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3D-simulations of convection in stellar atmospheres, with emphasis on
realistic input physics.
- The MHD equation of state (Mihalas, Hummer & Däppen)
- The state of art opacities
- Numerical diffusion, capable of handling supersonic flows
- Anders & Grevesse 1989 abundances
- Two grid-resolutions;
and
-
Regner Trampedach
Sat Jan 4 22:47:01 MET 1997