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OC3230-Paduan OC3230-Paduan images Copyright © McGraw Hill images Copyright © McGraw Hill Chap 9: Dynamics Chap 9: Dynamics Light Transmission Light Transmission Solar heating Solar heating supplies short- supplies short- wave radiation wave radiation to ocean to ocean surface; surface; Energy (light) Energy (light) penetrates the penetrates the water column to water column to different different depths as a depths as a function of its function of its wavelength and wavelength and the clarity of the clarity of the water the water
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Page 1: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Light TransmissionLight Transmission

Solar heating Solar heating supplies short-wave supplies short-wave radiation to ocean radiation to ocean surface;surface;

Energy (light) Energy (light) penetrates the water penetrates the water column to different column to different depths as a function depths as a function of its wavelength of its wavelength and the clarity of the and the clarity of the waterwater

Page 2: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Light TransmissionLight Transmission

I = II = Iooee-kz-kz (k = attenuation coefficient) (k = attenuation coefficient)

Attenuation with depthAttenuation with depth(clear water)(clear water)

1% light1% lightlevellevel

Page 3: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Light TransmissionLight Transmission

I = II = Iooee-kz-kz (k = attenuation coefficient) (k = attenuation coefficient)

Scattering is proportional to 1/Scattering is proportional to 1/44

(clear ocean looks blue)(clear ocean looks blue)

Absorption is highest for redAbsorption is highest for redcompared with blue lightcompared with blue light

Spreading is not a factorSpreading is not a factor(source is evenly distributed(source is evenly distributedover water surface)over water surface)

Page 4: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Light TransmissionLight Transmission

Blue:Blue: 1% light level ~170m1% light level ~170m

Red:Red: 1% light level ~7m1% light level ~7m(clear ocean case)(clear ocean case)

Page 5: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Light TransmissionLight Transmission

Optical instruments; Optical instruments; e.g., e.g., Portable Hyperspectral Imager for Low-Light Spectroscopy (PHILLS);PHILLS);

~500 spectral bands ~500 spectral bands ~1nm wide~1nm wide

Built around CCD Built around CCD cameras 640 pixels cameras 640 pixels acrossacross

Page 6: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Light TransmissionLight Transmission

PHILLS images PHILLS images offshore New Jersey, offshore New Jersey, 20012001

Every pixel in this Every pixel in this image includes a full image includes a full spectrum of spectrum of informationinformation

Page 7: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Light TransmissionLight Transmission

VegetatedVegetatedLandLand

CoastalCoastalWaterWater

Page 8: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics

z

Area

ρ

, ( )Pressure p on underside of parcel

g

Δ z ρ

p1

p

2

g

–(p

1

– p

2

) = ρ g Δ z

Pressure increase from

top surface of layer to

bottom surface = weight

of water in layer

Hydrostatic BalanceHydrostatic Balance

Hydrostatic Equation is a Hydrostatic Equation is a simplification of the simplification of the vertical component of vertical component of the equations of motion the equations of motion (momentum equations)(momentum equations)

Assume, instead that Assume, instead that there is no motion in the there is no motion in the vertical direction; vertical direction; Balance of forces is Balance of forces is between weight of the between weight of the water and the pressure water and the pressure that builds with depththat builds with depth

P =

Force

Area

=

ma

A

=

ρ Va

A

=

ρ Aza

A

= ρ zg

Force balance at the bottom of this boxForce balance at the bottom of this box

Many “boxes” stacked up in the water column:Many “boxes” stacked up in the water column:

Generalizing:Generalizing:

dp = – ρ gdz . .This is the differential form of the hydro eqn

Page 9: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Hydrostatic BalanceHydrostatic Balance

What if we want to use What if we want to use the hydrostatic equation the hydrostatic equation to compute pressure?to compute pressure?

