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Solar Convection and Mean Flows

Published online by Cambridge University Press:  05 March 2015

Mark S. Miesch*
Affiliation:
HAO/NCAR†, Boulder, CO, 80301 email: [email protected]
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

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