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Helicity–vorticity turbulent pumping of magnetic fields in the solar dynamo
2012
Proceedings of the International Astronomical Union
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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.
doi:10.1017/s1743921313002780
fatcat:xyma5dgavfdfhea2xq45lyqttq