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

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

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..271..403t&link_type=abstract

Astrophysical Dynamics: From Stars to Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 271,

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Computation

Convection, Hydrodynamics, Radiative Transfer, Sun: Interior

Scientific paper

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.

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