1D beam of data through a cosmological MHD run with primordial seeding of magnetic fields.

Each *.dat dataset contains the 1D distribution of quantities through a cosmological simulation, from z=0 to z=2, through a random line of sight. The additional .eps files show the trend of data in density, temperature and magnetic field. The simulation is non-radiative and has an initial magnetic field of B=10^-10 G at z=30. The fixed comoving resolution of the simulation is 20.8 kpc per cell. Each dataset is written as follows: "z","gas dens","DM dens","temp","Bx","By","Bz","Btot" with comoving units "# ", "[g/cm^3]","[g/cm^3]","[K]","[G/4pi]","[G/4pi_greek]","[G/4pi_greek]","[G/4pi_greek]" The parent simulations have been run on CSCS-ETHZ (Lugano) using the ENZO code, see Vazza et al. 2014 (http://adsabs.harvard.edu/abs/2014MNRAS.445.3706V) for details.

Identifier
Source https://b2share.eudat.eu/records/11be8e9d5f5d48e899c8ff92d3758a55
Metadata Access https://b2share.eudat.eu/api/oai2d?verb=GetRecord&metadataPrefix=eudatcore&identifier=oai:b2share.eudat.eu:b2rec/11be8e9d5f5d48e899c8ff92d3758a55
Provenance
Creator Franco Vazza
Publisher EUDAT B2SHARE; http://b2share.eudat.eu
Publication Year 2016
Rights Creative Commons Attribution-NonCommercial-ShareAlike (CC-BY-NC-SA); info:eu-repo/semantics/openAccess
OpenAccess true
Contact franco.vazza(at)hs.uni-hamburg.de
Representation
Language English
Resource Type Other
Format dat; eps; zip
Size 470.4 MB; 22 files
Discipline Other