Rayleigh–Taylor and Richtmyer–Meshkov instability induced flow, turbulence, and mixing. II

Zhou, Ye

doi:10.1016/j.physrep.2017.07.008

Title: Rayleigh–Taylor and Richtmyer–Meshkov instability induced flow, turbulence, and mixing. II

Journal Article · Wed Sep 27 00:00:00 EDT 2017 · Physics Reports

DOI:https://doi.org/10.1016/j.physrep.2017.07.008· OSTI ID:1569184

Zhou, Ye ^[1]

Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)

Rayleigh–Taylor (RT) and Richtmyer–Meshkov(RM) instabilities are well-known pathways towards turbulent mixing layers, in many cases characterized by significant mass and species exchange across the mixing layers (Zhou, 2017. Physics Reports, 720–722, 1–136). Mathematically, the pathway to turbulent mixing requires that the initial interface be multimodal, to permit cross-mode coupling leading to turbulence. Practically speaking, it is difficult to experimentally produce a non-multi-mode initial interface. Numerous methods and approaches have been developed to describe the late, multimodal, turbulent stages of RT and RM mixing layers. This paper first presents the initial condition dependence of RT mixing layers, and introduces parameters that are used to evaluate the level of “mixedness” and “mixed mass” within the layers, as well as the dependence on density differences, as well as the characteristic anisotropy of this acceleration-driven flow, emphasizing some of the key differences between the two-dimensional and three-dimensional RT mixing layers.

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Research Organization:: Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)

Sponsoring Organization:: USDOE National Nuclear Security Administration (NNSA)

Grant/Contract Number:: AC52-07NA27344

OSTI ID:: 1569184

Report Number(s):: LLNL-JRNL-751112; 936444; TRN: US2100266

Journal Information:: Physics Reports, Vol. 723-725, Issue C; ISSN 0370-1573

Publisher:: ElsevierCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 364 works

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Figures / Tables (100)

Fig. 12.4a,b,c(p. 149)

Table 12.2(p. 151)

Fig. 12.5(p. 152)

Table 12.3(p. 157)

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Related Subjects

70 PLASMA PHYSICS AND FUSION TECHNOLOGY
Rayleigh–Taylor instability
Richtmyer–Meshkov instability
Kelvin–Helmholtz instability
Shock waves
Transition
Turbulence
Mixing
Astrophysical fluid dynamics
SuperNovae
Inertial confinement fusion (ICF)
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