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Modelling of solar granulation

Published online by Cambridge University Press:  01 August 2006

H. J. Muthsam ,
B. Löw-Baselli ,
Chr. Obertscheider ,
M. Langer ,
P. Lenz  and
F. Kupka
H. J. Muthsam
Affiliation:
Institute of Mathematics, University of Vienna, Nordbergstrasse 15, A-1090 Vienna, Austria email: [email protected]
B. Löw-Baselli
Affiliation:
Institute of Mathematics, University of Vienna, Nordbergstrasse 15, A-1090 Vienna, Austria email: [email protected]
Chr. Obertscheider
Affiliation:
Institute of Mathematics, University of Vienna, Nordbergstrasse 15, A-1090 Vienna, Austria email: [email protected]
M. Langer
Affiliation:
Institute of Mathematics, University of Vienna, Nordbergstrasse 15, A-1090 Vienna, Austria email: [email protected]
P. Lenz
Affiliation:
Institute of Mathematics, University of Vienna, Nordbergstrasse 15, A-1090 Vienna, Austria email: [email protected] Institute for Astronomy, University of Vienna, Türkenschanzstrasse 17, A-1180 Vienna, Austria
F. Kupka
Affiliation:
Max-Planck-Institute for Astrophysics, Karl-Schwarzschild-Strasse 1, D-85741 Garching, Germany
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Abstract

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We present the essential features of the ANTARES code. ANTARES has been developed to perform the simulation of astrophysical flows in one, two, or three dimensions. Using, in particular, the option of grid refinement, we present results for solar granulation achieved at very high spatial resolution.

Keywords

Sun: granulationconvectionhydrodynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S239: Convection in Astrophysics , August 2006 , pp. 89 - 91
Copyright
Copyright © International Astronomical Union 2007

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