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New revelations on lightning initiation and evolution using a newly developed array of wideband electric field sensors.

机译:使用新开发的宽带电场传感器阵列,有关闪电引发和进化的新启示。

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摘要

Lightning is fundamentally a multi-scale discharge in atmosphere, spanning scales from less than a meter to many kilometers. This research introduces a new instrument array, named the Huntsville Alabama Marx Meter Array (HAMMA), capable of making measurements of the radiated electric field in the wideband frequency regime of ∼ 1 Hz – 500 kHz. The combination of sampling frequency (1 MHz) and baselines (∼ 15 km) of HAMMA sensors has never been attempted in prior published research.;This study chronicles the development and initial applications of HAMMA. Using time of arrival techniques, HAMMA can determine the spacetime position of the wideband radiation from a lightning flash. Measurements from the National Lightning Detection Network (NLDN) are used to quantify the spatial resolution of HAMMA sources; in particular, the average difference in locations of return strokes between HAMMA and NLDN is 250 m. Further, the spacetime positions of wideband sources map out the same general electrical extent of a lightning flash as VHF sources, a result that was previously thought unlikely.;The wideband waveforms measured by HAMMA are compared to space-based optical observations by the Lightning Imaging Sensor (LIS). Analysis shows when an optical emission is detected by the LIS, the wideband waveform also detects a distinct discharge. However, no unique signature is present in the VHF sources. LIS also detects return strokes at a far higher frequency than previous published research using VHF sources shows. Finally, the peak electric field radiated by return strokes is used to suggest there exists a threshold below which not enough optical emission is produced to be detected by LIS.;For the first time, wideband sources associated with initiation are found. These are compared with VHF sources and are found to differ by ∼310 m (horizontally) and ∼ 640 m (vertically). Further, the time difference between wideband and VHF sources are shown to be generally incompatible with the cosmic ray runaway breakdown theory of initiation. Finally, initiation locations are compared to radar data to show that lightning is preferentially initiated near dry snow and small hail/graupel, suggesting that these particular hydrometeors play a non-trivial role in initiation.
机译:从根本上讲,闪电是大气中的多尺度放电,范围从不到一米到几千米。这项研究引入了一种新的仪器阵列,称为Huntsville Alabama马克思仪表阵列(HAMMA),能够测量约1 Hz-500 kHz宽带频率范围内的辐射电场。在先前发表的研究中从未尝试过将HAMMA传感器的采样频率(1 MHz)和基线(〜15 km)相结合。该研究记录了HAMMA的开发和初始应用。使用到达时间技术,HAMMA可以确定闪电发出的宽带辐射的时空位置。来自国家闪电检测网络(NLDN)的测量结果用于量化HAMMA光源的空间分辨率。特别地,HAMMA与NLDN之间的回程位置的平均差为250m。此外,宽带源的时空位置映射出与VHF源相同的闪电一般电范围,这是以前认为不太可能的结果;;由HAMMA测量的宽带波形与闪电成像法与基于空间的光学观察结果进行了比较传感器(LIS)。分析表明,当LIS检测到光发射时,宽带波形也会检测到明显的放电。但是,VHF源中没有唯一的签名。 LIS还可以使用VHF信号源显示比以前发表的研究更高的频率来检测回程。最后,利用回程辐射的峰值电场来表明存在一个阈值,在该阈值以下,LIS无法检测到足够的光发射。首次发现与引发相关的宽带光源。将它们与甚高频源进行了比较,发现相差约310 m(水平)和约640 m(垂直)。此外,宽带和VHF源之间的时间差通常显示与宇宙射线失控击穿理论不兼容。最后,将启动位置与雷达数据进行比较,以显示闪电优先在干燥的积雪和小冰雹/雨滴附近启动,这表明这些特定的水凝物在启动中起着重要作用。

著录项

  • 作者

    Bitzer, Phillip M.;

  • 作者单位

    The University of Alabama in Huntsville.;

  • 授予单位 The University of Alabama in Huntsville.;
  • 学科 Engineering Electronics and Electrical.;Physics Electricity and Magnetism.;Atmospheric Sciences.
  • 学位 Ph.D.
  • 年度 2011
  • 页码 314 p.
  • 总页数 314
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 TS97-4;
  • 关键词

  • 入库时间 2022-08-17 11:44:17

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