Mathematics
Scientific paper
Jul 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981nassp.450..253m&link_type=abstract
In NASA. Goddard Space Flight Center The Sun as a Star p 253-262 (SEE N81-27008 17-90)
Mathematics
2
Compressible Flow, Convection Currents, Convective Flow, Gas Dynamics, Solar Granulation, Surface Layers, Convective Heat Transfer, Flow Theory, Mathematical Models, Navier-Stokes Equation, Stellar Structure, Sun, Thermal Diffusion
Scientific paper
The current state of understanding of the most directly observable solar convection, the granulation and supergranulation is summarized. The body of work in which the complete time dependent Navier-Stokes equations and entropy transport equation are solved for a fully compressible atmosphere is considered. Relevant anelastic and incompressible calculations in two dimensions are also discussed.
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