Structure and Shape of the Solar Corona during the Total Solar Eclipse on March 29, 2006

被引：5
|
作者：
Pishkalo, M. I. [1 ]
Sadovenko, E. V. [1 ]
机构：
[1] Taras Shevchenko Kyiv Natl Univ, Dept Phys, UA-03127 Kiev, Ukraine
来源：
KINEMATICS AND PHYSICS OF CELESTIAL BODIES | 2008年 / 24卷 / 01期
关键词：
D O I：
10.3103/S0884591308010066
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The structure and the shape of the solar corona during the total solar eclipse on March 29, 2006 were studied. The corona was of the intermediate pre-minimal type, it had northern and southern polar ray systems above the polar coronal holes and six streamers of different brightness in the middle and low heliographic latitudes. All the coronal structural features were found to have counterparts at the photosphere-chromosphere level on the limb and near it. The corona's photometric flattening index was equal to 0.17.
引用
收藏
页码：44 / 50
页数：7
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