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Observations of rotational discontinuity - Slow expansion fan structure of the magnetotail boundaryThis paper gives the first explicit test of the rotational discontinuity-slow expansion fan structure predicted by MHD models of the open tail boundary. The magnetic field and plasma data collected by IMP 8 during its magnetotail boundary crossings at geocentric distances near 25 Re and high latitudes are analyzed. Many crossings show the particle and field signatures of the paired MHD tail boundary structure. The openness of the tail is revealed by rotational discontinuities. They often show relatively large normal magnetic field components. Other crossings show properties that suggest a tangential discontinuity and reveal regions where, or times when, the tail is closed. Examples of each are given here.
Document ID
19900035652
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sanchez, E. R.
(California Univ. Los Angeles, CA, United States)
Siscoe, G. L.
(California, University Los Angeles, United States)
Gosling, J. T.
(California Univ. Los Angeles, CA, United States)
Hones, E. W., Jr.
(Los Alamos National Laboratory NM, United States)
Lepping, R. P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1990
Publication Information
Publication: Journal of Geophysical Research
Volume: 95
ISSN: 0148-0227
Subject Category
Geophysics
Accession Number
90A22707
Funding Number(s)
CONTRACT_GRANT: NSF ATM-85-03980
Distribution Limits
Public
Copyright
Other

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