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一次强飑线内强降水超级单体风暴的单多普勒雷达分析 总被引：21，自引：4，他引：17
文中利用位于福建建阳新一代S波段多普勒天气雷达资料和探空、地面观测资料,对2003年4月12日07-09时发生在建阳附近的一次强降水超级单体风暴进行了分析.天气分析显示,风暴发生于地面冷锋北侧、低层高湿、中等对流不稳定(1601 J/kg)和强风切变(0-5 km,22 m/s)环境,总理查逊数为16,同典型的强降水超级单体生成环境相当接近.雷达回波分析揭示,风暴发生在一强飑线系统的前沿,初期为一普通单体,随后逐渐发展成为弓状并发生分裂,分裂后风暴移动方向左侧单体逐渐减弱.而右侧的单体发展成为超级单体,持续时间约为1 h.在强降水超级单体成熟期,其移动前侧的低层反射率因子出现明显的钩状回波,中层反射率则显示在宽广的反射率高值区(>60 dBz)内存在有界弱回波区,强度大于40 dBz.沿入流方向穿过最强回波位置的反射率因子也呈现典型的回波悬垂和有界弱回波区.相应的中低层径向速度场显示在钩状回刎波附近的强降水区中存在一个强烈的中气旋,其起源于中层3.5-5 km,随后向上、下发展,最大旋转速度达到24 m/s,持续时间达1 h.由GBVTD方法分析,中气旋成熟时(08:33 UTC)轴对称环流结构显示,轴对称切向风分布在中层接近兰金涡旋模型,最大轴对称切线风位于高度4-5 km,离气旋中心约3 km,强度约20 m/s.4 km高度以下为气旋式辐合,气旋中心为上升运动.至4-7 km以旋转为主,在最大切向风半径以内为外流,以外为内流,相应的在最大风速半径处伴随较强的辐合和上升运动,7 km以上则为辐散对应的出流.此结构同经典超级单体内的中气旋结构相当一致.此外.风暴结构同Moller(1994)提出的中纬度强降水超级单体风暴的特征非常相似.但演变过程却明显不同,是由普通单体形成弓状回波,弓状回波分裂后沿移动方向右侧的单体发展成为强降水超级单体. 相似文献
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基于单多普勒天气雷达观测和双多普勒雷达反演风场,对2009年6月3日河南商丘发生的一次弓形回波的结构和演变机制进行细致分析。系统发生前的环境均具有中等对流有效位能和中等偏弱低空垂直风切变。雷达分析显示,该弓形回波从超级单体开始,经过风暴合并发展而成的经典弓形回波结构,生命史约3 h。在超级单体阶段,具有中纬度典型超级单体的低层钩状回波、中层有界弱回波区和中气旋结构。超级单体减弱后,因强降水拖曳和降水蒸发冷却,引起云内强的下沉运动,将云外干冷空气带到云内,形成中层后方入流,并在地面形成强冷池,触发干冷后向入流,回波逐渐演化成为弓形。弓形回波成熟阶段,风暴相对后向入流急流在对流区后部2 km高度加速下沉,系统前沿增强至20 m·s-1。在中层,系统后侧南北两端形成气旋和反气旋涡旋对,此中层涡旋对后向入流强度贡献约20%。在系统前缘低层（1.5 km）、出流边界附近,存在一气旋式涡旋。受后向入流急流和此低层涡旋的共同作用,在顶点附近产生超过32 m·s-1的最大地面相对风速。至减弱期,低层出流扩展至系统前方20 km,截断了低层暖湿入流,使其快速减弱。 相似文献
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南海台风Vongfong(2002)登陆前后内核结构和近海加强原因的数值模拟研究 总被引：4，自引：1，他引：3
利用6 km细网格区域的显式模拟结果分析了Vongfong(2002)的内核结构;对Vongfong近海加强的动力学机制进行了研究.结果表明:(1) 轴对称性结构中,Vongfong最大风速半径(RMW)在强盛期随高度递减.Vongfong在近海时,低层最强的流入在其移行的前方,而流出区在其后方.这些特征与大西洋飓风和西太平洋台风相反.(2) 动力场和热力场都有明显的不对称结构.在强盛期,对流西北强、东南弱;强对流云带与最大风速区的位置一致.在加强期,低层西冷东暖、中高层西暖东冷;到强盛期,低层和中高层都有明显的暖心结构.(3) 中纬度中上层冷低压系统和台风的相互作用是Vongfong近海加强的重要原因.①由于冷低压系统外围的冷空气从西北侧进入台风的中层,低层有暖湿空气配合,使得位势不稳定能量增加,对流发展.②因为冷低压中心的下沉气流正是二级环流的下沉支,冷低压南移填塞,台风近海加强.两个方面最终通过CISK(第二类条件不稳定)机制来实现. 相似文献
