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Rotation and magnetism of solar-like stars: from scaling laws to spot-dynamos

Published online by Cambridge University Press:  07 August 2014

Allan Sacha Brun
Allan Sacha Brun*
Affiliation:
AIM-IRFU/SAp, CEA/CNRS/University of Paris 7, CEA-Saclay, 91191 Gif-sur-Yvette, France email: [email protected]
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Abstract

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The Sun is the archetype of magnetic star and its proximity coupled with very high accuracy observations has helped us understanding how solar-like stars (e.g with a convective envelope) redistribute angular momentum and generate a cyclic magnetic field. However most solar models have been so fine tuned that when they are applied to other solar-like stars the agreement with observations is not good enough. I will thus discuss, based on theoretical considerations and multi-D MHD stellar models, what can be considered as robust properties of solar-like star dynamics and magnetism and what is still speculative. I will derive scaling laws for differential rotation and magnetic energy as a function of stellar parameters, discuss recent results of stellar dynamo models and define the new concept of spot-dynamo, e.g. global dynamo that develops self-consistent magnetic buoyant structures that emerge at the surface.

Keywords

Sun: convectionrotationmagnetismdynamostellar magnetism and rotation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S302: Magnetic Fields throughout Stellar Evolution , August 2013 , pp. 114 - 125
Copyright
Copyright © International Astronomical Union 2014 

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