Numerical Simulations of Solar and Stellar Convection using the ANTARES code

Details Numerical Simulations of Solar and Stellar Convection using the ANTARES code Numerical Simulations of Solar and Stellar Convection using the ANTARES code

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011eas....44...97m&link_type=abstract

EAS Publications Series, Volume 44, 2011, pp.97-100

Physics

Scientific paper

The ANTARES code (A Numerical Tool for Astrophysical RESearch) is designed for doing 1D, 2D and 3D stellar (radiation-, magneto-) hydrodynamics with realistic microphysics, applying various high-resolution numerical schemes, optionally local grid refinement and works with rectilinear or spherical coordinates. - We present results on turbulent solar granulation flows which have been done in 2D and 3D and comment on our simulations of the pulsation-convection interaction in Cepheid variables, presently 2D.

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