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首页> 外文期刊>Journal of atmospheric and solar-terrestrial physics >Long-delayed bright dancing sprite with large Horizontal displacement from its parent flash
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Long-delayed bright dancing sprite with large Horizontal displacement from its parent flash

机译:长距离明亮的跳舞小精灵,其父闪光灯的水平位移较大

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We reported in this paper the observation of a very bright long-delayed dancing sprite with distinct horizontal displacement from its parent stroke. The dancing sprite lasted only 60 ms, and the morphology consisted of three fields with two slim dim sprite elements in the first two fields and a very bright large element in the third field, different from other observations where the dancing sprites usually contained multiple elements over a longer time interval, and the sprite shape and brightness in the video field are often similar to the previous fields. The bright sprite was displaced at least 38 km from its parent cloud-to-ground (CG) stroke and occurred over comparatively higher cloud top region. The parent flash of this compact dancing sprite was of positive polarity, with only one return stroke (approximately +24 kA) and obvious continuing current process, and the charge moment change of stroke was small (barely above the threshold for sprite production). All the sprite elements occurred during the continuing current stage, and the bright long-delayed sprite element induced a considerable current pulse. The dancing feature of this sprite may be linked to the electrical charge structure, dynamics and microphysics of parent storm, and the inferred development of parent CG flash was consistent with previous very high-frequency (VHF) observations of lightning in the same region. (C) 2015 Elsevier Ltd. All rights reserved.
机译:我们在本文中报告了观察到的非常明亮的长延时跳舞小精灵,其父笔画具有明显的水平位移。舞动精灵仅持续60 ms,形态由三个场组成,前两个场中有两个细长的昏暗精灵元素,第三场中是一个非常明亮的大元素,这与其他观察结果不同,舞动精灵通常包含多个元素。较长的时间间隔,并且视频场中的子画面形状和亮度通常与以前的场相似。明亮的精灵距离其父云到地面(CG)冲程至少38 km,并发生在相对较高的云顶区域。这个紧凑的跳舞小精灵的母闪光是正极性的,只有一个返回冲程(大约+24 kA)和明显的连续电流过程,并且小冲程的充电力矩变化很小(略高于小精灵产生的阈值)。所有的子画面元素都在持续的电流阶段发生,并且明亮的长时延的子画面元素感应出相当大的电流脉冲。该子画面的跳舞特征可能与父风暴的电荷结构,动力学和微观物理学有关,并且推断父CG闪光的发展与先前在同一区域对闪电的甚高频(VHF)观测结果一致。 (C)2015 Elsevier Ltd.保留所有权利。

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