magnetosphere. The authors report the first
detection of an exterior caustic surface near L approximately 3.5 for VLF
ground transmitter signals injected into the magnetosphere. They also
report the first direct detection of a magnetospheric duct at L=2.94 which
was believed to be responsible for the ducted propagation of Khabarovsk
signals observed on the COSMOS 1809 satellite. The results have direct
implications for the question of accessibility of waves injected from the
ground to various regions of the ionosphere and the magnetosphere
	},
	keywords={
		magnetospheric electromagnetic wave propagation
		radiowave propagation
		VLF ground transmitter signals
		Dynamic Explorer 1
		Cosmos 1809
		magnetospheric caustic
		magnetospheric duct
		Khabarovsk transmitter signals
		AD 1989 08
		linear wave receiver
		Alpha transmitter
		Omega transmitter
		natural VLF emissions
		hiss
		chorus
		wideband impulsive signals
		whistler mode signals
		Earth magnetosphere
		exterior caustic surface
		ionosphere
		15 Mm
		960 km
		15 kHz
		10.2 to 15.6 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{Jasna93,
	author={Jasna, D. and Inan, U.S. and Bell, T.F.},
	title={
Resonant interactions between radiation belt electrons and whistler mode
waves in the magnetosphere
	},
	journal={Publications of the Faculty of Electrical Engineering, Series: EngineeringPhysics},
	volume={},
	number={},
	year={1993},
	month={},
	pages={49-66},
	abstract={
A computer simulation model is developed to study the interaction between
relativistic charged particles and whistler mode waves traveling obliquely
with respect to the ambient magnetic field. The authors use this test
particle simulation model based on gyro-averaged equations of motion to
study the influence of oblique magnetospherically reflected (MR) whistlers
on the near-loss-cone distribution function of radiation belt electrons.
The authors find that MR whistlers originating in lightning can resonantly
interact with radiation belt electrons over a broad range of L-shells and
precipitate higher energy electrons from lower L-shells. Electrons in the
energy range of 1-26 MeV are precipitated from L=2, whereas from L=4 the
precipitated electron energy range is 150-220 keV. The precipitated
differential electron flux, due to this interaction, is higher for higher
L-shells, and the maximum value ranges from Phi /sub Eprec/(1.11
MeV)=5.2*10/sup -4/ el/cm/sup 2/.s.keV at L=2 to Phi /sub Eprec/(173
keV)=4.6*10/sup -1/ el/cm/sup 2/.s.keV at L=4. The lifetimes of radiation
belt electrons in a given magnetic flux tube around the L-shell on which
the interaction takes place are found to be of the order of several days,
comparable to lifetimes corresponding to electron loss induced by hiss,
which was heretofore assumed to be the dominant loss mechanism. The minimum
electron lifetimes vary from 2.47 days for E=1.11 MeV electrons at L=2 to
4.64 days for E=173 keV electrons at L=4
	},
	keywords={
		atmospheric electron precipitation
		electromagnetic waves
		radiation belts
		whistlers
		resonant interaction
		radiation belt electrons
		whistler mode waves
		magnetosphere
		particle sources
		loss processes
		dynamic equilibrium
		pitch angle
		energetic electrons
		computer simulation model
		relativistic charged particles
		ambient magnetic field
		oblique magnetospherically reflected whistlers
		loss-cone distribution
		L-shells
		electron precipitation
		radiation belt electron lifetimes
		magnetic flux tube
		electron loss
		150 keV to 2.6 MeV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Bell93,
	author={Bell, T.F. and Inan, U.S. and Reising, S.C. and Rodriguez, J.V.},
	title={
VLF signatures of ionospheric heating by HIPAS
	},
	booktitle={Proceedings and Program for the 7th International Ionospheric EffectsSymposium},
	volume={},
	number={},
	year={1993},
	month={},
	pages={6B/4/1},
	abstract={
Summary form only given, as follows. The amplitude and phase of
subionospherically propagating VLF signals are known to be sensitive
indicators of the electron density and temperature at D-region altitudes.
The authors describe new observations at multiple stations in Alaska
positioned to provide measurements of VLF signals that have propagated
beneath the ionospheric region heated by the HIPAS HF heating facility.
Preliminary analysis of data from the HIPAS campaign conducted in
September-October 1992, has demonstrated the feasibility of the
measurement. In one case, the amplitude of the 23.4 kHz signal from the NPM
transmitter in Hawaii as measured in Fort Yukon, Alaska, exhibited a
approximately 0.3 dB change in amplitude with the same 100 ms on/900 ms off
modulation pattern as that of the HIPAS HF transmissions at 2.8 MHz.
Results of observations on different days and at two stations in Alaska are
reviewed
	},
	keywords={
		D-region
		electromagnetic wave propagation in plasma
		electron density
		ionospheric electromagnetic wave propagation
		ionospheric techniques
		plasma radiofrequency heating
		radiowave propagation
		AD 1992 09 to 10
		on/off modulation
		ionospheric heating
		VLF signals
		electron density
		temperature
		D-region altitudes
		Alaska
		HIPAS HF heating facility
		measurement
		NPM transmitter
		Hawaii
		Fort Yukon
		HF transmissions
		23.4 kHz
		2.8 MHz
		100 ms
		900 ms
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Inan93,
	author={Inan, U.S. and Lev-Tov, S.},
	title={
Lightning-induced ionospheric disturbances and their effects on VLF/ELF
propagation
	},
	booktitle={Proceedings and Program for the 7th International Ionospheric EffectsSymposium},
	volume={},
	number={},
	year={1993},
	month={},
	pages={5B1/7/1},
	abstract={
Transient perturbations in the amplitude and phase of subionospheric
VLF/ELF signals, observed in association with lightning discharges, are
interpreted using a new three dimensional model of VLF/ELF propagation.
Data from a few different colinearly configured great circle paths are
compared with one another and with model predictions for different
ionospheric conditions and localized disturbance characteristics (size,
location, altitude profile). Transient amplitude changes on the 24.8 kHz
signals, originating respectively at Jim Creek, Washington and Silver
Creek, Nebraska are found at times to be up to 5-10 dB, although more
typical changes are <5 dB. Comparison with the model indicates a sensitive
dependence on the location of the disturbance along the propagation path
	},
	keywords={
		ionosphere
		ionospheric electromagnetic wave propagation
		lightning
		radiowave propagation
		United States
		ELF
		VLF
		ionospheric disturbances
		propagation
		amplitude
		phase
		lightning discharges
		great circle paths
		Jim Creek
		Washington
		Silver Creek
		Nebraska
		28.4 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{RodriguezJan94,
	author={Rodriguez, J.V. and Inan, U.S.},
	title={
Electron density changes in the nighttime D region due to heating by
very-low-frequency transmitters
	},
	journal={Geophysical Research Letters},
	volume={21},
	number={2},
	year={1994},
	month={Jan},
	pages={93-6},
	abstract={
Modification of the nighttime D-region electron density (N/sub e/) due to
heating by very-low-frequency (VLF) transmitters is investigated
theoretically using a four-species model of the ion chemistry. The effects
of a 100 kW, a 265 kW, and a 1000 kW VLF transmitter are calculated for
three ambient N/sub e/ profiles. The results indicate that N/sub e/ is
reduced by up to 26% at approximately 80 km altitude over a 1000 kW
transmitter
	},
	keywords={
		atmospheric chemistry
		atmospheric ionisation
		D-region
		electron density
		ionospheric electromagnetic wave propagation
		ionosphere electron density modification
		lower ionosphere VLF heating
		aeronomy
		VLF transmitter power
		upper atmosphere chemistry
		very-low-frequency transmitters
		nighttime D-region electron density
		four-species model
		ion chemistry
		50 to 100 km
		90 to 95 km
		21.4 to 28.5 kHz
		24.0 kHz
		100 to 1000 kW
		70 to 90 km
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{TaranenkoDec93,
	author={Taranenko, Y.N. and Inan, U.S. and Bell, T.F.},
	title={
The interaction with the lower ionosphere of electromagnetic pulses from
lightning: excitation of optical emissions
	},
	journal={Geophysical Research Letters},
	volume={20},
	number={23},
	year={1993},
	month={Dec},
	pages={2675-8},
	abstract={
A self consistent and fully kinetic simulation of the interaction of
lightning radiated electromagnetic (EM) pulses with the nighttime lower
ionosphere indicates that optical emissions observable with conventional
instruments would be excited. For example, emissions of the 1st and 2nd
positive bands of N/sub 2/ occur at rates reaching 7*10/sup 7/ and 10/sup
7/ cm/sup -3/ s/sup -1/ respectively at approximately 92 km altitude for a
lightning discharge with an electric field E/sub 100/=20 V/m (normalized to
a 100 km distance). The maximum height integrated intensities of these
emissions are 4*10/sup 7/ and 6*10/sup 6/ R respectively lasting for
approximately 50 mu s
	},
	keywords={
		atmospherics
		D-region
		lightning
		nightglow
		nitrogen
		plasma
		thermosphere
		lower ionosphere
		electromagnetic pulses
		lightning
		optical emissions excitation
		kinetic simulation
		nighttime
		2nd positive band
		1st positive band
		electric field
		maximum height integrated intensities
		92 km
		N/sub 2/
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SonwalkarApr94,
	author={Sonwalkar, V.S. and Inan, U.S. and Bell, T.F. and Helliwell, R.A. and Molchanov, O.A. and Green, J.L.},
	title={
DE 1 VLF observations during Activny wave injection experiments
	},
	journal={Journal of Geophysical Research},
	volume={99},
	number={A4},
	year={1994},
	month={Apr},
	pages={6173-86},
	abstract={
Reports on coordinated high-altitude satellite observations in support of
one of space-based VLF wave injection experiments, namely the USSR Aktivny
mission. The Activny satellite (A) was designed to carry a VLF transmitter
(freq approximately 10 kHz, power approximately 10 kW) coupled to a
20-m-diameter loop antenna in a nearly polar orbit (83 degrees inclination,
apogee approximately 2500 km, perigee approximately 500 km). The authors
focus their attention on conjunction experiments between the Activny and DE
1 satellites. Because of problems in the deployment of the loop antenna,
the radiated power capability of the antenna was significantly reduced. The
DE 1/Activny conjunction experiments were carried out as a means of
possibly placing an upper limit on the radiated power. During the period
November 1989 through April 1990, a total of 10 DE 1/Activny wave injection
sessions were conducted. During each session the Activny transmitter
operated at 10.537 kHz with 1 s On-1 s Off format, for a period of 6 min
centered around the conjunction time. During three conjunction periods both
DE 1 and Activny were in the southern hemisphere, and DE 1 was at
relatively low altitudes, thus providing the best conjunction possibilities
according to the ray tracing criteria developed above. On most days Omega
transmitter signals as well as commonly occurring natural wave phenomena
such as whistlers and hiss were clearly seen but there was no evidence of
the Activny 1 s On/1 s Off pattern. The experimental constraints allow an
upper limit to be placed on the total power radiated by the Activny
transmitter in the whistler-mode
	},
	keywords={
		magnetospheric electromagnetic wave propagation
		whistlers
		magnetosphere
		conjugate radiowave propagation
		whistler
		VLF
		DE 1
		Activny wave injection experiment
		AD 1989
		AD 1990
		USSR Aktivny
		upper limit
		radiated power
		conjugate hemisphere
		radiowave injection
		whistlers
		total power radiated
		on off pattern
		satellite experiment
		10.537 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PaquetteMar94,
	author={Paquette, J.A. and Matthews, D.J. and Rosenberg, T.J. and Lanzerotti, L.J. and Inan, U.S.},
	title={
Source regions of long-period pulsation events in electron precipitation
and magnetic fields at South Pole Station
	},
	journal={Journal of Geophysical Research},
	volume={99},
	number={A3},
	year={1994},
	month={Mar},
	pages={3869-77},
	abstract={
Pulsation events with long (100-1000 s) periods with a consistent frequency
in both particle precipitation and surface geomagnetic field variations
have been reported in data from South Pole Station (1982-1989). The onset
times of these events were determined, and the results compared with
predictions based on the work of Coroniti and Kennel (1970). This mechanism
ascribes the occurrence of correlated magnetic and precipitation pulsations
to ULF modulation of equatorial VLF wave-particle interactions. For this
reason, VLF data from South Pole Station were also examined. Taking into
consideration the ULF wave and particle transit times from an interaction
region near the magnetic equator to the ground leads to an expectation that
the onset of pulsations in the magnetometer data will lag the onset of
pulsations in the riometer data by several minutes. This disparity in onset
times, together with modulation of VLF emissions in the 0.5-1 kHz band,
serves as an important indicator of whether or not an event can be
explained by the above-cited theory. While about a third of the events fit
the prediction of Coroniti and Kennel, another third do not. In these
events, the onset of magnetic and precipitation pulsations is nearly
simultaneous, and possible alternative generation mechanisms are explored.
In the remaining third of the events, magnetic pulsations begin
substantially earlier than precipitation pulsations. This third class of
events is probably the result of the differing areas to which the riometer
and magnetometer are sensitive and can be accounted for by considering the
effects of transverse motion of a persistent precipitation region
	},
	keywords={
		atmospheric electron precipitation
		magnetosphere
		micropulsations
		plasma waves
		long-period pulsation events
		electron precipitation
		magnetic fields
		South Pole Station
		long-period pulsation event
		surface geomagnetic field variations
		onset times
		ULF modulation
		equatorial VLF wave-particle interactions
		VLF data
		interaction region
		magnetic pulsations
		100 to 1000 s
		0.5 to 1.0 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanNov93,
	author={Inan, U.S. and Rodriguez, J.V. and Idone, V.P.},
	title={
VLF signatures of lightning-induced heating and ionization of the nighttime
D-region
	},
	journal={Geophysical Research Letters},
	volume={20},
	number={21},
	year={1993},
	month={Nov},
	pages={2355-8},
	abstract={
48.5 kHz signals from a transmitter in Silver Creek, Nebraska, propagating
to Huntsville (HU), Alabama over a approximately 1200 km Great Circle Path
(GCP) exhibit characteristic amplitude changes which appear within 20 ms of
cloud-to-ground (CG) flashes located within 50 km of the path. The data are
consistent with the heating of ionospheric electrons by the electromagnetic
(EM) pulse from lightning, producing ionization changes in the D-region
over the thunderstorm
	},
	keywords={
		atmospheric ionisation
		atmospheric temperature
		D-region
		ionospheric electromagnetic wave propagation
		lightning
		thunderstorms
		ionosphere VLF waves propagation
		central United States
		ionospheric electrons heating
		lightning EM pulse
		USA
		ionosphere D-region ionisation
		lightning-induced ionisation
		cloud-to-ground flashes
		VLF signals amplitude changes
		lower ionosphere
		AD 1990 01 25
		VLF signatures
		lightning-induced heating
		nighttime D-region
		48.5 kHz signals
		Silver Creek
		Nebraska
		Huntsville
		Alabama
		Great Circle Path
		thunderstorm
		48.5 kHz
		20 ms
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BellSep93,
	author={Bell, T.F. and Helliwell, R.A. and Inan, U.S. and Lauben, D.S.},
	title={
The heating of suprathermal ions above thunderstorm cells
	},
	journal={Geophysical Research Letters},
	volume={20},
	number={18},
	year={1993},
	month={Sep},
	pages={1991-4},
	abstract={
Ion heating in the topside ionosphere directly over thunderstorm cells is
estimated. The primary heating is due to lower hybrid waves excited through
linear mode coupling as intense electromagnetic (EM) whistler mode
radiation from lightning is scattered from small scale (2-20 m)
magnetic-field-aligned plasma density irregularities in the topside
ionosphere. For typical radiated EM fields, it was found that suprathermal
H/sup +/ ions in the >or=6 eV energy range can be heated by 20 to 40 eV as
a result of a single lightning discharge. They also show how the number
density of >or=6 eV H/sup +/ ions is enhanced by preheating resulting from
the absorption of proton whistlers in the 500-1000 km altitude range. For
lightning discharge rates of one or more per second over a 10/sup 4/ km/sup
2/ area, the authors' model predicts a total energy gain for the H/sup +/
ions of 400 eV to 2 KeV and a perpendicular ion flux of j/sub perpendicular
to / approximately 10/sup 5/ to 10/sup 6/ cm/sup -2/ sec/sup -1/. These
fluxes should be observable on low altitude spacecraft using presently
available instrumentation
	},
	keywords={
		ionosphere
		ionospheric electromagnetic wave propagation
		thunderstorms
		whistlers
		ion heating
		lower atmosphere
		meteorology
		plasma wave
		radiowave
		suprathermal ions
		thunderstorm cells
		topside ionosphere
		lower hybrid waves
		linear mode coupling
		intense electromagnetic
		whistler mode radiation
		lightning
		field-aligned plasma density irregularities
		H/sup +/
		whistlers
		500 to 1000 km
		H
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{TaranenkoAug93,
	author={Taranenko, Y.N. and Inan, U.S. and Bell, T.F.},
	title={
Interaction with the lower ionosphere of electromagnetic pulses from
lightning: heating, attachment, and ionization
	},
	journal={Geophysical Research Letters},
	volume={20},
	number={15},
	year={1993},
	month={Aug},
	pages={1539-42},
	abstract={
A Boltzmann formulation of the electron distribution function and Maxwell's
equations for the electromagnetic (EM) fields are used to simulate the
interaction of lightning radiated EM pulses with the lower ionosphere.
