\n \n

\n $\"\"$ <\/p>\n

\n Papers held up by rising air currents above a radiator demonstrate the important principle that warm air rises.\n <\/p>\n <\/div>\n

\n Why does warm air rise (Figure<\/strong> above<\/a>)? Gas molecules are able to move freely and if they are uncontained, as they are in the atmosphere, they can take up more or less space.\n <\/p>\n

\n
When gas molecules are cool, they are sluggish and do not take up as much space. With the same number of molecules in less space, both air density and air pressure are higher.\n <\/li>\n
When gas molecules are warm, they move vigorously and take up more space. Air density and air pressure are lower.\n <\/li>\n <\/ul>\n
\n Warmer, lighter air is more buoyant than the cooler air above it, so it rises. The cooler air then sinks down, because it is denser than the air beneath it. This is convection, which was described in the Plate Tectonics chapter.\n <\/p>\n
\n The property that changes most strikingly with altitude is air temperature. Unlike the change in pressure and density, which decrease with altitude, changes in air temperature are not regular. A change in temperature with distance is called a temperature gradient<\/strong>.\n <\/p>\n
\n The atmosphere is divided into layers based on how the temperature in that layer changes with altitude, the layer\u2019s temperature gradient (Figure<\/strong> below<\/a>). The temperature gradient of each layer is different. In some layers, temperature increases with altitude and in others it decreases. The temperature gradient in each layer is determined by the heat source of the layer (Figure<\/strong> below<\/a>).\n <\/p>\n
\n \n
\n $\"\"$ <\/p>\n
\n The four main layers of the atmosphere have different temperature gradients, creating the thermal structure of the atmosphere.\n <\/p>\n <\/div>\n
\n \n
\n $\"\"$ <\/p>\n
\n The layers of the atmosphere appear as different colors in this image from the International Space Station.\n <\/p>\n <\/div>\n
\n Most of the important processes of the atmosphere take place in the lowest two layers: the troposphere and the stratosphere.\n <\/p>\n
\n Troposphere\n <\/h2>\n
\n The temperature of the troposphere<\/strong> is highest near the surface of the Earth and decreases with altitude. On average, the temperature gradient of the troposphere is 6.5\u00b0C per 1,000 m (3.6\u00b0F per 1,000 ft.) of altitude. What is the source of heat for the troposphere?\n <\/p>\n
\n Earth\u2019s surface is a major source of heat for the troposphere, although nearly all of that heat comes from the Sun. Rock, soil, and water on Earth absorb the Sun\u2019s light and radiate it back into the atmosphere as heat. The temperature is also higher near the surface because of the greater density of gases. The higher gravity causes the temperature to rise.\n <\/p>\n
\n Notice that in the troposphere warmer air is beneath cooler air. What do you think the consequence of this is? This condition is unstable. The warm air near the surface rises and cool air higher in the troposphere sinks. So air in the troposphere does a lot of mixing. This mixing causes the temperature gradient to vary with time and place. The rising and sinking of air in the troposphere means that all of the planet\u2019s weather takes place in the troposphere.\n <\/p>\n
\n Sometimes there is a temperature inversion<\/strong>, air temperature in the troposphere increases with altitude and warm air sits over cold air. Inversions are very stable and may last for several days or even weeks. Inversions form:\n <\/p>\n
\n
Over land at night or in winter when the ground is cold. The cold ground cools the air that sits above it, making this low layer of air denser than the air above it.\n <\/li>\n
Near the coast where cold seawater cools the air above it. When that denser air moves inland, it slides beneath the warmer air over the land.\n <\/li>\n <\/ul>\n
\n Since temperature inversions are stable, they often trap pollutants and produce unhealthy air conditions in cities (Figure<\/strong> below<\/a>).\n <\/p>\n
\n \n
\n $\"\"$ <\/p>\n
\n Smoke makes a temperature inversion visible. The smoke is trapped in cold dense air that lies beneath a cap of warmer air.\n <\/p>\n <\/div>\n
