Geoscience Reference
In-Depth Information
The relationship between
Ri
f
and
Ri
g
can be derived easily using the lux-gradient
relationships:
z
L
z
L
φ
K
K
m
Ri
=
h
Ri
=
Ri
(3.34)
f
g
g
φ
m
h
Thus the relationship between
Ri
f
and
Ri
g
does depend on stability (as does the rela-
tionship between
Ri
f
and
z/L
). If we combine Eqs. (
3.32
) and (
3.34
), we ind that
z
L
z
L
z
L
z
L
φ
φ
h
h
z
L
Ri
=
Ri
=
(3.35)
g
f
2
φ
φ
m
m
Using the empirical expressions for the lux-gradient relationships (Eqs. (
3.21
) and
(
3.34
)), we ind that:
z
L
z
L
=
Ri
,
for
<
0
g
(3.36)
Ri
z
L
z
L
g
=
−
,
for
>
0
15
Ri
g
An important consequence of the stable side of Eq. (
3.36
) is that the expression for
z/L
has a singularity at
Ri
g
= 0.2. For that value
z/L
tends to ininity and the condi-
tions become so stable that all turbulence is suppressed. The value of
Ri
g
where this
happens is called the
critical
Richardson number,
Ri
gc
. The value of 0.2 is a direct
consequence of Eq. (
3.36
), but the exact value of
Ri
gc
is still a subject of debate (see,
e.g., Zilitinkevich et al.,
2007
). For stable stratiication a relationship similar to Eq.
(
3.36
) can be derived for the bulk Richardson number (DeBruin,
1982
; Launiainen,
1995
; Basu et al.,
2008
):
z
−
z
=
z
z
−
Ri
z
L
2
1
ln
2
b
,
for
>
0
(3.37)
L
15
Ri
1
b
Question 3.20:
Compute the two production terms (shear and buoyancy production)
in the TKE equation (Eq. (
3.10
)) as well as their ratio (
Ri
f
) for the following condi-
tions (use the lux-gradient relationship to determine the wind speed gradient, and use
a height of 10 m).
a)
H
= 140 W m
-2
,
L
v
E
= 250 W m
-2
,
u
*
= 0.3 m s
-1
.
b)
H
= -50 W m
-2
,
L
v
E
= 5 W m
-2
,
u
*
= 0.2 m s
-1
.
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