On the inner magnetic field of the sun in the global magnetic cycle

被引：0

作者：

Makarov, VI ^{[1
]}

机构：

[1] Pulkovo Observ, Kislovodsk Solar Stn, Kislovodsk 357700, Russia

来源：

SYNOPTIC SOLAR PHYSICS | 1998年 / 140卷

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：

The structure of the polar corona during the total solar eclipses was analyzed from 1871 to 1995. The depth of the effective magnetic pole (EMP) with the phase of the global magnetic cycle was found. In the epoch of the solar magnetic field reversal the EMP is situated at the depth of 0.5R.. This period corresponds to the maximum activity of the spots. At the minimum activity, the EMP is situated at the depth of 0.7R. and in this time the high polar activity of the Sun is observed. It was shown that the angle between the rotation axis and the magnetic axis of the Sun is 6 degrees.

引用

页码：83 / 87

页数：5

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