Flux-Transport Solar Dynamos

被引:46
作者
Dikpati, Mausumi [1 ]
Gilman, Peter A. [1 ]
机构
[1] HAO NCAR, Boulder, CO 80301 USA
关键词
Solar activity; Dynamo; Meridional circulation; UPPER CONVECTION ZONE; SUNS MAGNETIC FIELD; MERIDIONAL FLOW; DIFFERENTIAL ROTATION; TORSIONAL OSCILLATIONS; FREQUENCY SPLITTINGS; CIRCULATION; TACHOCLINE; MODELS; VELOCITY;
D O I
10.1007/s11214-008-9484-3
中图分类号
P1 [天文学];
学科分类号
070403 [天体物理学];
摘要
Large-scale solar dynamo models were first built by Parker (1955). Over the past half a century these models have evolved significantly. We discuss here the development of a class of large-scale dynamo models which include, along with the alpha-effect and Omega-effect, an important third process, flux transport by meridional circulation. We present the properties of this 'flux-transport' dynamo, including the crucial role meridional circulation plays in giving this dynamo predictive power.
引用
收藏
页码:67 / 75
页数:9
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