\n At the top of the troposphere is a thin layer in which the temperature does not change with height. This means that the cooler, denser air of the troposphere is trapped beneath the warmer, less dense air of the stratosphere. Air from the troposphere and stratosphere rarely mix.\n <\/p>\n
\n A science experiment that clearly shows how a temperature inversion traps air, along with whatever pollutants are in it, near the ground is seen in this video (5c)<\/strong>: http:\/\/www.youtube.com\/watch?v=LPvn9qhVFbM<\/a> (2:50).\n <\/p>\n
\n \n
https:\/\/www.youtube.com\/embed\/LPvn9qhVFbM<\/p>\n <\/div>\n
\n Stratosphere\n <\/h2>\n
\n Ash and gas from a large volcanic eruption may burst into the stratosphere<\/strong>, the layer above the troposphere. Once in the stratosphere, it remains suspended there for many years because there is so little mixing between the two layers. Pilots like to fly in the lower portions of the stratosphere because there is little air turbulence.\n <\/p>\n
\n In the stratosphere, temperature increases with altitude. What is the heat source for the stratosphere? The direct heat source for the stratosphere is the Sun. Air in the stratosphere is stable because warmer, less dense air sits over cooler, denser air. As a result, there is little mixing of air within the layer.\n <\/p>\n
\n The ozone layer<\/strong> is found within the stratosphere between 15 to 30 km (9 to 19 miles) altitude. The thickness of the ozone layer varies by the season and also by latitude.\n <\/p>\n
\n The ozone layer is extremely important because ozone gas in the stratosphere absorbs most of the Sun\u2019s harmful ultraviolet (UV) radiation. Because of this, the ozone layer protects life on Earth. High-energy UV light penetrates cells and damages DNA, leading to cell death (which we know as a bad sunburn). Organisms on Earth are not adapted to heavy UV exposure, which kills or damages them. Without the ozone layer to reflect UVC and UVB radiation, most complex life on Earth would not survive long (Figure<\/strong> below<\/a>).\n <\/p>\n
\n \n
\n $\"\"$ <\/p>\n
\n Even with the ozone layer, UVB radiation still manages to reach Earth's surface, especially where solar radiation is high.\n <\/p>\n <\/div>\n
\n Mesosphere\n <\/h2>\n
\n Temperatures in the mesosphere<\/strong> decrease with altitude. Because there are few gas molecules in the mesosphere to absorb the Sun\u2019s radiation, the heat source is the stratosphere below. The mesosphere is extremely cold, especially at its top, about -90\u00b0C (-130\u00b0F).\n <\/p>\n
\n The air in the mesosphere has extremely low density: 99.9% of the mass of the atmosphere is below the mesosphere. As a result, air pressure is very low (Figure<\/strong> below<\/a>). A person traveling through the mesosphere would experience severe burns from ultraviolet light since the ozone layer which provides UV protection is in the stratosphere below. There would be almost no oxygen for breathing. Stranger yet, an unprotected traveler\u2019s blood would boil at normal body temperature because the pressure is so low.\n <\/p>\n
\n \n
\n $\"\"$ <\/p>\n
\n Meteors burn in the mesosphere even though the gas is very thin; these burning meteors are shooting stars.\n <\/p>\n <\/div>\n
\n Thermosphere and Beyond\n <\/h2>\n
\n \n
\n $\"\"$ <\/p>\n
\n The International Space Station (ISS) orbits within the upper part of the thermosphere, at about 320 to 380 km above the Earth.\n <\/p>\n <\/div>\n
\n The density of molecules is so low in the thermosphere<\/strong> that one gas molecule can go about 1 km before it collides with another molecule. Since so little energy is transferred, the air feels very cold (Figure<\/strong> above<\/a>).\n <\/p>\n
\n Within the thermosphere is the ionosphere<\/strong>. The ionosphere gets its name from the solar radiation that ionizes gas molecules to create a positively charged ion and one or more negatively charged electrons. The freed electrons travel within the ionosphere as electric currents. Because of the free ions, the ionosphere has many interesting characteristics.\n <\/p>\n
