Large-scale electric fields in solar flare regions

被引:9
|
作者
Pudovkin, MI [1 ]
Zaitseva, SA
Shumilov, NO
Meister, CV
机构
[1] St Petersburg State Univ, Inst Phys, St Petersburg 198904, Russia
[2] Univ Potsdam, Inst Theoret Phys & Astrophys, D-14469 Potsdam, Germany
基金
俄罗斯基础研究基金会;
关键词
D O I
10.1023/A:1004943102679
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A method of separating electric field in the flare region in the potential and vortex (induced) parts is discussed. According to the proposed model, the motion of flare ribbons from the central line of the Bare region is caused by the vortex component of the coronal electric field, while the motion of bright spots within the flare region towards the central line is driven by the potential component of that field. The intensity of both the components of the flare region electric field is estimated to equal approximately 1-3 V cm(-1), which provides the input of the electromagnetic energy into the active region at a rate of about 10(10) erg cm(-2) s(-1).
引用
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页码:125 / 136
页数:12
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