共查询到18条相似文献，搜索用时 140 毫秒
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爆发性气旋的合成诊断及形成机制研究 总被引：5，自引：1，他引：5
该文对发生在太平洋和大西洋的16个爆发性气旋作了合成分折, 对强弱爆发性气旋作了对比及诊断.研究发现, 基本场上存在不少明显的差异.分析得出, 强爆发性气旋的形成与高空急流的非纬向性以及反气旋性弯曲密切相关.非纬向高空急流为爆发性气旋提供了强的辐散、斜压性、斜压不稳定场.高层强爆发性气旋前部的反气旋曲率易造成重力惯性波在能量北传时发展, 促使气旋快速加深.暖平流及非绝热加热可使反气旋曲率加强.一般情况下, 当气旋西部位涡的大值区与北部位涡的大值区叠加下沉时, 有利于气旋爆发性发展. 相似文献
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远距离台风暴雨过程的正/斜压不稳定 总被引：15，自引：2，他引：15
利用正／斜压联合不稳定计算方法，分析了由9711号台风引起的远距离台风暴雨(实况及MM4模拟结果)过程中不同时段、不同位置的正／斜压项。结果表明：台风暴雨初始时段的降水主要由台风系统本身正压不稳定扰动引起，随着台风与西风带系统的结合，其南北部出现了2个雨区，均是正／斜压联合不稳定的产物；北部雨区的斜压不稳定较明显，且有随高空急流的非纬向性增强而增强的趋势。 相似文献
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球面斜压大气中上传行星波与纬向平均气流的相互作用 总被引：8，自引：3，他引：8
本文指出在球面斜压大气中的行星尺度扰动与纬向平均气流相互作用中必须考虑非地转风分量对位涡度南北方向输送的作用,从而证明了球面大气中行星尺度运动的波作用守恒,并求得球面大气中的行星尺度扰动与纬向平均气流相互作用的欧拉平均运动方程组。 本义利用1979年2月的实际天气观测资料分析了北半球一次对流层阻塞形势建立与平流层爆发性增温过程的行星波与纬向平均气流的相互作用。从分析结果可以看到:由于行星波向上传播,使得在高纬度对流层中、上层出现行星波的波作用通量(也称E-P通量)辐合,使得西风气流减速,因而在高纬度对流层中、上层形成阻塞形势。并且,随着行星波的继续向上传播,使得平流层下、中层的基本气流相继减速并出现东风,因而在平流层下、中层出现爆发性增温。然而,由于高纬度对流层低层出现东风,行星波不能往上传播,在上层波的E-P通量矢量变成辐散,气流由东风又变成西风。 相似文献
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本文研究了在各种定常基本状态下大气对位于热带及中纬度地区的定常强迫源的响应。进一步证实了东风基本气流将限制热带扰动向中高纬度的传播,从而也抑制了两半球的相互作用;西风基本气流则有利于热带波动向中纬度传播,有利于中纬度扰动通过热带向另一半球传播。赤道地区基本气流随经度的变化对罗斯贝波的传播也有重大影响,波动能量将在基本气流辐合的地区累积并向中纬度发射。因此赤道西风辐合最大的地区就是热带与中纬度相互作用以及两半球相互作用最明显的地区。应用实测风场作基本气流所进行的实验表明,冬季与夏季热带波动的传播特征,两半球相互作用的状况均有明显差异。 相似文献
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基本流场切变对赤道长Rossby波的影响 总被引：9，自引：2，他引：9
文中应用赤道β平面近似 ,建立一个简单的斜压大气半地转模式 ,在热力学方程中引入表征基本位温场 (θ)经向分布特征的无量纲参数 σ,对线性化的扰动方程进行了频率分析 ,研究基本位温场经向非均匀分布以及基本气流垂直切变对赤道纬向超长尺度 Rossby波动的影响 ,并指出仅考虑基本气流垂直切变或者基本位温场变化的作用是不合适的。定性分析结果表明 :基本位温场经向温差必然有基本气流垂直切变与其相匹配 ,而基本气流垂直切变将导致赤道长 Rossby波动不稳定并影响其纬向传播速度 相似文献
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非纬向基流的非线性斜压不稳定 总被引：2，自引：1，他引：2
本文从含Ekman摩擦的非线性两层斜压模式出发,应用Serrin-Joseph的能量方法,按变分原理,分别用扰动总能量、总位涡拟能和两者的线性组合导得了非纬向基流的非线性斜压稳定性判据。并和线性判据作了比较。 相似文献
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本文利用线性化的能量方程和交叉谱方法分别研究了准两周振荡和准40天振荡的能量来源及其转换过程。发现:在热带对流层中,对于低频振荡过程来说,来自中高纬度的侧向强迫作用和水汽凝结的加热作用是非常重要的,为扰动的产生和维持提供了重要能源。而正、斜压不稳定作用对扰动发展的作用是极小的。并且指出,在东亚热带对流层上部,准两周振荡通过与平均气流的相互作用为基本气流提供许多能量,对于维持这里的高空东风急流有重要作用。准40天振荡向平流层输送能量,对平流层平均环流的演变可能有重要贡献。 相似文献
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斜压不稳定理论是中高纬度地区天气尺度扰动生成和发展的机制,是继长波理论之后大气动力学上的又一重大进展,对现代天气预报具有重要的指导意义。按照斜压不稳定理论发展的时间脉络,阐述了赵九章、查尼和伊迪在斜压不稳定方面开展的研究工作,分析了3位科学家各自的研究特点及历史贡献。赵九章1946年发表在《Journal of Meteorology》上的论文,最早提出了"斜压不稳定"这一概念,给出了不稳定的临界波长,并阐述了在不稳定扰动情况下能量的转换,以及不稳定波对大气环流带来的可能影响,尽管得出的不稳定临界波长与观测差别较大,但其对波-流相互作用的讨论在当时是超前的。查尼于1947年采用滤波和尺度分析等方法,将大气扰动方程简化为一个可以求解的系统,推导出大气稳定状态的判据,建立了斜压不稳定理论,其结果与实况比较接近;并据此把准地转模式成功应用于数值天气预报实践中,促使数值天气预报获得首次成功。1949年,伊迪在查尼研究工作的基础上通过合理的简化方法,得到了更为简洁的模型。最后,通过对比他们的研究思路,重点分析了赵九章未能使得斜压不稳定理论提前一年建立的原因:由于其研究思路始终局限在大气水平运动上,忽略了斜压系统发展中散度项的贡献,因而未能抓住天气系统发生、发展的本质,致使其最终与斜压不稳定理论的成功建立失之交臂,其论文本身存在的一些亮点也因此被后人忽视。 相似文献
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Variational principle of instability of atmospheric motions 总被引：2，自引：0，他引：2
Zeng Qingcun 《大气科学进展》1989,6(2):137-172
