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Statics and dynamics of Giacobini-Zinner magnetic tailThe data gathered by the International Cometary Explorer during its traversal of Comet Giacobini-Zinner's tail are subjected to stress balance requirements, yielding estimates of unmeasured quantities. It is noted that the comet's tail is embedded in an ionosheath whose static pressure is nearly equal to the solar wind stagnation pressure, leading to a large lobe field strength. A systematic variation is found in the ion temperature across the tail, implying the variation of the pickup velocity of new ions. Axial stress balance yields an expression for the strength of the lobe field which reveals weak variation with axial distance.
Document ID
19860047286
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Siscoe, G. L.
(California, University Los Angeles, United States)
Slavin, J. A.
(California Univ. Los Angeles, CA, United States)
Smith, E. J.
(California Univ. Los Angeles, CA, United States)
Tsurutani, B. T.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Jones, D. E.
(Brigham Young University Provo, UT, 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
Accession Number
86A32024
Funding Number(s)
CONTRACT_GRANT: JPL-955376
Distribution Limits
Public
Copyright
Other

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