共查询到20条相似文献，搜索用时 15 毫秒
1.
台风云娜（2004）的高分辨率数值模拟研究:眼壁小尺度对流运动 总被引：2，自引：0，他引：2
通过对2004年云娜台风高分辨率模拟结果的分析,发现在环境垂直风切变不是单一方向情况下,中尺度涡旋只在对流层低层的眼壁区域形成.这些涡旋中有的伴随气旋环流是闭合的,有的则为非闭合;并且有的伴随着小尺度对流上升运动,而有的则没有.进一步分析发现当环境入流与涡旋的出流相遇产生辐合时,或者入流受涡旋本身阻挡产生辐合时,小尺度对流上升运动随即发生.中尺度涡旋伴随着对流上升活动在眼壁中沿气旋方向移动,表现出涡旋Rossby波特征,当移动至垂直风切变矢量下风向时对流加强,加强的上升气流通过拉伸涡管使得相麻的涡旋环流也加强,通常对流在移向垂直风切变矢量上风向时逐渐减弱.反观在眼壁区域的对流层中上层,没有明显的中尺度涡旋活动,强对流活动主要集中在眼壁东南侧,并且强上升运动也呈现小尺度特征.眼壁区域中速度大于1 m/s的上升运动仪占14%,大于2 m/s的则小于7%,但速度超过1 m/s的向上的质量通量约占整个上升运动的30%,表明尽管这些小尺度强对流运动所占空间比例较小,却在眼壁质量输送中起着重要作用.另外,这些强上升运动核表现出正的浮力特征,大值浮力分布与上升运动核位置一致的特征也进一步说明眼壁中大量的垂直质量通量输送与只占很小范围的小尺度上升运动有关. 相似文献
2.
热带气旋眼墙非对称结构的研究综述 总被引：2，自引：0，他引：2
热带气旋的眼墙非对称结构与其发展过程密切相关。在热带气旋移动过程中,非对称风场伴随着边界层内非对称摩擦而引起的辐合,影响着热带气旋眼墙内的对流分布。此外,风垂直切变作为影响热带气旋强度的重要因子,将上层暖心吹离表层环流,引起眼墙垂直运动的非对称,导致云、降水在方位角方向的非均匀分布。当存在平均涡度的径向梯度时,罗斯贝类型的波动可以存在于涡旋内核区域,影响眼墙非对称结构。海洋为热带气旋提供潜热和感热形式的能量,是热带气旋发展的重要能量来源,关于海洋如何影响热带气旋眼墙非对称结构的相关研究较少。文中着重回顾了热带气旋与海洋相互作用的研究成果,并提出海洋影响热带气旋眼墙非对称结构的机制。海洋对热带气旋最显著的响应特征是冷尾效应,该效应通过降低海表温度,减少海洋向大气输送的潜热和感热,从而影响热带气旋眼墙非对称结构。此外,海浪改变海表粗糙度,通过边界层影响移动热带气旋的眼墙结构。 相似文献
3.
Summary Current understanding of tropical cyclone (TC) structure and intensity changes has been reviewed in this article. Recent studies in this area tend to focus on two issues: (1) what factors determine the maximum potential intensity (MPI) that a TC can achieve given the thermodynamic state of the atmosphere and the ocean? and (2) what factors prevent the TCs from reaching their MPIs? Although the MPI theories appear mature, recent studies of the so-called superintensity pose a potential challenge. It is notable that the maximum intensities reached by real TCs in all ocean basins are generally lower than those inferred from the theoretical MPI, indicating that internal dynamics and external forcing from environmental flow prohibit the TC intensification most and limit the TC intensity. It remains to be seen whether such factors can be included in improved MPI approaches.Among many limiting factors, the unfavorable environmental conditions, especially the vertical shear-induced asymmetry in the inner core region and the cooling of sea surface due to the oceanic upwelling under the eyewall region, have been postulated as the primary impediment to a TC reaching its MPI. However, recent studies show that the mesoscale processes, which create asymmetries in the TC core region, play key roles in TC structure and intensity changes. These include the inner and outer spiral rainbands, convectively coupled vortex Rossby waves, eyewall cycles, and embedded mesovortices in TC circulation. It is also through these inner core processes that the external environmental flow affects the TC structure and intensity changes. It is proposed that future research be focused on improving the understanding of how the eyewall processes respond to all external forcing and affect the TC structure and intensity changes. Rapid TC intensity changes (both strengthening and weakening) are believed to involve complex interactions between different scales and to be worthy of future research.The boundary-layer processes are crucial to TC formation, maintenance, and decaying. Significant progress has been made to deduce the drag coefficient on high wind conditions from the measurements of boundary layer winds in the vicinity of hurricane eyewalls by Global Positioning System (GPS) dropsondes. This breakthrough can lead to reduction of the uncertainties in the calculation of surface fluxes, thus improving TC intensity forecast by numerical weather prediction models. 相似文献
4.
