共查询到19条相似文献，搜索用时 15 毫秒
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利用NCEP再分析资料、探空资料、闪电定位资料和南京、常州多普勒雷达资料,通过对比分析南京2012年2月22日春季雷暴和2011年8月10日夏季雷暴两次过程,研究不同季节影响雷暴发生的大气结构以及强弱雷暴地闪特征的差异。结果表明:风矢位温(V-3θ)图揭示的大气动力热力水汽特征能够为雷暴的潜势预报提供先兆信息。两者相较而言,春季雷暴的动力抬升作用明显;夏季雷暴主要由热对流引起,对流层上层的动力抽吸作用不明显。春季弱雷暴正地闪在总地闪中所占比例较高。无论春季弱雷暴还是夏季强雷暴,地闪落点与辐合区对应关系明显,且地闪的落点也与雷达反射率因子有较好的对应关系:地闪主要分布在强回波区(大于40 d Bz)及其外围区域。但在较强雷暴云的发展阶段,地闪多发生在风暴体伸展方向的一侧,具有引导雷达回波移动的作用,夏季强雷暴地闪簇集在垂直风切变区域。 相似文献
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针对2006年7月31日发生于陕西省的强雷暴灾害性天气过程,对闪电定位监测资料、多普勒雷达资料以及自动站降水资料之间的相关特征进行了分析。研究表明：局地性短时暴雨天气发生前,地闪频数有一个“跃增”;短时暴雨发生时,地闪频数较高,正闪与负闪的比例较低,各区最大正负闪比例仅6．7％,强度较大的地闪多分布于地闪密集区。空间上,地闪密度大值区与短时暴雨中心落区基本一致;时间上,地闪最大频率出现比短时强降水的发生提前30min以上,说明地闪最大频率的出现对强降水发生有指示意义。通过地闪与不同仰角多普勒雷达基本反射率回波的叠加分析,发现1．5°仰角上二者具有很好的对应关系,地闪演变对30dBz以上雷达回波的强度和移动演变有引导作用。 相似文献
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杨美荣 《沙漠与绿洲气象(新疆气象)》2020,14(2):90-97
利用地闪探测系统资料、多普勒雷达资料和卫星云图资料,分析了河南省一次雷暴过程的地闪特征及其与云体结构的关系,结果表明:在雷暴整个生命史中负地闪占据主导地位,占总地闪的99.5%;地闪平均强度与地闪频次存在负相关关系;初次地闪出现时雷暴强度迅速增强;40 d BZ强回波顶高、6 km高度50 dBZ强回波面积以及5 km高度之上50 dBZ强回波体积与地闪频次存在明显的正相关关系,在整个雷暴过程中的相关系数分别为0.80、0.91和0.93,而在雷暴不同发展阶段3种雷达参量与地闪频次的相关性有不同的变化趋势;地闪一般分布在6 km高度雷达回波≥40 dBZ、云顶亮温≤200 K的区域,有助于识别强对流区。 相似文献
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基于2014—2015年5—9月西藏那曲地区多普勒天气雷达数据,结合地闪观测数据,识别雷暴单体样本,统计分析了地闪位置附近的雷达回波分布特征,并研究了高原雷暴的雷达参量与地闪频次的相关关系。结果表明:那曲地区地闪发生位置附近的雷达最大反射率因子呈正态分布,峰值分布区间集中于34~41 dBZ。发生地闪位置附近的20 dBZ回波顶主要集中于11~15 km高度,30 dBZ回波顶高分布的峰值区间则为8.5~12 km。分析表明:表征局地雷暴对流发展强度的雷达参量与地闪频次之间一对一的相关关系较差,但相关性随地闪频次增加而增强。基于雷达参量分段统计得到的对应分段平均地闪频次与雷达参量之间表现出较强相关关系,体现了宏观上闪电活动强度与雷暴发展强度之间的正向关系。其中,基于原始数值进行区间划分的强回波（组合反射率因子不小于30 dBZ）面积与平均地闪频次的线性相关系数达0.75,基于对数数值区间划分的7~11 km累积可降冰含量的对数值和地闪频次的线性相关系数达0.95。文中对比了多个雷达参量和地闪频次线性拟合与幂函数拟合结果,整体上幂函数拟合略好于线性拟合。 相似文献
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利用湖北省2013—2018年6—8月ADTD闪电探测数据对该地区的闪电活动进行特征分析后发现, 地闪密度和日变化特征与地形密切相关, 其中, 闪电密度高值区出现在海拔500~1 500 m的中尺度山脉向平原的过渡地带以及山脉之间的平原(河谷)地区; 山区的地闪集中在午后至傍晚时段, 具有明显的单峰特征, 平原的地闪日变化相对平缓, 虽然主峰值同样出现在午后, 但夜间地闪活动依然活跃。基于2015—2016年6—8月逐6 min雷达组合反射率拼图产品和地闪资料挑选了94例伴有显著闪电活动的雷暴系统个例, 经统计分析后发现, 雷暴系统的初次地闪、峰值地闪和末次地闪均集中出现在13:00—18:00, 其中, 山区雷暴的地闪持续时间较短, 地闪频数峰值较小; 平原雷暴的地闪持续时间更长, 地闪频数峰值也更大; 山麓雷暴的特征则介于两者之间。利用ERA-Interim再分析资料进行成因分析后可知, 地形强迫和局地热力不稳定是影响湖北山区夏季闪电密度分布和日变化特征的关键因子。 相似文献
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为提高江苏省地区雷暴监测预警能力，利用S波段双偏振多普勒天气雷达雷暴探测回波资料和闪电定位资料对江苏省2014年7—8月的夏季雷暴进行特征研究，研究了雷暴反射率核心区域的演变特征、不同温度层反射率因子与地闪频数随时间的相关性问题和雷暴发展过程云内粒子的演变特征。研究结果表明：在雷暴成熟之前，雷暴的反射率因子核心区域的强度、高度和云顶高度不断增加，以及对流发展旺盛，当雷暴成熟之后，雷暴的强反射率因子核心的强度和对应高度就会不断降低，雷暴将趋于消散；雷暴能够发生闪电的主要特征是40 dBZ回波顶高度要高于0℃温度层高度；雷暴中闪电的产生和霰粒子有着密切的联系，尤其是湿霰粒子。 相似文献
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冀南地区一次强雷暴过程分析 总被引：4，自引：1，他引：3
利用MTSAT卫星云图、雷达回波、常规天气资料和闪电资料,对2007年7月18日邯郸地区强雷暴天气过程进行了综合分析,结果表明:雷暴云的发展与水汽通量、不稳定区有较好的对应关系.雷暴初始阶段,地闪以负闪为主,正闪较少;随云系发展,闪电密度增大;云系发展成熟阶段,正闪密度变化不大,负闪密度明显减小.雷暴云回波强度＞36 dBz,就有闪电发生,且强回波区与闪电区一致. 相似文献
