Title of article
Large-scale reconnection in a large flare Original Research Article
Author/Authors
B.V. Somov، نويسنده , , T. Kosugi، نويسنده , , I.V. Oreshina، نويسنده , , G.P. Lyubimov، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2005
Pages
11
From page
1712
To page
1722
Abstract
Some specific features of the large-scale magnetic reconnection in large solar flares are briefly reviewed. In particular, the large-scale structure and dynamics of the 3B/X5.7 flare on 14 July 2000 are interpreted in terms of the topological model. The role of the betatron effect in collapsing magnetic traps, that are created by reconnection in the solar corona, is considered. We discuss some possibilities to observe the collapsing trap acceleration in solar flares.
Keywords
Flares , Acceleration of particles , X-rays , Sun , Magnetic fields
Journal title
Advances in Space Research
Serial Year
2005
Journal title
Advances in Space Research
Record number
1130187
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