[外语类试卷]大学英语六级模拟试卷227及答案与解析.doc
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1、大学英语六级模拟试卷 227及答案与解析 一、 Part I Writing (30 minutes) 1 Directions: For this part, you are allowed 30 minutes to write a letter on behalf of the Students Union and the Academic Lectures Association to invite a visiting foreign professor, David, to deliver a presentation to the students in your univers
2、ity. You are NOT allowed to include the name of your university in this letter. You should write at least 150 words following the outline given below. 1. 对这位知名的外籍教授的到来表示欢迎 2表达希望该教授就某个话题在学校进行讲座的希望和对 讲座的一些基本设想 3希望教授可以接受邀请,并对教授的宝贵时间表示感谢 二、 Part II Reading Comprehension (Skimming and Scanning) (15 minut
3、es) Directions: In this part, you will have 15 minutes to go over the passage quickly and answer the questions attached to the passage. For questions 1-4, mark: Y (for YES) if the statement agrees with the information given in the passage; N (for NO) if the statement contradicts the information give
4、n in the passage; NG (for NOT GIVEN) if the information is not given in the passage. 1 Greenhouse Effect . Introduction Greenhouse Effect, the capacity of certain gases in the atmosphere to trap heat emitted from the Earths surface, thereby insulating and warming the Earth. Without the thermal blank
5、eting of the natural greenhouse effect, the Earths climate would be about 33 Celsius degrees coolertoo cold for most living organisms to survive. The greenhouse effect has warmed the Earth for over 4 billion years. Now scientists are growing increasingly concerned that human activities may be modify
6、ing this natural process, with potentially dangerous consequences. Since the advent of the Industrial Revolution in the 1700s, humans have devised many inventions that burn fossil fuels such as coal, oil, and natural gas. Burning these fossil fuels, as well as other activities such as clearing land
7、for agriculture or urban settlements, releases some of the same gases that trap heat in the atmosphere, including carbon dioxide, methane, and nitrous oxide. These atmospheric gases have risen to levels higher than at any time in the last 420,000 years. As these gases build up in the atmosphere, the
8、y trap more heat near the Earths surface, causing Earths climate to become warmer than it would naturally. Scientists call this unnatural heating effect global warming and blame it for an increase in the Earths surface temperature of about 0.6 Celsius degrees over the last nearly 100 years. Without
9、remedial measures, many scientists fear that global temperatures will rise 1.4 to 5.8 Celsius degrees by 2100. These warmer temperatures could melt parts of polar ice caps and most mountain glaciers, causing a rise in sea level of up to lm within a century or two, which would flood coastal regions.
10、Global warming could also affect weather patterns causing, among other problems, prolonged drought or increased flooding in some of the worlds leading agricultural regions. . How the Greenhouse Effect Works The greenhouse effect results from the interaction between sunlight and the layer of greenhou
11、se gases in the Earths atmosphere that extends up to 100 km above Earths surface. Sunlight is composed of a range of radiant energies known as the solar spectrum, which includes visible light, infrared light (红外线 ), X-rays, and ultraviolet light. When the Suns radiation reaches the Earths atmosphere
12、, some 25 percent of the energy is reflected back into space by clouds and other atmospheric particles. About 20 percent is absorbed in the atmosphere. For instance, gas molecules in the uppermost layers of the atmosphere absorb the Suns X-rays. The Suns ultraviolet (紫外线的 ) radiation is absorbed by
13、the ozone layer, located 19 to 48 km above the Earths surface. About 50 percent of the Suns energy, largely in the form of visible light, passes through the atmosphere to reach the Earths surface. Soils, plants, and oceans on the Earths surface absorb about 85 percent of this heat energy, while the
14、rest is reflected back into the atmospheremost effectively by reflective surfaces such as snow, ice, and sandy deserts. In addition, some of the Suns radiation that is absorbed by the Earths surface becomes heat energy in the form of long-wave infrared radiation, and this energy is released back int
15、o the atmosphere. Certain gases in the atmosphere, including water vapor, carbon dioxide, methane, and nitrous oxide, absorb this infrared radiant heat, temporarily preventing it from dispersing into space. As these atmospheric gases warm, they in mm emit infrared radiation in all directions. Some o
16、f this heat returns back to Earth to further warm the surface in what is known as the greenhouse effect, and some of this heat is eventually released to space. This heat transfer creates equilibrium between the total mount of heat that reaches the Earth from the Sun and the amount of heat that the E
17、arth radiates out into space. This equilibrium or energy balancethe exchange of energy between the Earths surface, atmosphere, and spaceis important to maintain a climate that can support a wide variety of life. The heat-trapping gases in the atmosphere behave like the glass of a greenhouse. They le
18、t much of the Suns rays in, but keep most of that heat from directly escaping. Because of this, they are called greenhouse gases. Without these gases, heat energy absorbed and reflected from the Earths surface would easily radiate back out to space, leaving the planet with an inhospitable temperatur
19、e close to-19 , instead of the present average surface temperature of 15 . To appreciate the importance of the greenhouse gases in creating a climate that helps sustain most forms of life, compare Earth to Mars and Venus (金星 ). Mars has a thin atmosphere that contains low concentrations of heat-trap
20、ping gases. As a result, Mars has a weak greenhouse effect resulting in a largely frozen surface that shows no evidence of life. In contrast, Venus has an atmosphere containing high concentrations of carbon dioxide. This heat-trapping gas prevents heat radiated from the planets surface from escaping
21、 into space, resulting in surface temperatures that average 462 too hot to support life. . Understanding the Greenhouse Effect Although concern over the effect of increasing greenhouse gases is a relatively recent development, scientists have been investigating the greenhouse effect since the early
22、1800s. French mathematician and physicist Jean Baptist Joseph Fourier, while exploring how heat is conducted through different materials, was the first to compare the atmosphere to a glass vessel in 1827. Fourier recognized that the air around the planet lets in sunlight, much like a glass roof. In
23、the 1850s British physicist John Tyndall investigated the transmission of radiant heat through gases and vapors. Tyndall found that nitrogen and oxygen, the two most common gases in the atmosphere, had no heat-absorbing properties. He then went on to measure the absorption of infrared radiation by c
24、arbon dioxide and water vapor, publishing his findings in 1863 in a paper titled “On Radiation Through the Earths Atmosphere.“ Swedish chemist Svante August Arrhenius, best known for his Nobel Prize-winning work in electrochemistry, also advanced understanding of the greenhouse effect. In 1896 he ca
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- 外语类 试卷 大学 英语六级 模拟 227 答案 解析 DOC