Problems of instability of rotating atmospheric motions are investigated by using nonlinear governing equations and the variational principle. The method suggested in this paper is universal for obtaining criteria of instability in all models with all possible basic flows. For example, the model can be barotropic or baroclinic, layer or continuous, quasi-geostrophic or primitive equations; the basic flow can be zonal or nonzonal, steady or unsteady.Although the basic flows possess a great deal of variety, they all are the stationary points in the functional space determined by an appropriate invariant functional. The basic flow is an unsteady one if the conservation of angular momentum is included in the associated functional.The second variation, linear or nonlinear, gives the criteria of instability. Especially, the general criteria of instability for unsteady basic flow, orographically disturbed flow as well as nongeostrophic flow are first obtained by the method described in this paper.It is also shown that the difference between the criteria of instability obtained by the linear theory and our variational principle clearly indicates the importance of using nonlinear governing equations.In the appendix the theory is extended to cases such as in a β-plane where the fluid does not possess finite total energy, hence the variational principle can not be directly applied. However, a generalized Liapounoff norm can still be obtained on the basis of variational consideration. 相似文献
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The linear baroclinic instabilities of a basic geostrophic shear flow in a stratified, thermally active ocean are considered, including the β-effect. It is shown that the internal heat production, even if it introduces only minor changes into the geostrophic balance, may deeply modify the stability properties of the stationary solutions. If density, geostrophic basic flow, and heat production are all regarded as arbitrary functions of depth only, and if a linear nonzonal assumption is made about the geostrophic pressure field, it can be shown how the geostrophic equilibrium is altered and how the internal heating affects both the directions of propagation and the growth rates of quasi-geostrophic disturbances. A semicircle theorem valid for every direction of propagation is proved, by generalizing well-known results obtained for adiabatic geostrophic flows.Finally, it is found that the modified instability can be described adequately by a directional Richardson number related to the perturbed stationary geostrophic flow. 相似文献
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The linear two-layer barotropic primitive equations in cylindrical coordinates are used to derive a gen- eralized energy equation, which is subsequently applied to explain the instability of the spiral wave in the model. In the two-layer model, there are not only the generalized barotropic instability and the super high- speed instability, but also some other new instabilities, which fall into the range of the Kelvin-Helmholtz instability and the generalized baroclinic instability, when the upper and lower basic flows are different. They are perhaps the mechanisms of the generation of spiral cloud bands in tropical cyclones as well. 相似文献
