How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer?
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Title
How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer?
Authors
Keywords
Active regions, Magnetic fields, Magnetic extrapolations, Corona active, Solar wind, Radio Bursts, Type I, Radio emission, Quiet
Journal
SOLAR PHYSICS
Volume 289, Issue 11, Pages 4151-4171
Publisher
Springer Nature
Online
2014-08-20
DOI
10.1007/s11207-014-0582-y
References
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