On the topological trigger of large eruptive solar flares

被引：5
|
作者：
Somov, B. V. [1 ]
机构：
[1] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119992, Russia
来源：
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2008年 / 34卷 / 09期
基金：
俄罗斯基础研究基金会;
关键词：
Sun; solar flares; magnetic reconnection; particle acceleration; X-ray emission;
D O I：
10.1134/S1063773708090065
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The possibility of studying the topological properties of the magnetic fields in solar active regions is considered in terms of simple models. Analysis of the field topology shows that the topological trigger effect should be taken into account when large eruptive flares are modeled.
引用
收藏
页码：635 / 645
页数：11
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