\n At night, radio waves bounce off the ionosphere and back to Earth. This is why you can often pick up an AM radio station far from its source at night.\n <\/p>\n
\n The Van Allen radiation belts are two doughnut-shaped zones of highly charged particles that are located beyond the atmosphere in the magnetosphere<\/strong>. The particles originate in solar flares and fly to Earth on the solar wind. Once trapped by Earth\u2019s magnetic field, they follow along the field\u2019s magnetic lines of force. These lines extend from above the equator to the North Pole and also to the South Pole then return to the equator.\n <\/p>\n
\n When massive solar storms cause the Van Allen belts to become overloaded with particles, the result is the most spectacular feature of the ionosphere -- the nighttime aurora<\/strong> (Figure<\/strong> below<\/a>). The particles spiral along magnetic field lines toward the poles. The charged particles energize oxygen and nitrogen gas molecules, causing them to light up. Each gas emits a particular color of light.\n <\/p>\n
\n \n
\n $\"\"$ <\/p>\n
\n (a) Spectacular light displays are visible as the aurora borealis or northern lights in the Northern Hemisphere. (b) The aurora australis or southern lights encircles Antarctica.\n <\/p>\n <\/div>\n
\n There is no real outer limit to the exosphere<\/strong>, the outermost layer of the atmosphere; the gas molecules finally become so scarce that at some point there are no more. Beyond the atmosphere is the solar wind. The solar wind<\/strong> is made of high-speed particles, mostly protons and electrons, traveling rapidly outward from the Sun.\n <\/p>\n
\n This video is very thorough in its discussion of the layers of the atmosphere. Remember that the chemical composition of each layer is nearly the same except for the ozone layer that is found in the stratosphere (8a)<\/strong>: http:\/\/www.youtube.com\/watch?v=S-YAKZoy1A0<\/a> (6:44).\n <\/p>\n
\n \n\nhttps:\/\/www.youtube.com\/watch?v=S-YAKZoy1A0\n\n <\/div>\n
\n KQED: Illuminating the Northern Lights\n <\/h3>\n
\n What would Earth's magnetic field look like if it were painted in colors? It would look like the aurora! This QUEST video looks at the aurora, which provides clues about the solar wind, Earth's magnetic field and Earth's atmosphere. Learn more at: http:\/\/science.kqed.org\/quest\/video\/illuminating-the-northern-lights\/<\/a>.\n <\/p>\n
\n \n
https:\/\/www.youtube.com\/embed\/o6soo_lFbGI<\/p>\n <\/div>\n
\n Lesson Summary\n <\/h2>\n
\n
Features of the atmosphere change with altitude: density decreases, air pressure decreases, temperature changes vary.\n <\/li>\n
Different temperature gradients create different layers within the atmosphere.\n <\/li>\n
The lowest layer is the troposphere where most of the atmospheric gases and all of the planet\u2019s weather are located. The troposphere is heated from the ground, so temperature decreases with altitude. Because warm air rises and cool air sinks, the troposphere is unstable.\n <\/li>\n
In the stratosphere, temperature increases with altitude. The stratosphere contains the ozone layer, which protects the planet from the Sun\u2019s harmful UV radiation.\n <\/li>\n <\/ul>\n
\n Review Questions\n <\/h2>\n
\n 1. Give a detailed explanation of why warm air rises.\n <\/p>\n
\n 2. Why doesn\u2019t air temperature change uniformly with altitude? Give examples.\n <\/p>\n
\n 3. Describe how the ground acts as the heat source for the troposphere. What is the source of energy and what happens to that energy?\n <\/p>\n
\n 4. How stable is an inversion and why? How does an inversion form?\n <\/p>\n
\n 5. Phoenix, Arizona, is a city in the Southwestern desert. Summers are extremely hot. Winter days are often fairly warm but winter nights can be quite chilly. In December, inversions are quite common. How does an inversion form under these conditions and what are the consequences of an inversion to this sprawling, car-dependent city?\n <\/p>\n
\n 6. Why can\u2019t air from the troposphere and the stratosphere mix freely?\n <\/p>\n
\n 7. What is the heat source for the stratosphere? How is that heat absorbed?\n <\/p>\n
\n 8. Describe ozone creation and loss in the ozone layer. Does one occur more than the other?\n <\/p>\n
