Magnetic pinching of hyperbolic flux tubes. I. Basic estimations

被引:103
作者
Titov, VS [1 ]
Galsgaard, K
Neukirch, T
机构
[1] Ruhr Univ Bochum, D-44780 Bochum, Germany
[2] Univ St Andrews, Sch Math & Stat, St Andrews KY16 9SS, Fife, Scotland
关键词
MHD; Sun : corona; Sun : flares; Sun : magnetic fields;
D O I
10.1086/344799
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The concept of hyperbolic flux tubes (HFTs) is a generalization of the concept of separator field lines for coronal magnetic fields with a trivial magnetic topology. An effective mechanism of a current layer formation in HFTs is proposed. This mechanism is called magnetic pinching, and it is caused by large-scale shearing motions applied to the photospheric feet of HFTs in a way as if trying to twist the HFT. It is shown that in the middle of an HFT such motions produce a hyperbolic flow that causes an exponentially fast growth of the current density in a thin force-free current layer. The magnetic energy associated with the current layer that is built up over a few hours is sufficient for a large are. Other implications of HFT pinching for solar flares are discussed as well.
引用
收藏
页码:1172 / 1189
页数:18
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