Ionization and dissociative attachment induced by the heated electrons
cause significant changes in the local electron density (N/sub e/). Due to
'slow' field changes of typical lightning EM pulses over time scales of
tens of mu s, the distribution function follows the quasi-equilibrium
solution of the Boltzmann equation in the altitude range of interest (70 to
100 km). The EM pulse is simulated as a planar 100 mu s-long single period
oscillation of a 10-kHz wave injected at 70 km. Under nighttime conditions,
individual pulses of intensity 10-20 V/m (normalized to 100 km horizontal
distance) produce changes in N/sub e/ of 1-30% while a sequence of pulses
leads to strong modification of N/sub e/ at altitudes <95 km. The N/sub e/
changes produce a 'sharpening' of the lower ionospheric boundary by causing
a reduction in electron density at 75-85 km (due to attachment) and a
substantial increase at 85-95 km (due to ionization) (e.g. the scale height
decreases by a factor of approximately 2 at approximately 85 km for a
single 20 V/m EM pulse). No substantial N/sub e/ changes occur during
daytime
	},
	keywords={
		atmospheric ionisation
		electromagnetic pulse
		electron attachment
		ionospheric electromagnetic wave propagation
		lightning
		plasma heating
		lower ionosphere
		lightning radiated EM pulses
		heating
		VLF perturbations
		ionization
		Boltzmann equation
		Maxwell equations
		dissociative attachment
		heated electrons
		local electron density
		oscillation
		nighttime conditions
		modification
		70 to 100 km
		100 mus
		10 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Inan93,
	author={Inan, U.S. and Rodriguez, J.V.},
	title={
Lightning-induced effects on VLF/LF radio propagation
	},
	booktitle={ELF/VLF/LF Radio Propagation and Systems Aspects (AGARD-CP-529)},
	volume={},
	number={},
	year={1993},
	month={},
	pages={9/10 pp.},
	abstract={
At least two different ways in which energy from lightning discharges
couples into the lower ionosphere and the radiation belts have come to the
fore. This paper briefly reviews these results especially from the point of
view of their effects on VLF/LF radio propagation in the earth-ionosphere
waveguide. Lightning-induced electron precipitation, and lightning-induced
heating and ionization of the lower ionosphere are discussed. A planned
active VLF wave-injection experiment is designed to investigate ionospheric
heating by VLF waves under controlled conditions and to generate ELF waves
by modulated VLF heating
	},
	keywords={
		atmospheric electron precipitation
		atmospheric ionisation
		ionospheric electromagnetic wave propagation
		lightning
		radiation belts
		radiowave propagation
		lightning-induced electron precipitation
		lower ionosphere
		radiation belts
		VLF/LF radio propagation
		earth-ionosphere waveguide
		lightning-induced heating
		ionospheric heating
		modulated VLF heating
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PoulsenSep93,
	author={Poulsen, W.L. and Bell, T.F. and Inan, U.S.},
	title={
The scattering of VLF waves by localized ionospheric disturbances produced
by lightning-induced electron precipitation
	},
	journal={Journal of Geophysical Research},
	volume={98},
	number={A9},
	year={1993},
	month={Sep},
	pages={15553-9},
	abstract={
A 3D model of the scattering of VLF waves in the Earth-ionosphere waveguide
by localized disturbances in the lower ionosphere is examined for typical
disturbances expected to be produced by lightning-induced electron
precipitation events. Results indicate that the scattering is generally
independent of the conductivity and permittivity of the Earth's surface
immediately beneath the disturbed region except for extremely low
conductivities such as that found over deep ice caps. Thus the scattered
signal is principally a function of the ionospheric perturbation. For
typical disturbances characterized by altitude profiles of enhanced
ionization expected for 1.4<or=L<or=3, most of the measurable wave energy
scatters within a fairly narrow angular region centered on the forward
scatter direction. Thus moderate to large-scale disturbances (radius 50-200
km) must be located within <250 km of a moderate-length path (3000-16.000
km) in order to scatter a measurable signal to the receiver. These two
findings suggest that the scattered signals can be used with confidence as
a diagnostic tool to determine the characteristics of the energetic
electron precipitation
	},
	keywords={
		atmospheric electron precipitation
		ionospheric electromagnetic wave propagation
		ionospheric techniques
		radiowave propagation
		measurement technique
		radiowave propagation
		scattering
		VLF
		localized ionospheric disturbance
		lightning-induced electron precipitation
		model
		three dimensional
		Earth-ionosphere waveguide
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BurgessSep93,
	author={Burgess, W.C. and Inan, U.S.},
	title={
The role of ducted whistlers in the precipitation loss and equilibrium flux
of radiation belt electrons
	},
	journal={Journal of Geophysical Research},
	volume={98},
	number={A9},
	year={1993},
	month={Sep},
	pages={15643-65},
	abstract={
New experimental evidence suggests that every ducted whistler component may
precipitate bursts of radiation belt electrons into geomagnetically
conjugate ionospheric regions. Strong spatial and temporal associations are
seen between transient ionospheric disturbances observed in conjugate
regions and ducted whistlers monitored at Palmer Station, Antarctica. The
ionospheric disturbances were detected by their characteristic perturbing
effects ("Trimpi events") on subionospheric VLF, LF, and MF signals
recorded at Palmer Station and at northern hemisphere sites. Of 74 such
events examined on four different days, all were time-associated with
ducted whistlers. In no case was the arrival azimuth or dispersion of the
associated whistlers inconsistent with the locations of the conjugate
ionospheric disturbances, which were inferred from the configuration of
perturbed signal paths. Signal perturbation onset behavior was consistent
with multiple regions of precipitation induced by components of multipath
whistlers and with theoretical predictions for ducted whistler-induced
precipitation. The results not only support the hypothesis that ducted
whistlers are responsible for burst precipitation of energetic electrons
but imply that such bursts may be induced by every ducted whistler
component
	},
	keywords={
		atmospheric electron precipitation
		magnetospheric electromagnetic wave propagation
		radiation belts
		whistlers
		EM wave particle interaction
		magnetosphere
		ducted whistler
		precipitation loss
		equilibrium flux
		radiation belt
		electron precipitation
		bursts
		geomagnetically conjugate ionospheric regions
		transient ionospheric disturbance
		Trimpi event
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{DraganovJul93,
	author={Draganov, A.B. and Inan, U.S. and Sonwalkar, V.S. and Bell, T.F.},
	title={
Whistlers and plasmaspheric hiss: wave directions and three-dimensional
propagation
	},
	journal={Journal of Geophysical Research},
	volume={98},
	number={A7},
	year={1993},
	month={Jul},
	pages={11401-10},
	abstract={
Wave data from the DE 1 satellite showing simultaneously nonducted
whistlers and hiss are analyzed to determine wave propagation directions.
At L=3.8 and a geographic latitude of lambda /sub g/=12 degrees S, the
average wave normal directions of discrete whistlers are measured to be
approximately 51 degrees for f=4.5 kHz and approximately 60 degrees for
f=3.5 kHz, forming a small (<20 degrees ) angle with the magnetic
meridional plane. Hiss wave normal angles were determined as approximately
70 degrees and approximately 77 degrees for f=3.5 kHz and 2.5 kHz,
respectively, with the wave vector being almost perpendicular to the
meridional plane. While the measured wave normal angles of whistlers and
hiss are consistent with generation of hiss by magnetospheric whistlers,
the existence of a significant azimuthal component indicates that further
assessment of this connection must be based on three-dimensional ray
tracing. A new approximate analytical formation of three-dimensional
propagation of whistler waves is developed and used to model the drift of
magnetospherically reflected whistlers in azimuth
	},
	keywords={
		magnetospheric electromagnetic wave propagation
		whistlers
		whistler
		plasmasphere
		radiowave emission
		magnetosphere
		radiowave
		ELF
		VLF
		AD 1982 03 24
		hiss
		three-dimensional propagation
		directions
		whistlers
		wave normal angles
		azimuthal component
		ray tracing
		model
		2.5 to 4.5 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{HendersonJun93,
	author={Henderson, T.R. and Sonwalkar, V.S. and Helliwell, R.A. and Inan, U.S. and Fraser-Smith, A.C.},
	title={
A search for ELF/VLF emissions induced by earthquakes as observed in the
ionosphere by the DE 2 satellite
	},
	journal={Journal of Geophysical Research},
	volume={98},
	number={A6},
	year={1993},
	month={Jun},
	pages={9503-14},
	abstract={
Satellite observations of ELF/VLF wave activity by groups from both the
Soviet Union and France have indicated the possibility of ELF/VLF radio
emissions generated by earthquakes. However, an examination of ELF/VLF wave
data from the low-altitude Dynamics Explorer 2 (DE 2) satellite showed no
clearly distinguishable ELF/VLF signatures associated with earthquakes.
After an initial survey of approximately 5000 DE 2 orbits, ELF and VLF wave
data were selected from 63 satellite orbits, called earthquake orbits, in
which the ionospheric footprint of the DE 2 crossed the geographic latitude
while passing within +or-20 degrees geographic longitude of the epicenters
of imminent or recent earthquakes of magnitude >or=5.0. ELF/VLF noise
measured near the epicenters was analyzed for occurrence rates and average
spectra, as well as for peak and mean electric field intensities in three
spectrometers covering a frequency range of 4 Hz-512 kHz in 20 channels
	},
	keywords={
		atmospheric radiation
		earthquakes
		ionosphere
		ionospheric electromagnetic wave propagation
		magnetosphere
		terrestrial electricity
		ELF
		VLF
		radiowave emission
		earthquake induced
		EM wave
		geoelectric
		precursor
		AD 1983
		magnetosphere
		AD 1981
		AD 1982
		ionosphere
		DE 2
		0.3 to 512 kHz
		4 to 300 Hz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PoulsenFeb93,
	author={Poulsen, W.L. and Inan, U.S. and Bell, T.F.},
	title={
A multiple-mode three-dimensional model of VLF propagation in the
Earth-ionosphere waveguide in the presence of localized D region
disturbances
	},
	journal={Journal of Geophysical Research},
	volume={98},
	number={A2},
	year={1993},
	month={Feb},
	pages={1705-17},
	abstract={
Transient localized D region disturbances, such as those associated with
lightning discharges, affect the characteristics of VLF waves propagating
in the Earth-ionosphere waveguide. In particular, both phase and amplitude
changes in the subionospheric signal can be observed at receiving sites as
a result of the wave scattering that takes place in the disturbed region.
The authors present a multiple-mode three-dimensional model of VLF
propagation in the Earth-ionosphere waveguide in the presence of localized
D region disturbances. This new model is applied to experimental
observations and is found to be in general agreement. The diagnostics
potential of the model for characterizing energetic particle precipitation
events is discussed
	},
	keywords={
		atmospheric elementary particle precipitation
		D-region
		ionospheric electromagnetic wave propagation
		radiowave propagation
		D-region
		radiowave propagation
		multiple-mode three-dimensional model
		VLF propagation
		Earth-ionosphere waveguide
		VLF waves
		phase
		amplitude
		subionospheric signal
		energetic particle precipitation events
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanOct92,
	author={Inan, U.S. and Rodriguez, J.V. and Lev-Tov, S. and Oh, J.},
	title={
Ionospheric modification with a VLF transmitter
	},
	journal={Geophysical Research Letters},
	volume={19},
	number={20},
	year={1992},
	month={Oct},
	pages={2071-4},
	abstract={
Detectable heating of the nighttime D-region by a 28.5 kHz signal is
observed in 16 out of 144 cases with events occurring under conditions of
moderate to low D-region electron densities as represented by the
unperturbed VLF signal levels. Three dimensional modeling of the effects of
NAU heating on a probe VLF signal predicts values in general agreement with
observations and suggests that maximum effects should occur under tenuous
D-region conditions
	},
	keywords={
		D-region
		ionospheric electromagnetic wave propagation
		plasma radiofrequency heating
		night
		radiowave heating
		D-region
		ionosphere modification
		three-dimensional model
		AD 1989
		VLF transmitter
		nighttime
		modeling
		28.5 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{RodriguezOct92,
	author={Rodriguez, J.V. and Inan, U.S. and Bell, T.F.},
	title={
D region disturbances caused by electromagnetic pulses from lightning
	},
	journal={Geophysical Research Letters},
	volume={19},
	number={20},
	year={1992},
	month={Oct},
	pages={2067-70},
	abstract={
Electromagnetic pulses from weak lightning discharges (E/sub 100/=1 V/m,
where E/sub 100/ is the field strength in the radiation pattern maximum at
100 km) may substantially heat D region electrons, while only pulses with
E/sub 100/>or=20 V/m may create electron density enhancements >or=10% of
ambient. A E/sub 100/=20 V/m pulse from a horizontal radiator at 5 km
altitude (e.g. the cloud discharge at the stepped-leader onset) increases
the electron temperature by a factor of approximately 400 maximum and the
electron density (in one ionization cycle) by approximately 230 cm/sup 3/
maximum; the widths at half-maximum of the heated and ionized regions are
200 km and 90 km. A E/sub 100/=40 V/m pulse from a vertical radiator at 0
km altitude (e.g. the vertical return stroke channel) increases the
electron temperature by a factor of approximately 350 maximum and the
electron density by approximately 80 cm/sup 3/ maximum
	},
	keywords={
		D-region
		lightning
		electron heating
		modification
		EM pulse
		EM radiation
		disturbance
		radiowave emission
		D-region
		ionosphere
		electromagnetic pulses
		lightning
		electron temperature
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{TaranenkoSep92,
	author={Taranenko, Y.N. and Inan, U.S. and Bell, T.F.},
	title={
Optical signatures of lightning-induced heating of the D region
	},
	journal={Geophysical Research Letters},
	volume={19},
	number={18},
	year={1992},
	month={Sep},
	pages={1815-18},
	abstract={
Lightning-induced heating of the nighttime D region leads to the excitation
of a number of lines of O, O/sub 2/, N/sub 2/, O/sub 2//sup +/, and N/sub
2//sup +/, at intensities of 10-10/sup 9/ rayleighs (R) for vertical
observations. For example, the 5577 AA emission from O has intensity
approximately 60 R lasting for approximately 350 ms while the 1st and 2nd
positive bands of N/sub 2/ are at approximately 10/sup 9/ R but last only
approximately 50 mu s
	},
	keywords={
		airglow
		D-region
		lightning
		plasma heating
		visible
		D-region
		ionosphere
		airglow
		lightning-induced heating
		O
		O/sub 2/
		N/sub 2/
		O/sub 2//sup +/
		N/sub 2//sup +/
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{GlukhovNov92,
	author={Glukhov, V.S. and Pasko, V.P. and Inan, U.S.},
	title={
Relaxation of transient lower ionospheric disturbances caused by
lightning-whistler-induced electron precipitation bursts
	},
	journal={Journal of Geophysical Research},
	volume={97},
	number={A11},
	year={1992},
	month={Nov},
	pages={16971-9},
	abstract={
A quantitative model of the relaxation of transient lower ionospheric
(D-region) disturbances caused by lightning-induced electron precipitation
is developed, taking advantage of known particular features of the
lightning-induced disturbances, such as the fact that they are produced in
typically <1 s and decay over 10-100 s. The model represents the nighttime
D-region as consisting of only four kinds of charged particles (electrons,
positive ions, negative ions, and positive cluster ions) and is
particularly suited for description of the detailed behavior of the
electron density. Application of the model to some previously modeled
disturbances indicates that some of the least known chemical reaction rates
in the nighttime D-region altitudes may be measurable using subionospheric
VLF data
	},
	keywords={
		atmospheric electron precipitation
		D-region
		ionosphere
		lightning
		D-region
		transient lower ionospheric disturbances
		lightning-whistler-induced electron precipitation bursts
		quantitative model
		relaxation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{JasnaAug92,
	author={Jasna, D. and Inan, U.S. and Bell, T.F.},
	title={
Precipitation of suprathermal (100 eV) electrons by oblique whistler waves
	},
	journal={Geophysical Research Letters},
	volume={19},
	number={16},
	year={1992},
	month={Aug},
	pages={1639-42},
	abstract={
Electron precipitation induced by oblique whistler waves is investigated
using a new test particle simulation code based on gyro-averaged equations
of motion. The results indicate that highly oblique waves can efficiently
pitch angle scatter suprathermal electrons (10-100 eV). At L=3, for
example, in a single encounter with a wave with power density S
approximately 8 pW/m/sup 2/ propagating at psi =60 degrees with respect to
the Earth's magnetic field B/sub 0/, the average pitch angle scattering of
100 eV electrons is approximately 0.1 degrees . In comparison, the average
scattering of energetic (100 keV) electrons by a parallel propagating wave
with the same S is approximately 0.01 degrees . Estimates indicate that the
precipitated electron energy fluxes resulting from the interaction of
approximately 100 eV electrons with oblique waves can be up to 30 times
larger than that due to the precipitation of 100 keV electrons by parallel
propagating waves
	},
	keywords={
		atmospheric electron precipitation
		magnetosphere
		magnetospheric electromagnetic wave propagation
		plasma
		radiation belts
		whistlers
		radiation belt electrons
		VLF
		magnetosphere suprathermal electrons precipitation
		wave-particle interactions
		wave propagation direction
		whistler wave power density
		oblique whistler waves
		test particle simulation code
		gyro-averaged equations of motion
		highly oblique waves
		average pitch angle scattering
		precipitated electron energy fluxes
		100 eV
		10 to 25 kHz
		5.60 to 15.79 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{ImhofSep92,
	author={Imhof, W.L. and Voss, H.D. and Mobilia, J. and Datlowe, D.W. and Gaines, E.E. and McGlennon, J.P. and Inan, U.S.},
	title={
Relativistic electron microbursts
	},
	journal={Journal of Geophysical Research},
	volume={97},
	number={A9},
	year={1992},
	month={Sep},
	pages={13829-37},
	abstract={
The authors report the first satellite observations of relativistic (>1
MeV) electron precipitation in microbursts with measured durations of less
than 1 s. The data on these relativistic microbursts appear to indicate
that many of the bursts may be due to wave-particle interaction not with
whistler mode chorus but possibly with other waveforms. The locations of
many of the relativistic microbursts are concentrated at the outer edge of
the trapped radiation belt, where the gyroradii of the electrons are
comparable to the curvature of the magnetic field lines and stable trapping
may therefore not occur. The preferred location of the microbursts, which
may be primarily spatial in character, implies the possible importance of
irregularities in the magnetic field lines near the trapping boundary as
the responsible mechanism
	},
	keywords={
		atmospheric electron precipitation
		radiation belts
		magnetosphere
		atmosphere
		electron microbursts
		relativistic microbursts
		wave-particle interaction
		trapped radiation belt
		gyroradii
		1 MeV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanApr92,
	author={Inan, U.S. and Chiu, Y.T. and Davidson, G.T.},
	title={
Whistler-mode chorus and morningside aurorae
	},
	journal={Geophysical Research Letters},
	volume={19},
	number={7},
	year={1992},
	month={Apr},
	pages={653-6},
	abstract={
Quasi-electrostatic ELF/VLF chorus emissions immediately above the
equatorial half-gyrofrequency, observed to propagate with wave normal angle
( psi ) within 0.4-1.2 degrees of the resonance cone ( psi /sub r/) (Muto
et al., 1987), are shown to efficiently resonate with 0.1-10 keV electrons.
These waves may thus be important in driving the relatively low energy (<10
keV) component of pulsating aurorae and the morning-side diffuse aurorae (
approximately 1 keV)
	},
	keywords={
		atmospheric electron precipitation
		aurora
		magnetospheric electromagnetic wave propagation
		radiowave propagation
		whistlers
		whistler mode chorus
		electron precipitation
		quasielectrostatic ELF-VLF chorus emission
		radiowaves
		magnetosphere
		morningside aurorae
		pulsating aurorae
		diffuse aurorae
		0.1 to 10 keV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{DraganovFeb92,
	author={Draganov, A.B. and Inan, U.S. and Sonwalkar, V.S. and Bell, T.F.},
	title={
Magnetospherically reflected whistlers as a source of plasmaspheric hiss
	},
	journal={Geophysical Research Letters},
	volume={19},
	number={3},
	year={1992},
	month={Feb},
	pages={233-6},
	abstract={
Ray-tracing simulations and estimates of whistler wave damping show that
magnetospherically reflected whistlers can persist for approximately 10/sup
2/ s in a low frequency band (f approximately 1 kHz). The combined
contribution from whistler rays produced by a single lightning flash but
entering the magnetosphere at different points form a continuous hiss-like
signal, as observed at a fixed point. Estimates indicate that the total
whistler wave energy input into the magnetosphere from lightning discharges
may maintain experimentally observed levels of magnetospheric hiss
	},
	keywords={
		magnetosphere
		magnetospheric electromagnetic wave propagation
		whistlers
		magnetosphere
		plasmasphere
		radiowave emission
		ELF
		whistler
		reflection
		reflected whistlers
		hiss
		whistler wave damping
		lightning
		magnetosphere
		1 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{MielkeJan92,
	author={Mielke, T.A. and Elkins, C.J. and Helliwell, R.A. and Inan, U.S.},
	title={
Excitation of whistler mode signals via injection of polarized VLF waves
with the Siple transmitter
	},
	journal={Radio Science},
	volume={27},
	number={1},
	year={1992},
	month={Jan},
	pages={31-46},
	abstract={
Whistler mode waves (2-4 kHz) of various polarizations were transmitted by
the Siple Station, Antarctica, VLF transmitter and received near the
geomagnetic conjugate point at Lake Mistissini, Quebec. Excitation of a
multiplicity of magnetospheric propagation paths and the received signal
strength were observed to depend on the transmitter antenna polarization.