\n 9. How and where are \"shooting stars\" created?\n <\/p>\n
\n 10. Why would an unprotected traveler\u2019s blood boil in the mesosphere?\n <\/p>\n
\n Further Reading \/ Supplemental Links\n <\/h2>\n
\n NASA, The Mystery of the Aurora: http:\/\/www.youtube.com\/watch?v=PaSFAbATPvk<\/a>.\n <\/p>\n
\n Points to Consider\n <\/h2>\n
\n
How does solar energy create the atmosphere\u2019s layers?\n <\/li>\n
How does solar energy create the weather?\n <\/li>\n
What would happen to life on Earth if there was less ozone in the ozone layer?\n <\/li>\n <\/ul>\n<\/body>","rendered":"
\n Lesson Objectives
\n <\/h2>\n
\n
List the major layers of the atmosphere and their temperatures.\n <\/li>\n
Discuss why all weather takes place in the troposphere.\n <\/li>\n
Discuss how the ozone layer protects the surface from harmful radiation.\n <\/li>\n<\/ul>\n
\n Vocabulary
\n <\/h2>\n
\n
aurora\n <\/li>\n
exosphere\n <\/li>\n
inversion\n <\/li>\n
ionosphere\n <\/li>\n
magnetosphere\n <\/li>\n
mesosphere\n <\/li>\n
ozone layer\n <\/li>\n
solar wind\n <\/li>\n
stratosphere\n <\/li>\n
temperature gradient\n <\/li>\n
thermosphere\n <\/li>\n
troposphere\n <\/li>\n<\/ul>\n
\n Introduction
\n <\/h2>\n
\n The atmosphere is layered, corresponding with how the atmosphere\u2019s temperature changes with altitude. By understanding the way temperature changes with altitude, we can learn a lot about how the atmosphere works. While weather takes place in the lower atmosphere, interesting things, such as the beautiful aurora, happen higher in the atmosphere.\n <\/p>\n
\n Air Temperature
\n <\/h2>\n
\n <\/p>\n
\n $\"\"$ <\/p>\n
\n Papers held up by rising air currents above a radiator demonstrate the important principle that warm air rises.\n <\/p>\n<\/p><\/div>\n
\n Why does warm air rise (Figure<\/strong> above<\/a>)? Gas molecules are able to move freely and if they are uncontained, as they are in the atmosphere, they can take up more or less space.\n <\/p>\n
\n
When gas molecules are cool, they are sluggish and do not take up as much space. With the same number of molecules in less space, both air density and air pressure are higher.\n <\/li>\n
When gas molecules are warm, they move vigorously and take up more space. Air density and air pressure are lower.\n <\/li>\n<\/ul>\n
\n Warmer, lighter air is more buoyant than the cooler air above it, so it rises. The cooler air then sinks down, because it is denser than the air beneath it. This is convection, which was described in the Plate Tectonics chapter.\n <\/p>\n
\n The property that changes most strikingly with altitude is air temperature. Unlike the change in pressure and density, which decrease with altitude, changes in air temperature are not regular. A change in temperature with distance is called a temperature gradient<\/strong>.\n <\/p>\n
\n The atmosphere is divided into layers based on how the temperature in that layer changes with altitude, the layer\u2019s temperature gradient (Figure<\/strong> below<\/a>). The temperature gradient of each layer is different. In some layers, temperature increases with altitude and in others it decreases. The temperature gradient in each layer is determined by the heat source of the layer (Figure<\/strong> below<\/a>).\n <\/p>\n
\n <\/p>\n
\n $\"\"$ <\/p>\n
\n The four main layers of the atmosphere have different temperature gradients, creating the thermal structure of the atmosphere.\n <\/p>\n<\/p><\/div>\n
\n <\/p>\n
\n $\"\"$ <\/p>\n
\n The layers of the atmosphere appear as different colors in this image from the International Space Station.\n <\/p>\n<\/p><\/div>\n
\n Most of the important processes of the atmosphere take place in the lowest two layers: the troposphere and the stratosphere.\n <\/p>\n
\n Troposphere
\n <\/h2>\n
\n The temperature of the troposphere<\/strong> is highest near the surface of the Earth and decreases with altitude. On average, the temperature gradient of the troposphere is 6.5\u00b0C per 1,000 m (3.6\u00b0F per 1,000 ft.) of altitude. What is the source of heat for the troposphere?\n <\/p>\n
