A new evolution equation for C_epsilon2 in k-epsilon modeling that incorporates Reynolds-number dependence and finite cascade time effects, shown to match simulation data for forced and decaying isotropic turbulence across a range of Reynolds numbers.
The large-scale structure of homogeneous turbulence,
2 Pith papers cite this work. Polarity classification is still indexing.
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A model based on Chandrasekhar's 1951 time-invariant quantity quantitatively explains the Mach-number dependence of the density power spectrum slope in isothermal supersonic turbulence and demonstrates that the slope cannot reliably determine the Mach number.
citing papers explorer
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A variable-coefficient model for decay of isotropic turbulence capturing effects of finite cascade time and Reynolds number
A new evolution equation for C_epsilon2 in k-epsilon modeling that incorporates Reynolds-number dependence and finite cascade time effects, shown to match simulation data for forced and decaying isotropic turbulence across a range of Reynolds numbers.
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The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence
A model based on Chandrasekhar's 1951 time-invariant quantity quantitatively explains the Mach-number dependence of the density power spectrum slope in isothermal supersonic turbulence and demonstrates that the slope cannot reliably determine the Mach number.