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1.
M. B. Mathur 《Meteorology and Atmospheric Physics》1992,50(1-3):127-142
Summary Convective to planetary scale processes govern the motion and structure of tropical storms. A model with a high resolution and a large domain is required for accurate prediction of a storm's track and intensity. A series of integrations are performed using a primitive equation model and an initial state that defines a tropical storm that later developed into a hurricane in the real atmosphere. Increasing the horizontal resolution or domain of the model improves the forecast track. However only the increase in the horizontal resolution produces a better hurricane structure.Banded structure in the vertical motion field, asymmetries in the low tropospheric winds similar to those observed and upper tropospheric cyclonic outflow develop in high horizontal resolution experiments. It is shown that horizontal advection and pressure gradient terms produce wind tendencies in the low troposphere that displace the vortex in the observed direction. A high pressure area surrounding the central low pressure area appears in the upper troposphere. Around this high pressure area large pressure gradients develop that induce outflow winds in the distal storm area. 相似文献
2.
Intensity forecasting is one of the most challenging aspects of tropical cyclone (TC) forecasting. This work examines the impact of assimilating high-resolution all-sky infrared radiance observations from geostationary satellite GOES-13 on the convection-permitting initialization and prediction of Hurricane Joaquin (2015) with an ensemble Kalman filter (EnKF) based on the Weather Research and Forecasting (WRF) model. Given that almost all operational global and regional models struggled to capture Hurricane Joaquin (2015)’s intensity, this study examines the potential in improving Joaquin’s prediction when assimilating all-sky infrared radiances from GOES-13’s water vapor channel. It is demonstrated that, after a few 3-hour cycles assimilating all-sky radiance, the WRF model was able to forecast reasonably well Joaquin’s intensity, including its rapid intensification (RI). The improvement was largely due to a more realistic initial hurricane structure with a stronger, warmer, and more compact inner-core. Ensemble forecasts were used to further explore the important physical mechanisms driving the hurricane’s RI. Results showed that the RI forecasts were greatly impacted by the initial inner-core vortex structure. 相似文献
3.
为评价静止卫星大气温度廓线产品资料同化对飓风预报的影响,以2018年飓风“迈克尔”为例,选用GOES-16温度廓线产品,开展静止卫星资料同化及其对飓风预报影响的研究。首先,通过评估温度廓线产品精度,选取质量较好的高度层并以统计的各层均方根误差作为观测误差用于同化试验;然后,利用WRF-3DVar系统进行不同稀疏化及不同同化频次的循环同化敏感性试验;最后,利用WRF模式开展24 h数值预报。试验结果表明,在飓风“迈克尔”期间温度廓线在200~1 000 hPa之间的误差在2 K以内,将水平分辨率稀疏化为模式分辨率的6倍且循环同化频次为6 h时同化该资料对模式的初始场有最为合理的改进,从大尺度环境场上看使模式具备更合理的环流形势,能够有效提高对飓风的路径及强度的预报效果,更准确地模拟降水落区及美国佛罗里达州等降水关键区域的雨强。 相似文献
4.
利用WRF模式,研究了模式水平和垂直网格分辨率对台风“天鸽”（2017）模拟的影响。结果表明:水平分辨率的改变会对台风路径造成一定的影响,这种影响与改变水平分辨率以后所引起的台风强度和结构的变化有关。使用更高的水平分辨率时模拟的台风强度往往更强。此外,改变垂直分辨率对台风的路径模拟也有一定的影响。采用双曲正切的垂直分层方法,提高垂直层数,模式大气的垂直分辨率都有增加,但是在低层和高层垂直分辨率的增加更大。低层和高层垂直分辨率增加,模拟的台风强度增强。模式的水平分辨率和垂直分辨率之间匹配才能比较好地模拟台风,双向嵌套模式在提高嵌套层数的同时也要增加模式的垂直分辨率。台风强度和结构变化密切相关,台风强度增强的重要原因是台风云墙随着分辨率的增加更加陡峭,垂直风速随着水平分辨率的提高逐渐增强。 相似文献
5.
