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Detailed Reference Information |
Huddleston, D.E., Strangeway, R.J., Warnecke, J., Russell, C.T., Kivelson, M.G. and Bagenal, F. (1997). Ion cyclotron waves in the Io torus during the Galileo encounter: Warm plasma dispersion analysis. Geophysical Research Letters 24: doi: 10.1029/97GL01203. issn: 0094-8276. |
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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 to torus composition ratios, pickup ion ring-type velocity-space distributions, and a thermal background plasma of typical torus 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 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.¿ 1997 American Geophysical Union |
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Abstract |
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Keywords
Planetology, Solar System Objects, Jovian satellites, Magnetospheric Physics, Magnetosphere interactions with satellites and rings, Space Plasma Physics, Wave/particle interactions, Magnetospheric Physics, Plasma waves and instabilities |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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