Physics
Scientific paper
Sep 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997georl..24.2143h&link_type=abstract
Geophysical Research Letters, vol. 24, p. 2143
Physics
47
Cyclotron Radiation, Galileo Spacecraft, Ion Cyclotron Radiation, Plasma Diffusion, Toroidal Plasmas, Extraterrestrial Environments, Plasma Interactions, Electromagnetic Radiation, Wave Dispersion, Free Energy, Space Probes
Scientific paper
During the Galileo-Io flyby, nearly field-aligned, left-hand circularly polarized ion cyclotron waves were observed in a band near the sulfur-dioxide ion gyrofrequency. We have performed a warm plasma dispersion analysis using nominal Io torus composition ratios, pickup ion 'ring'-type velocity-space distributions, and a thermal background plasma of typical toms temperature. Analysis shows that the SO2(+) wave is dominant, particularly as the ring begins to broaden. The observed spectral peak indicates that the ring distribution of pickup SO2(+) is highly unstable and generates waves, but there is unlikely to be sufficient time for ions to fully the thermalize before dissociation occurs. Assuming wave-particle scattering of ions towards a 'bispherical' shell-type distribution, a free energy analysis and comparison with observed wave amplitudes suggests that the ions are not scattered far from the ring and/or that the SO2(+) composition ratio in the Io torus falls off considerably from Io wake values.
Bagenal Fran
Galland Kivelson Margaret
Huddleston D. E.
Russell Christopher T.
Strangeway Robert J.
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