Shaken and stirred: the effects of turbulence and rotation on disc and outflow formation during the collapse of magnetized molecular cloud cores (dataset)

Lewis, Benjamin T.; Bate, Matthew R.

dc.contributor.author	Lewis, Benjamin T.
dc.contributor.author	Bate, Matthew R.
dc.date.accessioned	2018-04-03T08:34:44Z
dc.date.issued	2018-04-03
dc.date.updated	2018-04-03T05:52:15Z
dc.description.abstract	This is the dataset that was used to produce the paper published in MNRAS. Included are the binary dump files from all eighteen of the calculations in the paper.	en_GB
dc.description.sponsorship	Science and Technology Facilities Council	en_GB
dc.description.sponsorship	European Research Council under the European Community's Seventh Framework Programme (FP7/2007-2013)	en_GB
dc.description.sponsorship	This work used the DiRAC Complexity system, operated by the University of Leicester IT Services, which forms part of the STFC DiRAC HPC Facility (www.dirac.ac.uk). This equipment is funded by BIS National E-Infrastructure capital grant ST/K000373/1 and STFC DiRAC Operations grant ST/K0003259/1. DiRAC is part of the National E-Infrastructure.	en_GB
dc.description.sponsorship	Calculations were also performed on the University of Exeter Supercomputer, a DiRAC Facility jointly funded by STFC, the Large Facilities Capital Fund of BIS and the University of Exeter.	en_GB
dc.identifier.doi	10.24378/exe.203
dc.identifier.uri	http://hdl.handle.net/10871/32288
dc.language.iso	en	en_GB
dc.publisher	University of Exeter	en_GB
dc.relation.url	http://hdl.handle.net/10871/32997	en_GB
dc.rights	CC BY 2.0 (UK)	en_GB
dc.title	Shaken and stirred: the effects of turbulence and rotation on disc and outflow formation during the collapse of magnetized molecular cloud cores (dataset)	en_GB
dc.type	Dataset	en_GB
dc.date.available	2018-04-03T08:34:44Z
dc.description	The XZ compressed tarballs in this repository contain the binary output data from the smoothed particle radiation magnetohydrodynamics (SPRMHD) calculations presented in the paper.	en_GB
dc.description	The tarballs are named according to the following scheme: mAAMBB[R][-rCCC].tar.xz. Here, the letters AA represent the mass-to-flux ratio used in the calculation, e.g. a ratio of 5 would imply AA=05, and so on. The letters BB represent the turbulent Mach number multiplied by ten, e.g. Mach 0.1 entails BB=01. The presence of the letter R indicates a calculation using a radiative as opposed to a barotropic equation of state. Finally, the presence of the -rCCC suffix indicates changes to the initial rotational beta, where CCC indicates the beta value multiplied by one hundred, e.g. CCC=001 implies a beta of 0.01. This nomenclature is identical to column 1 of Table 1 in the published paper, which also details any other initial conditions which are relevant.	en_GB
dc.description	Within each tarball are a number of FORTRAN unformatted binary files in big-endian format. These files are named according to the scheme DAT????. In all the calculations without an -rCCC suffix, these are spaced at one-hundredths of a free-fall time, so that, e.g., DAT0050 corresponds to one-half of a free-fall time. In the -rCCC calculations the temporal spacing is more complex. Until one free-fall time the spacing is as before, however after that point the binary outputs are separated by 1/1600th of a free-fall time, so that DAT0101 corresponds to 1601/1600 free-fall times, and so on.	en_GB
dc.description	The data files can be read using the open source tool SPLASH written by Daniel Price (see http://users.monash.edu.au/~dprice/splash/). This tool was also used to produce all the rendered figures in the paper. Other figures were produced from data derived from the binary files.	en_GB
dc.description	The article associated with this dataset is located in ORE at: http://hdl.handle.net/10871/32997	en_GB
dc.identifier.journal	Monthly Notices of the Royal Astronomical Society	en_GB
dc.rights.uri	https://creativecommons.org/licenses/by/2.0/uk	en_GB