中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Observation of Post-Sunset Equatorial Plasma Bubbles with BDS Geostationary Satellites over South China

文献类型:期刊论文

作者Ma, Guanyi6,7; Li, Jinghua6,7; Fan, Jiangtao6,7; Wan, Qingtao6,7; Maruyama, Takashi5,7; Dong L(董亮)4; Gao, Yang2,3; Zhang, Le2,3; Wang, Dong1
刊名REMOTE SENSING
出版日期2024-09
卷号16期号:18
关键词equatorial plasma bubble (EPB) temporal fluctuation of TEC (TFT) longitudinal variability wave-like structure
DOI10.3390/rs16183521
产权排序第4完成单位
文献子类Article
英文摘要An equatorial plasma bubble (EPB) is characterized by ionospheric irregularities which disturb radio waves by causing phase and amplitude scintillations or even signal loss. It is becoming increasingly important in space weather to assure the reliability of radio systems in both space and on the ground. This paper presents a newly established GNSS ionospheric observation network (GION) around the north equatorial ionization anomaly (EIA) crest in south China, which has a longitudinal coverage of similar to 30 degrees from 94 degrees E to 124 degrees E. The measurement with signals from geostationary earth orbit (GEO) satellites of the BeiDou navigation satellite system (BDS) is capable of separating the temporal and spatial variations of the ionosphere. A temporal fluctuation of TEC (TFT) parameter is proposed to characterize EPBs. The longitude of the EPBs' generation can be located with TFT variations in the time-longitude dimension. It is found that the post-sunset EPBs have a high degree of longitudinal variability. They generally show a quasiperiodic feature, indicating their association with atmospheric gravity wave activities. Wave-like structures with different scale sizes can co-exist in the same night.
学科主题地球科学
URL标识查看原文
出版地ST ALBAN-ANLAGE 66, CH-4052 BASEL, SWITZERLAND
WOS关键词SPREAD-F ; IRREGULARITIES ; SCINTILLATIONS
资助项目the National Natural Science Foundation of China[12073049]; the National Natural Science Foundation of China[12273062]; the National Natural Science Foundation of China[42150105]; National Natural Science Foundation of China[178GJHZ2023180MI]; CAS-JSPS Joint Research Project
WOS研究方向Environmental Sciences & Ecology ; Geology ; Remote Sensing ; Imaging Science & Photographic Technology
语种英语
WOS记录号WOS:001323093100001
出版者MDPI
资助机构the National Natural Science Foundation of China[12073049, 12273062, 42150105] ; National Natural Science Foundation of China[178GJHZ2023180MI] ; CAS-JSPS Joint Research Project
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/27630]  
专题云南天文台_射电天文研究组
作者单位1.Shenzhen Astronomical Observatory, Shenzhen 518121, China
2.CSST Science Center for the Guangdong-Hong Kong-Macau Great Bay Area, SYSU, Zhuhai 518082, China;
3.School of Physics and Astronomy, Sun Yat-sen University, Zhuhai 519082, China;
4.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China;
5.National Institute of Information and Communications Technology, Koganei 184-8795, Tokyo, Japan;
6.University of Chinese Academy of Sciences, Beijing 100049, China;
7.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;
推荐引用方式
GB/T 7714
Ma, Guanyi,Li, Jinghua,Fan, Jiangtao,et al. Observation of Post-Sunset Equatorial Plasma Bubbles with BDS Geostationary Satellites over South China[J]. REMOTE SENSING,2024,16(18).
APA Ma, Guanyi.,Li, Jinghua.,Fan, Jiangtao.,Wan, Qingtao.,Maruyama, Takashi.,...&Wang, Dong.(2024).Observation of Post-Sunset Equatorial Plasma Bubbles with BDS Geostationary Satellites over South China.REMOTE SENSING,16(18).
MLA Ma, Guanyi,et al."Observation of Post-Sunset Equatorial Plasma Bubbles with BDS Geostationary Satellites over South China".REMOTE SENSING 16.18(2024).

入库方式: OAI收割

来源:云南天文台

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