Approximation models of the solar convective zone on the basis of modifications of mixing length theory

Details Approximation models of the solar convective zone on the basis of modifications of mixing length theory Approximation models of the solar convective zone on the basis of modifications of mixing length theory

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...21a&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, July-Aug. 1986, p. 21-26. In Russian.

Physics

3

Convective Heat Transfer, Mixing Length Flow Theory, Solar Physics, Stellar Models, Approximation, Atmospheric Models, Energy Transfer, Flow Velocity, Solar Atmosphere, Vertical Motion

Scientific paper

Modifications of mixing length theory are used to obtain approximation models of the solar convective zone which agree with the HOLMU and VAL 80 empirical models of the solar atmosphere at the outer boundary, and with the Abraham-Iben (1971) model of the internal solar structure at the inner boundary. Limits on the ascent velocity of convective elements are imposed in accordance with observations.

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