Title of article :
Computing turbulent flows driven by Rayleigh-Taylor and Richtmyer-Meshkov instabilities
Author/Authors :
Zhou، Y. C. نويسنده , , Rubinstein، R. نويسنده , , Eliason، D. نويسنده , , Cabot، W. نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2003
Pages :
-378
From page :
379
To page :
0
Abstract :
We develop a two-scale turbulence model for turbulent mix induced by Rayleigh-Taylor and Richtmyer-Meshkov instabilities. In this model, the large scales are dominated by production by instability mechanisms, while small scales satisfy Kolmogorov dynamics. The model allows transfer rates in the two spectral regions to be unequal. Constraints on model coefficients that permit relaxation to a unique self-similar state in free decay and self-similar growth are derived.
Keywords :
turbulence , Supernovae , general , instabilities , stars
Journal title :
Astronomy and Astrophysics
Serial Year :
2003
Journal title :
Astronomy and Astrophysics
Record number :
76602
Link To Document :
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