Radio observations of gyroresonance emission from coronal magnetic fields

被引：84

作者：

White, SM

Kundu, MR

机构：

[1] University of Maryland,Department of Astronomy

来源：

SOLAR PHYSICS | 1997年 / 174卷 / 1-2期

关键词：

D O I：

10.1023/A:1004975528106

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review the basic characteristics of thermal gyroresonance (also known as cyclotron) emission from solar active regions, and show how radio observations combined with our understanding of the basic mechanism can reveal much of the magnetic and thermal structure of the corona over active regions.

引用

页码：31 / 52

页数：22

共 36 条

[1]

ACHWANDEN MH, 1984, ASTROPHYS J, V426, P425

[2] THE MEASUREMENT OF MAGNETIC-FIELDS IN THE SOLAR ATMOSPHERE ABOVE SUNSPOTS USING GYRORESONANCE EMISSION [J].