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Solar magnetic reconnection seen in detail

โœ Scribed by Miller, Johanna L.


Book ID
121013887
Publisher
American Institute of Physics
Year
2013
Tongue
English
Weight
433 KB
Volume
66
Category
Article
ISSN
0031-9228

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Quasi-steady high-temperature current sheets are an energy source during the 'main' or 'hot' phase of solar flares. Such sheets are shown to be stabilized with respect to the tearing instability by a small transverse component of magnetic field existing in the sheets. \* Send offprint requests to B.