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The Temporal Relationship Between Terrestrial Gamma-Ray Flashes and Associated Optical Pulses From Lightning.
Skeie, C A; Østgaard, N; Mezentsev, A; Bjørge-Engeland, I; Marisaldi, M; Lehtinen, N; Reglero, V; Neubert, T.
Afiliação
  • Skeie CA; Birkeland Centre for Space Science Institute of Physics and Technology University of Bergen Bergen Norway.
  • Østgaard N; Birkeland Centre for Space Science Institute of Physics and Technology University of Bergen Bergen Norway.
  • Mezentsev A; Birkeland Centre for Space Science Institute of Physics and Technology University of Bergen Bergen Norway.
  • Bjørge-Engeland I; Birkeland Centre for Space Science Institute of Physics and Technology University of Bergen Bergen Norway.
  • Marisaldi M; Birkeland Centre for Space Science Institute of Physics and Technology University of Bergen Bergen Norway.
  • Lehtinen N; INAF-OAS Bologna Bologna Italy.
  • Reglero V; Birkeland Centre for Space Science Institute of Physics and Technology University of Bergen Bergen Norway.
  • Neubert T; Imaging Processing Laboratory University of Valencia Valencia Spain.
J Geophys Res Atmos ; 127(17): e2022JD037128, 2022 Sep 16.
Article em En | MEDLINE | ID: mdl-36246842
ABSTRACT
We present 221 Terrestrial Gamma-ray Flashes (TGFs) and associated optical pulses observed by the Atmosphere-Space Interactions Monitor (ASIM) on board the International Space Station. The events were detected between the end of March 2019 and November 2020 and consist of X- and gamma-ray energy detections, as well as photometer data (180-230, 337, and 777 nm) and optical camera data (337 and 777 nm). Using the available ASIM data and applying a consistency check based on TGF characteristics and lightning detections from lightning radio atmospherics close in time, we determine the most likely position of the TGFs in relation to the photometer field of view (FoV), and the association to the observed optical pulses. Out of the 221 events we find 72 events where the TGF and optical data are determined to be associated and inside the photometer FoV. Using the measured TGF durations and the time between the onsets of the TGFs and optical pulses we find (a) That the TGF onsets are always before or at the same time as the optical pulse onsets (taking into account cloud scattering). (b) A tendency for longer duration TGFs to have longer delays between onsets. (c) Two groups of events (a) where there is a possible overlap between the TGFs and the optical emissions, as the TGFs last longer than the delay between onsets and (b) where the TGFs and optical emissions do not overlap, as there are long delays between the onsets, which cannot be explained by cloud scattering.
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Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Risk_factors_studies Idioma: En Revista: J Geophys Res Atmos Ano de publicação: 2022 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Risk_factors_studies Idioma: En Revista: J Geophys Res Atmos Ano de publicação: 2022 Tipo de documento: Article