Observation of tropical positive cloud-to-ground flashes accompanied by chaotic and regular pulse trains

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2024-06-28 DOI:10.1016/j.jastp.2024.106285
Muhammad Haziq Mohammad Sabri , Mohd Riduan Ahmad , Yuji Takayanagi , Muhammad Zuhair Bolqiah Edris , Shamsul Ammar Shamsul Baharin , Takeshi Morimoto , Zen-Ichiro Kawasaki , Mohd Zafri Baharuddin , Vernon Cooray
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Abstract

This study investigates the occurrence of chaotic pulse trains (CPTs) and regular pulse trains (RPTs) in tropical positive cloud-to-ground (CG) lightning flashes. These flashes are categorized into four types based on the initial polarity of the initial breakdown (IB) pulses and their relationship to the first return stroke (RS). A total of 71 positive CG flashes from five thunderstorm events were analyzed. The analysis reveals instances of CPTs and RPTs both before and after the first positive RS, along with the occurrence of mixed polarities in RPTs. Variations in IB pulse polarities and the presence of CPTs and RPTs before the first positive RS were observed, contrasting with previous findings in negative CG flashes. All positive CG flashes have been detected when cloud top height occurrences were between 12 and 18 km. In contrast, for negative CG flashes with CPTs and RPTs the cloud top height occurrences were between 5 and 12 km. It is interesting that CPTs and RPTs can be detected during IB process of positive CG flashes at relatively high altitude in the thundercloud. Perhaps due to low pressure at higher altitudes in the cloud, electrical process associated with CPTs and RPTs are easily discharged before the occurrence first positive return stroke. The altitudes of cloud top heights for the inverse polarity of IB pulses were located between 16 and 18 km. This research enhances the understanding of positive CG lightning initiation process and their relationship with CPTs and RPTs, as well as the occurrence of recoil leaders.

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观测到伴有混乱和规则脉冲序列的热带正向云地闪光
本研究调查了热带正云层到地面(CG)闪电中出现的混沌脉冲串(CPT)和规则脉冲串(RPT)。根据初始击穿(IB)脉冲的极性及其与第一个返回冲程(RS)的关系,将这些闪电分为四种类型。共分析了五次雷暴事件中的 71 个正 CG 闪光灯。分析结果显示,在第一个正向 RS 之前和之后都出现了 CPT 和 RPT,RPT 中还出现了混合极性。观察到 IB 脉冲极性的变化,以及第一个正 RS 之前 CPT 和 RPT 的存在,这与之前在负 CG 闪烁中的发现形成了对比。当云顶高度出现在 12 至 18 千米之间时,所有正 CG 闪烁都被探测到。相比之下,带有 CPT 和 RPT 的负向 CG 闪烁的云顶高度在 5 至 12 千米之间。有趣的是,在雷云中相对较高高度的正 CG 闪烁 IB 过程中,可以检测到 CPT 和 RPT。也许是由于云中较高高度的气压较低,与 CPT 和 RPT 相关的电过程很容易在出现第一个正向返回冲程之前释放。IB 脉冲反极性的云顶高度位于 16 至 18 千米之间。这项研究加深了人们对正CG闪电启动过程及其与CPTs和RPTs的关系以及反冲领导的发生的理解。
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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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