Evolution processes of a group of equatorial plasma bubble (EPBs) simultaneously observed by ground-based and satellite measurements in the equatorial region of China | |
Sun, Longchang; Xu, Jiyao; Wang, Wenbin; Yuan, Wei; Zhu, Yajun; Sun, LC (reprint author), Chinese Acad Sci, Natl Space Sci Ctr, State Key Lab Space Weather, Beijing, Peoples R China.; Sun, LC (reprint author), Univ Chinese Acad Sci, Coll Earth Sci, Beijing, Peoples R China. | |
Department | 空间科学部 |
Source Publication | JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
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2017 | |
Volume | 122Issue:4Pages:4819-4836 |
ISSN | 2169-9380 |
Language | 英语 |
Abstract | This paper for the first time reports conjugate observations of a group of evolving equatorial plasma bubbles (EPBs) generated in the longitudinal sector of China on 4/5 November 2013 using simultaneous airglow and Communication/Navigation Outage Forecasting System (C/NOFS) observations. The airglow depletion structures seen by two all-sky airglow imagers had the same zonal wavelength as that of the longitudinally periodic electron density depletions observed by the C/NOFS satellite which occurred at almost the same time but at magnetically conjugate latitudes. Data from a VHF radar and a Digisonde were combined to investigate the evolution of the EPB group, including their generation, development, and dissipation. Results indicate that the EPB group developed from the bottomside large-scale wave-like structure (LSWS) at about 195-210 km height with a characteristic zonal wavelength and longitudinal extension of about 450 km and 2250 km, respectively. The EPB group also caused periodic bottomside type spread F associated with the LSWS. We found that the development of the EPB group and their associated spread F could be limited by the equatorward motion of equatorial ionization anomaly (EIA) and the southwestward motion of an extremely bright airglow region (SMEBAR). The SMEBAR is a newly discovered structure of plasma density increase but not a plasma blob reported before. Both EIA and SMEBAR could feed high plasma density into an EPB airglow depletion structure that was eventually seen as a bright airglow structure or disappeared. Meanwhile, spread F associated with the EPBs did not evolve from the bottomside type into the strong range type. |
Indexed By | SCI |
Document Type | 期刊论文 |
Identifier | http://ir.nssc.ac.cn/handle/122/5990 |
Collection | 空间科学部 |
Corresponding Author | Sun, LC (reprint author), Chinese Acad Sci, Natl Space Sci Ctr, State Key Lab Space Weather, Beijing, Peoples R China.; Sun, LC (reprint author), Univ Chinese Acad Sci, Coll Earth Sci, Beijing, Peoples R China. |
Recommended Citation GB/T 7714 | Sun, Longchang,Xu, Jiyao,Wang, Wenbin,et al. Evolution processes of a group of equatorial plasma bubble (EPBs) simultaneously observed by ground-based and satellite measurements in the equatorial region of China[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2017,122(4):4819-4836. |
APA | Sun, Longchang.,Xu, Jiyao.,Wang, Wenbin.,Yuan, Wei.,Zhu, Yajun.,...&Sun, LC .(2017).Evolution processes of a group of equatorial plasma bubble (EPBs) simultaneously observed by ground-based and satellite measurements in the equatorial region of China.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,122(4),4819-4836. |
MLA | Sun, Longchang,et al."Evolution processes of a group of equatorial plasma bubble (EPBs) simultaneously observed by ground-based and satellite measurements in the equatorial region of China".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 122.4(2017):4819-4836. |
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