Appropriate to static (not Appropriate to static (not moving) water columns moving) water columns but is also a good but is also a good approximation to moving approximation to moving situationssituations €

dP

dzdz = − ρgdz

0

z

∫0

z

∫Integrate (sum up) equation:Integrate (sum up) equation:

Expand, where Expand, where P(atm)P(atm) = = P(0)P(0) = Atmos Press: = Atmos Press:

P(z) = P(atm) − ρgdz0

z

∫ = −ρ ogz

Pressure is equal to thePressure is equal to theweight of overlying waterweight of overlying water only if only if ρρ = constant = constant

Related topics:Related topics:

1)1) Static Stability of a water columnStatic Stability of a water column

2)2) Geostrophic Method for computing (horizontal) currentsGeostrophic Method for computing (horizontal) currents

Page 10: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Static StabilityStatic Stability

The notion of static stability assess whether the vertical The notion of static stability assess whether the vertical distribution of density is stable relative to the downward force distribution of density is stable relative to the downward force of gravity; i.e., is there light water over heavy water, which is of gravity; i.e., is there light water over heavy water, which is stable, or the opposite, which is unstable?stable, or the opposite, which is unstable?

E = −1

ρ

∂ρ

∂z−

g

c 2≈ −

1

ρ o

∂ρ

∂z

Related to compres-Related to compres-sibility (sound speed);sibility (sound speed);often neglectedoften neglected

Stability parameter, EStability parameter, E

E > 0, stableE > 0, stable

E < 0, unstableE < 0, unstable

E = 0, neutralE = 0, neutral

zzρρ

Page 11: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Static StabilityStatic Stability

The notion of static stability assess whether the vertical The notion of static stability assess whether the vertical distribution of density is stable relative to the downward force distribution of density is stable relative to the downward force of gravity; i.e., is there light water over heavy water, which is of gravity; i.e., is there light water over heavy water, which is stable, or the opposite, which is unstable?stable, or the opposite, which is unstable?

E = −1

ρ

∂ρ

∂z−

g

c 2≈ −

1

ρ o

∂ρ

∂z

Related to compres-Related to compres-sibility (sound speed);sibility (sound speed);often neglectedoften neglected

Buoyancy Frequency, NBuoyancy Frequency, N

Used to characterizeUsed to characterizeinternal wave oscillationsinternal wave oscillations

““Brunt-Väisälä” Frequency; “Natural Frequency”Brunt-Väisälä” Frequency; “Natural Frequency”

N 2 = gE =g

ρ o

∂ρ

∂z

Page 12: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Static StabilityStatic Stability

The Buoyancy Period is P = 2The Buoyancy Period is P = 2/N/N

Typical values:Typical values:

10-33 min in seasonal thermocline10-33 min in seasonal thermocline

6 hr in deep ocean6 hr in deep ocean

Buoyancy Frequency, NBuoyancy Frequency, N

Used to characterizeUsed to characterizeinternal wave oscillationsinternal wave oscillations

““Brunt-Väisälä” Frequency; “Natural Frequency”Brunt-Väisälä” Frequency; “Natural Frequency”

N 2 = gE =g

ρ o

∂ρ

∂z

E = −1

ρ

∂ρ

∂z−

g

c 2≈ −

1

ρ o

∂ρ

∂z

The notion of static stability assess whether the vertical The notion of static stability assess whether the vertical distribution of density is stable relative to the downward force distribution of density is stable relative to the downward force of gravity; i.e., is there light water over heavy water, which is of gravity; i.e., is there light water over heavy water, which is stable, or the opposite, which is unstable?stable, or the opposite, which is unstable?

