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Part 1. Energy and Mass Chapter 4. Atmospheric Pressure and Wind.

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Presentation on theme: "Part 1. Energy and Mass Chapter 4. Atmospheric Pressure and Wind."— Presentation transcript:

1 Part 1. Energy and Mass Chapter 4. Atmospheric Pressure and Wind

2 Introduction Pressure = Force per unit area Gases exert equal pressure in all directions Average atmospheric pressure is controlled by the “weight” of overlying air--it decreases with height Average sea level air pressure is 1013.25 mb Air pressure changes depending on the air density and temperature Dalton’s Law: Where several different gases are mixed, the total gas pressure is equal to the sum of the partial pressures of the individual gases

3 Air pressure is less at a higher elevation (p 2 ) than at a lower elevation (p 1 ) Gravity is always trying to pull the air downward toward the Earth’s surface

4 Air pressure decreases with elevation according to this curve Meteorologists use air pressure as a measure of elevation in the atmosphere (i.e., the 500 mb level or the 200 mb level)

5 The Equation of State (Ideal Gas Law) For a gas, the following measurable parameters are inter-related: Pressure Temperature Density Changes in air pressure occur with changes in air temperature or density (or both)

6 Molecular movement in a sealed container Pressure increases by increasing density (b) or temperature (c)

7 Aneroid barometer (left) and its workings (right) A barograph continually records air pressure through time

8 The distribution of air pressure is important for determining weather patterns Air always tries to move from higher pressure to lower pressure The greater the pressure difference between high and low pressure, the greater the force trying to move the air Isobars = lines of equal air pressure Pressure gradient = change in pressure with distance Steep pressure gradients are represented by closely spaced isobars

9 Sea level air pressure depicted on a weather map Air pressure measurements made at high elevations must be corrected to give the air pressure at sea level High pressure gradient area (windy) Low pressure gradient area (calm)

10 Pressure Gradient Force Initiates air motion –High to lower pressure –Wind speed reflects gradient Horizontal Pressure Gradients Usually small across large spatial scales Vertical Pressure Gradients Usually greater than horizontal gradients Pressure always decreases with altitude

11 Hydrostatic Equilibrium = Force of gravity balances vertical air pressure gradient Local imbalances in hydrostatic equilibrium cause updrafts and downdrafts

12 Heating causes a density decrease in a column of air All columns have the same total mass Warmer air has lower density and therefore greater column height Both air columns are at the same temperature The air in the right column is warmer than the air in the left column

13 500 mb height contours for May 3, 1995 Upper air pressure maps depict the height to the specific air pressure level (such as the height to the 500 mb air pressure level) 500 mb elevation 5880 m 500 mb elevation 5280 m Lines of equal elevation

14 Upper air heights decrease with latitude Warmer air in south, 500 mb level at higher elevation Colder air in south, 500 mb level at lower elevation

15 Forces that Affect the Speed and Direction of Winds 1) The Pressure Gradient Force (pgf): Air tries to move from areas of high pressure to areas of low pressure; a larger pressure gradient gives a larger pgf and faster winds

16 2) The Coriolis Force Free-moving objects are affected by the Earth’s rotation; the coriolis force causes an apparent deflection to the right in the northern hemisphere and to the left in the southern hemisphere The coriolis force is greater at high latitudes than at low latitudes The faster the air is moving, the greater the coriolis force on the air

17 Coriolis Deflection

18 3) The Friction Force The friction force acts in the opposite direction from the direction of movement of the air; it acts to slow the air movement Air friction if greatest near the Earth’s surface Above an elevation of 1.5 km (1500 m or about 4500 ft), air friction is negligible

19 Winds in the Upper Atmosphere are affected by only the pressure gradient force and the Coriolis force When the pressure gradient force balances with the Coriolis force, the result is the geostrophic wind (parallel to the isobars)

20 Free Atmosphere (no friction) Pressure Gradient This plot shows the direction of the pressure gradient force at the 500 mb level. The pgf is always perpendicular to the isobars.

21 Geostrophic Flow Development (a) Air particle starts moving (b) As air starts moving, it starts being affected by the Coriolis force (c) Faster air movement results in a larger Coriolis force (d) When the pgf and the Coriolis force become equal and opposite, the geostrophic wind results

22 If the pgf and Coriolis forces never balance, Supergeostrophic and Subgeostrophic Flow results Supergeostrophic and subgeostrophic flows follow curved air pressure contours Supergeostrophic flow occurs in ridges Subgeostrophic flow occurs in troughs These flows are called Gradient flows

23 Supergeostrophic flow Subgeostrophic flow High pressure “ridge” Low pressure “trough”

24 Gradient Wind

25 Cyclones, Anticyclones, Troughs, and Ridges High pressure areas (anticyclones) Clockwise motion in northern hemisphere Descending air Clear skies Low pressure areas (cyclones) Counterclockwise motion in northern hemisphere Ascending air Clouds Upper atmosphere Ridges = surface anticyclones Troughs = surface cyclones

26 Due to friction, near surface air crosses isobars at an angle

27 Northern and Southern Hemisphere anticyclonic air patterns

28 Northern and Southern Hemisphere cyclonic air patterns

29 Ridges and troughs in the northern hemisphere

30 Maps depicting troughs, ridges, cyclones, and anticyclones

31 Measuring Wind Wind direction indicates direction from which wind blows Azimuth = degree of angle from 0 to 360 o Wind vanes indicate wind direction Anemometers record wind speed Aerovanes indicate wind speed and direction

32 An aerovane An azimuth

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