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Correlated luminosity and magnetic field peaks produced by canton tower-strokes

机译:广州塔行程产生的相关光度和磁场峰值

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摘要

Simultaneously measured luminosity and magnetic field induced by the return strokes in typical upward and downward flashes occurring on the 600 m-tall Canton Tower were presented. The correlation between peak relative luminosity and peak relative magnetic field induced by return strokes were examined for 4 upward and 4 downward flashes. All the flashes contained 3 or more return strokes and all the return strokes in a same flash followed the same path. Luminosity of the lightning channel close to the top of the Canton Tower exhibited characteristics of pronounced initial peak with 20-90% rise time of about 5.2 mu s (arithmetic mean value, based on 43 samples) for subsequent strokes, which was inferred to be related to the secondary (typically largest) peak current at the top of the Canton Tower. The magnetic field induced by subsequent strokes exhibited characteristics of pronounced initial peak with 20-90% rise time of about 1.2 mu s (arithmetic mean value, based on 47 samples). The initial peak magnetic field was modified to proportionally represent the largest peak current at the top of the Canton Tower. Roughly linear and quadratic relation between the initial peak luminosity and modified peak magnetic field were found for subsequent strokes in both upward and downward flashes. The quadratic relation fit the data slightly better than the linear relation. The ratio of peaks of luminosity to magnetic field of the downward first stroke were considerably larger than those of the subsequent strokes, the possible reasons were also discussed.
机译:同时介绍了在600 m高的广州塔上发生的典型的向上和向下闪光过程中,由回程引起的光度和磁场的同时测量。对于4次向上和4次向下的闪烁,检查了由回程引起的峰值相对亮度和峰值相对磁场之间的相关性。所有闪光灯都包含3个或更多的返回行程,并且同一闪光灯中的所有返回行程都遵循相同的路径。接近广州塔顶部的雷电通道的光度表现出明显的初始峰特征,其随后的冲程具有约5.2μs(算术平均值,基于43个样本)的20-90%上升时间,据推测是与广州塔顶部的次级(通常是最大)峰值电流有关。随后的笔触感应出的磁场表现出明显的初始峰,上升时间为20-90%,约为1.2μs(算术平均值,基于47个样品)。修改了初始峰值磁场,以按比例代表广州塔顶部的最大峰值电流。在向上和向下闪烁中,对于随后的笔划,发现初始峰值光度和修改的峰值磁场之间大致呈线性和二次关系。二次关系拟合数据比线性关系稍好。向下的第一个笔触的光度峰值与磁场的比值明显大于随后的笔触的峰值,还讨论了可能的原因。

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  • 来源
    《Atmospheric research》 |2019年第4期|59-69|共11页
  • 作者单位

    China Meteorol Adm, Inst Trop & Marine Meteorol, Guangzhou 510080, Guangdong, Peoples R China|Chinese Acad Meteorol Sci, State Key Lab Severe Weather, 46 Zhongguancun South Ave, Beijing 100081, Peoples R China;

    Chinese Acad Meteorol Sci, State Key Lab Severe Weather, 46 Zhongguancun South Ave, Beijing 100081, Peoples R China;

    FuDan Univ, Dept Atmospher & Ocean Sci, Shanghai 200938, Peoples R China|FuDan Univ, Inst Atmospher Sci, Shanghai 200938, Peoples R China;

    Chinese Acad Meteorol Sci, State Key Lab Severe Weather, 46 Zhongguancun South Ave, Beijing 100081, Peoples R China;

    Chinese Acad Meteorol Sci, State Key Lab Severe Weather, 46 Zhongguancun South Ave, Beijing 100081, Peoples R China;

    Chinese Acad Meteorol Sci, State Key Lab Severe Weather, 46 Zhongguancun South Ave, Beijing 100081, Peoples R China;

    Univ Alabama, Earth Syst Sci Ctr, Huntsville, AL 35899 USA;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Lightning; Return stroke; Peak luminosity; Peak magnetic field;

    机译:闪电;回程;峰值光度;峰值磁场;

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