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Plasma observations near Saturn - Initial results from Voyager 1The Voyager 1 encounter with Saturn and its satellites yielded extensive measurements of magnetospheric low-energy plasma electrons and positive ions, both heavy and light, probably of hydrogen and nitrogen or oxygen. At radial distances between 15 and 7 Saturn radii on the inbound trajectory, the plasma appears to corotate with a velocity within 20% of that theoretically expected for rigid corotation. The Titan data, taken while the moon was inside the Saturn magnetosphere, shows a clear signature characteristic of the interaction between a subsonic corotating magnetospheric plasma and the atmospheric or ionospheric exosphere of Titan.
Document ID
19810043829
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Bridge, H. S.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Belcher, J. W.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Lazarus, A. J.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Olbert, S.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Sullivan, J. D.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Bagenal, F.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Gazis, P. R.
(MIT Cambridge, Mass., United States)
Hartle, R. E.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Ogilvie, K. W.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Scudder, J. D.
(NASA Goddard Space Flight Center Greenbelt, Md., United States)
Date Acquired
August 11, 2013
Publication Date
April 10, 1981
Publication Information
Publication: Science
Volume: 212
Subject Category
Lunar And Planetary Exploration
Accession Number
81A28233
Funding Number(s)
CONTRACT_GRANT: JPL-953733
Distribution Limits
Public
Copyright
Other

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