Radiative MHD Modeling of Sunspot Fine Structure

Details Radiative MHD Modeling of Sunspot Fine Structure Radiative MHD Modeling of Sunspot Fine Structure

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..415..351r&link_type=abstract

The Second Hinode Science Meeting: Beyond Discovery-Toward Understanding ASP Conference Series, Vol. 415, proceedings of a meeti

Astronomy and Astrophysics

Astronomy

1

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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