对流边界层的Lyapounov稳定性分析

针对一个简单的大气边界层干热对流模式,根据耗散结构理论及Ｌｙａｐｏｕｎｏｖ第二稳定性理论,分析了热对流边界层的热力学和动力学稳定性,并将二者结合构造了一个广义Ｌｙａｐｏｕｎｏｖ函数,进而在小扰动下给出了边界层的非平衡定态（参考态）发生不稳定的临界Ｒａｙｌｅｉｇｈ数和对流得以发展的临界浮力加速度。数值试验结果与理论分析一致。     

大对流有效位能和条件不稳定下地形降水的三维理想数值研究

利用WRF(V3.01)中尺度数值模式,对具有大对流有效位能和条件不稳定层结下中小尺度地形对降水的影响进行了一系列三维理想数值试验,探讨了不同地形高度、尺度、形状(水平形态比)以及环境气流对降水模态和分布的影响.结果发现:在大对流有效位能(2875 J/kg)和条件不稳定(Nw≈0.01 s-1)下,地形重力波破碎触发...     

AMSU-B微波资料反演对流云中冰粒子含量

微波遥感可以穿透云顶直接探测云内的冰粒子分布,NOAA系列卫星微波湿度计(AMSU-B)的3个水汽吸收波段对冰粒子含量的变化有着很好的响应,受冰粒子的强烈散射衰减作用,亮温随冰粒子的增加而降低.因此,可以利用3个水汽通道亮温变化判断云中冰粒子的含量.根据模拟实验结果,确定了对流云状态下各水汽通道对冰粒子的响应高度,冰粒...     

Low latitude dynamical response to vortex split sudden stratospheric warming: An Eliassen Palm Flux perspective

The present work extensively describes the tropical dynamical changes during the Vortex split Major Stratospheric Warming (V-MSW) event occurred in recent decades. For better visualization of high latitude influence of tropical atmosphere, in this study, we have utilized three successive major vortex split warming events occurred in winters 1984/85, 1988/89 and 2008/09. The realistic visualization of planetary wave activity and its tropical response can be achieved by using Eliassen –Palm flux as a diagnostic tool. The investigation reveals that the tropical weather shows significant changes in temperature, convection and wind circulation during the course of vortex split major stratospheric warming.     

The onset of magnetoconvection at large Prandtl number in a rotating layer II. Small magnetic diffusion

Abstract

This paper develops further a convection model that has been studied several times previously as a very crude idealization of planetary core dynamics. A plane layer of electrically-conducting fluid rotates about the vertical in the presence of a magnetic field. Such a field can be created spontaneously, as in the Childress-Soward dynamo, but here it is uniform, horizontal and externally-applied. The Prandtl number of the fluid is large, but the Ekman, Elsasser and Rayleigh numbers are of unit order. In Part I of this series, it was also supposed that the ratio thermal diffusivity diffusivity/magnetic diffusivity is O(1), but here we suppose that this ratio is large. The character of the solution is changed in this limit. In the case of main interest, when the layer is confined between electrically-insulating no-slip walls, the solution is significantly different from the solution when the mathematically simpler, illustrative boundary conditions also considered in Part I are employed. As in Part I, attention is focussed on the onset of convection as the temperature difference applied across the layer is increased, and on the preferred mode, i.e., the planform and time-dependence of small amplitude convection.     

Convection in a rotating magnetic system and Taylor's constraint

Abstract

A system is considered in which electrically conducting fluid is contained between two rigid horizontal planes and bounded laterally by a circular cylinder. The fluid is permeated by a strong azimuthal magnetic field. The strength of the field increases linearly with distance from the vertical axis of the cylinder, about which the entire system rotates rapidly. An unstable temperature gradient is maintained by heating the fluid from below and cooling from above. When viscosity and inertia are neglected, an arbitrary geostrophic velocity, which is aligned with the applied azimuthal magnetic field and independent of the axial coordinate, can be superimposed on the basic axisymmetric state. In this inviscid limit, the geostrophic velocity which occurs at the onset of convection is such that the net torque on geostrophic cylinders vanishes (Taylor's condition). The mathematical problem which describes the ensuing marginal convection is nonlinear, and was discussed previously for the planar case by Soward (1986). Here new features are isolated which result from the cylindrical geometry. New asymptotic solutions are derived valid when Taylor's condition is relaxed to include viscous effects.     