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
5.
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
6.
Strong vertical motion(10 m s~(-1)) has profound implications for tropical cyclone(TC) structure changes and intensity. While extreme updrafts in the TC are occasionally observed in real TCs, the associated small-scale features remain unclear. Based on an analysis of the extreme eyewall updrafts in two numerical experiments conducted with the Advanced Research version of the Weather Research and Forecasting(WRF) model, in which the large-eddy simulation(LES) technique was used with the finest grid spacings of 37 and 111 m, for the first time this study demonstrates that the simulated extreme updrafts that occur mainly in the enhanced eyewall convection on the down-shear left side are comparable to available observations. The simulated extreme updraft exhibits relatively high frequencies in the lower(750 m), middle(6.5 km) and upper(13 km) troposphere, which are associated with different types of small-scale structures.While the lower-level extreme updraft is mainly related to the tornado-scale vortex, the extreme updraft at upper levels is closely associated with a pair of counter-rotating horizontal rolls oriented generally along the TC tangential flow, which are closely associated with the enhanced eyewall convection. The extreme updraft at middle levels is related to relatively complicated small-scale structures. The study suggests that extreme updrafts can be simulated when the grid spacing is about 100 m or less in the WRF-LES framework, although the simulated small-scale features need further verification in both observation and simulation. 相似文献
7.
Three Types of Tropical Waves Related to Tropical Cyclogenesis over the Western North Pacific 
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下载免费PDF全文 CHEN Guang-Hua 《大气和海洋科学快报》2009,2(6):321-326
The present study applies a space-time filter to identify three dominant types of tropical waves： Madden-Julian oscillations （MJOs）, equatorial Rossby （ER） waves, and tropical depression （TD）-type disturbances. The impacts of these waves on tropical cyclones （TCs） were investigated based on 131 observations during the period 2000-07. The results suggest that 72% of TC geneses were related to the joint impacts of more than one type of wave. The composites for cases in different categories reveal that TCs related to the concurrence of the three types of waves have strong and large initial vortices at the time of TC genesis. In the absence of the MJO, ER- and TD-related TC genesis, embedded in easterly flow, exhibits a relatively fast initiation process and gives rise to a relatively small scale vortex. In contrast, without the ER wave contribution, TCs associated with ER and TD waves did not require strong convection at the time of genesis because an initial vortex can rapidly develop in the MJO active phase through persistent energy transfer. The MJO-related TC geneses were scattered in geographic distribution, as opposed to the clustered and eastward shift observed for genesis cases without contributions from MJOs. 相似文献
8.
The effect of equatorially trapped waves on the movement of tropical cyclones (TC) is studied numerically based on a two-dimensional barotropic model in a beta-plane approximation. According to recent studies, equatorially trapped waves contribute to the genesis of TCs. It is thus natural to assume that these waves affect also the movement of the TC. The effect of three types of equatorially trapped waves, namely Kelvin, Rossby, and n = 0 eastward inertio-Gravity (EIG) waves, on the TC trajectory is investigated with a focus on the sensitivity on some key physical parameters such as the wavenumber and wavespeed. Using a simple barotropic model forced by a prescribed baroclinic flow, the barotropic response to equatorially trapped waves is simulated for a period of 50 days, under various wave parameter configurations. This response is then used as a background flow where TC’s can evolve and propagate. TC-like flows are injected into this wavefield background at arbitrary times during the simulation, and the TC trajectories are tracked and recorded for 48h after the injection time. The resulting TC trajectory patterns with respect to the injection times and wave parameters appear to be stochastic and the mean paths and the associated standard deviations are calculated and reported here. The statistics are different for different wave types. Kelvin waves make shorter length of TC trajectories and small divergence of direction. On the contrary, Rossby waves cause rather dramatic changes in the TC path and yield longer trajectories. Meanwhile, TCs in EIG waves maintain fairly the same direction and typically have longer trajectories though less dramatic. A robustness test using a random forcing instead has also been conducted.
