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Solar magneto-convection

Published online by Cambridge University Press:  18 July 2013

Manfred Schüssler
Manfred Schüssler*
Affiliation:
Max-Planck-Institut für Sonnensystemforschung 37191 Katlenburg-Lindau, Germany
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Abstract

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An overview is given about recent developments and results of comprehensive simulations of magneto-convective processes in the near-surface layers and photosphere of the Sun. Simulations now cover a wide range of phenomena, from whole active regions, over individual sunspots and pores, magnetic flux concentrations and vortices in intergranular lanes, down to the intricate mixed-polarity structure of the magnetic field generated by small-scale dynamo action. The simulations in concert with high-resolution observations have provided breakthroughs in our understanding of the structure and dynamics of the magnetic fields in the solar photosphere.

Keywords

Sun: magnetic fieldsSun: photosphereconvection(magnetohydrodynamics:) MHD
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S294: Solar and Astrophysical Dynamos and Magnetic Activity , August 2012 , pp. 95 - 106
Copyright
Copyright © International Astronomical Union 2013 

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