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contributor authorBoureima, Ismael
contributor authorRamaprabhu, Praveen
contributor authorAttal, Nitesh
date accessioned2019-02-28T10:59:18Z
date available2019-02-28T10:59:18Z
date copyright12/22/2017 12:00:00 AM
date issued2018
identifier issn0098-2202
identifier otherfe_140_05_050905.pdf
identifier urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4251461
description abstractWe describe the behavior of a multimode interface that degenerates into a turbulent mixing layer when subjected to a spherical implosion. Results are presented from three-dimensional (3D) numerical simulations performed using the astrophysical flash code, while the underlying problem description is adopted from Youngs and Williams (YW). During the implosion, perturbations at the interface are subjected to growth due to the Richtmyer–Meshkov (RM) instability, the Rayleigh–Taylor (RT) instability, as well as the Bell–Plesset (BP) effects. We report on several quantities of interest to the turbulence modeling community, including the turbulent kinetic energy (TKE), components of the anisotropy tensor, density self-correlation, and atomic mixing, among others.
publisherThe American Society of Mechanical Engineers (ASME)
titleProperties of the Turbulent Mixing Layer in a Spherical Implosion
typeJournal Paper
journal volume140
journal issue5
journal titleJournal of Fluids Engineering
identifier doi10.1115/1.4038401
journal fristpage50905
journal lastpage050905-8
treeJournal of Fluids Engineering:;2018:;volume( 140 ):;issue: 005
contenttypeFulltext


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