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Radiation belts of Jupiter - A second lookThe outbound leg of the Pioneer 11 Jupiter flyby explored a region farther from the equator than that traversed by Pioneer 10, and the new data require modification or augmentation of the magnetodisk model based on the Pioneer 10 flyby. The inner moons of Jupiter are sinks of energetic particles and sometimes sources. A large spike of particles was found near Io. Multiple peaks occurred in the particle fluxes near closest approach to the planet; this structure may be accounted for by a complex magnetic field configuration. The decrease in proton flux observed near minimum altitude on the Pioneer 10 flyby appears attributable to particle absorption by Amalthea.
Document ID
19750045136
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Fillius, R. W.
Mcilwain, C. E.
Mogro-Campero, A.
(California, University La Jolla, Calif., United States)
Date Acquired
August 8, 2013
Publication Date
May 2, 1975
Publication Information
Publication: Science
Volume: 188
Subject Category
Lunar And Planetary Exploration
Accession Number
75A29208
Funding Number(s)
CONTRACT_GRANT: NAS2-6552
Distribution Limits
Public
Copyright
Other

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