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Lecture 10 : Circulation

  Ekman Pumping  -Driven Circulation

ESS228 Prof. JinJin--YiYi Yu Basic Ocean Structures Warm up by sunlight!

 Upper Ocean (~100 m) Shallow, warm upper layer where light is abundant and where most can be found.

 Deep Ocean Cold, dark, deep ocean where plenty supplies of nutrients and carbon exist.

ESS228 No sunlight! Prof. JinJin--YiYi Yu Basic Ocean Systems

Upper Ocean surface circulation

Deep Ocean

deep ocean circulation

ESS228 (from “Is The Rising?” ) Prof. JinJin--YiYi Yu Vertical Structure of Ocean

Mixed Layer: T and S well mixed by

Temperature : large gradient of T and S

Salinity Deep Ocean: T and S independent of height cold salty high nutrient level

(from System Modeling ) ESS228 Prof. JinJin--YiYi Yu Processes  The depth of the mixed layer is determined by (1) the rate of generation and (2) the rate of kinetic energy supply.  The can affect the mixed layer through three processes: heating, wind forcing, and freshening (P-E).  The global-average depth of the mixed layer is about 70 m.  The heat capacity of the mixed layer is about 30 times the heat (from Global Physical ) capacity of the atmosphere.

ESS228 Prof. JinJin--YiYi Yu Seasonal Variation of Mixed Layer

 Summer: warm and thin.  : cold and deep (several hundred meters).

(from Global Physical Climatology ) ESS228 Prof. JinJin--YiYi Yu Two Circulation Systems

-driven wind-driven circulation (Figure from The System ) circulation ESS228 Prof. JinJin--YiYi Yu Global Surface Currents

(from Modeling ) ESS228 Prof. JinJin--YiYi Yu Six Great Current Circuits in the World Ocean

 5 of them are geostrophic gyres: Indian

 The 6 th and the largest current: Antarctic Circumpolr Current (also called West Wind Drift)

(Figure from by Tom Garrison)

ESS228 Prof. JinJin--YiYi Yu Characteristics of the Gyres (Figure from Oceanography by Tom Garrison)  Currents are in geostropic balance  Each gyre includes 4 current components: two boundary currents: western and eastern two transverse currents: easteward and westward Western (jet stream of ocean) the fast, deep, and narrow current moves warm water polarward (transport ~50 Sv or greater) Eastern boundary current the slow, shallow, and broad current moves cold water equatorward (transport ~ 10-15 Sv) Trade wind-driven current the moderately shallow and broad westward current (transport ~ 30 Sv) Westerly-driven current the wider and slower (than the trade wind-driven Volume transport unit: current) eastward current 1 sv = 1 Sverdrup = 1 million m 3/sec ESS228 (the Amazon river has a transport of ~0.17 Sv) Prof. JinJin--YiYi Yu Major Current Names

 Western Boundary Current  Trade Wind-Driven Current (in the North Atlantic) (in the North Pacific) (in the South Atlantic) Eastern Australian Current (in the South Pacific) (in the )

 Eastern Boundary Current  Westerly-Driven Current (in the North Atlantic) (in the North Atlantic) Current (in the North Pacific) (in the North Pacific) (in the South Atlantic) Peru Current (in the South Pacific) Western Australian Current (in the Indian Ocean)

ESS228 Prof. JinJin--YiYi Yu Gulf Stream

A river of current

Jet stream in the ocean

 Speed = 2 m/sec  Depth = 450 m  Width = 70 Km  Color: clear and blue

(Figure from Oceanography by Tom Garrison) ESS228 Prof. JinJin--YiYi Yu Surface Current ––GeostrophicGeostrophic Gyre

 Mixed Layer Currents controlled by frictional + force  wind-driven circulation  Ekman transport (horizontal direction)  convergence/divergence  / at the bottom of mixed layer

 Thermocline downwelling/upwelling in the mixed layer  gradient force +   Sverdrup transport (horizontal)

ESS228 Prof. JinJin--YiYi Yu Step 1: Surface Winds

Oceanography (Figure from by Tom Garrison) ESS228 Prof. JinJin--YiYi Yu Winds and Surface Currents

Polar Cell Ferrel Cell

Hadley Cell

(Figure from The Earth System ) ESS228 Prof. JinJin--YiYi Yu Step 2: (frictional force + Coriolis Force)

Oceanography (Figure from by Tom Garrison) ESS228 Prof. JinJin--YiYi Yu ––AA Result of Coriolis Force

ESS228 (Figure from The Earth System ) Prof. JinJin--YiYi Yu Formula for Ekman Transport

ESS228 Prof. JinJin--YiYi Yu How Deep is the Ekman Layer?

