非线性垂直切变基流中横波型扰动的不稳定

通过数值计算扰动的波谱和谱函数,对垂直非线性切变基流中横波型扰动的不稳定作了数值研究,给出了不稳定谱函数的结构,讨论了不稳定的性质。主要结论有:在基流为非线性垂直切变时,对三支波动连续谱区互不重叠的天气尺度情况,此时出现的不稳定扰动其性质是准地转涡旋波的不稳定,即Rossby波的斜压不稳定。在中α尺度中高端,虽有涡旋波和重力惯性波连续谱区的部分重叠,但这时不稳定的性质仍是涡旋波的不稳定,即准平衡的斜压不稳定。在中α尺度低端,既有准平衡涡旋波的不稳定,又有非平衡的涡旋-重力惯性混合波的不稳定(第一类混合波不稳定)。中β尺度不稳定的性质则是非平衡的涡旋-重力惯性混合波的不稳定,包括第一类混合波不稳定和第二类混合波不稳定。上述情况与线性垂直切变基流的结论相一致,但这里因基流垂直分布较复杂,垂直方向会出现散涡比以1为界的多段交替分布。综上,对于横波型扰动,只要基流不是常数,且层结稳定,虽此时存在纯重力惯性波连续谱区,但均无纯重力惯性波的不稳定,只有涡旋-重力惯性混合波的不稳定。     

切变基流中惯性重力波的发展

采用分层浅水波方程、一简单的二层模式和ＷＫＢ方法，考虑基本气流的垂直切变，水平切变以及地形的影响，分析了惯性重力波的发展变化，得到有关导式波和曳式波发展的环境条件。     

垂直切变和地形影响下惯性重力波的发展

采用分层浅水波方程和ＷＫＢ方法，分别讨论了在基流垂直切变和地形的影响下，二维惯性重力波的稳定性及其发展，并根据理论结果试图解释１９９２年６月２１日发生在京津冀的一次飑线演变与惯性重力波之间的关系，这可能为飑线预报提供一种思路     

经向基流和地形对惯性重力波的影响

采用分层浅水波方程组和ＷＫＢ方法，分别讨论了经向基流的垂直切变和南北走向的地形对二维惯性重力波的移速，稳定性以及发展的影响。     

切变基流对赤道大气波动稳定性的作用

在赤道β平面近似条件下，使用纬向切变基流下线性化Boussinesq方程组，分析了在纬向切变基流下几种赤道大气波动的稳定性特征。研究结果表明，基本气流的水平切变对赤道大气波动起到不稳定的作用，但是对赤道大气Kelvin波的频率、稳定性以及传播的相速度并不起作用。基本气流的水平切变使得相对于基本气流向东传播的重力惯性内波相速度减慢，而使得相对于基本气流向西传播的重力惯性内波的相速度加快，却造成相对于基本气流向西传播的Rossby波相速度减慢。基本气流的水平切变对于对赤道混合Rossby-重力惯性内波的影响主要取决于纬向波数k值的范围大小。当纬向波数k值较小时，基流的水平切变使得相对于基本气流向西传播的混合Rossby-重力惯性内波相速度加快；而当纬向波数k值较大时，则使得相对于基本气流向西传播的混合Rossby-重力惯性内波相速度减慢。在半地转近似下，风速水平切变的存在，会使得波长较大（纬向波数k→0）的赤道Rossby波相对于基本气流向西传播的相速度减慢；而风速垂直切变的存在，必然会引起这种波长较大（k→0）的Rossby波出现不稳定增长，同样也会造成赤道Rossby波相对于基本气流向西传播的相速度减慢。最后通过扰动发展能量方程，说明了基本气流的水平切变和垂直切变可以为扰动的发展提供能量来源。     

低纬斜压两层模式大气半地转适应过程

利用斜压两层模式研究了赤道平面近似下的低纬热带大气适应过程。指出低纬斜压大气适应过程主要受重力惯性内波控制。通过重力惯性内波对初始非地转能量的频散，使纬向运动达到地转平衡，而经向维持非地转运动，正压模式下称为半地转平衡，斜压模式下称为半热成风平衡。通过对垂直运动方程的求解，可知，垂直运动只与重力惯性内波相联系，其产生与初始斜压位涡度无关，而只与初始时刻的垂直运动和垂直运动倾向有关，半地转适应使运动趋向水平运动。讨论了半热成风平衡的建立及其物理机制，指出由于重力惯性内波激发出垂直运动，与垂直运动相联系的水平辐合辐散调整流场和温度场之间的关系，使温压场最终达到半热成风平衡。通过对适应过程终态的分析，指出平均温度场和切变流场之间的适应方向决定于初始非半地转扰动的尺度与斜压Ｒｏｓｓｂｙ变形半径有关的特征尺度的比值，当比值大于１时，切变流场向平均温度场适应；当比值小于１时，平均温度场向切变流场适应     

