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

Published online by Cambridge University Press:  18 July 2013

V. V. Pipin
V. V. Pipin*
Affiliation:
Institute Solar-Terrestrial Physics, Irkutsk, Russia email: pip@iszf.irk.ru
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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.

Keywords

TurbulenceMean-field magnetohydrodynamicsSunmagnetic fieldStars: Dynamo activity
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 

References

Brandenburg, A., Rädler, K.-H., & Kemel, K. 2012, Astron. Astrophys., 539, A35 CrossRefGoogle Scholar
Leprovost, N. & Kim, E.-J. 2010, Geophysical and Astrophysical Fluid Dynamics, 104, 167 CrossRefGoogle Scholar
Mitra, D., Käpylä, P. J., Tavakol, R., & Brandenburg, A. 2009, Astron. Astrophys., 495, 1 CrossRefGoogle Scholar
Pipin, V. V. 2008, Geophysical and Astrophysical Fluid Dynamics, 102, 21 CrossRefGoogle Scholar
Rogachevskii, I., Kleeorin, N., Käpylä, P. J., & Brandenburg, A. 2011, Phys. Rev. E, 84, 056314 CrossRefGoogle Scholar