-
Tabulated volume filling factor of simulated extragalactic fields (23 models)
23 tabulated files for all magnetic field models (at z=0) investigated in Vazza et al. 2017 http://iopscience.iop.org/article/10.1088/1361-6382/aa8e60 See Table 1 and 2 for a... -
Magnetic power spectra of extragalactic magnetisation models
23 tabulated files for the magnetic power spectra of all magnetic field models (at z=0) investigated in Vazza et al. 2017... -
1D profile of a cosmic volume from z=0 to z=1
1-dimensional profile of simulated fields for long beams through a simulated volume from z=0 to z=1. Each dataset is a column formatted file containing: a) x-position [kpc] b)... -
E5a, AMR8 at z=0.2, reconstructed down to the 6th AMR level (16kpc/cell)
Each HDF5 dataset contains triplets of fields: -6_8mdm001R_dt_012 contains "Density", "Dark_Matter_Density" and "Temperature" (a 640^3 grid for each); -6_8mdm001R_v_012... -
1-D beams crossing a relaxed simulated gal.cluster
150 lines of sight through the volume of a simulated relaxed galaxy cluster at z=0, produced by F.Vazza et al. running ENZO-MHD on the Jureca supercluster in Juelich. Each line... -
Tabulated volume filling factor of simulated extragalactic fields (23 models)
23 tabulated files for all magnetic field models (at z=0) investigated in Vazza et al. 2017 http://iopscience.iop.org/article/10.1088/1361-6382/aa8e60 See Table 1 and 2 for a... -
E18 cluster data at the 6th AMR level
3D dimensional dataset (256^3 cells) in HDF5 format, of a high-resolution MHD cosmological simulations obtained with the ENZO code (Bryan et al. 2015), employing 6 levels of... -
E5a, AMR8 at z=0.02, reconstructed down to the 6th AMR level (16kpc/cell)
Each HDF5 dataset contains triplets of fields: -6_8mdm001R_dt_015 contains "Density", "Dark_Matter_Density" and "Temperature" (a 640^3 grid for each); -6_8mdm001R_v_015... -
E14 high resolution dataset (innermost volume)
3D dimensional dataset (256^3 cells) in HDF5 format, of a high-resolution MHD cosmological simulations obtained with the ENZO code (Bryan et al. 2015). The data are mapped onto... -
E18 cluster data at the 4th and 5th AMR levels
3D dimensional dataset (256^3 cells) in HDF5 format, of a high-resolution MHD cosmological simulations obtained with the ENZO code (Bryan et al. 2015), employing 4 or 5 levels... -
E18B high resolution dataset (innermost volume)
3D dimensional dataset (256^3 cells) in HDF5 format, of a high-resolution MHD cosmological simulations obtained with the ENZO code (Bryan et al. 2015). The data are mapped onto... -
E5a, AMR8 at z=0.4, reconstructed down to the 6th AMR level (16kpc/cell)
Each HDF5 dataset contains triplets of fields: -6_8mdm001R_dt_010 contains "Density", "Dark_Matter_Density" and "Temperature" (a 640^3 grid for each); -6_8mdm001R_v_010... -
1-D beams crossing a perturbed simulated gal.cluster
150 lines of sight through the volume of a simulated galaxy cluster at z=0, produced by F.Vazza et al. running ENZO-MHD on the Jureca supercluster in Juelich. Each line is... -
MHD run for a single cluster simulated with 640^3 cells with ENZO-MHD at z=0.
Hdf5 files for 3D dataset for a cluster run using a uniform grid box with 640^3 cells. Details as in http://adsabs.harvard.edu/abs/2014arXiv1409.2640V. snap_s138: gas density,... -
E5a, AMR8 at z=0.05, reconstructed down to the 6th AMR level (16kpc/cell)
Each HDF5 dataset contains triplets of fields: -6_8mdm001R_dt_014 contains "Density", "Dark_Matter_Density" and "Temperature" (a 640^3 grid for each); -6_8mdm001R_v_014... -
Simulated cosmic volume - Primordial magnetic seeding models.
These are 2 subsets (300^3 cells each) derived from larger 1024^3 cosmological MHD simulations produced using ENZO on Piz-Daint (CSCS) by F.Vazza& collaborators. In these... -
Simulated cosmic volume - astrophysical seeding scenario
These are 3 subsets (300^3 cells each) derived from larger 1024^3 cosmological MHD simulations produced using ENZO on Piz-Daint (CSCS) by F.Vazza& collaborators. In these... -
Simulated cosmic volume - dynamo amplification
This is one subset (300^3 cells) derived from a larger 1024^3 cosmological MHD simulation produced using ENZO on Piz-Daint (CSCS) by F.Vazza& collaborators. In these... -
100 simulated line of sights up to z=1
100 column data up to z=1 from an MHD cosmological simulation run using ENZO (Bryan+14). All dataset are written in a formatted way. Each column contains: redshift, electron... -
Initial conditions for pre-merger cluster simulation with ENZO
Initial conditions for ENZO (enzo-project.org) AMR simulations of a pair of massive clusters in an early merger stage. Nested initial conditions are needed to produce 2 sets of...
