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

2. 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.

3. Because of earth’s rotation we have several circulation cells not just one per hemisphere Global Circulation

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

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

6. Semi-Permanent Pressure (January)

7. 500-mb streamline and isotherms in January

8. Stronger Winter PGF

9. Semi-Permanent Pressure (July)

10. 500-mb streamline and isotherms in July

13. Weaker Summer PGF

14. 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

15. Equatorial Cumulus and Thunderstorms ITCZ

16. India Monsoon Precipitation

17. Monsoons (dry)

18. Monsoons (wet)

19. Subtropical High and the ITCZ (Sahara)

20. Sahara Desert and the Sahel of Africa

23. Jet Locations Jet stream locations greatly affect local and global climate.

24. Jet Formation Sharply varying pressure and temperature differences create the exaggerated situation shown. Tightly packed isobars create stronger winds aloft in the frontal region.

25. Polar Jet Winds 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.

26. Seasonal Polar Jet Changes Location and Velocity variations

27. What cause the jets? L = m v r –r = distance from rotational axis –m = mass –v = velocity

28. Fig. 4, p. 270

29. Higher Angular Momentum, Yields more zones? Jupiter’s Bands

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

31. The Dishpan Experiment Uneven heating of the equator and poles of the earth. Rotation. Viscosity and turbulence.

32. Rossby Waves Kinking in the jet stream occurs on a cyclic basis. Weather patterns are also somewhat cyclic.

33. Rossby Cycle A complete Rossby cycle observed over ~ 6 weeks.

35. Ocean Currents

36. Gulf Stream

37. Coastal Upwelling

38. Ekman spiral, Ekman layer, and Ekman transport

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

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

41. 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.

42. Fig. 10-21b, p. 276

43. 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

44. Weather pattern changes during El Nino condition

45. Weather pattern changes during La Nina condition

46. Global hydrological impacts of El Nino

47. Pacific Decadal Oscillation (PDO)

50. North Atlantic Oscillation (NAO)

51. Fig. 10-26a, p. 280

52. Fig. 10-26b, p. 280