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Solar Convection and Mean Flows

Published online by Cambridge University Press:  05 March 2015

Mark S. Miesch
Mark S. Miesch*
Affiliation:
HAO/NCAR†, Boulder, CO, 80301 email: miesch@ucar.edu
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Abstract

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We briefly review our current understanding of how the solar differential rotation and meridional circulation are maintained, which has important implications for understanding cyclic magnetic activity in the Sun and stars.

Keywords

Sun: rotationSun: interiorSun: activitystars: rotationstars: interiorsstars: activityconvectionMHD
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 92 - 93
Copyright
Copyright © International Astronomical Union 2015 

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