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• W158254295 abstract "The advance of a Rayleigh-Taylor mixing front such as that described in Linden & Redondo (1991), may be shown to follow a dependence with time such that the average mixing region is described as h = 2cgAt where h is the width of the growing region of instability, g is the gravitational acceleration and A is the Atwood number. The detailled structure of the front will afect the overall mixing as well as the transport properties between the fluids of different densities subject to gravitational acceleration. A Large Eddy Simulation numerical model using FLUENT as well as a dedicated code is used to predict some of the features of the experiments, (Figure 1 ) different models on the interaction of the bubble generated buoyancy flux and on the boundary conditions are compared with the experiments. The aspect ratios of the bubble induced convective cells are seen to depend on the boundary conditions applied to the enclosure. In the context of determining the influence of structure on mixing ability, multifractal analysis is used to determine the regions of the front which contribute most to molecular mixing and relating intermittency to the structure functions and to the maximum local fractal dimension." @default.
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• W158254295 date "2004-01-01" @default.
• W158254295 modified "2023-09-23" @default.
• W158254295 title "Multifractal structure and intermittent mixing in Rayleigh- Taylor driven fronts" @default.
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