共查询到20条相似文献，搜索用时 140 毫秒
1.
The basic structure and cloud features of Typhoon Nida
(2016) are simulated using a new microphysics scheme (Liuma)
within the Weather Research and Forecasting (WRF) model. Typhoon
characteristics simulated with the Liuma microphysics scheme are
compared with observations and those simulated with a commonly-
used microphysics scheme (WSM6). Results show that using
different microphysics schemes does not significantly alter the
track of the typhoon but does significantly affect the intensity
and the cloud structure of the typhoon. Results also show that
the vertical distribution of cloud hydrometeors and the
horizontal distribution of peripheral rainband are affected by
the microphysics scheme. The mixing ratios of rain water and
graupel correlate highly with the vertical velocity component
and equivalent potential temperature at the typhoon eye-wall
region. According to the simulation with WSM 6 scheme, it is
likely that the very low typhoon central pressure results from
the positive feedback between hydrometeors and typhoon
intensity. As the ice-phase hydrometeors are mostly graupel in
the Liuma microphysics scheme, further improvement in this
aspect is required. 相似文献
2.
台风“云娜”在近海强度变化及结构特征的数值研究Ⅰ:云微物理参数化对云结构及降水特征的影响 总被引：2，自引：1，他引：1
首先对AREM模式模拟的台风基本结构和云结构进行验证,检验了模拟结果的可靠性.在此基础上,设计了5组试验来研究云微物理参数化方案对台风"云娜"云结构及降水特征的影响.试验设计主要突出冰相云微物理过程、云微物理特征引发的冷却效应以及霰下落速度的重要性.结果表明:云微物理参数化过程对云的发展和降水特征的影响更为显著.各试验的水凝物分布和强度不同,降水类型和强度存在较大差异,由此引起的云中热力结构也有较大区别;在所有试验方案中,24 h降水率最大差异为52.5 mm/h.云微物理过程对云和降水特征的具体影响表现在:(1)如果不考虑雨水蒸发冷却效应,此时台风内核上升运动强度最强(达到-19 Pa/s),雨水和霰粒子增长最明显,相对于对照试验增量分别为1.8和2.5 g/kg.(2)霰和雪的融化对于螺旋雨带中雨滴的增长十分重要,但他们可能不是云墙中雨水形成的主导因子.(3)不同方案的降水模拟特征也存在较大差别,采用暖云参数化后,降水区域最小,但其中对流降水比例最大(63.19%);霰落速减半后,降水区域最大,其中非对流降水比例也最大(51.15%). 相似文献
3.
With the Reisner-2 bulk microphysical parameterization of the fifth-generation Pennsylvania State University–U.S. National Center for Atmospheric Research (PSU–NCAR) Mesoscale Model (MM5), this paper investigates the microphysical sensitivities of Typhoon Chanchu. Four different microphysical sensitivity experiments were designed with an objective to evaluate their respective impacts in modulating intensity forecasts and microphysics budgets of the typhoon. The set of sensitivity experiments were conducted ... 相似文献
4.
By using the Advanced Regional Eta-coordinate Model (AREM),the basic structure and cloud features of Typhoon Rananim are simulated and verified against observations.Five sets of experiments are designed to investigate the effects of the cloud microphysical processes on the model cloud structure and precipitation features.The importance of the ice-phase microphysics,the cooling effect related to microphysical characteristics change,and the influence of terminal velocity of graupel are examined.The results indicate that the cloud microphysical processes impact more on the cloud development and precipitation features of the typhoon than on its intensity and track.Big differences in the distribution pattern and content of hydrometeors,and types and amount of rainfall occur in the five experiments,resulting in different heating and cooling effects.The largest difference of 24-h rain rate reaches 52.5 mm h-1.The results are summarized as follows:1) when the cooling effect due to the evaporation of rain water is excluded,updrafts in the typhoon's inner core are the strongest with the maximum vertical velocity of-19 Pa s-1 and rain water and graupel grow most dominantly with their mixing ratios increased by 1.8 and 2.5 g kg-1,respectively,compared with the control experiment; 2) the melting of snow and graupel affects the growth of rain water mainly in the spiral rainbands,but much less significantly in the eyewall area; 3) the warm cloud microphysical process produces the smallest rainfall area and the largest percentage of convective precipitation (63.19％),while the largest rainfall area and the smallest percentage of convective precipitation (48.85％) are generated when the terminal velocity of graupel is weakened by half. 相似文献
5.
