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Solutions to bi-Maxwellian transport equations for the polar windIn this study, polar wind solutions are obtained for a broad range of O(+) density, H(+) drift velocity, electron temperature and H(+) temperature boundary conditions. The bi-Maxwellian-based 16-moment set of transport equations is used, since this set is expected to be superior to Maxwellian-based equations in describing large temperature anisotropies and heat flows. The present solutions corroborate earlier results when similar boundary conditions are used. Also, for previously unexplored combinations of boundary conditions, the present solutions are often qualitatively different from any obtained before.
Document ID
19890047621
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Demars, H. G.
(Utah State Univ. Logan, UT, United States)
Schunk, R. W.
(Utah State University Logan, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Publication Information
Publication: Planetary and Space Science
Volume: 37
ISSN: 0032-0633
Subject Category
Geophysics
Accession Number
89A34992
Funding Number(s)
CONTRACT_GRANT: F49620-86-C-0109
CONTRACT_GRANT: NAGW-77
Distribution Limits
Public
Copyright
Other

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