相似文献9.
Initial mesoscale vortex effects on the tropical cyclone(TC) motion in a system where three components coexist(i.e.,an environmental vortex(EV),a TC,and mesoscale vortices) were examined using a barotropic vorticity equation model with initial fields where mesoscale vortices were generated stochastically.Results of these simulations indicate that the deflection of the TC track derived from the initial mesoscale vortices was clearly smaller than that from the beta effect in 60% of the cases.However,they may have a more significant impact on the TC track under the following circumstances.First,the interaction between an adjacent mesoscale vortex and the TC causes the emergence of a complicated structure with two centers in the TC inner region.This configuration may last for 8 h,and the two centers undergo a cyclonic rotation to make the change in direction of the TC motion.Second,two mesoscale vortices located in the EV circulation may merge,and the merged vortex shifts into the EV inner region,intensifying both the EV and steering flow for the TC,increasing speed of the TC. 相似文献
10.
Guanghua Chen 《大气科学进展》2016,33(8):945-954
The sensitivity of TC intensification and track to the initial inner-core structure on a β plane is investigated using a numerical model. The results show that the vortex with large inner-core winds(CVEX-EXP) experiences an earlier intensification than that with small inner-core winds(CCAVE-EXP), but they have nearly the same intensification rate after spin-up. In the early stage, the convective cells associated with surface heat flux are mainly confined within the inner-core region in CVEXEXP, whereas the vortex in CCAVE-EXP exhibits a considerably asymmetric structure with most of the convective vortices being initiated to the northeast in the outer-core region due to the β effect. The large inner-core inertial stability in CVEX-EXP can prompt a high efficiency in the conversion from convective heating to kinetic energy. In addition, much stronger straining deformation and PBL imbalance in the inner-core region outside the primary eyewall ensue during the initial development stage in CVEX-EXP than in CCAVE-EXP, which is conducive to the rapid axisymmetrization and early intensification in CVEX-EXP. The TC track in CVEX-EXP sustains a northwestward displacement throughout the integration, whereas the TC in CCAVE-EXP undergoes a northeastward recurvature when the asymmetric structure is dominant. Due to the enhanced asymmetric convection to the northeast of the TC center in CCAVE-EXP, a pair of secondary gyres embedded within the large-scale primary β gyres forms, which modulates the ventilation flow and thus steers the TC to move northeastward. 相似文献
11.
12.
Simulation of the Electrification of a Tropical Cyclone Using the WRF-ARW Model：An Idealized Case 总被引：2，自引：1，他引：1 下载免费PDF全文
下载免费PDF全文 Evolution of the electrifi cation of an idealized tropical cyclone （TC） is simulated by using the Advanced Weather Research and Forecasting （WRF-ARW） model. The model was modifi ed by addition of explicit electrifi cation and a new bulk discharge scheme. The characteristics of TC lightning is further examined by analyses of the electrifi cation and the charge structure of the TC. The fi ndings thus obtained are able to unify most of the previous inconsisitent observational and simulation studies. The results indicate that the TC eyewall generally exhibits an inverted dipole charge structure with negative charge above the positive. In the intensifi cation stage, however, the extremely tall towers of the eyewall may exhibit a normal tripole structure with a main negative region between two regions of positive charge. The outer spiral rainband cells display a simple normal dipole structure during all the stages. It is further found that the diff erences in the charge structure are associated with diff erent updrafts and particle distributions. Weak updrafts, together with a coexistence region of diff erent particles at lower levels in the eyewall, result in charging processes that occur mainly in the positive graupel charging zone （PGCZ）. In the intensifi cation stage, the occurrence of charging processes in both positive and negative graupel charging zones is associated with strong updraft in the extremely tall towers. In addition, the coexistence region of graupel and ice crystals is mainly situated at upper levels in the outer rainband, so the charging processes mainly occur in the negative graupel charging zone （NGCZ）. 相似文献
13.