Studies on tropical cyclone(TC) inner-core size have become increasingly active in recent years. However, few studies have investigated the trend of TC inner-core size. Here, we introduce a new index to measure TC inner-core size and calculate the observed trend. This index can greatly reduce the influence of data heterogeneity and uncertainty. It also considers public concern because the new index is mainly determined by the inner-core size of strong TCs, which attract more public attention than weak TCs. The results show that in the past decades, TC inner-core size has a significant downtrend that is significant above the 99% confidence level when the new index is used. We also show that this trend is probably related to the increase in TC intensity and relatively small inner-core size of strong TCs. Moreover, relative sea surface temperature(SST) is assumed to make contributions to the downtrend of TC inner-core size, which has a significant negative correlation with the new index. 相似文献
6.
基于GRAPES区域中尺度数值预报系统(GRAPES_MESO),针对700 hPa、500 hPa和200 hPa的位势高度场H,温度场T,风场纬向分量U,经向分量V和地面降水场,在给定的模式物理过程下,分别考察了时间步长和空间分辨率对于模式预报效果的影响。研究结果表明,空间分辨率(0.3°×0.3°)相同时,各变量在不同层次的预报几乎都存在最优时间步长使得预报技巧最高,初步说明最优时间步长理论在复杂的偏微分方程组中的适用性。随后,将空间分辨率为0.3°×0.3°时最优时间步长(240 s)的预报结果与当前业务中(空间分辨率为0.15°×0.15°、时间步长为90 s)的预报结果进行比较,发现前者的变量H、T、U、V和地面降水场的预报技巧均高于后者,表明并不是空间分辨率越高预报效果越好。 相似文献
7.
Atmospheric turbulence is an important factor in the modelling of wind forces on structures and the losses they produce in
extreme wind events. However, while turbulence in non-hurricane winds has been thoroughly researched, turbulence in tropical
cyclones and hurricanes that affect the Gulf and Atlantic coasts has only recently been the object of systematic study. In
this paper, Florida Coastal Monitoring Program surface wind measurements over the sea surface and open flat terrain are used
to estimate tropical cyclone and hurricane wind spectra and cospectra as well as integral length scales. From the analyses
of wind speeds obtained from five towers in four hurricanes it can be concluded with high confidence that the turbulent energy
at lower frequencies is considerably higher in hurricane than in non-hurricane winds. Estimates of turbulence spectra, cospectra,
and integral turbulence scales presented can be used for the development in experimental facilities of hurricane wind flows
and the forces they induce on structures. 相似文献
8.
Typhoon Usagi (1319) was simulated by using the Advanced Weather Research and Forecasting numerical model (WRF) with different horizontal resolution to understand the impact of horizontal resolution on the intensity and characteristics of typhoon’s microstructures (including dynamic and microphysical structure). The simulated results show that the improvement of horizontal resolution from 5 km to 1 km has little impact on the track which is comparable to real results, but has a significant impact on the intensity and microstructures, and especially, the impact on wind speed at 10 m height, the vertical movement and precipitation intensity is the greatest. When the resolution is increased to 1 km, the intensity and characteristics of typhoon’s microstructures can be simulated better. In lower resolution simulations, some structural characteristics, including more asymmetrical and more outward tilted eyewall, and less water vapor flux on sea surface, work together to weaken typhoon intensity. 相似文献
9.
Summary The first part of the paper comprises of a control experiment and its forecasts validations with the observed. The PSU-NCAR
mesoscale model MM5 was utilized at a horizontal resolution of 4 km using the data sets for hurricane Charley of 2004. The
model configures some of the best available versions for physics and microphysical parameterizations schemes to produce forecasts
which are close to the observed trend of hurricane Charley. The basic validations of the control run were carried out in terms
of track, intensity (sea-level pressure and surface wind speed), storm propagation speed, precipitation and radar reflectivity
with that of observed. The validations were necessary because this control experiment will be considered as a benchmark forecast
for comparison with other microphysics sensitive experiments forecasts in the second part of this paper. In general, the control
run forecasts closely comply with that of observed track and intensity of the hurricane Charley. We also note that control
run manage to reproduce much of the important structural characteristics features of the hurricane as observed. 相似文献
10.
