A CASE OF MESOSCALE CONVECTIVE COMPLEX EVOLVING INTO A VORTEX

A case of mesoscale convective complex(MCC)which evolved into a vortex is documented in this paper.As theMCC entered into the dissipating phase,a well-defined spirally banded structure became visible in the satellite image.The blackbody temperature(TBB)of the residual cold-cloud-shield indicates the vortex existed in the layer from 400 to250 hPa.According to the upper air analysis,the upper level vortex was an anticyclone.The MCC-generated vortex wasvisualized in the satellite images because it was located in the subtropical high where the wind field was very weak.     

暴雨类冷涡与非暴雨类冷涡的合成对比分析

选择了８例典型的东北冷涡暴雨过程和８例典型的东北冷涡弱降水过程进行了合成对比分析，发现暴雨类冷涡其暴雨主要出现在冷涡的发展阶段，而非暴雨类冷涡的降水主要发生在冷涡的成熟阶段；暴雨类冷涡与其南侧的副热带低值系统联系密切，非暴雨类冷涡的这一特点不甚明显；暴雨类冷涡的两个降水中心分别出现在系统东侧偏南和南侧偏东一些的地，距系统中心大约３００－４００ｋｍ和７００－８００ｋｍ，这些区域处于低层辐合、高层辐菜     

A CASE OF MESOSCALE CONVECTIVE COMPLEX EVOLVING INTO A VORTEX*

A case of mesoscale convective complex(MCC) which evolved into a vortex is documented in this paper.As the MCC entered into the dissipating phase,a well-defined spirally banded structure became visible in the satellite image.The blackbody temperature(TBB) of the residual cold-cloud-shield indicates the vortex existed in the layer from 400 to 250 hPa.According to the upper air analysis,the upper level vortex was an anticyclone.The MCC-generated vortex was visualized in the satellite images because it was located in the subtropical high where the wind field was very weak.     

Hydrodynamical Modeling Of Oceanic Vortices

Mesoscale coherent vortices are numerous in the ocean.Though they possess various structures in temperature and salinity,they are all long-lived, fairly intense and mostly circular. Thephysical variable which best describes the rotation and the density anomaly associated with coherent vortices is potential vorticity. It is diagnostically related to velocity and pressure, when the vortex is stationary. Stationary vortices can be monopolar (circular or elliptical) or multipolar; their stability analysis shows thattransitions between the various stationary shapes are possible when they become unstable. But stable vortices can also undergo unsteady evolutions when perturbed by environmental effects, likelarge-scale shear or strain fields, -effect or topography. Changes in vortex shapes can also result from vortex interactions. such as the pairing, merger or vertical alignment of two vortices, which depend on their relative polarities and depths. Such interactions transfer energy and enstrophy between scales, and are essential in two-dimensional and in geostrophic turbulence. Finally, in relation with the observations, we describe a few mechanisms of vortex generation.     

The 1.5–5-day eastward waves in the upper stratosphere–mesosphere as observed by the Esrange meteor radar and the SABER instrument

Data of neutral meridional wind obtained by the meteor radar at Esrange and data of temperature and pressure measured by the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument on board the Thermosphere–Ionosphere–Mesosphere Energetics and Dynamics (TIMED) spacecraft were studied with respect to a day-to-day atmospheric variability with periods ranging from 1.5 to 5 days. The detailed analysis was carried out for February 2004. Perturbations of the atmospheric parameters at the examined periods appeared mainly as eastward-propagating waves of zonal wavenumbers 1 and 2. We suggested that these waves excited by the jet instability on both flanks of the polar-night jet in the upper stratosphere and mesosphere interact nonlinearly with each other, and this interaction generates secondary waves. The radar observed both primary and secondary waves at mesospheric heights. The data analysis supports this suggestion. Under conditions of weaker instability observed in February 2003 the perturbations of atmospheric parameters of periods ranging from 1.5 to 5 days had smaller amplitudes at heights of the mesosphere than those in February 2004. It was found that the Eliassen-Palm fluxes calculated for the waves generated by the jet instability were mainly downward directed. This result suggests a possible dynamical influence of the mesospheric layers on the lower atmospheric levels.     

青藏高原大气低频振荡的源、汇特征分析

使用1998年美国NCAR再分析的逐日资料，研究了1998年夏季青藏高原大气低频振荡的源、汇特征。青藏高原对于纬向风的低频波来说，有时是低频振荡的源区，有时是汇区。通过计算低频涡度的通量散度，进一步研究了低频涡源、涡汇特征。青藏高原在不同时间和不同部位，低频涡源、涡汇具有不同的分布特征，传播特征也不尽相同，青藏高原上空100hPa低频涡源、涡汇受到了南亚高压的很大影响。     

一次强龙卷风过程破坏力的估计

估计了 1 975年 6月 7日山东省栖霞县一次强龙卷风的环流参数 :最大风速可达6 2m·s-1,最大平移风速 1 2m·s-1,最大旋转风速 50m·s-1,总压力降为 2 7 5hPa。对龙卷风产生的极强的瞬时荷载、强烈的旋转扭曲、突然压力降及飞射物造成的破坏力进行了估计。     

非定常不稳定液固两相流动中旋涡对颗粒运动影响的数值研究

构建起双向耦合的液固两相流动旋涡动力学模型与数值方法;应用离散涡方法,计算非定常不稳定水流场;采用Lagrange方法模拟颗粒运动,颗粒对流体的反作用通过修正涡泡运动速度来实现。利用所建模型,计算了两种St数的泥沙粒子在圆柱绕流场中的运动。结果证明了液固两相流动中颗粒运动与旋涡存在着明确的相关结构:(1)当水沙混合物中的泥沙颗粒碰上旋涡时,泥沙颗粒被卷入旋涡中,被卷入旋涡中的泥沙颗粒在运动过程中始终分布于旋涡区;(2)均匀水沙混合物绕圆柱流动,由于流体流过圆柱时产生剧烈分离流动,使得在尾迹流内中等St数 (St～o (1))的泥沙颗粒从均匀水沙混合物中分离出来而往旋涡区聚集。     

北半球大气臭氧层的遥相关结构分析

本文分析了北半球冬春季和夏秋季大气O_3层的遥相关结构.结果发现,O_3层存在一系列遥相关型,其时域特征与O_3层槽脊及大气环流型的变化有关,主要可分为:(1)O_3槽间型,(2)O_3槽脊型,(3)O_3脊间型.表明遥相关区域的空间分布具有波状结构.随着环流型的季节调整,冬春季与夏秋季O_3层的遥相关结构存在着差异.所得结果可显示出大气环流对O_3的输送作用以及环流系统振荡导致的O_3层异常分布,这对进一步揭示O_3层的时域演变特征具有重要意义.     

试论旋扭构造形成的地球动力学模式——以欧亚旋扭构造体系为例

形成旋扭构造的动力可概括为五个方面:地块随着地球自转速率的变化,局部发生的旋扭;漂移在软流圈之上的地块遇到上拱的“热柱”受到局部牵制而旋扭;地幔熔融体物质对流循环产生蠕动式旋扭;岩石圈拖曳牵动引起旋扭;重力控制下密度分异所引起的水平漫流碰接于上升物质而旋转。欧亚大陆上分布着涡轮状、帚状、莲花状、连环状等各种旋扭构造。