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A semikinetic model for early stage plasmasphere refilling. II - Effects of wave-particle interactionsThe paper treats the early stages of plasmasphere refilling along an initially depleted L = 4 magnetic flux tube through a semikinetic model, with special attention given to the effects of wave-particle interactions in which stochastic diffusion of ions in perpendicular velocity due to equatorially concentrated electromagnetic ion cyclotron waves plays a central role. Characteristic individual ion trajectories are examined, as well as the devolution of bulk parameters and ion distribution functions when equal 'polar wind' streams are injected at the northern and southern ionospheres. In the ion trajectories, relatively modest and realistic perpendicular electric field power levels are found to lead to decreased mirror latitudes, substantial acceleration, and equatorial entrainment of these ions. A substantial equatorial density depletion is also found, in agreement with the results of Olsen (1992).
Document ID
19920041881
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lin, J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Horwitz, J. L.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Wilson, G. R.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Ho, C. W.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Brown, D. G.
(Alabama, University Huntsville, United States)
Date Acquired
August 15, 2013
Publication Date
February 1, 1992
Publication Information
Publication: Journal of Geophysical Research
Volume: 97
ISSN: 0148-0227
Subject Category
Geophysics
Accession Number
92A24505
Funding Number(s)
CONTRACT_GRANT: NAG8-134
CONTRACT_GRANT: NSF ATM-89-11799
CONTRACT_GRANT: NAGW-2128
Distribution Limits
Public
Copyright
Other

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