Observational study of solar magnetic active phenomena

被引:4
作者
Zhang, Honqi [1 ]
机构
[1] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
关键词
Sun : activity; flares; magnetic fields;
D O I
10.1007/BF02702534
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The electric current separated into two parts reflected the quantative properties of heterogeneity and chirality of magnetic field, and defined them as the shear and twist components of current. We analyze the basic configuration and evolution Of superactive region NOAA 6580-6619-6659. It is found that the contribution of the twist component of current cannot be reflected in the normal analysis of the magnetic shear and gradient of the active regions. The observational evidence of kink magnetic ropes generated from the subatmosphere cannot be found completely in some super delta active regions.
引用
收藏
页码:305 / 314
页数:10
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