Physics
Scientific paper
Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982georl...9.1167c&link_type=abstract
Geophysical Research Letters, vol. 9, Oct. 1982, p. 1167-1170.
Physics
28
Ion Motion, Ionospheric Disturbances, Plasma Pumping, Plasma-Particle Interactions, Satellite Observation, Wave Excitation, Auroral Zones, Cyclotron Frequency, Electrostatics, Emission Spectra, Plasma Frequencies, Propagation Modes, Wave Propagation
Scientific paper
Discrete emissions at the lower hybrid frequency are often seen on the S3-3 satellite. Simultaneous observation of perpendicularly heated ions suggests that these ions may provide the free energy necessary to drive the instability. Studies of the dispersion relation for flute modes excited by warm ion rings in velocity space show that waves are excited with real frequencies near the lower hybrid frequency and with growth rates ranging from about 0.01 to 1 times the ion cyclotron frequency. Numerical results are therefore consistent with the possibility that the observed ions are the free energy source for the observed waves.
Cattell Cynthia
Hudson Mary
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