Physics
Scientific paper
Jan 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006coast.147...85d&link_type=abstract
Communications in Asteroseismology, vol. 147, p. 85-88
Physics
7
Scientific paper
Time-Dependent Convection (TDC) models obtained by combining the local treatment of Gabriel (1996) and Grigahcene et al. (2005) and the non-local prescriptions of Spiegel (1963) are presented. We show that in the stationary unperturbed case, these non-local treatments can be constrained by the results of 3D hydrodynamic simulations (Stein & Nordlund 1998). We consider here the case of solar-type stars with a large convective envelope and A-F type stars with two very thin surface convection zones.
Dupret Marc-Antoine
Gabriel Michael
Goupil Marie Jo
Grigahcène A.
Samadi Reza
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