Three-dimensional simulations of solar magneto-convection including effects of partial ionization
In recent decades, REALISTIC three-dimensional radiative-magnetohydrodynamic simulations have become the dominant theoretical tool for understanding the complex interactions between the plasma and magnetic field on the Sun. Most of such simulations are based on approximations of magnetohydrodynamics, without directly considering the consequences of
Khomenko, E. et al.
Fecha de publicación:
10
2018