A Model of Time-Dependent and Non-Local Convection Included in a Stellar Evolution Code
2002 ◽
Vol 185
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pp. 456-457
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AbstractThe Kuhfuß theory of convection is derived from the exact hydrodynamic equations by means of anelastic approximation and diffusion approximation. In the local and time-independent limit the result is identical to the MLT case. In the more general case the theory includes overshooting and convective mixing as well as time-dependence. We present test calculations in a simple box model and first steps toward the implementation in a stellar code.
1991 ◽
Vol 9
(1)
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pp. 26-31
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2009 ◽
1992 ◽
Vol 72
(4)
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pp. 1557-1562
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2002 ◽
Vol 132
(1)
◽
pp. 75-89
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