Page 13: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Static StabilityStatic Stability

EnhancedEnhancedmixing ismixing isproduced byproduced bydouble diffusiondouble diffusion

Effect is due toEffect is due tothe differencethe differencebetween rate ofbetween rate ofdiffusion of saltdiffusion of saltversus heatversus heat

Heat:Heat: = 1.4 x 10 = 1.4 x 10-3-3 cm cm22 sec sec-1-1

Salt:Salt: = 1.1 x 10 = 1.1 x 10-5-5 cm cm22 sec sec-1-1

e.g.,:e.g.,:

∂C

∂t= ε∇ 2C

Page 14: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Static StabilityStatic Stability

EnhancedEnhancedmixing ismixing isproduced byproduced bydouble diffusiondouble diffusion

Effect is due toEffect is due tothe differencethe differencebetween rate ofbetween rate ofdiffusion of saltdiffusion of saltversus heatversus heat

Heat:Heat: = 1.4 x 10 = 1.4 x 10-3-3 cm cm22 sec sec-1-1

Salt:Salt: = 1.1 x 10 = 1.1 x 10-5-5 cm cm22 sec sec-1-1

e.g.,:e.g.,:

∂C

∂t= ε∇ 2C

WF/CS WS/CF CF/WS CS/WF

Standard Case Salt Fingers Salt Layers Unstable

dT/dz > 0 dT/dz > 0 dT/dz < 0 dT/dz < 0

dS/dz < 0 dS/dz > 0 dS/dz < 0 dS/dz > 0

This is the typical situation in the ocean. It is stable and it does not lead to mixing due to double diffusion because both heat and salt fluxes act to reduce gradient

Case can lead to salt fingers because a “blob” of water perturbed up into top layer will continue to be sent up by the quick flux of heat into it

Case can lead to layers because rapid flux of heat into upper layer causes it to rise away from interface between layers

This case is always unstable, hence it cannot exist in a still condition in which double diffusion could operate

Page 15: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics

EnhancedEnhancedmixing ismixing isproduced byproduced bydouble diffusiondouble diffusion

Likelihood ofLikelihood ofdouble diffusiondouble diffusionis measuredis measuredby the densityby the densityratio, R:ratio, R:

R must be positiveR must be positivefor double diffusionfor double diffusion(dT/dz and dS/dz same sign)(dT/dz and dS/dz same sign)

R =

αdT

dz

βdS

dz

Static StabilityStatic Stability

WF/CS WS/CF CF/WS CS/WF

Standard Case Salt Fingers Salt Layers Unstable

dT/dz > 0 dT/dz > 0 dT/dz < 0 dT/dz < 0

dS/dz < 0 dS/dz > 0 dS/dz < 0 dS/dz > 0

This is the typical situation in the ocean. It is stable and it does not lead to mixing due to double diffusion because both heat and salt fluxes act to reduce gradient

Case can lead to salt fingers because a “blob” of water perturbed up into top layer will continue to be sent up by the quick flux of heat into it

Case can lead to layers because rapid flux of heat into upper layer causes it to rise away from interface between layers

This case is always unstable, hence it cannot exist in a still condition in which double diffusion could operate

Page 16: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Rotation EffectsRotation Effects

““Even for those with Even for those with considerable sophistication considerable sophistication in physical concepts, one’s in physical concepts, one’s first introduction to the first introduction to the consequences of the consequences of the Coriolis force often Coriolis force often produces something produces something analogous to intellectual analogous to intellectual trauma.”trauma.”

John A. KnaussJohn A. Knauss

Page 17: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Rotation EffectsRotation Effects

Gaspard-Gustave de Coriolis (1792-1843)Gaspard-Gustave de Coriolis (1792-1843)

Sir Isaac Newton (1642-1727)Sir Isaac Newton (1642-1727)

(only for non-(only for non-acceleratingacceleratingreference frames)reference frames)

F = maF = ma

QuickTime™ and aYUV420 codec decompressor

are needed to see this picture.

Page 18: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Rotation EffectsRotation Effects

Page 19: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics Rotation EffectsRotation Effects

ra =

dr v

dt

⎝ ⎜

⎠ ⎟inertial

=d

r v

dt

⎝ ⎜

⎠ ⎟earth

+ 2r Ω ×

r v +

r Ω ×

r Ω ×

r R ( )

Coriolis Acceleration Coriolis Acceleration accounts for the fact that accounts for the fact that the rotating Earth the rotating Earth coordinate system is coordinate system is notnot an inertial reference an inertial reference systemsystem

