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The anisotropic radiative transfer problem in optically thick, strongly magnetized plasma - A comparison of resultsThe accuracy of four different methods for solving the coherent radiative transfer problem in a strongly magnetized plasma is compared. Specific attention is given to the case of a semi-infinite homogeneous plasma with a magnetic field perpendicular to the surface. The four approaches evaluated were: diffusion approximation schemes; the generalized H-function method of Silant'ev (1982) the Feautrier method of Nagel (1981) and the integral equation approach of Meszares and Bonazzola (1981). It is found that the coupled diffusion approximation schemes of Nagel (1981) and Kaminker et al. (1982) provided satisfactory results and were more efficient in many cases than direct numerical methods.
Document ID
19850049767
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Pavlov, G. G.
(Academy of Sciences (USSR) Leningrad, Ussr)
Shibanov, Iu. A.
(Academy of Sciences (USSR) Leningrad, Ussr)
Silantev, N. A.
(Akademiia Nauk SSSR Fiziko-Tekhnicheskii Institut, Leningrad, Ussr)
Nagel, W.
(Max-Planck-Institut fuer Physik und Astrophysik, Garching, West Germany; Harvard-Smithsonian Center for Astrophysics, Cambridge MA, United States)
Date Acquired
August 12, 2013
Publication Date
April 1, 1985
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 291
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
85A31918
Funding Number(s)
CONTRACT_GRANT: NAGW-246
Distribution Limits
Public
Copyright
Other

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