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Using simulations of solar surface convection as boundary conditions on global simulations

Published online by Cambridge University Press:  12 August 2011

Regner Trampedach  and
Kyle Augustson
Regner Trampedach
Affiliation:
JILA, University of Colorado, 440 UCB, Boulder, CO 80309-0440, U.S.A. email: [email protected], [email protected]
Kyle Augustson
Affiliation:
JILA, University of Colorado, 440 UCB, Boulder, CO 80309-0440, U.S.A. email: [email protected], [email protected]
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Abstract

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Direct numerical simulations of convective stellar envelopes, are divided between two different physical regimes, that are rather difficult to reconcile — at least with the computational power of present-day computers. This paper outlines an attempt at bridging the gap between surface and interior simulations of convection.

Keywords

convectionhydrodynamicsradiative transferSun: interior
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S271: Astrophysical Dynamics: From Stars to Galaxies , June 2010 , pp. 403 - 404
Copyright
Copyright © International Astronomical Union 2011