Geoscience Reference
In-Depth Information
11.4.2 The entrainment velocity
The mixed layer over land typically deepens at a few tens of meters to perhaps
100 m per hour (
1-3 cm s 1 ) . But the convective velocity scale w
is typically
at least 1 m s 1 and often larger. Why is w e
w ?
The answer lies in the effects of stability on turbulence. In the i nter facial layer
the buoyant production term represents a rate of TKE loss because is negative
there. Thus the turbulent energy budget under quasi-steady conditions says:
rate of TKE gain from shear production , turbulent and pressure transport
rate of TKE loss to viscous dissipation and buoyancy . (11.44)
If the underlying boundary layer is in free convection the shear production term
vanishes, and it can also be quite small in a barotropic CBL. In such cases the only
source term in the TKE budget is turbulent and pressure transport from below.
In the interfacial layer capping a convective ABL we can estimate this transport
term as of order w 3
=
/h , with h the thickness of the interfacial layer (Figure 11.1) .
If h scales with z i ,thisisoforder w 3
/z i . Therefore a flux Richardson number
characteristic of interfacial-layer turbulence is
g
θ 0 w e
w 3
rate of energy loss to buoyancy
rate of energy gain by transport
R f =
.
(11.45)
/z i
Observations suggest that R f in steady turbulence cannot exceed a relatively small
value, say 0.2-0.3; at larger values the turbulence is extinguished.
We can look at this another way. If in the interfacial layer R f
constant
=
a ,
then a crude statement of the TKE budget there is
a w 3
g
θ 0 1 =
z i
.
(11.46)
It then follows from the definition of w
a. This is a common
closure in CBL modeling - that the entrainment flux of temperature is a constant
negative fraction of the surface flux.
Another Richardson number, one characteristic of CBL structure ( Prob-
lem 11.21 ) ,is( Deardorff and Willis , 1985 )
that
1 /Q 0
=
g
θ 0 z i
w 2
R =
.
(11.47)
R is typically large; for example, if z i =1km, =1K, w =1ms 1 ,then
R =
30. The definitions of R f and R , Eqs. (11.45) and (11.47) , imply that they
are related by
 
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