Radiative-MHD Simulations of Sunspot Structure

Details Radiative-MHD Simulations of Sunspot Structure Radiative-MHD Simulations of Sunspot Structure

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..416..461r&link_type=abstract

Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology: GONG 2008/SOHO 21 ASP Conference Series, Vol. 416, proceedings

Astronomy and Astrophysics

Astronomy

1

Scientific paper

For a long time 3D numerical 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. We summarize here briefly the most recent developments and discuss future directions.

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