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Numerical simulation of mass injection for the formation of prominence magnetic field configurations. II - Symmetric injectionA two-dimensional MHD model simulating the formation of Kippenhahn-Schluter (1957) quiescent prominence (QP) magnetic field configurations is used to explore symmetric mass injection into a dipole magnetic field. An optimum magnetic field strength for QP formation by mass injection is obtained. It is found that a weaker magnetic field strength is more favorable for the condensation of the injected plasma but that a stronger field is more favorable for supporting the condensed plasma against gravity.
Document ID
19890031636
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
An, C.-H.
(Alabama Univ. Huntsville, AL, United States)
Bao, J. J.
(Alabama Univ. Huntsville, AL, United States)
Wu, S. T.
(Alabama, University Huntsville, United States)
Suess, S. T.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1988
Publication Information
Publication: Solar Physics
Volume: 115
Issue: 1 19
ISSN: 0038-0938
Subject Category
Solar Physics
Accession Number
89A19007
Funding Number(s)
CONTRACT_GRANT: NAGW-9
CONTRACT_GRANT: NAG8-53
Distribution Limits
Public
Copyright
Other

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