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Energetics and dynamics of resonant and nonresonant scattering in strong magnetic fieldsThe energetics and the dynamics resulting from electron-photon resonant and nonresonant scattering in a plasma with magnetic field about 10 to the 12th G are studied in detail. Precise analytic results are obtained in the optically thin limit, and numerical results are presented for the optically thick case. For the latter, it is found that when the equilibrium temperature T(C) is determined by the cooling/heating balance due solely to cyclotron resonant scattering, the ratio of T(C) to the superstrong field B remains fairly constant for N(e) up to about 6 x 10 to the 21st electrons/sq cm. This line-dominated region comes to an end when the extra heating from the hard continuum photons becomes competitive with the line processes and drives T(C) well above the pure line value. For parameters characteristic of GB 880205, the thickness of the line-dominated region is determined to be between 10 to the 21st and 10 to the 22nd electrons/sq cm.
Document ID
19910028056
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lamb, Don Q.
(Chicago Univ. Chicago, IL, United States)
Wang, John C. L.
(Chicago, University IL, United States)
Wasserman, Ira M.
(Cornell University Ithaca, NY, United States)
Date Acquired
August 14, 2013
Publication Date
November 10, 1990
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 363
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
91A12679
Funding Number(s)
CONTRACT_GRANT: NSF AST-89-13112
CONTRACT_GRANT: NAGW-666
CONTRACT_GRANT: NAGW-830
CONTRACT_GRANT: NAGW-1284
Distribution Limits
Public
Copyright
Other

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