垂直切变基流中东西向地形对惯性重力波稳定性的影响

利用分层浅水波方程和小参数(WKB)方法，考虑具有垂直切变的基流和地形的作用，求得惯性重力波的局地频率方程，并根据此方程分析讨论了在多种环境条件下波动的稳定性情况。     

影响惯性重力波活动规律的动力学因子研究

通过探测发现大气重力波有明显的活动规律:重力波强度在冬、春季强于夏、秋季,在5月和10月发生急剧减弱和加强的转变,无天气过程时晚上比白天强,尤其短周期的重力波,周期为40~80min的重力波平均强度最强,其他较弱。在斜压大气和考虑积云对流加热条件下,运用积云对流参数化、Taylor公式展开等方法,推导出惯性重力波的非线性KdV方程,求出其孤立波解,以此解释以上得出的大气重力波的活动规律:惯性重力波强度随风速垂直切变增大而增大,急流是最重要的惯性重力波波源,是重力波强度在冬、春季强于夏、秋季的主要原因,亚洲急流在5月和10月的北跃和南落,是重力波强度发生急剧变化的原因,急流下方是激发惯性重力波最强的地方。一般情况下,惯性重力波强度随着大气背景流场绝对涡度增大而增大,正涡度对惯性重力波起激发和增强的作用。当惯性重力波向下传播时,波的强度随层结稳定度(N2)增大而增大,由于太阳辐射的作用白天大气层结稳定度比晚上小,这解释了在无天气过程时晚上重力波强度强于白天的原因。惯性重力波强度和波的频率成正比,这解释了周期为40~80 min比周期为140~160 min的重力波强的原因。重力波强度还与非线性积云对流参数常数b及科氏力参数f成正比。     

β中尺度暴雨系统发生发展的一种可能物理机制I. 涡旋Rossby波的相速度

使用纬向基流下横波型扰动的Boussinesq近似方程组, 分析了这种沿着基本气流方向传播的中尺度扰动发生不稳定时, 大尺度背景流场在垂直方向上的各种分布特征.在大气层结比较稳定的情况下, 如果基本气流在低层和高层较大(有可能存在低空急流和高空急流), 此时产生的β中尺度不稳定扰动相对于基流向东传播, 甚至于快速向东传播.基本气流在垂直方向上的风速切变对于中尺度横波型的扰动起着不稳定的作用.如果考虑基流的二次切变, 可以得到涡旋Rossby波的相速度表达式, 涡旋Rossby波相对于基本气流是单向传播的.涡旋Rossby波产生的物理根源是基本流场的风速二次切变, 亦即基本流场y方向的平均涡度在空间z方向上的不均匀所致.涡旋Rossby波的相速度与纬向波数也有关, 它的能量是频散的, 其在纬向x方向也存在群速度.在基本流场的风速存在二次切变时, 横波型不稳定可能是混合的涡旋Rossby重力波的不稳定; 而在基本流场的风速仅仅存在线性切变, 不存在二次切变时, 横波型扰动的不稳定则是重力惯性波的不稳定.     

台风中螺旋云带的线性理论

在指出台风中螺旋云带本质上反映了一类重力惯性内波后,应用缓变波列理论讨论了这类螺旋波的色散关系和群速度,同时进一步指出曳式波发展的能源主要是背景场转动角速度在水平和垂直方向上的不均匀性,特别是垂直切变更为重要。     