CoriolisCoriolistermsterms

CentripetalCentripetalAccelAccel

v = u i + v j + w k ; Ω = ∅ i + Ω cos θ j + Ω sin θ k

θθ

ΩΩ

ΩΩθθ

ΩΩ is a vector parallel is a vector parallel to the axis of to the axis of rotation whose rotation whose magnitude is equal magnitude is equal to 1 cycle/dayto 1 cycle/day

Page 20: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics

F = maF = ma

Equations of MotionsEquations of Motions

Based on momentum balance (Newton’s 2nd Law):Based on momentum balance (Newton’s 2nd Law):

Vector form (written as F/m = a):Vector form (written as F/m = a):

d v

dt

+ 2 Ω × v = – 1

ρ

∇ + p g + F

2 Ω × v =

i j k

∅ 2 Ω cos θ 2 Ω sin θ

u v w

=

2w Ω cos θ - 2v Ω sin θ i +

2u Ω sin θ j +

2u Ω cos θ k

AccelerationAcceleration CoriolisCoriolis Press Gravity FrictionPress Gravity FrictionGradientGradient

Coriolis expanded:Coriolis expanded:

ff = 2 = 2ΩΩsinsinθθ = Coriolis Parameter = Coriolis Parameter

Page 21: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics

F = maF = ma

Equations of MotionsEquations of Motions

Based on momentum balance (Newton’s 2nd Law):Based on momentum balance (Newton’s 2nd Law):

Vector form (written as F/m = a):Vector form (written as F/m = a):

d v

dt

+ 2 Ω × v = – 1

ρ

∇ + p g + F

AccelerationAcceleration CoriolisCoriolis Press Gravity FrictionPress Gravity Friction

GradientGradient

du

dt+ (2Ωcosθ)w − fv = −

1

ρ

∂p

∂x+ Fx

dv

dt+ fu = −

1

ρ

∂p

∂y+ Fy

dw

dt+ (2Ωcosθ)u = −

1

ρ

∂p

∂z− ρg + Fz

x-equationx-equation

y-equationy-equation

z-equationz-equation(hydrostatic)(hydrostatic)

neglectneglect

neglectneglect neglectneglect

Page 22: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics GeostrophyGeostrophy

−fv = −1

ρ

∂p

∂x

+ fu = −1

ρ

∂p

∂y

x-equationx-equation

y-equationy-equation

CoriolisCoriolis PressPressGradientGradient

The (numerically) largest The (numerically) largest terms in the horizontal terms in the horizontal momentum equations for momentum equations for large-scale oceans large-scale oceans currents are the currents are the CoriolisCoriolis acceleration effect and acceleration effect and horiz. horiz. pressure gradientspressure gradients

Currents that follow this dynamical balance of forces Currents that follow this dynamical balance of forces (accelerations) are called (accelerations) are called GeostrophicGeostrophic, which means “earth , which means “earth turning”turning”

Note: these currents represent a Note: these currents represent a steady statesteady state balance balance

Page 23: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics

−fv = −1

ρ

∂p

∂x

+ fu = −1

ρ

∂p

∂y

High Elevation (pressure)

Low Elevation (pressure)

Coriolis Accel Press Grad

Start-up

period: not

in steady

state, geo-

strophic

balance

Steady state, geostrophic balance

set up between pressure gradient

and Coriolis acceleration

Initial movement is driven toward high pressure (or downhill) Initial movement is driven toward high pressure (or downhill) but Coriolis effect acts to turn track to the right (in the N.H.) and but Coriolis effect acts to turn track to the right (in the N.H.) and the final, steady state or equilibrium result is parallel to lines of the final, steady state or equilibrium result is parallel to lines of constant pressure (around the hill)constant pressure (around the hill)

Rule:Rule: with your left hand in the direction of with your left hand in the direction of low pressure, the wind/current will hit low pressure, the wind/current will hit you in the back (in the N.H.)you in the back (in the N.H.)