Where whistler mode growth and emission triggering occurred, saturated peak
values of received signals were independent of antenna polarization and
initial injected power levels. Propagation paths of ducted Siple signals
observed at Lake Mistissini were identified with propagation paths deduced
from natural whistlers, from which the L shell values and equatorial number
densities for the paths were calculated. The observations are discussed in
the context of a simplified model of the coupling from the Siple antenna
into the ionosphere, which provides reasonable agreement with observations
	},
	keywords={
		magnetospheric electromagnetic wave propagation
		radiowave propagation
		whistlers
		VLF
		ELF
		radiowaves
		ducted signals
		whistler mode signals
		polarized VLF waves
		Siple transmitter
		magnetospheric propagation paths
		received signal strength
		transmitter antenna polarization
		growth
		emission triggering
		injected power levels
		L shell values
		equatorial number densities
		ionosphere
		2 to 4 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{TaranenkoJan92,
	author={Taranenko, Y.N. and Inan, U.S. and Bell, T.F.},
	title={
VLF-HF heating of the lower ionosphere and ELF wave generation
	},
	journal={Geophysical Research Letters},
	volume={19},
	number={1},
	year={1992},
	month={Jan},
	pages={61-4},
	abstract={
For incident wave power densities of 10/sup -6/-10/sup -2/ W/m/sup 2/ (at
30 km altitude), VLF heating of the D-region (<90 km) is found to be 2-10
times more effective (depending on power) than HF heating, resulting in
comparable perturbations of subionospheric VLF probe waves in spite of up
to 10/sup 3/ times larger power density utilized in HF heating and at least
as efficient in ELF wave generation. In view of generally larger (100*100
km) areas of the ionosphere illuminated by VLF transmitters, ELF wave
generation by modulated VLF heating is estimated to produce ELF power
levels of approximately 100 mW, comparable with or larger than those
produced in typical HF heating experiments. ELF wave generation in a
typical midlatitude ambient ionosphere occurs primarily via the modulation
of Pedersen current whereas in a typical auroral ionosphere Hall current is
dominant for pump wave frequencies up to approximately 6 MHz. For 10-30 MHz
and power densities >10/sup -4/ W/m/sup 2/, Pedersen current modulation is
again dominant, potentially providing up to 2-15 times higher ELF dipole
moment than those found in experiments using 3-5 MHz heaters
	},
	keywords={
		ionospheric electromagnetic wave propagation
		plasma radiofrequency heating
		radiowave propagation
		radiowave absorption
		lower ionosphere
		ELF wave generation
		power densities
		VLF heating
		D-region
		HF heating
		perturbations
		heating experiments
		Pedersen current
		auroral ionosphere Hall current
		pump wave frequencies
		modulation
		dipole moment
		30 to 150 km
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{RodriguezJan92,
	author={Rodriguez, J.V. and Inan, U.S. and Li, Y.Q. and Holzworth, R.H. and Smith, A.J. and Orville, R.E. and Rosenberg, T.J.},
	title={
A case study of lightning, whistlers, and associated ionospheric effects
during a substorm particle injection event
	},
	journal={Journal of Geophysical Research},
	volume={97},
	number={A1},
	year={1992},
	month={Jan},
	pages={65-75},
	abstract={
Simultaneous ground-based observations of narrowband and broadband VLF
radio waves and of cloud-to-ground lightning were made at widely spaced
locations during the 1987 Wave-Induced Particle Precipitation (WIPP)
campaign, conducted from Wallops Island, Virginia. Based on these
observations, the first case study has been made of the relationships among
located cloud-to-ground (CG) lightning flashes, whistlers, and associated
ionospheric effects during a substorm particle injection event. This event
took place two days after the strongest geomagnetic storm of 1987, during a
reintensification in geomagnetic activity (Kp=5) that did not affect the
high rate of whistlers observed at Faraday Station, Antarctica (L=2.46). At
the time of the injection event, several intense nighttime thunderstorms
were located over Long Island and the coast of New England, between 400 km
northwest and 600 km north of the region geomagnetically conjugate to
Faraday
	},
	keywords={
		atmospherics
		lightning
		magnetic storms
		whistlers
		cloud to ground flashes
		atmospherics
		United States
		lightning
		whistlers
		ionospheric effects
		substorm particle injection event
		VLF radio waves
		geomagnetic storm
		geomagnetic activity
		intense nighttime thunderstorms
		Long Island
		New England
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanApr91,
	author={Inan, U.S. and Bell, T.F. and Rodriguez, J.V.},
	title={
Heating and ionization of the lower ionosphere by lightning
	},
	journal={Geophysical Research Letters},
	volume={18},
	number={4},
	year={1991},
	month={Apr},
	pages={705-8},
	abstract={
Nighttime ionospheric electrons at 90-95 km altitude are heated by a factor
of 100-500 during the upward passage of short (<100 mu s) pulses of intense
(5-20 V/m at 100 km distance) electromagnetic radiation from lightning.
Heated electrons with average energy of 4-20 eV in turn produce secondary
ionization, of up to 400 cm/sup -3/ at approximately 95 km altitude in a
single ionization cycle ( approximately 3 mu s). With the time constant of
heating being 5-10 mu s, a number of such ionization cycles can occur
during a 50 mu s radiation pulse, leading to even higher density
enhancements. This effect can account for observations of 'early' or 'fast'
subionospheric VLF perturbations
	},
	keywords={
		atmospheric ionisation
		atmospheric radiation
		atmospheric temperature
		atmospheric thermodynamics
		D-region
		electron density
		ionosphere
		ionospheric electromagnetic wave propagation
		lightning
		nighttime ionospheric electrons heating
		aeronomy
		short intense EM radiation pulses
		ionosphere ionisation
		D-region ionisation
		hot electrons energy
		ionisation cycle time
		EM pulse duration
		ionosphere heating time constant
		fast VLF perturbations
		ionisation bubbles
		lower ionosphere
		lightning
		secondary ionization
		single ionization cycle
		density enhancements
		subionospheric VLF perturbations
		90 to 95 km
		3000 ns
		100 km
		5 to 10 mus
		50 mus
		4 to 20 eV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{DraganovJun91,
	author={Draganov, A.B. and Inan, U.S. and Taranenko, Y.N.},
	title={
ULF magnetic signatures at the Earth surface due to ground water flow: a
possible precursor to earthquakes
	},
	journal={Geophysical Research Letters},
	volume={18},
	number={6},
	year={1991},
	month={Jun},
	pages={1127-30},
	abstract={
Magnetic field fluctuations at the Earth's surface of Delta B/B
approximately 10/sup -5/ at <1 Hz are shown to result from motion with a
peak velocity of approximately 4 cm/s of ground water ( approximately 4
S/m) at approximately 5 km depth. Surface field changes can occur due to
either divergence free fluid motion with transverse spatial wavelengths of
a few tens of km, and/or homogeneous flow which displaces local
inhomogeneities in the Earth magnetic field
	},
	keywords={
		earthquakes
		groundwater
		seismology
		terrestrial electricity
		earthquake
		seismology
		groundwater
		magnetic field fluctuation
		ULF magnetic signatures
		Earth surface
		ground water flow
		precursor
		divergence free fluid motion
		0.01 to 0.5 Hz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BellMar91,
	author={Bell, T.F. and Inan, U.S. and Sonwalkar, V.S. and Helliwell, R.A.},
	title={
DE-1 observations of lower hybrid waves excited by VLF whistler mode waves
	},
	journal={Geophysical Research Letters},
	volume={18},
	number={3},
	year={1991},
	month={Mar},
	pages={393-6},
	abstract={
Recent satellite data show high amplitude lower hybrid (LH) waves excited
by electromagnetic (EM) whistler mode waves throughout magnetospheric
regions where small scale magnetic-field-aligned plasma density
irregularities exist. One important consequence in the auroral acceleration
region is the heating of suprathermal ions by the excited LH waves. To
evaluate such heating it is necessary to know the wavelength ( lambda )
range of the waves, information not previously available since most past
observations were made with long (l>or=75; l=antenna length) electric
dipole antennas which have very poor response for lambda <l. New
observations using the short 9 m electric dipole antenna on the DE-1
spacecraft are discussed
	},
	keywords={
		magnetosphere
		plasma
		whistlers
		AD 1989 01 02
		AD 1990 07 20
		plasma
		DE-1 observations
		lower hybrid waves
		VLF whistler mode waves
		magnetospheric regions
		small scale magnetic-field-aligned plasma density irregularities
		auroral acceleration region
		heating
		suprathermal ions
		wavelength
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{YipJan91,
	author={Yip, W.-Y. and Inan, U.S. and Orville, R.E.},
	title={
On the spatial relationship between lightning discharges and propagation
paths of perturbed subionospheric VLF/LF signals
	},
	journal={Journal of Geophysical Research},
	volume={96},
	number={A1},
	year={1991},
	month={Jan},
	pages={249-58},
	abstract={
A study has been made of the spatial relationship between propagation paths
of subionospheric VLF/LF signals exhibiting sudden amplitude perturbations
(Trimpi events) and time correlated cloud-to-ground lightning flashes. On
each of the 4 days examined the storm centers were located close to the
signal path from the NAU transmitter (28.5 kHz) in Puerto Rico to Stanford
(SU) and were at large distances from the propagation path of the 48.5-kHz
transmitter signal from Nebraska to SU
	},
	keywords={
		ionospheric electromagnetic wave propagation
		lightning
		radiowave propagation
		tropospheric electromagnetic wave propagation
		magnetospheric conditions
		spatial relationship
		lightning discharges
		propagation paths
		perturbed subionospheric VLF/LF signals
		sudden amplitude perturbations
		Trimpi events
		cloud-to-ground lightning flashes
		28.5 kHz
		48.5 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanJan91,
	author={Inan, U.S. and Bell, T.F.},
	title={
Pitch angle scattering of energetic particles by oblique whistler waves
	},
	journal={Geophysical Research Letters},
	volume={18},
	number={1},
	year={1991},
	month={Jan},
	pages={49-52},
	abstract={
First order cyclotron or Landau resonant pitch angle scattering of
electrons by oblique whistler waves propagating at large angles to the
ambient field are found to be at least as large as that due to parallel
propagating waves. Commonly observed precipitation of >40 keV electrons in
association with ducted whistlers may thus be accompanied by substantial
fluxes of lower energy (10 eV-40 keV) electrons precipitated by the
nonducted components
	},
	keywords={
		atmospheric electron precipitation
		magnetosphere
		radiation belts
		EM wave
		radiowave
		electron precipitation
		radiation belt
		loss process
		magnetosphere
		wave particle interaction
		first order cyclotron
		energetic particles
		oblique whistler waves
		Landau resonant pitch angle scattering
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{WolfDec90,
	author={Wolf, T.G. and Inan, U.S.},
	title={
Path-dependent properties of subionospheric VLF amplitude and phase
perturbations associated with lightning
	},
	journal={Journal of Geophysical Research},
	volume={95},
	number={A12},
	year={1990},
	month={Dec},
	pages={20997-10015},
	abstract={
A comprehensive study of lightning-associated amplitude and phase
perturbations on multiple VLF/LF signals (Trimpi events) observed at
Stanford, California and at Palmer Station, Antarctica, has revealed a
number of new properties that appear to be characteristic of the particular
signal paths. None of the existing models of the Trimpi effect are found to
explain all of the observed new features. Instead, the new experimental
findings provide an empirical framework to guide the evaluation of more
sophisticated models
	},
	keywords={
		ionospheric electromagnetic wave propagation
		lightning
		radiowave propagation
		subionospheric amplitude perturbations
		phase perturbations
		lightning
		multiple VLF/LF signals
		Trimpi events
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{JasnaOct90,
	author={Jasna, D. and Inan, U.S. and Bell, T.F.},
	title={
Equatorial gyroresonance between electrons and magnetospherically reflected
whistlers
	},
	journal={Geophysical Research Letters},
	volume={17},
	number={11},
	year={1990},
	month={Oct},
	pages={1865-8},
	abstract={
Magnetospherically reflected whistlers resonantly interact with energetic
(of order 100 keV) electrons in a relatively narrow energy range during
multiple equatorial crossings over a wide range of L-shells (1.5<L<4).
Results indicate that wave energy that enters the magnetosphere at a fixed
location can potentially contribute to the loss of particles over a wide
range of latitudes
	},
	keywords={
		atmospheric electron precipitation
		magnetospheric electromagnetic wave propagation
		radiowave propagation
		whistlers
		equatorial gyroresonance
		magnetosphere
		particle precipitation
		resonant interaction
		electrons
		whistlers
		wave energy
		loss of particles
		100 keV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SonwalkarOct90,
	author={Sonwalkar, V.S. and Helliwell, R.A. and Inan, U.S.},
	title={
Wideband VLF electromagnetic bursts observed on the DE 1 satellite
	},
	journal={Geophysical Research Letters},
	volume={17},
	number={11},
	year={1990},
	month={Oct},
	pages={1861-4},
	abstract={
Wideband VLF electromagnetic bursts are observed on the DE 1 satellite by
both the electric and magnetic field sensors in the frequency range of
0.650 kHz to 16.0 kHz. The impulsive signals endure for a relatively short
time ( approximately 1 s or less) and exist in the frequency range from
well below to well above the local gyrofrequency. They are typically found
at L>4 over a approximately 40 degrees range of latitudes including the
geomagnetic equator and are often accompanied by discrete emissions or a
band of hiss. Some observed features are consistent with previous
observations of electrostatic plasma waves (Ondoh et al., 1989; Reinleitner
et al., 1983); however, the magnetic measurements clearly indicate that the
impulsive signals are electromagnetic in nature. The possibility of
spacecraft discharge effects as the cause of these signals is discussed
	},
	keywords={
		artificial satellites
		atmospheric radiation
		magnetosphere
		AD 1985 01 to 1989 12
		magnetosphere
		wideband VLF EM bursts
		Dynamics Explorer 1
		DE 1 satellite
		discrete emissions
		hiss
		impulsive signals
		spacecraft discharge effects
		0.650 to 16.0 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanOct90,
	author={Inan, U.S. and Knifsend, F.A. and Oh, J.},
	title={
Subionospheric VLF 'imaging' of lightening-induced electron precipitation
from the magnetosphere
	},
	journal={Journal of Geophysical Research},
	volume={95},
	number={A10},
	year={1990},
	month={Oct},
	pages={17217-31},
	abstract={
High-resolution measurements of subionospheric VLF signals at multiple
sites are used as a new tool to assess the spatial distribution and
occurrence of ionospheric disturbances associated with lightning-induced
electron precipitation. Simultaneous observations in California,
Saskatchewan and Quebec of VLF signals from multiple sources allow the
monitoring of event activity over a coarse grid covering the continental
United States. Association of the observed VLF signal perturbations with
lightning is often made on the basis of time correlation with prominent
radio atmospherics. Simultaneous observations of individual events on
subionospheric paths that 'cross' one another are used to locate the
disturbed ionospheric region(s). Absence of perturbations on nearby paths
permits assessment of the spatial extent of the region with a varying
degree of accuracy, depending on the distribution of signal paths
	},
	keywords={
		atmospheric electron precipitation
		ionosphere
		magnetosphere
		subionospheric imaging
		lightening-induced electron precipitation
		magnetosphere
		spatial distribution
		occurrence
		ionospheric disturbances
		California
		Saskatchewan
		Quebec
		United States
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{GailSep90,
	author={Gail, W.B. and Inan, U.S. and Helliwell, R.A. and Carpenter, D.L.},
	title={
Gyroresonant wave-particle interactions in a dynamic magnetosphere
	},
	journal={Journal of Geophysical Research},
	volume={95},
	number={A9},
	year={1990},
	month={Sep},
	pages={15103-12},
	abstract={
Experimental and theoretical methods for studying gyroresonant
wave-particle interactions (WPI) in the magnetosphere commonly assume that
the magnetic field is static over the time scales of interest. In order to
investigate the effect of nonequilibrium or dynamic magnetospheric
processes in WPI, the response of the interaction mechanism to
time-dependent perturbations in the magnetic field was examined using the
global field compressions that occur during sudden commencements (sc). By
measuring modifications of the wave spectrum and electron distribution
during sc, the response of the WPI mechanism to slow variations in the
magnetic field and plasma environment can be determined. This technique was
used to examine the applicability of both nonlinear and quasi-linear
descriptions of gyroresonant WPI to dynamic environments
	},
	keywords={
		magnetosphere
		plasma
		nonequilibrium processes
		atmosphere
		dynamic magnetosphere
		gyroresonant wave-particle interactions
		magnetic field
		time-dependent perturbations
		global field compressions
		sudden commencements
		wave spectrum
		electron distribution
		plasma
		quasi-linear descriptions
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{CarlsonSep90,
	author={Carlson, C.R. and Helliwell, R.A. and Inan, U.S.},
	title={
Space-time evolution of whistler mode wave growth in the magnetosphere
	},
	journal={Journal of Geophysical Research},
	volume={95},
	number={A9},
	year={1990},
	month={Sep},
	pages={15073-89},
	abstract={
A new model is developed to simulate the space-time evolution of a
propagating coherent whistler mode wave pulse in the magnetosphere. The
model is applied to the case of single frequency (2-6 kHz) wave pulses
injected into the magnetosphere near L approximately=4, using the VLF
transmitting facility at Siple Station, Antarctica. The mechanism for
growth is cyclotron resonance between the circularly polarized waves and
the gyrating energetic electrons of the radiation belts
	},
	keywords={
		magnetospheric electromagnetic wave propagation
		radiowave propagation
		whistlers
		whistler mode wave growth
		magnetosphere
		space-time evolution
		VLF
		cyclotron resonance
		radiation belts
		2 to 6 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{JamesAug90,
	author={James, H.G. and Inan, U.S. and Rietveld, M.T.},
	title={
Observations on the DE 1 spacecraft of ELF/VLF waves generated by an
ionospheric heater
	},
	journal={Journal of Geophysical Research},
	volume={95},
	number={A8},
	year={1990},
	month={Aug},
	pages={12187-95},
	abstract={
Radio waves at frequencies between 1525 and 5925 Hz were observed on the DE
1 satellite during a pass over the Heating facility of the
Max-Planck-Institut fur Aeronomie (MPAe Heating) near Tromso, Norway. The
waves were detected during a 2-min period on December 12, 1981, and
measurements indicated pulse stretching by a few hundred milliseconds and
spectral broadening of about 10 Hz. Measured signal delays are compared
with those calculated using three-dimensional ray tracing. Scattering by
density irregularities may be responsible for the observed long delays and
spectral broadening
	},
	keywords={
		ionospheric electromagnetic wave propagation
		plasma radiofrequency heating
		radiowave propagation
		radiowave heating
		AD 1981 12 12
		MF
		ELF/VLF waves
		ionospheric heater
		DE 1 satellite
		MPAe Heating
		pulse stretching
		spectral broadening
		signal delays
		density irregularities
		1525 Hz
		5925 Hz
		2.759 MHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{RosenbergMay90,
	author={Rosenberg, T.J. and Wei, R. and Detrick, D.L. and Inan, U.S.},
	title={
Observations and modeling of wave-induced microburst electron precipitation
	},
	journal={Journal of Geophysical Research},
	volume={95},
	number={A5},
	year={1990},
	month={May},
	pages={6467-75},
	abstract={
Energy-time features of X-ray microbursts are examined and compared with
the predictions of a test particle simulation model of wave-induced
electron precipitation resulting from gyroresonant wave-particle
interactions in the magnetosphere. The observations were obtained on a
balloon flight at Siple station, Antarctica (L approximately=4.2) on
December 30, 1980. The energy and time evolution of the microbursts were
studied for X-rays in the energy range from 25 to 175 keV. The authors
identify the narrow microbursts with electrons which are precipitated
directly after undergoing pitch-angle scattering interactions with the wave
pulse; the wide microbursts are identified with electrons which, after
interacting with the wave, mirror in the conjugate ionosphere before
precipitating into the southern ionosphere. In general, the results provide
further support for the gyroresonant test particle simulation model, and
for the belief that the observed type of microbursts originates in the
vicinity of the magnetic equator in a gyroresonant process involving
discrete chorus emissions
	},
	keywords={
		atmospheric electron precipitation
		atmospheric radiation
		magnetosphere
		radiation belts
		AD 1980 12 30
		ionosphere
		radiation belt
		wave-induced microburst electron precipitation
		X-ray microbursts
		test particle simulation model
		gyroresonant wave-particle interactions
		magnetosphere
		pitch-angle scattering interactions
		25 to 175 keV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanMay90,
	author={Inan, U.S.},
	title={
VLF heating of the lower ionosphere
	},
	journal={Geophysical Research Letters},
	volume={17},
	number={6},
	year={1990},
	month={May},
	pages={729-32},
	abstract={
A controlled wave-injection experiment with a 28.5 kHz transmitter having a
radiated power of 100 kW has revealed evidence of ionospheric heating by
the VLF waves. Calculations indicate that the observed effect can be
attributed to the absorption of wave energy in the lower ionosphere, which
is estimated to result in a 30% enhancement in the collision frequency at
85 km. This process also represents a new means of direct coupling of
lightning energy to the lower ionosphere
	},
	keywords={
		atmospherics
		ionosphere
		lightning
		radiowave heating experiment
		atmospherics
		ionospheric modification
		VLF heating
		lower ionosphere
		wave-injection experiment
		absorption
		wave energy
		direct coupling
		lightning energy
		28.5 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{HelliwellApr90,
	author={Helliwell, R.A. and Mielke, T. and Inan, U.S.},
	title={
Rapid whistler-mode wave growth resulting from frequency-time curvature
	},
	journal={Geophysical Research Letters},
	volume={17},
	number={5},
	year={1990},
	month={Apr},
	pages={599-602},
	abstract={
The rapid (<50 ms) temporal growth of ducted whistlers is simulated using
controlled injection of VLF pulses from the Siple Station, Antarctica
transmitter. The results show that, when the frequency-time function of the
injected pulse has a positive slope and negative curvature, producing a
kind of 'chirp' such that it approximates the f(t) shape of a
lightning-generated whistler at frequencies above the 'nose' frequency,
growth up to a saturation level (20-30 dB) commonly occurs within <50 ms as
opposed to 200-300 ms that is required for monochromatic input signals. The
phenomenon is explained in terms of second-order-resonance theory
	},
	keywords={
		whistlers
		whistlers
		EM wave
		rapid growth
		whistler-mode wave growth
		frequency-time curvature
		ducted whistlers
		controlled injection
		VLF pulses
		Siple Station
		injected pulse
		second-order-resonance theory
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{GailJan90,
	author={Gail, W.B. and Inan, U.S.},
	title={
Characteristics of wave-particle interactions during sudden commencements.