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一次飑线过程多普勒雷达资料分析 总被引：3，自引：0，他引：3
利用济南CINRAD/SA多普勒雷达产品,针对2006年7月5日飑线天气过程,分析回波发展演变、流场结构,讨论外流边界、强下沉气流与大风的关系,分析组合反射率因子、垂直液态含水量、中气旋产品特征.结果发现,飑线过境时风速出现两个极大值,一个出现在外流边界影响时段,另一个发生在强回波下沉气流影响时段;在横槽南下过程中,飑线后部强入流不断补充,前侧暖湿气流沿着后部入流爬升,不断产生新的单体,使得风暴得以维持发展;在垂直流场结构上表现为前侧暖湿气流倾斜上升,然后主体部分向后倾斜,后部有冷空气注入,形成下沉气流,下沉气流在地面附近辐散,与前侧入流形成低层阵风锋,是造成地面破坏性大风的主要因素.在水平流场结构上表现为低层存在气流辐合上升运动,中层有气旋性旋转气流,风暴高层为辐散气流.飑线消散阶段后期中层出现MARC,带来大风天气,而同时伴有冰雹天气的风灾产生在飑线达到最强至开始减弱的时段.当回波强度≥50dBz,且垂直液态含水量≥35kg·m-2,当有中气旋时,有利于产生冰雹和大风天气;外流边界的出现,反映了强对流回波后部下沉气流较强,是灾害性大风的前兆. 相似文献
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2019年8月16日渤海北部沿岸出现了一次冷涡背景下的EF1级龙卷。利用营口S波段双偏振多普勒天气雷达探测资料、5 min间隔的地面自动气象站观测资料、盘锦风廓线雷达探测资料及ERA5再分析资料,研究了该龙卷风暴产生的环境条件、龙卷风暴结构特征及龙卷形成的可能物理过程。结果表明:此次龙卷过程发生在500 hPa冷涡主体控制下,低空位于“利奇马”台风残涡西侧水汽输送带内,环境条件表现为弱的风垂直切变和强低层热力不稳定。营口双偏振雷达位于距龙卷发生地15 km处,探测到产生龙卷的微型超级单体钩状回波、下沉反射率核心（DRC）、弱回波洞（WEH）、龙卷残片特征（TDS）等结构。处于消亡阶段雷暴的阵风锋出流向西传播,而营口附近海风锋缓慢东移,两条边界层辐合线相遇加强,在水平切变不稳定的作用下,辐合线上有γ中尺度涡旋形成。辐合线相遇造成的辐合抬升、低层强热力不稳定导致的环境正浮力以及中层中气旋扰动低压共同作用产生强上升气流,γ中尺度涡旋与上升气流叠置,强拉伸作用增强了垂直涡度,可能是低层微尺度气旋形成的关键机制。微尺度气旋直径收缩至最小伴随旋转速度达到最大时刻,对应龙卷生成,中层中气旋与微尺度气旋分离导致龙卷消亡。 相似文献
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应用Qiu等提出的两步变分反演法,由厦门、长乐两部雷达观测资料反演0604号台风"碧利斯"登陆福建霞浦前的风场,并利用反演的水平风场检验几种常用的台风涡旋模型对此次台风的合理性,以期对雷达资料应用于台风过程分析和模拟有更进一步的认识。结果表明,两步变分法可以较好地反演出台风的水平、垂直风场特征,水平风场呈现不对称性且有明显的偏心结构,流场随高度表现出漏斗形特征,垂直风速与水平流场对应较好,台风中心有下沉气流,外围有上升气流。通过对台风物理量的分析发现,此次台风过程存在以最大风速半径随高度向外倾斜的主环流圈和低层向中心流入,高层向外流出的次环流圈。利用反演的水平风场对常用的对称风场涡旋模型进行了验证,发现在最大风速圈内取Rankine模式,最大风速圈外取Chen3模式对此次台风过程拟合较好。 相似文献
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T-TREC方法反演登陆中国台风风场结构 总被引：3，自引：2，他引：1
