Studies of the solar corona based on solar eclipse observations at IZMIRAN

被引：0
|
作者：
Gulyaev, R. A. [1 ]
机构：
[1] Russian Acad Sci IZMIRAN, Pushkov Inst Terr Magnetism Ionosphere & Radiowav, Troitsk 142190, Moscow Region, Russia
来源：
GEOMAGNETISM AND AERONOMY | 2011年 / 51卷 / 02期
基金：
俄罗斯基础研究基金会;
关键词：
3-DIMENSIONAL STRUCTURE; SHEET;
D O I：
10.1134/S0016793211020071
中图分类号：
P3 [地球物理学]; P59 [地球化学];
学科分类号：
0708 ; 070902 ;
摘要：
From 1945 to 2009, fellows of IZMIRAN participated in 24 expeditions devoted to observations of solar eclipses. The following characteristics of the solar corona were mainly studied: the emission structure, intensity, and polarization; the line and continuous spectra; etc. This paper reviews the most important results, which promoted the development of the present-day concepts of the solar corona structure and physical properties.
引用
收藏
页码：170 / 177
页数：8
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