Numerical Simulation of an Idealised Richtmyer-Meshkov Instability Shock Tube Experiment
Michael Groom, Ben Thornber

TL;DR
This study uses numerical simulations to analyze how initial conditions affect the early to intermediate evolution of the Richtmyer-Meshkov instability, comparing results with experimental data and exploring the impact of perturbation bandwidth.
Contribution
It provides a detailed numerical analysis of RMI evolution under different initial conditions, highlighting the effects of broadband versus narrowband perturbations and validating against experimental results.
Findings
Good agreement between simulations and experiments for mixing layer growth.
Broadband perturbations lead to faster mixing layer growth than narrowband.
Finite bandwidth effects persist and influence the growth rate of the instability.
Abstract
The effects of initial conditions on the evolution of the Richtmyer-Meshkov instability (RMI) at early to intermediate times are analysed, using numerical simulations of an idealised version of recent shock tube experiments performed at the University of Arizona. The experimental results are bracketed by performing both implicit large-eddy simulations of the high-Reynolds-number limit as well as direct numerical simulations (DNS) at Reynolds numbers lower than those observed in the experiments. Various measures of the mixing layer width, based on both the plane-averaged turbulent kinetic energy and volume fraction profiles are used to explore the effects of initial conditions on and are compared with the experimental results. The decay rate of the total fluctuating kinetic energy is also used to estimate based on a relationship that assumes self-similar growth of the…
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Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Laser-Plasma Interactions and Diagnostics · Computational Fluid Dynamics and Aerodynamics
