Visualizing the Radiation of the Kelvin-Helmholtz Instability
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].
April 11, 2014 by hgpu
Recent source codes
