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Detailed Reference Information |
Cowee, M.M., Winske, D., Russell, C.T. and Strangeway, R.J. (2007). 1D hybrid simulations of planetary ion-pickup: Energy partition. Geophysical Research Letters 34: doi: 10.1029/2006GL028285. issn: 0094-8276. |
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Ion pickup in planetary environments results in unstable newborn ion populations with sufficient free energy to generate electromagnetic plasma waves. Estimates of the SO2 + pickup rates near the Jovian moon, Io, based on ion cyclotron wave observations assumed that the newborn pickup ions lose 50% of their energy to wave growth. Using one-dimensional initial-value hybrid simulation, we test this assumption and predict that at most ~25% of the energy of the newborn ion population is lost to wave growth for conditions at Io. This energy is lost over >1400 SO2 + gyroperiods (~1 hour), with the majority lost after saturation of the instability. Thus the saturation wave energy is low, at <3% of the newborn ion population's energy. In contrast, newborn ions in cometary environments saturate at substantially higher wave energies (~30% of the newborn ion population's energy), but do not continue to lose energy afterwards. |
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Abstract |
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Keywords
Interplanetary Physics, Pickup ions, Ionosphere, Plasma waves and instabilities, Planetary Sciences, Solar System Objects, Jovian satellites, Planetary Sciences, Solar System Objects, Io, Planetary Sciences, Solar System Objects, Comets |
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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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