2017
DOI: 10.1063/1.4993464
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Late-time growth rate, mixing, and anisotropy in the multimode narrowband Richtmyer–Meshkov instability: The θ-group collaboration

Abstract: Turbulent Richtmyer-Meshkov instability (RMI) is investigated through a series of high resolution three dimensional smulations of two initial conditions with eight independent codes. The simulations are initialised with a narrowband perturbation such that instability growth is due to non-linear coupling/backscatter from the energetic modes, thus generating the lowest expected growth rate from a pure RMI. By independently assessing the results from each algorithm, and computing ensemble averages of multiple alg… Show more

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Cited by 93 publications
(165 citation statements)
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“…An analysis of turbulent transport in an inhomogeneous compressible turbulent mixing layer induced by Richtmyer-Meshkov instability has been presented. The analysis used data from four independent ILES codes which were applied to the quarter-scale problem presented in the θ -group collaboration 16 . All terms in the high-Reynolds number (inviscid) limit of the Reynolds-averaged transport equations for momentum, species mass fraction, turbulent kinetic energy, and mass fraction variance were computed in the inhomogeneous direction.…”
Section: Discussionmentioning
confidence: 99%
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“…An analysis of turbulent transport in an inhomogeneous compressible turbulent mixing layer induced by Richtmyer-Meshkov instability has been presented. The analysis used data from four independent ILES codes which were applied to the quarter-scale problem presented in the θ -group collaboration 16 . All terms in the high-Reynolds number (inviscid) limit of the Reynolds-averaged transport equations for momentum, species mass fraction, turbulent kinetic energy, and mass fraction variance were computed in the inhomogeneous direction.…”
Section: Discussionmentioning
confidence: 99%
“…With a sufficiently strong impulse, time to develop, and high Reynolds number, linear growth will be followed by a transition to turbulence, where velocity fluctuations decay in time, and the layer grows at a relatively slow rate ∝ t θ with θ ≈ 0.2 to 1 (possible if dominated by linear modes, although a fully turbulent layer is limited to 8 θ ≤ 2/3) with a strong dependence on initial conditions [9][10][11][12][13][14][15] . As an example θ ≈ 0.29 for the configuration studied in this paper 16 , compared to KHI (∝ t) and RTI (∝ t 2 ). Despite the relatively small temporal exponent, the growth rate of RMI is sufficiently high that it significantly impacts the physics of the aforementioned applications, and so there is substantial interest in the accurate modelling of turbulent transport and mixing in RMI.…”
Section: Introductionmentioning
confidence: 88%
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