The dynamic effects of solar eclipses of October 25, 2022, and October 14, 2023, on GPS-derived total electron content

This study analyzes total electron content (TEC) variations during two solar eclipse events that occurred on October 25, 2022, and October 14, 2023. The solar eclipse of October 25, 2022, was a partial solar eclipse, while the eclipse of October 14, 2023, was an annular solar eclipse. For this study...

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Main Authors: Vishal Chauhan, Vishakha, Rakesh Singh, Shishupal Singh, Vikram Singh, Om Prakash Singh
Format: Article
Language:English
Published: KeAi Communications Co., Ltd. 2025-01-01
Series:Geodesy and Geodynamics
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Online Access:http://www.sciencedirect.com/science/article/pii/S1674984724000697
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author Vishal Chauhan
Vishakha
Rakesh Singh
Shishupal Singh
Vikram Singh
Om Prakash Singh
author_facet Vishal Chauhan
Vishakha
Rakesh Singh
Shishupal Singh
Vikram Singh
Om Prakash Singh
author_sort Vishal Chauhan
collection DOAJ
description This study analyzes total electron content (TEC) variations during two solar eclipse events that occurred on October 25, 2022, and October 14, 2023. The solar eclipse of October 25, 2022, was a partial solar eclipse, while the eclipse of October 14, 2023, was an annular solar eclipse. For this study, the data of eight International GNSS Service (IGS) stations from different eclipse coverage zones are used to analyze TEC variations. It is found that the stations located in the maximum eclipse cover zone exhibited notable decreases in TEC values. The minimum variation of about 11.76% in TEC values is observed at the station situating in about 20 percent eclipse cover zone, while it varies from 22% to 38% at the stations falling in about 60 percent eclipse cover zone. The highest variation in TEC values of about 44% is found at the stations in about 80 percent eclipse cover zone. The time of occurrence of maximum depletion in TEC values at each station is in line with their longitudinal sequence. Atmospheric gravity waves (AGWs) are also observed by performing wavelet analysis on TEC data. The global TEC maps visualize and confirm observed TEC variations, providing spatial and temporal insights into the ionospheric response. This analysis highlights the influence of station location and eclipse coverage on the magnitude and spatial distribution of TEC variations.
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publishDate 2025-01-01
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spelling doaj-art-cd6d61368a1d47b58502637c8ff4053b2025-08-20T02:35:36ZengKeAi Communications Co., Ltd.Geodesy and Geodynamics1674-98472025-01-01161758610.1016/j.geog.2024.06.003The dynamic effects of solar eclipses of October 25, 2022, and October 14, 2023, on GPS-derived total electron contentVishal Chauhan0 Vishakha1Rakesh Singh2Shishupal Singh3Vikram Singh4Om Prakash Singh5Department of Physics, Graphic Era Hill University, Dehradun 248002, India; Corresponding author.Department of Physics, Graphic Era Hill University, Dehradun 248002, IndiaDepartment of Petroleum Engineering, Graphic Era (Deemed to be University), Dehradun 248002, IndiaDepartment of Physics, Graphic Era Hill University, Dehradun 248002, IndiaDepartment of Physics, St. John's College, Agra 282002, IndiaDepartment of Applied Sciences & Humanities, Institute of Engineering & Technology, Lucknow 226021, IndiaThis study analyzes total electron content (TEC) variations during two solar eclipse events that occurred on October 25, 2022, and October 14, 2023. The solar eclipse of October 25, 2022, was a partial solar eclipse, while the eclipse of October 14, 2023, was an annular solar eclipse. For this study, the data of eight International GNSS Service (IGS) stations from different eclipse coverage zones are used to analyze TEC variations. It is found that the stations located in the maximum eclipse cover zone exhibited notable decreases in TEC values. The minimum variation of about 11.76% in TEC values is observed at the station situating in about 20 percent eclipse cover zone, while it varies from 22% to 38% at the stations falling in about 60 percent eclipse cover zone. The highest variation in TEC values of about 44% is found at the stations in about 80 percent eclipse cover zone. The time of occurrence of maximum depletion in TEC values at each station is in line with their longitudinal sequence. Atmospheric gravity waves (AGWs) are also observed by performing wavelet analysis on TEC data. The global TEC maps visualize and confirm observed TEC variations, providing spatial and temporal insights into the ionospheric response. This analysis highlights the influence of station location and eclipse coverage on the magnitude and spatial distribution of TEC variations.http://www.sciencedirect.com/science/article/pii/S1674984724000697Solar eclipseIonosphereGPSTECAGW
spellingShingle Vishal Chauhan
Vishakha
Rakesh Singh
Shishupal Singh
Vikram Singh
Om Prakash Singh
The dynamic effects of solar eclipses of October 25, 2022, and October 14, 2023, on GPS-derived total electron content
Geodesy and Geodynamics
Solar eclipse
Ionosphere
GPS
TEC
AGW
title The dynamic effects of solar eclipses of October 25, 2022, and October 14, 2023, on GPS-derived total electron content
title_full The dynamic effects of solar eclipses of October 25, 2022, and October 14, 2023, on GPS-derived total electron content
title_fullStr The dynamic effects of solar eclipses of October 25, 2022, and October 14, 2023, on GPS-derived total electron content
title_full_unstemmed The dynamic effects of solar eclipses of October 25, 2022, and October 14, 2023, on GPS-derived total electron content
title_short The dynamic effects of solar eclipses of October 25, 2022, and October 14, 2023, on GPS-derived total electron content
title_sort dynamic effects of solar eclipses of october 25 2022 and october 14 2023 on gps derived total electron content
topic Solar eclipse
Ionosphere
GPS
TEC
AGW
url http://www.sciencedirect.com/science/article/pii/S1674984724000697
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