In this paper the impacts of vertical resolution on the simulations of Typhoon Talim (2005) are examined using the Weather Research and Forecasting (WRF) model, with cumulus parameterization scheme representing the cumulus convection implicitly. It is shown that the tropical cyclone (TC) track has little sensitivity to vertical resolution, whereas the TC intensity and structure are highly sensitive to vertical resolution. It is partly determined by the sensitivity of the planetary boundary layer (and the surface layer) and the cumulus convection processes to vertical resolution. Increasing vertical resolution in the lower layer could strengthen the TC effectively. Increasing vertical resolution in the upper layer is also beneficial for the storm intensification, but to a lesser degree. In contrast, improving the midlevel resolution may cause the convergence of environmental air, which inhibits the TC intensification. The results also show that the impacts of vertical resolution on features of the TC structure, such as the tangential winds, secondary circulations and the evolution of the warm-core structure, are consistent with the impacts on the TC intensity. It is suggested that in the simulations of TCs, the vertical levels should be distributed properly rather than the more the better, with higher vertical resolution being expected both in the lower and upper layer, while the middle layer should not hold too many levels. 相似文献
11.
Response of hurricane-type vortices to global warming as simulated by ARPEGE-Climat at high resolution 总被引：1，自引：0，他引：1
Atlantic hurricanes and their sensitivity to anthropogenic warming are investigated using very high (0.5°×0.5° over the Atlantic domain) resolution global simulations. The ARPEGE-Climat variable resolution grid demonstrates its usefulness in regional climate studies since resolution can be multiplied by a factor of 2.5 over the domain of interest compared to a uniform grid, for a similar computer cost. The question of hurricane characteristics dependence on anthropogenic warming is tackled trough the implementation of a tracking method. Changes in the total number, as well as locations, of hurricanes appear to depend more on sea surface temperature (SST) spatial patterns anomaly than Atlantic mean intensity, essentially through the change in large scale vertical wind shear. A uniform SST anomaly forcing produces increased and eastward shifted systems while a spatially contrasted anomaly leads to a decrease. Comparison between cyclogenesis density calculated from tracking or large scale combined variables (as a modified Gray parameter) brings some confidence in the use of the latter to investigate low resolution simulations. Mean hurricane dynamical characteristics are weakly changed by the warming but precipitation core and latent heat flux are enhanced in all scenarios. 相似文献
12.
The sensitivity of precipitation was studied by conducting control aqua-planet experiments(APEs) with a model to determine atmospheric general circulation.The model includes two versions: that with a spectral dynamical core(SAMIL) and that with a finite-volume dynamical core(FAMIL).Three factors were investigated including dynamical core,time-step length,and horizontal resolution.Numerical results show that the dynamical core significantly affects the structure of zonal averaged precipitation.FAMIL exhibited an equatorial precipitation belt with a single narrow peak,and SAMIL showed a broader belt with double peaks.Moreover,the time step of the model physics is shown to affect the zonal-averaged tropical convective precipitation ratio such that a longer time step leads to more production and consumption of convective available potential energy and convection initiated away from the equator,which corresponds to equatorial double peaks of precipitation.Further,precipitation is determined to be sensitive to horizontal resolution such that higher horizontal resolution allows for more small-scale kinetic energy to be resolved and leads to a broader probability distribution of low-level vertical velocity.This process results in heavier rainfall and convective precipitation extremes in the tropics.Abstract The sensitivity of precipitation was studied by conducting control aqua-planet experiments(APEs)with a model to determine atmospheric general circulation.The model includes two versions:that with a spectral dynamical core(SAMIL)and that with a finite-volume dynamical core(FAMIL).Three factors were investigated including dynamical core,time-step length,and horizontal resolution.Numerical results show that the dynamical core significantly affects the structure of zonal averaged precipitation.FAMIL exhibited an equatorial precipitation belt with a single narrow peak,and SAMIL showed a broader belt with double peaks.Moreover,the time step of the model physics is shown to affect the zonal-averaged tropical convective precipitation ratio such that a longer time step leads to more production and consumption of convective available potential energy and convection initiated away from the equator,which corresponds to equatorial double peaks of precipitation.Further,precipitation is determined to be sensitive to horizontal resolution such that higher horizontal resolution allows for more small-scale kinetic energy to be resolved and leads to a broader probability distribution of low-level vertical velocity.This process results in heavier rainfall and convective precipitation extremes in the tropics. 相似文献
13.
