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dc.contributor.authorLi, Dongshuai
dc.contributor.authorLuque, Alejandro
dc.contributor.authorGordillo-Vazquez, F.J.
dc.contributor.authorPérez-Invernón, F.J.
dc.contributor.authorHusbjerg, Lasse Skaaning
dc.contributor.authorNeubert, Torsten
dc.contributor.authorChanrion, Olivier
dc.contributor.authorLu, Gaopeng
dc.contributor.authorZhang, Hongbo
dc.contributor.authorHan, Jing
dc.contributor.authorLehtinen, Nikolai Grigorievich
dc.contributor.authorØstgaard, Nikolai
dc.contributor.authorReglero, Víctor
dc.date.accessioned2024-05-06T12:19:13Z
dc.date.available2024-05-06T12:19:13Z
dc.date.created2023-06-08T14:43:28Z
dc.date.issued2023
dc.identifier.issn2169-897X
dc.identifier.urihttps://hdl.handle.net/11250/3129250
dc.description.abstractSingle- and multi-pulse blue corona discharges are frequently observed in thunderstorm clouds. Although we know they often correlate with Narrow Bipolar Events (NBEs) in Very Low Frequency/Low Frequency radio signals, their physics is not well understood. Here, we report a detailed analysis of different types of blue corona discharges observed by the Atmosphere-Space Interactions Monitor during an overpass of a thundercloud cell nearby Malaysia. Both single- and multi-pulse blue corona discharges were associated with positive NBEs at the top of the cloud, reaching about 18 km altitude. We find that the primary pulses of multi-pulse discharges have weaker current moments than the single-pulse discharges, suggesting that the multi-pulse discharges either have shorter vertical channels or have weaker currents than the single-pulse discharges. The subsequent pulse trains of the multi-pulse discharges delayed some milliseconds are likely from horizontally oriented electrical discharges, but some NBEs, correlated with both single-and multi-pulse discharges, include small-amplitude oscillations within a few microseconds inside their waveforms, which are unresolved in the optical observation and yet to be understood. Furthermore, by jointly analyzing the optical and radio observations, we estimate the photon free mean path at the cloud top to be ∼6 m.en_US
dc.language.isoengen_US
dc.publisherAGUen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titleDifferent Types of Corona Discharges Associated With High-Altitude Positive Narrow Bipolar Events Nearby Cloud Topen_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2023 The Author(s)en_US
dc.source.articlenumbere2022JD037883en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.doi10.1029/2022JD037883
dc.identifier.cristin2153128
dc.source.journalJournal of Geophysical Research (JGR): Atmospheresen_US
dc.identifier.citationJournal of Geophysical Research (JGR): Atmospheres. 2023, 128 (4), e2022JD037883.en_US
dc.source.volume128en_US
dc.source.issue4en_US


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