Flux-transport solar dynamos

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.

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An edited version of this paper was published by Springer. Copyright 2009, Springer Science+Business Media B.V.
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Author Dikpati, Mausumi
Gilman, Peter A.
Publisher UCAR/NCAR - Library
Publication Date 2009-01-17T00:00:00
Digital Object Identifier (DOI) Not Assigned
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Topic Category geoscientificInformation
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Metadata Date 2025-07-17T15:54:16.316683
Metadata Record Identifier edu.ucar.opensky::articles:15291
Metadata Language eng; USA
Suggested Citation Dikpati, Mausumi, Gilman, Peter A.. (2009). Flux-transport solar dynamos. UCAR/NCAR - Library. https://n2t.org/ark:/85065/d7t154pf. Accessed 23 August 2025.

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