Opacity for realistic 3D MHD simulations of cool stellar atmospheres
Context. Realistic three-dimensional time-dependent simulations of stellar near-surface convection employ the opacity binning method for the efficient and accurate computation of the radiative energy exchange. The method provides several orders of magnitude of speedup, but its implementation includes a number of free parameters. Aims: Our aim is to
Perdomo García, A. et al.
Fecha de publicación:
7
2023