The Great Reduction of Equatorial Electrojet During the Solar Eclipse on 14 December 2020

Abstract The solar eclipse has a great influence on the variability of the ionosphere because of the obscuration of solar radiation. Using the equatorial electrojet (EEJ) and plasma measurements from Swarm, zonal winds from the Michelson Interferometer for Global High‐resolution Thermospheric Imagin...

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Main Authors: Kedeng Zhang, Hui Wang
Format: Article
Language:English
Published: Wiley 2022-12-01
Series:Space Weather
Online Access:https://doi.org/10.1029/2022SW003295
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author Kedeng Zhang
Hui Wang
author_facet Kedeng Zhang
Hui Wang
author_sort Kedeng Zhang
collection DOAJ
description Abstract The solar eclipse has a great influence on the variability of the ionosphere because of the obscuration of solar radiation. Using the equatorial electrojet (EEJ) and plasma measurements from Swarm, zonal winds from the Michelson Interferometer for Global High‐resolution Thermospheric Imaging on Ionospheric Connection Explorer mission, and electron density from the Constellation Observing Systems for Meteorology, Ionosphere, and Climate mission, the temporal responses of EEJ to the total solar eclipse on 14 December 2020, have been examined. In comparison with non‐eclipse EEJ, EEJ at the eclipse/early post‐eclipse phase is significantly reduced, with a percentage of more than 29%. The reduced EEJ is primarily attributed to both the weakened electric field and the reversed zonal winds. The reversed zonal winds could drive corresponding currents and electric field, indicating the direct and indirect roles. The depleted plasma plays a secondary role in the decrease of EEJ.
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institution Kabale University
issn 1542-7390
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publishDate 2022-12-01
publisher Wiley
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series Space Weather
spelling doaj-art-ecf7ee9d1d484d30bdb7d5f4927d59082025-01-14T16:30:23ZengWileySpace Weather1542-73902022-12-012012n/an/a10.1029/2022SW003295The Great Reduction of Equatorial Electrojet During the Solar Eclipse on 14 December 2020Kedeng Zhang0Hui Wang1Department of Space Physics School of Electronic Information Wuhan University Wuhan ChinaDepartment of Space Physics School of Electronic Information Wuhan University Wuhan ChinaAbstract The solar eclipse has a great influence on the variability of the ionosphere because of the obscuration of solar radiation. Using the equatorial electrojet (EEJ) and plasma measurements from Swarm, zonal winds from the Michelson Interferometer for Global High‐resolution Thermospheric Imaging on Ionospheric Connection Explorer mission, and electron density from the Constellation Observing Systems for Meteorology, Ionosphere, and Climate mission, the temporal responses of EEJ to the total solar eclipse on 14 December 2020, have been examined. In comparison with non‐eclipse EEJ, EEJ at the eclipse/early post‐eclipse phase is significantly reduced, with a percentage of more than 29%. The reduced EEJ is primarily attributed to both the weakened electric field and the reversed zonal winds. The reversed zonal winds could drive corresponding currents and electric field, indicating the direct and indirect roles. The depleted plasma plays a secondary role in the decrease of EEJ.https://doi.org/10.1029/2022SW003295
spellingShingle Kedeng Zhang
Hui Wang
The Great Reduction of Equatorial Electrojet During the Solar Eclipse on 14 December 2020
Space Weather
title The Great Reduction of Equatorial Electrojet During the Solar Eclipse on 14 December 2020
title_full The Great Reduction of Equatorial Electrojet During the Solar Eclipse on 14 December 2020
title_fullStr The Great Reduction of Equatorial Electrojet During the Solar Eclipse on 14 December 2020
title_full_unstemmed The Great Reduction of Equatorial Electrojet During the Solar Eclipse on 14 December 2020
title_short The Great Reduction of Equatorial Electrojet During the Solar Eclipse on 14 December 2020
title_sort great reduction of equatorial electrojet during the solar eclipse on 14 december 2020
url https://doi.org/10.1029/2022SW003295
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