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Coronal heating through braiding of magnetic field lines
ASTROPHYSICAL JOURNAL, no. 1 (2004): L85-L88
Abstract
Cool stars such as our Sun are surrounded by a million degree hot outer atmosphere, the corona. For more than 60 years, the physical nature of the processes heating the corona to temperatures well in excess of those on the stellar surface have remained puzzling. Recent progress in observational techniques and numerical modeling now opens ...More
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