\n Earth\u2019s surface is a major source of heat for the troposphere, although nearly all of that heat comes from the Sun. Rock, soil, and water on Earth absorb the Sun\u2019s light and radiate it back into the atmosphere as heat. The temperature is also higher near the surface because of the greater density of gases. The higher gravity causes the temperature to rise.\n <\/p>\n
\n Notice that in the troposphere warmer air is beneath cooler air. What do you think the consequence of this is? This condition is unstable. The warm air near the surface rises and cool air higher in the troposphere sinks. So air in the troposphere does a lot of mixing. This mixing causes the temperature gradient to vary with time and place. The rising and sinking of air in the troposphere means that all of the planet\u2019s weather takes place in the troposphere.\n <\/p>\n
\n Sometimes there is a temperature inversion<\/strong>, air temperature in the troposphere increases with altitude and warm air sits over cold air. Inversions are very stable and may last for several days or even weeks. Inversions form:\n <\/p>\n
\n
Over land at night or in winter when the ground is cold. The cold ground cools the air that sits above it, making this low layer of air denser than the air above it.\n <\/li>\n
Near the coast where cold seawater cools the air above it. When that denser air moves inland, it slides beneath the warmer air over the land.\n <\/li>\n<\/ul>\n
\n Since temperature inversions are stable, they often trap pollutants and produce unhealthy air conditions in cities (Figure<\/strong> below<\/a>).\n <\/p>\n
\n <\/p>\n
\n $\"\"$ <\/p>\n
\n Smoke makes a temperature inversion visible. The smoke is trapped in cold dense air that lies beneath a cap of warmer air.\n <\/p>\n<\/p><\/div>\n
\n At the top of the troposphere is a thin layer in which the temperature does not change with height. This means that the cooler, denser air of the troposphere is trapped beneath the warmer, less dense air of the stratosphere. Air from the troposphere and stratosphere rarely mix.\n <\/p>\n
\n A science experiment that clearly shows how a temperature inversion traps air, along with whatever pollutants are in it, near the ground is seen in this video (5c)<\/strong>: http:\/\/www.youtube.com\/watch?v=LPvn9qhVFbM<\/a> (2:50).\n <\/p>\n
\n
<\/iframe><\/p>\n<\/p><\/div>\n<h2>\n Stratosphere<br \/>\n <\/h2>\n<p>\n Ash and gas from a large volcanic eruption may burst into the <strong>stratosphere<\/strong>, the layer above the troposphere. Once in the stratosphere, it remains suspended there for many years because there is so little mixing between the two layers. Pilots like to fly in the lower portions of the stratosphere because there is little air turbulence.\n <\/p>\n<p>\n In the stratosphere, temperature increases with altitude. What is the heat source for the stratosphere? The direct heat source for the stratosphere is the Sun. Air in the stratosphere is stable because warmer, less dense air sits over cooler, denser air. As a result, there is little mixing of air within the layer.\n <\/p>\n<p>\n The <strong>ozone layer<\/strong> is found within the stratosphere between 15 to 30 km (9 to 19 miles) altitude. The thickness of the ozone layer varies by the season and also by latitude.\n <\/p>\n<p>\n The ozone layer is extremely important because ozone gas in the stratosphere absorbs most of the Sun\u2019s harmful ultraviolet (UV) radiation. Because of this, the ozone layer protects life on Earth. High-energy UV light penetrates cells and damages DNA, leading to cell death (which we know as a bad sunburn). Organisms on Earth are not adapted to heavy UV exposure, which kills or damages them. Without the ozone layer to reflect UVC and UVB radiation, most complex life on Earth would not survive long (<strong>Figure<\/strong> <a href=\"#x-ck12-SFMtRVMtMTUtMTAtVWx0cmF2aW9sZXQtcmFkaWF0aW9uLmpwZw..\">below<\/a>).\n <\/p>\n<div class=\"x-ck12-img-postcard x-ck12-nofloat\">\n <\/p>\n<p>\n <img decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images-archive-read-only\/wp-content\/uploads\/sites\/682\/2015\/07\/22230121\/201412291419878707692244_f94825c988701f898089b2bfc007ffd5-201412291419879343542192.jpg\" title=\"\" longdesc=\"Even%20with%20the%20ozone%20layer%2C%20UVB%20radiation%20still%20manages%20to%20reach%20Earth%27s%20surface%2C%20especially%20where%20solar%20radiation%20is%20high.