Overall Morphology of Prominent Zonal Differences in Low Latitude Ionosphere

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Yuyan Yang, Libo Liu, Wenbo Li, Xiukuan Zhao, Yiding Chen, Huijun Le, Ruilong Zhang, Jianyong Lu
{"title":"Overall Morphology of Prominent Zonal Differences in Low Latitude Ionosphere","authors":"Yuyan Yang,&nbsp;Libo Liu,&nbsp;Wenbo Li,&nbsp;Xiukuan Zhao,&nbsp;Yiding Chen,&nbsp;Huijun Le,&nbsp;Ruilong Zhang,&nbsp;Jianyong Lu","doi":"10.1029/2024JA033165","DOIUrl":null,"url":null,"abstract":"<p>This paper reports the overall morphology of prominent zonal differences in total electron content (TEC) data from Beidou geostationary orbit (GEO) satellites in the low latitude ionosphere over the Asia sector. Using GEO TEC observations from the GXZY receiver (26.2°N, 110.6°E) from 1 November 2019 to 30 November 2022, 64 prominent zonal difference events under geomagnetic quiet conditions were selected. We clarify the global longitude structures corresponding to these prominent zonal difference events at low latitudes through the global TEC products from the Massachusetts Institute of Technology. The structures that can cause the prominent zonal difference features in GEO TEC data are mainly divided into large-scale wave-like structures and featured regional structures. Among them, 19 cases of prominent zonal difference features were caused by large-scale wave-like structures, and 45 cases were caused by regional longitude structures. Prominent zonal differences generated from Large-scale wave-like structures are explained by the day-to-day variation of wave components, which creates an amplitude superposition and amplifies the crest intensity in a region. The featured regional structures cover a longitudinal range of about 10°–30°. In addition, we discussed the possible reasons for this small longitudinal structure by utilizing plasma drift velocity data at the magnetic equator from the Ionospheric Connection Explorer mission. The delicate longitude structures of vertical and zonal plasma drift likely contribute to the prominent zonal difference features in certain events.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"130 1","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2024-12-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JA033165","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

This paper reports the overall morphology of prominent zonal differences in total electron content (TEC) data from Beidou geostationary orbit (GEO) satellites in the low latitude ionosphere over the Asia sector. Using GEO TEC observations from the GXZY receiver (26.2°N, 110.6°E) from 1 November 2019 to 30 November 2022, 64 prominent zonal difference events under geomagnetic quiet conditions were selected. We clarify the global longitude structures corresponding to these prominent zonal difference events at low latitudes through the global TEC products from the Massachusetts Institute of Technology. The structures that can cause the prominent zonal difference features in GEO TEC data are mainly divided into large-scale wave-like structures and featured regional structures. Among them, 19 cases of prominent zonal difference features were caused by large-scale wave-like structures, and 45 cases were caused by regional longitude structures. Prominent zonal differences generated from Large-scale wave-like structures are explained by the day-to-day variation of wave components, which creates an amplitude superposition and amplifies the crest intensity in a region. The featured regional structures cover a longitudinal range of about 10°–30°. In addition, we discussed the possible reasons for this small longitudinal structure by utilizing plasma drift velocity data at the magnetic equator from the Ionospheric Connection Explorer mission. The delicate longitude structures of vertical and zonal plasma drift likely contribute to the prominent zonal difference features in certain events.

求助全文
约1分钟内获得全文 求助全文
来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信