JC Song - The Physics of fluids, 1987 - pubs.aip.org
In applications to turbulent reactive flows, the probability density function approach requires a model for molecular diffusivity. The objective of the present work is to develop a consistent …
Scalar mixing models are required to model turbulent molecular mixing in full probability density function (pdf) simulations of turbulent reacting flows. Despite the existence of direct …
CB Devaud, RW Bilger, T Liu - Physics of Fluids, 2004 - pubs.aip.org
A new method for calculating the conditional scalar dissipation rate< N| η> is derived from the probability density function (pdf) transport equation for the conserved scalar Z. Two …
BL Sawford - New Journal of Physics, 2004 - iopscience.iop.org
We use simple scalar mixing models coupled to a Lagrangian stochastic trajectory model to calculate a range of conditional scalar statistics for three different source configurations, a …
SS Girimaji - Physics of Fluids A: Fluid Dynamics, 1992 - pubs.aip.org
The objectives of this paper are (i) to establish analytically some important features of the scalar diffusion process in turbulence and (ii) to derive a closure model for this process in …
GW He, R Rubinstein - Journal of Turbulence, 2003 - iopscience.iop.org
A novel mapping closure approximation (MCA) technique is developed to construct a model for the conditional dissipation rate (CDR) of a scalar in homogeneous turbulence. It is shown …
A Kronenburg, RW Bilger - Physics of Fluids, 1997 - pubs.aip.org
The modelling of differential diffusion with a conditional moment closure (CMC) method is considered. Direct numerical simulations for scalar fields in homogeneous isotropic …
A Juneja, SB Pope - Physics of Fluids, 1996 - pubs.aip.org
We employ direct numerical simulations to study the mixing of two passive scalars in stationary, homogeneous, isotropic turbulence. The present work is a direct extension of that …
We analyze experimentally the statistical properties of a turbulent mixing created in the gap between two counter-rotating disks at a Taylor Reynolds number R λ≈ 400. Local isotropy is …