Microphysical and cloud-to-ground lightning characteristics of three tornadoes in a squall line

IF 1.9 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Min Bao , Tinglong Zhang , Hongwu Guo , Tiantao Cheng , Zhe Li , Hai Yu , Yuanyuan Li
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引用次数: 0

Abstract

Convective weather events accompanied by multiple tornadoes are rare. However, on 29 August 2019, a typhoon-induced squall line produced three tornadoes on Hainan Island. This rare event provides a valuable opportunity to investigate the microphysical characteristics and cloud-to-ground (CG) lightning activity during tornado periods. This research employed data from S-band dual-polarimetric Doppler weather radar and a VLF/LF three-dimensional lightning location system. Results showed that during the first tornado (developing stage), hydrometeor particles were sparse and dispersed, resulting in minimal CG lightning activity. In contrast, during the second tornado (mature stage), hydrometeor particles were abundant and concentrated, leading to the most active CG lightning. During the third tornado (dissipating stage), hydrometeor particles began to dissipate, though CG lightning activity remained higher than during the first tornado. The characteristics of hydrometeor particles and CG lightning in tornadoes were consistent with the concurrent developmental phase of the squall line. The rapid rise in the top altitude of the 40 dBZ echoes was a significant indicator of tornado formation. Furthermore, dry graupel, wet graupel, and dry snow particles exhibited strong correlations with CG lightning activity. These findings enhance our understanding of the microphysical and electrification mechanisms associated with tornadoes and provide valuable insights for improving tornado prediction.
飑线中三个龙卷风的微物理和云对地闪电特征
对流天气事件伴随多个龙卷风是罕见的。然而,2019年8月29日,一条台风诱发的飑线在海南岛产生了三场龙卷风。这一罕见的事件为研究龙卷风期间的微物理特征和云对地闪电活动提供了宝贵的机会。本研究采用了s波段双极化多普勒天气雷达和VLF/LF三维闪电定位系统的数据。结果表明:在第一次龙卷风(发展阶段),水流星颗粒稀疏分散,导致CG闪电活动最小;而在第二次龙卷风(成熟阶段),水流星颗粒丰富且集中,导致了最活跃的CG闪电。在第三次龙卷风(消散阶段),水流星粒子开始消散,但CG闪电活动仍然高于第一次龙卷风。龙卷风中水流星粒子和CG闪电的特征与飑线同步发展相一致。40 dBZ回波顶高度的快速上升是龙卷风形成的重要标志。此外,干霰、湿霰和干雪颗粒与CG闪电活动表现出较强的相关性。这些发现增强了我们对与龙卷风相关的微物理和电气化机制的理解,并为改进龙卷风预测提供了有价值的见解。
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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