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Large amplitude, low frequency plasma fluctuations at Comet Giacobini-ZinnerVery large amplitude fluctuations in electron density, temperature, and flow velocity were a prominent aspect of the solar wind interaction with Comet Giacobini-Zinner during the ICE encounter in September 1985. These fluctuations were detected at a distance of at least 900,000 km and grew in amplitude as ICE approached the comet, peaking in amplitude 60,000 km from closest approach. A typical period associated with the fluctuations was about 2 min, which corresponds to a scale length in the solar wind frame of about 50,000 km. For the most part these fluctuations appear to be a product of one or more plasma instabilities associated with the solar wind pick up of cometary ions.
Document ID
19860047281
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Gosling, J. T.
(Los Alamos National Lab. NM, United States)
Asbridge, J. R.
(Los Alamos National Lab. NM, United States)
Bame, S. J.
(Los Alamos National Lab. NM, United States)
Thomsen, M. F.
(Los Alamos National Lab. NM, United States)
Zwickl, R. D.
(Los Alamos National Laboratory NM, United States)
Date Acquired
August 12, 2013
Publication Date
March 1, 1986
Publication Information
Publication: Geophysical Research Letters
Volume: 13
ISSN: 0094-8276
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0094-8276
Accession Number
86A32019
Funding Number(s)
CONTRACT_GRANT: NASA ORDER S-04039-D
Distribution Limits
Public
Copyright
Other

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