Physics
Scientific paper
Aug 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995cophc..89..119w&link_type=abstract
Computer Physics Communications, vol. 89, Issue 1-3, pp.119-126
Physics
11
Scientific paper
A method for calculating energy transfer due to turbulent convection in
self-gravitating radiating spherical flows of general, non-ideal media
is described. A model for time-dependent turbulent convection in stars
due to Kuhfu in its simplest version is discretized on a self-adaptive
grid.
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