在传统的基于天气雷达反射率因子的相关方法跟踪回波运动(TREC)技术的基础上,本研究发展出适用于台风环流反演的T-TREC方法.同传统的TREC技术相比,T-TREC根据台风环流呈逆时针方向旋转的特征,利用雷达观测资料客观选取台风中心,选取扇形网格单元,在以台风中心为原点的极坐标系下进行逆时针方向同波追踪.同时,该方法也利用雷达径向风资料客观选取切向的搜索范围并建立风场相关矩阵,以减少主观设定搜索区域造成的误差.通过利用中国新一代天气雷达网(CINRAD WSR-98D)观测的登陆台风桑美(0608)资料对方法进行验证,结果表明T-TREC方法可以更加准确估计强台风环流,反演的径向风平均误差小于4 m/s.其中径向风信息的引入明显提高了反演风场精度,特别是改善了在眼墙区因回波结构较均匀造成的风场低估.当台风靠近陆地时,因地物回波以及台风环流与地形相瓦作用激发对流的影响,使得低层风场反演误差增加.文中也探讨了台风中心、搜索网格单元大小等因子对反演精度的影响,结果显示,反演结果对于中心定化比较敏感,中心位置偏移4 km将造成反演的径向风平均误差增加约10%.而搜索单元大小对反演结果影响和台风尺度相关,若台风尺度较小,则较小的搜索单元反演效果较好. 相似文献
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为研究降雹超级单体风暴的三维结构特征,利用厦门、龙岩、梅州3部新一代天气雷达（CINRAD/SA）基数据,采用基于动态地球坐标系的双雷达和三雷达三维风场反演技术,分析了2016年4月8日傍晚福建省南部漳州地区出现的一次冰雹过程的回波强度、三维风场及相关物理量分布变化。主要结果为：（1）冰雹云初生、发展阶段,低层水平流场出现气旋性辐合,云体内部形成较强的上升运动。（2）冰雹云强盛阶段,回波顶高度达16 km,其中大于60 dBz的回波高度由5.3 km发展至9 km,最强回波达74.5 dBz,伴随出现最长达25 km的三体散射长钉回波和32.7 km的旁瓣回波。低层水平维持气旋性流场的同时,高层出现反气旋性流场。4-8 km高度内,大于20 m/s的强上升气流持续近37 min。最大垂直速度达51.06 m/s,出现在超级单体悬垂部（约7.5 km高度处）。（3）降雹时段,出现明显的下沉气流。降雹超级单体的三维流场结构表现为：风暴移向前沿低层气旋性气流进入风暴后逐渐倾斜上升,到达风暴顶形成反气旋性气流,并逐渐向下形成下沉气流。（4）系统减弱阶段,出现系统性下沉气流,强回波底及地。双雷达和三雷达能较好地反演降雹超级单体的三维风场精细结构,有助于加深对冰雹云结构的认识进而提高冰雹预报能力。 相似文献
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In this study, the kinematic and precipitation structures of a mesocyclone associated with a hook echo were analyzed using single Doppler radar data. The mesocyclone was embedded in a mesoscale convective rainband near northern Taiwan coastline on 10 September 2004. The synoptic environment was
characterized by a moderate convective available potential energy (CAPE) and a moderate ambient vertical shear from surface to 5 km.In addition, a pronounced low-level mesoscale shear/convergence
zone, which resulted from the interaction of two tropical depressions, was also identified in the northwest coast of Taiwan,providing a favorable dynamic condition for the development of the mesocyclone.
