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Solar flare physics

Published online by Cambridge University Press:  14 March 2005

Boris V. Somov
Boris V. Somov
Affiliation:
Solar Physics Department, Astronomical Institute, Moscow State University, Universitetskii Prospekt 13, Moscow 119992, Russia, email: somov@sai.msu.ru
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Abstract

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Specific features of magnetic reconnection in solar flares are briefly reviewed and illustrated. In particular, the large-scale structure and dynamics of large flares are interpreted in terms of the rainbow reconnection model. The role of the betatron effect in collapsing magnetic traps is considered.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 417 - 424
Copyright
© 2004 International Astronomical Union