湿地边界层通量影响热带气旋登陆维持和降水的数值试验

用MM5v3模式及其TC Bogus方案对台风Nina(7503)在中国大陆上的维持加强过程进行模拟,并通过各种敏感性试验,研究了饱和湿地对热带气旋在大陆上维持和降水的影响。结果表明:湿地边界层内各通量对登陆热带气旋的强度、结构及其降水具有明显影响。潜热通量和感热通量均有利于热带气旋的维持和加强,其中潜热输送的作用显著,感热输送的作用较小。潜热和感热通量有利于热带气旋雨带螺旋结构的维持,对台风降水分布有明显影响,动量通量对热带气旋风场有显著的削弱作用,是其能量耗散、低压填塞的主要原因,但对台风降水具有局地增幅作用。     

海洋飞沫对热带气旋影响的数值试验

将最新版的Andreas海洋飞沫通量参数化方案与中尺度大气模式MM5V3耦合,对0514号热带气旋Nabi进行数值模拟,探讨海洋飞沫蒸发对热带气旋发展和演变的影响.模拟结果表明,考虑海洋飞沫的作用后,热带气旋范围内(气旋中心附近600 km左右范围内)的潜热和感热通量明显增强,尤其是潜热通量,最大值可提高35%～80%,潜热通量的大值区对应热带气旋眼墙处的最大风速区.无论是否考虑海洋飞沫作用,模式均能较好地模拟出热带气旋Nabi的移动路径,但考虑飞沫作用后,由于飞沫对海气界面通量交换的贡献,使得模拟热带气旋中心的最低海平面气压降低,最大风速增强,暖心结构更加明显.     

美国“狂飙”计划的现状及未来

狂飙计划由美国国家海洋大气局进行,目的是研究热带气旋的结构与动力学问题,和对它进行人工影响的可能性。一、“狂飙”假说狂飙试验通过改变风暴中心附近能量的分布,达到减慢风速的目的。热带气旋的能量几乎完全来自空气迅速对流时释放的潜热。在低空,热带海洋上的暖湿空气向着风暴中心卷入,挟带着大量潜热及感热。当气流进入风暴时,它要从海洋补充能量。空气的上升运动大部分发生于眼壁(这是环绕台风眼的一条云带)以及周围的雨带云之中。入流气流所包含的潜热,大部分在这些云中释放成为驱动风暴的主要能量来源。从入流气流层到外流气流层之间,上升气流的     

热带气旋强度与结构研究新进展

主要回顾热带气旋(TC)强度与结构变化的研究发展近况。以往热带气旋的理论研究认为在给定的大气和海洋热状况下，存在着一个TC所能达到的最大可能强度(MPI)。但实际上，海洋生成的热带气旋达到的最大强度普遍要比由MPI理论计算得到最大强度要低。近几年的研究表明，存在着内部和外部的不利因子通过对TC结构的改变来阻碍其加强，从而限制TC的强度。以往认为在诸多因子中，垂直风切变产生的内核区非对称结构与眼墙区下方海水上涌造成的海面冷却是制约TC达到MPI的主要因子。最新的研究进一步指出，产生TC非对称性的中尺度过程对其强度与结构的变化至关重要。中尺度过程包含有对流耦合的涡旋Rossby波、内外圈螺旋雨带、嵌于TC环流内的中尺度涡旋。外部的环境气流也是通过这些眼墙的中尺度过程影响到TC的强度与结构变化。     

热带气旋过程中海-气界面热量交换

为探索热带气旋与海洋相互作用,采用国家海洋局南海分局Marex(马瑞克斯)数据浮标实测资料,计算了1986年南海的7个热带气旋海气界面热量交换值.结果表明:热带气旋海气界面热量交换强烈,主要贡献来自潜热通量;热带气旋环流内水温、气温均是下降趋势,气温下降更为明显;夏季热带气旋环流内,感热通量会出现负值,海面有效反射辐射通量出现减弱现象;秋季热带气旋环流内,感热通量和海面有效反射辐射通量显著加强;在热带气旋环流内,海面吸收的短波辐射通量均出现减弱现象;热带气旋环流内受到冷空气影响时,感热变得相当重要,热带气旋表现为对海洋的响应为主.     