利用TMI反演的水汽凝结物对热带气旋潜热结构分布的探索研究 总被引：3，自引：0，他引：3
本文利用热带测雨卫星TRMM（Tropical Rainfall Measuring Mission）微波成像仪TMI（TRMM Microwave Imager）2A12 水汽凝结物（Hydrometeor）反演资料,对西北太平洋地区从1998～2009 年的236 个热带气旋个例的1776 个“快照”（snapshot）的水汽凝结物的结构特征进行了分析,并探讨了水汽凝结物的时空变化与热带气旋强度演变联系。研究结果表明:（1）TMI 2A12 水汽凝结物资料显示出了热带气旋内部的细致结构及变化特征,水汽凝结物的峰值集中于数十公里到一百多公里的热带气旋眼壁及云墙区;在热带气旋发展过程中,随着热带气旋强度的增强,水汽凝结物增多且往其中心靠拢,从发展阶段到成熟阶段,水汽凝结物的大值中心基本上集中在距离热带气旋中心约50 km 区域,而且强度越强的热带气旋,水汽凝结物的大值中心与热带气旋中心的距离越近;在热带气旋消亡的过程中,水汽凝结物不断减弱且往外围扩散,逐渐扩展到远离中心的区域;（2）热带气旋强度与水汽凝结物的分布关系密切,热带气旋强度变化与热带气旋中心附近200 km 范围内的水汽凝结物含量存在显著的正相关,而200 km 以外的外围水汽凝结物含量存在负相关;（3）热带气旋强度变化与水汽凝结物的变化存在时间差,水汽凝结物的变化超前于热带气旋强度的变化,在热带气旋迅速发展之前数小时,热带气旋中心0～50 km 环状区域的水汽凝结物含量就已经提前增加了,在热带气旋减弱前数小时到十数小时,即使热带气旋还处于它强度的鼎盛时期,其中心0～50 km 环状区域的水汽凝结物含量就已经提前显著减少了,这种水汽凝结物的变化超前于热带气旋强度的变化的现象,可能是热带气旋强度预报的潜在线索。 相似文献
14.
Based on high-fidelity numerical simulation by using the Weather Research and Forecast (WRF) model, we analyzed the formation and replacement mechanism of the concentric eyewall of Super Typhoon Muifa (1109) from the aspects of the potential vorticity (PV), dynamic/ thermodynamic structure change, sea surface flux, and water vapor content. Observational data and sensitivity tests were also adopted to verify the results. We found that: (1) The abnormal increase of the PV in the rain zone is mainly due to the condensation latent heat. Sufficient water vapor conditions are beneficial to the formation of the outer eyewall structure, and when the environmental water vapor content is larger, the intensity of the outer eyewall becomes greater. (2) After the formation of the typhoon’s outer eyewall, in the area where the outer eyewall is located, the increase of inertial stability contributes to the decrease of the intensity of the inner eyewall. When the intensity of the outer eyewall is larger, the divergence and subsidence motion in the upper layer of the outer eyewall has a greater weakening effect on the intensity of the inner eyewall. (3) The increase of potential temperature of the outer eyewall is mainly due to the condensation latent heat release and the warming of dry air subsidence motion in the moat area. (4) The increase of sea surface heat flux can prolong the concentric eyewall replacement process. 相似文献
15.
