The depth of the solar convection zone: two models with overshoot.

Details The depth of the solar convection zone: two models with overshoot. The depth of the solar convection zone: two models with overshoot.

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nawg.1996..230s&link_type=abstract

Nachr. Akad. Wiss. Göttingen II, Jahrg. 1996, Nr. 4, p. 230 - 233

Physics

Solar Convective Zone: Numerical Methods, Solar Interior: Convection, Solar Models: Opacities

Scientific paper

Two models of the present Sun are calculated: one with a Los Alamos opacity table, and one with an opacity table form the Lawrence Livermore Laboratory. Both models have a layer of convective overshoot at the base of their outer convection zones, calculated with a non-local version of the mixing-length theory. The total depth of the convection zones in the two models is 0.274 Rsun and 0.286 Rsun, respectively; the second of these values is within the limits set by helioseismic results.

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