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Lightning-Initiation Locations as a Remote Sensing Tool of Large Thunderstorm Electric Field Vectors

机译:大雷暴电场矢量的闪电起始位置作为遥感工具

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The lightning data that are recorded with a three-dimensional lightning mapping array (LMA) are compared with data from an electric field change sensor (in this case a flat-plate antenna operated both as a "slow" and a "fast" antenna). The goal of these comparisons is to quantify any time difference that may exist between the initial responses of the two instruments to a lightning flash. The data consist of 136 flashes from two New Mexico thunderstorms. It is found that the initial radiation source detected by the LMA usually precedes the initial response of both the slow and fast antennas. In a small number of cases, the flat-plate antenna response precedes the initial LMA source, but by no more than 2 ms. The observations of such a close time coincidence suggest that the first LMA radiation source of each flash was located at or very near the flash-initiation point. Thus, the first LMA radiation source and the initial sequence of sources from a lightning flash can be used as remote sensing tools to give information about the magnitude of the electric field (relative to lightning-initiation thresholds) and the direction of the electric field at the initiation location.
机译:将用三维雷电映射阵列(LMA)记录的雷电数据与来自电场变化传感器(在这种情况下,平板天线同时用作“慢”和“快”天线)的数据进行比较。 。这些比较的目的是量化两个仪器对闪电的初始响应之间可能存在的任何时间差。数据包括两次来自新墨西哥州雷暴的136次闪光。已经发现,LMA检测到的初始辐射源通常先于慢速天线和快速天线的初始响应。在少数情况下,平板天线响应在初始LMA源之前,但不超过2 ms。如此接近的时间巧合的观察结果表明,每个闪光灯的第一个LMA辐射源都位于闪光灯起始点处或附近。因此,第一个LMA辐射源和闪电的初始源序列可以用作遥感工具,以提供有关电场强度(相对于闪电起始阈值)和电场方向的信息。起始位置。

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