2003年淮河大水期间亚洲北部阻塞高压的形成特征 总被引：3，自引：2，他引：1
利用观测资料和NCEP再分析资料分析2003年淮河大水期间亚洲北部阻塞高压的形成维持机制, 结果表明, 2003年淮河梅汛期亚洲中高纬地区阻塞高压的异常活动中, 波流作用十分显著。6月上旬, 阻高建立前期和维持过程中, 上游地区天气尺度波动活跃, 欧洲斜压区不断有瞬变动能生成, 并在阻塞区向阻高平均流转化。从瞬变涡动的作用来看, 上游传播而来的瞬变波不断将较低纬度的低位涡空气向阻塞区输送, 有利于阻塞高压的建立维持; 平均流则使位涡呈相反形势发展, 引导阻塞高压向东频散, 削弱了扰动位涡输送的作用, 对阻高的维持起到耗散作用。阻高建立前, 瞬变涡位涡输送作用强于平均流位涡平流, 造成阻塞区位涡降低, 有利于阻高生成; 阻高维持期间, 瞬变涡位涡输送与平均流位涡平流输送量相当; 6月25～30日, 阻塞高压明显西退, 该阶段瞬变涡动明显强于平均耗散作用, 引导低位涡场向西移动。研究表明, 大气内部的波波作用对阻高的建立维持也十分重要。1波与5波在一定范围内的共同作用可能是阻高建立维持的决定因素, 而天气尺度波动扰动则对阻塞高压的建立、 维持和崩溃起到重要的作用。波波作用表明, 2003年6月份阻塞高压建立、 维持时, 尺度较长的波一般从平均动能得到扰动动能的转化, 尤其5波, 斜压能的转换不但是其能量的来源, 同时非线性作用也使得尺度更小或更长的波向其提供能量; 阻高衰退时, 5波则通过非线性作用向其他波动输送能量, 同时也存在斜压耗散, 能量逐渐失去。 相似文献
16.
In this study, we first show that tropical cyclone (TC) Usagi evolved from a mid-level vortex over the South China Sea (SCS) in August 2001. The initial disturbance of TC Usagi had a maximum potential vorticity (PV) near 500 hPa, and an anticyclonic circulation with a cold core near the surface. The cyclonic circulation and its warm core of the mid-level vortex developed gradually downward toward the surface when environmental easterly and dry air intruded from the upper troposphere; finally, the mid-level vortex evolved into TC Usagi under favorable environment conditions such as weak vertical wind shear, deep moist layer, etc. To investigate the dynamic and thermodynamic processes during TC Usagi genesis, the technique of piecewise PV inversion is employed. The results show that the actions of upper-layer PV and potential temperature anomalies were not important in TC Usagi genesis. Surface-layer thermal anomalies mainly produced negative disturbances of temperature at the vortex center below 800 hPa, which was unfavorable to the genesis of a cyclonic circulation near the surface. Middle-to-lower-layer latent heat played a key role in TC Usagi genesis and downward development of dynamic and thermodynamic processes. The actions of dry air intrusion from the upper troposphere, environmental westerly changing into easterly in the middle and lower troposphere, and baroclinic structure of the vortex were also important. The cyclonic circulation of the mid-level vortex could develop downward quickly from the middle troposphere toward the surface. However, whether the warm core of the vortex developed near the surface depended on the combined actions of surface-layer thermal anomaly and middle-to-lower-layer latent heat. Finally, we present a conceptual model of TC Usagi genesis induced by a mid-level vortex over the SCS. 相似文献
17.
以三个西北太平洋热带气旋（TC）为例,利用WRF（Weather Research and Forecasting）模式进行了一系列海表温度（SST）敏感性数值试验,揭示了西北太平洋SST增暖对TC的强度、尺度及潜在破坏力的影响及其机理。结果表明,在距TC中心100 km以内区域的SST升高有利于TC强度增加,但会减小TC内核尺度;而在距TC中心100 km以外的SST升高并不会使TC强度明显增加甚至使TC强度减弱,但同时会增加TC内核尺度。伴随着低层向眼墙的入流,升高的外区SST会使TC区表层的大气温度和湿度升高,造成眼墙附近海气温差和湿度差及向内的气压梯度力减小,进而减少进入TC眼墙内的感热和潜热,不利于TC增强,但有利于眼墙向外移动,使TC内核尺度增加。内区SST升高与外区SST升高对TC强度及尺度变化的作用机理相反。因此,当TC移过冷或暖洋面时,TC的强度和尺度的变化不仅取决于局地洋面的冷或暖状况,还取决于TC内区和外区SST的差异。由于TC内区和外区SST对TC强度和内核尺度的不同作用,可能存在一个临界范围,当暖池范围在这个临界范围之内时TC潜在破坏力随暖池范围的扩大而增大,但当暖池范围超过这个临界范围时TC潜在破坏力便不会随着暖池范围的继续扩大而增大,甚至会有所减小。 相似文献
18.
