M Modestov, E Khomenko, N Vitas, A de Vicente, A Navarro, P A González-Morales, M Collados, T Felipe, D Martínez-Gómez, P Hunana, M Luna, M Koll Pistarini, B Popescu Braileanu, A Perdomo García, V Liakh, I Santamaria, M M Gomez Miguez
The Mancha3D code is a versatile tool for numerical simulations of magnetohydrodynamic (MHD) processes in solar/stellar atmospheres. The code includes nonideal physics derived from plasma partial ionization, a realistic equation of state and radiative transfer, which allows performing high-quality realistic simulations of magnetoconvection, as well as idealized simulations of particular processes, such as wave propagation, instabilities or energetic events. The paper summarizes the equations and methods used in the Mancha3D (Multifluid (-purpose -physics -dimensional) Advanced Non-ideal MHD Code for High resolution simulations in Astrophysics 3D) code...
2024: Solar Physics