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Magnetohydrodynamic 3-D Models of the Solar Convection Zone

Published online by Cambridge University Press:  30 March 2016

Allan Sacha Brun
Allan Sacha Brun*
Affiliation:
DSM/DAPNIA/SAp, CEA-Saclay, 91191 Gif-sur-Yvette, France

Extract

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We have conducted 3-D simulations of the complex magnetohydrodynamics of the solar convective envelope in spherical shells using our anelastic spherical harmonics (ASH) code (Brun & Toomre 2002). We here briefly discuss the properties of the kinetic and current helicities established in such systems.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 94
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Brun, A.S. & Toomre, J. 2002, ApJ, 570, 865.CrossRefGoogle Scholar
Brun, A.S., Miesch, M.S. & Toomre, J. 2004, ApJ 614, 1073.CrossRefGoogle Scholar
Pevtsov, A.A, Canfield, R.C. & Latushko, S.M. 2001, ApJ, 549, L261.CrossRefGoogle Scholar