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The effect of Jupiter's satellites on the diffusion of protonsProton diffusion data are calculated for the Jovian satellites Amalthea, Io, Europa, Ganymede, and Callisto, assuming an equatorial magnetic field at Jupiter's surface of 10 gauss. The cyclotron radius, bounce period, and drift period are calculated for 1 MeV protons. These characteristics and the proton energy at the satellite, mean life near the satellite before impact, and diffusion time are also calculated for 100 MeV protons which conserve their first adiabatic invariant. The longitudinal distance between successive bounces is of the order of a few satellite radii.
Document ID
19720020214
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Mead, G. D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 6, 2013
Publication Date
July 1, 1972
Publication Information
Publication: JPL Proc. of the Jupiter Radiation Belt Workshop
Subject Category
Space Sciences
Accession Number
72N27864
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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