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(1)

Vorticity in the

Ocean

Principles of

Oceanography

(2)

Introduction

 Definitions of Vorticity

 Conservation of Vorticity

 Influence of Vorticity

 Vorticity and Ekman pumping

 Consequence

(3)

Definitions of vorticity

 Vorticity is analagous to angular

momentum.

 Vorticity is a conserved quantity

(Conservation of Vorticity)

 Two types of vorticity

Planetary Vorticity f

Rotation imparted by Earth

 Relative Vorticity z

Due to currents in the ocean

2D flow assumption

Order z << f

(4)

Planetary Vorticity f and Relative

Vorticity z

 Planetary Vorticity: Every object on earth has a vorticity given to it by the rotation of the earth (except an object on the

equator). This vorticity is dependent on latitude.

 Relative Vorticity: The ocean and rotate at exactly the same rate as earth. They haveatmosphere do not some rotation

relative to earth due to currents and winds. Relative vorticity ζ is the vorticity due to currents in the ocean. Mathematically it is:

y k u x

j v x w z

i u z v y

w w

v u

z y

x

k j

i



 

 

 



 

 

 



 

 

 

 

 u

(5)

 ζ is usually much smaller than f, and it is greatest at the edge of fast currents such as the Gulf Stream. To

obtain some understanding of the size of ζ, consider the edge of the Gulf Stream off Cape Hatteras where the velocity decreases by 1 m/s in 100 km at the

boundary. The curl of the current is approximately (1m/s)/(100 km) = 0.14 cycles/day = 1 cycle/week.

Hence even this large relative vorticity is still almost seven times smaller than f. A more typical values of relative vorticity, such as the vorticity of eddies, is a cycle per month.

(6)

Absolute Vorticity

 The sum of the planetary and relative vorticity

 Equations of Motion for frictionless flow

(7)

Derivation of Vorticity equation

Fx

x fv p Dt

Du

1

Fy

y fu p Dt

Dv

1

0 0

x fv p y

v u x u u t u Dt

Du

) 1 ( ) (

y fu p y

v v x u v t v Dt

Dv

) 1 ( ) (

y f v yv f y x

p y

v u y u y v y x u u x u y u y u

t

2

2 2

2 1

) ( )

(

x f u xu f y x

p y

x v v y v x v x u v x v x u x v

t

2 2

2

2 1

) ( )

(

yv u f x f y v x f u y

u x v y v y u x v x u y u x v v y

y u x v u x

y u x v

t

























0









v

y u f x f y v x f u y v x u v y

u x

tz z z z

0





v

y f y v x f u

Dt

Dz z

0

0 0

 0



Dt

Df y v x f u

Dt

Dz z

(8)

Potential Vorticity

 As a conserved quantity potential vorticity is a valuable tool in

studying ocean dynamics. The potential vorticity is defined as the

product of the absolute vorticity and the stratification.

 P is conserved along a fluid trajectory

Barotropic, geostrophic flow in an ocean with depth H(x, y, t)

Fig 1.1

Integrate the continuity equation

Vertical velocity

(9)

Conservation of Vorticity

 Conservation of z in a spinning ocean

Transfer of momentum between two bodies

Friction is essential

Air-sea boundary  Ekman layer  transfer momentum

Sea-bottom boundary  Ekman layer  transfer momentum

Sides of subsea mountains  friction  pressure differences  form drag

In the vast interior of the ocean  frictionless  vorticity is conserved

Conservation of the angular momentum

The angular momentum of any isolated spinning body is conserved

Transfer of angular momentum between two bodies

Need not be in physical contact; gravitational forces can transfer momentum between bodies in space

(10)

Ocean Surface

Ocean bottom

A parcel of water moves east

(constant latitude) in N.Hemis.

As the parcel hits the bump, H

decreases. We know that (f +

ξ )/H=Constant. So if H decreases,

(f + ξ ) must decrease. If f

decreases, the parcel moves

equatorward. If ξ decreases the

parcel spins clockwise.

An example of

conservation of

vorticity when H

doesn’t stay constant

H

Bump in bottom

H

What happens when the

parcel leaves the bump?

(11)

North

South

A parcel of water moves east

(constant latitude) in N.Hemis.

As the parcel hits the bump, H

decreases. We know that (f + ξ

)/H=Constant. So if H decreases, (f

+ ξ ) must decrease. If f decreases,

the parcel moves equatorward. If

ξ decreases the parcel spins

clockwise. Or a combination.

An example of

conservation of

vorticity when

H doesn’t stay

constant

Bump in bottom

H

H

From ABOVE

Parcel Moves Equatorward

(12)

Conservation of Potential

Vorticity

The conservation of potential vorticity couples changes in depth, relative vorticity, and changes in latitude. All three interact:

 Changes in the depth H of the flow causes changes in the

relative vorticity. The concept is analogous with the way figure skaters decreases their spin by extending their arms and legs.

The action increases their moment of inertia and decreases their rate of spin

 Changes in latitude require a corresponding change in ζ. As a column of water moves equatorward, f decreases, and ζ must increase.

(13)

Influence of Vorticity

 The concept of conservation of potential vorticity has far reaching consequences, and its application to fluid flow in the ocean gives a deeper understanding of ocean currents.

f >> z  f / H = constant

The flow in an ocean of constant depth be zonal

Depth is not constant, but in general, currents tend to be east-west rather than north south

Wind makes small changes in z, leading to a small meridional component to the flow

Figure 11.3

(14)

Influence of Vorticity

Barotropic flows are diverted by seafloor features

Figure 1.4: a flow encounters a subsea ridge, Friction along the sides of sub-sea mountains leads to pressure differences on either side of the mountain which causes another kind of drag called form drag.

