Solar Magneto-Convection Simulations

Details Solar Magneto-Convection Simulations Solar Magneto-Convection Simulations

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.0401s&link_type=abstract

American Astronomical Society, SPD meeting #40, #4.01; Bulletin of the American Astronomical Society, Vol. 41, p.810

Astronomy and Astrophysics

Astronomy

Scientific paper

We present preliminary results of magneto-convection simulations of the rise of initially horizontal magnetic flux from 20 Mm deep through the solar surface in a domain 48 Mm wide. The magnetic field is stretched upward in the diverging upflows and pulled down in the downdrafts which produces a hierarchy of loop like structures. The strength varies with depth as the square root of the density. The field is swept to the boundaries of small supergranular like structures to form a magnetic network.

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