The theory and numerical simulation of non-local mixing-length convection.
Local convection theory makes the unphysical prediction that turbulent mixing terminates at the Schwarzschild stability boundary, and existing non-local convection theories have been criticized by Renzini (1987). Since the size of convecting cores bears upon stellar structure and evolution, a self-c...
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| Language: | en |
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The University of Arizona.
1992
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| Online Access: | http://hdl.handle.net/10150/185821 |