β效应和垂直切变对台风非对称结构及眼墙替换的影响

利用一个完全可压、非静力及原始方程热带气旋模式(TCM4),通过对f平面和β平面中不同强度的垂直风切变下理想热带气旋的模拟,研究了β效应和垂直风切变对热带气旋强度和结构的影响。结果表明:(1)理想气旋植入相对较弱的垂直风切变之后其强度最终将会进入一种近似常定状态,通过研究这种准常定状态对切变强度的敏感性发现,研究垂直风切变对理想气旋影响,应该讨论理想气旋能否维持在一个特定强度(台风、热带风暴及热带低压等)的极限垂直切变,而不是去讨论决定理想气旋将减弱还是增强的极限垂直风切变值;(2)在f平面下,由于垂直风切变造成涡度平流随高度变化,使得在顺切变前部以及左侧边界层附近产生辐合,伴随着空气的气旋式螺旋上升,外流层对应区域产生辐散,从而使得强对流和强降水发生在顺切变左侧。(3)行星涡度梯度(β效应)也能使涡旋产生一定的非对称性。当考虑β效应和垂直风切变的双重叠加效应时,所产生的非对称性比单纯由β效应或垂直风切变产生的非对称性更大,并且强对流区主要集中在顺切变左前部。(4)热带气旋眼墙替换过程或许可以被预测,因为它们似乎与β效应和环境流(VWS)存在联系。     

环境气流及非绝热加热对热带气旋结构和移动的影响

设计一个三层的准地转斜压模式,研究了不同结构环境气流和环境非绝热加热场中热带气旋移动路径和结构的特征.数值试验的结果表明:(1)无外界影响下热带气旋向西北方向移动,垂直速度场有明显的螺旋结构;(2)热带气旋主要受基本环境气流引导,非对称环流中的小扰动干扰了热带气旋的移动;(3)非绝热加热场对热带气旋影响较大,热带气旋有向加热中心移动的倾向,同时热带气旋的水平、垂直结构都有较大的变化.     

热带气旋外眼墙形成机制研究综述

介绍了国内外关于热带气旋外眼墙形成和维持过程的相关研究进展,包括大尺度环境场和热带气旋涡旋内部动力学过程,如涡旋罗斯贝波理论、轴对称化过程、涡丝化作用、β-skirt轴对称化外眼墙形成假说和边界层非平衡动力过程等。随着对外眼墙形成机理研究的不断深入,当前存在多种外眼墙形成的机制理论,而这些机制均强调在外眼墙的形成阶段,热带气旋外围有大量对流及位势涡度扰动的发生发展。因此,热带气旋外眼墙的形成很有可能是多种机制相互作用导致的。最后,提出研究多种机制相互作用导致外眼墙处的对流和位势涡度扰动的发生发展过程具有重大意义。     

1986年东海与南海的海-气界面热量交换

采用实测资料计算1986年7—12月东海和南海观测海域海-气界面热量交换。结果表明：7—9月上旬,大气向观测海域输送热量是主要现象,因为这时的气温比水温高,潜热通量与感热通量出现反相变化,天气晴好,海洋大量吸热;9月中旬—12月,观测海域向大气输送热量是主要现象,东海表现得比南海更为明显,主要贡献来自潜热通量和感热通量。受冷空气影响时,感热通量重要;在热带辐合带和热带气旋系统内海-气界面热量交换强烈,大气对海洋的响应为主。     

地形和边界层摩擦对登陆热带气旋路径和强度影响的研究

采用准地转的正压模式, 研究了无非绝热加热时地形和边界层摩擦对登陆热带气旋路径和强度的影响.结果表明: 地形作用对登陆热带气旋西北移动路径的影响比较明显, 而对登陆热带气旋强度的影响不明显; 边界层摩擦可以通过改变热带气旋X方向上和Y方向上的移动速度以及改变热带气旋水平环流结构对登陆热带气旋西北移动路径产生一定的影响, 边界层摩擦对登陆热带气旋强度的影响非常明显, 其中摩擦是造成登陆热带气旋强度迅速减弱的一个重要因素.     

海温及海浪对台风眼墙中尺度涡的影响

本文利用包括海气耦合、气浪耦合及浪流耦合的完全耦合系统,着重研究了2006年“格美”(Kaemi)台风眼墙内的中尺度涡结构。中尺度涡作为影响台风眼墙非对称结构的内部因子,与风垂直切变密切相关,其发展过程受台风下垫面海洋状况的影响。在顺切变右侧,垂直气流逐渐增强,在顺切变左侧达到最大后逐渐减弱。当不考虑海表温度的冷涌反馈作用时,海气间的热通量输送较大,由此引起眼墙内的中尺度对流加强,但集中爆发区仍然位于顺切变方向,不受热通量输送变化的影响。当不考虑海浪对海表粗糙度的影响时,在较小的海表粗糙度条件下,眼墙非对称性减弱,使得中尺度对流涡在切向方向上的分布较为均匀。     

