Near-surface constraints on the structure of stellar convection zones

Details Near-surface constraints on the structure of stellar convection zones Near-surface constraints on the structure of stellar convection zones

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997assl..225...73t&link_type=abstract

SCORe'96 : Solar Convection and Oscillations and their Relationship, Proceedings of a workshop, held in Aarhus, Denmark, May 27

Physics

12

Solar Physics, Convection, Hydrodynamics

Scientific paper

By simulating the convection in the upper layers of six different stars
and matching these simulations to 1D-mixing length models using the same
input physics, we have been able to infer the behaviour of the
mixing-length parameter, $\alpha$, as the stellar parameters changes.

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