24.3 Solar Energy and Winds

The heat you feel when you're out in the sun is one effect of solar energy. You might think that sunlight heats the air directly, just as it heats you directly. But the process is more complicated than that.

Energy in the Atmosphere

Some solar energy that reaches Earth's atmosphere is reflected back, some is absorbed by the atmosphere, and some is absorbed by Earth's surface. About 30 percent of the incoming solar energy is reflected back into space by clouds, dust in the air, gases, and Earth's surface. About 20 percent of the sun's energy is absorbed by clouds and gases. But the greatest amount of solar energy—about half—passes through the atmosphere and is absorbed by the surface.

The atmosphere is heated primarily by energy that is reradiated by Earth's surface. Unlike incoming solar energy, which has much of its energy in the visible spectrum, the energy radiated back into the atmosphere is mostly infrared radiation. Certain gases in the atmosphere, including water vapor and carbon dioxide, allow visible light to pass through but absorb most infrared radiation. These gases radiate some of this absorbed energy back to Earth's surface, warming the lower atmosphere in a process called the greenhouse effect. Without the greenhouse effect, Earth's surface would be much cooler than it is.

Energy is transferred within the troposphere in three ways: radiation, convection, and conduction. As the How It Works box on page 756 explains, these processes work together to heat the troposphere.

Figure 11 About half of the sunlight that reaches Earth is absorbed by the surface. The rest is either reflected back into space or absorbed in the atmosphere.

A diagram of the surface of the Earth shows how most energy absorbed by the
surface is reradiated back into the
atmosphere. 
 

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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