西北太平洋海温增暖对热带气旋潜在破坏力的影响:高分辨模式个例分析

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。      

Air-sea Interaction of Typhoon Sinlaku （2002） Simulated by the Canadian MC2 Model

Three experiments for the simulation of typhoon Sinlaku (2002) over the western North Pacific are performed in this study by using the Canadian Mesoscale Compressible Community (MC2) atmospheric model. The objective of these simulations is to investigate the air-sea interaction during extreme weather conditions, and to determine the sensitivity of the typhoon evolution to the sea surface temperature (SST)cooling induced by the typhoon. It is shown from the three experiments that the surface heat fluxes have a substantial influence on the slow-moving cyclone over its lifetime. When the SST in the East China coastal ocean becomes 1℃ cooler in the simulation, less latent heat and sensible heat fluxes from the underlying ocean to the cyclone tend to reduce the typhoon intensity. The cyclone is weakened by 7 hPa at the time of its peak intensity. The SST cooling also has impacts on the vertical structure of the typhoon by weakening the warm core and drying the eye wall. With a finer horizontal resolution of (1/6)°×(1/6)°, the model produces higher surface wind, and therefore more surface heat fluxes are emitted from the ocean surface to the cyclone, in the finer-resolution MC2 grid compared with the relatively lower resolution of 0.25°×0.25°MC2 grid.     

THE CHARACTERISTICS OF AIR-SEA HEAT FLUX EXCHANGE DURING THE GENERATION AND DEVELOPMENT OF LOCAL TYPHOONS OVER THE SOUTH CHINA SEA

A South China Sea （SCS） local TC （SLT） is defined as a tropical cyclone （TC） that forms within the SCS region and can reach the grade of tropical storm （TS） or above. The statistical features of the SLTs from 1985 to 2007 are analyzed first. It is found that over the SCS about 68% of the TCs can develop into TSs. The SLT intensity is relatively weak and associated with its genesis latitude as well as its track. The SLT monthly number presents a seasonal variation with two peaks in May and July to September. Based on the daily heat flux data from the Woods Hole Oceanographic Institution_Objectively Analyzed air-sea Fluxes （WHOI_OAFlux） in the same period, the air-sea exchange during the process of generation and development of the SLT is studied. Results show that the heat fluxes released to the atmosphere increase significantly day by day before cyclogenesis. The ocean to the south to the TC center provides the main energy. Along with the development of SLT, the regions with large heat fluxes spread clockwise to the north of TC, which reflects the energy dispersion property of vortex Rossby waves in the periphery of the TC. Once the SLT forms the heat fluxes are not intensified as much. During the whole process, the net heat, latent heat and sensible heat flux display a similar evolution, while the latent heat flux makes a main contribution to the net heat flux. The maximum air-sea heat exchange always occurs at the left side of the TC moving direction, which may reflect the influence of the SCS summer monsoon on TC structure.     

Impact of Surface Exchange Coefficients and Sea Surface Cooling on Tropical Cyclone Simulation

The surface flux exchange associated with the exchange coefficients and upper ocean conditions is essential to the development of tropical cyclones (TCs). Using the Weather Research and Forecasting (WRF) model, the present study has investigated the impact of exchange coefficients and ocean coupling during Super Typhoon Saomai (2006). Firstly, two experiments with different formula of roughness are conducted. The experiment with the Donelan formula for drag coefficient (Cd) and ramped formula for enthalpy coefficient (Ck) can simulate stronger intensity compared to other experiments due to the increased surface wind and enthalpy fluxes. That is because the new formulas allows for a smaller Cd and larger Ck in the high wind regime than the former formulas did. Moreover, two coupled simulations between WRF and a one-dimensional ocean model are conducted to examine the feedback of sea surface cooling to the TC. In the experiments with a horizontal uniform mixed layer depth of 70 m, the sea surface cooling is too weak to change the evolution of TC. While in the experiment with an input mixed layer calculated using the Hybrid Coordinate Ocean Model (HYCOM) data, the significant sea surface cooling induces obvious impact on TC intensity and structure. Under the negative feedback of sea surface cooling, the sensible and latent heat fluxes decreases, especially in the right part of Saomai (2006). The negative feedback with coupled ocean model plays a vital role in simulating the intensity and structure of TC.     

