Applications of magnetic line ratio method to magnetographic observations of large-scale solar magnetic fields

被引：0
|
作者：
Veretsky, RM [1 ]
Demidov, ML [1 ]
机构：
[1] Inst Solar Terr Phys, Irkutsk 664033, Russia
来源：
SOLAR-TERRESTRIAL MAGNETIC ACTIVITY AND SPACE ENVIRONMENT | 2002年 / 14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：
We interpret Measurements of the large-scale magnetic field strength, obtained with the magnetograph of the STOP telescope at the Sayan observatory, in terms of a two-component model. Theoretical magnetic field strength ratios for used spectral lines are calculated. For this purpose, the Stokes-V parameters are derived by solving the radiative transfer equations for four flux tube models. By means of a comparison of experimental data and theoretical data, estimates of the "true values" and the gradients of the magnetic field strength are obtained.
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页码：71 / 73
页数：3
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