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Turbulent Convection: Comparing the Moment Equations to Numerical Simulations

Published 1999 October 22 © 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation F. Kupka 1999 ApJ 526 L45 DOI 10.1086/312363

1538-4357/526/1/L45

Abstract

The nonlocal hydrodynamic moment equations for compressible convection are compared to numerical simulations. Convective and radiative flux typically deviate less than 20% from the three-dimensional simulations, while mean thermodynamic quantities are accurate to at least 2% for the cases we have investigated. The moment equations are solved in minutes rather than days as required on standard workstations. We conclude that this convection model has the potential to considerably improve the modeling of convection zones in stellar envelopes and cores, in particular those of A and F stars.

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10.1086/312363