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Saturn's magnetic tail - Structure and dynamicsVoyager 1 magnetic field observations have provided evidence of a Saturnian magnetic tail. Tail current system distributions are inferred through comparison of the observations with a realistic magnetotail current system model. Temporal variations observed in the tail were probably produced by solar wind variations.
Document ID
19810060824
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1038/292753a0
Authors
Behannon, K. W. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Connerney, J. E. P. (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 11, 2013
Publication Date
February 20, 1981
Publication Information
Publication: Nature
Volume: 292
Subject Category
Lunar And Planetary Exploration
Accession Number
81A45228
Distribution Limits
Public
Copyright
Other

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