2. Spacecraft observations
	},
	journal={Journal of Geophysical Research},
	volume={95},
	number={A1},
	year={1990},
	month={Jan},
	pages={139-47},
	abstract={
For pt.I see ibid., vol.95, no.A1, p.110-37 (1990). Wave data from the DE 1
spacecraft for 50 sudden commencements were analyzed for amplitude and
spectral modifications and correlated with data from ground-based
observatories. Changes in wave activity were identified in 14 of the events
studied. The changes, which were commonly observed at frequencies below the
local electron gyrofrequency, exhibited a complex structure both in
frequency and in time and varied considerably among events
	},
	keywords={
		magnetic storms
		magnetospheric electromagnetic wave propagation
		plasma
		radiowave propagation
		spacecraft observations
		magnetic storms
		magnetosphere
		plasma
		amplitude modification
		wave-particle interactions
		sudden commencements
		DE 1
		spectral modifications
		wave activity
		0.3 to 30 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{GailJan90,
	author={Gail, W.B. and Inan, U.S. and Helliwell, R.A. and Carpenter, D.L. and Krishnaswamy, S. and Rosenberg, T.J. and Lanzerotti, L.J.},
	title={
Characteristics of wave-particle interactions during sudden commencements.
1. Ground-based observations
	},
	journal={Journal of Geophysical Research},
	volume={95},
	number={A1},
	year={1990},
	month={Jan},
	pages={119-37},
	abstract={
ELF-VLF (0.3-30 kHz) wave data measured at ground-based observatories for
250 sudden commencements were analyzed for amplitude and spectral
modifications and correlated with magnetic field and precipitating particle
observations. Changes in ELF-VLF wave activity at high-latitude stations
were observed in 50-60% of the events studied and for approximately 80% of
the events when the observing station was on the dayside. Characteristic,
well-defined modifications of both coherent and incoherent ELF-VLF wave
emissions were observed
	},
	keywords={
		magnetic storms
		magnetospheric electromagnetic wave propagation
		plasma
		radiowave propagation
		ELF
		VLF
		ground based observation
		magnetosphere
		plasma
		magnetic storm
		amplitude modification
		wave-particle interactions
		sudden commencements
		spectral modifications
		magnetic field
		precipitating particle
		wave activity
		0.3 to 30 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BurgessMar90,
	author={Burgess, W.C. and Inan, U.S.},
	title={
Simultaneous disturbance of conjugate ionospheric regions in association
with individual lightning flashes
	},
	journal={Geophysical Research Letters},
	volume={17},
	number={3},
	year={1990},
	month={Mar},
	pages={259-62},
	abstract={
Characteristic whistler-associated amplitude perturbations of
subionospheric VLF or LF signals ('Trimpi events') observed within one
second of each other at Palmer Station, Antarctica and at Arecibo, Puerto
Rico suggest that ionospheric regions in both northern and southern
hemispheres are disturbed together in association with individual lightning
flashes. During a one hour period on March 21, 1989, the onsets of 44 out
of 47 perturbations measured on a 21.4 kHz signal from Maryland to Arecibo
occurred within 1 s of perturbation onsets measured on a 23.4 kHz signal
from Hawaii to Palmer Station. Similar activity occurred before and after
this period, and on the preceding and following days. The observations are
consistent with the disturbance of geomagnetically conjugate ionospheric
regions by multiple bounces between hemispheres of bursts of radiation belt
electrons, scattered in pitch angle by whistlers in the magnetosphere.
Analysis of patterns of perturbations with corresponding whistler and
lightning information from this period suggests that there were at least
two distinct ionospheric disturbances in each hemisphere
	},
	keywords={
		ionosphere
		whistlers
		ionosphere
		conjugate region
		Trimpi event
		AD 1989 03 21
		disturbance
		lightning flashes
		whistler-associated amplitude perturbations
		VLF
		LF
		Palmer Station
		Antarctica
		Arecibo
		Puerto Rico
		magnetosphere
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PoulsenMar90,
	author={Poulsen, W.L. and Bell, T.F. and Inan, U.S.},
	title={
Three-dimensional modeling of subionospheric VLF propagation in the
presence of localized D region perturbations associated with lightning
	},
	journal={Journal of Geophysical Research},
	volume={95},
	number={A3},
	year={1990},
	month={Mar},
	pages={2355-66},
	abstract={
A theoretical model of single-mode, subionospheric VLF wave propagation in
the presence of localized perturbations of the nighttime D region has been
developed. Values for changes in the amplitude and phase of a received
signal were obtained and compared with amplitude and phase measurements of
a VLF signal received at Palmer Station, Antarctica, from the NPM
transmitter (23.4 kHz) in Hawaii during energetic electron precipitation
events. Positive phase and/or negative amplitude shifts in the received
signal are produced by perturbations centered on the great circle (GC)
path, whereas both positive and negative amplitude (or phase) shifts in a
single-mode signal can be produced by perturbations lying in regions off
the GC path. The magnitude of the signal scattered by the perturbation
towards the receiver continuously decreases with distance away from the GC
path, becoming insignificant beyond approximately 20 lambda . On or near
the GC path, the magnitude of the scattered signal was proportional to the
scale of the perturbation parallel to the GC path
	},
	keywords={
		atmospheric electromagnetic wave propagation
		atmospheric electron precipitation
		atmospheric ionisation
		D-region
		ionospheric electromagnetic wave propagation
		plasma
		radiowave propagation
		upper atmosphere
		D-region lightning-induced perturbations
		night-time D-region
		single-mode VLF wave propagation
		received signal amplitude changes
		signal phase changes
		positive phase shifts
		negative phase shifts
		negative amplitude shifts
		scattered radio signal strength
		ionisation perturbation location
		perturbation scale size
		single waveguide mode theory
		subionospheric VLF propagation
		localized perturbations
		VLF signal
		Palmer Station
		Antarctica
		NPM transmitter
		Hawaii
		energetic electron precipitation events
		negative amplitude shifts
		single-mode signal
		23.4 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{ImhofAug89,
	author={Imhof, W.L. and Voss, H.D. and Mobilia, J. and Walt, M. and Inan, U.S. and Carpenter, D.L.},
	title={
Characteristics of short-duration electron precipitation bursts and their
relationship with VLF wave activity
	},
	journal={Journal of Geophysical Research},
	volume={94},
	number={A8},
	year={1989},
	month={Aug},
	pages={10079-93},
	abstract={
Energetic (>6 keV) electron data from the SEEP payload on the low altitude
( approximately 200 km) polar orbiting S81-1 satellite indicate a high rate
of occurrence of short duration (<0.6 s) electron precipitation bursts.
Characteristics of events observed at night (2230 MLT) versus daytime (1030
MLT) and at midlatitudes (2<L<3) versus higher latitudes (L>3) were
distinctly different in several ways. Comparison of the electron data with
simultaneous VLF wave data from Palmer (L approximately=2.4) and Siple (L
approximately=4.3) stations in Antarctica indicated a varying degree of
association of electron bursts with whistlers and chorus emissions. Several
of the electron bursts observed at nighttime and at 2<L<3 were correlated
with lightning-generated whistlers observed at Palmer Station. When daytime
bursts at higher latitudes (L>3) were observed on satellite passes within
+or-50 degrees of the Siple meridian, chorus was invariably detected at
Siple, but correlation of electron bursts with individual chorus spectral
elements was not evident
	},
	keywords={
		atmospheric electron precipitation
		whistlers
		radiowave emission
		magnetosphere
		ionosphere
		short-duration electron precipitation bursts
		VLF wave activity
		whistlers
		chorus
		lightning-generated
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SonwalkarJun89,
	author={Sonwalkar, V.S. and Inan, U.S.},
	title={
Lightning as an embryonic source of VLF hiss
	},
	journal={Journal of Geophysical Research},
	volume={94},
	number={A6},
	year={1989},
	month={Jun},
	pages={6986-94},
	abstract={
Data from the DE 1 satellite show that lightning-generated whistlers often
trigger hiss emissions that endure for up to 10- and 20-s periods. The data
consist of the measured electric and magnetic fields in the frequency range
of 1.5 kHz to 6.0 kHz, during 22 DE 1 passes during the period December 28,
1986 to January 18, 1987. The 22 passes covered L shells of 3.4 to 5.1 and
geomagnetic latitude of 20 degrees N to 40 degrees S in the afternoon (
approximately 1400-1500 MLT) sector. The whistler-triggered hiss emissions
were observed on 16 of the passes, and they generally exhibited the
following characteristics: emission spectra were wide band (1-2 kHz) and
rather structureless; and well-defined and sustained fading patterns were
observed at twice the spin frequency over 10- to 20-s periods. These
results indicate that lightning-generated whistlers may be an important
embryonic source for magnetospheric hiss and that whistlers and emissions
triggered by them often constitute the dominant wave activity in the
approximately 1.5- to 6-kHz range during geomagnetically quiet periods
	},
	keywords={
		atmospheric electron precipitation
		atmospheric proton precipitation
		atmospheric spectra
		atmospherics
		lightning
		magnetosphere
		radiation belts
		wideband structureless emission spectra
		ELF
		magnetosphere electric fields
		L-shells 3.4 to 5.1
		afternoon sector
		wave normal angle
		trapped electrons loss
		ring current protons precipitation
		AD 1986 12 28 to 1987 01 18
		VLF hiss
		DE 1 satellite
		lightning-generated whistlers
		hiss emissions
		magnetic fields
		DE 1 passes
		December 28, 1986 to January 18, 1987
		geomagnetic latitude
		whistler-triggered hiss emissions
		sustained fading patterns
		spin frequency
		embryonic source
		magnetospheric hiss
		dominant wave activity
		geomagnetically quiet periods
		1.5 to 6.0 kHz
		3.4 to 5.1 Earthradii
		0.5 to 50 keV
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanFeb89,
	author={Inan, U.S. and Walt, M. and Voss, H.D. and Imhof, W.L.},
	title={
Energy spectra and pitch angle distributions of lightning-induced electron
precipitation: analysis of an event observed on the S81-1 (SEEP) satellite
	},
	journal={Journal of Geophysical Research},
	volume={94},
	number={A2},
	year={1989},
	month={Feb},
	pages={1379-401},
	abstract={
Temporal and spectral signatures of a lightning-induced electron
precipitation (LEP) burst observed on the S81-1 (SEEP) satellite are
analyzed and compared with the predictions of a test particle model of the
gyroresonant whistler-particle interaction in the magnetosphere. The flux
to be detected by specific detectors on the low altitude ( approximately
220 km) satellite at L approximately=2.24 is calculated in terms of the
integral counting rate as a function of time and in terms of the dynamic
energy spectra during the initial approximately 300-ms precipitation pulse.
For a whistler wave packet with frequency range 500 Hz to 6 kHz the dynamic
energy spectra are found to depend sensitively on the electron angular
distribution in the vicinity of the loss cone. In the case of a whistler
wave originating in northern hemisphere lightning the maximum
whistler-induced pitch angle scattering of electrons occurs near
approximately 10 degrees S geomagnetic latitude
	},
	keywords={
		atmospheric electron precipitation
		ionosphere
		magnetosphere
		ionosphere
		wave particle interaction
		pitch angle distributions
		lightning-induced electron precipitation
		burst
		test particle model
		gyroresonant whistler-particle interaction
		magnetosphere
		whistler wave
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{GurnettMay88,
	author={Gurnett, D.A. and Inan, U.S.},
	title={
Plasma wave observations with the Dynamics Explorer 1 spacecraft
	},
	journal={Reviews of Geophysics},
	volume={26},
	number={2},
	year={1988},
	month={May},
	pages={285-316},
	abstract={
Reviews the results from the plasma wave instrument on the Dynamics
Explorer 1 (DE 1) spacecraft. The DE 1 spacecraft was launched on August 3,
1981, into an elliptical polar orbit with initial perigee and apogee radial
distances of 1.09 and 4.65 R/sub E/. In the roughly 6 years since the
launch of the spacecraft, DE 1 has provided basic new information on a wide
variety of magnetospheric plasma wave phenomena. These include auroral
kilometric radiation, auroral hiss, Z mode radiation, narrow-band
electromagnetic emissions associated with equatorial upper hybrid waves,
whistler mode emissions, wave-particle interactions stimulated by ground
VLF transmitters, equatorial ion cyclotron emissions, ion Bernstein mode
emissions, and electric field turbulence along the auroral field lines. The
authors first give a brief review of the basic plasma wave modes that can
exist in the equatorial and polar regions of the magnetosphere. After the
basic terminology is established, each of the above areas of plasma wave
research is discussed in detail
	},
	keywords={
		magnetosphere
		reviews
		AD 1981 to 1987
		DE satellite
		plasma wave
		ionosphere
		magnetosphere
		EM wave
		radiowave emissions
		Dynamics Explorer 1
		auroral kilometric radiation
		auroral hiss
		Z mode radiation
		narrow-band electromagnetic emissions
		equatorial upper hybrid waves
		whistler mode emissions
		wave-particle interactions
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanOct88,
	author={Inan, U.S. and Shafer, D.C. and Yip, W.Y. and Orville, R.E.},
	title={
Subionospheric VLF signatures of nighttime D region perturbations in the
vicinity of lightning discharges
	},
	journal={Journal of Geophysical Research},
	volume={93},
	number={A10},
	year={1988},
	month={Oct},
	pages={11455-72},
	abstract={
A 12-hour sequence of perturbations of subionospheric VLF signals observed
in association with lightning provided preliminary evidence that the
ionospheric regions perturbed in these events may be confined to within
approximately 150 km of the lightning discharges, and that intracloud
flashes as well as cloud-to-ground lightning may be important in producing
the perturbations. High-resolution analysis of event signatures indicated
the presence of two different classes of events. For one set of events,
observed during the most active central 6 hours of the observation period,
a approximately 0.6-s delay between the causative lightning and VLF event
onset and a approximately 1-s onset duration was observed, consistent with
previously suggested models of the gyroresonant whistler-particle
interaction that leads to particle precipitation and perturbation of the
Earth-ionosphere waveguide. However, another set of events, observed during
the first 2 hours of the observation period, exhibited a very different
temporal signature, characterized by a much smaller (<50 ms) delay and
sometimes also very short (<50 ms) rise times
	},
	keywords={
		atmospheric radiation
		D-region
		lightning
		whistlers
		night
		radiowave emission
		D-region
		ionosphere perturbation
		AD 1987 03
		nighttime
		lightning discharges
		subionospheric VLF signals
		gyroresonant whistler-particle interaction
		particle precipitation
		Earth-ionosphere waveguide
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanSep88,
	author={Inan, U.S. and Wolf, T.G. and Carpenter, D.L.},
	title={
Geographic distribution of lightning-induced electron precipitation
observed as VLF/LF perturbation events
	},
	journal={Journal of Geophysical Research},
	volume={93},
	number={A9},
	year={1988},
	month={Sep},
	pages={9841-53},
	abstract={
Expected occurrence characteristics of lightning-induced electron
precipitation (LEP) events at longitudes of the western (110 degrees W)
versus eastern (71 degrees W) United States are considered from the point
of view of available trapped particle flux at the edge of the loss cone.