将中国气象科学研究院（CAMS）混合双参数云微物理方案用于中尺度天气模式WRF,开展了对2013年超强台风天兔（1319）的模拟,通过与台风最佳路径、强度及热带降雨测量卫星（TRMM）资料对比,分析CAMS云微物理方案在模拟台风中的适用性及云微物理过程对模拟台风天兔的影响机制。设计了3组敏感性试验:修改雪粒子质量和落速系数（EXP1）,采用海洋性云滴参数（EXP2）,同时修改雪粒子质量和落速系数并采用海洋性云滴参数（EXP3）。结果表明:EXP1和EXP3由于霰碰并雪速率的增加及减小的雪下落通量,导致雪含量显著降低,同时也减少了整体冰相物的含量;EXP2和EXP3模拟的台风眼区对流有效位能快速减小,再现了前期台风的快速增强过程,路径偏差也最小;各试验模拟的小时降水率总体偏强,EXP3的降水空间分布与实况更接近,明显降低雪粒子含量,并一定程度上改善模拟的台风路径、强度及降水分布等。该结果不但可为改进适用于台风的云微物理参数化方案提供思路,也可加深云微物理过程对台风影响的认识。 相似文献
6.
本文以GFS资料为初始场,利用WRF（v3.6.1）模式对2015年第22号台风“彩虹”进行了数值研究。采用CMA（中国气象局）台风最佳路径、MTSAT卫星、自动站降水为观测资料,对比了4个微物理方案（Lin、WSM6、GCE和Morrison）对“彩虹”台风路径、强度、结构、降水的模拟性能。模拟发现上述4个云微物理方案都能较好地模拟出“彩虹”台风西行登陆过程,但是其模拟的台风强度、结构及降水存在较大差异;就水成物而言,除GCE方案对雨水的模拟偏高以外,其他方案对云水、雨水过程的模拟较为接近,其差异主要存在于云冰、雪、霰粒子的模拟上。本文对比分析了WSM6和Morrison两个方案模拟的云微物理过程,发现WSM6方案模拟的雪和霰粒子融化过程显著强于Morrison方案,但是冰相粒子间转化过程的强度明显弱于Morrison方案。云微物理过程的热量收支分析表明:WSM6方案模拟的眼区潜热更强,暖心结构更为显著,台风中心气压更低。细致的云微物理转化分析表明,此次台风降水的主要云微物理过程是水汽凝结成云水和凝华为云冰;生成的云水一方面被雨水收集碰并直接转化为雨水,另一方面先被雪粒子碰并收集转化为霰,然后霰粒子融化成雨水;而生成的云冰则通过碰并增长转化为雪。小部分雪粒子通过碰并收集过冷水滴并淞附增长为霰粒子,随后融化为雨水,大部分雪粒子则直接融化形成地面降水。 相似文献
7.
Based on different parameterization schemes of planetary boundary layer (PBL), the uncertainty of intensity and structure of the Super-strong Typhoon Rammasun (1409) is investigated using the WRF model (v3.4) with six PBL parameterization schemes. Results indicate that PBL uncertainty leads to the uncertainty in tropical cyclone (TC) prediction, which increases with forecast time. The uncertainty in TC prediction is mainly reflected in the uncertainty in TC intensity, with significant differences in the TC intensity forecasts using various PBL schemes. The uncertainty in TC prediction is also reflected in the uncertainty in TC structures. Greater intensity is accompanied by smaller vortex width, tighter vortex structure, stronger wind in the near-surface layer and middle and lower troposphere, stronger inflow (outflow) wind at the lower (upper) levels, stronger vertical upward wind, smaller thickness of the eye wall, smaller outward extension of the eye wall, and warmer warm core at the upper levels of eye. PBL height, surface upward heat flux and water vapor flux are important factors that cause the uncertainty in TC intensity and structure. The more surface upward heat flux and water vapor flux and the lower PBL height, the faster TC development and the stronger TC intensity. 相似文献
8.
