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Currents in Saturn's magnetosphereA model of Saturn's magnetospheric magnetic field is obtained from the Voyager 1 and 2 observations. A representation consisting of the Z sub 3 zonal harmonic model of Saturn's planetary magnetic field together with an explicit model of Saturn's planetary magnetic field and a model of the equatorial ring current fits the observations well within r 20 R sub S, with the exception of data obtained during the Voyager 2 inbound pass. Previously announced in STAR as N83-30345
Document ID
19840030079
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Connerney, J. E. P. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Acuna, M. H. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Ness, N. F. (NASA Goddard Space Flight Center Laboratory for Extraterrestrial Physics, Greenbelt, MD, United States)
Date Acquired
August 12, 2013
Publication Date
November 1, 1983
Publication Information
Publication: Journal of Geophysical Research
Volume: 88
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0148-0227
Accession Number
84A12866
Distribution Limits
Public
Copyright
Other

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