Hydrodynamic simulation of the radiation-convection transition region

Details Hydrodynamic simulation of the radiation-convection transition region Hydrodynamic simulation of the radiation-convection transition region

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997assl..225..131k&link_type=abstract

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

Astronomy and Astrophysics

Astrophysics

3

Convection, Sun:Interior, Turbulence

Scientific paper

To study the turbulent convection and the interaction with radiation around the highly super-adiabatic layer (SAL), the Eddington approximation has been employed for the treatment of radiation in the hydrodynamic simulations. The fully compressible hydrodynamics equations, and the equation of radiative transport with Eddington approximation, have been solved, utilizing the ADI technique. The simulation domain of our first test contains about four and a half pressure scale heights around the SAL.

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