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Results from 2-D Numerical Simulations of Solar Granules
Published online by Cambridge University Press: 08 February 2017
Extract
We have carried out detailed numerical simulations of solar granular convection cells of different horizontal dimension. The calculations account for the basic physics of compressible convection, including the ionization of H I, He I and He II, and H2 molecule formation as well as non-local, multi-dimensional radiative transfer (grey approximation in LTE). A more detailed description of the simulations has been given by Steffen and Muchmore (1988) and by Steffen et al. (1989).
- Type
- IV. Magnetohydrodynamics of the Photosphere
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- Copyright © Kluwer 1990