Numerical simulation of atmospheric general circulation under different obliquity of Earth

Xinhua Liu
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引用次数: 3

Abstract

By using the second version of the Community Atmosphere Model (CAM2) of NCAR, the general circulations of the Earth's atmosphere were simulated under different obliquity condition. The results imply that three-cell circulation turn weak when the obliquity turn large except that the three-cell circulation in Northern Hemisphere in winter, Hadley circulation in Southern Hemisphere in spring and Hadley circulation in Southern Hemisphere in summer turn strong with the obliquity turns large. For annual mean three-cell circulation, its intensity turns weak with the obliquity turn large. The extension of Hadley circulation in Southern Hemisphere turn large when the obliquity turns large, while the extension of Hadley circulation in Northern Hemisphere and Ferrel circulation in Southern Hemisphere turn small with the obliquity turns large. The ascending branch of Hadley circulation in the Southern Hemisphere turn strong significantly under the 60° obliquity condition then normal obliquity of Earth. Furthermore, for annual mean the extension and the velocity of easterly wind in stratosphere over the equator turn large when the obliquity turns large. While the extension of the westerly wind turn small with the obliquity turns large. With the obliquity turns large, the strength of jet stream in Northern Hemisphere turn weak, the strength of jet stream in Southern Hemisphere turn strong. The same characteristics for the four seasons are that with the obliquity turns large, the easterly in the troposphere and westerly in the Northern Hemisphere turn weak, the strength of jet stream at mid-latitude in Northern Hemisphere turn weak. The difference are that with the obliquity turns large, the strength of jet stream at mid-latitude in Southern Hemisphere in spring turn strong, the westerly wind at middle and high latitude have opposite change trends in summer and autumn in Southern Hemisphere, the global westerly wind in winter turn weak.
不同地球倾角下大气环流的数值模拟
利用NCAR第二版群落大气模式(CAM2),模拟了不同倾角条件下的地球大气环流。结果表明:除了北半球冬季环流、南半球春季Hadley环流和南半球夏季Hadley环流随着倾角增大而变强外,北半球冬季环流、南半球春季Hadley环流和南半球夏季Hadley环流在倾角增大时变弱。对于年平均三单元环流,其强度随着倾角的增大而减弱。当倾角变大时,南半球Hadley环流的扩展变大,而北半球Hadley环流和南半球Ferrel环流的扩展随着倾角变大而变小。南半球Hadley环流上升分支在地球60°倾角条件下明显转强,而在地球正常倾角条件下则明显转强。此外,年平均赤道上空平流层东风的延伸和速度随着倾角的增大而增大。而西风的延伸范围随着倾角的增大而变小。随着倾角变大,北半球急流强度变弱,南半球急流强度变强。四季的相同特征是,随着倾角变大,对流层东风和北半球西风减弱,北半球中纬度急流强度减弱。不同之处在于,随着倾角变大,南半球春季中纬度急流强度变强,南半球夏季和秋季中高纬度西风变化趋势相反,冬季全球西风变弱。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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