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Coordinated observations of sprites and in-cloud lightning flash structure

期刊

JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES
卷 118, 期 12, 页码 6607-6632

出版社

AMER GEOPHYSICAL UNION
DOI: 10.1002/jgrd.50459

关键词

red sprite; positive cloud-to-ground ( plus CG) stroke; Lightning Mapping Array; lightning charge transfer; in-cloud lightning structure; mesoscale convective system

资金

  1. DARPA Nimbus program
  2. NSF Physical and Dynamic Meteorology program
  3. William P. Winn of Langmuir Laboratory
  4. Matuszeski Graduate Research Fund of New Mexico Tech.
  5. Directorate For Geosciences
  6. Div Atmospheric & Geospace Sciences [1047588, 1063966, 1205727] Funding Source: National Science Foundation
  7. Directorate For Geosciences
  8. Div Atmospheric & Geospace Sciences [1042198] Funding Source: National Science Foundation

向作者/读者索取更多资源

The temporal and spatial development of sprite-producing lightning flashes is examined with coordinated observations over an asymmetric mesoscale convective system (MCS) on 29 June 2011 near the Oklahoma Lightning Mapping Array (LMA). Sprites produced by a total of 26 lightning flashes were observed simultaneously on video from Bennett, Colorado and Hawley, Texas, enabling a triangulation of sprites in comparison with temporal development of parent lightning (in particular, negatively charged stepped leaders) in three-dimensional space. In general, prompt sprites produced within 20ms after the causative stroke are less horizontally displaced (typically <30km) from the ground stroke than delayed sprites, which usually occur over 40ms after the stroke with significant lateral offsets (>30km). However, both prompt and delayed sprites are usually centered within 30km of the geometric center of relevant LMA sources (with affinity to negative stepped leaders) during the prior 100ms interval. Multiple sprites appearing as dancing/jumping events associated with a single lightning flash could be produced either by distinct strokes of the flash, by a single stroke through a series of current surges superposed on an intense continuing current, or by both. Our observations imply that sprites elongated in one direction are sometimes linked to in-cloud leader structure with the same elongation, and sprites that were more symmetric were produced above the progression of multiple negative leaders. This suggests that the large-scale structure of sprites could be affected by the in-cloud geometry of positive charge removal. Based on an expanded dataset of 39 sprite-parent flashes by including more sprites recorded by one single camera over the same MCS, the altitude (above mean sea level, MSL) of positively charged cloud region tapped by sprite-producing strokes declined gradually from similar to 10km MSL (-35 degrees C) to around 6km MSL (-10 degrees C) as the MCS evolved through the mature stage. On average, the positive charge removal by causative strokes of sprites observed on 29 June is centered at 3.6km above the freezing level or at 7.9km above ground level.

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