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北半球准定常行星波经向结构及特征尺度分析
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  • 英文篇名:Meridional structure and characteristic scale of quasi-stationary planetary waves in the Northern Hemisphere
  • 作者:孙诚 ; 张静 ; 宫湛秋 ; 李建平
  • 英文作者:SUN Cheng;ZHANG Jing;GONG Zhanqiu;LI Jianping;College of Global Change and Earth System Science,Beijing Normal University;Laboratory for Regional Oceanography and Numerical Modeling,Qingdao National Laboratory for Marine Science and Technology;
  • 关键词:准定常行星波 ; 经向波动 ; 纬向波动 ; 定常波数
  • 英文关键词:quasi-stationary planetary wave;;meridional fluctuation;;latitude fluctuation;;stationary wave
  • 中文刊名:BSDZ
  • 英文刊名:Journal of Beijing Normal University(Natural Science)
  • 机构:北京师范大学全球变化与地球系统科学研究院;青岛海洋科学与技术国家实验室区域海洋动力学与数值模拟功能实验室;
  • 出版日期:2019-02-15
  • 出版单位:北京师范大学学报(自然科学版)
  • 年:2019
  • 期:v.55
  • 基金:国家自然科学基金资助项目(41775038,41790474)
  • 语种:中文;
  • 页:BSDZ201901001
  • 页数:10
  • CN:01
  • ISSN:11-1991/N
  • 分类号:5-14
摘要
准定常行星波对于热带外地区的天气和气候有着举足轻重的影响.以往对于准定常行星波的研究主要针对某一纬度或多纬度平均的纬向波动进行分析,因此准定常行星波的经向结构及特征尺度尚不清楚.利用经典的Rossby波的频散关系,对传统定常波的水平全波数的计算方法进行了改进,将纬向和经向波数进行分离,得到了描述准定常行星波运动学特征的纬向和经向特征波数,从理论上给出了准定常行星波空间尺度的动力约束条件,进而对北半球行星波动的经向结构及特征空间尺度进行了分析.结果表明:在北半球热带外地区,冬季准定常行星波的经向尺度以1波为主,表明准定常行星波的经向结构多为偶极子型;而纬向波数随纬度的增高而减小,表明大尺度的准定常波可以在高纬度传播,而较小尺度的准定常波只能在较低纬度传播.进一步利用大气环流观测资料分析冬季不同纬度间准定常行星波(纬向1~3波)的位相关系,发现不同纬度间的准定常行星波以反位相关系为主,且行星波的经向活动区域随着纬向波数的减小而向极地延伸.观测得到的冬季准定常行星波的纬向和经向结构特征,与理论推导的纬向和经向特征波数的时空分布特征基本对应.
        Quasi-stationary planetary waves have significant impact on weather and climate in both tropical and extra-tropical regions.Previous studies mainly focused on latitudinal fluctuations,but meridional structure and characteristic scale were unclear.Classical Rossby wave dispersion relation was used to improve calculation of horizontal full wave number in conventional steady wave,with separated zonal wave number and meridional wave number.Latitudinal and meridional characteristics describing kinematics of quasi-stationary planetary wave were obtained,characteristic spatial scales of planetary waves in the Northern Hemisphere were analyzed.In extra-tropical regions in the northern hemisphere,meridional scale of quasi-stationary planetary waves in winter was dominated by 1 wave,indicating that meridional structure of quasi-stationary planetary waves was mostly of the dipole type.Latitudinal wave number was found to decrease with increasing latitude,indicating that large-scale quasi-steady waves could propagate at high latitudes while smaller scale quasi-steady waves could only propagate at lower latitudes.Analyzing phase relations of quasi-stationary planetary waves(1-3 waves in latitude)between different latitudes in winter found that quasi-stationary planetary waves between different latitudes were mainly inversely related.Further,meridional region of planetary waves was found to extend to the poles as zonal wave number decreased.Observed characteristics of latitudinal and meridional structures of quasi-stationary planetary waves in winter basically corresponded to space-time distribution characteristics of characteristic wave number in zonal and meridional directions.
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