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Updated: Apr 5, 2026

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Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
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Modal interactions between a large-wavelength inclined interface and small-wavelength multimode perturbations in a
Jacob A McFarland1, David Reilly2, Wolfgang Black1
1Department of Mechanical and Aerospace Engineering, University of Missouri, Columbia, Missouri 65211, USA.
Summary
The Richtmyer-Meshkov instability
Area of Science:
- Fluid dynamics
- Plasma physics
- Computational physics
Background:
- The Richtmyer-Meshkov instability (RMI) is a fundamental fluid instability occurring when a shock wave accelerates a perturbed interface between two fluids.
- Understanding RMI is crucial for fields like inertial confinement fusion and astrophysics.
- Previous studies often focused on single perturbation types or 2D simulations.
Purpose of the Study:
- To investigate the interaction between small-wavelength multimodal and large-wavelength inclined interface perturbations in reshocked RMI.
- To analyze the influence of initial perturbation characteristics on mixing and turbulence development.
- To validate simulation code against experimental data.
Main Methods:
- Three-dimensional simulations using the ares code.
- Code validation through comparison with experiments at the Georgia Tech Shock Tube facility.
- Analysis of simulation results for four cases with varying perturbation amplitudes and types.
Main Results:
- The flow retains a memory of initial conditions before reshock, affecting both entrainment and mixing.
- After reshock, the flow transitions to a turbulent-like state.
- High-amplitude large-wavelength perturbations can induce small-scale mixing similar to small-wavelength perturbations.
Conclusions:
- Initial perturbation characteristics significantly influence RMI evolution and resulting turbulence.
- The flow exhibits memory effects of initial conditions even after reshock.
- Large-wavelength perturbations, particularly at high amplitudes, play a critical role in generating small-scale turbulent features.
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