Topographic steering:

H ζ f the flow is turned toward the equator

Topographic blocking

If the change in depth is sufficiently large, no change in latitude will be sufficient to conserve potential vorticity, and the flow will be unable to cross the ridge

Fig.1.4

(15)

Influence of Vorticity

 An alternate explanation for the existence

of western boundary currents

 Figure 12.5

 Wind blow  negative z

 Eastern boundary  southward flow  f

providing positive z  conservation

 Western boundary  northward flow  f

providing negative z  conservation?!!

 A strong source of positive vorticity is provided by the current shear in the western boundary current as the current rubs against the coast causing the northward velocity to go to zero at the coast

(16)

Convergence/Divergence

 This idea is nothing more then the piling up or moving of water away from a region.

 Conservation of VOLUME: (du/dx+dv/dy+dw/dz=0)

 Rearranging... du/dx + dv/dy = -dw/dz

 If water comes into the box (du/dx + dv/dy)>0 there is a velocity out of the box: dw/dz < 0 DOWNWARD

(17)

Vorticity and Ekman Pumping

 First consider flow in a fluid with constant rotation

 Secondly, how vorticity constrains the flow of a fluid with rotation that varies with latitude

Fluid dynamics on the f Plane: the Taylor-Proudman Theorem

f-plane, constant rotation f = f0

Slowly varying flow in a homogeneous (constant density ρ0), rotating, inviscid fluid

Geostrophic equations

Continuity equation

(18)

Vorticity and Ekman Pumping

 Taking the z derivative and using gives;

 Similarly, for the u-component of velocity

 The vertical derivative of the horizontal velocity field must be zero

 Because w = 0 at the sea surface and at the sea floor, if the bottom is level, there can be no vertical velocity on an f–plane.

(19)

Vorticity and Ekman Pumping

(Fluid dynamics on the f Plane: the Taylor-Proudman Theorem)

 Implication

Rotation greatly stiffens the flow

Cannot expand or contract in the vertical direction

As rigid as a steel bar

Geostrophic flow cannot go over a seamount, it must go around it

w(z=0) = 0 + w(z=H) = 0 + w/z = 0  w(z) = 0

(20)

Vorticity and Ekman Pumping (Fluid

Dynamics on the Beta Plane)

Ekman pumping

b-plane

Consider, f = f0 + b y

G: geostrophic flow

Using the continuity equation, and recalling that β y ≪ f0

Thus the variation of Coriolis force with latitude allows vertical velocity gradients in the geostrophic interior of the ocean, and the vertical velocity leads to north-south currents.

This explains why Sverdrup and Stommel both needed to do their calculations on a β-plane.

(21)

In the central region of the jet, some streamlines that are not purely horizontal are also visible. They correspond to beads trapped in the bottom or top Ekman layers and show net fuid exchange from source to sink.

(22)

Vorticity and Ekman Pumping

Winds at the sea surface drive Ekman transports to the right of the wind in this northern hemisphere example (bold arrows in shaded Ekman layer). The converging Ekman transports driven by the trades and westerlies drives a downward geostrophic flow just below the Ekman layer (bold vertical arrows), leading to downward bowing constant density surfaces i. Geostrophic currents associated with the warm water are shown by bold arrows.

(23)

Vorticity and Ekman Pumping

An example of how winds produce geostrophic currents running upwind. Ekman

transports due to winds in the north Pacific (Left) lead to Ekman pumping (Center), which sets up north-south pressure gradients in the upper ocean. The pressure gradients are balanced by the Coriolis force due to east- west geostrophic currents (Right). Horizontal lines indicate regions where the curl of the zonal wind stress changes sign. AK: Alaskan Current, NEC: North Equatorial Current, NECC: North

Equatorial Counter Current

(24)

Ocean Surface

Mixed Layer

Ocean bottom

A parcel of water moves into an

area of downwelling. It

becomes shorter (and fatter).

f/H must be

conserved!

We know that (f + ξ )/H= Constant. So if H

decreases, (f + ξ ) must decrease. I gave

examples before that either f or ξ could

change. But in this process; it is f that

decreases. f can only decrease by the parcel

moving equatorward.

With DOWNWELLING, the

vertical velocity is downward.

This pushes on the column of

water, making it shorter (and

fatter). What happens when a

column of water gets short and

fat (Vorticity must be

conserved).

H H

Ekman Convergence

(25)

Ekman transport creates convergence and

divergence of upper waters.

Convergence

Convergence

Divergence

Divergence

Divergence

(26)

Sea Surface Height and Mean Geostrophic Ocean Circulation

(27)

Important concepts

 Vorticity strongly constrains ocean dynamics.

 Vorticity due to Earth's rotation is much greater

than other sources of vorticity.

 Taylor and Proudman showed that vertical

velocity is impossible in a uniformly rotating flow.

The ocean is rigid in the direction parallel to the

rotation axis. Hence Ekman pumping requires

that planetary vorticity vary with latitude. This

explains why Sverdrup and Stommel found that

realistic oceanic circulation, which is driven by

Ekman pumping, requires that f vary with latitude

(28)

Important concepts (cont.)

 The curl of the wind stress adds relative vorticity to central gyres of each ocean basin. For steady state circulation in the gyre, the ocean must lose vorticity in western boundary currents.

 Positive wind stress curl leads to divergent flow in the Ekman layer. The ocean's interior geostrophic

circulation adjusts through a northward mass transport.

 Conservation of absolute vorticity in an ocean with constant density leads to the conservation of potential vorticity. Thus changes in depth in an ocean of

constant density requires changes of latitude of the current.

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