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Numerical simulation of reconnection in an emerging magnetic flux regionThe resistive MHD equations are numerically solved in two dimensions for an initial-boundary-value problem which simulates reconnection between an emerging magnetic flux region and an overlying coronal magnetic field. The solution involves both ideal-MHD and resistive-MHD processes, and the solution shows an evolution which is remarkably suggestive of the preflare, impulsive, and main phases of the flare-cycle.
Document ID
19850046159
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0273-1177(84)90159-5
Authors
Forbes, T. C. (New Hampshire, University Durham, NH, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1984
Publication Information
Publication: Advances in Space Research
Volume: 4
Issue: 7 19
ISSN: 0273-1177
Subject Category
Solar Physics
Accession Number
85A28310
Funding Number(s)
CONTRACT_GRANT: NAGW-76
Distribution Limits
Public
Copyright
Other

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