TURBULENT TRANSPORT OF MAGNETIC-FIELDS AND THE SOLAR DYNAMO

被引：0
|
作者：
KITCHATINOV, LL
机构：
来源：
COSMIC DYNAMO | 1993年 / 157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：
The effect of anisotropic transport of the mean magnetic field by turbulence in a stratified rotating fluid is briefly discussed to find its qualitative correspondence to the observed field redistribution over a solar cycle. A kinematic model of a dynamo in a spherical shell is developed with the transport effect included to assess its importance in a more consistent way. The anisotropic transport brings the simulated field behavior closer to that observed on the Sun.
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页码：13 / 17
页数：5
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