广州地区雷暴过程云-地闪特征及其环境条件

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。     

2007年深圳市雷电灾害气候特征分析

通过对2007年深圳市雷电气候特征、雷电密度分布、重要雷电天气过程分析和雷电灾害情况分析,探讨雷电发生的天气背景以及致灾的成因,为雷电预测预警技术提供科学依据.     

雷电防护技术在现代建筑中的应用

针对建筑物遭受雷击的危害及方式,探讨建筑工程设计与施工中应采取的各种防雷措施,以及防雷装置安装与使用中值得注意的问题.     

野外组装可移动式防直击雷装置的研究

通过对9m×9m的实际接地网进行计算,对于二类和三类防雷建筑物,可以应用当环形接地网的等效面积大于78.5m2后,采取不计接地网接地电阻的设计方法来实现野外可移动式接地网设计,并将避雷针和避雷线组合的接闪器设计成标构件,方便组装,实现野外组装可移动式防直击雷装置.     

New magnetic field measurements of β Cephei stars and slowly pulsating B stars

We present the results of the continuation of our magnetic survey with FORS 1 at the VLT of a sample of B‐type stars consisting of confirmed or candidate β Cephei stars and Slowly Pulsating B (hereafter SPB) stars, along with a small number of normal B‐type stars. A weak mean longitudinal magnetic field of the order of a few hundred Gauss was detected in three β Cephei stars and two stars suspected to be β Cephei stars, in five SPB stars and eight stars suspected to be SPB stars. Additionally, a longitudinal magnetic field at a level larger than 3σ has been diagnosed in two normal B‐type stars, the nitrogen‐rich early B‐type star HD 52089 and in the B5 IV star HD 153716. Roughly one third of β Cephei stars have detected magnetic fields: Out of 13 β Cephei stars studied to date with FORS 1, four stars possess weak magnetic fields, and out of the sample of six suspected β Cephei stars two show a weak magnetic field. The fraction of magnetic SPBs and candidate SPBs is found to be higher: Roughly half of the 34 SPB stars have been found to be magnetic and among the 16 candidate SPBs eight stars possess magnetic fields. In an attempt to understand why only a fraction of pulsating stars exhibit magnetic fields, we studied the position of magnetic and non‐magnetic pulsating stars in the H‐R diagram. We find that their domains in the H‐R diagram largely overlap, and no clear picture emerges as to the possible evolution of the magnetic field across the main sequence. It is possible that stronger fields tend to be found in stars with lower pulsating frequencies and smaller pulsating amplitudes. A somewhat similar trend is found if we consider a correlation between the field strength and the v sin i ‐values, i.e. stronger magnetic fields tend to be found in more slowly rotating stars (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Microphysical Characteristics of Extreme-Rainfall Convection over the Pearl River Delta Region,South China from Polarimetric Radar Data during the Pre-summer Rainy Season

During the pre-summer rainy season, heavy rainfall occurs frequently in South China. Based on polarimetric radar observations, the microphysical characteristics and processes of convective features associated with extreme rainfall rates(ERCFs) are examined. In the regions with high ERCF occurrence frequency, sub-regional differences are found in the lightning flash rate(LFR) distributions. In the region with higher LFRs, the ERCFs have larger volumes of high reflectivity factor above the freezin...     

地基微波辐射计遥感人工触发闪电的观测研究

为了深入研究雷电产生的微波热辐射特征,从2016年初夏开始利用地基微波辐射计在中国气象局雷电野外科学实验基地开展了连续4年的观测实验,根据雷电热效应的特征,制定了观测方案,并为地基微波辐射计设置了“引雷观测模式”。结果表明,地基微波辐射计具有对雷电热效应产生响应的能力。2017—2019年,辐射计一共成功捕获了30次人工触发闪电,观测效率逐年增长,平均为71.4 %;微波亮温脉冲幅度的最大值约125 K。结合其中28次触发事件的雷电流数据,分析了亮温脉冲幅度和雷电流积分量之间的相关性,并发现了最大亮温脉冲幅度与总电流作用积分之间可能存在指数关系。根据亮温观测数据估算了雷电热效应的持续时间,平均约0.5 s,其中25次触发事件的雷电流热效应持续时间与雷电流持续时间变化较为一致,相关系数约0.73。     

基于全球闪电定位网的江淮闪电定位网探测效率分析：以台风“利奇马”为例

基于全球闪电定位网(World Wide Lightning Location Network,WWLLN)获取的闪电定位资料对江淮闪电定位网(Jianghuai Area Sferic Array,JASA)在内陆及近海区域的闪电实时探测性能进行评估。通过对2019年第9号超强台风“利奇马”期间产生的闪电活动进行对比分析,发现JASA和WWLLN对台风闪电的径向分布、时间变化和空间变化有较好的一致性,绝大部分闪电发生在云顶亮温小于220 K区域;在台风发展阶段,内核区闪电活动较为频繁,在台风成熟和消亡阶段时,闪电主要分布外雨带,内核区的闪电活动少但集中。在探测效率方面,JASA对江淮区域实时定位到的闪电数远多于WWLLN,相对探测效率和绝对探测效率分别为69.12%和92.51%。而在海洋区域(114～130°E,20～24°N和123～130°E,24～32°N),由于受到JASA站点位置分布的限制,闪电实时定位数略少于WWLLN,其相对探测效率和绝对探测效率分别为32.67%和52.26%。研究结果表明了JASA对内陆及近海区域雷暴具备较强的捕获能力,为实时监测台风期间强对流闪电...     

青岛地区电场仪资料在一次雷暴天气过程中的应用分析

利用大气电场仪资料,结合天气实况、天气雷达和闪电定位仪等资料,对2013年7月1日青岛地区一次雷暴天气过程进行了综合分析。结果表明,当地面电场强度曲线在几十到几百毫秒量级内发生极性反转,变化幅度在2 kV/m以上,且完成后电场值会迅速回到极性反转前的电场值附近时,可以判断为发生了一次地闪。单站电场强度曲线可以反映出雷暴云与测站间距离的变化,闪电发生前电场强度的增加可为雷电预警提供时间。大气电场仪组网监测资料可以对雷暴云的移动路径做出判断。综合分析大气电场仪组网数据、天气雷达以及闪电定位资料等多源资料,可以更好地判断雷暴云的活动状况,提高雷电的预警准确率和时间提前量。     

Oxidized Nitrogen in the Remote Pacific: The Role of Electrical Discharges over the Oceans

Simulations of oxidized nitrogen performed withglobal transport tracer models systematicallyunderestimate the concentrations of total nitrate atremote marine locations in the Mid-Pacific. Higheremission rates in the models of nitrogen oxides( ) from continental sources or alarger influx from the stratosphere do not seem tobe able to account for the shortfall. We are led toconclude that there has to be a substantial sourcelocated in oceanic areas. We speculate that -emission from electrical discharges overthe oceans could be the source we are looking for.Airborne observations of atmospheric concentrationsof oxidized nitrogen and ozone in the remoteatmosphere and observations of nitrate wetdeposition in remote sites are used as additionalconstraints to check the plausibility of thishypothesis. We find that a larger emission of due to lightning activity over the oceansindeed results in a much improved simulation oftotal nitrate in the remote Pacific, particularly inthe Equatorial and Tropical South Pacific and thatsuch a scenario is generally consistent withavailable observations of nitrate wet deposition andatmospheric concentrations of oxidized nitrogen andozone. An alternative hypothesis is that there is ahitherto unknown in situ source of over thePacific Ocean.