Turbulent flow in a three-dimensional driven cavity has been simulated
directly by solving the Navier-Stokes equations. The results at Re =
3200 and 10 000 compare well with the experimental data. Viscous dissi
pation rate has been calculated without making the assumption of isotr
opy. Near the top moving wall, the instantaneous dissipation rate is v
ery high and also has high amplitude. Its frequency increases bur ampl
itude decreases as one moves away from the wall and it becomes intermi
ttent in the vortex core. The high Reynolds number assumption that dis
sipation is mainly due to the fluctuating velocity components is seen
to be true in the present case except near the wall. The Kolmogorov le
ngth scale attains higher values in the core of the primary vortex due
to low dissipation rate there. A value of 0.01 times the size of the
cubic cavity is a good representative value at Re = 10 000. Even thoug
h the present (84x84x84) grid cannot resolve this scale very well, it
can resolve all the scales dynamically significant in the How as seen
from the velocity and dissipation spectra. (C) 1998 The Japan Society
of Fluid Mechanics Incorporated and Elsevier Science B.V. All rights r
eserved.