Physics
Scientific paper
Apr 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ssrv..144...67d&link_type=abstract
Space Science Reviews, Volume 144, Issue 1-4, pp. 67-75
Physics
10
Solar Activity, Dynamo, Meridional Circulation
Scientific paper
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 α-effect and Ω-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.
Dikpati Mausumi
Gilman Peter A.
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