%20\" alt=\"\" id=\"x-ck12-SFMtRVMtMTUtMTAtVWx0cmF2aW9sZXQtcmFkaWF0aW9uLmpwZw..\" \/><\/p>\n<p>\n Even with the ozone layer, UVB radiation still manages to reach Earth’s surface, especially where solar radiation is high.\n <\/p>\n<\/p><\/div>\n<h2>\n Mesosphere<br \/>\n <\/h2>\n<p>\n Temperatures in the <strong>mesosphere<\/strong> decrease with altitude. Because there are few gas molecules in the mesosphere to absorb the Sun\u2019s radiation, the heat source is the stratosphere below. The mesosphere is extremely cold, especially at its top, about -90\u00b0C (-130\u00b0F).\n <\/p>\n<p>\n The air in the mesosphere has extremely low density: 99.9% of the mass of the atmosphere is below the mesosphere. As a result, air pressure is very low (<strong>Figure<\/strong> <a href=\"#x-ck12-RWFyU2NpLTE1MDItMDMuanBn\">below<\/a>). A person traveling through the mesosphere would experience severe burns from ultraviolet light since the ozone layer which provides UV protection is in the stratosphere below. There would be almost no oxygen for breathing. Stranger yet, an unprotected traveler\u2019s blood would boil at normal body temperature because the pressure is so low.\n <\/p>\n<div class=\"x-ck12-img-postcard x-ck12-nofloat\">\n <\/p>\n<p>\n <img decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images-archive-read-only\/wp-content\/uploads\/sites\/682\/2015\/07\/22230122\/201412291419878707715565_450bbe80e2d62241d17d82045d4749b1-201412291419879343952127.jpg\" title=\"\" longdesc=\"Meteors%20burn%20in%20the%20mesosphere%20even%20though%20the%20gas%20is%20very%20thin%3B%20these%20burning%20meteors%20are%20shooting%20stars.%20\" alt=\"\" id=\"x-ck12-RWFyU2NpLTE1MDItMDMuanBn\" \/><\/p>\n<p>\n Meteors burn in the mesosphere even though the gas is very thin; these burning meteors are shooting stars.\n <\/p>\n<\/p><\/div>\n<h2>\n Thermosphere and Beyond<br \/>\n <\/h2>\n<div class=\"x-ck12-img-postcard x-ck12-nofloat\">\n <\/p>\n<p>\n <img decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images-archive-read-only\/wp-content\/uploads\/sites\/682\/2015\/07\/22230124\/201412291419878708030819_fec9fe3465f1cac69cf86dc249fd1e1a-201412291419879344384890.jpg\" title=\"\" longdesc=\"The%20International%20Space%20Station%20%28ISS%29%20orbits%20within%20the%20upper%20part%20of%20the%20thermosphere%2C%20at%20about%20320%20to%20380%20km%20above%20the%20Earth.%20\" alt=\"\" id=\"x-ck12-RWFyU2NpLTE1MDItMDQuanBn\" \/><\/p>\n<p>\n The International Space Station (ISS) orbits within the upper part of the thermosphere, at about 320 to 380 km above the Earth.\n <\/p>\n<\/p><\/div>\n<p>\n The density of molecules is so low in the <strong>thermosphere<\/strong> that one gas molecule can go about 1 km before it collides with another molecule. Since so little energy is transferred, the air feels very cold (<strong>Figure<\/strong> <a href=\"#x-ck12-RWFyU2NpLTE1MDItMDQuanBn\">above<\/a>).\n <\/p>\n<p>\n Within the thermosphere is the <strong>ionosphere<\/strong>. The ionosphere gets its name from the solar radiation that ionizes gas molecules to create a positively charged ion and one or more negatively charged electrons. The freed electrons travel within the ionosphere as electric currents. Because of the free ions, the ionosphere has many interesting characteristics.\n <\/p>\n<p>\n At night, radio waves bounce off the ionosphere and back to Earth. This is why you can often pick up an AM radio station far from its source at night.\n <\/p>\n<p>\n The Van Allen radiation belts are two doughnut-shaped zones of highly charged particles that are located beyond the atmosphere in the <strong>magnetosphere<\/strong>. The particles originate in solar flares and fly to Earth on the solar wind. Once trapped by Earth\u2019s magnetic field, they follow along the field\u2019s magnetic lines of force. These lines extend from above the equator to the North Pole and also to the South Pole then return to the equator.\n <\/p>\n<p>\n When massive solar storms cause the Van Allen belts to become overloaded with particles, the result is the most spectacular feature of the ionosphere — the nighttime <strong>aurora<\/strong> (<strong>Figure<\/strong> <a href=\"#x-ck12-SFMtRVMtMTUtMTMtQXVyb3Jhcw..