Analyzing single Doppler dipole signature shows that this mesocyclone formed initially at low levels, then deepened and strengthened rapidly into mature stage with the vertical depth exceeding 8 km. The diameter of the mesocyclone decreased with the height at the time of vortexgenesis, and then evolved into columnar structure accompanied with the broader diameter in middle layer. The mesocyclone lasted for about 2 h. The Ground-Based Velocity Track Display (GBVTD) method was applied to retrieve the axisymmetric circulation of the mesocyclone. The GBVTD-derived primary circulation showed the radius of maximum wind (RMW) of the mesocyclone was about 5--6 km and varied from inward tilting to outward tilting with time. The axisymmetric radial wind field was initially characterized by a low-level inflow inside the RMW and outflow outside the RMW, respectively. The strongest reflectivity was associated with a stronger updraft near the RMW, and a weak downdraft was located at the center of the mesocyclone.Subsequently the downdraft and reflectivity near the mesocyclone
center strengthened obviously, accompanied with the low-level outflow, strong updraft as well as high reflectivity extending outside the RMW. The relative tangential wind initially exhibited a wavenumber 1 asymmetric structure with the maximum wind region at the left portion of the meso cyclone and shifted counterclockwise with height. The axisymmetric tangential wind strengthened and reached its maximum intensity with a value about 20 m s-1 at z=1 km. After that the axisymmetric tangential
wind decreased rapidly, meanwhile the wave-1 asymmetric structure redeveloped with the maximum wind at the left-front of motion. In summary, the evolution and structure of the mesocyclone is similar
to that observed within a non-supercell mesocyclone. It is worth to mention that the axisymmetric circulation characteristics of the mesocyclone at its mature stage are very similar to those
observed in a mature typhoon. However, there are significant differences, i.e., the size is much smaller, the lifetime is much shorter, and the downdraft in the center is produced by precipitation instead of compensating subsidence. 相似文献
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Single-Doppler Radar Observations of a High Precipitation Supercell Accompanying the 12 April 2003 Severe Squall Line in Fujian Province 
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下载免费PDF全文 In this study,single Doppler radar data were used to examine the structure and evolution of a high precipitation(HP) supercell embedded in a cold front near Jianyang,Fujian Province on 12 April 2003.The synoptic environment was characterized by high humidity at low levels,moderate CAPE(convective available potential energy;1601 J kg~(-1)),moderate wind shear(22 m s~(-1) in 0-5 km),and veering of the horizontal winds with height,similar to those HP supercells previously observed in midlatitudes.In additio... 相似文献
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Firstly, typical features of a supercell, which occurred in Guangzhou on August 11, 2004, are discussed by using the new generation weather radar data. V-notch, finger-echo, weak echo region, overhang and echo-wall are observed from reflectivity products. A vertical cross section of the radial velocity is made along the direction of the low-level inflow and across the maximum reflectivity core, which displays a part of strong updraft and downdraft. Secondly, a 3-D convective storm model is used to simulate the supercell. The maximum reflectivity and the core thickness of the simulated radar echo are 75 dBz and 14km, respectively. These values are more than the counterparts that are detected by radar. The reason is that attenuation is not calculated in the model. The wind field structure is also given when the storm is the strongest. Divergence, caused by thunderstorm outflow, is in the low level. In the middle and high level, convergence is dominant, but the plume is not simulated at the top. Finally, the evolution of the simulated vertical motion is documented. The interaction between the environmental wind and the updraft, which is formed by the convergence on the ground at the beginning, makes the storm stronger. Then, downdraft occurs and grows. When it becomes dominant, the supercell collapses. 相似文献
