Solar models with strong turbulence

Details Solar models with strong turbulence Solar models with strong turbulence

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.202...77c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 202, no. 1, p. 77-80.

Physics

Magnetohydrodynamic Turbulence, Solar Physics, Stellar Models, Turbulence Models, Mixing Length Flow Theory, Numerical Integration

Scientific paper

A series of evolutionary models for the sun were constructed using the strong turbulence model of the variable mixing-length theory (AMLT) of Canuto (1990). The present values of the solar model were obtained by an initial composition X = 0.754, Z = 0.019, and alpha(x) = 1.1. The physical variables which were obtained by applying the strong turbulence case of AMLT were similar to those of weak turbulence model (Kiziloglu and Civelek, 1992) if we focused on the fitting of the present solar radius and luminosity.

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