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arXiv · 1404.2507

Visualizing the Radiation of the Kelvin-Helmholtz Instability

Axel Huebl·David Pugmire·Felix Schmitt·Richard Pausch·Michael Bussmann
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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].

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Axel Huebl, David Pugmire, Felix Schmitt, Richard Pausch, Michael Bussmann. 2014-04-04. Visualizing the Radiation of the Kelvin-Helmholtz Instability. https://doi.org/10.1109/tps.2014.2327392

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