云物理过程是云和降水形成的重要环节。本文针对2011年6月23日发生在北京地区的一次大暴雨过程进行了云降水与天气特征分析,并开展了WRF模式中10种不同云微物理方案对此次暴雨强度、落区和发生时间的敏感性数值模拟试验。研究结果表明,此次大暴雨是由多单体组织、合并形成深厚的中尺度对流系统,并具有明显的短时局地特征和有利的高低空、高低纬度大中尺度天气环流形势及强烈的水汽输送条件。暴雨强度、落区和发生时间的数值模拟结果对云物理方案非常敏感。不同云物理方案对累积降水量≥50 mm和≥100 mm的暴雨模拟的ETS评分显示,只有Thompson方案对此暴雨量级的评分均为正,其他方案的ETS评分均不理想,特别是对累积降水量≥100 mm的大暴雨模拟。在小时暴雨强度和发生时间方面,Thompson方案模拟效果也较好,其次是Lin方案和WSM6方案;对区域累积最大降水量和落区的模拟方面,Thompson方案和Morrison方案模拟的最大累积降水量更接近观测值,但在落区方面,一些具有完整云物理过程的单参数方案（Lin方案、WSM6方案）模拟效果较好,但模拟的最大降水量偏小。针对暖雨的双参数方案WDM6对区域平均降水模拟较好,但对暴雨极端降水模拟较差。对造成差异的原因分析表明,不同云物理方案的差异主要体现在雪和霰的参数化方面,由于采用的粒子谱分布、密度和末速度不同,导致云中粒子间的碰并和形成过程不同,大部分云物理方案模拟的霰含量高,雪含量低。这种云微物理过程的差异会导致云动力过程的反馈作用出现明显不同,但这种反馈作用的差异主要体现在降水粒子对上升气流的拖曳作用不同。尽管云中相变潜热过程对云动力过程具有很重要的影响,但不同云物理方案在相变潜热过程和温度廓线分布方面造成的差异并不明显。因此,云物理方案中考虑合理的粒子谱分布、形态和密度变化,有利于提高暴雨的模拟效果。 相似文献
9.
在分析云微物理参数化对云结构和降水特征的影响的基础上,研究云微物理参数化过程对台风"云娜"强度与路径的影响.结果表明:云微物理过程对台风强度和路径有一定影响,其中不考虑雨水蒸发冷却效应后,比其他试验最终地面最大风速强7 m/s以上,但此时登陆地点误差最大,与对照试验偏离150 km左右.我们还从螺旋雨带结构变化及环境风切变影响角度分析台风临近登陆时强度模拟减弱的原因,发现过强的外围螺旋雨带以及环境风场垂直切变对于台风的加深、维持是不利的,他们可能会造成"云娜"临近登陆时强度的下降.不难看出,云微物理过程可以加强甚至产生外螺旋雨带,当外围雨带发展加强之后,可以引起局地辐合强度增强,从而限制了大量水汽和能量向台风内核输送,从而会导致台风强度下降.此外,外围螺旋雨带的发展,还可以从对流层中层带来干冷空气入侵行星边界层;而当入流边界层中雨水下落时,其自身的蒸发也会使周围气块温度下降;这些干冷气团在入流气流的输送下进入台风内核,从而对云墙产生了"冷侵蚀",最终引起台风强度下降.因此,减小上述两方面的模拟误差,应能改进台风"云娜"登陆过程中强度的模拟效果. 相似文献
10.
