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arXiv · 1211.6253

Solar magneto-convection

Manfred Schüssler
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Abstract

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.

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Manfred Schüssler. 2012-11-27. Solar magneto-convection. https://doi.org/10.1017/s1743921313002329

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