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Energy release in the solar corona from spatially resolved magnetic braids

✍ Scribed by Cirtain, J. W.; Golub, L.; Winebarger, A. R.; De Pontieu, B.; Kobayashi, K.; Moore, R. L.; Walsh, R. W.; Korreck, K. E.; Weber, M.; McCauley, P.; Title, A.; Kuzin, S.; DeForest, C. E.


Book ID
120004773
Publisher
Nature Publishing Group
Year
2013
Tongue
English
Weight
825 KB
Volume
493
Category
Article
ISSN
0028-0836

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πŸ“œ SIMILAR VOLUMES


Magnetic reconnection and energy release
✍ G. E. Vekstein; E. R. Priest; C. D. C. Steele πŸ“‚ Article πŸ“… 1991 πŸ› Springer 🌐 English βš– 802 KB

The heating of the solar corona by resistive turbulence of coronal magnetic fields is considered. The theory of this process, based on the Taylor-Heyvaerts-Priest hypothesis and a magnetic relaxation equation, is developed. Such an approach allows one to obtain the successive magnetic reconnection c