Structure of the Sun
1 The temperature of the Sun is over 5,000 degrees Fahrenheit at the surface, but it rises to perhaps more than 16 million degrees at the center. The Sun is so much hotter than the Earth that matter can exist only as a gas, except at the core. In the core of the Sun, the pressures are so great against the gases that, despite the high temperature, there may be a small solid core. However, no one really knows, since the center of the Sun can never be directly observed.
2 Solar astronomers do know that the Sun is divided into five layers of zones. Starting at the outside and going down into the sun, the zones are the corona, chromosphere, photosphere, convection zone, and finally the core. The first three zones are regarded as the Suns atmosphere. But since the Sun has no solid surface, it is hard to tell where the atmosphere ends and the main body of the Sun begins.
3 The Suns outermost layer begins about l0000 miles above the visible surface and goes outward for millions of miles. This is the only part of the Sun that can be seen during an eclipse such as the one in February 1979. At any other time, the corona can be seen only when special instruments are used on cameras and telescopes to shut out the glare of the Suns rays.
4 The corona is a brilliant, pearly white, filmy light, about as bright as the full Moon. Its beautiful rays are a sensational sight during an eclipse. The coronas rays flash out in a brilliant fan that has wispy spider-like rays near the Suns north and south poles. The corona is thickest at the Suns equator.
5 The corona rays are made up of gases streaming outward at tremendous speeds and reaching a temperature of more than 2 million degrees Fahrenheit. The rays of gas thin out as they reach the space around the planet. By the time the Suns corona rays reach the Earth, they are weak and invisible.
23Paragraph 2
24Paragraph 3
25Paragraph 4
26Paragraph 5
A.Basic description of the core
B. Characteristics of the corona
C. The composition of the corona rays
D. Five layers of zones of the sun
E. Characteristics of the corona rays
F. The eclipse in February 1979
正确答案:DBEC
6月雅思写作大预测
雅思趋势预测及备考指导—口语话题
2月4日雅思考试听力真题预测分析
雅思作文回顾之政府类
雅思预测:10月9日口语考试展望
9月11日全国口语预测
3月10日A类雅思写作预测(一)
8月13日雅思考试预测
4月12、14日雅思口语预测(Part2-place)
雅思口语:10月份考试趋势展望及预测
2月4日雅思考试阅读真题预测分析
雅思作文回顾之社会类别篇
雅思作文预测:大作文一级预测类
1月22日雅思考试全面预测
2月19日雅思预测
1月12日A类雅思写作预测
雅思作文回顾之教育类别篇
雅思预测:10月9日阅读考试展望
4月12、14日雅思口语预测(Part 1)
4月30日雅思考试预测
雅思必备:3月份雅思口语考试最新预测
权威预测:3月5日3G雅思考试预测
10月30日雅思写作考试预测
10月30日雅思口语预测
雅思考试小作文预测
2月25日G类雅思大作文预测
2012年1月21日雅思考试全面预测
3月10日A类雅思写作预测(二)
雅思作文预测:大作文三级预测类
雅思阅读考试题型展望
| 不限 |
| 英语教案 |
| 英语课件 |
| 英语试题 |
| 不限 |
| 不限 |
| 上册 |
| 下册 |
| 不限 |