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Chanh Q. Kieu 《Meteorology and Atmospheric Physics》2012,115(1-2):47-56
The radius of the maximum tangential wind (RMW) associated with the hurricane primary circulation has been long known to undergo continuous contraction during the hurricane development. In this study, we document some characteristic behaviors of the RMW contraction in a series of ensemble real-time simulations of Hurricane Katrina (2005) and in idealized experiments using the Rotunno and Emanuel (Mon Weather Rev 137:1770–1789, 1987) axisymmetric hurricane model. Of specific interest is that the contraction appears to slow down abruptly at the middle of the hurricane intensification, and the RMW becomes nearly stationary subsequently, despite the rapidly strengthening rotational flows. A kinematic model is then presented to examine such behaviors of the RMW in which necessary conditions for the RMW to stop contracting are examined. Further use of the Emanuel’s (J Atmos Sci 43:585–605, 1986) analytical hurricane theory reveals a connection between the hurricane maximum potential intensity and the hurricane eye size, an issue that has not been considered adequately in previous studies. 相似文献
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Previous numerical simulations have focused mainly on the mesoscale structure of the principal rainband in tropical cyclones with a relatively coarse model resolution. In this study, the principal rainband was simulated in a semi-idealized experiment at a horizontal grid spacing of 1/9 km and its convective-scale structure was examined by comparing the convective elements of the simulated principal rainband with previous observational studies. It is found that the convective scale structure of the simulated principal rainband is well comparable to the observation. The azimuthal variations of the convective scale structure were examined by dividing the simulated principal rainband into the upwind, middle and downwind portions. Some new features are found in the simulated principal rainband. First, the overturning updraft contains small-scale rolls aligned along the inward side of the outward-leaning reflectivity tower in the middle portion. Second, the inner-edge downdraft is combined with a branch of inflow from the upper levels in middle and downwind portions, carrying upper-level dry air to the region between the overturning updrafts and eyewall, and the intrusion of the upper-level dry air further limits the altitude of the overturning updrafts in the middle and downwind portions of the principal rainband. Third, from the middle to downwind portions, the strength of the secondary horizontal wind maximum is gradually replaced by a low-level maximum of the tangential wind collocated with the low-level downdraft. 相似文献
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采用分钟级加密自动气象站观测资料,盐城、淮安和岳阳、荆州雷达探测数据,以及欧洲中期天气预报中心（ECMWF）高分辨率的ERA-Interim全球再分析数据,对比分析了2016年6月23日江苏阜宁龙卷灾害和2015年6月1日湖北监利下击暴流大风灾害的环境特征与超级单体的结构特征。结果表明:（1）两次强对流大风灾害发生在相似的低空环流背景下:风灾发生在低空急流出口区左侧的暖区内、850 hPa低涡中心东侧6—7个经距的位置;环境大气的对流有效位能大于2000 J/kg。但是风灾的类型不同,江苏阜宁大风灾害主要由超级单体龙卷造成,监利“东方之星”沉船事故主要是超级单体触发的下击暴流造成。短时强降水中心与风灾中心的相对位置不同:阜宁龙卷移动方向的左侧伴随着最强短时降水;湖北监利沉船事件发生期间,风灾中心与短时强降水中心基本重合。鉴于不同性质的对流大风位置与超级单体母体的中心位置对应关系上存在差异,通过比较地面观测的瞬时大风与瞬时强降水中心的相对位置将有助于区分强对流大风的性质。（2）环境风垂直切变强度对对流风暴结构、发展、维持有重要影响:阜宁龙卷发生时,其上空0—6 km风垂直切变达4×10-3 s-1,超级单体有明显的向前倾斜结构,形成有界弱回波区;而监利强对流沉船位置0—6 km风垂直切变只有2.3×10-3 s-1左右,风暴单体中的上升气流近乎于垂直。阜宁超级单体中气旋,首先出现在0—1.5 km风垂直切变和0—3 km风暴相对螺旋度带状大值区,在向抬升凝结高度更低的环境移动过程中,其底部不断下降,形成龙卷;而在监利沉船区,中低层风切变和风暴相对螺旋度相对要弱得多,对应风暴单体中的中气旋强度、持续性较弱,中气旋底部高度维持在1.6 km左右。（3）环境湿度垂直结构特征不同可能是风暴单体形成不同类型灾害大风的重要环境因子。监利下击暴流造成的风灾发生时,在地面气温迅速下降过程中,气压变化呈现快速跳升又快速下降的“尖锥”形,气压峰值比降水峰值提前4 min出现。它与对流层中高层环境大气中较为深厚的干空气卷入对流风暴中造成水物质强烈蒸发、冷却过程有关。而阜宁风灾过程中,环境大气中层仅存在非常浅薄的干层,加之低层较为深厚的饱和大气环境,对应的地面冷池效应相对较弱。 相似文献
17.
