Upward Leaders Initiated From Instrumented Lightning Rods During the Approach of a Downward Leader in a Cloud‐To‐Ground Flash

闪电(连接器) 闪光灯(摄影) 电流(流体) 电场 脉搏(音乐) 气象学 电气工程 机械 光学 物理 地质学 工程类 电压 功率(物理) 医学 替代医学 病理 量子力学
作者
Marcelo M. F. Saba,Paola Beatriz Lauria,Carina Schumann,José Claudio de O. Silva,Felipe de Lima Mantovani
出处
期刊:Journal Of Geophysical Research: Atmospheres [Wiley]
卷期号:128 (8) 被引量:7
标识
DOI:10.1029/2022jd038082
摘要

Abstract In this paper we analyze electric‐field and current measurements of upward leaders induced by a downward negative lightning flash that struck a residential building. The attachment process was recorded by two high‐speed cameras running at 37,800 and 70,000 images per second and the current measured in two lightning rods. Differently from previous works, here we show, for the first time, current measurements of multiple upward leaders that after initiation propagate to connect the negative downward moving leader. At the beginning of the propagation of the leaders that initiate on the instrumented lightning rods, current pulses appear superimposed to a steadily increasing DC current. The upward leader current pulses increase with the approach of the downward leader and are not synchronized but present an alternating pattern. All 2D leader speeds are approximately constant. The upward leaders are slower than the downward leader speed. The average time interval between current pulses in upward leaders is close to the interstep time interval found by optical or electric field sensors for negative cloud‐to‐ground stepped leaders. The upward leaders respond to different downward propagating branches and, as the branches alternate in propagation and intensity, so do the leaders accordingly. Right before the attachment process the alternating pattern of the leaders ceases, all downward leader branches intensify, and consequently upward leaders synchronize and pulse together. The average linear densities for upward leaders (49 and 82 μC/m) were obtained for the first time for natural lightning.
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