SENSITIVITY OF LANDFALLING TYPHOON STRUCTURE AND PRECIPITATION TO VARYING CLOUD MICROPHYSICAL PROCESSES 总被引：1，自引：0，他引：1
Typhoon KROSA in 2007 is simulated using GRAPES, a mesoscale numerical model, in which a two-parameter mixed-phase microphysics scheme is implanted. A series of numerical experiments are designed to test the sensitivity of landfalling typhoon structure and precipitation to varying cloud microphysics and latent heat release. It is found that typhoon track is sensitive to different microphysical processes and latent heat release. The cloud structures of simulated cyclones can be quite different with that of varying microphysical processes. Graupel particles play an important role in the formation of local heavy rainfall and the maintenance of spiral rainbands. Analysis reveals that the feedback of latent heat to dynamic fields can significantly change the content and distribution of cloud hydrometeors, thus having an impact on surface precipitation. 相似文献
11.
利用WRF模式中三种云微物理参数化方案(Lin、Eta和WSM6)对青藏高原一次强降水过程进行模拟试验,将模拟降水结果与实测资料进行对比,以评估不同云微物理参数化方案对该区域降水过程的模拟性能。结果表明:三种方案均能够模拟出此次降水天气过程的发生,但在主要降水区域和降水强度两方面仍与实测资料存在偏差;在水凝物方面,三种方案对冰粒子的模拟较接近,Lin和WSM6方案模拟的雪粒子差异较大,但霰粒子无明显差异。进一步对比分析了Lin和WSM6方案模拟的云微物理转化过程,结果表明:这两种方案都表现出了霰向雨水转化的特点。在Lin方案中,通过水汽向霰粒子凝华、霰碰并水汽凝华生成的雪粒子以及霰碰并云水这三种过程生成的霰粒子最终融化为雨水。而在WSM6方案中,一方面水汽凝结成云水,云水被雪和霰粒子碰并收集转化为霰,之后霰融化为雨水;另一方面水汽凝华为冰粒子,一部分冰转化为雪,雪直接融化为雨水或转化为霰融化为雨水,另一部分冰转化为霰,霰融化为雨水。 相似文献
12.
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
13.
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
14.
基于WRF(Weather Research and Forecasting)模式及其3Dvar(3-Dimentional Variational)资料同化系统,采用36、12、4 km嵌套网格进行快速更新循环同化和不同的微物理及积云对流参数化方案对比试验,对2011年5月8日鲁中一次局地大暴雨过程进行了研究。结果表明,快速更新循环同化地面观测资料是影响模式降水落区预报准确性的关键因素,不同的微物理和积云对流参数化方案主要影响降水强度预报。采用不同的微物理参数化方案和积云对流参数化方案进行降水预报对比试验表明,LIN方案和WSM6(WRF Single-Moment 6-class)微物理参数化方案对降水预报均较好,LIN方案降水预报较WSM6方案略强。4 km网格预报使用K-F (Kain-Fritsch)积云对流参数化方案或不使用积云对流参数化方案,预报的降水均较好。4 km网格使用旧的K-F积云对流参数化方案,预报的近地层大气风场偏弱,导致大气动力抬升作用偏弱,从而造成模式降水预报偏弱。 相似文献
15.
Idealized supercell storms are simulated with two aerosol-aware bulk microphysics schemes(BMSs),the Thompson and the Chen-Liu-Reisner(CLR),using the Weather Research and Forecast(WRF)model.The objective of this study is to investigate the parameterizations of aerosol effects on cloud and precipitation characteristics and assess the necessity of introducing aerosols into a weather prediction model at fine grid resolution.The results show that aerosols play a decisive role in the composition of clouds in terms of the mixing ratios and number concentrations of liquid and ice hydrometeors in an intense supercell storm.The storm consists of a large amount of cloud water and snow in the polluted environment,but a large amount of rainwater and graupel instead in the clean environment.The total precipitation and rain intensity are suppressed in the CLR scheme more than in the Thompson scheme in the first three hours of storm simulations.The critical processes explaining the differences are the auto-conversion rate in the warm-rain process at the beginning of storm intensification and the low-level cooling induced by large ice hydrometeors.The cloud condensation nuclei(CCN)activation and auto-conversion processes of the two schemes exhibit considerable differences,indicating the inherent uncertainty of the parameterized aerosol effects among different BMSs.Beyond the aerosol effects,the fall speed characteristics of graupel in the two schemes play an important role in the storm dynamics and precipitation via low-level cooling.The rapid intensification of storms simulated with the Thompson scheme is attributed to the production of hail-like graupel. 相似文献
16.
