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Wind Blow

 

Overview

Anyone who has ever lived through the fury of a hurricane or witnessed the destructive power of a twister knows just how much punch the wind can pack! What many people don't realize is that when they see the wind blow, they're really watching the power of the sun! On Earth, our surface is surrounded by an ocean of air called the atmosphere, which, like water, is quite fluid. Just like there are currents in the ocean, our atmosphere has wind currents controlled by many of the same factors, including temperature differences, density differences, and the spin of the planet. Most winds get started because of local changes in the density of air. As with most matter, when air is heated, it expands, causing it to become less dense. Just like in a hot-air balloon, warm air is buoyant. Cool air, which is more dense, moves in and literally pushes the warmer air up, or, in common terms, the warm air rises. We sense the motion as wind. All of the energy to heat the air comes from the sun, but in general the sun heats the air indirectly. Solar radiation in the form of visible light penetrates our atmosphere and strikes Earth's surface, where it's converted into heat and, as described above, begins to rise. Since the surface of the Earth is quite variable in its makeup (rock, tree, water, and pavement), the air is not heated evenly. Instead, separate pockets of rising warm air masses called thermals are formed, ultimately driving the local wind directions. While small variations in Earth's surface help to cause localized wind conditions, differential heating and cooling of the atmosphere generates global-scale winds as well. Hot air rising over the equator pushes northward and southward. Upper atmosphere cooling causes the hot air masses to become more dense and sink. Once near the warm Earth, the air heats up and rises again. A vertically circling flow of air, called convection cells, results. The cyclic motion of these air masses is further modified by Earth's own rotation, deflecting them to the east and west. Known as the Coriolis effect, this rotation deflection is what gives rise to the global wind belts including the polar easterlies, mid-latitude westerlies, and tropical trade winds.

Activity

Convection cells are circular currents of air that result when hot air rises into the upper atmosphere, cools and contracts, sinks down near the Earth's surface, heats up and expands, and then rises again. The rotation of Earth causes these air masses to move in the form of wind. In this activity, you'll create small convection cells and watch their patterns as you put the spin on them. Materials
  • 2 aluminum pie pans
  • opaque, white dishwashing liquid
  • red or green food coloring with a dropper
  • candle in a holder and matches
  • watch with second hand 1. Fill one of the aluminum pie plates with a half inch of dishwashing liquid. Fill the other plate with a half inch of water. 2. Using the plate with the dishwashing liquid, place several drops of food coloring about halfway between the center and the edge of the plate. 3. Light the candle and place it in its holder. Hold the plate over the candle so that the drops of food coloring are directly over the flame. Wait about 45 seconds and observe what happens to the drops of food coloring. Describe how they look and how they move. 4. When heated, your drops of food coloring act like convection cells that form near Earth's surface. To see how the Earth's rotation might affect these cells, place the first pie plate into the pie plate containing water and spin it for about 30 seconds. Describe the patterns that are formed. Questions 1. How did the shape of the convection cells change as you heated the plate? 2. The patterns that formed when you spun the plate can be compared to the wind patterns in Earth's atmosphere. Do you think wind patterns flow the same around other planets? Why or why not?
  • Resources

      Gipe, P. (1995) Wind energy comes of age. New York: John Wiley & Sons, Inc.
      Greeley, R. (1994, Jan 21) Wind streaks on Venus: Clues to atmospheric circulation. Science, p. 358.
      Onish, L (1995) Wind and weather. New York: Scholastic Voyages of Discovery.
      Rennicke, J. (1995, Nov) Why the wind blows. Reader's Digest, p. 82.
      Schaefer, V. & Day, J. (1981) A field guide to the atmosphere (a Peterson field guide). Boston: Houghton Mifflin.

      Organizations
      National Oceanic and Atmospheric Administration
      NOAA Environmental and
      Information Services
      1315 East West Highway, Room 15400
      Silver Spring, MD 20910
      (301) 713-0575

      Web sites
      National Weather Service
      www.nws.noaa.gov
      The Wind: Our Fierce Friend
      sln.fi.edu.tfi/units/energy/wind.html