Considering published data on nighttime fluxes of >68 keV electrons
observed at L approximately=2.5, and for 'direct' precipitation into the
northern hemisphere induced by northern hemisphere lightning, the
occurrence rate and flux levels are expected to be a factor of 20-200
higher in the west than in the east, assuming no significant variation in
lightning source activity with longitude. Again assuming lightning sources
in the north, it is predicted that at 71 degrees W, 'mirrored'
precipitation into the southern hemisphere would involve precipitation
fluxes 30-300 times higher than 'direct' precipitation into the northern
hemisphere. However, at 110 degrees W and again assuming lightning in the
north, southern hemisphere precipitation would tend to be limited to that
small fraction of particles that were initially scattered into the northern
loss cone and that were then backscattered from the northern atmosphere so
as to reach the south
	},
	keywords={
		atmospheric electron precipitation
		ionosphere
		magnetosphere
		atmospherics
		LEP
		ionosphere
		magnetosphere
		lightning-induced electron precipitation
		United States
		available trapped particle flux
		occurrence rate
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SonwalkarJul88,
	author={Sonwalkar, V.S. and Inan, U.S.},
	title={
Wave normal direction and spectral properties of whistler mode hiss
observed on the DE 1 satellite
	},
	journal={Journal of Geophysical Research},
	volume={93},
	number={A7},
	year={1988},
	month={Jul},
	pages={7493-514},
	abstract={
A new study of magnetospheric hiss as a spatially and temporally enduring
phenomenon is undertaken using a recently developed formalism that allows
the representation of hiss by a field distribution function (FDF). This
formalism explicitly takes into account the whistler mode relationships and
the linear and spin motion of the satellite, so that on a spin-stabilized
satellite, it becomes possible to measure the wave propagation direction(s)
from the observed fading patterns in the received electromagnetic field
data. The authors have analyzed hiss signals received by electric and
magnetic field antennae aboard the DE 1 satellite during a approximately
3-hour period on September 23, 1983. A band of hiss at frequencies <2 kHz
was observed continuously from 0236 UT t0 0539 UT over a range of
geomagnetic latitudes from lambda /sub m/=45 degrees N to lambda /sub m/=20
degrees S and L shells of L=4.3 to L=5.3. Electron density deduced from in
situ and remote measurements indicate that during this time the DE 1
satellite was near the boundary of the plasmasphere. The observations are
summarized
	},
	keywords={
		atmospheric radiation
		magnetosphere
		whistlers
		radiowave emission
		wave normal direction
		magnetosphere
		ELF
		AD 1983 09 23
		VLF
		spectral properties
		whistler mode hiss
		magnetospheric hiss
		field distribution function
		formalism
		wave propagation direction
		boundary
		plasmasphere
		1 to 4 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanFeb88,
	author={Inan, U.S. and Burgess, W.C. and Wolf, T.G. and Shafer, D.C. and Orville, R.E.},
	title={
Lightning-associated precipitation of MeV electrons from the inner
radiation belt
	},
	journal={Geophysical Research Letters},
	volume={15},
	number={2},
	year={1988},
	month={Feb},
	pages={172-5},
	abstract={
Transient perturbations of subionospheric very low frequency radiowave
signals provide new evidence for lightning-induced electron precipitation
events involving (<1 s) bursts of >1 MeV electrons from the Earth's inner
radiation belt at L<or=1.8. The signal amplitude changes are attributed to
increased absorption in the Earth-ionosphere waveguide and/or alterations
of the waveguide mode structure due to localized secondary ionization
enhancements produced in the nighttime lower ionosphere and the mesosphere
by the precipitating electrons. The otherwise stably trapped electrons are
believed to be scattered in pitch angle during cyclotron resonant
interactions in the magnetosphere with the lightning-generated whistler
waves. That some precipitation bursts consist partly of MeV electrons is
suggested by confinement of the perturbed subionospheric signal path to low
magnetic latitudes (L<or=1.8), and the temporal signatures of the
perturbation events, which often exhibit an unusually rapid initial
recovery followed by further recovery at rates believed characteristic of
less energetic events ( tau approximately 5-20 s)
	},
	keywords={
		atmospheric electromagnetic wave propagation
		atmospheric electron precipitation
		atmospheric ionisation
		ionospheric electromagnetic wave propagation
		lightning
		magnetosphere
		mesosphere
		radiation belts
		whistlers
		short electron bursts
		VLF signals transient perturbations
		EM wave absorption
		gyroresonant electron energies
		pitch angle scattering
		AD 1987 03 to 05
		USA
		wave-particle interactions
		S United States
		Gulf Coast excess ionisation effective loss rate
		altitude dependence
		MeV electrons
		inner radiation belt
		subionospheric very low frequency radiowave signals
		lightning-induced electron precipitation
		signal amplitude changes
		increased absorption
		Earth-ionosphere waveguide
		waveguide mode structure
		localized secondary ionization enhancements
		nighttime lower ionosphere
		mesosphere
		precipitating electrons
		stably trapped electrons
		cyclotron resonant interactions
		magnetosphere
		lightning-generated whistler waves
		perturbed subionospheric signal path
		low magnetic latitudes
		temporal signatures
		perturbation events
		rapid initial recovery
		0.2 to 6.0 kHz
		28.5 kHz
		0 to 1 s
		1.8 Earthradii
		5 to 20 s
		1.0 MeV
		40 to 70 km
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{PoulsenMar88,
	author={Poulsen, W.L. and Inan, U.S.},
	title={
Satellite observations of a new type of discrete VLF emission at L<4
	},
	journal={Journal of Geophysical Research},
	volume={93},
	number={A3},
	year={1988},
	month={Mar},
	pages={1817-38},
	abstract={
A new type of discrete whistler mode emission has been observed in the
magnetosphere at L<4. The emission elements are confined to a bandwidth of
1-5 kHz, with the lower cutoff frequency of the band varying with L shell,
being equal to approximately 0.2-0.5 f/sub Heq/, where f/sub Heq/ is the
equatorial electron gyrofrequency. The discrete and burstlike nature of the
emissions is similar to that of chorus emissions typically observed at
higher L; however, dispersion of individual elements is often different
from typical chorus, and the emissions are observed inside as well as
outside the plasmapause. The phenomenon seems to occur mainly in the early
morning local time sector and is well correlated with geomagnetic activity,
occurring mostly when Sigma Kp>30. The emissions may be generated near the
equatorial plane at frequencies of approximately 0.2 F/sub Heq/ inside and
approximately 0.35 f/sub Heq/ outside the plasmapause. The parallel energy
of electrons for gyroresonance with the observed waves is found to be
approximately 20-50 keV in both cases
	},
	keywords={
		atmospherics
		dispersion (wave)
		ionospheric electromagnetic wave propagation
		magnetic storms
		magnetosphere
		magnetospheric electromagnetic wave propagation
		whistlers
		emission elements bandwidth
		K/sub p/-index
		plasmasphere
		burstlike emissions
		emission elements dispersion
		equatorial whistlers source
		ISIS-2 satellite
		gyroresonant electrons parallel energy
		ionospheric reflections
		discrete VLF emission
		discrete whistler mode emission
		magnetosphere
		lower cutoff frequency
		equatorial electron gyrofrequency
		chorus emissions
		plasmapause
		early morning local time sector
		geomagnetic activity
		equatorial plane
		1 to 5 kHz
		5 to 25 kHz
		2 to 4 Earthradii
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{FishmanFeb88,
	author={Fishman, G.J. and Inan, U.S.},
	title={
Observation of an ionospheric disturbance caused by a gamma-ray burst
	},
	journal={Nature},
	volume={331},
	number={6155},
	year={1988},
	month={Feb},
	pages={418-209},
	abstract={
Reports a first observation of an ionospheric disturbance from a gamma-ray
burst. The burst, GB 830801, occurred at 22:14:18 UT on 1 August 1983 and
was one of the strongest ever observed. The total fluence was 2*10/sup -3/
erg cm/sup -2/, most of which occurred in the first 4 s of the burst.
Simultaneously, a change was observed in the amplitude of a
very-low-frequency (VLF) radio signal from a transmitter in Rugby, England,
monitored at Palmer Station, Antarctica, indicative of an ionospheric
disturbance. Weaker disturbances were also recorded at the same time
receiving site on signals from VLF stations in Annapolis, Maryland and
Lualualei, Hawaii. The times of the burst and the disturbances are
coincident within the 10-s resolution of the VLF recording system. No
similar disturbances were observed within 60 h around the time of the
burst. In the future, a network of VLF burst monitors may provide
measurements of the total ionizing energy fluence from a burst, as well as
some limited directional information
	},
	keywords={
		atmospheric ionisation
		gamma-ray sources (astronomical)
		ionosphere
		X-ray sources
		atmospheric ionisation
		ionospheric disturbance
		gamma-ray burst
		GB 830801
		1 August 1983
		total fluence
		VLF
		times
		resolution
		total ionizing energy fluence
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanApr87,
	author={Inan, U.S.},
	title={
Waves and instabilities
	},
	journal={Reviews of Geophysics},
	volume={25},
	number={3},
	year={1987},
	month={Apr},
	pages={588-98},
	abstract={
This review concentrates on US research activities in the area of waves and
instabilities during the mid-1982 to mid-1986 period. Plasma waves and
instabilities are phenomena that are central to the energization,
acceleration, transport, and loss of energetic particles in magnetized
plasmas. As such, they play a dominant role in almost all energy exchange
phenomena that occur in planetary magnetospheres. The US research can be
somewhat arbitrarily divided into the following six categories: (1)
whistler mode wave-electron interactions, (2) wave-induced particle
precipitation, (3) ULF wave phenomena, (4) ion-mode waves and
instabilities, (5) auroral kilometric radiation, (6) ionospheric
irregularities and instabilities, and (7) waves and instabilities in the
outer magnetosphere
	},
	keywords={
		ionosphere
		magnetosphere
		reviews
		plasma wave
		magnetosphere
		plasma stability
		whistler mode wave-electron interactions
		wave-induced particle precipitation
		ULF wave phenomena
		ionospheric
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{CarpenterApr87,
	author={Carpenter, D.L. and Inan, U.S.},
	title={
Seasonal, latitudinal and diurnal distributions of whistler-induced
electron precipitation events
	},
	journal={Journal of Geophysical Research},
	volume={92},
	number={A4},
	year={1987},
	month={Apr},
	pages={3429-35},
	abstract={
The seasonal, latitudinal, and diurnal distributions of whistler-induced
electron precipitation events, detected as subionospheric signal
perturbations (Trimpi events), have been studied by means of data sets
acquired in 1982-3 at Palmer and Siple stations, Antarctica. The authors
also compare simultaneous records from L approximately 2.4 and L
approximately 4.3, and find evidence of an inner magnetospheric maximum in
burst precipitation activity for E>40 keV in the range L approximately 2-3,
consistent with theoretical predictions
	},
	keywords={
		atmospheric electron precipitation
		whistlers
		AD 1982 to 1983
		VLF
		seasonal variation
		latitudinal variation
		diurnal distributions
		whistler-induced electron precipitation events
		subionospheric signal perturbations
		Trimpi events
		Palmer
		Siple
		Antarctica
		inner magnetospheric maximum
		burst precipitation activity
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanApr87,
	author={Inan, U.S. and Carpenter, D.L.},
	title={
Lightning-induced electron precipitation events observed at L approximately
2.4 as phase and amplitude perturbations on subionospheric VLF signals
	},
	journal={Journal of Geophysical Research},
	volume={92},
	number={A4},
	year={1987},
	month={Apr},
	pages={3293-303},
	abstract={
Lightning-induced electron precipitation (LEP) events are studied using the
Trimpi effect, in which the precipitation-induced ionization enhancements
in the lower ionosphere (D region) give rise to rapid perturbations of
subionospheric VLF signals. In 1983, the phase and amplitude of signals
from the NPM transmitter in Hawaii (23.4 kHz) and the Omega transmitter in
Argentina (12.9 kHz) were measured at Palmer, Antarctica (L approximately
2.4), together with the magnetospheric whistler background. The long
baseline and over-sea great circle paths from these two sources make it
possible for the observed perturbations to be interpreted using a single
waveguide mode theory. Analytical expressions are used to relate the
magnitude of the phase perturbations to differential changes in ionospheric
reflection height along a segment of the propagation path. The predicted
relationship between relative perturbation sizes on the two different
signals is compared with measurements. From this information, the
whistler-induced flux levels are inferred to be in the 10/sup -4/-10/sup
-2/ erg cm/sup -2/ s/sup -1/ range and the precipitation regions are
inferred to be roughly 'circular' in shape, rather than elongated along L
shells
	},
	keywords={
		atmospheric electron precipitation
		ionospheric electromagnetic wave propagation
		AD 1983
		phase perturbation
		radiowave propagation
		lightning induced
		ionosphere
		D-region
		electron precipitation events
		amplitude perturbations
		subionospheric VLF signals
		Trimpi effect
		precipitation-induced ionization enhancements
		lower ionosphere
		whistler
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{HurrenAug86,
	author={Hurren, P.J. and Smith, A.J. and Carpenter, D.L. and Inan, U.S.},
	title={
Burst precipitation induced perturbations on multiple VLF propagation paths
in Antarctica
	},
	journal={Annales Geophysicae, Series A (Upper Atmosphere and Space Sciences)},
	volume={4},
	number={4},
	year={1986},
	month={Aug},
	pages={311-18},
	abstract={
The burst precipitation of energetic (E>40 keV) electrons near L=4 has been
detected as amplitude perturbations (Trimpi events) on subionospheric 3.79
kHz CW signals from the Siple (L=4.2) VLF transmitter that were observed at
Halley (L/sup -/=4.3), Palmer (L=2.3) and South Pole ( Lambda =74 degrees )
Antarctic stations. The observations were made on the dayside of the Earth
but beneath a locally dark ionosphere during a generally disturbed 6 d
period in July 1982 when the plasmapause projection was equatorward of the
Siple-Halley and Siple-South Pole paths
	},
	keywords={
		atmospheric electron precipitation
		ionospheric electromagnetic wave propagation
		radiowave propagation
		ionosphere
		radiowave
		energetic electrons
		AD 1982 07 12 to 17
		multiple VLF propagation paths
		Antarctica
		burst precipitation
		amplitude
		Trimpi events
		CW signals
		Siple
		Halley
		Palmer
		South Pole
		plasmapause projection
		3.79 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanJan87,
	author={Inan, U.S.},
	title={
Gyroresonant pitch angle scattering by coherent and incoherent whistler
mode waves in the magnetosphere
	},
	journal={Journal of Geophysical Research},
	volume={92},
	number={A1},
	year={1987},
	month={Jan},
	pages={127-42},
	abstract={
A test particle approach is used to compare gyroresonant pitch angle
scattering of energetic electrons by coherent versus incoherent whistler
mode waves, for the case in which the coherent wave amplitude is below the
nonlinear phase trapping threshold. Wave packets of 400 ms duration
propagating along the magnetic field at L=4 within the plasmasphere are
considered, and the wave-induced pitch angle scattering along the
propagation path from one hemisphere to the other and the resulting
precipitation flux are computed. An incoherent wave spectrum is simulated
by random modulation of the wave frequency at intervals of 1 ms, thereby
generating signals with nearly constant power spectral density over a
bandwidth of 2 kHz centered at 5.5 kHz. The associated pitch angle
scattering is compared with that of a monochromatic 5.5 kHz signal of 400
ms duration. Results of the test particle analysis are compared with those
expected on the basis of a classical diffusion treatment
	},
	keywords={
		atmospheric elementary particle precipitation
		magnetospheric electromagnetic wave propagation
		plasma
		radiation belts
		whistlers
		EM wave
		atmosphere
		VLF
		radiation belt
		plasma
		incoherent whistler mode waves
		magnetosphere
		test particle approach
		gyroresonant pitch angle scattering
		energetic electrons
		coherent wave amplitude
		nonlinear phase trapping threshold
		magnetic field
		plasmasphere
		precipitation flux
		wave spectrum
		random modulation
		wave frequency
		power spectral density
		classical diffusion treatment
		5.5 kHz
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{TolstoyDec86,
	author={Tolstoy, A. and Rosenberg, T.J. and Inan, U.S. and Carpenter, D.L.},
	title={
Model predictions of subionospheric VLF signal perturbations resulting from
localized, electron precipitation-induced ionization enhancement regions
	},
	journal={Journal of Geophysical Research},
	volume={91},
	number={A12},
	year={1986},
	month={Dec},
	pages={13473-82},
	abstract={
Whistler-induced precipitation of energetic electrons produces transient
ionospheric conductivity variations that perturb the amplitude and phase of
VLF signals propagating in the Earth-ionosphere waveguide. This study uses
a waveguide mode theoretic propagation model to predict the effect of
localized ionization enhancement (IE) regions on nighttime long-path VLF
signals from the US Navy navigational transmitters NSS, NAA, NLK and NPM to
Antarctic receiving stations. The predictions are then compared with the
observed signal behavior in Trimpi events from which inferences can be
drawn about an IE region's approximate characteristics. The study also
examines the effects of transmitter-induced electron precipitation on the
VLF signals
	},
	keywords={
		atmospheric electricity
		atmospheric electron precipitation
		atmospheric ionisation
		ionosphere
		ionospheric electromagnetic wave propagation
		radiowave propagation
		D-region
		whistlers
		atmosphere
		radiowave
		subionospheric VLF signal perturbations
		electron precipitation-induced ionization enhancement regions
		transient ionospheric conductivity variations
		amplitude
		phase
		Earth-ionosphere waveguide
		propagation
		nighttime
		US Navy navigational transmitters
		Antarctic receiving stations
		Trimpi events
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanApr86,
	author={Inan, U.S.},
	title={
Jovian VLF chorus and Io torus aurora
	},
	journal={Journal of Geophysical Research},
	volume={91},
	number={A4},
	year={1986},
	month={Apr},
	pages={4543-50},
	abstract={
A test particle model of the cyclotron resonance interaction of waves and
trapped radiation belt particles is used to estimate the energetic electron
fluxes precipitated by Jovian VLF chorus waves observed on the Voyager 1
and 2 spacecraft near the Io torus. The precipitation fluxes induced by
1-s-long chorus wave packets at L approximately=7.6 and 8.6 are estimated
to be bursts of approximately 5 s duration with a peak of 0.3-3 and 0.7-7
ergs/cm/sup 2/ s that consist of electrons of approximately 5-100 keV
energy and that arrives at the ionosphere approximately 15 s after the
generation of the chorus wave at the equatorial plane. The effects in the
Jovian ionosphere of the chorus-induced precipitation are estimated using
existing ionospheric models
	},
	keywords={
		Jupiter
		planetary atmospheres
		planetary satellite atmospheres
		Jupiter
		planetary atmosphere
		radiowave emission
		plasma torus
		magnetosphere
		electron precipitation
		VLF chorus
		Io torus aurora
		test particle model
		cyclotron resonance interaction
		radiation belt
		energetic electron fluxes
		ionosphere
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{HelliwellApr86,
	author={Helliwell, R.A. and Carpenter, D.L. and Inan, U.S. and Katsufrakis, J.P.},
	title={
Generation of band-limited VLF noise using the Siple transmitter: a model
for magnetospheric hiss
	},
	journal={Journal of Geophysical Research},
	volume={91},
	number={A4},
	year={1986},
	month={Apr},
	pages={4381-92},
	abstract={
Band-limited VLF noise generated by the experimental transmitter at Siple
Station, Antarctica, is used to simulate the interaction of natural
magnetospheric hiss with energetic radiation belt particles. While the
observed spectrum of the generated noise at times closely resembles that of
natural VLF hiss, at other times discrete emissions are found to be
generated from the incoherent noise signal. Results imply that
magnetospheric chorus can be triggered by hiss signals, indicating the
similarity of generation mechanisms for coherent and incoherent VLF
emissions. A model based on second-order cyclotron resonance can explain
the conversion of the relatively short duration wavelets of a hiss spectrum
into the longer, semicoherent discrete emissions that are typical of chorus
	},
	keywords={
		magnetosphere
		radiowave emission
		generation
		wave particle interaction
		band-limited VLF noise
		model
		magnetospheric hiss
		interaction
		natural
		radiation belt particles
		discrete emissions
		chorus
		generation mechanisms
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanMar86,
	author={Inan, U.S. and Carpenter, D.L.},
	title={
On the correlation of whistlers and associated subionospheric VLF/LF
perturbations
	},
	journal={Journal of Geophysical Research},
	volume={91},
	number={A3},
	year={1986},
	month={Mar},
	pages={3106-16},
	abstract={
Several periods of whistler-associated subionospheric signal perturbations
(i.e. Trimpi events) observed at Palmer, Antarctica (L approximately 2.4)
have been studied. In a case study of the time signature of the signal
perturbations during a 10-min recording period on March 30, 1983, the time
delay between the whistler-producing spheric and the onset of the change
was found to be in the range 0.52-0.62 s, independent of the amplitude of
the change. Event amplitude, as expected from previous work, was found to
be well correlated with the associated whistler wave intensity. Other
temporal features such as the rise and decay times of the perturbations
were also found to be independent of the event amplitude. These results are
consistent with a recent theoretical model of gyroresonant particle
scattering interaction in the magnetosphere
	},
	keywords={
		magnetosphere
		magnetospheric electromagnetic wave propagation
		whistlers
		associated subionospheric perturbations
		VLF
		LF
		magnetosphere
		AD 1983 03 Trimpi event
		correlation
		whistlers
		spheric
		onset
		gyroresonant particle scattering interaction
		magnetosphere
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SonwalkarJan86,
	author={Sonwalkar, V.S. and Inan, U.S.},
	title={
Measurements of Siple transmitter signals on the DE 1 satellite: wave
normal direction and antenna effective length
	},
	journal={Journal of Geophysical Research},
	volume={91},
	number={A1},
	year={1986},
	month={Jan},
	pages={154-64},
	abstract={
A new experimental technique is developed to simultaneously measure the
wave propagation direction and the effective length of a small (L<< lambda
) electric dipole antenna on a spin stabilized satellite in the
magnetosphere. The technique relies on the near simultaneous measurement of
single components of the electric and magnetic fields of a coherent VLF
signal injected into the medium from a ground-based source. The spin fading
characteristics of the signal received by the electric dipole and the
magnetic loop antenna permit the measurement of the wave normal direction.
