EE 350 Radioscience Seminar
Professor Umran S. Inan
Winter 2003-2004
Date: Wednesday, January 7, 2004
Time: 4:15 PM – Refreshments at 4:00
Location: Bldg.
360, Room 361A
Remote Sensing the Earth's
Plasmasphere
Prof. Don Carpenter STAR Lab, EE, Stanford University
Abstract
The Earth's plasmasphere, discovered some 50 years ago using
ground based radio techniques, is a torus-like region that
encircles the Earth. Its outer boundary, called the plasmapause,
is aligned with the Earth's dipole magnetic field, typically
reaching an equatorial distance of 4 Earth radii. The
plasmapause region exhibits many dynamic effects, including fast
inward displacements during storm-like intervals in space,
instabilities, and complex wave activity. The storm-time
displacements are believed to be due to the physics of
interactions between the cooler plasmas of the plasmasphere and
the hot plasmas that move inward toward the Earth during stormy
periods. Much that we know about the plasmasphere has been
accomplished through remote sensing. For example, teams of
researchers on the IMAGE satellite, launched in March 2000, have
been studying the plasmasphere using a variety of imaging
techniques, including radio sounding. Some remarkable results
from the IMAGE mission will be described.
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