Magnetogenesis Scenarios In Cosmological Simulations - Uniform Primordial B0=1nG

One ENZO-MHD cosmological simulation of a comoving 85Mpc^3 volume, saved at z=0. The simulation features a primordial uniform magnetic field seed, 1nG B0=comoving. All datasets are written in HDF5 format, and they represent the physical fields (Gas Density, Temperature, Dark Matter Density, 3D velocity components and 3D magnetic components) on a uniform 1024^3 cartesian grid with uniform spacing. More details of the simulations and on the physical models of magnetism explored here can be found in: https://ui.adsabs.harvard.edu/abs/2021Galax...9..109V/abstract https://ui.adsabs.harvard.edu/abs/2021MNRAS.500.5350V/abstract https://ui.adsabs.harvard.edu/abs/2017CQGra..34w4001V/abstract