Measurements of the local cold plasma density are used to determine the
refractive index. The wave electric field is then inferred from the wave
magnetic field as measured on the loop antenna, the refractive index and
the direction of propagation. Comparing this electric field with the
measured voltage across the dipole antenna leads to the effective length of
the receiving electric dipole
	},
	keywords={
		artificial satellites
		atmospheric electricity
		atmospheric techniques
		geomagnetism
		magnetosphere
		magnetospheric electromagnetic wave propagation
		whistlers
		VLF whistler mode signals
		small dipole antenna
		magnetosphere EM wave propagation
		HZ 4025
		signal electric fields components
		AD 1982 07 28
		dipole antenna voltage
		magnetospheric technique
		Earth radii 004.5 to 005.5
		Siple transmitter signals
		DE 1 satellite
		wave normal direction
		antenna effective length
		wave propagation direction
		electric dipole antenna
		spin stabilized satellite
		near simultaneous measurement
		single components
		magnetic fields
		coherent VLF signal
		ground-based source
		spin fading characteristics
		magnetic loop antenna
		local cold plasma density
		refractive index
		wave electric field
		wave magnetic field
		receiving electric dipole
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{HelliwellJan86,
	author={Helliwell, R.A. and Inan, U.S. and Katsufrakis, J.P. and Carpenter, D.L.},
	title={
Beat excitation of whistler mode sidebands using the Siple VLF transmitter
	},
	journal={Journal of Geophysical Research},
	volume={91},
	number={A1},
	year={1986},
	month={Jan},
	pages={143-53},
	abstract={
The process of whistler mode sideband generation in the magnetosphere is
studied by transmitting two monochromatic signals closely spaced in
frequency ( Delta f=5-45 Hz) from the experimental VLF transmitter at Siple
Station, Antarctica. The signals were observed following ducted
magnetospheric propagation to the conjugate station at Roberval, Quebec.
Sidebands up to seventh order were generated extending to +or-100 Hz with
respect to the average frequency of the carriers. New frequencies were
observed both under conditions of little or no growth of the input signals
and when one of the input signals did grow significantly. A small signal
mechanism is proposed in which emissions are triggered by each beat between
the input waves but are then suppressed by the following beat. The energy
from the phase bunched particles is believed to feed preferentially into
the sidebands. The observed process of sideband generation provides a
mechanism to break down the coherence of relatively narrowband waves in the
magnetosphere and may account for the transformation of relatively coherent
wave packets into broader more variable bands of noiselike signals
	},
	keywords={
		atmospherics
		magnetosphere
		magnetospheric electromagnetic wave propagation
		whistlers
		whistler sidebands beat excitation
		ELF atmospherics
		magnetosphere EM wave propagation
		two-frequency signal
		seventh-order sidebands
		carriers average frequency
		input signals growth rate
		phase bunched particles energy
		VLF emissions triggering
		Hz 2200 to 3800
		AD 1983 06 30
		AD 1983 07 11
		Siple VLF transmitter
		whistler mode sideband generation
		monochromatic signals
		Siple Station
		Antarctica
		ducted magnetospheric propagation
		conjugate station
		Roberval
		Quebec
		small signal mechanism
		relatively coherent wave packets
		noiselike signals
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{DejnakarintraDec85,
	author={Dejnakarintra, M. and Inan, U.S. and Carpenter, D.L.},
	title={
Transient tropospheric electric fields resulting from sudden changes in
ionospheric conductivity
	},
	journal={Journal of Geophysical Research},
	volume={90},
	number={A12},
	year={1985},
	month={Dec},
	pages={12271-81},
	abstract={
The transient electric fields that would be generated by sudden changes in
the atmospheric conductivity profile are estimated using a theoretical
model. The model assumes the existence of a horizontal electric field with
a spatial extent of >or=20-km at 150-km altitude and involves the solution
of the boundary value problem in two dimensions. The geomagnetic field
lines below 150-km altitude are assumed to be vertical, but the anisotropy
of the medium above approximately 70-km altitude is fully accounted for.
The computed electric field strength depends sensitively on the size of the
source field as well as the conductivity profile of the atmosphere. During
a transient the peak electric fields produced in the case of a small-scale
source field can be considerably larger than those due to large-scale
source distributions
	},
	keywords={
		atmospheric electricity
		troposphere
		troposphere
		transient electric field
		atmosphere
		electrical conductivity
		sudden changes
		ionospheric conductivity
		theoretical model
		horizontal electric field
		boundary value problem
		source field
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanAug85,
	author={Inan, U.S. and Carpenter, D.L. and Helliwell, R.A. and Katsufrakis, J.P.},
	title={
Subionosphere VLF/LF phase perturbations produced by lightning-whistler
induced particle precipitation
	},
	journal={Journal of Geophysical Research},
	volume={90},
	number={A8},
	year={1985},
	month={Aug},
	pages={7457-69},
	abstract={
New evidence of phase perturbations of subionospheric VLF/LF signals,
produced by lightning-whistler-induced precipitation of bursts of radiation
belt electrons, is reported. Phase changes of 0.1-1.0 mu s on a 12.9-kHz
signal arriving at Palmer, Antarctica (L approximately 2.4), over a
approximately 2400-km path are regularly observed with a characteristic
signature of a rapid (<or=1 s) onset followed by a relatively slow (10-30
s) recovery. Event occurrence peaks during equinoctial periods, with
typical rates of 1-40 events per hour lasting for several hours per night.
The observed phase perturbations are interpreted
	},
	keywords={
		atmospheric electron precipitation
		ionospheric electromagnetic wave propagation
		radiation belts
		radiowave propagation
		whistlers
		ionospheric
		atmosphere
		VLF
		LF
		radiowave propagation
		phase perturbations
		lightning-whistler induced particle precipitation
		subionospheric VLF/LF signals
		radiation belt electrons
		Palmer
		Antarctica
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{ChangJul85,
	author={Chang, H.C. and Inan, U.S.},
	title={
Test particle modeling of wave-induced energetic electron precipitation
	},
	journal={Journal of Geophysical Research},
	volume={90},
	number={A7},
	year={1985},
	month={Jul},
	pages={6409-18},
	abstract={
A test particle computer model of the precipitation of radiation belt
electrons is extended to compute the dynamic energy spectrum of transient
electron fluxes induced by short-duration VLF wave packets travelling along
the geomagnetic field lines. The model is adapted to estimate the count
rate and associated spectrum of precipitated electrons that would be
observed by satellite based particle detectors with given geometric factor
and orientation with respect to the magnetic field. A constant-frequency
wave pulse and a lightning-induced whistler wave packet are used as
examples of the stimulating wave signals
	},
	keywords={
		atmospheric electron precipitation
		magnetosphere
		radiation belts
		test particle model
		magnetosphere
		EM wave
		wave particle interaction
		wave-induced energetic electron precipitation
		radiation belt electrons
		dynamic energy spectrum
		transient electron fluxes
		short-duration VLF
		geomagnetic field lines
		constant-frequency wave pulse
		whistler
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{ImhofMay85,
	author={Imhof, W.L. and Gaines, E.E. and Voss, H.D. and Reagan, J.B. and Datlowe, D.W. and Mobilia, J. and Helliwell, R.A. and Inan, U.S. and Katsufrakis, J. and Joiner, R.G.},
	title={
Results from the SEEP active space plasma experiment: effects on the
ionosphere
	},
	journal={Radio Sci. (USA), Radio Science},
	volume={20},
	number={3},
	year={1985},
	month={May},
	pages={511-18},
	abstract={
An active satellite-ground coordinated space plasma experiment was
conducted from May to December, 1982, in which electrons were precipitated
from the radiation belts into the ionosphere by the controlled injection of
VLF signals from ground-based transmitters. The results confirm the
hypothesis that electrons can be precipitated from the radiation belts by
ground-based VLF transmitters, and they provide information relating to the
effects of such precipitation on the ionosphere
	},
	keywords={
		atmospheric electron precipitation
		ionospheric electromagnetic wave propagation
		radiation belts
		radiowave propagation
		AD 1982 05 to 12
		electron precipitation
		SEEP active space plasma experiment
		ionosphere
		May to December, 1982
		radiation belts
		VLF signals
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{RastaniMay85,
	author={Rastani, K. and Inan, U.S. and Helliwell, R.A.},
	title={
DE 1 observations of Siple transmitter signals and associated sidebands
	},
	journal={Journal of Geophysical Research},
	volume={90},
	number={A5},
	year={1985},
	month={May},
	pages={4128-40},
	abstract={
VLF signals from the Siple Station, Antarctica, transmitter received on the
DE 1 spacecraft provide new information on the whistler mode signal
propagation paths in the magnetosphere. In two case studies, the measured
group delay in conjunction with in situ density measurements and ray
tracing analysis are used to distinguish between direct nonducted
propagation and a hybrid mode consisting of one-hop propagation in a duct
followed after ionospheric reflection by nonducted propagation. The extent
of the observations both in space and time indicates that such a hybrid
propagation mode may be an important means by which whistler mode signals
generated or amplified in ducts can populate the magnetosphere
	},
	keywords={
		ionospheric electromagnetic wave propagation
		magnetospheric electromagnetic wave propagation
		radiowave propagation
		whistlers
		EM wave
		DE 1
		Siple transmitter signals
		sidebands
		VLF signals
		Antarctica
		whistler mode signal propagation paths
		magnetosphere
		group delay
		density
		ray tracing
		direct nonducted propagation
		hybrid mode
		one-hop propagation
		ionospheric reflection
		nonducted propagation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{CarpenterMay85,
	author={Carpenter, D.L. and Inan, U.S. and Paschal, E.W. and Smith, A.J.},
	title={
A new VLF method for studying burst precipitation near the plasmapause
	},
	journal={Journal of Geophysical Research},
	volume={90},
	number={A5},
	year={1985},
	month={May},
	pages={4383-8},
	abstract={
VLF signals in the 2-4 kHz range transmitted from Siple Station, Antarctica
(L approximately 4.3), and received at various Antarctic locations have
been used to detect the occurrence of burst precipitation of electrons
(E>or=50 keV) into the nighttime lower ionosphere. The receiving stations,
each approximately 1400 km from Siple, were located to the north at Palmer
(L approximately 2.3), to the east at Halley (L approximately 4.3), and to
the south at South Pole ( Lambda approximately 74 degrees ). Rapid changes
in the received phase and amplitude of the Siple signal ('Trimpi events')
were observed in conjunction with the reception of one-hop whistlers. Phase
measurements appear to be a particularly sensitive means of detecting burst
precipitation activity under experimental conditions of the kind described.
The length and spatial distribution of the signal paths provide a basis for
studying the occurrence and approximate location of burst precipitation in
regions outside the observing range of most instruments used for detection
of precipitation
	},
	keywords={
		atmospheric electron precipitation
		ionospheric techniques
		electron precipitation
		measurement
		technique
		ionosphere
		VLF method
		burst precipitation
		plasmapause
		occurrence
		nighttime lower ionosphere
		phase
		occurrence
		approximate location
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanJan85,
	author={Inan, U.S. and Chang, H.C. and Helliwell, R.A. and Imhof, W.L. and Reagan, J.B. and Walt, M.},
	title={
Precipitation of radiation belt electrons by man-made waves: a comparison
between theory and measurement
	},
	journal={Journal of Geophysical Research},
	volume={90},
	number={A1},
	year={1985},
	month={Jan},
	pages={359-69},
	abstract={
The temporal and spectral shape and the absolute flux level of particle
pulses precipitated by a VLF transmitter are examined from a theoretical
point of view. A test-particle model of the gyroresonant wave-particle
interactions is applied to the parameters of the observed cases for
calculating the precipitation characteristics. The temporal shapes of the
precipitation pulses are found to be controlled (1) by the pitch angle
dependence of the particle distribution near the edge of the loss cone and
(2) by the multiple interaction of the particles with the waves due to
significant atmospheric backscatter
	},
	keywords={
		atmospheric electron precipitation
		magnetosphere
		radiation belts
		radiowave propagation
		magnetosphere
		electron precipitation
		artificial
		modification experiment
		transmitter induced
		radiation belt electrons
		man-made waves
		theory
		VLF
		test-particle model
		gyroresonant wave-particle interactions
		precipitation pulses
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SmithJan85,
	author={Smith, A.J. and Carpenter, D.L. and Inan, U.S.},
	title={
Whistler-triggered VLF noise bursts observed on the DE-1 satellite and
simultaneously at Antarctic ground stations
	},
	journal={Annales Geophysicae},
	volume={3},
	number={1},
	year={1985},
	month={Jan},
	pages={81-8},
	abstract={
Whistler-triggered bursts of very low frequency chorus in the 5-7 kHz
range, occurring quasi-periodically every 3-5 min, have previously been
observed at ground stations under conditions of relatively deep quieting
following moderate magnetic disturbance. It was found that these wave
bursts propagate outside the plasmapause and that they can induce
detectable electron precipitation at ionospheric D-region altitudes. This
paper reports simultaneous observations of such wave events on the ground
at Antarctic stations Halley and Siple (L=4.3) and on the high altitude
satellite DE-1
	},
	keywords={
		atmospherics
		magnetosphere
		whistlers
		whistler-triggering
		chorus
		kHz 0005 to 0007
		ducted propagation
		VLF noise bursts
		DE-1 satellite
		Antarctic ground stations
		electron precipitation
		ionospheric D-region
		Halley
		Siple
		high altitude satellite
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanFeb85,
	author={Inan, U.S. and Bell, T.F.},
	title={
Spectral broadening of VLF transmitter signals observed on DE 1: a
quasi-electrostatic phenomenon?
	},
	journal={Journal of Geophysical Research},
	volume={90},
	number={A2},
	year={1985},
	month={Feb},
	pages={1771-5},
	abstract={
Spectrally broadened VLF transmitter signals are observed on the DE 1
satellite using alternatively both electric and magnetic field sensors. It
is found that at times when the electric field component undergoes
significant bandwidth expansion (up to approximately 110 Hz) the magnetic
field component has a bandwidth of less than 10 Hz. The results support the
theory that the off-carrier components are quasi-electrostatic in nature.
Measurement of the absolute E and B field magnitudes of the broadened
signals are used to determine the wave Poynting vector
	},
	keywords={
		ionospheric electromagnetic wave propagation
		radiowave propagation
		radiowave propagation
		quasielectrostatic
		ionosphere
		spectral broadening
		offcarrier
		transionospheric
		VLF transmitter signals
		theory
		off-carrier
		wave Poynting vector
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{ChangFeb85,
	author={Chang, H.C. and Inan, U.S.},
	title={
Lightning-induced electron precipitation from the magnetosphere
	},
	journal={Journal of Geophysical Research},
	volume={90},
	number={A2},
	year={1985},
	month={Feb},
	pages={1531-41},
	abstract={
Precipitation of radiation belt particles induced by whistlers that are
generated by atmospheric lightning discharges and propagate over L shells
of 2-4.5 is considered. Using a test particle model of the
whistler-particle interaction, the energy spectra and temporal profile of
whistler-induced fluxes as a function of L shell are quantitatively
determined for representative plasmaspheric cold plasma distribution.
Results indicate that for higher energy electron precipitation (E>40 keV)
there exists an inner magnetospheric region (2<L<3) where the level of
whistler-induced precipitation can be expected to be comparatively high
	},
	keywords={
		atmospheric electron precipitation
		magnetosphere
		radiation belts
		whistlers
		lightning induced
		EM wave
		wave particle interaction
		trapped particle
		radiowave
		energy distribution
		electron precipitation
		magnetosphere
		radiation belt
		whistlers
		test particle model
		whistler-particle interaction
		temporal profile
		L shell
		plasmaspheric cold plasma distribution
		inner magnetospheric
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{CarpenterNov84,
	author={Carpenter, D.L. and Inan, U.S. and Trimpi, M.L. and Helliwell, R.A. and Katsufrakis, J.P.},
	title={
Perturbations of subionospheric LF and MF signals due to whistler-induced
electron precipitation bursts
	},
	journal={Journal of Geophysical Research},
	volume={89},
	number={A11},
	year={1984},
	month={Nov},
	pages={9857-62},
	abstract={
First evidence of whistler-induced burst precipitation effects on
subionospherically propagating signals in the LF and MF ranges have been
observed at Palmer (L approximately 2.4) and Siple stations (L
approximately 4.3), Antarctica. The occurrence rate on a 37.2-kHz LF signal
originating in California was usually comparable to that on the more
disturbed VLF paths. At Palmer, examples at 37.2 kHz were seen on 70% of
the nights during a March-April 1983 observing period. Perturbations on a
approximately 1800 km-long 780-kHz MF path to Palmer occurred on nights of
high activity on VLF paths, but fewer than 10 MF events were usually
detected as compared to >50 on the active VLF paths. The MF perturbations
were of order 50% in amplitude and were not in general followed by a
approximately 30-s decay toward a pre-event level, as is usually the case
for the VLF signals
	},
	keywords={
		atmospheric electron precipitation
		ionospheric electromagnetic wave propagation
		radiowave propagation
		whistlers
		LF
		radiowave propagation
		ionosphere
		subionospheric
		MF
		whistler-induced electron precipitation bursts
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{TkalcevicDec84,
	author={Tkalcevic, S. and Inan, U.S. and Helliwell, R.A.},
	title={
Nonlinear pitch angle scattering and trapping of energetic particles during
Landau resonance interactions with whistler mode waves
	},
	journal={Journal of Geophysical Research},
	volume={89},
	number={A12},
	year={1984},
	month={Dec},
	pages={10813-26},
	abstract={
The time averaged equations of motivation derived by Inan and Tkalcevic
(1982) are used in a test particle study of Landau resonant interactions of
whistler mode waves and energetic particles in the magnetosphere. By
computing individual particle trajectories it is shown that the pitch angle
scattering and energy exchange is significantly different for the two
classes of particles, trapped and untrapped. The trapped particles are
characterized by a bounded phase variation, whereas the nontrapped
particles exhibit unbounded phase variation. The threshold wave electric
field intensities necessary for trapping are determined. Full distribution
test particle simulation is carried out to determine the precipitated
electron flux that would be induced as a result of these interactions
	},
	keywords={
		atmospheric electron precipitation
		magnetosphere
		whistlers
		nonlinear
		trapped particle
		EM wave
		wave particle interaction
		pitch angle scattering
		trapping
		energetic particles
		Landau resonance interactions
		whistler mode waves
		equations of motivation
		energy exchange
		untrapped
		nontrapped
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{VossDec84,
	author={Voss, H.D. and Imhof, W.L. and Walt, M. and Mobilia, J. and Gaines, E.E. and Reagan, J.B. and Inan, U.S. and Helliwell, R.A. and Carpenter, D.L. and Katsufrakis, J.P. and Chang, H.C.},
	title={
Lightning-induced electron precipitation
	},
	journal={Nature},
	volume={312},
	number={5996},
	year={1984},
	month={Dec},
	pages={740-2},
	abstract={
The authors report the first satellite measurements of electron
precipitation induced by lightning. The measured energy deposition of these
conspicuous lightning-induced electron precipitation (LEP) bursts (
approximately 10/sup -3/ erg cm/sup -2/) is sufficient to deplete the
Earth's radiation belts and to alter subionospheric radiowave propagation
(<or approximately=1 MHz). A one-to-one correlation is found between
ground-based measurements of VLF spherics and whistlers at Palmer,
Antarctica, and low-altitude satellite (S81-1) measurements of
precipitating energetic electrons
	},
	keywords={
		atmospheric electron precipitation
		lightning
		magnetosphere
		radiation belts
		lightning induced
		ionosphere
		VLF
		spherics
		atmospherics
		radiowave emission
		magnetosphere
		whistler
		precipitation burst
		electron precipitation
		radiation belts
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{LeyserOct84,
	author={Leyser, T.B. and Inan, U.S. and Carpenter, D.L. and Trimpi, M.L.},
	title={
Diurnal variation of burst precipitation effects on subionospheric VLF/LF
signal propagation near L=2
	},
	journal={Journal of Geophysical Research},
	volume={89},
	number={A10},
	year={1984},
	month={Oct},
	pages={9139-43},
	abstract={
Burst precipitation effects on subionospheric VLF/LF signal propagation are
studied using data recorded at Palmer Station, Antarctica (L approximately
2.4) between March 3 and April 7, 1983. Relatively abrupt signal amplitude
changes known as 'Trimpi' effects were observed in conjunction with
magnetospheric whistlers, which are inferred to induce electron
precipitation that in turn causes enhanced ionization at the 80 to 90-km
altitude level. Earlier findings that Trimpi effects occur predominantly
under nighttime ionospheric conditions were confirmed by comparing the
sunrise-sunset terminator position with perturbation activity on three
VLF/LF signal paths for which the arrival bearings range from magnetic
north to west. Events were found to occur on 70% of the observing nights.