An explicit simulation with a fine mesh at intervals of 6 km is used to explore the inner-core
structures of Vongfong (0214). The dynamic mechanism for the inshore strengthening of Vongfong is
examined. It is found as follows. (1) The radius of maximum wind of the axisymmetric structures of the
typhoon decreased with height during its mature stage. When Vongfong was inshore, the strongest
low-layer inflow located in front of it and the outflow was to the rear of it, which was just reversed from
the Atlantic hurricanes and other Pacific typhoons. (2) The dynamic and thermodynamic fields were highly
asymmetric in structure. Convection was stronger in the northwest quadrant of the typhoon than in the
southeast; the strongest convective cloud bands were consistent with the maximum wind region. During its
strengthening stage, it was cold west of and warm east of the eye in the lower layer but warm in the west
and cold in the east of the mid-upper layer. During its mature stage, a warm-core structure was evident in
the lower and middle-upper layer. (3) The interactions between a mid-latitude cold low in the
middle-upper troposphere and the typhoon were responsible for the latter to strengthen inshore. Firstly, the
outer circulation of the cold low entered the typhoon from the middle troposphere when an outer cold
airflow from the cold low flowed into the northwest quadrant of the typhoon so that geopotentially instable
energy increased and convection developed. Secondly, the downdraft in the cold low was just the
corresponding branch of the secondary circulation of the typhoon system; when the cold low weakened
while moving south, the typhoon strengthened inshore. Due to the CISK mechanism, these two phenomena
might be realized. 相似文献
18.
观测发现热带气旋(TC)眼墙附近低层(3 km以下)存在着强烈的上升运动,严重威胁低空观测飞机的安全,由于对实际TC观测的样本非常有限,目前对极端上升运动(大于10 m/s)的了解不多。通过三个水平分辨率自次千米(333 m)至次百米(37 m)大涡数值试验模拟眼墙附近低层上升运动的分布特征。结果表明,TC眼墙附近的最强上升运动主要分布在眼墙处最大风速半径(RMW)内侧,并且主要出现在台风眼墙强对流的一侧。对比不同试验发现,在大涡试验中,随着模式水平分辨率的提高,模式可以模拟出更强的上升运动,且极端上升运动最大频数的分布高度随着水平分辨率的提高而降低。研究表明,与现有观测结果比较,当大涡试验水平分辨率到达111 m时,可以模拟出与实际观测比较相似的极端上升运动空间分布和强度。 相似文献
19.
为研究雹暴结构和大冰雹的形成机制,利用潍坊CINRAD/SA新一代天气雷达、青岛S波段双偏振多普勒天气雷达探测数据,结合探空、地面气象观测站观测和实地冰雹调查资料,对2019年8月16日发生在山东诸城的一次罕见强雹暴过程的天气背景、风雹灾害、雷达回波演变、雹云结构及大冰雹形成机制进行分析。结果表明,受冷涡天气系统影响,鲁中山区、鲁东南地区低层暖湿、高层干冷,0—6 km高度风矢量差为30.3 m/s,十分有利于强雹暴的发展。雹云发展迅速,历经发生、跃增、酝酿、降雹和消亡等5个阶段,在发生阶段即观测到中气旋、有界弱回波区等结构并不断增强,长时间维持;降雹阶段的雹云具有典型的有界弱回波区—悬垂回波—回波墙和“S”型水平流场等特征,有界弱回波区与旋转上升气流和水平速度为0的“0线”结构相关联,“0线”穿过悬垂回波和有界弱回波区顶部强回波区,指向雹云对流上冲云顶,具有特定的成雹功能;强降雹时段,雹云有界弱回波区北侧回波墙及其上方强回波区的水平反射率因子大于60 dBz,对应的差分反射率因子大多为?1—0 dB,表明为大冰雹的聚集区。依据对成熟阶段雹云雷达回波形态、径向速度和三维风场的分析,给出了实例雹云内主上升气流框架和具有成雹功能的“0线”结构示意图,有助于理解“0线”结构在大雹循环增长中的可能作用机理。 相似文献