Ion cyclotron waves in the Io torus during the Galileo encounter: Warm plasma dispersion analysis

Physics

Scientific paper

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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.

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