GeostrophyGeostrophy

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OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics

FFcc: Coriolis; : Coriolis; FFgg: Pressure Gradient (related to gravity): Pressure Gradient (related to gravity)

Rule:Rule: with your left hand in the direction of with your left hand in the direction of low pressure, the wind/current will hit low pressure, the wind/current will hit you in the back (in the N.H.)you in the back (in the N.H.)

GeostrophyGeostrophy

Page 25: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics GeostrophyGeostrophy

Page 26: OC3230-Paduan images Copyright © McGraw Hill Chap 9: Dynamics Light Transmission Solar heating supplies short-wave radiation to ocean surface; Energy (light)

OC3230-PaduanOC3230-Paduan images Copyright © McGraw Hillimages Copyright © McGraw Hill

Chap 9: DynamicsChap 9: Dynamics GeostrophyGeostrophy

The Dynamic Method (or Geostrophic Method) for computing The Dynamic Method (or Geostrophic Method) for computing ocean currents depends on density observations to estimate ocean currents depends on density observations to estimate pressure gradients and, finally, currentspressure gradients and, finally, currents

2 or more 2 or more ρρ profiles profiles pp

ΔΔ

u,vu,v

It is not possible to directly measure pressure because depth It is not possible to directly measure pressure because depth cannot be determined with enough accuracycannot be determined with enough accuracy

Recall the hydrostatic equation:Recall the hydrostatic equation:

Quantity gdz is related to amount of work to move a unit of Quantity gdz is related to amount of work to move a unit of mass a unit distance in the vertical direction; we define the mass a unit distance in the vertical direction; we define the geopotential, geopotential, , by: d, by: d = gdz = – = gdz = –ααdpdp

Dynamic Height, D = Dynamic Height, D = /10, is numerical equiv to height in m/10, is numerical equiv to height in m

Hydrostatic EqnHydrostatic Eqn

dp

dz

= –g ρ ; , = or gdz-1

ρ

= –dp α dp = d= d

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Chap 9: DynamicsChap 9: Dynamics GeostrophyGeostrophy

∂p

∂z= −ρg

∂p

∂zdz

z

η

∫ = − ρgdzz

η

∫p(η ) − p(z) = − (ρ o + γ)gdz = ρ ogz − γgdz

z

≈o

∫z

η

∫p(z) = patm − ρ og(z −η ) + γgdz

z

≈o

Hydrostatic eqnHydrostatic eqn

Integrate wrt depthIntegrate wrt depth

Let, Let, ρρ = = ρρoo + +

Solve for press at depth,Solve for press at depth,z < 0z < 0

SmallSmall “Barotropic” (depth“Barotropic” (depth “Baroclinic” (depth)“Baroclinic” (depth)atmos.atmos. independent)independent) dependent)dependent)pressurepressure

Note: Note: ρρoo >> >> We usually can’t obtain the barotropic portion so we:We usually can’t obtain the barotropic portion so we:1) Measure sea surface using satellite altimetry1) Measure sea surface using satellite altimetry2) Map velocity at one depth directly (current meters, floats)2) Map velocity at one depth directly (current meters, floats)3) Assume a 3) Assume a level of no motionlevel of no motion at some depth at some depth

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Chap 9: DynamicsChap 9: Dynamics

fu = −1

ρ

∂p

∂y= −g

∂η

∂y+

∂yg γdz

z

o

∫( )

GeostrophyGeostrophy

−fv = −1

ρ

∂p

∂x= −g

∂η

∂x+

∂xg γdz

z

o

∫( )

p(z) = patm − ρ og(z −η ) + γgdzz

≈o

Sea Surface SlopeSea Surface Slope InternalInternal(barotropic)(barotropic) (baroclinic)(baroclinic)

.

x

y

z

sea surface

isopycnals

level of no motion

Due to sea surface Due to isopycnals Total

Current Contributions:

Use Use p(z)p(z) solution in solution in geostophic equationsgeostophic equations

Typically Typically assume a assume a level of no level of no motion and motion and compute the compute the required required surface slope surface slope (or dynamic (or dynamic height)height)


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