Characteristics of Nighttime Medium‐Scale Traveling Ionospheric Disturbances: Longitudinal Comparison of Their Seasonal and Local Time Variations

Abstract This study presents a statistical analysis of the occurrence rate of midlatitude nighttime medium scale traveling ionospheric disturbances (MSTIDs) that were detected in Swarm plasma density measurements from 2014 to 2023. Monthly and local time variations of MSTID occurrence rates are comp...

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Main Authors: Zama T. Katamzi‐Joseph, John Bosco Habarulema, Yuichi Otsuka, Tshimangadzo M. Matamba, Amoré E. Nel
Format: Article
Language:English
Published: Wiley 2025-07-01
Series:Space Weather
Online Access:https://doi.org/10.1029/2024SW004254
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author Zama T. Katamzi‐Joseph
John Bosco Habarulema
Yuichi Otsuka
Tshimangadzo M. Matamba
Amoré E. Nel
author_facet Zama T. Katamzi‐Joseph
John Bosco Habarulema
Yuichi Otsuka
Tshimangadzo M. Matamba
Amoré E. Nel
author_sort Zama T. Katamzi‐Joseph
collection DOAJ
description Abstract This study presents a statistical analysis of the occurrence rate of midlatitude nighttime medium scale traveling ionospheric disturbances (MSTIDs) that were detected in Swarm plasma density measurements from 2014 to 2023. Monthly and local time variations of MSTID occurrence rates are compared in four longitude sectors: America, Africa, Asia, and Pacific. The spatial distribution showed a longitudinal variation as the MSTIDs were abundant in the Pacific region and scarce in the African sector. While the MSTIDs had occurrence peaks during both solstices, the winter solstice peak dominated in all longitude sectors, representing a seasonal asymmetry. The local time variation of the MSTIDs revealed they occur predominantly during the post‐midnight hours in all longitude sectors. However, post‐sunset MSTIDs observations were enhanced over the Asian and Pacific sectors during the solstices. The longitudinal variation in the occurrence of MSTIDs is probably linked to the E–F coupling as it matched that of the nighttime sporadic E variation obtained from ionosonde measurements. While the winter dominance of MSTIDs matches that of gravity wave activity, the semiannual seasonal variation may be explained by interhemispheric E–F coupling. This indicates that gravity waves probably play a major role in seeding the MSTIDs observed in this study. Theoretical assessments of the longitudinal variations of MSTID driving mechanisms are needed to better understand the seasonal asymmetry and how it is affected by solar activity.
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spelling doaj-art-cef756ca6d8a4ac09635dddea411d8aa2025-08-20T03:09:16ZengWileySpace Weather1542-73902025-07-01237n/an/a10.1029/2024SW004254Characteristics of Nighttime Medium‐Scale Traveling Ionospheric Disturbances: Longitudinal Comparison of Their Seasonal and Local Time VariationsZama T. Katamzi‐Joseph0John Bosco Habarulema1Yuichi Otsuka2Tshimangadzo M. Matamba3Amoré E. Nel4SANSA Hermanus South AfricaSANSA Hermanus South AfricaInstitute for Space‐Earth Environmental Research Nagoya University Nagoya JapanSANSA Hermanus South AfricaSANSA Hermanus South AfricaAbstract This study presents a statistical analysis of the occurrence rate of midlatitude nighttime medium scale traveling ionospheric disturbances (MSTIDs) that were detected in Swarm plasma density measurements from 2014 to 2023. Monthly and local time variations of MSTID occurrence rates are compared in four longitude sectors: America, Africa, Asia, and Pacific. The spatial distribution showed a longitudinal variation as the MSTIDs were abundant in the Pacific region and scarce in the African sector. While the MSTIDs had occurrence peaks during both solstices, the winter solstice peak dominated in all longitude sectors, representing a seasonal asymmetry. The local time variation of the MSTIDs revealed they occur predominantly during the post‐midnight hours in all longitude sectors. However, post‐sunset MSTIDs observations were enhanced over the Asian and Pacific sectors during the solstices. The longitudinal variation in the occurrence of MSTIDs is probably linked to the E–F coupling as it matched that of the nighttime sporadic E variation obtained from ionosonde measurements. While the winter dominance of MSTIDs matches that of gravity wave activity, the semiannual seasonal variation may be explained by interhemispheric E–F coupling. This indicates that gravity waves probably play a major role in seeding the MSTIDs observed in this study. Theoretical assessments of the longitudinal variations of MSTID driving mechanisms are needed to better understand the seasonal asymmetry and how it is affected by solar activity.https://doi.org/10.1029/2024SW004254
spellingShingle Zama T. Katamzi‐Joseph
John Bosco Habarulema
Yuichi Otsuka
Tshimangadzo M. Matamba
Amoré E. Nel
Characteristics of Nighttime Medium‐Scale Traveling Ionospheric Disturbances: Longitudinal Comparison of Their Seasonal and Local Time Variations
Space Weather
title Characteristics of Nighttime Medium‐Scale Traveling Ionospheric Disturbances: Longitudinal Comparison of Their Seasonal and Local Time Variations
title_full Characteristics of Nighttime Medium‐Scale Traveling Ionospheric Disturbances: Longitudinal Comparison of Their Seasonal and Local Time Variations
title_fullStr Characteristics of Nighttime Medium‐Scale Traveling Ionospheric Disturbances: Longitudinal Comparison of Their Seasonal and Local Time Variations
title_full_unstemmed Characteristics of Nighttime Medium‐Scale Traveling Ionospheric Disturbances: Longitudinal Comparison of Their Seasonal and Local Time Variations
title_short Characteristics of Nighttime Medium‐Scale Traveling Ionospheric Disturbances: Longitudinal Comparison of Their Seasonal and Local Time Variations
title_sort characteristics of nighttime medium scale traveling ionospheric disturbances longitudinal comparison of their seasonal and local time variations
url https://doi.org/10.1029/2024SW004254
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