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On long-duration 3D simulations of stellar convection using ANTARES

Published online by Cambridge University Press:  03 March 2020

F. Kupka ,
D. ,
Fabbian ,
D. ,
Krüger ,
N. ,
Kostogryz ,
L.  and
Gizon
F. Kupka
Affiliation:
Institut für Astrophysik Göttingen, Georg-August-Universität Göttingen, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany email: [email protected]
Fabbian
Affiliation:
Institut für Astrophysik Göttingen, Georg-August-Universität Göttingen, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany email: [email protected]
Krüger
Affiliation:
Institut für Astrophysik Göttingen, Georg-August-Universität Göttingen, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany email: [email protected] Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany Fakultät für Mathematik, Universität Wien, Oskar-Morgenstern-Platz 1, 1090 Wien, Österreich
Kostogryz
Affiliation:
Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany
Gizon
Affiliation:
Institut für Astrophysik Göttingen, Georg-August-Universität Göttingen, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany email: [email protected] Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany
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Abstract

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We present initial results from three-dimensional (3-D) radiation hydrodynamical simulations for the Sun and targeted Sun-like stars. We plan to extend these simulations up to several stellar days to study p-mode excitation and damping processes. The level of variation of irradiance on the time scales spanned by our 3-D simulations will be studied too. Here we show results from a first analysis of the computational data we produced so far.

Keywords

Convectionhydrodynamicsradiative transferSun: oscillationsstars: oscillations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium A30: Astronomy in Focus XXX , August 2018 , pp. 373 - 376
Copyright
© International Astronomical Union 2020

References

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