Geoscience Reference
In-Depth Information
where δ is the Dirac delta function and u i is the velocity at x i ,t in realization α .
Thus the probability that in realization α the velocity at (x i ,t) is within dv i of v i
is β α (v i ;
u i , as required. Averaging this
expression over all realizations (and denoting this by angle brackets) yields
β(v i ; x i ,t) = β α (v i ; x i ,t) = δ(u i v i ) .
x i ,t)dv i
=
δ(u i
v i )dv i
=
1if v i
=
(13.36)
In equating the probability density of velocity u i (x i ,t) to the expected value
of a delta function involving velocity, Eq. (13.36) provides a link between the
dynamics of the velocity field and those of its probability density. Before showing
how Lundgren ( 1967 ) used that link, we'll need to generalize Eq. (13.36) to joint
probability densities.
The probability density β v ( 1 )
,t is the “one-point” form. Its product with
x ( 1 )
;
i
i
dv ( 1 )
is the probability that the velocity at x ( 1 )
and time t is within dv i of v ( 1 )
.
i
i
i
From Eq. (13.36) it is written as
β v ( 1 )
δ u i x ( 1 )
v ( 1 i
δ u ( 1 )
v ( 1 i
,t
,t
x ( 1 )
;
=
β( 1 ).
i
i
i
i
(13.37)
The “two-point”, or joint, probability density β 2 v ( 1 )
t is the
,v ( 2 )
x ( 1 )
,x ( 2 )
;
;
i
i
i
i
probability that at time t the velocity at x ( 1 )
is within dv i of v ( 1 )
and the velocity at
i
i
x ( 2 )
is within dv i of v ( 2 )
. By extension of the arguments leading to Eq. (13.37) it is
i
i
δ u ( 1 )
v ( 2 i
β 2 v ( 1 )
t
v ( 1 i δ u ( 2 )
,v ( 2 )
x ( 1 )
,x ( 2 )
;
;
=
β( 1 , 2 ).
i
i
i
i
i
i
(13.38)
Lundgren's derivation of the pdf evolution equation proceeds as follows. The
time derivative of Eq. (13.37) is
∂δ u ( 1 )
v ( 1 i
u ( 1 )
v ( 1 i
v ( 1 i
∂t δ u ( 1 )
∂t β( 1 )
i
i
=
=
u ( 1 )
v ( 1 i
i
∂t
i
∂v ( 1 )
.
δ u ( 1 )
v ( 1 i
∂t u ( 1 )
=−
(13.39)
i
i
i
Lundgren then evaluated the right side of Eq. (13.39) with the Navier-Stokes and
continuity equations through tedious calculations. The resulting evolution equation
for the probability density is
 
Search WWH ::




Custom Search