40
Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory [email protected]

Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory [email protected]

  • View
    214

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Ocean Stratification and Circulation

Martin VisbeckDEES, Lamont-Doherty Earth Observatory

[email protected]

Page 2: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

General Atmosphere Ocean CirculationThe surface energy balance

Top of atmosphere

Air-sea interface

seafloor

Imbalance of energy flux at the top can be balanced by:

Atmospheric Heat Transport

Oceanic Heat Transport

Page 3: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Sea Surface Temperature

The link between ocean and climate depends on exchange of energy (mainly heat and radiation) and materials (water, gases) across the sea surface. T atmosphere 'sees', influences and responds to the sea surface temperature (SST), by way of sea-air heat flux. SST generally cools with increasing latitude, but important deviations from a pure latitudinal dependence occurs. These are generally due to the movement of sea water in both the horizontal and vertical directions. Temperature and density of ocean water are related inversely: warm water means low density, cold water means denser sea water.

Page 4: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Ocean Salinity

As the range of salt concentration in the ocean varies from about 3.2 to 3.8%, oceanographers, who refer to salt content as 'salinity', express salt concentration as parts per thousand; 34.9 ppt is the average salinity.

Page 5: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Ocean Salinity

The more saline, the denser the sea water

Density of sea water is a function of temperature and salinity, both play an important role

Page 6: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Stratification

Waters warmer than 10°C dominate the sea surface but do not extend much below 500 m in the ocean; the warm waters provide just a veneer of warmth over a cold ocean. The sharp drop off in temperature with depth is called the thermocline. Deeper cold waters derive their properties at the sea surface during winter at high latitude.

Page 7: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Ocean simulation in tank

Cool waterlightlight

Page 8: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Ocean Propertie

s Temperature

Salinity Diagramsat the surface

Page 9: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Ocean Propertie

s Temperature

Salinity at 150 meter water depth

Page 10: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Ocean Propertie

s Temperature

Salinity at 500 meter water depth

Page 11: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Ocean Propertie

s Temperature

Salinity at 1000 meter water depth

Page 12: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Ocean Propertie

s Temperature

Salinity at 3000 meter water depth

Page 13: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

How does the Ocean move heat?

Top of atmosphere

Atmosphere

Ocean

Page 14: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Effect of Atmospheric Forcing on Ocean

Page 15: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Ocean Circulation

Ocean circulation is produced by:

1) the wind stress acting on the sea surface and

2) by buoyancy (heat and freshwater) fluxes between the ocean and atmosphere.

The former induces the wind driven ocean circulation, the latter the thermohaline circulation.

Page 16: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Ocean Circulation

The wind driven flow is by far the more energetic and for the most part resides in the upper kilometer.

The sluggish thermohaline circulation forces ocean overturning reaching in some regions to the sea floor, resulting in the formation of the major water masses of the global ocean:

North Atlantic Deep Water and

Antarctic Bottom Water.

Page 17: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Wind Driven Ocean Circulation

The wind driven circulation, which by far is the more energetic, though confined mostly to the upper kilometer of the ocean and generally moves water in the horizontal plane.

Page 18: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Wind Driven Ocean Circulation

How, does the wind induce an ocean circulation?

The wind exerts a force or stress on the ocean surface. This stress is proportional to the square of the wind speed. This produces ocean waves and ocean currents. The wind makes the surface layer of the ocean move ….

Page 19: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Wind Driven Ocean Circulation

The wind makes the surface layer of the ocean move, though not in the way that intuition might dictate - its not in the direction of the wind stress, but rather at an angle to it.

This is because of the Coriolis Force.

Eventually a balance is achieved between the wind stress and the Coriolis Force. The surface Ekman layer extends to about 100 to 300 meters depth, is a boundary layer feature in which the direct stress of the wind are felt.

Page 20: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Wind Driven Ocean Circulation

The transport within the Ekman layer is 90° towards the right of the wind in the northern hemisphere, to the left in the southern hemisphere.

The Ekman transport is proportional to the wind stress, which is proportional to the square of the wind speed. Typically a surface current is around 2 or 3% of the wind speed.

