TL;DR
This paper reviews recent advances in simulating solar magneto-convection, highlighting how comprehensive models have improved understanding of magnetic structures and dynamics in the Sun's surface layers.
Contribution
It provides an overview of recent simulation developments covering various solar magnetic phenomena, integrating high-resolution observations to enhance understanding.
Findings
Simulations now encompass entire active regions and small-scale magnetic features.
Breakthroughs in understanding magnetic field structures in the solar photosphere.
Enhanced correlation between simulations and high-resolution observations.
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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