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Nonlinear computations of a solar flare modelA cylindrical axisymmetric tearing mode model for solar flares is investigated numerically. Large magnetic energy release only occurs when there are at least two mode rational surfaces in the current-carrying plasma.
Document ID
19840064010
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1063/1.864864
Authors
Strauss, H. (New York University New York, NY, United States)
Van Hoven, G. (California, University Irvine, CA, United States)
Date Acquired
August 12, 2013
Publication Date
August 1, 1984
Publication Information
Publication: Physics of Fluids
Volume: 27
ISSN: 0031-9171
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0031-9171
Accession Number
84A46797
Distribution Limits
Public
Copyright
Other

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