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Density ratio dependence of Rayleigh–Taylor mixing for sustained and impulsive acceleration histories
347
Citations
65
References
2000
Year
Marine HydrodynamicsFluid Density RatioImpulsive Acceleration HistoriesEngineeringUnsteady FlowPhysicsAerospace EngineeringConstant AccelerationFluid MechanicsHydrodynamicsTurbulenceTurbulence ModelingTurbulent Flow Heat TransferHydromechanicsMultiphase FlowHydrodynamic StabilityImpulsive SystemTurbulent Rayleigh–taylor Instability
The turbulent Rayleigh–Taylor instability is investigated over a comprehensive range of fluid density ratio (R)1.3⩽R⩽50 [0.15⩽A=(R−1)/(R+1)⩽0.96] and different acceleration histories g(t) using the Linear Electric Motor. The mixing layer is diagnosed with backlit photography and laser-induced fluorescence. For a constant acceleration, the bubble (2) and spike (1) amplitudes are found to increase as hi=αiAgt2 with α2∼0.05±0.005 and α1∼α2RDα with Dα∼0.33±0.05. For temporally varying accelerations Ag(t)>0, this can be generalized to hi=2αiAS using S=[∫gdt]2/2 rather than the displacement Z=∫∫gdt′ dt. For impulsive accelerations, S remains constant during the coast phase and the amplitudes obey a power law hi∼tθi with θ2∼0.25±0.05 and θ1∼θ2RDθ with Dθ∼0.21±0.05. These values of Dα and Dθ compare favorably with numerical simulations and mix models. The average diameter at the mixing front for bubbles is found to increase as d2∼h2(1+A)/4 in qualitative agreement with “merger” models, but the associated dhi/dt is two times larger than the terminal velocity of an isolated bubble. The spikes become relatively narrow at large R, yet they still grow as gt2.
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