On the three-dimensional structure of the solar corona

被引：0
|
作者：
Koutchmy, S
Ershov, AV
Molodenskii, MM
机构：
[1] MOSCOW MV LOMONOSOV STATE UNIV,MOSCOW,RUSSIA
[2] RUSSIAN ACAD SCI,INST EARTH MAGNET IONOSPHERE & RADIOWAVE DISP,TROITSK,RUSSIA
来源：
ASTRONOMICHESKII ZHURNAL | 1996年 / 73卷 / 01期
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Data on the magnetic field of the solar corona on the ''source surface'' are used to construct a model for the surface of zero radial field B-r = 0. Calculations performed for three solar eclipses show that the positions of folds and wrinkles appearing as a result of projection of this surface onto the plane of the sky coincide with helmet streamers observed in the corona.
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页码：125 / 129
页数：5
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