Sunspots provide astronomers with insights into the motions of the sun. The Italian scientist Galileo Galilei discovered that the sun rotates by observing the motion of sunspots. Later observations showed that the sun doesn't spin as a solid body the way Earth does. Instead, sunspots near the sun's equator move faster than sunspots near the sun's poles. This means that the sun rotates faster at its equator than near its poles.

Prominences

Prominences are spectacular features of the sun's atmosphere that occur near sunspots. As shown in Figure 7A, prominences are huge loops of gas that erupt from sunspot regions. They extend upward from the photosphere into the chromosphere and sometimes into the corona. Prominences travel along the magnetic field lines that connect sunspots. Some prominences reach heights of more than 100,000 kilometers above the sun's surface.

Figure 7 The sun's magnetic field produces prominences and flares visible with special red filters. A This prominence forms a huge twirling loop connecting sunspot regions. B A solar flare erupts on the edge of the sun.

A set of images to show formation of prominences and flares due to the Sun's magnetic fields. d
Solar Flares

The sun's surface sometimes erupts dramatically, producing X-rays and hurling charged particles into space at speeds of 1000 km/s or more. Such a sudden release of energy from the sun is called a solar flare. Like prominences, solar flares usually occur near sunspots. Solar flares heat the corona to a temperature near 20 million K and greatly increase the solar wind. When the additional high-energy particles and radiation from a solar flare reach Earth, they can cause magnetic storms in Earth's upper atmosphere. These storms disrupt electric power transmission as well as radio, television, and telephone signals.


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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