A computationally efficient approach that solves for the spatial covariance
matrix along the dense particle ensemble-averaged trajectory has been succ
essfully applied to describe turbulent dispersion in swirling flows. The pr
ocedure to solve for the spatial covariance matrix is based on turbulence i
sotropy assumption, and it is analogous to Taylor's approach for turbulent
dispersion. Unlike stochastic dispersion models, this approach does not inv
olve computing a large number of individual particle trajectories in order
to adequately represent the particle phased a few representative particle e
nsembles are sufficient to describe turbulent dispersion. The particle Lagr
angian properties required in this method are based on a previous study (Sh
irolkar and McQuay, 1998). The fluid phase information available from pract
ical turbulence models is sufficient to estimate the time and length scales
in the model. In this study, two different turbulence models are used to s
olve for the fluid phase - the standard k-epsilon model, and a multiple-tim
e-scale (NITS) model. The models developed here are evaluated with the expe
riments of Sommerfeld and Qiu (1991). A direct comparison between the dispe
rsion model developed in this study and a stochastic dispersion model based
on the eddy lifetime concept is also provided. Estimates for the Reynolds
stresses required in the stochastic model are obtained from a set of second
-order algebraic relations. The results presented in the study demonstrate
the computational efficiency of the present dispersion modeling approach. T
he results also show that the NITS model provides improved single-phase res
ults in comparison to the k-epsilon model. The particle statistics, which a
re computed based on the fundamentals of the present approach, compare favo
rably with the experimental data. Furthermore, these statistics closely com
pare to those obtained using a stochastic dispersion model. Finally, the re
sults indicate that the particle predictions are relatively unaffected by w
hether the Reynolds stresses are based on algebraic relations or on the tur
bulence isotropy assumption. (C) 2001 Editions scientifiques et medicales E
lsevier SAS.