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Kolmogorovs theory of turbulence

This appears to be in agreement with experimental observations. Since the viscosity term has the highest derivative in the Navier-Stokes equation the limit v — 0 is singular and corresponds to divergent velocity gradients. This is an example of a dissipative anomaly in which the time-reversal symmetry, that is broken for the viscous flow, is not restored in the limit of vanishing viscosity. [Pg.11]

Using the dissipation rate (e) as the only relevant flow parameter in the v — 0 limit, from dimensional considerations the typical fluctuations of the velocity field over a distance l and the corresponding characteristic timescales r(Z), usually interpreted as eddy turnover time , can be estimated as [Pg.12]

in the Re — oo limit the turbulent velocity field is a rough non-differentiable function Sv(l) l1/3 for l -h. 0. This expression identifies the so-called Holder exponent as a = 1/3. It is easy to see that the energy transfer rate 8v(1)2/t(1) is independent of the length scale l and applying the first of the above formulas to the integral scale (L) one can relate the energy dissipation rate to the large scale properties of the flow as u3/l. [Pg.12]

The results of this dimensional analysis are supported by an exact result obtained by Kolmogorov for the third-order longitudinal structure function. The structure functions are moments of velocity differences measured at a given distance. More specifically the structure function of order n, Sn(l), is defined as [Pg.12]

Brackets denote spatial or ensemble averages. Starting from the Navier-Stokes equation and assuming a statistically isotropic and homogeneous velocity field one can derive the Karman-Howarth equation for the longitudinal structure functions as [Pg.12]


The dependence of the Reynolds number on the local velocity can be established in terms of the Kolmogorov theory of turbulence. [Pg.403]




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