Geoscience Reference
In-Depth Information
∂
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
+