1. 1 The Wind

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3. 3 The origin of wind The earth is unevenly heated by the sun resulting in the poles receiving less energy from the sun than the equator does. Also the dry land heats up (and cools down) more quickly than the seas do. The differential heating powers a global atmospheric convection system reaching from the earth's surface to the stratosphere which acts as a virtual ceiling.

4. 4 The atmosphere around the globe is a very thin layer. The globe has a diameter of 12,000 km. The troposphere, which extends to about 11 km altitude, is where all of our weather, and the greenhouse effect occurs. On the picture you can see a stretch of islands 300 km across, and the approximate height of the troposphere. To look at it at a different scale: If the globe were a ball with a diameter of 1.2 meters the atmosphere would only be 1 mm thick. The Atmosphere (Troposphere) Source: www.windpower.org

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6. 6 An estimated 1 to 3 % of energy from the Sun that hits the earth is converted into wind energy. This is about 50 to 100 times more energy than is converted into biomass by all the plants on earth through photosynthesis. Most of this wind energy can be found at high altitudes where continuous wind speeds of over 160 km/h occur. Eventually, the wind energy is converted through friction into diffuse heat all through the earth's surface and atmosphere.

7. 7 The wind resource The Geostrophic Wind Geographical variations Global circulations Annual and seasonal variations Synoptic and diurnal variations The surface boundary layer Turbulence The energy in the wind

8. 8 The Geostrophic Wind winds balanced by the Coriolis and Pressure Gradient forces An air parcel initially at rest will move from high pressure to low pressure because of the pressure gradient force. However, as that air parcel begins to move, it is deflected by the Coriolis force to the right in the northern hemisphere (to the left on the southern hemisphere). As the wind gains speed, the deflection increases until the Coriolis force equals the pressure gradient force. At this point, the wind will be blowing parallel to the isobars. When this happens, the wind is referred to as geostrophic. The geostrophic wind is found at altitudes above 1000 meters above ground level. Source: http://ww2010.atmos.uiuc.edu

9. 9 Geographical variations Different surface heating from the sun –High surface heating close to equator –Day and night differences The non-uniformity of the earth’s surface –Land masses and ocean –Hills an mountains

10. 10 Source: www.bergey.com

11. 11 Wind Resources at 50 (45) m Above Ground Level Color Sheltered Open At a sea Open sea Hills and terrain plain coast ridges Source: www.windpower.org

12. 12 Global circulations Source: Wind Power Plants, Fundamentals, Design, Construction and Operation. http://www.windpower.org/en/tour/wres/globwin.htm

13. 13 Global circulations Rossby circulation –Northern and southern hemisphere –Moves warm air to the poles and cold air to the subtropical areas Hadley circulation –Equatorial regions (30 o S – 30 o N) –Produces the constant wind systems of the north-east and south-east trade winds Monsoons –Large scale motion due to differences in temperature Indian ocean Atlantic ocean Africa Tropical cyclones –Rising hot humid air at the equatorial regions

14. 14 Annual and seasonal variations Year to year variation in annual wind speeds is hard to predict Characterized by probably distribution –Wind speed probability is calculated as a Weibull curve Where: FWind speed probability[ - ] kShape factor[ - ] AWeibull parameter[ - ] VWind velocity[m/s]

15. 15 Synoptic and diurnal variations Synoptic variations –Passage of weather systems Catabatic wind Diurnal variations –Predictable daily variations Sea land breeze Mountain top – mountain valley wind

16. 16 Catabatic wind Synoptic variation Source: Wind Power Plants, Fundamentals, Design, Construction and Operation.

17. 17 Sea land breeze Diurnal variation Source: Wind Power Plants, Fundamentals, Design, Construction and Operation.

18. 18 Sea land breeze Diurnal variation

19. 19 Surface Boundary Layer The principal effects governing the properties of the boundary layer: –Strength of the geostrophic wind –Surface roughness –Coriolis force –Thermal effects

20. 20 Vertical wind speed gradient Source: Wind Power Plants, Fundamentals, Design, Construction and Operation. And Wind Energy Handbook Where: h 1 Reference height [m] h 2 Height [m] z 0 Roughness length[m] v 1 Wind velocity at the reference height [m/s] v 2 Wind velocity [m/s]

21. 21 Obstacles on the ground Source: Wind Power Plants, Fundamentals, Design, Construction and Operation.

22. 22 The wind stream over hills Source: Wind Power Plants, Fundamentals, Design, Construction and Operation. The wind stream over hills with a gradient lower than 10% is accelerated at the hill top, but without disturbing stalls and turbulence. This is an excellent opportunity for utilizing the power in the wind

23. 23 Wind Spectrum Synoptic variations –Passage of weather systems Diurnal variations –Predictable daily variations Turbulence Source: Wind Energy Handbook

24. 24 Turbulence Turbulence refers to fluctuations in wind speed on a relatively fast time-scale, typically less than 10 min. Where: VWind velocity[m/s] VMean wind velocity[m/s] v’Turbulent velocity[m/s]

25. 25 The power and energy in the wind Where:  Density[kg/m 3 ] VWind velocity[m/s] AArea[m 2 ]

26. 26 Time [hours] Energy [MWh]

27. 27 Wind measurements The cup anemometer The vane anemometer The ultrasonic anemometer The hot-wire anemometer

28. 28 The wind Rose To show the information about the distributions of wind speeds, and the frequency of the varying wind directions, one may draw a so-called wind rose on the basis of meteorological observations of wind speeds and wind directions.