\">below<\/a>). The particles spiral along magnetic field lines toward the poles. The charged particles energize oxygen and nitrogen gas molecules, causing them to light up. Each gas emits a particular color of light.\n <\/p>\n<div class=\"x-ck12-img-fullpage x-ck12-nofloat\">\n <\/p>\n<p>\n <img decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images-archive-read-only\/wp-content\/uploads\/sites\/682\/2015\/07\/22230125\/201412291419878708061963_dcf66efd73b26e632451c664a07ea070-201412291419879344826543.jpg\" title=\"\" longdesc=\"%28a%29%20Spectacular%20light%20displays%20are%20visible%20as%20the%20aurora%20borealis%20or%20northern%20lights%20in%20the%20Northern%20Hemisphere.%20%28b%29%20The%20aurora%20australis%20or%20southern%20lights%20encircles%20Antarctica.%20\" alt=\"\" id=\"x-ck12-SFMtRVMtMTUtMTMtQXVyb3Jhcw..\" \/><\/p>\n<p>\n (a) Spectacular light displays are visible as the aurora borealis or northern lights in the Northern Hemisphere. (b) The aurora australis or southern lights encircles Antarctica.\n <\/p>\n<\/p><\/div>\n<p>\n There is no real outer limit to the <strong>exosphere<\/strong>, the outermost layer of the atmosphere; the gas molecules finally become so scarce that at some point there are no more. Beyond the atmosphere is the solar wind. The <strong>solar wind<\/strong> is made of high-speed particles, mostly protons and electrons, traveling rapidly outward from the Sun.\n <\/p>\n<p>\n This video is very thorough in its discussion of the layers of the atmosphere. Remember that the chemical composition of each layer is nearly the same except for the ozone layer that is found in the stratosphere <strong>(8a)<\/strong>: <a href=\"http:\/\/www.youtube.com\/watch?v=S-YAKZoy1A0\">http:\/\/www.youtube.com\/watch?v=S-YAKZoy1A0<\/a> (6:44).\n <\/p>\n<div itemprop=\"video\" itemscope=\"itemscope\" itemtype=\"http:\/\/schema.org\/VideoObject\">\n<p><iframe loading=\"lazy\" id=\"oembed-1\" title=\"Layers of the Atmosphere-Hommocks Earth Science Department\" width=\"500\" height=\"281\" src=\"https:\/\/www.youtube.com\/embed\/S-YAKZoy1A0?feature=oembed&rel=0\" frameborder=\"0\" allowfullscreen=\"allowfullscreen\"><\/iframe><\/p><\/div>\n<h3>\n KQED: Illuminating the Northern Lights<br \/>\n <\/h3>\n<p>\n What would Earth’s magnetic field look like if it were painted in colors? It would look like the aurora! This QUEST video looks at the aurora, which provides clues about the solar wind, Earth’s magnetic field and Earth’s atmosphere. Learn more at: <a href=\"http:\/\/science.kqed.org\/quest\/video\/illuminating-the-northern-lights\/\">http:\/\/science.kqed.org\/quest\/video\/illuminating-the-northern-lights\/<\/a>.\n <\/p>\n<div itemprop=\"video\" itemscope=\"itemscope\" itemtype=\"http:\/\/schema.org\/VideoObject\">\n<p>https:\/\/youtube.com\/watch?v=o6soo_lFbGI<\/p>\n<\/p><\/div>\n<h2>\n Lesson Summary<br \/>\n <\/h2>\n<ul>\n<li>Features of the atmosphere change with altitude: density decreases, air pressure decreases, temperature changes vary.\n <\/li>\n<li>Different temperature gradients create different layers within the atmosphere.\n <\/li>\n<li>The lowest layer is the troposphere where most of the atmospheric gases and all of the planet\u2019s weather are located. The troposphere is heated from the ground, so temperature decreases with altitude. Because warm air rises and cool air sinks, the troposphere is unstable.\n <\/li>\n<li>In the stratosphere, temperature increases with altitude. The stratosphere contains the ozone layer, which protects the planet from the Sun\u2019s harmful UV radiation.\n <\/li>\n<\/ul>\n<h2>\n Review Questions<br \/>\n <\/h2>\n<p>\n 1. Give a detailed explanation of why warm air rises.\n <\/p>\n<p>\n 2. Why doesn\u2019t air temperature change uniformly with altitude? Give examples.\n <\/p>\n<p>\n 3. Describe how the ground acts as the heat source for the troposphere. What is the source of energy and what happens to that energy?\n <\/p>\n<p>\n 4. How stable is an inversion and why? How does an inversion form?