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Formation and stability of the self-consistent one-dimensional tail current sheetThe paper investigates the formation, the structure, and the stability of self-consistent one-dimensional current sheets in which the ions carry most of the current and momentum (the occurrence of which was suggested by observations of Mitchell et al., 1990; and Sergeev et al., 1990). Results of the analysis showed that, for the case of a cold current sheet, the characteristic thickness lamba equals to about (Bz/B0) exp 4/3 c/omega(p0), where Bz is the normal field component, B0 is the asymptotic magnitude of the reversing field, and c/omega(p0)is the collisionless ion skin depth based on lobe density. A two-dimensional self-consistent dynamical simulation model is developed, which demonstrates that these idealized current sheets are unstable to kink perturbations driven by the anisotropic pressure distribution produced by the chaotic nature of the particle orbits in a field-reversal region.
Document ID
19930032331
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Pritchett, P. L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Coroniti, F. V.
(California Univ. Los Angeles, United States)
Date Acquired
August 15, 2013
Publication Date
November 1, 1992
Publication Information
Publication: Journal of Geophysical Research
Volume: 97
Issue: A11
ISSN: 0148-0227
Subject Category
Geophysics
Accession Number
93A16328
Funding Number(s)
CONTRACT_GRANT: NAG5-1480
CONTRACT_GRANT: NSF ATM-89-22133
CONTRACT_GRANT: NSF ATM-90-17759
Distribution Limits
Public
Copyright
Other

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