共查询到18条相似文献，搜索用时 140 毫秒
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本文推导出柱坐标系下含有粘性摩擦项的正压方程组。选取2005年台风麦莎登陆浙江过程中的8月6日15时的WRF(Weather Research and Forecasting)模式输出资料,利用数值差分方法对该正压方程组求特征波解,分析粘性摩擦对台风麦莎内部正压特征波动的影响。结果表明,重力惯性外波在粘性摩擦的影响下,最不稳定波的波数为45左右,波动在摩擦的影响下衰减,波动沿逆时针传播,在半径1000 km处,1波波速为47.43 m/s,在半径r>800 km的范围内,径向风分量扰动加大,辐合辐散运动增强;而摩擦影响下的涡旋Rossby波,2波最不稳定,波动增长率减小,在半径r=200 km处波动相速度为4.282~29.172 m/s,扰动涡度大值区范围减小,涡旋Rossby波的波动区域沿着径向向台风中心收缩。分析包含所有波动时,考虑摩擦后,最不稳定波数在45左右且波动衰减,1波波速在r=1000 km处(外螺旋雨带)为26.374 m/s;在半径r=200 km(内螺旋雨带)为5.275 m/s,考虑径向基本气流后,最不稳定波的波数保持不变,半径r=1000 km处的波速增加为30.324 m/s,r=200 km(内螺旋雨带)处波速为6.065 m/s,摩擦使得径向风分量扰动明显增大,辐合辐散运动加强。 相似文献
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本文采用美国新一代非静力中尺度数值模式WRFV3．1．1版本对2006年8月14日的1次高原低涡过程进行了3重嵌套的数值模拟，分析模拟输出的高时空分辨率资料，发现涡度散度在各层次上均存在着正负值区域的相临交替分布，体现出一定的波动性，并随时间的变化而旋转，由此对高原低涡中的涡旋波的产生和发展进行详细分析，发现高原低涡中同时具有产生涡旋Rossby波与惯性重力波的条件，进一步粗略计算了涡旋波切向的移速介于涡旋Rossby波与惯性重力波的理论移速之间。由分析结果得出结论认为，在低涡中心区域，由于较高的涡度径向梯度，同时有较强的辐合辐散，波动表现出以涡旋Rossby波与惯性重力波混合的特性为主；低涡外围区域中涡度径向梯度大大减弱，失去了产生涡旋Rossby的条件，显现为惯性重力波的特性。同时高原低涡生命期相对较短，波动在圆周上的传播条件不均匀，这说明可能大多高原低涡螺旋形态的发展并不均匀或并不完整，较难形成如同海上热带气旋般比较均匀和完整的螺旋云带。另外，模拟也发现，在低涡成熟阶段，低涡呈现暖心结构，中心区域垂直运动较弱，表现为相对平静的眼区域。 相似文献
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基于WRF的高原低涡内波动特征及空心结构的初步研究 总被引：2，自引：0，他引：2
本文采用美国新一代非静力中尺度数值模式WRFV3.1.1版本对2006年8月14日的1次高原低涡过程进行了3重嵌套的数值模拟,分析模拟输出的高时空分辨率资料,发现涡度散度在各层次上均存在着正负值区域的相临交替分布,体现出一定的波动性,并随时间的变化而旋转,由此对高原低涡中的涡旋波的产生和发展进行详细分析,发现高原低涡中同时具有产生涡旋Rossby波与惯性重力波的条件,进一步粗略计算了涡旋波切向的移速介于涡旋Rossby波与惯性重力波的理论移速之间.由分析结果得出结论认为,在低涡中心区域,由于较高的涡度径向梯度,同时有较强的辐合辐散,波动表现出以涡旋Rossby波与惯性重力波混合的特性为主;低涡外围区域中涡度径向梯度大大减弱,失去了产生涡旋Rossby的条件,显现为惯性重力波的特性.同时高原低涡生命期相对较短,波动在圆周上的传播条件不均匀,这说明可能大多高原低涡螺旋形态的发展并不均匀或并不完整,较难形成如同海上热带气旋般比较均匀和完整的螺旋云带.另外,模拟也发现,在低涡成熟阶段,低涡呈现暖心结构,中心区域垂直运动较弱,表现为相对平静的眼区域. 相似文献
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利用多重尺度摄动法，推导出非线性涡旋Rossby波波包的演变方程是非线性Schroedinger方程。对该非线性Schroedinger方程的周期波动解及其稳定性进行了研究，得到了有关稳定和不稳定的判据。数值计算表明：非线性涡旋Rossby波的相速值为10^0m／s量级，这和台风中的螺旋雨带实测移速的量级是一致的，可以从涡旋Rossby波说中较好地解释台风中的螺旋雨带的形成和维持。 相似文献
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本文使用柱坐标系下的正压浅水方程组以及斜压扰动方程组,分析得出台风涡旋系统中的涡旋Rossby波划分为两种类型。由于切向基本气流的二阶径向水平切变或者基本气流的垂直涡度在径向方向的变化(β*因子)所导致的涡旋Rossby波称之为第一类涡旋Rossby波(正压涡旋Rossby波),它产生的根本原因是β*因子的作用。这种第一类涡旋Rossby波相对于切向基本气流是单向传播的,其传播方向则与β*因子的正负符号有关。当基本流场垂直涡度-ζz沿着径向r方向增大时,第一类涡旋Rossby波是沿着切向圆周方向逆时针方向传播的;反之则是沿着切向圆周方向顺时针方向传播。如果考虑切向基流的二次垂直切变时,可以得到台风涡旋系统中第二类涡旋Rossby波(斜压涡旋Rossby波)的相速度表达式,第二类涡旋Rossby波产生的物理根源是切向基本流场风速的二次垂直切变或者基本流场径向r方向的平均涡度在空间z方向上的不均匀性(亦即β**因子)。第二类涡旋Rossby波相对于切向基本气流也是单向传播的,当-ζr沿着空间z方向上增大时,第二类涡旋Rossby波就是相对于基本气流-V0是顺时针方向传播的;反之则是相对于基本气流逆时针方向传播。在基本流场的风速-V存在二次径向水平切变或者垂直切变时,台风中的波动可能是混合的涡旋Rossby波——重力波;而当基本流场的风速-V仅仅存在线性切变,不存在二次切变时,此时根本不存在涡旋Rossby波,台风系统中的波动则仅仅是重力惯性波。最后,采用WRF模式对“云娜”台风进行了数值模拟,验证了上述结论。 相似文献
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台风麦莎的正压特征波动结构及其稳定性 总被引：1，自引：1，他引：0
利用中尺度WRF模式对2005年8月西北太平洋台风麦莎（Matsa）进行了精细的数值模拟。使用模式输出资料,对正压浅水方程组进行了数值差分计算,分析它在最大强度时刻的正压特征波动结构和稳定性。结果表明,台风麦莎内部包含有沿逆时针方向传播的重力惯性外波和涡旋Ross-by波,两种波动的结构和稳定性存在显著性差异。前者主要存在于台风外围,增长率随波长的减小而增加,台风外围的波动相速度为48．9～68．5m／s;后者主要位于距离台风中心200km内,表现为3波最不稳定,半径100km处相速度约为5m／s。此外,重力惯性外波的扰动风场与高度场基本相垂直,扰动散涡比值大于3倍,甚至达到10＾3倍,运动以辐合、辐散为主;涡旋Rossby波的扰动风场基本平行于高度场,扰动散涡比值为10＾-1～10＾-2,涡旋运动是其主要运动,与内螺旋雨带沿着切向圆周方向的传播具有密切关系。 相似文献
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热带风暴中波动特征的研究进展和问题 总被引：9，自引：2，他引：9
