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ATMOSPHERIC STRUCTURE. The vertical distribution of
ATMOSPHERIC STRUCTURE. The vertical distribution of

... increase and begins to drop as the air loses heat to space by radiation, mainly from carbon dioxide. The temperature drops to near -90°C at the top of this layer, the mesopause, at an altitude of about 85 to 90 kilometers. The mesosphere is where meteors heat up and become visible. [See Mesosphere. ...
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... consists of several layers with different temperatures, pressures, and compositions. ...
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atmosphere_and_wind - Red Hook Central Schools

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... • There will be more global warming is in our future according to the results of computer models summarized by the IPCC. For the next two decades warming of about 0.2° Celsius is projected. If we continue to emit as many, or more, greenhouse gases, this will cause more warming during the 21st Centur ...
L`atmosphère : la pression atmosphérique
L`atmosphère : la pression atmosphérique

... include oxygen (O2), which is necessary for ________________________, and carbon dioxide (CO2), which is necessary for ________________________ in plants. b) The Earth’s ________________________ pulls the gas particles toward the Earth. This explains why most gases in the air are near the __________ ...
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Layers of the Atmosphere

... In the upper mesosphere and the lower thermosphere, nitrogen and oxygen atoms absorb harmful solar energy. This area is called the ionosphere. ...
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Earth`s Atmospheric Layers

... • Average temperature: -50º to 0º • Ozone layer located at the top of this layer. • Gets warmer as you go up in the layer: ozone absorbs radiation from the sun, which makes it hotter. • As altitude increases, temperature increases ...
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... • Average temperature: -50º to 0º • Ozone layer located at the top of this layer. • Gets warmer as you go up in the layer: ozone absorbs radiation from the sun, which makes it hotter. • As altitude increases, temperature increases ...
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Name_______________________ Chapter 9 Atmosphere Study

... Sun’s uneven heating of Earth’s surface forms giant loops, or cells, of moving air. The Coriolis effect deflects the surface winds to the west, or east, setting up belts of prevailing winds that distribute heat and moisture around the globe. ...
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... In the troposphere, ozone is a pollutant. However, ozone in the stratosphere is beneficial. It blocks harmful It can harm plant and animal tissues ultraviolet rays from the sun, protecting life on Earth. Without the and it can damage rubber and plastic. ozone layer in the stratosphere, more of the S ...
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... Manmade (ex. the burning of hydrocarbon fossil fuels, CnH2n+2) and natural (ex. volcanic eruptions) releases of “Greenhouse gases” into the atmosphere may increase temperatures on the Earth over the next century, leading to the melting of glaciers; disruptions in weather patterns, climate zones, and ...
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Study Guide – EARTH`S ENERGY FINAL EXAM

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Met10_lecture_01 - Department of Meteorology and Climate

... Oxygen molecules in this layer absorb energetic solar rays which warm the air. Since there are few atoms and molecules the absorption of a small amount of solar energy can cause a large increase in temperature that may exceed 500°C! It is in this layer that charged particles from the sun interact wi ...
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The Earth`s Atmosphere The Earth`s Atmosphere

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Atmosphere of Venus



The atmosphere of Venus is the layer of gases surrounding Venus. It is composed primarily of carbon dioxide and is much denser and hotter than that of Earth. The temperature at the surface is 740 K (467 °C, 872 °F), whereas the pressure is 93 bar. The Venusian atmosphere supports opaque clouds made of sulfuric acid, making optical Earth-based and orbital observation of the surface impossible. Information about the topography has been obtained exclusively by radar imaging. Aside from carbon dioxide, the other main component is nitrogen. Other chemical compounds are present only in trace amounts.Mikhail Lomonosov was the first person to hypothesize the existence of an atmosphere on Venus based on his observation of the transit of Venus of 1761 in a small observatory near his house in Saint Petersburg.The atmosphere is in a state of vigorous circulation and super-rotation. The whole atmosphere circles the planet in just four Earth days, much faster than the planet's sidereal day of 243 days. The winds supporting super-rotation blow as fast as 100 m/s (~360 km/h or 220 mph). Winds move at up to 60 times the speed of the planet's rotation, while Earth's fastest winds are only 10% to 20% rotation speed. On the other hand, the wind speed becomes increasingly slower as the elevation from the surface decreases, with the breeze barely reaching the speed of 10 km/h on the surface. Near the poles are anticyclonic structures called polar vortices. Each vortex is double-eyed and shows a characteristic S-shaped pattern of clouds.Unlike Earth, Venus lacks a magnetic field. Its ionosphere separates the atmosphere from outer space and the solar wind. This ionised layer excludes the solar magnetic field, giving Venus a distinct magnetic environment. This is considered Venus's induced magnetosphere. Lighter gases, including water vapour, are continuously blown away by the solar wind through the induced magnetotail. It is speculated that the atmosphere of Venus up to around 4 billion years ago was more like that of the Earth with liquid water on the surface. A runaway greenhouse effect may have been caused by the evaporation of the surface water and subsequent rise of the levels of other greenhouse gases.Despite the harsh conditions on the surface, the atmospheric pressure and temperature at about 50 km to 65 km above the surface of the planet is nearly the same as that of the Earth, making its upper atmosphere the most Earth-like area in the Solar System, even more so than the surface of Mars. Due to the similarity in pressure and temperature and the fact that breathable air (21% oxygen, 78% nitrogen) is a lifting gas on Venus in the same way that helium is a lifting gas on Earth, the upper atmosphere has been proposed as a location for both exploration and colonization.On January 29, 2013, ESA scientists reported that the ionosphere of the planet Venus streams outwards in a manner similar to ""the ion tail seen streaming from a comet under similar conditions.""
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