Three-dimensional high-resolution simulations (up to 8 billion zones) have been performed for a Richtmyer-Meshkov instability produced by passing a shock through a contact discontinuity with a two-scale initial perturbation. The setup approximates shock tube experiments with a membrane pushed through a wire mesh. The simulation produces mixing-layer widths similar to those observed experimentally. Comparison of runs at various resolutions sug-gests a transition from unstable to turbulent flow as the numerical Reynolds number is increased. At the highest resolutions, the spectrum exhibits a re-gion of power-law decay, in which the spectral flux is approximately constant, suggestive of an inertial range, but with a weaker wavenumber dependenc...
The Richtmyer-Meshkov instability (RMI) refers to the baroclinic generation of vorticity at a pertur...
The growth dynamics of two- and three-dimensional single-mode reshocked Richtmyer–Meshkov instabilit...
A material interface between two fluids of different density accelerated by a shock wave is unstable...
Three-dimensional high-resolution simulations are performed of the Richtmyer- Meshkov (RM) instabili...
A program MVFT3D of large-eddy simulation is developed and performed to solve the multi compressible...
evolution of single- and two-mode Richtmyer-Meshkov instability-induced mixing. The numerical method...
We present results from large-eddy simulations (LES) of three-dimensional Richtmyer-Meshkov (RM) ins...
This paper examines, by computational simulation, a canonical Richtmyer-- Meshkov instability realiz...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/90692/1/AIAA-2011-3689-674.pd
The dynamics of the reshocked multi-mode Richtmyer–Meshkov instability is investigated using 513 × ...
This work presents on-going research on large-eddy simulations of shock-generated mixing in Richtmye...
Direct numerical simulation (DNS) is used to study flow characteristics after interaction of a plana...
Large-eddy simulations of the Richtmyer–Meshkov instability with reshock are pre- sented and the res...
The Richtmyer–Meshkov instability RMI refers to the baroclinic generation of vorticity at a perturb...
The Richtmyer-Meshkov instability (RMI) refers to the baroclinic generation of vorticity at a pertur...
The Richtmyer-Meshkov instability (RMI) refers to the baroclinic generation of vorticity at a pertur...
The growth dynamics of two- and three-dimensional single-mode reshocked Richtmyer–Meshkov instabilit...
A material interface between two fluids of different density accelerated by a shock wave is unstable...
Three-dimensional high-resolution simulations are performed of the Richtmyer- Meshkov (RM) instabili...
A program MVFT3D of large-eddy simulation is developed and performed to solve the multi compressible...
evolution of single- and two-mode Richtmyer-Meshkov instability-induced mixing. The numerical method...
We present results from large-eddy simulations (LES) of three-dimensional Richtmyer-Meshkov (RM) ins...
This paper examines, by computational simulation, a canonical Richtmyer-- Meshkov instability realiz...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/90692/1/AIAA-2011-3689-674.pd
The dynamics of the reshocked multi-mode Richtmyer–Meshkov instability is investigated using 513 × ...
This work presents on-going research on large-eddy simulations of shock-generated mixing in Richtmye...
Direct numerical simulation (DNS) is used to study flow characteristics after interaction of a plana...
Large-eddy simulations of the Richtmyer–Meshkov instability with reshock are pre- sented and the res...
The Richtmyer–Meshkov instability RMI refers to the baroclinic generation of vorticity at a perturb...
The Richtmyer-Meshkov instability (RMI) refers to the baroclinic generation of vorticity at a pertur...
The Richtmyer-Meshkov instability (RMI) refers to the baroclinic generation of vorticity at a pertur...
The growth dynamics of two- and three-dimensional single-mode reshocked Richtmyer–Meshkov instabilit...
A material interface between two fluids of different density accelerated by a shock wave is unstable...