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A computational code for two-dimensional unsteady magnetohydrodynamics by the method of characteristicsA computational code for solving two-dimensional, time-dependent MHD equations by the method of characteristics is presented. Its capabilities are demonstrated by solving two very different problems for which analytical solutions exist: linearized, standing MHD wave motions in a magnetized cylindrical plasma, and nonlinear self-similar expansion of a magnetized plasma ball. The nonlinear development of standing MHD wave solutions in a cylindrical plasma is also studied. The method can be naturally embedded in the computational architecture of massively parallel processors.
Document ID
19870051107
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lou, Y. Q.
(Harvard Univ. Cambridge, MA, United States)
Rosner, R.
(Harvard University Cambridge, MA, United States)
Ulmschneider, P.
(Heidelberg, Universitaet Germany)
Date Acquired
August 13, 2013
Publication Date
April 1, 1987
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 315
ISSN: 0004-637X
Subject Category
Plasma Physics
Accession Number
87A38381
Funding Number(s)
CONTRACT_GRANT: NSF AST-85-06640
CONTRACT_GRANT: DFG-SFB-132
Distribution Limits
Public
Copyright
Other

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