Turbulent compressible convection

Details Turbulent compressible convection Turbulent compressible convection

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...370..282c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 370, March 20, 1991, p. 282-294.

Astronomy and Astrophysics

Astrophysics

211

Compressible Flow, Free Convection, Late Stars, Magnetohydrodynamic Turbulence, Stellar Interiors, Stellar Motions, Astronomical Spectroscopy, Statistical Analysis, Stellar Evolution, Stellar Models, Transport Properties

Scientific paper

Numerical simulations with high spatial resolution (up to 96-cubed
gridpoints) are used to study three-dimensional, compressible
convection. A sequence of four models with decreasing viscous
dissipation is considered in studying the changes in the flow structure
and transport properties as the convection becomes turbulent.

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