Radiative MHD Simulations of Sunspot Structure-Challenges and recent developments

Details Radiative MHD Simulations of Sunspot Structure-Challenges and recent developments Radiative MHD Simulations of Sunspot Structure-Challenges and recent developments

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1171..315r&link_type=abstract

RECENT DIRECTIONS IN ASTROPHYSICAL QUANTITATIVE SPECTROSCOPY AND RADIATION HYDRODYNAMICS: Proceedings of the International Confe

Computer Science

Numerical Analysis

Radiative Transfer, Magnetohydrodynamics, Numerical Analysis, Radiative Transfer, Scattering, Magnetohydrodynamics And Plasmas, Numerical Approximation And Analysis

Scientific paper

For a long time 3D radiative MHD simulations of sunspots were out of reach. With increasing computing power there has been recently substantial progress in modeling magneto-convection in strong magnetic field regions and complete sunspots including the transition from umbra toward plage like solar granulation. 3D simulations point toward a unified understanding of sunspot fine structure in terms of a magneto convection process in a background field with varying inclination angle. We summarize here briefly the most recent developments.

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