Signal paths making larger angles with the terminator were used to deduce
that most events were caused by ionospheric effects occurring within
approximately 1000 km of Palmer Station
	},
	keywords={
		atmospheric electromagnetic wave propagation
		atmospheric electron precipitation
		atmospheric ionisation
		ionosphere
		ionospheric electromagnetic wave propagation
		upper atmosphere
		whistlers
		ionospheric disturbances
		upper atmosphere
		atmospheric EM wave propagation
		equinox
		electron precipitation events
		altitude km 0080 to 0090
		ionospheric events distance
		AD 1983 03 03 to 04 07
		kHz 0013 to 0780
		precipitation effects diurnal variation
		burst precipitation effects
		subionospheric VLF/LF signal propagation
		Palmer Station
		Antarctica
		signal amplitude changes
		magnetospheric whistlers
		enhanced ionization
		80 to 90-km altitude level
		Trimpi effects
		nighttime ionospheric conditions
		sunrise-sunset terminator position
		perturbation activity
		VLF/LF signal paths
		arrival bearings
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanMar84,
	author={Inan, U.S. and Pon, M. and Banks, P.M. and Williamson, P.R. and Raitt, W.J. and Shawhan, S.D.},
	title={
Modulated beam injection from the Space Shuttle during magnetic
conjunctions of STS 3 and the DE 1 satellite
	},
	journal={Radio Science},
	volume={19},
	number={2},
	year={1984},
	month={Mar},
	pages={487-95},
	abstract={
An electron beam emitted from the Office of Space Sciences 1 pallet on STS
3 was pulsed with specially designed very low frequency (VLF) formats in an
attempt to generate whistler mode waves. Modulated operations of the beam
emitted by a fast pulse electron generator (FPEG) were initiated during
times of magnetic conjunctions between STS 3 and the high-altitude DE 1
satellite equipped with broadband VLF receivers. Coordinated FPEG/VLF
modulation and DE 1 wide-band data acquisition were achieved in 12
different cases. No evidence of any waves generated by FPEG were detected
on the DE 1 analog wideband data. Reasons are discussed
	},
	keywords={
		electron beam effects
		ionosphere
		plasma
		plasma-beam interactions
		space vehicles
		whistlers
		modulated beam injection
		plasma beam interaction
		Space Shuttle
		magnetic conjunctions
		STS 3
		DE 1 satellite
		whistler mode waves
		fast pulse electron generator
		VLF
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{SonwalkarMay84,
	author={Sonwalkar, V.S. and Bell, T.F. and Helliwell, R.A. and Inan, U.S.},
	title={
Direct multiple path magnetospheric propagation: a fundamental property of
nonducted VLF waves
	},
	journal={Journal of Geophysical Research},
	volume={89},
	number={A5},
	year={1984},
	month={May},
	pages={2823-30},
	abstract={
ISEE 1 satellite observations of nonducted whistler mode signals from the
Siple Station VLF transmitter show that all well-defined pulses are
elongated by 20 ms to 200 ms. This elongation is attributed to closely
spaced multiple paths of propagation between the ground and the satellite.
The results are illustrated by two cases: one on October 29, 1977, inside
the plasmapause and the other on May 7, 1979, outside the plasmapause. The
results establish that, in general, at any point in the magnetosphere the
direct signals transmitted from the ground arrive almost simultaneously
along two or more closely spaced direct ray paths. It is shown that
multiple paths can be explained by assuming field-aligned irregularities of
1 to 10-km horizontal scale in the ionosphere with a few percent
enhancement or depletion in the plasma density
	},
	keywords={
		atmospheric ionisation
		ionosphere
		ionospheric electromagnetic wave propagation
		magnetospheric electromagnetic wave propagation
		plasma
		whistlers
		direct multiple path magnetospheric propagation
		pulse elongation
		EM wave propagation
		atmospheric ionisation
		AD 1977 10 29
		plasma density irregularities characteristic size
		AD 1979 05 07 wave-particle interactions
		cyclotron resonant electron
		wave Doppler broadening
		nonducted VLF waves
		ISEE 1 satellite observations
		whistler mode signals
		Siple Station VLF transmitter
		closely spaced multiple paths
		October 29, 1977
		plasmapause
		May 7, 1979
		direct ray paths
		field-aligned irregularities
		horizontal scale
		ionosphere
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanMay84,
	author={Inan, U.S. and Chang, H.C. and Helliwell, R.A.},
	title={
Electron precipitation zones around major ground-based VLF signal sources
	},
	journal={Journal of Geophysical Research},
	volume={89},
	number={A5},
	year={1984},
	month={May},
	pages={2891-906},
	abstract={
The spatial distribution of electron precipitation induced by VLF signals
from ground-based transmitters is determined by using a test particle
computer model of the gyroresonant wave-particle interaction (Inan et al.,
1982). The results are presented as contours of energy flux on a map of the
region around each transmitter. It is shown that the size of the
precipitation zones is a strong function of the geographic location of the
transmitter, as well as its radiated power and operating frequency. In
general, the precipitation zones are much wider in longitude than in
latitude and are oriented along lines of constant geomagnetic latitude.
Assuming backscatter and/or wave echoing, precipitation zones around the
points that are magnetically conjugate to the sources are also estimated.
The results presented can be used to interpret satellite- or ground-based
measurements of the precipitation induced by ground-based VLF transmitters
	},
	keywords={
		atmospheric electron precipitation
		ionosphere
		magnetosphere
		magnetospheric electromagnetic wave propagation
		radiation belts
		whistlers
		geomagnetic parallels
		precipitation zones dimensions
		magnetically conjugate precipitation zones
		magnetosphere EM wave propagation
		whistler mode waves
		induced precipitation
		energy flux contours
		radiation belts particle losses
		ground-based VLF signal sources
		spatial distribution
		electron precipitation
		ground-based transmitters
		test particle computer model
		gyroresonant wave-particle interaction
		geographic location
		radiated power
		operating frequency
		constant geomagnetic latitude
		backscatter
		wave echoing
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{ChangDec83,
	author={Chang, H.C. and Inan, U.S.},
	title={
A theoretical model study of observed correlations between whistler mode
waves and energetic electron precipitation event in the magnetosphere
	},
	journal={Journal of Geophysical Research},
	volume={88},
	number={A12},
	year={1983},
	month={Dec},
	pages={10053-64},
	abstract={
A recently extended test particle computer model of the gyroresonance
wave-particle interaction in the magnetosphere is applied to previously
reported cases of observed correlations between whistler mode waves and
ionospheric responses to particle precipitation. Three different
ionospheric effects, namely X-ray bursts, photoemissions, and D region
perturbations, all correlated with VLF waves and believed to be caused by
precipitated particles, are considered. The precipitation flux level, the
pulse shape, and the associated time delays are computed for the parameters
relevant to each case and are compared with values deduced from the data.
The results demonstrate that the existing theoretical model can be useful
for interpreting experimental results of this kind
	},
	keywords={
		atmospheric electron precipitation
		magnetosphere
		whistlers
		EM wave
		trapped particle
		wave particle interaction
		ionosphere
		theoretical model
		correlations
		whistler mode waves
		energetic electron precipitation event
		magnetosphere
		gyroresonance
		VLF waves
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{ChangSep83,
	author={Chang, H.C. and Inan, U.S. and Bell, T.F.},
	title={
Energetic electron precipitation due to gyroresonant interactions in the
magnetosphere involving coherent VLF waves with slowly varying frequency
	},
	journal={Journal of Geophysical Research},
	volume={88},
	number={A9},
	year={1983},
	month={Sep},
	pages={7037-50},
	abstract={
A test particle simulation model (Inan et al., 1982) of the gyroresonance
wave-particle interaction in the magnetosphere is extended to study the
transient particle precipitation fluxes induced by various coherent VLF
waves with slowly varying frequency propagating along the Earth's magnetic
field lines. For moderate wave intensities (B/sub omega /<or=10 pT at L=4)
a comparison between input signals with linearly rising and falling
frequencies shows that they induce the same amount of precipitated particle
energy deposition. However, when the wave growth near the principal
interaction region is considered, the precipitation induced by a riser is
considerably higher than that induced by a faller
	},
	keywords={
		atmospheric electron precipitation
		magnetosphere
		ionosphere
		wave particle interaction
		pitch angle scattering
		electron precipitation
		gyroresonant interactions
		magnetosphere
		coherent VLF waves
		test particle simulation model
		gyroresonance
		transient particle precipitation
		slowly varying frequency
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{Imhof83,
	author={Imhof, W.L. and Reagen, J.B. and Voss, H.D. and Gaines, E.E. and Datlowe, D.W. and Mobilia, J. and Helliwell, R.A. and Inan, U.S. and Katsufrakis, J. and Joiner, R.G.},
	title={
The modulated precipitation of radiation belt electrons by controlled
signals from VLF transmitters
	},
	journal={Geophys. Res. Lett. (USA), Geophysical Research Letters},
	volume={10},
	number={8},
	year={1983},
	month={},
	pages={615-18},
	abstract={
Reports the detection of the precipitation of radiation belt electrons by
the controlled injection of signals from the US Navy VLF transmitters at
Cutler, Maine (NAA) or at Annapolis, Maryland (NSS) modulated in a 3s ON/2s
OFF format. During each of these events the fluxes of precipitating
electrons were observed repeatedly to display a characteristic time
behavior with respect to the transmitter modulation: a relatively slow rate
of increase after start of the ON period leading to a maximum about 2
seconds later. Details of this consistent pattern and the statistics of
occurrence of modulation events are presented along with comparisons of the
absolute fluxes of precipitating electrons observed during normal
transmitter operation with those recorded when one of the transmitters was
modulated
	},
	keywords={
		atmospheric electron precipitation
		magnetospheric electromagnetic wave propagation
		radiation belts
		radiowave propagation
		SEEP
		Stimulated Emission of Energetic Particles
		modulated precipitation
		radiation belt electrons
		VLF transmitters
		Cutler, Maine
		Annapolis, Maryland
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanAug83,
	author={Inan, U.S. and Helliwell, R.A. and Kurth, W.S.},
	title={
Terrestrial versus Jovian VLF chorus; a comparative study
	},
	journal={Journal of Geophysical Research},
	volume={88},
	number={A8},
	year={1983},
	month={Aug},
	pages={6171-80},
	abstract={
The relevant parameters of the magnetospheres of Jupiter and Earth are
studied from the point of view of wave-particle resonant interactions that
are believed to be responsible for the generation of VLF chorus emissions
observed on Voyager-1. Using existing models of the cold and energetic
plasma distributions in the Jovian magnetosphere, expressions for the
wave-particle interaction length (L/sub I/) and the nonlinearity parameter
( rho ) are derived. Values of these parameters are compared with those
computed for the Earth's magnetosphere. It is found that the typical
interaction lengths are at least 2-5 times larger in the Jovian than in the
terrestrial magnetosphere. Also, the wave intensity necessary to reach the
threshold of nonlinearity in the Jovian magnetosphere was found to be up to
5-100 times lower
	},
	keywords={
		Jupiter
		magnetosphere
		planetary atmospheres
		radioastronomy
		Earth
		Jupiter
		planet
		radiowave emission
		wave particle interaction
		chorus burst
		growth rate
		VLF chorus
		resonant interactions
		generation
		magnetosphere
		wave-particle interaction length
		nonlinearity parameter
		threshold
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{ImhofApr83,
	author={Imhof, W.L. and Reagan, J.B. and Vos, H.D. and Gaines, E.E. and Datlowe, D.W. and Mobilia, J. and Helliwell, R.A. and Inan, U.S. and Katsufrakis, J. and Joiner, R.G.},
	title={
Direct observation of radiation belt electrons precipitated by the
controlled injection of VLF signals from a ground-based transmitter
	},
	journal={Geophysical Research Letters},
	volume={10},
	number={4},
	year={1983},
	month={Apr},
	pages={361-4},
	abstract={
Radiation belt electrons precipitated by controlled injection of VLF
signals from a ground based transmitter have been directly observed for the
first time. These observations were part of the SEEP (Stimulated Emission
of Energetic Particles) experiment conducted during May-December 1982. Key
elements of SEEP were the controlled modulation of VLF transmitters and a
sensitive low altitude satellite payload to detect the precipitation. An
outstanding example of time-correlated wave and particle data occurred from
8680 to 8740 seconds UT on 17 August 1982 when the satellite passed near
the VLF transmitter at Cutler, Maine, as it was being modulated with a
repeated ON (3-s)/OFF (2-s) pattern. The measured energy spectra revealed
that approximately 15 to 50 percent of the enhanced electron flux was
concentrated near the resonant energies for first order cyclotron
interactions occurring close to the magnetic equator with the nearly
monochromatic waves emitted from the transmitter
	},
	keywords={
		atmospheric electron precipitation
		ionosphere
		magnetosphere
		magnetospheric electromagnetic wave propagation
		radiation belts
		ionosphere
		electron precipitation
		direct bounce loss cone
		VLF
		radiowave excitation
		magnetosphere
		propagation
		AD 1982
		EM wave particle interaction
		trapped particle motion
		radiation belt electrons
		SEEP
		Stimulated Emission of Energetic Particles
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BellJun83,
	author={Bell, T.F. and James, H.G. and Inan, U.S. and Katsufrakis, J.P.},
	title={
The apparent spectral broadening of VLF transmitter signals during
transionospheric propagation
	},
	journal={Journal of Geophysical Research},
	volume={88},
	number={A6},
	year={1983},
	month={Jun},
	pages={4813-40},
	abstract={
VLF/ELF electric field wave data acquired on the ISIS 1, ISIS 2, and ISEE 1
satellites demonstrate the existence of a new phenomenon in which initially
narrowband ( approximately 1 Hz) upgoing signals from ground-based VLF
transmitters undergo a significant spectral broadening as they propagate
through the ionosphere and protonosphere up to altitudes in the range
600-3800 km. For transmitter signals in the range 10-20 kHz, the spectral
broadening can be as high as 10% of the nominal frequency of the input
signal. Spectral broadening occurs only in the presence of impulsive VLF
hiss and/or a lower hybrid resonance noise band with an irregular lower
cutoff frequency, and only for signals whose frequency exceeds the LHR
frequency at the satellite location
	},
	keywords={
		ionospheric electromagnetic wave propagation
		radiowave propagation
		VLF
		ionosphere
		radiowave propagation
		ELF
		topside
		apparent spectral broadening
		transmitter signals
		transionospheric propagation
		narrowband
		upgoing
		spectral broadening
		ionosphere
		protonosphere
		impulsive VLF hiss
		lower hybrid resonance noise
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BellJan83,
	author={Bell, T.F. and Inan, U.S. and Kimura, I. and Matsumoto, H. and Mukai, T. and Hashimoto, K.},
	title={
EXOS-B/Siple Station VLF wave-particle interaction experiments. II.
Transmitter signals and associated emissions
	},
	journal={Journal of Geophysical Research},
	volume={88},
	number={A1},
	year={1983},
	month={Jan},
	pages={295-309},
	abstract={
For pt.I see ibid., vol.88, no.A1, p.282-94 (1983). Interactions between
coherent VLF waves and energetic particles in the magnetosphere have been
studied in a joint program involving the Japanese high-altitude satellite
EXOS-B and Siple Station VLF transmitter. During the period July
15-September 7, 1979, transmissions to the EXOS-B satellite were carried
out on 50 separate occasions when the spacecraft was within +or-60 degrees
longitude of the magnetic field lines linking Siple Station, Antarctica
with its conjugate station at Roberval, Canada. The transmitter signals
were detected on EXOS-B on 50% of the occasions when transmissions were
attempted, and on 5 occasions the transmitter signals were observed to have
triggered VLF emissions somewhere along their ray path between the
ionosphere and the satellite. Analysis of the emission triggering events
provided strong evidence that the triggering took place inside
whistler-mode ducts and that the emissions reached the satellite only after
being scattered at one end of the ducts by ionospheric irregularities. The
authors conclude that in the noon sector of the magnetosphere the amplitude
of nonducted signals from the Siple transmitter is generally less than the
threshold level necessary for triggering in the nonducted mode
	},
	keywords={
		ionospheric electromagnetic wave propagation
		magnetosphere
		magnetospheric electromagnetic wave propagation
		radiowave emission
		VLF
		propagation
		triggered
		AD 1979 07 to 09
		wave-particle interaction
		coherent
		ionosphere
		whistler-mode ducts
		ionospheric irregularities
		magnetosphere
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{ChangJan83,
	author={Chang, H.C. and Inan, U.S.},
	title={
Quasi-relativistic electron precipitation due to interactions with coherent
VLF waves in the magnetosphere
	},
	journal={Journal of Geophysical Research},
	volume={88},
	number={A1},
	year={1983},
	month={Jan},
	pages={318-28},
	abstract={
The generalised equations of motion for the gyroresonance interaction
between energetic electrons and coherent VLF waves in the magnetosphere are
employed to study quasi-relativistic electron precipitation. It is
suggested that these exact equations be used for particle energies higher
than 50 keV. Based on these equations and the relativistic cyclotron
resonance condition, a previous test particle simulation method is extended
to higher energies and is used to study the wave-particle interactions
involving the near-loss-cone quasi-relativistic particles. The root mean
square (RMS) pitch angle scattering of the near-loss-cone particles and the
corresponding precipitated energy spectrum are then calculated and
compared. It is argued that the full width at half maximum of the RMS
scattering pattern would give an upper bound to that of the energy spectrum
of the precipitated flux. It is suggested that the observed narrow peaks in
precipitated energy spectra may be caused by monochromatic signals injected
into the magnetosphere by VLF transmitters
	},
	keywords={
		atmospheric electron precipitation
		magnetosphere
		quasirelativistic
		relativistic
		high energy
		ionosphere
		wave particle interaction
		trapped particle
		electron precipitation
		interactions
		coherent VLF waves
		magnetosphere
		gyroresonance interaction
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{KimuraJan83,
	author={Kimura, I. and Matsumoto, H. and Mukai, T. and Hashimoto, K. and Bell, T.F. and Inan, U.S. and Helliwell, R.A. and Katsufrakis, J.P.},
	title={
EXOS-B/Siple Station VLF wave-particle interaction experiments. I. General
description and wave-particle correlations
	},
	journal={Journal of Geophysical Research},
	volume={88},
	number={A1},
	year={1983},
	month={Jan},
	pages={282-94},
	abstract={
In situ measurements of both energetic particles and VLF waves have been
carried out in a joint program involving the Japanese satellite EXOS-B and
the Siple Station VLF transmitter. A general description of the experiment
is given as well as some results concerning wave particle correlations.
