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中国沙漠 ›› 2008, Vol. 28 ›› Issue (3): 509-513.

• 天气与气候 • 上一篇    下一篇

夏季强沙尘暴内部热力动力特征的个例研究

岳 平1,2,3, 牛生杰3, 张 强1, 沈建国4
  

  1. 1.中国气象局兰州干旱气象研究所/甘肃省干旱气候变化与减灾重点实验室/中国气象局干旱气候变化与减灾重点开放实验室, 甘肃 兰州 730020; 2.张掖国家气候观象台, 甘肃 张掖 734000; 3.南京信息工程大学气象灾害国家重点实验室培育点, 江苏 南京 210044; 4.内蒙古自治区气象局, 内蒙古 呼和浩特 010051
  • 收稿日期:2007-02-13 修回日期:2007-04-29 出版日期:2008-05-20 发布日期:2008-05-20

Case Study of Dynamical and Thermo-dynamical Structureof Serve Dust-storm in Summer

YUE Ping1,2,3, NIU Sheng-jie3, ZHANG Qiang1, SHEN Jian-guo4   

  1. 1.Institute of Arid Meteorology, China Meteorology Administration; Opening Key Laboratory of Arid Climatic Changing and Reducing Disaster of China Meteorology Administration; Key Laboratory of Arid Climatic Changing and Reducing Disaster of Gansu Province, Lanzhou 730020, China; 2.Zhangye National Climatological Observatory, Zhangye 734000, Gansu, China; 3.KLME, Nanjing University of Information Science & Technology, Nanjing 210044, China; 4.Inner Mongolia Autonomous Region Meteorological Bureau, Hohhot 010051, China
  • Received:2007-02-13 Revised:2007-04-29 Online:2008-05-20 Published:2008-05-20

摘要:

根据对流体在热低压条件下激发强沙尘暴的机理,并应用Rennó和Ingersoll于1996年提出的热机自然对流理论,对2004年7月12日甘肃省酒泉基准站发生的强沙尘暴内部动力热力结构进行了探讨。结果表明:①在沙尘暴发生前的一小时大气底层处于干热状态,垂直方向巨大的温度梯度有利于干对流发展。②激发强沙尘暴的对流体的切向旋转速度和垂直运动速度的大小,很大程度上决定了沙尘暴的强弱。③利用酒泉站探空资料计算出的沙尘暴对流体的最大切向旋转速度为11.4 m·s-1,垂直运动速度为14.0 m·s-1;地面沙尘暴观测系统记录的平均环境风速仅为5.5 m·s-1,瞬间最大风速只9.3 m·s-1。

关键词: 沙尘暴, 动力热力结构, 自然对流, 切向速度, 垂直速度

Abstract: According to the formation mechanism of dust-storm stimulated by serve convection system under hot-low, the thermodynamical structure of a dust-storm which occurred in the Jiuquan area of Gansu Province at 20:00 on July 12, 2004 was analyzed based on the theory of hot-engine natural convection proposed by Renn and Ingersoll in 1996. Findings are as follows: ①The atmospheric bottom layer was dry and heat in an hour before dust-storm occurrence, and there was extreme temperature grade between 200 hPa and 300 hPa, which was advantageous to the development of dry convection. ②The intensity of the dust-storm was closely related to the tangential and vertical velocity of micro-scale and meso-scale convections. Being computed by the sounding data from Jiuquan station the tangential velocity of dust-storm was 11.4 m·s-1 and the vertical velocity was 14 m·s-1; the maximal surrounding velocity recorded by the surface dust-storm observational system was only 9.3 m·s-1, and the average was 5.5 m·s-1.

Key words: dust-storm, thermodynamic structure, natural convection, tangential velocity, vertical velocity

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