热带气旋的快速增强机制目前仍然不太清楚,不少研究开始关注快速增强过程中热带气旋内核结构的变化。通过比较模拟的西北太平洋超强台风Rammasun (2014)和大西洋5级飓风Wilma (2005)快速增强过程中内核结构的变化特点,理解内核结构在快速增强过程中的变化特点。飓风Wilma是一个典型的快速增强热带气旋,快速增强期间具有弱的环境垂直切变、对称的眼墙、较小的中心倾斜以及比较直立的眼墙。但是,台风Rammasun快速增强发生在较强切变(超过10 m/s)环境下,眼墙对流呈高度不对称,强对流基本固定在台风中心的南侧。整个快速增强期间,Rammasun在垂直方向上维持较大的中心倾斜以及较大的眼墙倾斜。结果表明,快速增强也可能在不完全对称的内核结构和倾斜垂直结构的情况下发生。 相似文献
14.
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
15.
高分辨率模式中积云参数化方案对模拟台风“凡亚比”的影响 总被引：1，自引：0，他引：1
在高水平分辨率模式(3～6 km)中,对于是否应该再使用积云参数化方案,仍存在着争论.为此,利用WRF模式,在5 km水平分辨率下,研究了不同云降水方案对一次台风过程模拟的影响,并对影响原因进行了初步探索.结果表明,即使在5 km高水平分辨率下,使用积云参数化方案仍能有效改善对台风路径的模拟,同时,成熟的混合冰相微物理方案对模拟台风路径也非常重要;对台风强度模拟,对积云参数化方案的选择较为敏感和复杂;在48 h预报时效内,只使用微物理方案模拟的降水较好,使用积云参数化方案容易产生较多的虚假降水,但能改善第3天24 h累积降水模拟.这些研究结果为利用高水平分辨率模式模拟台风和改进积云参数化方案提供一定借鉴. 相似文献
16.
基于大气辐射传输理论分别建立Ku波段和C波段的降雨模型,模拟热带气旋降雨区洋面的雷达回波并反演了洋面10 m风场,用于研究降雨对测风的影响以及风云三号双频风场雷达 (WFR) 的测风能力。分析表明:回波的衰减或增强取决于降雨衰减项和后向散射项的相对大小;热带气旋的降雨使反演风速偏小,风向精度降低,Ku波段相对于C波段更易受影响,在高风速 (超过30 m·s-1) 条件下,可达5~20 m·s-1的负风速偏差。反演结果表明:双频反演的新方法能够结合Ku波段与C波段的优势,双频最大似然估计 (MLE) 方法在分辨率上优于C波段单频反演,相对Ku单频反演能降低降雨对测风的衰减作用,结合双频MLE方法和C波段单频反演优势的分区反演方法可以显著减小降雨偏差,提高风速反演精度,在有风云三号湿度计同步观测的条件下,是提高热带气旋降雨区测风精度的有效手段。 相似文献
17.
The fifth-generation Pennsylvania State University/NCAR Mesoscale Model Version 3 (MM5V3) was used to simulate extreme heavy rainfall events over the Yangtze River Basin in June 1999. The effects of model's horizontal and vertical resolution on the extreme climate events were investigated in detail. In principle, the model was able to characterize the spatial distribution of monthly heavy precipitation. The results indicated that the increase in horizontal resolution could reduce the bias of the modeled heavy rain and reasonably simulate the change of daily precipitation during the study period. A finer vertical resolution led to obviously improve rainfall simulations with smaller biases, and hence, better resolve heavy rainfall events. The increase in both horizontal and vertical resolution could produce better predictions of heavy rainfall events. Not only the rainfall simulation altered in the cases of different horizontal and vertical grid spacing, but also other meteorological fields demonstrated diverse variations in terms of resolution change in the model. An evident improvement in the simulated sea level pressure resulted from the increase of horizontal resolution, but the simulation was insensitive to vertical grid spacing. The increase in vertical resolution could enhance the simulation of surface temperature as well as atmospheric circulation at low levels, while the simulation of circulation at middle and upper levels were found to be much less dependent on changing resolution. In addition, cumulus parameterization schemes showed high sensitivity to horizontal resolution. Different convective schemes exhibited large discrepancies in rainfall simulations with regards to changing resolution. The percentage of convective precipitation in the Grell scheme increased with increasing horizontal resolution. In contrast, the Kain-Fritsch scheme caused a reduced ratio of convective precipitation to total rainfall accumulations corresponding to increasing horizontal resolution. 相似文献
18.
