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Direct Simulations of Radiative and Convective Zones

Published online by Cambridge University Press:  13 January 2006

G. Alecian ,
O. Richard ,
S. Vauclair  and
F. Kupka
F. Kupka*
Affiliation:
Max-Planck-Institute for Astrophysics, Karl-Schwarzschild Str. 1, 85741 Garching, Germany
*
fk@mpa-garching.mpg.de
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Abstract

Numerical simulations have become one of the main tools in the researchon stellar convection zones and they can be expected to become veryimportant for the study of the convection-diffusion interaction as well.In this review, I will first provide some historical background andthen select a few sample problems where numerical simulations of stellarconvection have provided useful results or are expected to do so inthe near future: solar granulation, interacting convection zones, andsemi-convection.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 17: Element Stratification in Stars: 40 Years of Atomic Diffusion , 2005 , pp. 177 - 186
Copyright
© EAS, EDP Sciences, 2005

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