318
DYNAMICAL OCEANOGRAPHY
Having identified these two different length scales, we know that the ratio δ D /δ a
provides a guideline for investigating the different balances that can occur in the
flow. The possible cases are systematically discussed below; we will indicate the
scale D of the thermocline below (don’t confuse this with the total layer thickness
as used in earlier chapters).
(A) First we consider the case where δ D /δ a ≫ 1, which corresponds to small W E
according to (Fig. 13.6a)
δ D
δ a
≈ W
−3/2
E
.
(13.92)
and hence the Ekman pumping is relatively weak.
δ
D
δ
a
surface
Ekman
layer
W
E
(A1)
(A2a)
(A2b)
D
(a)
δ
D
δ
a
surface
Ekman
layer
W
E
(B2)
(B1)
D
(b)
Figure 13.6. Sketch to help understand the different cases in the scales of the thermocline depth.
(a) Case A with δD/δa ≫ 1. (b) Case B with δD/δa ≪ 1.
There are now several choices that can be made for the characteristic vertical
length scale of the flow D:
(A1) If we choose D = δ a then it follows that
λ V =
K V r 0
UD 2 =
K V
W E D
=
δ D
D
=
δ D
δ a
≫ 1,
(13.93)
and because ρ = ρ s according to (13.89), the surface density extends
(because of large vertical mixing) to the deep sea which is not what is
observed.
DYNAMICAL OCEANOGRAPHY
Having identified these two different length scales, we know that the ratio δ D /δ a
provides a guideline for investigating the different balances that can occur in the
flow. The possible cases are systematically discussed below; we will indicate the
scale D of the thermocline below (don’t confuse this with the total layer thickness
as used in earlier chapters).
(A) First we consider the case where δ D /δ a ≫ 1, which corresponds to small W E
according to (Fig. 13.6a)
δ D
δ a
≈ W
−3/2
E
.
(13.92)
and hence the Ekman pumping is relatively weak.
δ
D
δ
a
surface
Ekman
layer
W
E
(A1)
(A2a)
(A2b)
D
(a)
δ
D
δ
a
surface
Ekman
layer
W
E
(B2)
(B1)
D
(b)
Figure 13.6. Sketch to help understand the different cases in the scales of the thermocline depth.
(a) Case A with δD/δa ≫ 1. (b) Case B with δD/δa ≪ 1.
There are now several choices that can be made for the characteristic vertical
length scale of the flow D:
(A1) If we choose D = δ a then it follows that
λ V =
K V r 0
UD 2 =
K V
W E D
=
δ D
D
=
δ D
δ a
≫ 1,
(13.93)
and because ρ = ρ s according to (13.89), the surface density extends
(because of large vertical mixing) to the deep sea which is not what is
observed.
