A comparison of characteristic times for satellite absorption of energetic protons trapped in the Jovian and Saturnian magnetic fields
Author:
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
http://www.agu.org/journals/gl/v008/i009/GL008i009p00976/GL008i009p00976.pdf
Reference17 articles.
1. The magnetic field of Saturn: Further studies of Pioneer 11 observations;Acuna;J. Geophys. Res.,1980
2. Jupiter's radiation belts;Brice;Icarus,1973
3. Low-energy charged particles in Saturn's raagnetosphere: Results from Voyager 1;Krimigis;Science,1981
4. If you've seen one magnetosphere, you haven't seen them all: Energetic particle observations in the Saturn magnetosphere;McDonald;J. Geophys. Res.,1980
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1. Energetic particle absorption by atmosphereless satellites and rings;Advances in Space Research;1993-10
2. Magnetospheric environments of outer planet rings: Influence of Saturn's axially symmetric magnetic field;Icarus;1987-07
3. Satellite sweeping in offset, tilted dipole fields;Journal of Geophysical Research;1987
4. An upper limit on the sizes of shepherding satellites at Saturn's ring G;Journal of Geophysical Research;1987
5. Monte Carlo simulation of charged particle impact on the satellites of Jupiter and Saturn;Journal of Geophysical Research;1986
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