Visualizing the Radiation of the Kelvin-Helmholtz Instability
Plasma Physics
2014-07-01 v1 Computational Physics
Abstract
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].
Keywords
Cite
@article{arxiv.1404.2507,
title = {Visualizing the Radiation of the Kelvin-Helmholtz Instability},
author = {Axel Huebl and David Pugmire and Felix Schmitt and Richard Pausch and Michael Bussmann},
journal= {arXiv preprint arXiv:1404.2507},
year = {2014}
}
Comments
2 pages, 1 figure. This paper is submitted to the 7th Triennial Special Issue of the IEEE Transactions on Plasma Science, Images in Plasma Science for possible publication. The IEEE copyright notice applies