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Acceleration of the solar wind as a result of the reconnection of open magnetic flux with coronal loops

โœ Scribed by Fisk, L. A.

Book ID
119658180
Publisher
American Geophysical Union
Year
2003
Tongue
English
Weight
155 KB
Volume
108
Category
Article
ISSN
0148-0227

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โœ A. W. Hood; E. R. Priest ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 789 KB

Solar coronal loops are observed to be remarkably stable structures. A magnetohydrodynamic stability analysis of a model loop by the energy method suggests that the main reason for stability is the fact that the ends of the loop are anchored in the dense photosphere. In addition to such line-tying,