微物理过程参数化方案对辽宁一次暴雪的数值模拟差异分析 总被引：1，自引：0，他引：1
利用WRFv3.9.1中尺度数值模式,采用Lin、WSM6、Thompson、WDM6四种微物理过程参数化方案对2007年3月4日辽宁特大暴雪过程进行了数值模拟研究。使用61个国家级气象站降水观测资料,评估了模式对此次降水过程的模拟能力,对比分析了不同微物理过程参数化方案模拟降雪过程中相态变化和水成物空间分布的差异。结果表明:4种微物理过程参数化方案均能模拟出与CloudSat卫星反演反射率分布相接近的结果,其中Thompson方案模拟的回波顶更高,向北伸展的范围也更大,其他3种方案回波顶高均在8 km附近。4种方案对降水落区的模拟略有差异,整体来看WSM6方案对本次降水的极值中心位置,以及不同降水量级的TS评分整体都优于其他3种参数化方案。降水相态模拟与观测的对比分析发现,WSM6、Lin和WDM6三种方案均能够模拟出雨雪分界线不断南压的过程且雨雪分界线位置准确,而Thompson方案对辽宁南部地区雨转雪时间模拟偏晚。从云微物理特征上看,4种方案均能模拟出大气低层存在的雨水粒子,其中WDM6方案模拟的雨水含量明显较其他3种方案更多,Thompson方案模拟出更多的雪粒子和最少的霰粒子,Lin方案霰粒子南北范围广、伸展高度高,WSM6和WDM6两种方案模拟出较少的霰粒子,这两种方案模拟的云冰高度也更低,正是各种水成物空间分布的差异决定了不同微物理过程参数化方案对降水量和降水相态模拟的差异。 相似文献
17.
利用WRF(Weather Research and Forecast)模式及WRFDA(WRF model data assimilation system)系统,针对2017年台风“天鸽”个例通过同化雷达径向速度(Vr)和反射率因子(RF),研究水凝物控制变量的雷达资料同化对台风分析预报的影响。研究表明：雷达径向速度的直接同化有效地改进了模式初始场中台风涡旋区的中小尺度信息,分析场中产生了气旋性的风场增量,对模式背景场中的台风有显著增强作用。通过在传统控制变量中扩展针对水凝物的控制变量可有效地同化雷达反射率因子资料,对初始场的水物质进行调整,并对随后确定性预报的台风路径和强度都有一定的正效果。此外,相比没有水凝物控制变量的雷达同化试验,加入了水凝物控制变量的雷达资料同化试验降水预报效果更好。这为将我国近海的地基多普勒天气雷达用于台风初始化分析和预报提供了一定的技术支撑和保障。 相似文献
18.
采用中尺度数值模式WRFv3.5对2014年超强台风“威马逊”进行数值模拟。利用雷达、卫星、自动站逐时降水资料,对比单参数WSM6云方案和双参数WDM6云方案在模拟台风路径、强度、降水分布及水成物含量上的差异,分析雨滴粒子的谱型特征及微物理源、汇项对云中雨水含量的影响。与上海台风研究所的最佳路径数据对比显示,两方案均较好地模拟出了台风“威马逊”的移动路径,WDM6方案的整体路径误差更小;模拟的强度差异则较为显著,WDM6方案的海平面最低气压值偏高,强度偏弱。两方案模拟的累积降雨分布虽与自动站实测资料基本一致,但WDM6方案模拟的强降水概率偏高,弱降水概率偏低。两方案模拟的对流区雪、霰、雨水含量均大于TRMM卫星反演结果,且WDM6方案的对流云较多,总体雨水含量偏高;两方案均模拟出了雷达回波分布的整体特征,但眼区尺度偏大,WDM6方案在融化层以下缺少眼墙之外的弱回波区且大于39 dBz的强回波区偏多,同样显示了雨水含量（或尺度）偏大。由于WDM6方案为暖雨（云、雨水）双参数模式,对云滴活化、云雨转换及云、雨谱型有一定的改进,其能较合理地模拟出雨滴谱随台风发展的演变特征;模拟显示,云、雨滴的收集碰并及固态粒子的融化是雨水的主要源项,WDM6方案增加了云雨水自动转化率及雨水碰并云水率,导致该方案的空中雨水含量偏高,且随高度的降低快速减小;此外,由于WDM6方案使用简单的寇拉公式进行云滴活化,初始云凝结核数的变化即可造成雪、霰、云雨水含量的改变,故建议在具体大气气溶胶条件下,对方案中的云滴生成参数化过程做相应的调整。 相似文献
19.
