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Helicity–vorticity turbulent pumping of magnetic fields in the solar dynamo
Published online by Cambridge University Press: 18 July 2013
Abstract
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The interaction of helical convective motions and differential rotation in the solar convection zone results in turbulent drift of a large-scale magnetic field. We discuss the pumping mechanism and its impact on the solar dynamo.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S294: Solar and Astrophysical Dynamos and Magnetic Activity , August 2012 , pp. 367 - 368
- Copyright
- Copyright © International Astronomical Union 2013
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