Properties and Stability of a Meso-Scale Line-Form Disturbance

By using the 3D dynamic equations for small- and meso-scale disturbances, an investigation is performed on the heterotropic instability (including symmetric instability and traversal-type instability) of a zonal line-like disturbance moving at any angle with respect to basic flow, arriving at the following results: (1) with linear shear available, the heterotropic instability of the disturbance will occur only when flow shearing happens in the direction of the line-like disturbance movement or in the direction perpendicular to the disturbance movement, with the heterotropic instability showing the instability of the internal inertial gravity wave; (2) in the presence of second-order non-linear shear, the disturbance of the heterotropic instability includes internal inertial gravity and vortex Rossby waves. For the zonal line-form disturbance under study, the vortex Rossby wave has its source in the second-order shear of meridional basic wind speed in the flow and propagates unidirectionally with respect to the meridional basic flow. As a mesoscale heterotropic instable disturbance, the vortex Rossby wave has its origin from the second shear of the flow in the direction perpendicular to the line-form disturbance and is independent of the condition in the direction parallel to the flow; (3) for general zonal line-like disturbances, if the second-order shear happens in the meridional wind speed, i.e., the second shear of the flow in the direction perpendicular to the line-form disturbance, then the heterotropic instability of the disturbance is likely to be the instability of a mixed Rossby–internal inertial gravity wave; (4) the symmetric instability is actually the instability of the internal inertial gravity wave. The second-order shear in the flow represents an instable factor for a symmetric-type disturbance; (5) the instability of a traversal-type disturbance is the instability of the internal inertial gravity wave when the basic flow is constant or only linearly sheared. With a second or nonlinear vertical shear of the basic flow taken into account, the instability of a traversal-type disturbance may be the instability of a mixed vortex Rossby – gravity wave.     

中尺度大气波动的波谱和谱函数——数学模型和计算方法

作者得到了准二维Boussinesq方程组，并用其研究了中尺度大气波动的波谱和谱函数。在一定条件下对该方程组线性化并取标准模后，可将其初边值问题转化为矩阵的广义特征值问题来进行数值求解，这样就可知原问题波谱和谱函数的性质。当无基本流且取地转参数、层结参数为常数时，可求得其波谱和谱函数的解析解。此时该模式中仅包含有一对重力惯性内波模态，且各模态均是简谐波；模态越高，垂直波数越大则波动传播得越慢，所有的模态均为离散谱，并存在聚点。对此作者用数值解作了验算，结果表明，该数值求解方案合理可行，对不太高的模态其精度也令人满意。在无基本流然而考虑层结的垂直变化后，则一般无法求取解析解，为此进行了数值求解。这时该模式仍仅包含有一对重力惯性内波的离散谱模态，不过由于层结参数的变化，各模态结构与简谐波出现了偏差。     

DEVELOPMENT OF INTERNAL INERTIAL GRAVITY WAVES IN THE ATMOSPHERE WITH HETEROGENEOUS STRATIFICATION

In this paper,by the WKB method the relation between the energy increase of internal inertial gravity waves andheterogeneous atmospheric stratification is derived,and a new generalized wave action is defined and its conservation isproved.     

与海南岛秋季暴雨有关的一类热带中尺度涡旋的动力学分析

对惯性重力内波方程组分别通过线性和非线性求解探讨造成2010年10月海南岛一次特大暴雨中一类热带中尺度涡旋生成发展的动力、热力机制,研究发现:（1）在副热带高压和大陆冷高压南侧反气旋性纬向水平风切变大值区、静力不稳定大气层结、积云对流潜热释放、低空急流、适当强度的冷空气有利于热带中尺度涡旋的形成和发展;（2）非线性惯性重力内波的孤立波解与这类热带中尺度涡旋有很好的联系,在静力不稳定的大气层结下,热带中尺度涡旋的形态主要由对流凝结潜热加热所决定,即潜热加热下的孤立波解要求热带中尺度涡旋在垂直方向是一个浅薄的涡旋系统;另外强盛的对流凝结潜热对热带中尺度涡旋垂直运动振幅的增强起主要作用,更有利于涡旋的发展和维持。基于天气事实分析的理论研究为深化影响海南的热带中尺度涡旋乃至南海中尺度对流系统的机理认识进行了探索。      

