The last lecture we saw how
conservation of potential vorticity governs the evolution of
flows in the ocean. What can we learn from vorticity about
the steady, large-scale circulation using vorticity?
Sverdrup combined geostrophy with Ekman dynamics to find a
powerful relation for the size and pattern of ocean's
circulation in response to the winds. We are going to derive
Sverdrup's balance by first considering the geostrophic
interior and the frictional surface boundary layer (Ekman
layer) separately, in order to highlight how these two regimes
couple to form an ocean gyre.
1. We start with geostrophy:
Initially, we cross differentiate the u and v momentum
equations as we did in last class, but this time we assume a
steady state:
Cross-differentiating:
Or:
Which is the
geostrophic vorticity equation, where:
Thus,
β << f
except near the Equator.
So, the divergence of the flow is proportional (at any
latitude) to its northward or meridional velocity. How
can that be? Remember last class, if you change the
thickness of a water column over a rotating sphere, it
will need to change its spin to conserve PV. If ζ
<< f, then the water will move north/south!
[Note:
in contrast to f, β is positive in both hemispheres.
We will see later that this has the important effect
of causing strong currents on the western side of
all ocean basins.]
If we vertically integrate the geostrophic velocity
balance we find:
With boundary
conditions w(zbottom)
= 0, w(ztop)
= wtop. Here, zbottom
is the seabed and ztop
is the top of the geostrophic interior. For w(zbottom)
= 0 we are assuming a flat-bottomed ocean.
Then:
Thus, at any latitude, the meridional transport is
proportional to the vertical velocity at the top of
the geostrophic ocean.
2. Now, let's look at Ekman:
Again we cross-differentiate these equations:
Vertically integrate over the depth of the Ekman
layer, using as boundary conditions w(z0)
= 0, w(zEk) = wEk:
The second term on the left hand side is small
except near the Equator, where β > f. The
equation then becomes:
This
states that the vertical velocity at the base of
the wind-driven Ekman layer is proportional to the
curl of the wind stress. For clockwise curl 𝜏,
the left hand side is negative ans so wEk
is downward. This is called EKMAN PUMPING. The
figure on the followinggives an example for the interior of the
North Atlantic subtropical gyre:
Conversely, for
anticlockwise winds, the Ekman transport is
divergent and the vertical velocity is upward. This
is called EKMAN SUCTION.
3. Combining the
geostrophic interior and Ekman layer:
We can combine the Ekman and geostrophic layers very
simply by looking at the two vorticity equations we
have.
Equating wEk = wtop gives the
SVERDRUP BALANCE:
This is a pointwise balance, true for anywhere in
the ocean where the following assumptions are valid:
- Flow is
steady - d/dt = 0;
- Flow is frictionless below the Ekman layer;
- wbottom is small - "flat bottom
assumption".
So, the wind-driven ocean gyres can be though of as
two layers:
(1) A surface layer where the curl of the wind field
drives convergences and divergences which drive
vertical flows (or changes in layer depth).
(2) An interior, geostrophic layer driven by the
vertical flows (Ekman pumping/suction) that result
from divergent/convergent Ekman transports.
Sverdrup did the entire problem at once, by taking
the curl of the momentum equations with the wind
stress terms included:
:
Vertically
integrating from the sea bottom to the sea surface,
with boundary conditions w(z = bottom) = 0 and w(z =
0) = 0, gives the Sverdrup balance:
This
depth-integrated balance drops the details of the
Ekman layer + geostrophic interior physics, to
give us the (deceptively) simple result that the
WIND STRESS CURL DRIVES THE MERIDIONAL TRANSPORT.
In terms of
vorticity, you can think of it as the input of
vorticity from the wind being "stored" in the
ocean by moving a column of water to a region with
higher or lower planetary vorticity.
Last
modified: Dec 2014
Lecture
14: The Sverdrup balance and gyre circulation