海气相互作用对台风结构的影响

利用前期工作中耦合试验和未耦合试验对台风Krovanh(2003年)数值模拟的结果,分析了海-气相互作用对台风结构的影响。结果表明,台风引起的海面降温大大降低了海洋向大气输送的潜热通量,同时使得感热通量向下传递到海洋。另一方面,台风引起的海表面温度(SST)降低,反馈到台风使其结构轴不对称性加强,且在中高层尤为显著。分析了台风对称结构的基本特征。     

NUMERICAL EXPERIMENTS ON THE IMPACTS OF SEA SPRAY ON TROPICAL CYCLONES

The latest version of sea spray flux parameterization scheme developed by Andreas is coupled with the PSU/NCAR model MM5 in this paper. A western Pacific tropical cyclone named Nabi in 2005 is simulated using this coupled air-sea spray modeling system to study the impacts of sea spray evaporation on the evolution of tropical cyclones. The results demonstrate that sea spray can lead to a significant increase of heat fluxes in the air-sea interface, especially the latent heat flux, the maximum of which can increase by up to about 35% - 80% The latent heat flux seems to be more important than the sensible heat flux for the evolution of tropical cyclones. Regardless of whether sea spray fluxes have been considered, the model can always simulate the track of Nabi well, which seems to indicate that sea spray has little impact on the movement of tropical cyclones. However, with sea spray fluxes taken into account in the model, the intensity of a simulated tropical cyclone can have significant increase. Due to the enhancement of water vapor and heat from the sea surface to the air caused by sea spray, the warm core structure is better-defined, the minimum sea level pressure decreases and the vertical speed is stronger around the eye in the experiments, which is propitious to the development and evolution of tropical cyclones.     

Current understanding of tropical cyclone structure and intensity changes – a review

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.     

Impacts of the Lowest Model Level Height on Tropical Cyclone Intensity and Structure简

Variable thicknesses in the lowest half-ηmodel level （LML） are often used in atmospheric models to compute surface diagnostic fields such as surface latent and sensible heat fluxes.The effects of the LML on simulated tropical cyclone （TC）evolution were investigated in this study using the Weather Research and Forecasting （WRF） model.The results demonstrated notable influences of the LML on TC evolution when the LML was placed below 12 m.The TC intensification rate decreased progressively with a lowering of the LML,but its ultimate intensity change was relatively small.The maximum 10-m winds showed different behavior to minimum sea level pressure and azimuthally-averaged tangential winds,and thus the windpressure relationship was changed accordingly by varying the LML.The TC circulation was more contracted in association with a higher LML.Surface latent heat fluxes were enhanced greatly by elevating the LML,wherein the wind speed at the LML played a dominant role.The changes in the wind speed at the LML were dependent not only on their profile differences,but also the different heights they were taken from.Due to the enhanced surface heat fluxes,more intense latent heat release occurred in the eyewall,which boosted the storm＇s intensification.A higher LML tended to produce a stronger storm,and therefore the surface friction was reinforced,which in turn induced stronger boundary layer inflow together with increased diabatic heating.     

Dynamical effects of environmental vertical wind shear on tropical cyclone motion, structure, and intensity

Summary A series of numerical experiments on an f plane are conducted using the fifth-generation Pennsylvania State University-National Center for Atmospheric Research Mesoscale Model, version 3 (MM5) to investigate how environmental vertical wind shear affects the motion, structure, and intensity of a tropical cyclone. The results show that a tropical cyclone has a motion component perpendicular to the vertical shear vector, first to the right of the shear and then to the left. An initially axisymmetric, upright tropical cyclone vortex develops a downshear tilt and wavenumber-one asymmetry when embedded in environmental vertical wind shear. In both small-moderate shears, a storm weakens slightly compared to that in a quiescent environment. The circulation centers between 300 hPa and the surface varies from 20 km to over 80 km. The secondary circulation becomes quite asymmetric about the surface cyclone center. As a result, convection on the upshear-right quadrant diminishes, limiting the upward heat transport in the eyewall and thus lowering the warm core and leading to a weakening of the storm. In strong vertical shear (above 12 m s⁻¹), the vertical tilt exceeds 160 km in 48 h of simulation and the secondary circulation on the upshear side is completely destroyed with low-level outflow. The axisymmetric component of eyewall convection weakens remarkably and becomes much less penetrative. As a result, the warm core becomes weak and appears at lower levels and the storm weakens rapidly accordingly. This up-down weakening mechanism discussed in this study is different from those previously discussed. It emphasizes the penetrative role of eyewall convection in transporting heat from the ocean to the mid-upper troposphere, maintaining the warm core structure of the tropical cyclone. The vertical shear is found negative to eyewall penetrative convection.