Flash Code Simulations of Rayleigh-Taylor and Richtmyer-Meshkov Instabilities in Laser-Driven Experiments

Details Flash Code Simulations of Rayleigh-Taylor and Richtmyer-Meshkov Instabilities in Laser-Driven Experiments Flash Code Simulations of Rayleigh-Taylor and Richtmyer-Meshkov Instabilities in Laser-Driven Experiments

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.307..227h&link_type=abstract

Astrophysics and Space Science, Volume 307, Issue 1-3, pp. 227-231

Astronomy and Astrophysics

Astrophysics

Adaptive Mesh Refinement, Rayleigh-Taylor, Richtmyer-Meshkov, Supernova, Code Validation, Omega Laser

Scientific paper

We present two- and three-dimensional simulations involving Richtmyer Meshkov and Rayleigh-Taylor instabilities run with the adaptive mesh refinement code, flash. Variations in the rate of mixing layer growth due to dimensionality, perturbation modes, and simulation resolution are explored. These simulations are designed for detailed comparisons with experiments run on the Omega laser to gain understanding of the mixing processes and to prepare for validation of the Flash code.

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