在分析热带风暴眼壁和螺旋雨带中尺度波动特征最新研究的基础上，指出这些研究所忽略的问题，其中包括重力惯性波和涡旋Rossby波波解存在的前提条件和约束、理论分析与观测研究存在的差异等。提出一种基于准平衡动力条件下，热带风暴内中尺度扰动涡散运动共存时，区别于标准模混合的不可分的混合涡旋Rossby-重力惯性波，并讨论了位涡守恒条件下这一类不可分混合波的可能成波机制。利用高分辨率的模式大气资料，采用非对称波分量的分解方法分析了Bonnie飓风中的中尺度波动特征，结果表明，热带风暴中1波型扰动既具有涡旋波性质，但也存在散度扰动的变化，而2波型扰动则体现了明显的不可分混合波的特性。 相似文献
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《Dynamics of Atmospheres and Oceans》2002,35(2):153-177
A complete theory of the linear initial-value problem for Rossby waves on a class of smooth circular vortices in both f-plane and polar-region geometries is presented in the limit of small and large Rossby deformation radius. Although restricted to the interior region of barotropically stable circular vortices possessing a single extrema in tangential wind, the theory covers all azimuthal wavenumbers. The non-dimensional evolution equation for perturbation potential vorticity is shown to depend on only one parameter, G, involving the azimuthal wavenumber, the basic state radial potential vorticity gradient, the interior deformation radius, and the interior Rossby number.In Hankel transform space the problem admits a Schrödinger’s equation formulation which permits a qualitative and quantitative discussion of the interaction between vortex Rossby wave disturbances and the mean vortex. New conservation laws are developed which give exact time-evolving bounds for disturbance kinetic energy. Using results from the theory of Lie groups a nontrivial separation of variables can be achieved to obtain an exact solution for asymmetric balanced disturbances covering a wide range of geophysical vortex applications including tropical cyclone, polar vortex, and cyclone/anticyclone interiors in barotropic dynamics. The expansion for square summable potential vorticity comprises a discrete basis of radially propagating sheared vortex Rossby wave packets with nontrivial transient behavior. The solution representation is new, and for this class of swirling flows gives deeper physical insight into the dynamics of perturbed vortex interiors than the more traditional approach of Laplace transform or continuous-spectrum normal-mode representations. In general, initial disturbances are shown to excite two regions of wave activity. At the extrema of these barotropically stable vortices and for a certain range of wavenumbers, the Rossby wave dynamics are shown to become nonlinear for all initial conditions. Extensions of the theory are proposed. 相似文献
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热带气旋内中尺度波动的不稳定机理研究进展 总被引：1，自引：0，他引：1
在回顾了近年来热带气旋波动动力学研究的基础上,介绍了热带气旋内中尺度波动不稳定机理研究方面的进展,分别对热带气旋三类中尺度特征波动的不稳定,即经典重力惯性波、涡旋Rossby波和具有物理性质不可分的混合波的不稳定进行了物理分析,给出了热带气旋内对称不稳定、横波不稳定、对流对称不稳定、涡旋Rossby波正压不稳定及混合波不稳定的动力解释,进一步说明热带气旋内中尺度扰动发展是与基本气流的动力(水平和垂直切变)及热力状态之间的相互作用密切相关。 相似文献
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Summary It is shown that there exists a mechanism that can cause north-northwest movement of tropical cyclones in addition to already recognised mechanisms such as steering current and beta drift. This mechanism depends on the interaction between organised convection and dynamics. In the initial stages of formation of a cyclone, it is assumed that the hydrodynamic instabilities result in an incipient disturbance that organises some convection giving rise to a heat source. The