If Earth were not rotating on its axis, global winds would move in roughly straight paths from the poles to the equator. However, because Earth rotates, global winds move in a curved path between the poles and the equator. Notice in Figure 13 that global winds curve to the right in the Northern Hemisphere and to the left in the Southern Hemisphere. The curving effect that Earth's rotation has on all freemoving objects, including global winds, is called the Coriolis effect. If Earth were not rotating, a rocket launched from the North Pole toward the equator would move in a straight line, as shown in Figure 15. However, because Earth is rotating underneath the rocket, the rocket would appear to an observer on Earth to curve to the right. Similary, Earth's rotation causes global winds to curve.

Monsoons

Seasonal changes in the heating of Earth's surface affect the circulation of the atmosphere. A monsoon is a wind system that is characterized by seasonal reversal of direction. Monsoons are similar to land and sea breezes except that they occur on a much wider scale and longer time frame. For example, the summer monsoon that occurs over much of South and Southeast Asia blows warm, humid air from the ocean onto land. As this air rises over land, it cools and brings heavy rainfall to parts of that region. In winter the monsoon reverses, blowing from land onto water and bringing drier weather.

Jet Stream

Global wind patterns are also affected by fast-moving streams of air at high altitudes. A belt of high-speed wind in the upper troposphere is called a jet stream. Jet streams are caused by great differences in air pressure that develop at high altitudes.

Figure 15 The Coriolis effect causes free-moving objects, such as rockets and global winds, to move in a curved path. A A rocket launched from the North Pole toward the equator would move in a straight line if Earth were not rotating. B The Coriolis effect causes such a rocket to appear to curve to the right. Similarly, the Coriolis effect causes global winds to curve to the right in the Northern Hemisphere.

A diagram of the Coriolis effect.dd

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Table of Contents

Physical Science CHAPTER 1 Science Skills CHAPTER 2 Properties of Matter CHAPTER 3 States of Matter CHAPTER 4 Atomic Structure CHAPTER 5 The Periodic Table CHAPTER 6 Chemical Bonds CHAPTER 7 Chemical Reactions CHAPTER 8 Solutions, Acids, and Bases CHAPTER 9 Carbon Chemistry CHAPTER 10 Nuclear Chemistry CHAPTER 11 Motion CHAPTER 12 Forces and Motion CHAPTER 13 Forces in Fluids CHAPTER 14 Work, Power, and Machines CHAPTER 15 Energy CHAPTER 16 Thermal Energy and Heat CHAPTER 17 Mechanical Waves and Sound CHAPTER 18 The Electromagnetic Spectrum and Light CHAPTER 19 Optics CHAPTER 20 Electricity CHAPTER 21 Magnetism CHAPTER 22 Earth's Interior CHAPTER 23 Earth's Surface CHAPTER 24 Weather and Climate CHAPTER 25 The Solar System CHAPTER 26 Exploring the Universe Skills and Reference Handbook