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

页码：281 / 290

页数：10

共 14 条

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[8] A NEW MULTIPLET TABLE FOR FE-I
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[10] Rubio LRB, 1999, ASTRON ASTROPHYS, V341, pL31

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