Multi-component magnetic field structure in solar flares

被引：0
|
作者：
Lozitsky, VG [1 ]
Staude, J [1 ]
机构：
[1] Kyiv Univ Astron Observ, UA-04053 Kiev, Ukraine
来源：
SOLAR POLARIZATION 3 | 2003年 / 307卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Stokes I and V profiles of several FeI lines observed in 2 flares have been analyzed. There are hints at the presence of subtelescopic magnetic elements with discrete field strengths of several kG.
引用
收藏
页码：378 / 381
页数：4
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