华南局地锋生及对流系统发展的模拟分析研究

2009年3月28日一条东西向的锋面出现在华南25°N附近。伴随着锋面的活动,对流降水回波午后开始在广西的梧州附近发展,并在随后几小时向东移动,组织发展成为中尺度对流系统(MCS),为广东中西部及珠三角地区带来了雷暴、暴雨、冰雹等灾害天气。应用地面自动站、雷达回波、卫星云图以及NCEP-FNL再分析资料和WRF模式的模拟结果,对锋面暴雨形成的天气特征进行了诊断分析,考察了中尺度对流系统的发展演变过程及其与局地锋生的相互关系。结果表明,锋面对流系统形成发展于一个东西向水平尺度约200km的地面中尺度辐合线附近,对流起始发展于具有较大对流有效位能(CAPE)和较小对流抑制位能(CIN)的区域。伴随着对流的发展,锋面强度增强。锋生函数的计算发现,非绝热项和倾斜项分别在由对流引起的次级环流的上升运动支和下沉运动支起锋生作用,是引发中尺度锋生的主要影响因子。而相对来说,水平辐合项和形变项的作用却比较小。这与大尺度的锋生过程不同,中尺度锋生更主要的是由热力直接触发的非地转环流所驱动。涡度场的演变分析还发现,沿着850hPa锋区大的正涡度区与500hPa的强上升运动区对应良好,对流系统发展与中尺度锋生之间存在着类似于第二条件不稳定机制的相互作用,对流增强了锋生过程,锋面则对中尺度对流系统的发展起组织作用。中尺度锋生对对流组织发展的作用作为此类灾害天气形成的原因值得关注。     

MJO对中国春季降水影响的数值模拟研究

利用IAP-AGCM4.0模式,通过多初值集合数值模拟研究了赤道附近的大气季节内振荡(MJO)传播的两个关键位相期对中国东部春季降水的影响.当在赤道中东印度洋及赤道西太平洋引进异常非绝热加热(强MJO活动)强迫时,模式很好地模拟出了中国东部地区春季降水的异常形势,模式模拟与先期所作的诊断分析结果极为相似,即在MJO的第2-3(6-7)位相,中国长江中下游地区多雨(中国东部大部分地区降水偏少).对模式输出的高度场、风场、散度和涡度场以及水汽输送场的分析表明,中国春季降水异常的发生分别与异常非绝热加热在东亚/西北太平洋地区所造成的异常大气环流形势密切相关.对逐日响应场的分析表明,就MJO活动影响中国春季降水的可能物理过程及机制进行的讨论表明,赤道附近的异常对流加热不仅可以在赤道附近激发产生大气的罗斯贝波和开尔文波型响应,而且,还会在大气中激发产生从热带到中高纬度的罗斯贝波列遥响应.但是,由于异常对流加热发生的地区不同,大气遥响应场的形势也会十分不同,它所导致的影响也就很不一样.当异常对流加热发生在赤道中东印度洋(对应MJO的第2-3位相)时,大气的罗斯贝波列遥响应将在东亚/西太平洋地区形成有利于中国东部(尤其是长江中下游地区)春季降水偏多的形势;当异常对流加热发生在赤道西太平洋(对应MJO的第6-7位相)时,大气的罗斯贝波列遥响应将在东亚/西太平洋地区形成不利于中国东部春季降水的形势.     

Large-Eddy Simulation Of Radiation Fog

In order to study the three-dimensional structure of radiation fogand to obtain a basic understanding of its generation mechanism,a numerical experiment is performed with a large-eddysimulation model and compared with the observation at Cabauw in the Netherlands. After confirming that the results are insatisfactory agreement with the observations, the structure of thefog and its generation mechanism are examined in more detail.Before the fog forms, the atmosphere is stable and an inversionlayer exists almost adjacent to the ground surface. As the fog grows, however, the stratification is destabilized and a mixed layerdevelops gradually. The longwave radiative cooling near thefog top contributes to the destabilization more than thecondensational heating does.The evolution of the fog can be classified into three stagesaccording to the behaviour of turbulent kinetic energy (TKE):formation, development, and dissipation stages.The fog layer has different flow structures at each stage.During the formation stage, longitudinal rolls similar tostreaks in channel flows appear near the ground surface.The development stage is characterized by an initiation oftransverse bands due to Kelvin–Helmholtz instability anda sudden increase of TKE. During the dissipation stage, longitudinalrolls and polygonal cells due to convective instability are organized.     

对流和加热对重力惯性波的激发

用线性模型讨论了对流和加热对重力惯性波的激发，分别讨论了初始垂直速度扰动和初始位温扰动及大气内部加热在静态层结大气中激发的重力惯性波，及重力惯性波过程引起的大气温压场的变化。得到的结果可以帮助理解中小尺度系统的发生发展、对流过程与环境大气的相互作用。