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Preliminary results on the plasma environment of Saturn from the Pioneer 11 plasma analyzer experimentThe Ames Research Center Pioneer 11 plasma analyzer experiment provided measurements of the solar wind interaction with Saturn and the character of the plasma environment within Saturn's magnetosphere. It is shown that Saturn has a detached bow shock wave and magnetopause quite similar to those at earth and Jupiter. The scale size of the interaction region for Saturn is roughly one-third that at Jupiter, but Saturn's magnetosphere is equally responsive to changes in the solar wind dynamic pressure. Saturn's outer magnetosphere is inflated, as evidenced by the observation of large fluxes of corotating plasma. It is postulated that Saturn's magnetosphere may undergo a large expansion when the solar wind pressure is greatly diminished by the presence of Jupiter's extended magnetospheric tail when the two planets are approximately aligned along the same solar radial vector.
Document ID
19800034946
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Wolfe, J. H.
(NASA Ames Research Center Moffett Field, CA, United States)
Mihalov, J. D.
(NASA Ames Research Center Moffett Field, CA, United States)
Collard, H. R.
(NASA Ames Research Center Moffett Field, CA, United States)
Mckibbin, D. D.
(NASA Ames Research Center Space Science Div., 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 10, 2013
Publication Date
January 25, 1980
Publication Information
Publication: Science
Volume: 207
Subject Category
Lunar And Planetary Exploration
Accession Number
80A19116
Distribution Limits
Public
Copyright
Other

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