A unified linear theory of wavelike perturbations under general ocean conditions

A linearized instability analysis model with five unknowns was proposed to describe disturbance motions under general oceanic background conditions, including large-scale current shear, density stratification, frontal zone, and arbitrary topography. A unified linear theory of wavelike perturbations for surface gravity waves, internal gravity waves and inertial gravity waves was derived for the adiabatic case, and the solution was then found using Fourier integrals. In this theory, we discarded the assumptions widely accepted in the literature concerning derivations of wave motions such as the irrotationality assumption for surface gravity waves, the rigid-lid approximation for internal gravity waves, and the long-wave approximation for inertial gravity waves. Analytical solutions based on this theory indicate that the complex dispersion relationships between frequency and wave-number describing the propagation and development of the three types of wavelike perturbation motions include three components: complex dispersion relationships at the sea surface; vertical invariance of the complex frequency; and expressions of the vertical wave-number (phase). Classical results of both surface waves and internal waves were reproduced from the unified theory under idealized conditions. The unified wave theory can be applied in the dynamical explanation of the generation and propagation properties of internal waves that are visible in the satellite SAR images in the southern part of the China Seas. It can also serve as the theoretical basis for both a numerical internal-wave model and analytical estimation of the ocean fluxes transported by wavelike perturbations.     

THE CISK MECHANISM AND THE INERTIAL GRAVITATIONAL WAVES IN SHEAR FLOW

By using the symmetric equations of atmospheric dynamics in y-z plane with vertical and horizontal shear of wind, the nonlinear ordinary differential equation is derived with the method of travelling wave.Its stability is discussed by using the theory of nonlinear stability and the KDV equation is solved. The effects of linear CISK, nonlinear CISK, inertial stability and vertical shear of wind on the amplitude and the width of isolated inertial gravitational wave are discussed. In order to understand deeply the formation and development of meso-scale synoptic systems, such as the squall line, MCC, the cold surge of Asia high and typhoon, the factors of development of the isolated inertial gravity wave are analysed.     

Atmospheric Disturbances that Generate Intermittent Turbulence in Nocturnal Boundary Layers

Using the unprecedented observational facilities deployed duringthe 1999 Cooperative Atmosphere-Surface Exchange Study (CASES-99),we found three distinct turbulent events on the night of 18October 1999. These events resulted from a density current,solitary wave, and internal gravity wave, respectively. Our studyfocuses on the turbulence intermittency generated by the solitarywave and internal gravity wave, and intermittent turbulenceepisodes associated with pressure change and wind direction shiftsadjacent to the ground. Both the solitary and internal gravitywaves propagated horizontally and downward. During the passage ofboth the solitary and internal gravity waves, local thermal andshear instabilities were generated as cold air was pushed abovewarm air and wind gusts reached to the ground. These thermal andshear instabilities triggered turbulent mixing events. Inaddition, strong vertical acceleration associated with thesolitary wave led to large non-hydrostatic pressure perturbationsthat were positively correlated with temperature. The directionaldifference between the propagation of the internal gravity waveand the ambient flow led to lateral rolls. These episodic studiesdemonstrate that non-local disturbances are responsible for localthermal and shear instabilities, leading to intermittentturbulence in nocturnal boundary layers. The origin of thesenon-local disturbances needs to be understood to improve mesoscalenumerical model performance.     

Some Possible Solutions of Nonlinear Internal Inertial Gravity Wave Equations in the Atmosphere

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THE SEMI-GEOSTROPHIC ADAPTATION PROCESS WITH TWO-LAYER BAROCLINIC MODEL IN LOW LATITUDE ATMOSPHERE

In this paper, the adaptation process in low latitude atmosphere is discussed by means of a two-layer baroclinic model on the equator β plane, showing that the adaptation process in low latitude is mainly dominated by the internal inertial gravity waves. The initial ageostrophic energy is dispersed by the internal inertial gravity waves, and as a result, the geostrophic motion is obtained in zonal direction while the ageostro-phic motion maintains in meridional direction, which can be called semi-geostrophic balance in barotropic model as well as semi-thermal-wind balance in baroclinic model. The vertical motion is determined both by the distribution of the initial vertical motion and that of the initial vertical motion tendency, but it is unrelated to the initial potential vorticity. Finally, the motion tends to be horizontal. The discussion of the physical mechanism of the semi-thermal-wind balance in low latitude atmosphere shows that the achievement of the semi-thermal-wind balance is due to the adjustment between the stream field and the temperature field through the horizontal convergence and divergence which is related to the vertical motion excited by the internal inertial gravity waves. The terminal adaptation state obtained shows that the adaptation direction between the mean temperature field and the shear flow field is determined by the ratio of the scale of the initial ageostrophic disturbance to the scale of one character scale related to the baroclinic Rossby radius of deformation. The shear stream field adapts to the mean temperature field when the ratio is greater than 1, and the mean temperature field adapts to the shear stream field when the ratio is smaller than 1.