Page 21: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Wind Driven Ocean Circulation

One clear effect of the Ekman transport can be seen in the eastern side of the subtropical ocean where cold subsurface water is pumped up to the sea surface from a depth of perhaps 200 meters as the sea surface water is forced offshore by the Ekman transport. These regions are rich in nutrients and support important fisheries. The cold SST of these regions also induce a specific climate, called Cape Verde climate, one of a very stable atmosphere, cool, fog, few storms.

Page 22: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Large Scale Wind Driven Ocean Circulation

It is this movement that produces the wind driven circulation of the ocean.

How?

Well the wind field changes in its strength and direction from place to place. This causes Ekman transport to either pile up water (convergence) in some places or remove it (divergence) in other regions. As surface water is less dense than deeper water this has the effect of heaping buoyant water in the convergence regions and removing it from the divergence regions.

Page 23: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Large Scale Wind Driven Ocean Circulation

The hills and valleys of the sea surface produced by the convergence and divergent causes a sea level relief (difference from lowest to highest sea level, neglecting tides and waves) of around 2 meters.

Page 24: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Large Scale Wind Driven Ocean Circulation

The wind produces convergences and divergences of surface water, which causes hills and depressions in sea level, which produce a horizontal gradient of pressure, or a pressure head reaching down to perhaps 1000 meters.

Convergent hills have an outward directed pressure gradient, depression an inward directed pressure gradient.

Page 25: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Large Scale Wind Driven Ocean Circulation

As the pressure gradients make the water move from high pressure to low pressure, the Coriolis Force starts its action, and eventually a balance is achieved in these two forces, the horizontal pressure gradient equals the magnitude of the Coriolis Force, but is directed in the opposite direction.

This balance is called the geostrophic balance, and a current in such a balance is called a geostrophic current. Ocean currents are very close to being in geostrophic balance

Page 26: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Large Scale Wind Driven Ocean Circulation

As the pressure gradients make the water move from high pressure to low pressure, the Coriolis Force starts its action, and eventually a balance is achieved in these two forces, the horizontal pressure gradient equals the magnitude of the Coriolis Force, but is directed in the opposite direction.

This balance is called the geostrophic balance, and a current in such a balance is called a geostrophic current. Ocean currents are very close to being in geostrophic balance

Page 27: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Large Scale Wind Driven Ocean Circulation

Page 28: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

How does the Ocean move heat?

Top of atmosphere

Atmosphere

Ocean

Page 29: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Buoyancy Driven Ocean Circulation

The buoyancy forces are capable of inducing overturning that reach from the sea surface to the sea floor.

Buoyancy fluxes are those fluxes between air and water that alter the density of the sea water.

Cooling of the ocean and evaporation makes the ocean (colder, saltier) denser, removing buoyancy.

Heating and excess precipitation has the opposite effect, they add buoyancy to the ocean.

Page 30: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Overturning

North Atlantic Deep Water

Antarctic Bottom Water

Intermediate Water

Page 31: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Overturning

North Atlantic Deep Water

Antarctic Bottom Water

Intermediate Water

Page 32: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Oceanic Heat Transport

Page 33: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Overturning

North Atlantic Deep Water

Antarctic Bottom Water

Intermediate Water

Page 34: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Intermediate Water

At the base of the thermocline is the low salinity Antarctic Intermediate water derived from the Antarctic Circumpolar Current.

Page 35: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

The Oceans Role in Climate

The sum of the wind driven and buoyancy driven ocean current transport large amounts of heat and fresh water over large distances.

Can you rationalise the signs?

Page 36: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Atmospheric Heat Transportsimulation in tank

Cool waterlightlight

Page 37: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Atmospheric Heat Transportsimulation in tank

Cool waterlightlight

Page 38: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Ocean Heat Transportsimulation in tank

Cool waterlightlight

Page 39: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Atmosphere-Ocean Heat Transportsimulation in tank

Cool waterlightlight

Atmosphere

Ocean

Why is the ocean heat transport so much smaller than the one in the atmosphere?

Page 40: Ocean Stratification and Circulation Martin Visbeck DEES, Lamont-Doherty Earth Observatory visbeck@ldeo.columbia.edu

Some Final Remarks

The atmosphere carries: • 75 percent of the heat transport in the Northern Hemisphere and• 90 percent in the Southern Hemisphere

• It would take a million 1,000-megawatt electric power stations - the largest power plants now used - to produce a quantity of energy equivalent to the heat the atmosphere carries on average from the tropics to polar regions.