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ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY Lecture 17 Learning objectives: understand the concepts & physics of 1. Ekman layer 2. Ekman transport 3. Ekman pumping
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ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

Feb 03, 2022

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Page 1: 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

Page 2: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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.

Page 3: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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.

Page 4: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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

Page 5: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

Vertical profiles of density, T, S

Surface mixed layer

Page 6: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

Observed Temperature along EQ Pacific.

Thermocline Depth of 20C Isotherm (D20): Used to represent Thermocline depth

Pycnocline (halocline: Vary a lot Regionally, not shown)

σ = ρ −1000

Surface mixed layer

Surface mixed layer

Page 7: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

Surface wind exerts stress, on the ocean

1 2

n

Xs = 0 at the bottom of Ekman layer

Laminar: layered flow; non-turbulent

Ys = 0

Ys = 0

Page 8: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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.

Page 9: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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

Page 10: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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.

Page 11: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

Ekman+geostrophic current

Interior: Only geostrophic current

Surface Ekman layer:

x

z

Bottom Ekman layer

Page 12: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

Because

Thus,

Ekman current; Ekman flow

Page 13: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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.

Page 14: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

NH

UE = uE dz =τ y

ρ0 f−HE

0∫ ,

VE = vE dz = −τ x

ρ0 f−HE

0∫

Page 15: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

Somali coastal upwelling (Western Indian Ocean)

Somalia

Summer monsoon

Page 16: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

Somali coastal downwelling

Somalia Winter monsoon

Page 17: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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

Page 18: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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

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

Page 19: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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.

Page 20: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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

Page 21: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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∫

Page 22: ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY class 17

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