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Wave phenomena in the upstream region of SaturnA search was carried out for the signatures of waves associated with both the electron and the ion foreshocks in the upstream region of Saturn, using magnetic-field data obtained by Voyager 1 and 2 during transit through this region. Two distinct bands of wave activity were found at frequencies around 0.5-mHz and 2-mHz in the upstream region. The two classes of waves differ considerably in their properties: the 0.5-mHz waves are righthanded and strongly elliptically polarized, while the 2-mHz waves are elliptically or circularly polarized in the left-handed sense. It is suggested that the two waves may be associated with two different backstreaming particle distributions, possibly those reflected from the shock and those leaking from the hot magnetic field at frequencies between 90 and 150 mHz.
Document ID
19930036987
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Orlowski, D. S.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Russell, C. T.
(California Univ. Los Angeles, United States)
Lepping, R. P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 16, 2013
Publication Date
December 1, 1992
Publication Information
Publication: Journal of Geophysical Research
Volume: 97
Issue: A12
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
93A20984
Funding Number(s)
CONTRACT_GRANT: NAGW-2349
Distribution Limits
Public
Copyright
Other

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