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2 u 1
∂x 1 ∂x 1
2
δ ij δ kn δ lm +
∂u i
∂x k ∂x m
∂u j
∂x l ∂x n =
δ ij δ ln δ km +
δ ij δ kl δ mn
6 δ il δ jn δ km +
1
δ il δ kn δ jm +
δ jl δ in δ km +
δ jl δ kn δ im
+
δ kl δ in δ jm +
δ kl δ jn δ im +
δ ik δ jl δ mn +
δ jk δ il δ mn +
δ ik δ jn δ lm
δ jk δ ln δ im .
+
δ ik δ ln δ jm +
δ jk δ in δ lm +
(14.24)
∂u 1
∂x 1
3
δ ij δ kl δ mn
3 δ ij δ km δ ln + δ ik δ lj δ mn + δ im δ jn δ kl
∂u i
∂x j
∂u k
∂x l
∂u m
4
∂x n =
6 δ ij δ kn δ lm + δ il δ kj δ mn + δ in δ kl δ jm
1
4 δ il δ kn δ jm +
δ in δ kj δ lm +
3
δ il δ km δ jn +
δ in δ km δ lj
δ im δ jk δ ln .
+
δ ik δ lm δ jn +
δ ik δ ln δ jm +
δ im δ jl δ kn +
(14.25)
14.5 Local isotropy
14.5.1 The concept
The concept of local isotropy is credited to Kolmogorov ( 1941 ). His short paper
appears in the Friedlander-Topper (1961) collection as a rather rough English trans-
lation. After defining locally isotropic turbulence in the formal terms of probability
statistics, he wrote:
It is natural that in so general and somewhat indefinite a formulation the just advanced
proposition cannot be rigorously proved. We may indicate here only certain general con-
siderations speaking for [it]. For very large R [Reynolds number] the turbulent flow may
be thought of in the following way: on the [ensemble] averaged flow… are superposed the
“pulsations of the first order” consisting in disorderly displacements of separate fluid vol-
umes, one with respect to another, of diameters of the order of magnitude ( 1 )
(where
is Prandtl's mixing [length]); the order of magnitude … of these relative velocities we
denote by v ( 1 ) . The pulsations of the first order are for very large R in their turn unsteady,
and on them are superposed the pulsations of second order with mixing [length] ( 2 ) < ( 1 )
and relative velocities v ( 2 ) <v ( 1 ) ; such a process of successive refinement of turbulent
pulsations may be carried until for the pulsations of some sufficiently large order n the
Reynolds number
=
(n) v (n)
ν
becomes so small that the effect of viscosity on the pulsations of the order n finally prevents
the formation of pulsations of the order n
R (n)
=
1.
From the energetical point of view it is natural to imagine the process of turbulent mixing
in the following way: the pulsations of the first order absorb the energy of the motion and
+
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