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Helicity-vorticity turbulent pumping of magnetic fields in the solar dynamo

Proceedings of the International Astronomical Union (2012) 8(S294) 367-368
DOI: 10.1017/S1743921313002780
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Abstract

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. © International Astronomical Union 2013.

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Pipin, V. V. (2012). Helicity-vorticity turbulent pumping of magnetic fields in the solar dynamo. In Proceedings of the International Astronomical Union (Vol. 8, pp. 367–368). https://doi.org/10.1017/S1743921313002780

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