atmospheric response to a localized heat source located off the equator in the northern hemisphere produces a low level vorticity field with a maximum in the northwest sector of the original heat source. If the Ekman-CISK which depends on the low level vorticity, was the dominating mechanism for moisture convergence, the location of the heat source would move to the new location of vorticity maximum. A repetition of this process would result in a northwest movement of the heat source and hence that of the cyclone. The movement of a tropical vortex under the influence of this mechanism which depends on asymmetries created by linear dispersion of Rossby waves is first illustrated using a linear model. It is then demonstrated that this process also enhances the motion of a tropical vortex in a nonlinear model. Importance of this feedback and the resulting movements of a tropical vortex in determining the actual track of a cyclone and in bogusing an initial vortex for prediction models are illustrated.With 6 Figures 相似文献
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In this study, the barotropic stability of vortex Rossby waves (VRWs) in 2D inviscid tropical cyclone (TC)-like vortices is explored in the context of rotational dynamics on an f-plane. Two necessary instable conditions are discovered: (a) there must be at least one zero point of basic vorticity gradient in the radial scope; and (b) the relative propagation velocity of perturbations must be negative to the basic vorticity gradient, which reflects the restriction relationship of instable energy. The maximum ... 相似文献
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Interaction of typhoon and mesoscale vortex 总被引：15，自引：1，他引：14
Under two types of initial tropical cyclone structures that are characterized by high and low vorticity zones, four sets of numerical experiments have been performed to investigate the interaction of a tropical cyclone with an adjacent mesoscale vortex (MSV) and its impact on the tropical cyclone intensity change,using a quasi-geostrophic barotropic vorticity equation model with a horizontal resolution of 0.5 km. The results suggest that the interaction of a tropical cyclone characterized by a high vorticity zonal structure and an MSV would result in an intensification of the cyclone. Its central pressure decreases by more than 14 hPa. In the process of tile interaction, the west and middle segments of the high vorticity zone evolve into two peripheral spiral bands of the tropical cyclone, and the merging of the east segment and the inward propagating MSV forms a new vorticity accumulation area, wherein the maximum vorticity is remarkably greater than that in the center of the initial tropical cyclone circulation. It is this process of merging and strengthening that causes a greater pressure decrease in the center of the tropical cyclone. This process is also more complicated than those that have been studied in the past, which indicated that only the inward transfer of vorticity of the MSV can result in the strengthening of the tropical cyclone. 相似文献
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Typhoon Rananim (2004) was one of the severest typhoons landfalling the Chinese mainland
from 1996 to 2004. It brought serious damage and induced prodigious economical loss. Using a new
