Inversion of Stokes profiles

被引：0
|
作者：
Frutiger, C [1 ]
Solanki, SK [1 ]
Fligge, M [1 ]
Bruls, JHMJ [1 ]
机构：
[1] ETH Zentrum, Inst Astron, CH-8092 Zurich, Switzerland
来源：
SOLAR POLARIZATION | 1999年 / 243卷
关键词：
flux tubes; polarization; radiative transfer; response functions;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present inversions based on two different flux-tube models, both of which reproduce the Stokes I and V profiles obtained in active region plages with high accuracy, including the V profile asymmetry. One model is almost identical to that employed by Bellot Rubio et al. (1997, 1999), and results in a significant downflow within the flux tube. The other, although similar in most respects, has mass conservation enforced inside the flux-tubes components.
引用
收藏
页码：281 / 290
页数：10
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