Simple model for the turbulent mixing width at an ablating surface
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Publication:4425515
DOI10.1063/1.868805zbMath1023.76553OpenAlexW1983215335MaRDI QIDQ4425515
Catherine Cherfils, Karnig O. Mikaelian
Publication date: 18 November 2003
Published in: Physics of Fluids (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1063/1.868805
Related Items (5)
Bubble merger and scaling law of the Rayleigh-Taylor instability with surface tension ⋮ Rayleigh-Taylor and Richtmyer-Meshkov instability induced flow, turbulence, and mixing. I ⋮ Density ratio dependence of Rayleigh–Taylor mixing for sustained and impulsive acceleration histories ⋮ A comparative study of the turbulent Rayleigh–Taylor instability using high-resolution three-dimensional numerical simulations: The Alpha-Group collaboration ⋮ Numerical simulation of single- and multi-mode Rayleigh-Taylor instability with surface tension in two dimensions
Cites Work
- Turbulent mixing generated by Rayleigh-Taylor and Richtmyer-Meshkov instabilities
- A k-ε model for turbulent mixing in shock-tube flows induced by Rayleigh–Taylor instability
- Self-consistent growth rate of the Rayleigh–Taylor instability in an ablatively accelerating plasma
- Effects of Diffusion on Interface Instability between Gases
- Potential flow models of Rayleigh–Taylor and Richtmyer–Meshkov bubble fronts
- The instability of liquid surfaces when accelerated in a direction perpendicular to their planes. I
- Effects of surface tension and viscosity on Taylor instability
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