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

页码：170 / 177

页数：8

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