S. Grossmann et D. Lohse, UNIVERSALITY IN FULLY-DEVELOPED TURBULENCE, Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics, 50(4), 1994, pp. 2784-2789
We extend the numerical simulations of She et al. [Phys. Rev. Lett. 70
, 3251 (1993)] of highly turbulent how with 15 less than or equal to T
aylor-Reynolds numbers Re lambda less than or equal to 200 up to Re la
mbda approximate to 45 000, employing a reduced wave vector set method
(introduced earlier) to approximately solve the Navier-Stokes equatio
n. First, also for these extremely high Reynolds numbers Re lambda, th
e energy spectra as well as the higher moments-when scaled by the spec
tral intensity at the wave number k(p) of peak dissipation-can be desc
ribed by one universal function of k/k(p) for all Re lambda. Second, t
he k-space inertial subrange scaling exponents zeta(m) of this univers
al function are in agreement with the 1941 Kolmogorov theory (the bett
er, the larger Re lambda is), as is the Re lambda dependence of k(p).
Only around k(p), viscous damping leads to a slight energy pileup in t
he spectra, as in the experimental data (bottleneck phenomenon).