\n <\/p>\n<p>\n 5. Phoenix, Arizona, is a city in the Southwestern desert. Summers are extremely hot. Winter days are often fairly warm but winter nights can be quite chilly. In December, inversions are quite common. How does an inversion form under these conditions and what are the consequences of an inversion to this sprawling, car-dependent city?\n <\/p>\n<p>\n 6. Why can\u2019t air from the troposphere and the stratosphere mix freely?\n <\/p>\n<p>\n 7. What is the heat source for the stratosphere? How is that heat absorbed?\n <\/p>\n<p>\n 8. Describe ozone creation and loss in the ozone layer. Does one occur more than the other?\n <\/p>\n<p>\n 9. How and where are “shooting stars” created?\n <\/p>\n<p>\n 10. Why would an unprotected traveler\u2019s blood boil in the mesosphere?\n <\/p>\n<h2>\n Further Reading \/ Supplemental Links<br \/>\n <\/h2>\n<p>\n NASA, The Mystery of the Aurora: <a href=\"http:\/\/www.youtube.com\/watch?v=PaSFAbATPvk\">http:\/\/www.youtube.com\/watch?v=PaSFAbATPvk<\/a>.\n <\/p>\n<h2>\n Points to Consider<br \/>\n <\/h2>\n<ul>\n<li>How does solar energy create the atmosphere\u2019s layers?\n <\/li>\n<li>How does solar energy create the weather?\n <\/li>\n<li>What would happen to life on Earth if there was less ozone in the ozone layer?\n <\/li>\n<\/ul>\n\n\t\t\t <section class=\"citations-section\" role=\"contentinfo\">\n\t\t\t <h3>Candela Citations<\/h3>\n\t\t\t\t\t <div>\n\t\t\t\t\t\t <div id=\"citation-list-633\">\n\t\t\t\t\t\t\t <div class=\"licensing\"><div class=\"license-attribution-dropdown-subheading\">CC licensed content, Shared previously<\/div><ul class=\"citation-list\"><li>Earth Science for High School. <strong>Provided by<\/strong>: CK-12. <strong>Located at<\/strong>: <a target=\"_blank\" href=\"http:\/\/www.ck12.org\/book\/CK-12-Earth-Science-For-High-School\/\">http:\/\/www.ck12.org\/book\/CK-12-Earth-Science-For-High-School\/<\/a>. <strong>License<\/strong>: <em><a target=\"_blank\" rel=\"license\" href=\"https:\/\/creativecommons.org\/licenses\/by-nc\/4.0\/\">CC BY-NC: Attribution-NonCommercial<\/a><\/em><\/li><\/ul><\/div>\n\t\t\t\t\t\t <\/div>\n\t\t\t\t\t <\/div>\n\t\t\t <\/section>","protected":false},"author":277,"menu_order":3,"template":"","meta":{"_candela_citation":"[{\"type\":\"cc\",\"description\":\"Earth Science for High School\",\"author\":\"\",\"organization\":\"CK-12\",\"url\":\"http:\/\/www.ck12.org\/book\/CK-12-Earth-Science-For-High-School\/\",\"project\":\"\",\"license\":\"cc-by-nc\",\"license_terms\":\"\"}]","CANDELA_OUTCOMES_GUID":"","pb_show_title":"on","pb_short_title":"","pb_subtitle":"","pb_authors":[],"pb_section_license":""},"chapter-type":[],"contributor":[],"license":[],"class_list":["post-633","chapter","type-chapter","status-publish","hentry"],"part":1279,"_links":{"self":[{"href":"https:\/\/courses.lumenlearning.com\/earthscienceck12\/wp-json\/pressbooks\/v2\/chapters\/633","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/courses.lumenlearning.com\/earthscienceck12\/wp-json\/pressbooks\/v2\/chapters"}],"about":[{"href":"https:\/\/courses.lumenlearning.com\/earthscienceck12\/wp-json\/wp\/v2\/types\/chapter"}],"author":[{"embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/earthscienceck12\/wp-json\/wp\/v2\/users\/277"}],"version-history":[{"count":1,"href":"https:\/\/courses.lumenlearning.com\/earthscienceck12\/wp-json\/pressbooks\/v2\/chapters\/633\/revisions"}],"predecessor-version":[{"id":1190,"href":"https:\/\/courses.lumenlearning.com\/earthscienceck12\/wp-json\/pressbooks\/v2\/chapters\/633\/revisions\/1190"}],"part":[{"href":"https:\/\/courses.lumenlearning.com\/earthscienceck12\/wp-json\/pressbooks\/v2\/parts\/1279"}],"metadata":[{"href":"https:\/\/courses.lumenlearning.com\/earthscienceck12\/wp-json\/pressbooks\/v2\/chapters\/633\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/courses.lumenlearning.com\/earthscienceck12\/wp-json\/wp\/v2\/media?parent=633"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/earthscienceck12\/wp-json\/pressbooks\/v2\/chapter-type?post=633"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/earthscienceck12\/wp-json\/wp\/v2\/contributor?post=633"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/earthscienceck12\/wp-json\/wp\/v2\/license?post=633"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}