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Pioneer 10 observations of the solar wind interaction with JupiterDetailed analysis of the Pioneer 10 plasma analyzer experiment flight data during the Jupiter flyby in late November and early December 1973 has been performed. The observations show that the interaction of Jupiter's magnetic field with the solar wind is similar in many ways to that at earth, but the scale size is over 100 times larger. Jupiter is found to have a detached standing bow shock wave of high Alfven Mach number. Like the earth, Jupiter has a prominent magnetopause that deflects the magnetosheath plasma and excludes its direct entry into the Jovian magnetosphere. Unlike that of the earth, the sunward hemisphere of Jupiter's outer magnetosphere is found to be highly inflated with thermal plasma and a high-beta region that is highly responsive to changes in solar wind dynamic pressure.
Document ID
19740060901
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Wolfe, J. H.
Mihalov, J. D.
Collard, H. R.
Mckibbin, D. D.
(NASA Ames Research Center Space Physics Branch, Moffett Field, Calif., United States)
Frank, L. A.
(Iowa, University Iowa City, Iowa, United States)
Intriligator, D. S.
(Southern California, University Los Angeles, Calif., United States)
Date Acquired
August 7, 2013
Publication Date
September 1, 1974
Publication Information
Publication: Journal of Geophysical Research
Volume: 79
Subject Category
Space Radiation
Accession Number
74A43651
Distribution Limits
Public
Copyright
Other

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