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首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >Testing sprite initiation theory using lightning measurements and modeled electromagnetic fields
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Testing sprite initiation theory using lightning measurements and modeled electromagnetic fields

机译:使用雷电测量和模拟电磁场测试精灵引发理论

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Previous research has shown that the statistical measurements of charge moment changes in sprite-producing lightning are in general agreement with the predictions based on the conventional breakdown theory for sprite initiation in the mesosphere. Measurements have progressed to the point where a detailed, event-level quantitative comparison between the measurements and predictions could more rigorously test the existing theories by estimating the electric fields above the thunderstorm clouds responsible for sprite initiation. We selected for this analysis a set of sprite events from the summer of 2004 whose initiation times are well bounded. Then we measured the current moments and charge moment changes of the parent lightning discharges using the radiated electromagnetic fields recorded by our extremely low frequency/ultra low frequency lightning remote sensing systems. The measured current moments were then used as the input of a two-dimensional cylindrical full-wave finite-difference time-domain model for lightning-generated electromagnetic field simulations. We compared the simulated mesospheric electric fields to the threshold electric field for conventional breakdown to see whether, according to theory, conventional breakdown (and thus a sprite) would be initiated by that electric field and at what altitude. By analyzing sprites that are both short and long delayed from the source lightning strokes, we compared measurements and theory across a wide range of timescales. The results show that for bright, short-delayed sprites, the measurement-inferred mesospheric electric field agrees within 20% with the threshold electric field for conventional breakdown. However, for long delayed sprite events and dimmer sprites, the measurement-inferred mesospheric electric field for sprite initiation is somewhat below the threshold for conventional breakdown.
机译:先前的研究表明,产生子画面的闪电中电荷矩变化的统计测量结果与基于常规击穿理论的中层子画面引发的预测基本一致。测量已经发展到这样的程度,在测量和预测之间进行详细的事件级定量比较,可以通过估计负责子星引发的雷暴云上方的电场来更严格地测试现有理论。为进行此分析,我们选择了2004年夏季开始的一系列精灵事件,其启动时间是有限的。然后,我们使用我们的极低频/超低频雷电遥感系统记录的辐射电磁场,测量了母体雷电放电的电流矩和充电矩变化。然后将测得的电流矩用作二维圆柱全波有限差分时域模型的输入,以进行雷电产生的电磁场模拟。我们将模拟的中层电场与常规击穿的阈值电场进行了比较,以了解根据理论,常规击穿(以及子画面)是否将由该电场以及在什么高度引发。通过分析与源雷击有短时间延迟和长时间延迟的子画面,我们在很宽的时间范围内比较了测量结果和理论。结果表明,对于亮的,短时延的子画面,测量推断的中层电场与常规击穿的阈值电场相吻合在20%以内。但是,对于长时间延迟的精灵事件和调光精灵,用于精灵启动的由测量推断的中层电场略低于常规击穿的阈值。

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