Properties of the Turbulent Mixing Layer in a Spherical Implosion

[1]  Mikaelian Stability and mix in spherical geometry. , 1990, Physical review letters.

[2]  B. Fryxell,et al.  FLASH: An Adaptive Mesh Hydrodynamics Code for Modeling Astrophysical Thermonuclear Flashes , 2000 .

[3]  P. Woodward,et al.  The Piecewise Parabolic Method (PPM) for Gas Dynamical Simulations , 1984 .

[4]  H. Robey,et al.  Onset of turbulence in accelerated high-Reynolds-number flow. , 2003, Physical review. E, Statistical, nonlinear, and soft matter physics.

[5]  D. I. Pullin,et al.  Small-amplitude perturbations in the three-dimensional cylindrical Richtmyer–Meshkov instability , 2009 .

[6]  Y. Zhou,et al.  Unification and extension of the similarity scaling criteria and mixing transition for studying astrophysics using high energy density laboratory experiments or numerical simulations , 2006 .

[7]  B. Hammel,et al.  Calibrating mix models for NIF tuning , 2010 .

[8]  D. I. Pullin,et al.  Turbulent mixing driven by spherical implosions. Part 2. Turbulence statistics , 2014, Journal of Fluid Mechanics.

[9]  M. D. Carrara,et al.  Rayleigh-Taylor instability at spherical interfaces between viscous fluids: Fluid/vacuum interface , 2015 .

[10]  D. Youngs,et al.  Numerical simulation of mixing by Rayleigh-Taylor and Richtmyer-Meshkov instabilities , 1994 .

[11]  J. Ristorcelli,et al.  Variable-density mixing in buoyancy-driven turbulence , 2007, Journal of Fluid Mechanics.

[12]  J. D. Ramshaw Simple model for linear and nonlinear mixing at unstable fluid interfaces in spherical geometry. , 1999, Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics.

[13]  D. Drikakis,et al.  The influence of initial conditions on turbulent mixing due to Richtmyer–Meshkov instability† , 2010, Journal of Fluid Mechanics.

[14]  E. Meshkov Instability of the interface of two gases accelerated by a shock wave , 1969 .

[15]  Paul R. Woodward,et al.  Cross-code comparisons of mixing during the implosion of dense cylindrical and spherical shells , 2014, J. Comput. Phys..

[16]  Mikaelian Rayleigh-Taylor and Richtmyer-Meshkov instabilities and mixing in stratified spherical shells. , 1990, Physical review. A, Atomic, molecular, and optical physics.

[17]  G. Taylor The instability of liquid surfaces when accelerated in a direction perpendicular to their planes. I , 1950, Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences.

[18]  John Lindl,et al.  Progress toward Ignition and Burn Propagation in Inertial Confinement Fusion , 1992 .

[19]  Andris M. Dimits,et al.  Progress in understanding turbulent mixing induced by Rayleigh–Taylor and Richtmyer–Meshkov instabilities , 2003 .

[20]  J. Strutt Scientific Papers: Investigation of the Character of the Equilibrium of an Incompressible Heavy Fluid of Variable Density , 2009 .

[21]  M. S. Plesset,et al.  On the Stability of Fluid Flows with Spherical Symmetry , 1954 .

[22]  D. Youngs,et al.  Turbulent mixing in spherical implosions , 2008 .

[23]  N. Swaminathan,et al.  On velocity and reactive scalar spectra in turbulent premixed flames , 2014, Journal of Fluid Mechanics.

[24]  P. Ramaprabhu,et al.  The Rayleigh-Taylor Instability driven by an accel-decel-accel profile , 2013 .

[25]  R. D. Richtmyer Taylor instability in shock acceleration of compressible fluids , 1960 .

[26]  R. F. Chisnell The motion of a shock wave in a channel, with applications to cylindrical and spherical shock waves , 1957, Journal of Fluid Mechanics.

[27]  Ben Thornber,et al.  A Comparison of Three Approaches to Compute the Effective Reynolds Number of the Implicit Large-Eddy Simulations , 2016 .

[28]  K. Mikaelian,et al.  Rayleigh-Taylor and Richtmyer-Meshkov Instabilities and Mixing in Stratified Cylindrical Shells , 2005 .

[29]  Daniel Livescu,et al.  High-Reynolds number Rayleigh–Taylor turbulence , 2008 .

[30]  Pullin,et al.  Turbulent mixing driven by spherical implosions. Part 1. Flow description and mixing-layer growth , 2014, Journal of Fluid Mechanics.