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The effect of barotropic shear in the basic flow on baroclinic instability is investigated using a linear multilevel quasi-geostrophic β-plane channel model and a nonlinear spherical primitive equation model. Barotropic shear has a profound effect on baroclinic instability. It reduces the growth rates of normal modes by severely restricting their structure, confirming earlier results with a two-layer model. Dissipation, in the form of Ekman pumping and Newtonian cooling, does not change the main characteristics of the effect of the shear on normal mode instability.Barotropic shear in the basic state, characterized by large shear vorticity with small horizontal curvature, also effects the nonlinear development of baroclinic waves. The shear limits the energy conversion from the zonal available potential energy to eddy energy, reducing the maximum eddy kinetic energy level reached by baroclinic waves. Barotropic shear, which controls the level of eddy activity, is a major factor which should be considered when parameterizing the eddy temperature and momentum fluxes induced by baroclinic waves in a climate model. 相似文献
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A conservation law for the Phillips model is derived. Using this law, the nonlinear saturation of purely baroclinic instability caused by the vertical velocity shear of the basic flow in the Phillips model-the case of energy-is studied within the context of Arnold's second stability theorem. Analytic upper bounds on the energy of wavy disturbances are obtained. For one unstable region in the parameter plane, the result here is a second-order correction in ε to Shepherd's; For another unstable region, the analytic upper bound on the energy of wavy disturbances offers an effective constraint on wavy (nonzonal) disturbances φ'i at any time. 相似文献
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《Dynamics of Atmospheres and Oceans》1999,30(1):1-24
A linear quasi-geostrophic model and a non-linear balanced model are used to study the properties of the oceanic baroclinic waves. From a linear point of view, the oceanic meso-scale (200–400 km) disturbances found near the Brazil and Falkland currents confluence zone seem to be generated by baroclinic instability. Non-geostrophic and non-linear effects due to a single original wave are superimposed on the linear fields associated with the most unstable wave. Characteristics very similar to observations are obtained in the evolution to finite amplitude. The evolution of oceanic thermal rings is very well reproduced by the non-linear model. However, the stage of saturation is not reached in the model results since the feedback to the thermal basic state is not included. 相似文献
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非平直基流中尺度扰动的对称发展 总被引：6，自引：0，他引：6
用ｆ平面非静力平衡滤声波模式，在自然坐标系下，运用ＷＫＢＪ方法及能量方法研究了非平直基流对中尺度扰动波包发展问题。结果表明：中尺度波包对称发展主要取决于扰动波结构与背景结构之间的匹配。 相似文献