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Magnetic fields and charged particles around major planets and their satellitesIt is noted that whereas Jupiter and Saturn have magnetospheres whose large-scale structure can be understood by analogy with earth, the ways in which the magnetospheres differ are of great interest. At earth, large-scale processes are dominated by convective flows of plasma driven by the solar wind. At Jupiter, centrifugal effects that are driven by planetary rotation are critical. Magnetic particle sources include not only the ionosphere and solar wind (as at earth) but also satellites and rings. The internal planetary magnetic moments controlling the scale of the magnetosphere differ by orders of magnitude between Jupiter and earth. It is pointed out that where the magnetic moments have been modeled from spacecraft data, the restricted spatial sampling has biased the results and limited confidence in details of the models. Voyager data suggest that Io may itself be magnetized and surrounded by an entirely unfamiliar type of magnetosphere.
Document ID
19820038419
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Kivelson, M. G.
(California, University Los Angeles, CA, United States)
Date Acquired
August 10, 2013
Publication Date
December 24, 1981
Subject Category
Lunar And Planetary Exploration
Accession Number
82A21954
Funding Number(s)
CONTRACT_GRANT: NSG-7295
CONTRACT_GRANT: NAS9-55232
Distribution Limits
Public
Copyright
Other

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