E18B high resolution dataset (innermost volume)

DOI

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 the highest resolution level available (3.95 kpc) and the region is the innermost ~Mpc^3 of a perturbed 1e15Msol cluster at z=0. The fields included are: - gas density [code units], gas temperature [K] and dark matter density [code units]; - x/y/z component of magnetic field, in microGauss. For the conversion into cgs: - gas/dark matter density must be multiplied by 2.6666447e-30 to get them in g/cm^3 - B-field values are already in microGauss. For more details, see http://cosmosimfrazza.myfreesites.net/amr-clusters Vazza et al. 2017 MNRAS (https://academic.oup.com/mnras/article-abstract/doi/10.1093/mnras/stx2830/4584474)

Identifier
DOI https://doi.org/10.23728/b2share.2c7482a63b1c4d9498f9f51be7f20fcd
Source https://b2share.eudat.eu/records/2c7482a63b1c4d9498f9f51be7f20fcd
Metadata Access https://b2share.eudat.eu/api/oai2d?verb=GetRecord&metadataPrefix=eudatcore&identifier=oai:b2share.eudat.eu:b2rec/2c7482a63b1c4d9498f9f51be7f20fcd
Provenance
Creator Franco Vazza
Publisher EUDAT B2SHARE
Publication Year 2017
Rights Creative Commons Attribution-NonCommercial-ShareAlike (CC-BY-NC-SA); info:eu-repo/semantics/openAccess
OpenAccess true
Contact franco.vazza2(at)unibo.it
Representation
Size 648.0 MB; 2 files
Discipline 3.4.3 → Physics → Astrophysics