Turbulence Generation by Shock Interaction with a Highly Non-Uniform Medium
Seth Davidovits, Christoph Federrath, Romain Teyssier, Kumar, S. Raman, David C. Collins, Sabrina R. Nagel

TL;DR
This study uses numerical simulations to analyze how shock waves interacting with highly non-uniform media generate turbulence, revealing scaling relations and dependencies on initial conditions that inform experimental and theoretical understanding.
Contribution
The paper introduces detailed numerical simulations and scaling relations for turbulence generation by shock interactions with highly non-uniform media, extending understanding of post-shock turbulence.
Findings
Turbulent velocity dispersion depends on initial density variance and shock speed.
Post-shock pressure and density can be predicted by simplified shock transition models.
Turbulence generation scales with the size of initial density perturbations.
Abstract
An initially planar shock wave propagating into a medium of non-uniform density will be perturbed, leading to the generation of post-shock velocity perturbations. Using numerical simulations we study this phenomenon in the case of highly-non-uniform density (order-unity normalized variance, ) and strong shocks (shock Mach numbers ). This leads to a highly disrupted shock and a turbulent post-shock flow. We simulate this interaction for a range of shock drives and initial density configurations meant to mimic those which might be presently achieved in experiments. Theoretical considerations lead to scaling relations, which are found to reasonably predict the post-shock turbulence properties. The turbulent velocity dispersion and turbulent Mach number are found to depend on the pre-shock density dispersion and shock speed in…
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