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E(A+M)PEC – An OpenCL Atomic and Molecular Plasma Emission Code For Interstellar Medium Simulations

Miguel A. de Avillez, Emanuele Spitoni, Dieter Breitschwerdt
Dept. Mathematics, U. Evora, R. Romao Ramalho 59, 7000 Evora, Portugal
arXiv:1109.5362v1 [astro-ph.GA] (25 Sep 2011)

@article{2011arXiv1109.5362D,

   author={de Avillez}, M.~A. and {Spitoni}, E. and {Breitschwerdt}, D.},

   title={"{E(A+M)PEC – An OpenCL Atomic {amp} Molecular Plasma Emission Code For Interstellar Medium Simulations}"},

   journal={ArXiv e-prints},

   archivePrefix={"arXiv"},

   eprint={1109.5362},

   primaryClass={"astro-ph.GA"},

   keywords={Astrophysics – Galaxy Astrophysics, Astrophysics – High Energy Astrophysical Phenomena},

   year={2011},

   month={sep},

   adsurl={http://adsabs.harvard.edu/abs/2011arXiv1109.5362D},

   adsnote={Provided by the SAO/NASA Astrophysics Data System}

}

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E(A+M)PEC traces the ionization structure, cooling and emission spectra of plasmas. It is written in OpenCL, runs in NVIDIA Graphics Processor Units and can be coupled to any HD or MHD code to follow the dynamical and thermal evolution of any plasma in, e.g., the interstellar medium (ISM).
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