 D ∝ (ν/f)1/2

ν = vertical diffusivity of momentum f = Coriolis parameter = 2 Ωsin φ

(from Climate System Modeling ) ESS228 Prof. JinJin--YiYi Yu Ekman Transport

(Figure from The Earth System ) ESS228 Prof. JinJin--YiYi Yu Step 3: Geostrophic Current (Pressure Gradient Force + Corioils Foce)

NASA-TOPEX Observations of -Level Hight

(from Oceanography by Tom Garrison)

ESS228 Prof. JinJin--YiYi Yu Ekman Transport  Convergence/Divergence

(Figure from The Earth System ) Surface wind + Coriolis Force

Ekman Transport

Convergence/divergence Thermocline (in the center of the gyre)

Pressure Gradient Force

Geostrophic Currents

ESS228 Prof. JinJin--YiYi Yu Geostrophic Current

Forces Geostrophic Gyre Currents

(Figure from The Earth System ) ESS228 Prof. JinJin--YiYi Yu Sverdrup Transport

• Continuity equation for an incompressible flow:

Ekman layer pumping  vertical depth decreases • Assume the horizontal flows are geostrophic:  move equatorward to conserve absolute .

• Replace the geostrophic flow pressure gradients:

Ekman layer suction • The continuity equation becomes:  vertical depth increases  move poleward to conserve absolute vorticity.

ESS228 Prof. JinJin--YiYi Yu Sverdrup Transport

• • Continuity equation for an incompressible flow: Integrate the equation from the bottom of the upper ocean (D w) to the bottom of the Ekman layer (D E): assume zero

• Assume the horizontal flows are geostrophic: • ѡ Ekman pumping ( E) is related to the convergence of the Ekman transport: • Replace the geostrophic flow pressure gradients:

• Therefore, we obtain:

• The continuity equation becomes: geostrophic Sverdrup - (Ekman transport transport Transport) • Therefore, ESS228 Sverdrup transport = Geostrophic transportProf. + JinJin--YiEkmanYi Yu transport Ekman and Sverdrup Transports

Eq E W E 90 °N

Ekman Layer

Ekman Pumping Ekman Suction (w<0) (w>0)

Equatorward Poleward Sverdrup Transport Sverdrup Transport

ESS228 Subtropical Gyre Prof. JinJin--YiYi Yu Conservation of Potential Vorticity

Pole  Potential Vorticity PV = f + ζ H f = planetary vorticity = 2 Ωsin φ f1 (ζζζ <<<0) 1 ζ = relative vorticity = ∂v/∂x- ∂u/∂y

 f1 + ζ1 = f 2 + ζ2

since f 1 > f2  ζ1 < ζ 2  If ζ < 0 , the vortex decreases rotation when f2 H moves toward lower and increases (ζζζ2> ζζζ1) rotation when moves toward higher latitudes.

Equator ESS228 Prof. JinJin--YiYi Yu Boundary Currents

(Figure from The Earth System ) ESS228 Prof. JinJin--YiYi Yu Step 4: Boundary Currents

Oceanography (Figure from by Tom Garrison) ESS228 Prof. JinJin--YiYi Yu Boundary Currents

Eastern boundary currents: broad and weak

Western boundary currents: narrow and strong ESS228 Prof. JinJin--YiYi Yu Eastern Boundary Current

 Cold water from higher ocean.  Costal upwelling associated with subtropical high pressure system.  Atmospheric subsidence produce persistent stratiform clouds, which further cool down SSTs by blocking (from Global Physical Climatology ) solar radiation.

ESS228 Prof. JinJin--YiYi Yu Costal Upwelling/Downwelling

 A result of Ekman transport and mass continuity.

(Figure from Oceanography by Tom Garrison)

ESS228 Prof. JinJin--YiYi Yu Global Surface Currents

ESS228 Prof. JinJin--YiYi Yu