中国中部低层大气行星波无线电探空仪的观测研究

通过分析武汉、宜昌和恩施气象局无线电探空仪2001-2003年的观测数据,研究了中国中部地区对流层和低平流层中行星波的特性.通过Lomb-Scargle(L-S)的周期图方法发现了周期为准16天和周期为准10天的谱分量占据着主导地位.观察发现,较大振幅的行星波振荡主要集中在5-15 km之间.准16天行星波沿纬圈向西传播,对应的纬圈波数大约为2,水平波长约为17 324.8 km,传播相速度约为-12.5 m·s-1(东向为正),通过计算准16天行星波在10 km以下相位随高度的改变可以得到其垂直波长大约为25-30 km,而在对波层顶附近其相位几乎没有发生改变,呈现出静态波特性.准10天行星波沿纬圈向东传播,对应的纬圈波数大约为4,水平波长约为8627.3 km,传播相速度约为10.0 m·s-1,垂直波长约为22-40 km. 

Radiosonde Observation of Planetary Waves in the Lower Atmosphere Over the Center China

Wind data by the radiosonde observation from Wuhan, Yichang, and Enshi Meteorological Stations in the period of 2001-2003 are used to analyze the Planetary Waves （PWs） in the lower atmosphere of the center China. L-S periodgrams show that quasi-16-day PWs and quasi-10-day PWs are dominating planetary wave components in the observed period over three sites. The largeamplitude oscillation of PWs can be observed primarily from 5 km to 15 km. The quasi-16-day PWs propagate westward with a zonal wave number of 2 （the horizontal wave length is 17 324.8 km）, and the corresponding phase velocity is estimated to be -12.5 m·s^-1 （positive eastward）. The vertical wavelength is estimated to be 25-30 km according to the phase variation with height below 10 km. The phases almost keep unchanged around the tropopause which indicates they may be stationary waves. Quasi-10-day PWs propagate eastward with a wave number of 4 （the horizontal wave length is 8627.3 km） and the corresponding phase velocity is estimated to be 10.0 m·s^-1, the vertical wave length is 22-40 km.