A 'fast' model of the solar convection zone

Details A 'fast' model of the solar convection zone A 'fast' model of the solar convection zone

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....91..356b&link_type=abstract

Astronomy and Astrophysics, vol. 91, no. 3, Nov. 1980, p. 356-359.

Astronomy and Astrophysics

Astrophysics

3

Convection Currents, Solar Oscillations, Stellar Models, Computer Programs, Mixing Length Flow Theory, Run Time (Computers)

Scientific paper

A model of solar convection zone incorporates the mixing-length theory in the method developed by Faulkner (1965) which accurately represents the superadiabatic layers. Interpolation formulas which save computer time, and are sufficiently accurate to limit discrepancies in pressure distribution and density through the convection zone, are used; the computer programs are 20 times faster than the programs of Baker and Temesvary (1966).

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