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On the nature of the interaction of the Jovian magnetosphere with the icy Galilean satellitesThe effects of plasma and micrometeoroid bombardment of each satellite are considered in the case of interactions between the Jovian magnetosphere and Europa, Ganymede, and Callisto, in an attempt to understand the influences of these exogenic processes on the surface properties of each of the three moons. Sublimated and sputtered H2O results in a net O2 atmosphere on each of the three moons, and the effectiveness of such an atmosphere in preventing the Jovian plasma from reaching each satellite surface is considered for a variety of magnetospheric conditions. Also studied are the effects of possible satellite magnetic field magnitude and orientation, in order to estimate satellite magnetosphere properties, and the orbits of charged micrometeroids in the Jupiter magnetosphere, in order to determine the relative flux of these particles over the satellite surfaces.
Document ID
19830052712
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Wolff, R. S.
(California Institute of Technology, Jet Propulsion Laboratory, Space Physics Section, Pasadena CA, United States)
Mendis, D. A.
(California, University La Jolla, CA, United States)
Date Acquired
August 11, 2013
Publication Date
June 1, 1983
Publication Information
Publication: Journal of Geophysical Research
Volume: 88
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
83A33930
Funding Number(s)
CONTRACT_GRANT: NSG-7102
CONTRACT_GRANT: NAS7-100
CONTRACT_GRANT: NGR-05-009-110
Distribution Limits
Public
Copyright
Other

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