generation of mesoscale model, named the Weather Research and Forecasting (WRF) modeling system,
with 1.667 km grid horizontal spacing on the finest nested mesh, Rananim was successfully simulated
in terms of track, intensity, eye, eyewall, and spiral rainbands. We compared the structures of
Rananim to those of hurricanes in previous studies and observations to assess the validity of
simulation. The three-dimensional (3D) dynamic and thermal structures of eye and eyewall were
studied based on the simulated results. The focus was investigation of the characteristics of
the vortex Rossby waves in the inner-core region. We found that the Rossby vortex waves propagate
azimuthally upwind against the azimuthal mean tangential flow around the eyewall, and their
period was longer than that of an air parcel moving within the azimuthal mean tangential flow.
They also propagated outward against the boundary layer inflow of the azimuthal mean vortex.
Futhermore, we studied the connection between the spiral potential vorticity (PV) bands and
spiral rainbands, and found that the vortex Rossby waves played an important role in the
formation process of spiral rainbands. 相似文献
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台风“海棠”的螺旋雨带结构及特征 总被引：5，自引：0，他引：5
利用中尺度数值模式WRF对2005年7月19—20日台风＂海棠＂登陆前后螺旋雨带的结构及特征进行了模拟和诊断分析。结果表明,本次台风造成的沿海暴雨与主次两条雨带活动有关。主雨带是涡旋Rossby波激发的螺旋雨带,与850 hPa正涡度带有很好的对应关系,降水强度大,辐合层次低,处在温度和切向风速梯度最大处。次雨带辐合层次相对较高,最大温度梯度和相当位温梯度发生在700 hPa以上,无明显切向风梯度配合,其发展主要与台风中心附近的阶梯状相当位温锋区有关。当台风中雨带合并时,易造成降水增幅。台风登陆前后存在螺旋雨带的断裂现象,台风中心西侧及西北侧的中低层的辐散流场使高层的气旋性流场出现和加强,台风在高层的气旋性环流与西部低压结合,使台风西部产生辐合,引起螺旋雨带的断裂,当高层的低压形成明显的气旋式切变时,也可使切变下方螺旋雨带断裂。 相似文献
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The evolution of spiral-band-like structures triggered by asymmetric heating in three tropical-cyclone-like vortices of different intensities is examined using the Three-Dimensional Vortex Perturbation Analyzer and Simulator （3DVPAS） model. To simulate the spiral bands, asymmetric thermal perturbations are imposed on the radius of maximum wind （RMW） of vortices, which can be considered as the location near the eyewall of real tropical cyclones （TCs）. All the three vortices experience a hydrostatic adjustment after the introduction of thermal asymmetries. It takes more time for weaker and stable vortices to finish such a process. The spiral-band-like structures, especially those distant from the vortex centers, form and evolve accompanying this process. In the quasi-balance state, the spiral bands are gradually concentrated to the inner core, the wave behavior of which resembles the features of classic vortex Rossby （VR） waves. The unstable vortices regain nonhydrostatic features after the quasi-balance stage. The spiral bands further from the vortex center, similar to distant spiral bands in real TCs, form and maintain more easily in the moderate basic-state vortex, satisfying the conditions of barotropic instability. The widest radial extent and longest-lived distant bands always exist in weak and stable vortices. This study represents an attempt to determine the role of TC intensity and stability in the formation and evolution of spiral bands via hydrostatic balance adjustment, and provides some valuable insights into the formation of distant spiral rainbands. 相似文献