Beyond mixing-length theory in convection

Details Beyond mixing-length theory in convection Beyond mixing-length theory in convection

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mmsai..55..293d&link_type=abstract

(European Physical Society, Ministero della Pubblica Istruzione, and Universita di Catania, EPS Study Conference on Oscillations

Astronomy and Astrophysics

Astronomy

Convection, Mixing Length Flow Theory, Solar Oscillations, Amplitudes, Closure Law, Solar Interior, Stellar Structure, Turbulence

Scientific paper

There currently exists no practical theory of the coupling between solar nonradial pulsations and convection. An attempt is presently made to formulate a theory of convection sufficiently easy to perturb so that its application to the solar case will yield the requisite statistical data on the amplitudes and coherence times of the solar oscillations. Viewed as an inverse problem, the theory will also put constraints on the structure and behavior of the solar interior.

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