The 3D MHD code GOEMHD3 for astrophysical plasmas with large Reynolds numbers
The 3D MHD code GOEMHD3 for astrophysical plasmas with large Reynolds numbers
The numerical simulation of turbulence and flows in almost ideal, large-Reynolds-number astrophysical plasmas motivates the implementation of almost conservative MHD computer codes. They should efficiently calculate, use highly parallelized schemes scaling well with large numbers of CPU cores, allows to obtain a high grid resolution over large simulation domains and …