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Towards understanding the global magnetism of the Sun and solar-like stars

Published online by Cambridge University Press:  26 February 2010

Allan Sacha Brun
Allan Sacha Brun*
Affiliation:
DSM/IRFU/SAp & UMR AIM, CEA-CNRS-Université of Paris 7, France
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Abstract

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The Sun and solar-like stars possess intense and cyclic magnetic activity. In order to understand how this comes about we have developed series of 2-D and 3-D models in order to simulate their global dynamics and magnetism. We here report on our latest findings.

Keywords

Sun: activityinteriormagnetic fieldsstars: activityconvectionMHDturbulence
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S264: Solar and Stellar Variability: Impact on Earth and Planets , August 2009 , pp. 161 - 170
Copyright
Copyright © International Astronomical Union 2010

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