Introduction to Atmospheric Circulation

Transcription

1 Introduction to Atmospheric Circulation

2 Start rotating table

3 Cloud Fraction Dice Results

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5 from

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7 Earth s Energy Budget At low latitudes, more solar radiation is absorbed than emitted back to space At high latitudes, less solar radiation is absorbed than emitted back to space The atmosphere and ocean transport energy from low latitudes to high latitudes to maintain energy balance Sun Earth

8 Set up tubs

9 Temperature, Density and Pressure Warm air and warm water are less dense than cold air and cold water Hydrostatic pressure is caused by the weight of overlying air or water warm cold less dense more dense lower pressure less weight higher pressure more weight

10 Hydrostatic Equation p = ρ g h density ρ 1,000 kg m -3 (water) 1 kg m -3 (air at sea level) acceleration of gravity g 10 m s -2 depth of fluid h 4,000 m (ocean) 10,000 m (atmosphere) Atmospheric pressure at sea level? Pressure at the bottom of the ocean? units should be N m -2 Reference: my body weight is about 1000 Newtons (kg m s -2 )

11 Hydrostatic Equation p = ρ g h density ρ 1,000 kg m -3 (water) 1 kg m -3 (air at sea level) acceleration of gravity g 10 m s -2 depth of fluid h 4,000 m (ocean) 10,000 m (atmosphere) Atmospheric pressure at sea level? 100,000 N m -2 Pressure at the bottom of the ocean? 40 million N m -2 Reference: my body weight is about 1000 Newtons (kg m s -2 )

12 Hydrostatic Equation p = ρ g h density ρ 1,000 kg m -3 (water) 1 kg m -3 (air at sea level) acceleration of gravity g 10 m s -2 depth of fluid h 4,000 m (ocean) 10,000 m (atmosphere) Atmospheric pressure at sea level? 100,000 N m -2 (100 Norris m -2 ) Pressure at the bottom of the ocean? 40 million N m -2 (40,000 Norris m -2 ) Reference: my body weight is about 1000 Newtons (kg m s -2 )

13 Temperature, Density and Pressure Warm air and warm water rise, cold air and cold water sink Fluid flows from high pressure to low pressure warm cold less dense lower pressure less weight fluid flow more dense higher pressure more weight

14 Tub experiment

15 Hadley Circulation Sun heats air most strongly near equator Warm air rises in Intertropical Convergence Zone Warm air is less dense and surface pressure is lower warm lower pressure Intertropical Convergence Zone Higher Latitudes

16 Hadley Circulation High above surface, warm air moves poleward Air cools by emitting thermal radiation to space Cool air sinks warm cool lower pressure Intertropical Convergence Zone Higher Latitudes

17 Hadley Circulation Cool air is more dense and surface pressure is higher Higher pressure pushes air towards lower pressure Near surface, cool air moves equatorward in Trade Winds warm cool Hadley Circulation lower pressure Intertropical Convergence Zone Trade Winds higher pressure Higher Latitudes

18 Earth s Rotation from

19 Put ice in rotating table

20 Conservation of Angular Momentum If no torque (force in direction of rotation), then angular momentum is conserved R 1 V 1 = R 2 V 2 R = distance from axis of rotation V = velocity V R

21 Conservation of Angular Momentum If no torque (force in direction of rotation), then angular momentum is conserved R 1 V 1 = R 2 V 2 V 2 R 2 V 1 R 1 R 1 < R 2 V 1 > V 2

22 Conservation of Angular Momentum Imagine that air at the equator is rotating at the same rate as the Earth. What is the speed of the wind relative to the Earth? V 2 R 2 V 1 R 1

23 Conservation of Angular Momentum Imagine that air at the equator is rotating at the same rate as the Earth. What is the speed of the wind relative to the Earth? V 2 R 2 V 1 R 1 Zero.

24 Conservation of Angular Momentum Imagine that air at the equator is rotating at the same rate as the Earth. Imagine that this air moves poleward while conserving angular momentum. V 2 R 2 V 1 R 1 Is the air now rotating faster, slower, or the same as Earth?

25 Conservation of Angular Momentum Imagine that air at the equator is rotating at the same rate as the Earth. Imagine that this air moves poleward while conserving angular momentum. V 2 R 2 V 1 R 1 Is the air now rotating faster, slower, or the same as Earth? Faster.

26 Conservation of Angular Momentum Imagine that air at the equator is rotating at the same rate as the Earth. Imagine that this air moves poleward while conserving angular momentum. V 2 R 2 V 1 R 1 What is the direction of the wind relative to the Earth? (from the west or from the east?)

27 Earth s Rotation from

28 Conservation of Angular Momentum Imagine that air at the equator is rotating at the same rate as the Earth. Imagine that this air moves poleward while conserving angular momentum. V 2 R 2 V 1 R 1 What is the direction of the wind relative to the Earth? From the west (westerly).

29 Conservation of Angular Momentum Imagine that air at 30 N is rotating at the same rate as the Earth. Imagine that this air moves equatorward while conserving angular momentum. V 2 R 2 V 1 R 1 Is the air now rotating faster, slower, or the same as Earth?

30 Conservation of Angular Momentum Imagine that air at 30 N is rotating at the same rate as the Earth. Imagine that this air moves equatorward while conserving angular momentum. V 2 R 2 V 1 R 1 Is the air now rotating faster, slower, or the same as Earth? Slower.

31 Conservation of Angular Momentum Imagine that air at 30 N is rotating at the same rate as the Earth. Imagine that this air moves equatorward while conserving angular momentum. V 2 R 2 V 1 R 1 What is the direction of the wind relative to the Earth? (from the west or from the east?)

32 Earth s Rotation from

33 Conservation of Angular Momentum Imagine that air at 30 N is rotating at the same rate as the Earth. Imagine that this air moves equatorward while conserving angular momentum. V 2 R 2 V 1 R 1 What is the direction of the wind relative to the Earth? From the east (easterly).

34 Hadley Circulation and Trade Winds

35 Examine rotating table

36 Is Momentum Always Conserved? Imagine that air at the equator is rotating at the same rate as the Earth. Imagine that this air moves to the North Pole while conserving angular momentum. V 2 R 2 V 1 R 1 What is the speed of the wind relative to the Earth?

37 Is Momentum Always Conserved? Imagine that air at the equator is rotating at the same rate as the Earth. Imagine that this air moves to the North Pole while conserving angular momentum. V 2 R 2 V 1 R 1 What is the speed of the wind relative to the Earth? Infinite!

38 The Jet Stream High above the surface, air moves poleward from the equator The wind becomes strongly westerly due to conservation of angular momentum The jet stream is so fast, that instabilities (waves or eddies) develop Momentum is no longer conserved These eddies transport heat farther poleward (and produce weather)

39 The Jet Stream

40 The Jet Stream

41 Jet stream animation

42 Examine rotating table

43 Extratropical Cyclones

44 Extratropical Cyclones

45 Extratropical Cyclones

46 The Jet Stream and Clouds

47 Heat Transport by Eddies Warm goes poleward Cold goes equatorward