GRAPES区域集合预报条件性台风涡旋重定位方法研究 总被引：1，自引：0，他引：1
为了在集合预报中更合理描述台风涡旋中心定位的不确定性,采用2009—2018年中国气象局和日本气象厅台风最佳路径数据,分析台风最佳路径涡旋中心定位的不确定性特征,在此基础上设计条件性台风涡旋重定位方法（Conditional Typhoon Vortex Relocation,CTVR）,构建集合成员台风涡旋中心重定位阈值条件、台风涡旋分离数学处理及涡旋重定位等数学处理过程,利用中国气象局数值预报中心区域集合预报系统（Global/Regional Assimilation and Prediciton System-Regional Ensemble System,GRAPES-REPS）对2018年西北太平洋上的3个台风（1808号“玛莉亚”、1824号“谭美”和1825号“康妮”）进行轴对称结构和轴对称+非对称结构条件性台风涡旋重定位两种方案的集合预报试验和检验评估。结果表明:（1）中国气象局和日本气象厅台风最佳路径误差平均值为13.72 km,可视为台风涡旋中心定位不确定性的合理估计值;（2）统计检验结果和典型个例分析表明,采用轴对称结构和轴对称+非对称结构条件性台风涡旋重定位方法的台风集合预报路径误差及集合预报一致性结果比较接近;（3）条件性台风涡旋重定位方法可以有效改进GRAPES-REPS区域集合预报台风路径概率预报效果,如台风路径集合预报平均误差有所减小,集合预报一致性（路径离散度与路径均方根误差比值）增大,特别是预报初期概率预报效果改进更为显著,而预报中后期改进有限;（4）通过对“玛莉亚”台风集合预报诊断分析发现,经过条件性台风涡旋重定位后,各集合成员的台风路径误差在预报初期明显减小且路径收敛,但随着预报时效的延长台风路径逐渐发散。应用条件性台风涡旋重定位方法后,台风涡旋环流与大尺度环境场仍然比较连续协调,且台风涡旋环流外的大尺度环境场具有一致性特点,最低气压误差、最大风速误差和降水预报技巧基本不变。可见,条件性台风涡旋重定位方法的应用可以提供更准确的台风路径预报不确定性信息,帮助预报员做出更准确的预报决策。 相似文献
20.
利用CIMSS微波卫星产品和多普勒天气雷达资料,分析超强台风利奇马（1909）的长时间双眼墙特征,并采用集合卡尔曼滤波方法同化雷达径向风资料,诊断利奇马双眼墙的三维结构演变特征。结果表明:在双眼墙演变过程初期,受强垂直风切变和中高层干空气入侵的影响,外眼墙对流减弱,呈非对称特征。Sawyer-Eliassen方程诊断结果显示:台风利奇马（1909）内、外眼墙次级环流之间的相互作用不明显,不同于发生眼墙替换过程的台风,其外眼墙处非绝热加热引起的下沉运动发生在内眼的眼心,内眼墙的上升运动并未受到外眼墙次级环流抑制。另外,在强垂直风切变条件下,非对称的外眼墙不能持续增强收缩并取代内眼墙,因此双眼墙结构得以长时间维持。可见,台风利奇马（1909）外眼墙的非对称结构和特殊的次级环流分布是其双眼墙能够长期维持的重要原因。 相似文献