Effect of initial perturbation amplitude on Richtmyer-Meshkov flows induced by strong shocks
- Stellingwerf Consulting, Huntsville, Alabama 35803 (United States)
We systematically study the effect of the initial perturbation on Richtmyer-Meshkov (RM) flows induced by strong shocks in fluids with contrasting densities. Smooth Particle Hydrodynamics simulations are employed. A broad range of shock strengths and density ratios is considered. The amplitude of the initial single mode sinusoidal perturbation of the interface varies from 0% to 100% of its wavelength. The simulations results are compared, wherever possible, with four rigorous theories, and with other experiments and simulations, achieving good quantitative and qualitative agreement. Our study is focused on early time dynamics of the Richtmyer-Meshkov instability (RMI). We analyze the initial growth-rate of RMI immediately after the shock passage, when the perturbation amplitude increases linearly with time. For the first time, to the authors' knowledge, we find that the initial growth-rate of RMI is a non-monotone function of the initial perturbation amplitude, thus restraining the amount of energy that can be deposited by the shock at the interface. The maximum value of the initial growth-rate depends on the shock strength and the density ratio, whereas the corresponding value of the initial perturbation amplitude depends only slightly on the shock strength and density ratio.
- OSTI ID:
- 22493748
- Journal Information:
- Physics of Plasmas, Journal Name: Physics of Plasmas Journal Issue: 9 Vol. 22; ISSN PHPAEN; ISSN 1070-664X
- Country of Publication:
- United States
- Language:
- English
Similar Records
Simulations and models for the Richtmyer–Meshkov instability with broadband perturbations
Simulations and models for the Richtmyer– Meshkov instability with broadband perturbations
Journal Article
·
Mon Feb 19 19:00:00 EST 2024
· Physics of Fluids
·
OSTI ID:2565525
Simulations and models for the Richtmyer– Meshkov instability with broadband perturbations
Technical Report
·
Mon Feb 19 23:00:00 EST 2024
·
OSTI ID:2386901