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GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

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GEU 0027: Meteorology Lecture 10 Wind: Global Systems
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Page 1: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

GEU 0027: MeteorologyLecture 10

Wind: Global Systems

Page 2: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Global Circulation• In the absence of rotation, air would tend to flow from the equator toward the poles.

Hot, less dense air

rising at the equator,

becomes denser as

it cools and descends

at the poles, traveling

back to tropical areas

to heat up again.

Page 3: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

• Because of earth’s rotation we have several circulation cells not just one per hemisphere

Global Circulation

Page 4: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

• With the 3 cell structure of wind circulation and the combination of PGF and Coriolis, semi-permanent circulation patterns are established.

Three-cell Model

Page 5: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Semi-permanent structures in the atmosphere provide consistent wind patterns and breeding grounds for air masses.

Semi-permanent Pressure and Winds

Page 6: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Semi-Permanent Pressure (January)

Page 7: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

500-mb streamline and isotherms in January

Page 8: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Stronger Winter PGF

Page 9: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Semi-Permanent Pressure (July)

Page 10: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

500-mb streamline and isotherms in July

Page 11: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.
Page 12: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.
Page 13: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Weaker Summer PGF

Page 14: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

• ITCZ

• Hot equatorial air rises in convection.

• Air moves away from the equator toward the poles.

• Low Pressure results around the equator.

• A band of convective thunderstorms circles the tropical areas of the globe.

Intertropical Convergence Zone

Page 15: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

• Equatorial Cumulus and Thunderstorms

ITCZ

Page 16: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

India Monsoon Precipitation

Page 17: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Monsoons (dry)

Page 18: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Monsoons (wet)

Page 19: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Subtropical High and the ITCZ (Sahara)

Page 20: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Sahara Desert and the Sahel of Africa

Page 21: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.
Page 22: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.
Page 23: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Jet Locations

Jet stream locations

greatly affect

local and global

climate.

Page 24: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Jet FormationSharply varying pressure and

temperature differences create the

exaggerated situation shown.

Tightly packed isobars create stronger

winds aloft in the frontal region.

Page 25: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Polar JetWinds are Westerly

and parallel to the

frontal boundary.

This creates the

polar jet stream.

It is strongest in the

winter and weakest

in the summer.

Page 26: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Seasonal Polar Jet Changes• Location and Velocity variations

Page 27: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

What cause the jets?

•L = m v r – r = distance from

rotational axis

– m = mass

– v = velocity

Page 28: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Fig. 4, p. 270

Page 29: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

• Higher Angular Momentum, Yields more zones?

Jupiter’s Bands

Page 30: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Wind Jets• Other jet formation mechanisms are less well known.

Page 31: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

The Dishpan Experiment

• Uneven heating of the equator and poles of the earth.• Rotation.• Viscosity and turbulence.

Page 32: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Rossby WavesKinking in the jet

stream occurs on

a cyclic basis.

Weather patterns

are also somewhat

cyclic.

Page 33: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Rossby CycleA complete

Rossby cycle

observed over

~ 6 weeks.

Page 34: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.
Page 35: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Ocean Currents

Page 36: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Gulf Stream

Page 37: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Coastal Upwelling

Page 38: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Ekman spiral, Ekman layer, and Ekman transport

Page 39: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Normal South Pacific Condition• Easterly “trade-winds” usually prevail and upwelling occurs• When exceptionally strong this cooling is called a La Nina.

Page 40: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

El Nino• During an El Nino, pressure conditions (and winds) reverse.• Extremely warm water and wind reversal affects weather.

Page 41: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Sea Surface Temperatures

A warm water wave

migrates eastward

during and El Nino

as upwelling and

cooling is severely

diminished along

the western coast

of S. America.

Page 42: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Fig. 10-21b, p. 276

Page 43: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

El Nino and La Nina events, and ENSO Cycle• La Nina versus El Nino conditions over the past 60 years.• The Y-axis is a parameter calculated from a combination of:

– air temperature

– water temperature

– air pressure (sea-level)

– wind speed and direction

– cloud cover

Page 44: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Weather pattern changes during El Nino condition

Page 45: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Weather pattern changes during La Nina condition

Page 46: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Global hydrological impacts of El Nino

Page 47: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Pacific Decadal Oscillation (PDO)

Page 48: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.
Page 49: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.
Page 50: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

North Atlantic Oscillation (NAO)

Page 51: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Fig. 10-26a, p. 280

Page 52: GEU 0027: Meteorology Lecture 10 Wind: Global Systems.

Fig. 10-26b, p. 280


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