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The method of projected characteristics for the evolution of magnetic archesA numerical method of solving fully nonlinear MHD equation is described. In particular, the formulation based on the newly developed method of projected characteristics (Nakagawa, 1981) suitable to study the evolution of magnetic arches due to motions of their foot-points is presented. The final formulation is given in the form of difference equations; therefore, the analysis of numerical stability is also presented. Further, the most important derivation of physically self-consistent, time-dependent boundary conditions (i.e. the evolving boundary equations) is given in detail, and some results obtained with such boundary equations are reported.
Document ID
19870058674
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Nakagawa, Y.
(Chiba Institute of Technology Narashino, Japan)
Hu, Y. Q.
(Chiba Inst. of Tech. Narashino, Japan)
Wu, S. T.
(Alabama, University Huntsville, United States)
Date Acquired
August 13, 2013
Publication Date
June 1, 1987
Publication Information
Publication: Astronomy and Astrophysics
Volume: 179
Issue: 1-2
ISSN: 0004-6361
Subject Category
Plasma Physics
Accession Number
87A45948
Funding Number(s)
CONTRACT_GRANT: NAS8-33526
CONTRACT_GRANT: NAGW-9
CONTRACT_GRANT: NAG8-53
CONTRACT_GRANT: F19628-82-K-0014
Distribution Limits
Public
Copyright
Other

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