11855

Visualizing the Radiation of the Kelvin-Helmholtz Instability

Axel Huebl, David Pugmire, Felix Schmitt, Richard Pausch, Michael Bussmann
Helmholtz-Zentrum Dresden – Rossendorf
arXiv:1404.2507 [physics.plasm-ph], (4 Apr 2014)

@article{2014arXiv1404.2507H,

   author={Huebl}, A. and {Pugmire}, D. and {Schmitt}, F. and {Pausch}, R. and {Bussmann}, M.},

   title={"{Visualizing the Radiation of the Kelvin-Helmholtz Instability}"},

   journal={ArXiv e-prints},

   archivePrefix={"arXiv"},

   eprint={1404.2507},

   primaryClass={"physics.plasm-ph"},

   keywords={Physics – Plasma Physics, 85-08},

   year={2014},

   month={apr},

   adsurl={http://adsabs.harvard.edu/abs/2014arXiv1404.2507H},

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

}

Emerging new technologies in plasma simulations allow tracking billions of particles while computing their radiative spectra. We present a visualization of the relativistic Kelvin-Helmholtz Instability from a simulation performed with the fully relativistic particle-in-cell code PIConGPU powered by 18,000 GPUs on the USA’s fastest supercomputer Titan [1].
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