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Автор COOK, ANDREW W.
Автор CABOT, WILLIAM
Автор MILLER, PAUL L.
Дата выпуска 2004
dc.description A large-eddy simulation technique is described for computing Rayleigh–Taylor instability. The method is based on high-wavenumber-preserving subgrid-scale models, combined with high-resolution numerical methods. The technique is verified to match linear stability theory and validated against direct numerical simulation data. The method is used to simulate Rayleigh–Taylor instability at a grid resolution of $1152^3$. The growth rate is found to depend on the mixing rate. A mixing transition is observed in the flow, during which an inertial range begins to form in the velocity spectrum and the rate of growth of the mixing zone is temporarily reduced. By measuring growth of the layer in units of dominant initial wavelength, criteria are established for reaching the hypothetical self-similar state of the mixing layer. A relation is obtained between the rate of growth of the mixing layer and the net mass flux through the plane associated with the initial location of the interface. A mix-dependent Atwood number is defined, which correlates well with the entrainment rate, suggesting that internal mixing reduces the layerʼs growth rate.
Издатель Cambridge University Press
Название The mixing transition in Rayleigh–Taylor instability
DOI 10.1017/S0022112004009681
Electronic ISSN 1469-7645
Print ISSN 0022-1120
Журнал Journal of Fluid Mechanics
Том 511
Первая страница 333
Последняя страница 362
Аффилиация COOK ANDREW W.; Lawrence Livermore National Laboratory
Аффилиация CABOT WILLIAM; Lawrence Livermore National Laboratory
Аффилиация MILLER PAUL L.; Lawrence Livermore National Laboratory

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