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应用雷电定位系统和高空观测资料并结合雷达回波资料, 对广州地区雷暴过程云-地闪特征进行分析, 并就有、无云-地闪出现的两组不同对流天气过程的环境条件进行了比较研究。结果表明:广州地区的雷暴过程以负的云-地闪为主, 负云-地闪所占比例在90%以上。云-地闪发生频率与雷暴系统强度演变有直接联系, 对于同一系统来说, 随着系统回波强度的增强, 云-地闪发生的频率也增高。但不同系统中, 云-地闪发生频率有很大不同, 回波强(弱)的对流系统并不意味着云-地闪发生的频率就高(低)。有云-地闪记录的对流天气过程具有更大的垂直切变、更高的相对风暴螺旋度以及更多的对流抑制能量, 云-地闪现象更易于出现在更加有组织和更强的对流系统中。研究还发现广州及周边城市区域对雷暴系统回波强度及云-地闪现象可能有影响, 两个典型个例分析表明, 雷暴系统移经城市区域时回波强度减弱, 云-地闪发生频率减小, 雷暴移过城市区域后, 强度可重新加强, 云-地闪发生频率增大。 相似文献
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低纬高原一次飑线过程的地闪演变特征分析 总被引：1，自引：0，他引：1
利用雷电定位资料、多普勒雷达资料和FY-2E红外卫星资料,分析了滇西南一次典型飑线过程的地闪变化特征。结果表明,这是一次由切变线云带内的对流单体与台风外围对流单体合并形成的典型飑线过程。在飑线发展初期,负地闪占主导地位,地闪频数在波动中缓慢增加;在飑线成熟阶段,地闪频数较高,负地闪频数达到最大峰值前10～15min,正地闪出现最大峰值;在飑线减弱阶段,地闪频数急速下降,正地闪所占比例急剧增加,当正地闪所占比例超过地闪总数的8%以上时,地闪活动开始呈减弱特征。负地闪主要发生在强对流区(>40dBz),对应着径向速度场上的辐合区,密集的正地闪发生在飑线成熟阶段,对应着辐合区附近>40dBz的强回波区域,稀疏的正地闪发生在强回波外围的云砧或稳定性降水部位。在飑线整个发展阶段,-10℃,-20℃层高度上雷达回波强度的每一次跳跃变化都对应着地闪频数的跳跃发展,且-10℃和-20℃层高度上雷达回波强度总在地闪频数变化之前6～30min。负地闪集中出现在-92～-90℃和-76～-74℃的云区,而正地闪集中发生在-90～-60℃的云区。 相似文献
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Lightning and Doppler radar observations of a squall line system 总被引：2，自引：0，他引：2
A typical squall line with damaging wind and hailstones occurred on 28 April 2006 in Shandong Province, middle eastern China, and caused great economic loss. The characteristics of cloud-to-ground lightning (CG) in the squall line were studied in detail by combining the data from the ground-based CG location network, two Doppler radars and the Lightning Imaging Sensor on the TRMM satellite. Results show that positive CG flashes accounted for 54.7% of the total CG flashes. During the initial developing stage, the CG flash rate was lower than 0.5fl min− 1 and most of the CG flashes were positive. It increased significantly, up to 4.5fl min− 1, along with the rapid development of the squall line, and the percentage of positive CG was more than 75% during this period. The CG flash rate began to decrease but the percentage of negative CG flash increased gradually and exceeded that of positive CG during the mature and dissipating stages. Positive CG flashes tended to occur on the right flank and negative ones on the left flank. Strong wind at the surface occurred in or near the regions with dense positive CG flashes. Almost all positive CG flashes occurred near the strong radar echo regions, in the front parts of the squall line. However, the negative CG flashes almost exclusively occurred in the regions with weak and uniform radar echoes. The total flash rate in the storm was very high, up to 136fl min− 1, and its ratio of intracloud flashes (IC) to CG flashes was 35:1. Dense positive CG flashes corresponded to updraft regions, they did not occur in the core of the updraft, but just behind and close to the main updraft instead. The rear inflow jet, between 3 and 6 km, played an important role in the formation of the bow echo and very strong wind at surface. The CG distribution features in the squall line were obviously different from that of an ordinary MCS. The charge structure could be roughly described as an inverted charge structure. 相似文献
