no code implementations • 26 Nov 2020 • Fan Zhang, Stefaan Poedts, Andrea Lani, Błażej Kuźma, Kris Murawski
In the present numerical simulations, the initial density is specified to reach hydrostatic equilibrium, and as a comparison, chemical equilibrium is also taken into account to provide a density profile that differs from typical hydrostatic equilibrium profiles.
Plasma Physics Solar and Stellar Astrophysics