强台风Chanchu（0601）的数值研究：转向前后内核结构和强度变化 总被引：3，自引：0，他引：3
使用FY卫星TBB资料和新一代非静力中尺度模式WRF分析南海强台风Chanchu(0601)"急翘"转向前后内核结构和强度变化过程。结果表明:转向后内核结构非对称特征明显。WRF数值模式较好地模拟出Chanchu强度和异常路径变化过程,再现了内核结构演变:转向前,垂直切变较弱,有利于快速加强,内核结构较为对称;转向后,垂直切变明显增大,强回波位于垂直切变下风方向的左侧,显示为内核非对称结构。使用傅立叶变换方法分解模拟结果中的雷达回波,发现眼壁和内螺旋雨带的2波非对称沿方位角移速与涡旋罗斯贝波(VRWs)的理论波速一致,Chanchu快速加强过程中断和强度维持的可能原因为:眼壁传播的VRWs受到外螺旋雨带的扰动以及涡旋倾斜加剧引起眼壁非对称性加强导致"急翘"时眼壁破裂,此后眼区和眼壁区水平混合过程加强,850 hPa眼区相当位温明显增加,抑制高层相对暖干空气和低层相对冷湿空气相互交换,使得随眼壁内侧下沉气流向下输送的暖干空气减少,低层增温作用减弱,快速加强过程中断;VRWs径向内传导致高值涡度由眼壁内侧向眼心传播,引起最大风速半径(RMW)内侧切向风速增大,RMW随时间向眼心延伸,眼壁进一步收缩,一定程度上抵消了垂直切变加大的负面影响,Chanchu维持强度。 相似文献
19.
By using idealized numerical simulations, the impact of tropical cyclone size on secondary eyewall formation (SEF) is examined. Both unbalanced boundary layer and balanced processes are examined to reveal the underlying mechanism. The results show that a tropical cyclone (TC) with a larger initial size favors a quicker SEF and a larger outer eyewall. For a TC with a larger initial size, it will lead to a stronger surface entropy flux, and thus more active outer convection. Meanwhile, a greater inertial stability helps the conversion from diabatic heating to kinetic energy. Furthermore, the progressively broadening of the tangential wind field will induce significant boundary layer imbalances. This unbalanced boundary layer process results in a supergradient wind zone that acts as an important mechanism for triggering and maintaining deep convection. In short, different behaviors of balanced and unbalanced processes associated with the initial wind profile lead to different development rates of the secondary eyewall. 相似文献
20.
The Role of Stationary and Transient Planetary Waves in the Maintenance of Stratospheric Polar Vortex Regimes in Northern Hemisphere Winter 总被引：1，自引：1，他引：0
Using 1958-2002 NCEPNCAR reanalysis data, we investigate stationary and transient planetary wave propagation and its role in wave-mean flow interaction which influences the state of the polar vortex (PV) in the stratosphere in Northern Hemisphere (NH) winter. This is done by analyzing the Eliassen-Palm (E-P) flux and its divergence. We find that the stationary and transient waves propagate upward and equatorward in NH winter, with stronger upward propagation of stationary waves from the troposphere to the stratosphere, and stronger equatorward propagation of transient waves from mid-latitudes to the subtropics in the troposphere. Stationary waves exhibit more upward propagation in the polar stratosphere during the weak polar vortex regime (WVR) than during the strong polar vortex regime (SVR). On the other hand, transient waves have more upward propagation during SVR than during WVR in the subpolar stratosphere, with a domain of low frequency waves. With different paths of upward propagation, both stationary and transient waves contribute to the maintenance of the observed stratospheric PV regimes in NH winter. 相似文献