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Explore the physical properties that contribute to the formation of wind through hands-on activities. Learn about the coriolis effect, the sun's rays, and the role of warm and cool air in wind formation. This document also includes extension ideas and related activities for further exploration.
What you will learn
Typology: Schemes and Mind Maps
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Objectives and Standards
Part 1.
Discussion These activities illustrate some of the forces acting on wind; the Coriolis effect and the Sun’s rays. What did you notice about the two activities showing the deflection caused by rotating the Earth? Is there a force that is working on the air that allows some movement? Do you notice this force in your every day life (like spinning in a circle with a bucket full of water, riding on a merry-go-round)? Warm air weighs less, so it floats on top of cool air. When the trash bag moved, it was just acting as a place holder for the air so we could see the air actually move. The warmer the air is relative to the surrounding cool air, the faster and higher it will travel. When the Sun heats the air, it warms and moves upward, and cool air moves down to take its place. We discussed in the introduction that the equator gets more energy from the Sun, so air flows up near the equator. It gets deflected by the rotating Earth, and as it moves upward and away from the equator, it gets cooler. This deflection is the same as the one seen when we poured water on the rotating ball. This creates a big circular path called a convection cell, or Hadley cell when talking about weather.