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Effects of magnetospheric electrons on polar plasma outflow - A semikinetic modelThe effect or hot magnetospheric electrons on the polar-plasma outflow was investigated, using a semikinetic model developed by Wilson et al. (1990) and Ho et al. (1991) to simulate the effect. The model is based on a hybrid particle-in-cell approach, in which the H(+) and O(+) ions are treated as adiabatic parallel-drifting gyrocenters injected as the upgoing portions of drifting bi-Maxwellian distributions at 1.6 R(E), while the electrons are treated as a massless neutralizing fluid. The results show that, in order to simulate the polar outflow under the influence of hot magnetospheric electrons, it is necessary to consider the effect of the electron temperature gradient.
Document ID
19920059378
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ho, C. W.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Horwitz, J. L.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Singh, N.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Wilson, G. R.
(Alabama, University Huntsville, United States)
Moore, T. E.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 15, 2013
Publication Date
June 1, 1992
Publication Information
Publication: Journal of Geophysical Research
Volume: 97
Issue: A6 J
ISSN: 0148-0227
Subject Category
Geophysics
Accession Number
92A42002
Funding Number(s)
CONTRACT_GRANT: NAG8-822
Distribution Limits
Public
Copyright
Other

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