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The research indicates that there is a positive correlation between the negative CG flash rate and the area of radar echo with its reflectivity being equal to or greater than 30 dBz in the mesoscale convective system in Beijing area.A maximum of the positive CG flash rate exists at both the initial and the dissipating stages.The CG flashes are usually located near but not within the high reflectivity center.The negative flashes are associated with.the positions of the updraft region,and with the regions of wind convergence and wind shear.Generally,the negative CG flashes are concentrative and the positive ones are dispersive. 相似文献
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The research indicates that there is a positive correlation between the negative CG flash rate and the area of radarecho with its reflectivity being equal to or greater than 30 dBz in the mesoscale convective system in Beijing area.A max-imum of the positive CG flash rate exists at both the initial and the dissipating stages.The CG flashes are usually locatednear but not within the high reflectivity center.The negative flashes are associated with.the positions of the updraft re-gion,and with the regions of wind convergence and wind shear.Generally,the negative CG flashes are concentrative andthe positive ones are dispersive. 相似文献
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OBSERVATION AND MODEL ANALYSES OF POSITIVE CLOUD-TO-GROUND LIGHTNING IN MESOSCALE CONVECTIVE SYSTEMS* 
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下载免费PDF全文 Yan Muhong Guo Changming Qie Xiushu Ge Zhengmo Zhang Guangshu 《Acta Meteorologica Sinica》1992,6(4):501-510
The analyses of spatial and temporal characteristics of positive cloud-to-ground(CG) lightning for four mesoscale convective systems and two severe local convective systems in 1989 and 1990 show that positive CG flash rate usually has two peak values.The major peak occurs during the developing stage of the storm and most of the positive CG flashes originate at the lower part of the storm.The minor occurs during the dissipative stage of the storm and most of the positive CG flashes originate at the upper part of the storm,especially in the region of the wind divergence in the storm anvil.The positive CG flash rate is almost an order of magnitude larger in the developing stage than in the dissipative stage.The appearing time of the peak of negative CG flash rate is in accordance with that of the valley of positive CG flash rate.The higher the intensity of the radar echo,the higher the positive CG flash rate.Most of the positive CG flashes occur when the weak echo area is larger,and mostly originate in the region where the radar echo intensity is about 10dBz and in the back region of the moving storms.The spatial distribution of the positive CG flashes is much more dispersive than that of the negative.The mesoscale analysis reveals a bipolar lightning pattern.The mean bipole-length reaches its minimum during the mature stage of the storm and reaches the maximum during the developing stage of the storm.The vertical distribution of the charge density is calculated by a one-dimensional charging model.Then,we discuss the producing condition of the positive CG lightning and forming cause of charge structure mentioned above. 相似文献
