ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17
Transcript of ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17
ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY
Lecture 17 Learning objectives: understand the concepts & physics of 1. Ekman layer 2. Ekman transport 3. Ekman pumping
1. The Ekman Layer Scale analyses show that: Interior Ocean: large scale ocean circulation obeys geostrophy; Ro<<1; Ek<<1 Boundary layer (western boundary, surface layer, bottom boundary layer): geostrophy does not necessarily hold. Why? Critical thinking Oceanic surface: subject to forcing by winds, heat and salinity fluxes (buoyancy flux). Not solely in geostrophic balance.
1 The Ekman layer Fridtjof Nansen, Norwegian explorer: Fram: ship 1893-1896 expedition; Icebergs: 20-40° to the right of wind Walfrid Ekman, Swedish physicist, (1905) : Explained Nansen’s observation
The ocean surface boundary layer is sometimes called the Ekman layer, the layer in which the surface wind stress directly acts. This layer is sometimes called: mixed layer because oceanic properties (T & S) are often well mixed.
In fact: Ekman layer thickness & Mixed layer depth: are not exactly the same Ekman layer: determined by wind Ekman layer thickness: will be defined later (determined by viscosity & f) Mixed layer: wind & buoyancy driven-turbulent mixing Usually: the depth at which density increase is equivalent to 0.5C (some uses 1C, etc) temperature decrease
Observed Temperature along EQ Pacific.
Thermocline Depth of 20C Isotherm (D20): Used to represent Thermocline depth
Pycnocline (halocline: Vary a lot Regionally, not shown)
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σ = ρ −1000
Surface mixed layer
Surface mixed layer
Surface wind exerts stress, on the ocean
1 2
n
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Xs = 0 at the bottom of Ekman layer
Laminar: layered flow; non-turbulent
Ys = 0
Ys = 0
Important: the ocean is viscous; assume stress linearly decreasing with depth (constant viscosity, laminar flow: non-turbulent). Force for a unit area:
Top of layer 2,
Top of layer 3,
……similarly, we can obtain stress for top of layer n.
The net stress working on layer n is: top - bottom
Net stress in x, y directions:
Force per unit mass:
They are momentum fluxes: vertical flux of horizontal momentum
Consider small Rossby number (Ro<<1), steady, and constant density: the equations of motion in Ekman layer are:
Stress X, Y decreases quickly with depth, their direct influence is felt only in the surface boundary layer.
Ekman+geostrophic current
Interior: Only geostrophic current
Surface Ekman layer:
x
z
Bottom Ekman layer
2. Ekman Transport Vertically integrate Ekman flow in the entire Ekman layer with depth HE, we obtain:
Following boundary conditions are used:
UE = uE dz =τ y
ρ0 f−HE
0∫ ,
VE = vE dz = −τ x
ρ0 f−HE
0∫ .
(X,Y ) = 0@z = −HE,(uE,vE ) = 0@z = −HE.
uEx + vEy +wEz dz = 0−HE
0∫
UE = uE dz =τ y
ρ0 f−HE
0∫ ,
VE = vE dz = −τ x
ρ0 f−HE
0∫
(X,Y ) = 0@z = −HE,(uE,vE ) = 0@z = −HE.
3. Ekman pumping Interaction between the surface Ekman layer and the interior ocean beneath
Surface windstress varies spatially, Producing “convergence” and “divergence” of Ekman transports
z x out into
isopycnals
Downwelling upwelling Northern Hemisphere
Ekman Pumping:
xfy
V
x
Uwdz
z
w
y
v
x
u y
hz
hE
E∂
∂=
∂
∂+
∂
∂=⇒=
∂
∂+
∂
∂+
∂
∂−=
−
∫τ
ρ
10)(
0
If we extend it to a general case with x and y components of the wind, we get
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wz= −hE
=∂U
∂x+∂V
∂y=1
ρf(∂τ y
∂x−∂τ x∂y
) =1
ρo fk ⋅ curlτ
The vertical velocity at the bottom of the surface Ekman layer is proportional to the vorticity of
the surface wind stress and it is independent of the detailed structure of the Ekman flow. the
vertical velocity is positive for the positive vorticity of the wind stress, and negative for the
negative vorticity of the wind stress.
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curlτ > 0
hE Ekman pumping
Ekman convergence/divergence cause ispycnals move up and down, generating horizontal pressure gradient force in the “ocean interior” below the Ekman layer, and thus driving the deep ocean in motion. Surely, in the surface mixed layer, they cause both Ekman flow and geostrophic currents (the sum of the two). Note: this is in a linear system.
Ekman pumping can be clearly demonstrated by integrating the continuity equation:
Or:
Because
We have
( is used in a baroclinic ocean)
Ekman transports At
uEx + vEy +wEz dz = 0−HE
0∫
z = −HE
wE =∂∂x( τ
y
ρ f)− ∂∂y( τ
x
ρ f)So,
This expression is valid for both constant and varying density.
UE = uE dz =τ y
ρ0 f−HE
0∫ ,
VE = vE dz = −τ x
ρ0 f−HE
0∫
z x out into
isopycnals
Winds => Ekman convergence, negative (downward) Ekman Pumping:
xfy
V
x
Uwdz
z
w
y
v
x
u y
hz
hE
E∂
∂=
∂
∂+
∂
∂=⇒=
∂
∂+
∂
∂+
∂
∂−=
−
∫τ
ρ
10)(
0
If we extend it to a general case with x and y components of the wind, we get
€
wz= −hE
=∂U
∂x+∂V
∂y=1
ρf(∂τ y
∂x−∂τ x∂y
) =1
ρo fk ⋅ curlτ
The vertical velocity at the bottom of the surface Ekman layer is proportional to the vorticity of
the surface wind stress and it is independent of the detailed structure of the Ekman flow. the
vertical velocity is positive for the positive vorticity of the wind stress, and negative for the
negative vorticity of the wind stress.
€
curlτ > 0
hE Ekman pumping