Observations of Red Sprites Above Hurricane Matthew

Abstract More than three dozen red sprites were captured above Hurricane Matthew on the nights of 1 and 2 October 2016 as it passed to the north of Venezuela after undergoing rapid intensification. Analyses using broadband magnetic fields indicate that all of the sprites were produced by positive cl...

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Main Authors: Anjing Huang, Gaopeng Lu, Jia Yue, Walter Lyons, Frankie Lucena, Fanchao Lyu, Steven A. Cummer, Wenjuan Zhang, Liangtao Xu, Xianghui Xue, Shuang Xu
Format: Article
Language:English
Published: Wiley 2018-12-01
Series:Geophysical Research Letters
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Online Access:https://doi.org/10.1029/2018GL079576
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author Anjing Huang
Gaopeng Lu
Jia Yue
Walter Lyons
Frankie Lucena
Fanchao Lyu
Steven A. Cummer
Wenjuan Zhang
Liangtao Xu
Xianghui Xue
Shuang Xu
author_facet Anjing Huang
Gaopeng Lu
Jia Yue
Walter Lyons
Frankie Lucena
Fanchao Lyu
Steven A. Cummer
Wenjuan Zhang
Liangtao Xu
Xianghui Xue
Shuang Xu
author_sort Anjing Huang
collection DOAJ
description Abstract More than three dozen red sprites were captured above Hurricane Matthew on the nights of 1 and 2 October 2016 as it passed to the north of Venezuela after undergoing rapid intensification. Analyses using broadband magnetic fields indicate that all of the sprites were produced by positive cloud‐to‐ground (CG) strokes located within the outer rainbands as defined by relatively cold cloud top brightness temperatures (≤194 K). Negative CG strokes with impulse charge transfers exceeding the threshold of sprite production also existed, but the timescale of the charge transfer was not sufficiently long to develop streamers. The reported observations are contrary to the finding of the Imager of Sprites/Upper Atmospheric Lightning showing that sprites are preferentially produced by negative strokes in the same geographic region. Further ground‐based observations are desired to obtain additional insights into the convective regimes associated with the dominance of negative sprites in many oceanic and coastal thunderstorms.
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institution OA Journals
issn 0094-8276
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language English
publishDate 2018-12-01
publisher Wiley
record_format Article
series Geophysical Research Letters
spelling doaj-art-03e6bc376f7d4e5ca9c85508884ede1f2025-08-20T02:31:37ZengWileyGeophysical Research Letters0094-82761944-80072018-12-01452313,15813,16510.1029/2018GL079576Observations of Red Sprites Above Hurricane MatthewAnjing Huang0Gaopeng Lu1Jia Yue2Walter Lyons3Frankie Lucena4Fanchao Lyu5Steven A. Cummer6Wenjuan Zhang7Liangtao Xu8Xianghui Xue9Shuang Xu10Key Laboratory of Middle Atmosphere and Global Environment Observation Institute of Atmospheric Physics,Chinese Academy of Sciences Beijing ChinaKey Laboratory of Middle Atmosphere and Global Environment Observation Institute of Atmospheric Physics,Chinese Academy of Sciences Beijing ChinaDepartment of Atmospheric and Planetary Sciences Hampton University Hampton VA USAFMA Research Ft. Collins CO USACabo Rojo Puerto RicoElectrical and Computer Engineering Department Duke University Durham NC USAElectrical and Computer Engineering Department Duke University Durham NC USAState Key Laboratory of Severe Weather Chinese Academy of Meteorological Sciences Beijing ChinaState Key Laboratory of Severe Weather Chinese Academy of Meteorological Sciences Beijing ChinaSchool of Earth and Space Sciences University of Science and Technology of China Hefei ChinaSchool of Earth and Space Sciences University of Science and Technology of China Hefei ChinaAbstract More than three dozen red sprites were captured above Hurricane Matthew on the nights of 1 and 2 October 2016 as it passed to the north of Venezuela after undergoing rapid intensification. Analyses using broadband magnetic fields indicate that all of the sprites were produced by positive cloud‐to‐ground (CG) strokes located within the outer rainbands as defined by relatively cold cloud top brightness temperatures (≤194 K). Negative CG strokes with impulse charge transfers exceeding the threshold of sprite production also existed, but the timescale of the charge transfer was not sufficiently long to develop streamers. The reported observations are contrary to the finding of the Imager of Sprites/Upper Atmospheric Lightning showing that sprites are preferentially produced by negative strokes in the same geographic region. Further ground‐based observations are desired to obtain additional insights into the convective regimes associated with the dominance of negative sprites in many oceanic and coastal thunderstorms.https://doi.org/10.1029/2018GL079576red spritesHurricane Matthewpositive cloud‐to‐ground (+CG) strokesoceanic thunderstormsland and sea difference
spellingShingle Anjing Huang
Gaopeng Lu
Jia Yue
Walter Lyons
Frankie Lucena
Fanchao Lyu
Steven A. Cummer
Wenjuan Zhang
Liangtao Xu
Xianghui Xue
Shuang Xu
Observations of Red Sprites Above Hurricane Matthew
Geophysical Research Letters
red sprites
Hurricane Matthew
positive cloud‐to‐ground (+CG) strokes
oceanic thunderstorms
land and sea difference
title Observations of Red Sprites Above Hurricane Matthew
title_full Observations of Red Sprites Above Hurricane Matthew
title_fullStr Observations of Red Sprites Above Hurricane Matthew
title_full_unstemmed Observations of Red Sprites Above Hurricane Matthew
title_short Observations of Red Sprites Above Hurricane Matthew
title_sort observations of red sprites above hurricane matthew
topic red sprites
Hurricane Matthew
positive cloud‐to‐ground (+CG) strokes
oceanic thunderstorms
land and sea difference
url https://doi.org/10.1029/2018GL079576
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