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accurate, especially in view of the accuracy of the
empirical
lux-gradient relation-
ships on which they are based. The solution for unstable conditions is:
2
u
H
c
κθ
∆∆
3
4
(
)
≈−
116
−
Ri
b
*
ρ
2
z
z
(3.47)
p
ln
2
1
κ
∆
u
z
z
1
4
(
)
u
≈
116
−
Ri
*
b
*
(3.48)
2
ln
1
where
∆
θθ θ
,
Ri
b*
is an 'effective' bulk-Richardson number, in this case
=
()
z
−
()
z
2
1
given by:
z
z
g
T
∆
∆
θ
(3.49)
Ri
=
zz
ln
2
b*
12
2
()
u
1
For stable conditions, the solution is even exact, due to the particular form (simply
linear) of the lux-gradient relationships. Starting from Eq. (
3.29
) and using the rela-
mulations for the luxes can be derived (Launiainen,
1995
; Basu et al.,
2008
):
2
u
H
c
κθ
∆∆
−
( )
2
=−
15
Ri
if 0 <
Ri
<
0
.
2
b
b
2
ρ
(3.50)
z
z
p
ln
2
1
κ
∆
u
z
z
−
( )
u
=
15
Ri
if 0 <
Ri
<
02
.
*
b
b
(3.51)
ln
2
1
where
zz
g
T
θ
()
∆
∆
b
=
( )
(3.52)
Ri
2
1
u
2
which is a standard formulation for the bulk Richardson number. It should be noted
that these results for the stable case have a singularity at
Ri
b
=
0.2 (the critical Rich-
ardson number). At that stability the luxes vanish because all turbulence has been
suppressed by buoyancy. For values of
Ri
b
>
0.2 the expressions in Eqs. (
3.50
) and
(
3.52
) are no longer valid: the luxes are simply equal to zero.
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