Correlations of electron flux and pitch angle anisotropy in the energy
range from 85 eV to 6.9 keV with waves in a range from 300 Hz to 9 kHz are
examined. These electrons sometimes have a pitch angle distribution with a
peak flux at 90 degrees pitch angle (so-called pancake distribution). On
five passes out of a total of 50 during the summer campaign in 1979, the
energy of the electrons that showed a high pitch angle anisotropy shifted
upward as the satellite moved into the plasmasphere, crossing the
plasmapause in the equatorial region. In two cases out of five, strong
Siple signals were observed in the geomagnetic equatorial region just
outside the plasmapause, in association with such a pancake pitch angle
distribution of electrons. The Siple signals are most likely amplified by
the cyclotron instability due to the high pitch angle anisotropy (HPAA)
	},
	keywords={
		magnetosphere
		magnetospheric electromagnetic wave propagation
		AD 1979
		propagation
		radiowave heating experiment
		magnetosphere
		trapped particle
		wave-particle interaction
		wave-particle correlations
		VLF
		electron flux
		pitch angle anisotropy
		plasmasphere
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanSep82,
	author={Inan, U.S. and Helliwell, R.A.},
	title={
DE-1 observations of VLF transmitter signals and wave-particle interactions
in the magnetosphere
	},
	journal={Geophysical Research Letters},
	volume={9},
	number={9},
	year={1982},
	month={Sep},
	pages={917-20},
	abstract={
A broadband VLF receiver on the DE-1 satellite measures signals injected
into the magnetosphere by ground-based transmitters. VLF emissions
triggered by these signals indicate that the waves interact strongly with
trapped energetic particles. The propagation paths from the source to the
satellite are deduced on the basis of the group time delay and Doppler
shift. Although there are many different paths, emissions are triggered by
the later-arriving pulses that have traversed the geomagnetic equator.
First satellite-based observations of emission triggering by high-power
communications transmitters and their possible implications are discussed
	},
	keywords={
		magnetosphere
		magnetospheric electromagnetic wave propagation
		radiowave emission
		radiosignal
		trapped particle
		VLF
		wave-particle interactions
		magnetosphere
		triggered
		propagation paths
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanAug82,
	author={Inan, U.S. and Bell, T.F. and Chang, H.C.},
	title={
Particle precipitation induced by short-duration VLF waves in the
magnetosphere
	},
	journal={Journal of Geophysical Research},
	volume={87},
	number={A8},
	year={1982},
	month={Aug},
	pages={6243-64},
	abstract={
An extension of a previous test particle simulation model (Inan et al.,
1978) of the hydroresonance wave-particle interaction in the magnetosphere
is used to compute the detailed time variation of the precipitated energy
flux induced by monochromatic short-duration VLF waves. The resulting
precipitation pulse is found to have a characteristic shape dependent on
the L value, cold plasma density, wave frequency, and duration, as well as
the energetic particle distribution function. The role of these variables
in determining the temporal variation and the magnitude of the precipitated
flux is discussed for a wide range of typical magnetospheric parameters
	},
	keywords={
		atmospheric electron precipitation
		atmospheric precipitation
		magnetosphere
		VLF
		EM wave
		gyroresonant
		induced
		short-duration
		magnetosphere
		wave-particle interaction
		flux
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{HelliwellMay82,
	author={Helliwell, R.A. and Inan, U.S.},
	title={
VLF wave growth and discrete emission triggering in the magnetosphere: a
feedback model
	},
	journal={Journal of Geophysical Research},
	volume={87},
	number={A5},
	year={1982},
	month={May},
	pages={3537-50},
	abstract={
Doppler-shifted cyclotron resonance between electrons and narrowband
whistler mode waves is employed in a new feedback model to account for
observed signal growth and emission triggering in controlled experiments
using the Siple Station, Antarctica, VLF transmitter. The interaction
region is centered on the magnetic equator and is treated like an unstable
feedback amplifier with a delay line. The temporal growth rate is given by
gamma =(G-1)/T, where G is the loop gain and T is the effective loop delay.
For G<1 the system acts like an amplifier, while for G>1 the system is
unstable and can generate self-excited oscillations. The self-excited
oscillations reach saturation when G falls to unity, which occurs when the
electron transit time through the interaction region is comparable with the
phase bunching time. At signal levels well below saturation the model
predicts exponential temporal growth
	},
	keywords={
		atmospheric radiation
		magnetosphere
		VLF
		radiowave emission
		triggering
		Doppler
		wave growth
		discrete emission
		magnetosphere
		feedback model
		cyclotron resonance
		narrowband whistler mode
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BellMay82,
	author={Bell, T.F. and Luette, J.P. and Inan, U.S.},
	title={
ISEE 1 observations of VLF line radiation in the Earth's magnetosphere
	},
	journal={Journal of Geophysical Research},
	volume={87},
	number={A5},
	year={1982},
	month={May},
	pages={3530-36},
	abstract={
A search has been carried out for magnetospheric line radiation in the VLF
data acquired during the period October 1977-August 1979. While the
satellite position varied between L=2 and L=8 and the satellite longitude
lay in the range 50 degrees W to 110 degrees W. This magnetospheric region
encompassed the main regions in which the occurrence of VLF chorus has been
actively linked to power line radiation. Line radiation was detected on
only 5 of 90 orbits, and all examples occurred at frequencies below 4 kHz.
Line radiation was detected during a period when whistler mode echoing was
quite pronounced on lower L shells and may actually have been a scattered
component of line radiation echoing between hemispheres on a magnetic shell
of lower L value. It is concluded that very little of the background VLF
wave energy in the outer magnetosphere is contained directly in VLF line
radiation
	},
	keywords={
		atmospheric radiation
		magnetosphere
		radiowave emission
		AD 1977 to 1979
		VLF line radiation
		magnetosphere
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanApr82,
	author={Inan, U.S. and Tkalcevic, S.},
	title={
Nonlinear equations of motion for Landau resonance interactions with a
whistler mode wave
	},
	journal={Journal of Geophysical Research},
	volume={87},
	number={A4},
	year={1982},
	month={Apr},
	pages={2363-7},
	abstract={
A simple set of equations are derived for describing the cyclotron averaged
motion of Landau resonant particles in a whistler mode wave propagating at
an angle to the static magnetic field. It is argued that for the parameters
of the inner magnetosphere, the equations would be an accurate description
of the near-resonant particles' motion. The relative magnitudes of the wave
magnetic and electric field forces are discussed and the parameter ranges
for which the wave magnetic field effects can be neglected are specified
	},
	keywords={
		ionosphere
		magnetosphere
		whistlers
		nonlinear
		ionosphere
		wave particle interaction
		equations of motion
		Landau resonance interactions
		whistler mode wave
		cyclotron
		inner magnetosphere
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BellOct81,
	author={Bell, T.F. and Inan, U.S.},
	title={
Transient nonlinear pitch angle scattering of energetic electrons by
coherent VLF wave packets in the magnetosphere
	},
	journal={Journal of Geophysical Research},
	volume={86},
	number={A11},
	year={1981},
	month={Oct},
	pages={9047-63},
	abstract={
With the aid of adiabatic theory, a study is made of the transient
nonlinear pitch angle scattering experienced by energetic electrons under
the influence of coherent VLF wave packets in the magnetosphere. Finite
wave packets of both fixed and variable frequency are considered, as are
wide ranges of L shell, wave frequency, and wave amplitude. The results
indicate that large mean pitch angle changes can be induced in the portion
of the energetic population that undergoes a nonlinear cyclotron resonance
interaction with the wave packet. Two classes of nonlinearly interacting
particles are involved, the nonlinearly resonant particles trapped in the
wave and the nonlinearly resonant nontrapped particles
	},
	keywords={
		magnetosphere
		magnetospheric electromagnetic wave propagation
		radiowave propagation
		L-shell
		radiowave propagation
		energetic electrons
		coherent VLF wave packets
		magnetosphere
		adiabatic theory
		transient nonlinear pitch angle scattering
		wave frequency
		wave amplitude
		nonlinear cyclotron resonance interaction
		nonlinearly interacting particles
		nonlinearly resonant particles
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{BellJun81,
	author={Bell, T.F. and Inan, U.S. and Helliwell, R.A.},
	title={
Nonducted coherent VLF waves and associated triggered emissions observed on
the ISEE-1 satellite
	},
	journal={Journal of Geophysical Research},
	volume={86},
	number={A6},
	year={1981},
	month={Jun},
	pages={4649-70},
	abstract={
Reports observations of non-ducted coherent VLF waves from ground-based
transmitters and associated VLF emissions in the magnetosphere. The data
reported were acquired by the Stanford University VLF Wave Injection
Experiment on the ISEE-1 satellite. The aim is to acquire understanding of
interactions between coherent VLF waves and energetic particles in the
magnetosphere, in particular the whistler mode instability through which
both natural and stimulated VLF emissions are produced
	},
	keywords={
		magnetosphere
		magnetospheric electromagnetic wave propagation
		radiowave propagation
		radiowave propagation
		AD 1977 10 to 1979 10
		triggered emissions
		non-ducted coherent VLF waves
		magnetosphere
		energetic particles
		whistler mode instability
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@CONFERENCE{Kimura81,
	author={Kimura, I. and Matsumoto, H. and Mukai, T. and Hashimoto, K. and Halliwell, R.A. and Bell, T.F. and Inan, U.S. and Katsufrakis, J.P.},
	title={
EXOS/B/Siple Station VLF wave-particle interaction experiment
	},
	booktitle={Relation Between Laboratory and Space Plasmas. Proceedings of theInternational Workshop},
	volume={},
	number={},
	year={1981},
	month={},
	pages={331-8},
	abstract={
It is well-known that ground-based VLF signals are often amplified or
associated with VLF emissions by virtue of interactions with
counterstreaming electrons in the magnetosphere. In order to clarify this
mechanism of the wave-particle interaction, a Japanese satellite EXOS-B was
used to monitor the energetic electron flux as well as VLF signals
transmitted from Siple Station in Antarctica, expecting to observe wave
excitations by the interaction between the Siple signal and the energetic
electrons. The experiments were carried out in July, August, September and
December 1979 and in January 1980. Telemetry data acquisition was made at
NASA tracking stations locating near the Siple meridian. During these
periods, VLF emissions triggered by the Siple signal were observed only in
August. In the present paper, the preliminary results of experiments are
briefly introduced
	},
	keywords={
		magnetosphere
		EM wave
		AD 1979
		AD 1980
		radiowave emission
		wave-particle interaction
		counterstreaming electrons
		magnetosphere
		energetic electron flux
		Siple Station
		Antarctica
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{KimuraDec80,
	author={Kimura, I. and Matsumoto, H. and Mukai, T. and Hashimoto, K. and Morikura, M. and Sasaki, C. and Helliwell, R.A. and Bell, T.F. and Inan, U.S. and Katsufrakis, J.P.},
	title={
Exos-B/Siple Station wave-particle interaction experiments
	},
	journal={Bulletin of the Institute of Space and Aeronautical Science, University ofTokyo B},
	volume={16},
	number={4B},
	year={1980},
	month={Dec},
	pages={1367-80},
	abstract={
In situ measurements of both energetic particles and VLF waves have been
carried out in a joint program involving the Japanese satellite EXOS-B and
the Siple Station VLF transmitter. A general description of the experiment
is given as well as some results concerning wave-particle correlations.
Telemetry data acquisition was made by NASA tracking stations during summer
in 1979 and during the succeeding winter. This report describes mainly the
results of the summer experiment. The Siple signal was detected on about
32% of the observed passes. Siple triggered emissions (ASE) were observed
on five passes concentrated in a period from August 14 to 18, while it was
geomagnetically quiet after a large magnetic storm on August 13. There were
two types of Siple ASE; one is due to a direct triggering, which is
normally found in the ground observation, and the other is one triggered by
echoing signals, which is not usually observed on the ground
	},
	keywords={
		artificial satellites
		atmospheric measuring apparatus
		ionosphere
		ionospheric electromagnetic wave propagation
		magnetosphere
		magnetospheric electromagnetic wave propagation
		atmospheric measuring apparatus
		JIKIKEN satellite
		ionosphere EM wave propagation
		magnetosphere
		AD 1979 08 14 to 18
		geomagnetic quiet period
		directly triggered emission
		telemetry data acquisition
		Exos-B/Siple Station wave-particle interaction experiments
		energetic particles
		VLF waves
		Japanese satellite
		Siple Station VLF transmitter
		wave-particle correlations
		NASA tracking stations
		Siple signal
		Siple triggered emissions
		magnetic storm
		echoing signals
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{YavuzAug78,
	author={Yavuz, D. and Inan, U.S.},
	title={
A novel approach for finding the spectrum of periodically modulated FM
carriers
	},
	journal={IEEE Transactions on Communications},
	volume={COM-26},
	number={8},
	year={1978},
	month={Aug},
	pages={1309-15},
	abstract={
A new technique for finding the frequency spectrum of a carrier frequency
modulated by a periodic signal is presented. The technique is based on the
frequency modulation (FM) equation due to Hess, which in the frequency
domain is a double convolution equation. The technique reduces the FM
spectrum problem to the solution of a set of linear equations in which the
FM side-band amplitudes are the unknowns. The technique is simple and as a
result its implementation on a standard computer is both simple and fast.
Furthermore, it is especially suitable when the modulating signal is in the
form of a Fourier series with a large number of terms or requires a large
number of terms to approximate it. Numerical results obtained using the
technique for a large number of complex modulating signals are presented
	},
	keywords={
		frequency modulation
		signal processing
		periodically modulated FM carriers
		frequency spectrum
		double convolution equation
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanJul78,
	author={Inan, U.S. and Bell, T.F. and Helliwell, R.A.},
	title={
Nonlinear pitch angle scattering of energetic electrons by coherent VLF
waves in the magnetosphere
	},
	journal={Journal of Geophysical Research},
	volume={83},
	number={A7},
	year={1978},
	month={Jul},
	pages={3235-53},
	abstract={
A computer simulation approach is used to study the nonlinear cyclotron
resonant interaction of energetic electrons and coherent VLF waves, with
special emphasis on the pitch angle scattering of the particles. Complete
equations of motion in an inhomogeneous magnetosphere are used, and the
effects of various parameters are studied. Comparison is made with linear
theory, and a quantitative and easy-to-use criterion to determine the
applicability of linear theory under any given conditions is presented. The
full distribution of particles is simulated by test electrons appropriately
distributed in energy and pitch angle. By computing the scattering of these
test particles and integrating over energy and pitch angle, the
precipitated flux is obtained. The results indicate that coherent VLF waves
can have a significant effect on the dynamics and lifetimes of energetic
electrons trapped in the magnetosphere on magnetic shells illuminated by
the waves
	},
	keywords={
		atmospheric electron precipitation
		atmospheric radiation
		magnetosphere
		magnetospheric electromagnetic wave propagation
		whistlers
		energetic electrons
		coherent VLF waves
		magnetosphere
		computer simulation
		nonlinear cyclotron resonant interaction
		pitch angle scattering
		linear theory applicability criterion
		1 to 2 keV electrons
		precipitated particle flux
		whistler mode waves
		wave/particle interactions
		particle energy integration
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanJul77,
	author={Inan, U.S. and Bell, T.F.},
	title={
The plasmapause as a VLF wave guide
	},
	journal={Journal of Geophysical Research},
	volume={82},
	number={19},
	year={1977},
	month={Jul},
	pages={2819-27},
	abstract={
The properties of the plasmapause as a VLF wave guide are studied. The
guidance that occurs is a form of gradient trapping of VLF wave energy. It
is shown that guiding is possible at both the inner and outer edges of the
plasmapause and that more efficient guiding occurs as the plasmapause
gradients become stronger. In the case of strong gradients, waves coming
from a wide latitude range ( approximately 8 degrees ) are focused tightly
about the plasmapause field lines, resulting in a wave intensity increase
of approximately 3 dB near the magnetic equatorial plane. It is shown that
plasmapause-guided waves can be observed on the ground and can echo between
hemispheres, precisely as can waves guided in normal whistler ducts. The
single distinguishing feature of plasmapause-guided waves is a lowered
upper cutoff frequency. The results indicate that the vicinity of the
plasmapause represents a natural and readily accessible region of VLF wave
guidance and focusing where both passive and active VLF experiments can be
studied through ground and in situ satellite measurements
	},
	keywords={
		guided electromagnetic wave propagation
		magnetospheric electromagnetic wave propagation
		radiowave propagation
		plasmapause
		VLF wave guide
		whistler mode waves
		},
	mynotes={UNREAD},
}
/usr/tmp/citation.tmp.28355
@ARTICLE{InanMar77,
	author={Inan, U.S. and Bell, T.F. and Carpenter, D.L. and Anderson, R.R.},
	title={
Explorer 45 and Imp 6 observations in the magnetosphere of injected waves
from the Siple Station VLF transmitter
	},
	journal={Journal of Geophysical Research},
	volume={82},
	number={7},
	year={1977},
	month={Mar},
	pages={1177-87},
	abstract={
Reports the first results of a Stanford University-University of Iowa joint
experiment in which VLF waves from the Siple Station transmitter in
Antarctica are injected into the magnetosphere along the Earth's magnetic
field lines and are detected near the magnetic equatorial plane by the
Explorer 45 and Imp 6 spacecraft. The purpose of this experiment is to
conduct a controlled in situ study of VLF wave-particle interactions, in
particular, to determine the propagation characteristics of the injected
waves in the magnetosphere, to determine the regions where VLF emissions
are produced, and to determine the effective volume of the magnetosphere
illuminated by the Siple transmitter
	},
	keywords={
		magnetosphere
		magnetospheric electromagnetic wave propagation
		radiowave propagation
		Explorer 45
		Imp 6
		magnetosphere
		injected waves
		Siple Station VLF transmitter
		Antarctica
		wave particle interactions
		},
	mynotes={UNREAD},
}
@ARTICLE{InanMar77,
	author={Inan, U.S. and Bell, T.F. and Anderson, R.R.},
	title={
Cold plasma diagnostics using satellite measurements of VLF signals from
ground transmitters
	},
	journal={Journal of Geophysical Research},
	volume={82},
	number={7},
	year={1977},
	month={Mar},
	pages={1167-76},
	abstract={
A new diagnostic technique to obtain the cold plasma density profile in the
magnetosphere is introduced. This method uses satellite measurements of
group delay and pulse duration of VLF signals from ground transmitters in
conjunction with a detailed ray tracing analysis. An iterative method is
involved. This method starts with an approximate density profile, computes
the ray paths for that profile, and then compares the properties of the
rays that reach the satellite location with the actual satellite
measurements. The density profile is then modified to account for any
discrepancies between the two results. The same process is repeated with
the new profile until one has reasonable agreement between the data and ray
tracing results. This method is applied to the case of an Imp 6 pass on
June 28, 1973, where strong signals from the Siple VLF transmitter were
observed for over 25 min. Good agreement is found between the results of
the new technique and the well-known ground whistler techniques of cold
plasma diagnostics. The results also serve to illustrate the wide diversity
of paths of propagation from ground transmitters to high-altitude
satellites during VLF wave injection experiments
	},
	keywords={
		atmospheric techniques
		magnetosphere
		magnetospheric electromagnetic wave propagation
		plasma
		plasma diagnostics
		satellite measurements
		VLF signals
		ground transmitters
		diagnostic technique
		cold plasma density profile
		magnetosphere
		ray tracing
		iterative method
		},
	mynotes={UNREAD},
}