浙江沿海登陆台风结构特性的多普勒雷达资料分析 总被引：1，自引：0，他引：1
利用浙江省新一代多普勒雷达组网资料,选取在浙江东南沿海近乎同一地点登陆的3个台风进行研究。从登陆前6 h到登陆后7 h,对比分析3个台风在登陆前后的雷达回波和降水结构时空变化特征。利用单多普勒雷达四维变分风场反演技术,对温州多普勒雷达探测资料进行了风场反演。结合利用雷达回波强度资料,对3个台风登陆前后1 h在云岩、昌禅等地造成特大暴雨的中尺度对流系统的三维结构及其演变特征进行了详细分析。结果表明,台风强度与其螺旋云带中的对流单体密切相关。台风强度愈强,其中低层环状平均回波强度就愈强,对流活动也就愈旺盛,降水强度也愈大。台风登陆前,回波(雨带)从眼墙向外围传播。台风登陆后,随着台风外围回波(雨带)明显减弱,台风眼墙回波(雨带)则明显增强,台风眼区逐渐被强回波所取代,使台风登陆后眼墙的平均雨强比登陆前增大。台风登陆后1 h,由于低(高)层水平辐合(散)增强,强对流回波中倾斜的上升(下沉)气流明显增大,使对流运动更加活跃,造成登陆后1 h的降雨量显著增强。台风强度与登陆后1 h降雨量的增强幅度成正比。台风强度越强,垂直风切变就越大,垂直切变风速大值区与最大降雨区有较好的对应关系。台风登陆后1 h,垂直切变风速的明显增加对登陆台风螺旋雨带中的中小尺度对流的加强和维持起到了非常重要的作用。 相似文献
19.
The sensitivity of the simulation of tropical cyclone(TC) size to microphysics schemes is studied using the Advanced Hurricane Weather Research and Forecasting Model(WRF). Six TCs during the 2013 western North Pacific typhoon season and three mainstream microphysics schemes–Ferrier(FER), WRF Single-Moment 5-class(WSM5) and WRF Single-Moment6-class(WSM6)–are investigated. The results consistently show that the simulated TC track is not sensitive to the choice of microphysics scheme in the early simulation, especially in the open ocean. However, the sensitivity is much greater for TC intensity and inner-core size. The TC intensity and size simulated using the WSM5 and WSM6 schemes are respectively higher and larger than those using the FER scheme in general, which likely results from more diabatic heating being generated outside the eyewall in rainbands. More diabatic heating in rainbands gives higher inflow in the lower troposphere and higher outflow in the upper troposphere, with higher upward motion outside the eyewall. The lower-tropospheric inflow would transport absolute angular momentum inward to spin up tangential wind predominantly near the eyewall, leading to the increment in TC intensity and size(the inner-core size, especially). In addition, the inclusion of graupel microphysics processes(as in WSM6) may not have a significant impact on the simulation of TC track, intensity and size. 相似文献
20.
Summary Seven different microphysical sensitivity experiments were designed with an objective to evaluate their respective impacts
in modulating hurricane intensity forecasts using mesoscale model MM5. Microphysical processes such as melting of graupel,
snow and cloud ice hydrometeors, suppression of evaporation of falling rain, the intercept parameter and fall speed of snow
and graupel hydrometeors are modified in the existing NASA Goddard Space Flight Center (GSFC) microphysical parameterization
scheme. We studied the impacts of cloud microphysical processes by means of track, intensity, precipitation, propagation speed,
kinematic and thermodynamic vertical structural characteristics of hurricane inner core. These results suggest that the set
of experiments where (a) melting of snow, graupel and cloud ice were suppressed (b) melting of snow and graupel were suppressed
and (c) where the evaporation of rain water was suppressed all produced most intense storms. The major findings of this study
are the interconversion processes such as melting and evaporation among hydrometeors and associated feedback mechanism are
significantly modulate the intensity of the hurricane. In particular an experiment where the melting of graupel, snow and
cloud ice hydrometeors was eliminated from the model parameterization scheme produced the most explosively intensified storm.
In the experiment where rain water evaporation was eliminated from the model, it produced a stronger storm as compared to
the control run but it was not as strong as the storms produced from absence of melting processes. The impact on intensity
due to variations made in intercept parameters of the hydrometeors (i.e., snow and graupel) were not that evident compared
to other experiments. The weakest storm was noted in the experiment where the fall speeds of the snow hydrometeors were increased
two fold. This study has isolated some of the factors that contributed to a stronger hurricane and concludes with a motivation
that the findings from this study will help in further improvement in the design of sophisticated explicit microphysical parameterization
for the mesoscale non-hydrostatic model for realistic hurricane intensity forecasts. 相似文献