Simulations of the Quiet Sun Magnetic Field: From the Upper Convection Zone into the Corona

Details Simulations of the Quiet Sun Magnetic Field: From the Upper Convection Zone into the Corona Simulations of the Quiet Sun Magnetic Field: From the Upper Convection Zone into the Corona

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spd....37.0701a&link_type=abstract

American Astronomical Society, SPD meeting #37, #7.1; Bulletin of the American Astronomical Society, Vol. 38, p.227

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the latest in a series of simulationsdesigned to directly investigate whether the magneticfield generated by a convective dynamo in the upperconvection zone can account for the observedproperties of the Quiet Sun magnetic field andatmosphere. The simulations are performed usinga new numerical code capable of evolving a modelsolar atmosphere that extends from the upper convectionzone into the low corona. This code is a parallel,semi-implicit solver capable of accomodating thespatial and temporal disparities intrinsic to thiscombined system.

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