Lp. Wang et al., EXAMINATION OF HYPOTHESES IN THE KOLMOGOROV REFINED TURBULENCE THEORYTHROUGH HIGH-RESOLUTION SIMULATIONS .1. VELOCITY-FIELD, Journal of Fluid Mechanics, 309, 1996, pp. 113-156
The fundamental hypotheses underlying Kolmogorov-Oboukhov (1962) turbu
lence theory (K62) are examined directly and quantitatively by using h
igh-resolution numerical turbulence fields. With the use of massively
parallel Connection Machine-5, we have performed direct Navier-Stokes
simulations (DNS) at 512(3) resolution with Taylor microscale Reynolds
number up to 195. Three very different types of flow are considered:
free-decaying turbulence, stationary turbulence forced at a few large
scales, and a 256(3) large-eddy simulation (LES) flow field. Both the
forced DNS and LES flow fields show realistic inertial-subrange dynami
cs. The Kolmogorov constant for the k(-5/3) energy spectrum obtained f
rom the 512(3) DNS flow is 1.68 +/- 0.15. The probability distribution
of the locally averaged disspation rate epsilon(r) over a length scal
e r is nearly log-normal in the inertial subrange, but significant dep
artures are observed for high-order moments. The intermittency paramet
er mu, appearing in Kolmogorov's third hypothesis for the variance of
the logarithmic dissipation, is found to be in the range of 0.20 to 0.
28. The scaling exponents over both epsilon(r) and r for the condition
ally averaged velocity increments delta(r)u\epsilon(r) are quantified,
and the direction of their variations conforms with the refined simil
arity theory. The dimensionless averaged velocity increments (delta(r)
u(n)\epsilon(r))/(epsilon(r)r)(n/3) are found to depend on the local R
eynolds number Re-epsilon r = epsilon(r)(1/3)r(4/3)/v in a manner cons
istent with the refined similarity hypotheses. In the inertial subrang
e, the probability distribution of delta(r)u/(epsilon(r)r)(1/3) is fou
nd to be universal. Because the local Reynolds number of K62, R(epsilo
n r) = epsilon(r)(1/3)r(4/3)/v, spans a finite range at a given scale
r as compared to a single value for the local Reynolds number R(r) = e
psilon(-1/3)r(4/3)/v in Kolmogorov's (1941a,b) original theory (K41),
the inertial range in the K62 context can be better realized than that
in K41 for a given turbulence held at moderate Taylor microscale (glo
bal) Reynolds number R(l)ambda. Consequently universal constants in th
e second refined similarity hypothesis can be determined quite accurat
ely, showing a faster-than-exponential growth of the constants with or
der n. Finally, some consideration is given to the use of pseudo-dissi
pation in the context of the K62 theory where it is found that the pro
bability distribution of locally averaged pseudo-dissipation epsilon(r
)' deviates more from a log-normal model than the full dissipation eps
ilon(r). The velocity increments conditioned on epsilon(r)', do not fo
llow the refined similarity hypotheses to the same degree as those con
ditioned on epsilon(r).