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Assessing Mix Layer Amplitude in 3D Decelerating Interface Experiments
Authors:C C Kuranz  R P Drake  T L Donajowski  K K Dannenberg  M Grosskopf  D J Kremer  C Krauland  D C Marion  H F Robey  B A Remington  J F Hansen  B E Blue  J Knauer  T Plewa  N Hearn
Institution:(1) University of Michigan, Ann Arbor, MI, USA;(2) Lawrence Livermore National Laboratory, Livermore, CA, USA;(3) University of Rochester, Rochester, NY, USA;(4) University of Chicago, Chicago, IL, USA
Abstract:We present data from recent high-energy-density laboratory experiments designed to explore the Rayleigh–Taylor instability under conditions relevant to supernovae. The Omega laser is used to create a blast wave structure that is similar to that of the explosion phase of a core-collapse supernova. An unstable interface is shocked and then decelerated by the planar blast wave, producing Rayleigh–Taylor growth. Recent experiments were performed using dual, side-on, x-ray radiography to observe a 3D “egg crate” mode and an imposed, longer-wavelength, sinusoidal mode as a seed perturbation. This paper explores the method of data analysis and accurately estimating the position of important features in the data.
Keywords:Rayleigh-Taylor instability  Supernova  Laboratory astrophysics
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