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A three-dimensional simulation of a coronal streamerA time-dependent MHD simulation was used to investigate the magnetic topology of an idealized streamerlike configuration in three dimensions. Starting from an initially current-free multipole field and a transonic flow, a quasi-steady, streamerlike configuration forms. The simulated streamer exhibits a closed magnetic field region bounded by a current layer and surrounded by open fields. This helmet region is surmounted by a current layer, with an enhanced density in the closed field and current sheet regions. The simulated streamer has a finite longitudinal extent, with the closed field region primarily confined to the center of the structure.
Document ID
19910036453
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Linker, Jon A.
(California Univ. Irvine, CA, United States)
Van Hoven, Gerard
(California, University Irvine, United States)
Schnack, Dalton D.
(Science Applications International Corp. San Diego, CA, United States)
Date Acquired
August 15, 2013
Publication Date
December 1, 1990
Publication Information
Publication: Geophysical Research Letters
Volume: 17
ISSN: 0094-8276
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0094-8276
Accession Number
91A21076
Distribution Limits
Public
Copyright
Other

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