Configuration of the magnetic field in solar active regions

被引：0
|
作者：
Zhang, HQ
机构：
[1] Beijing Astronomical Observatory,
[2] Chinese Academy of Sciences,undefined
来源：
SOLAR PHYSICS | 1997年 / 174卷 / 1-2期
关键词：
Atmosphere; Magnetic Field; Active Region; Solar Atmosphere; Astronomical Observatory;
D O I：
10.1023/A:1004975407745
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper we present the observational results of chromospheric and photospheric magnetograms in active regions obtained at the Huairou Solar Observing Station of the Beijing Astronomical Observatory. Simultaneous observations of the chromospheric and photospheric magnetic fields enable us to construct a possible configuration of the magnetic field in the solar atmosphere. The chromospheric magnetic field shows more diffusion than the photospheric magnetic field and consists of fibril-like features. We also discuss the possible configuration of the magnetic shear in highly sheared active regions.
引用
收藏
页码：219 / 227
页数：9
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