E3A, AMR8 at z=0.02, reconstructed down to the 7th AMR level (7.9kpc/cell)

Each HDF5 dataset contains triplets of fields: -7_8mdm001R_dt_015 contains "Density", "Dark_Matter_Density" and "Temperature" (a 512^3 grid for each); -7_8mdm001R_v_015 contains "x-velocity", "y-velocity" and "z-velocity" gas velocity fields (a 512^3 grid for each); -7_8mdm001R_b_015 contains "Bx", "By" and "Bz" - the components of the magnetic field (a 512^3 grid for each). All values must be *multiplied* by the following conversion factors in order to get them in CGS units, given in the corresponding *conv2 files, in which the 3rd entry is the redshift (z), the 4th (convd) entry gives the conversion to have Density and Dark_Matter_Density in g/cm^3; while the 5th entry (convv) gives the conversion for velocity components in cm/s; -convb=sqrt(convd*4*pi)*convv*(1+z)^2. to have the magnetic field components in Gauss. The comoving cell resolution is 7.9 kpc/cell. The model started from a uniform seed magnetic field of 0.1nG (comoving). Cosmological AMR simulations performed with the ENZO code, using the Dedner MHD method. More details can be found here http://cosmosimfrazza.myfreesites.net/amr_clusters