Generation of large-scale magnetic fields in young solar-type stars

被引：0
|
作者：
L. L. Kitchatinov
机构：
[1] Russian Academy of Sciences,Institute of Solar
来源：
Astronomy Reports | 2001年 / 45卷
关键词：
Magnetic Field; Evolutionary Stage; Axial Symmetry; Relic Field; Physical Reason;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Differential-rotation and dynamo models are computed for a young, solar-mass star at the initial stage of the formation of its radiative core. It is argued that the global magnetic fields in the radiative zones of the contemporary Sun and similar stars are due to the action of a hydromagnetic dynamo at early evolutionary stages. Our computations suggest that this field should be nonaxisymmetric. Physical reasons for departures from axial symmetry are discussed in detail. It is suggested that nonaxisymmetric relic fields are responsible for the phenomenon of active longitudes.
引用
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页码：816 / 823
页数：7
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