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dc.contributor.authorBjørge-Engeland, Ingrid
dc.contributor.authorØstgaard, Nikolai
dc.contributor.authorMezentsev, Andrey
dc.contributor.authorSkeie, Chris Alexander Kallevik
dc.contributor.authorSarria, David Alexandre Stephan
dc.contributor.authorLapierre, Jeff
dc.contributor.authorLindanger, Anders
dc.contributor.authorNeubert, Torsten
dc.contributor.authorMarisaldi, Martino
dc.contributor.authorLehtinen, Nikolai Grigorievich
dc.contributor.authorChanrion, Olivier
dc.contributor.authorUllaland, Kjetil
dc.contributor.authorYang, Shiming
dc.contributor.authorGenov, Georgi
dc.contributor.authorChristiansen, Freddy
dc.contributor.authorReglero, Victor
dc.date.accessioned2023-03-13T09:29:28Z
dc.date.available2023-03-13T09:29:28Z
dc.date.created2022-09-14T17:07:42Z
dc.date.issued2022
dc.identifier.issn2169-897X
dc.identifier.urihttps://hdl.handle.net/11250/3057873
dc.description.abstractThe Atmosphere-Space Interactions Monitor was designed to monitor Terrestrial Gamma-ray Flashes (TGFs) and Transient Luminous Events (TLEs) from space, enabling the study of how these phenomena are related. In this paper, we present observations of 17 TGFs with accompanying Elves. TGFs are short and highly energetic bursts of gamma photons associated with lightning discharges, whereas Elves are TLEs that are observed as concentric rings of ultraviolet (UV) and visible light at ionospheric altitudes, produced by the excitation of N2 molecules when an electromagnetic pulse hits the base of the ionosphere. Elves were identified when optical detections in the UV band could be clearly distinguished from other optical signals from lightning strokes. The TGFs they accompanied had short durations and were associated with particularly high peak current lightning. Lightning sferics associated with these events were detected by the global lightning network GLD360 and the World Wide Lightning Location Network, and they were, with the exception of one event, observed over ocean or coastal regions. It is likely that these events were associated with Energetic In-cloud Pulses. We show that short duration TGFs tend to be associated with higher peak currents than long duration TGFs.en_US
dc.language.isoengen_US
dc.publisherAGUen_US
dc.rightsNavngivelse-Ikkekommersiell 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by-nc/4.0/deed.no*
dc.titleTerrestrial Gamma-Ray Flashes With Accompanying Elves Detected by ASIMen_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2022 The Author(s)en_US
dc.source.articlenumbere2021JD036368en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.doi10.1029/2021JD036368
dc.identifier.cristin2051768
dc.source.journalJournal of Geophysical Research (JGR): Atmospheresen_US
dc.identifier.citationJournal of Geophysical Research (JGR): Atmospheres. 2022, 127 (11), e2021JD036368.en_US
dc.source.volume127en_US
dc.source.issue11en_US


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Navngivelse-Ikkekommersiell 4.0 Internasjonal
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