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OBSERVATION AND MODEL ANALYSES OF POSITIVE CLOUD-TO-GROUND LIGHTNING IN MESOSCALE CONVECTIVE SYSTEMS 总被引：1，自引：0，他引：1 下载免费PDF全文
下载免费PDF全文 Yan Muhong Guo Changming Qie Xiushu Ge Zhengmo Zhang Guangshu Lanzhou Institute of Plateau Atmospheric Physics Academia Sinica Lanzhou 《Acta Meteorologica Sinica》1992,(4)
The analyses of spatial and temporal characteristics of positive cloud-to-ground(CG)lightning for four mesoscaleconvective systems and two severe local convective systems in 1989 and 1990 show that positive CG flash rate usuallyhas two peak values.The major peak occurs during the developing stage of the storm and most of the positive CGflashes originate at the lower part of the storm.The minor occurs during the dissipative stage of the storm and most ofthe positive CG flashes originate at the upper part of the storm,especially in the region of the wind divergence in thestorm anvil.The positive CG flash rate is almost an order of magnitude larger in the developing stage than in thedissipative stage.The appearing time of the peak of negative CG flash rate is in accordance with that of the valley of pos-itive CG flash rate.The higher the intensity of the radar echo,the higher the positive CG flash rate.Most of the positive CG flashes oc-cur when the weak echo area is larger,and mostly originate in the region where the radar echo intensity is about 10dBzand in the back region of the moving storms.The spatial distribution of the positive CG flashes is much more dispersivethan that of the negative.The mesoscale analysis reveals a bipolar lightning pattern.The mean bipole--length reaches itsminimum during the mature stage of the storm and reaches the maximum during the developing stage of the storm.The vertical distribution of the charge density is calculated by a one-dimensional charging model.Then,we discussthe producing condition of the positive CG lightning and forming cause of charge structure mentioned above. 相似文献
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华北一次强对流天气系统的地闪时空演变特征分析 总被引：8，自引：3，他引：5
利用地面雷电探测网,多普勒天气雷达和常规天气资料,分析了2005年8月1日发生在山东北部的一次具有前部对流线,后部大范围层状云降水(LLTS)的典型中尺度对流系统(MCS)的闪电活动演变特征。结果表明:整个过程中负地闪占主导地位,最高频数达到260次/5min;与负地闪比较,正地闪呈现不活跃状态。负地闪主要落在>40 dBz的强回波区内部及其边缘区域,而正地闪则分布在前部云砧和后部层状云降水区内。对地闪位置与回波强度的进一步对比分析发现,45~55 dBz的回波是最有利于地闪发生的区域,回波强度低于这一区域,随着回波强度的增大,地闪活动呈递增趋势,地闪频数在50~55 dBz的回波区域内达到峰值,>55 dBz的回波区域内地闪频数明显降低。 相似文献
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南京一次雷雨的闪电特征与多尺度资料分析 总被引：2，自引：2，他引：2
为探究闪电与其他气象要素之间的关系及可预报性,本文利用探空资料、多普勒天气雷达资料、闪电定位仪资料、卫星云图资料和地面自动气象站资料,对2009年7月7日南京雷雨天气进行多尺度分析.结果表明:暴雨过程中负地闪始终占较大比例,正地闪的数目在雷暴消散阶段稍有增长;地闪频数与地面风速时序变化呈现很好的一致性;雷暴来临前风矢位温特征表明对流云发展高度较高,对流层顶的薄层超低温为强对流发生提供了热力不稳定的先兆信息,整层大气深厚的顺时针垂直切变及中低层偏南风为强对流天气提供了有利的动力和水汽条件,为雷暴潜势预报提供了依据;地闪分布与雷达回波顶高、强的风切变区域以及暴雨落区有明显对应关系;负地闪密集区位于雷达强回波核前方强度为40 ～45dBz区域处,对于回波的未来移向有指示作用. 相似文献