Thermal-magnetic relation of a sunspot as inferred from the inversion of 1.5μm spectral data

被引：0

作者：

Mathew, SK ^{[1
]}

Solanki, SK ^{[1
]}

Lagg, A ^{[1
]}

Krupp, N ^{[1
]}

Woch, J ^{[1
]}

Collados, M ^{[1
]}

Berdyugina, S ^{[1
]}

Frutiger, C ^{[1
]}

机构：

[1] Max Planck Inst Aeron, D-37191 Katlenburg Lindau, Germany

来源：

SOLMAG 2002: PROCEEDINGS OF THE MAGNETIC COUPLING OF THE SOLAR ATMOSPHERE EUROCONFERENCE AND IAU COLLOQUIUM 188 | 2002年 / 505卷

关键词：

sunspots : magnetic field; spectropolarimetry : infra-red;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the thermal-magnetic relation in a simple, isolated sunspot deduced from the inversion of 1.56 mum spectropolarimetric data. Due to the high Zeeman sensitivity of the g = 3, Fe 1 1.5648 mum line, we can study this relationship in the entire sunspot. An inversion technique based on response functions is used to derive various parameters, both as a function of location within the sunspot and of height in the atmosphere. In this paper we attempt to relate field strength, vertical and radial field components and the field inclination with temperature.

引用

页码：501 / 503

页数：3

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