Turbulent convection with overshooting - Reynolds stress approach

Details Turbulent convection with overshooting - Reynolds stress approach Turbulent convection with overshooting - Reynolds stress approach

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...392..218c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 392, no. 1, June 10, 1992, p. 218-232.

Statistics

Methodology

80

Convective Flow, Magnetohydrodynamic Turbulence, Reynolds Stress, Stellar Structure, Accretion Disks, Stellar Interiors, Stellar Models

Scientific paper

The Reynolds stress formalism is adopted to treat turbulent convection. This methodology is reviewed, and it is suggested that it may prove very useful to treat stellar and accretion disk turbulent convection, as well as in the construction of the subgrid models needed in large eddy simulations. A set of differential equations that yield the mean and turbulent quantities such as convective fluxes, turbulent viscosity, and turbulent conductivity is presented.

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