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A computational code for two-dimensional unsteady magnetohydrodynamics by the method of characteristics

Authors :
Y. Q. Lou
Robert Rosner
Peter Ulmschneider
Source :
The Astrophysical Journal. 315:349
Publication Year :
1987
Publisher :
American Astronomical Society, 1987.

Abstract

A 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.

Details

ISSN :
15384357 and 0004637X
Volume :
315
Database :
OpenAIRE
Journal :
The Astrophysical Journal
Accession number :
edsair.doi...........c2957eaa40cd06e7ecbd02ef8098ceee