期刊
SPACE SCIENCE REVIEWS
卷 144, 期 1-4, 页码 67-75出版社
SPRINGER
DOI: 10.1007/s11214-008-9484-3
关键词
Solar activity; Dynamo; Meridional circulation
资金
- NASA [NNH05AB521]
- ISSI
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.
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