The effect of atomic polarization on early estimates of prominence magnetic field strengths

被引：4

作者：

Brown, A ^{[1
]}

Ariste, AL ^{[1
]}

Casini, R ^{[1
]}

机构：

[1] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA

来源：

SOLAR PHYSICS | 2003年 / 215卷 / 02期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1023/A:1025656323640

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this paper we present our results of the application of the magnetograph formula to synthetic Stokes V profiles in prominences. We investigate both the Zeeman and atomic-polarization signatures within the V profile and question why previous attempts to determine magnetic field strength, on average, were correct, even if the magnetograph formula does not apply in general.

引用

页码：295 / 305

页数：11

共 21 条

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