THE RICHTMYER-MESHKOV INSTABILITY
By M. Brouillette. 2002
767 citations recorded by the source corpus.
Subfields: Atomic and Molecular Physics, and Optics, Computational Mechanics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/d9cebafb4ca9757dbb76317d4fc6344c511c7a53
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In Atomic and Molecular Physics, and Optics
In Computational Mechanics
- Gangtao Liang
- I. Mudawar
- Dale I. Pullin
- Carlos Pantano
- David J. Hill
- Tsuyoshi Inoue
- Sanjay Kumar
- Christopher D. Tomkins
In Nuclear and High Energy Physics
- Y. Fukui
- Tsuyoshi Inoue
- Dale I. Pullin
- S. Inutsuka
- R. Yamazaki
- Gangtao Liang
- I. Mudawar
- Sergio Pirozzoli
Citations in the corpus
- Large-eddy simulation and multiscale modelling of a Richtmyer–Meshkov instability with reshock (2006, background): “This last example alone has motivated considerable interest in the fundamental aspects of the RMI; recent reviews of the RMI include Zabusky (1999) and Brouillette (2002). This paper examines, by computational simulation, a canonical Richtmyer– Meshkov instability realized within the confines of a s”
- TURBULENCE AND MAGNETIC FIELD AMPLIFICATION IN SUPERNOVA REMNANTS: INTERACTIONS BETWEEN A STRONG SHOCK WAVE AND MULTIPHASE INTERSTELLAR MEDIUM (2009, background): “This type of vorticity generation is known as Richtmyer-Meshkov instability that is a kind of Rayleigh-Taylor type instability (e.g., Brouillette 2002).”
- An experimental investigation of mixing mechanisms in shock-accelerated flow (2008, background): “Reviews by Brouillette (2002) and Zabusky (1999) offer more comprehensive descriptions of the problem.”
- TOWARD UNDERSTANDING THE COSMIC-RAY ACCELERATION AT YOUNG SUPERNOVA REMNANTS INTERACTING WITH INTERSTELLAR CLOUDS: POSSIBLE APPLICATIONS TO RX J1713.7−3946 (2011, background): “The deformation of the shock front due to a pre-shock density fluctuation is known as the Richtmyer-Meshkov instability (see, Brouillette 2002, Nishihara et al. 2010 for reviews).”
- Review of mass and momentum interactions during drop impact on a liquid film (2016, background): “The Richtmyer–Meshkov instability arises when a shock wave interacts with an interface separating two different fluids [150], and combines compressibility effects with hydrodynamic instability.”