High Peak Current Lightning and the Production of Elves

Описание

Тип публикации: статья из журнала

Год издания: 2024

Идентификатор DOI: 10.1029/2023jd039849

Аннотация: <jats:title>Abstract</jats:title><jats:p>Elves are observed as expanding rings of light in the UV and visible optical bands. They are produced when electromagnetic pulses from lightning discharges interact with the lower parts of the ionosphere. Elves are well known to be associated with high peak current lightning discharges. HereПоказать полностью, we use data from the Modular Multi-spectral Imaging Array (MMIA) of the Atmosphere-Space Interactions Monitor (ASIM), and search for observations of Elves when high peak current lightning discharges are detected by Vaisala's Global Lightning Detection network GLD360. We present two groups of events; high peak current detections associated with Elves and high peak current detections not associated with Elves. To understand why some current pulses with high peak currents do not produce observable Elves, we investigate and compare the lightning activity occurring before these two types of events, in terms of both the number of lightning discharges detected by GLD360 and the peak currents of the preceding discharges. Our results, using data from GLD360, suggest that current pulses with peak currents above |120| kA tend to produce Elves nearly always, regardless of the preceding lightning activity. For current pulses with peak currents between |70| and |120| kA, the number of observed Elves might be affected by the preceding lightning activity, or is the result of the characteristics of the storm cells that produce the Elve.</jats:p>

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Издание

Журнал: Journal of Geophysical Research: Atmospheres

Выпуск журнала: Т. 129, 4

ISSN журнала: 21698996

Персоны

  • Bjørge-Engeland Ingrid (Birkeland Centre for Space Science University of Bergen Bergen Norway)
  • Østgaard Nikolai (Birkeland Centre for Space Science University of Bergen Bergen Norway)
  • Marisaldi Martino (Birkeland Centre for Space Science University of Bergen Bergen Norway)
  • Luque Alejandro (Instituto de Astrofisica de Andalucia CSIC Granada Spain)
  • Mezentsev Andrey (Birkeland Centre for Space Science University of Bergen Bergen Norway)
  • Lehtinen Nikolai (Birkeland Centre for Space Science University of Bergen Bergen Norway)
  • Chanrion Olivier (National Space Institute Technical University of Denmark Kgs. Lyngby Denmark)
  • Fuglestad Anders Nødland (Birkeland Centre for Space Science University of Bergen Bergen Norway)
  • Neubert Torsten (National Space Institute Technical University of Denmark Kgs. Lyngby Denmark)
  • Gordillo-Vazquez Francisco J. (Instituto de Astrofisica de Andalucia CSIC Granada Spain)

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