Copyright (C) 2013-2017 Juan D. Soler.
MAGNETAR was created by Juan D. Soler, but is now maintained by several people. See the MAGNETAR repository on GitHub for further details.
MAGNETAR is set of tools for the study of the magnetic field in simulations of MHD turbulence and polarization observations.
MAGNETAR calculates the histogram of relative orientation between density structure in the magnetic field in data cubes from simulations of MHD turbulence and observations of polarization using the method of histogram of relative orientations (HRO).
If you make use of this package in a publication, please cite our accompanying paper:
@ARTICLE{Soler2013,
author = {{Soler}, J.~D. and {Hennebelle}, P. and {Martin}, P.~G. and
{Miville-Desch{\^e}nes}, M.-A. and {Netterfield}, C.~B. and
{Fissel}, L.~M.},
title = "{An Imprint of Molecular Cloud Magnetization in the Morphology of the Dust Polarized Emission}",
journal = {\apj},
archivePrefix = "arXiv",
eprint = {1303.1830},
primaryClass = "astro-ph.GA",
keywords = {ISM: clouds, ISM: magnetic fields, magnetic fields, methods: statistical, polarization },
year = 2013,
month = sep,
volume = 774,
eid = {128},
pages = {128},
doi = {10.1088/0004-637X/774/2/128},
adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...774..128S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
Citation courtesy of ADS.
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