The Storm Time Evolution of the Ionospheric Disturbance Plasma Drifts
文献类型:期刊论文
作者 | Zhang, Ruilong1,2,3,4; Liu, Libo1,2,3,4; Le, Huijun1,2,3,4; Chen, Yiding1,2,3,4; Kuai, Jiawei5 |
刊名 | JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
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出版日期 | 2017-11-01 |
卷号 | 122期号:11页码:11665-11676 |
ISSN号 | 2169-9380 |
DOI | 10.1002/2017JA024637 |
文献子类 | Article |
英文摘要 | In this paper, we use the C/NOFS and ROCSAT-1 satellites observations to analyze the storm time evolution of the disturbance plasma drifts in a 24 h local time scale during three magnetic storms driven by long-lasting southward IMF B-z. The disturbance plasma drifts during the three storms present some common features in the periods dominated by the disturbance dynamo. The newly formed disturbance plasma drifts are upward and westward at night, and downward and eastward during daytime. Further, the disturbance plasma drifts are gradually evolved to present significant local time shifts. The westward disturbance plasma drifts gradually migrate from nightside to dayside. Meanwhile, the dayside downward disturbance plasma drifts become enhanced and shift to later local time. The local time shifts in disturbance plasma drifts are suggested to be mainly attributed to the evolution of the disturbance winds. The strong disturbance winds arisen around midnight can constantly corotate to later local time. At dayside the westward and equatorward disturbance winds can drive the F region dynamo to produce the poleward and westward polarization electric fields (or the westward and downward disturbance drifts). The present results indicate that the disturbance winds corotated to later local time can affect the local time features of the disturbance dynamo electric field. |
WOS关键词 | F-REGION ; ELECTRIC-FIELDS ; LOW LATITUDES ; DYNAMO ; ELECTRODYNAMICS ; THERMOSPHERE ; SATELLITE ; WINDS |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000419938600048 |
出版者 | AMER GEOPHYSICAL UNION |
资助机构 | National Natural Science Foundation of China(41231065 ; National Natural Science Foundation of China(41231065 ; National Natural Science Foundation of China(41231065 ; National Natural Science Foundation of China(41231065 ; National Important Basic Research Project of China(2012CB825604) ; National Important Basic Research Project of China(2012CB825604) ; National Important Basic Research Project of China(2012CB825604) ; National Important Basic Research Project of China(2012CB825604) ; 41621063) ; 41621063) ; 41621063) ; 41621063) ; National Natural Science Foundation of China(41231065 ; National Natural Science Foundation of China(41231065 ; National Natural Science Foundation of China(41231065 ; National Natural Science Foundation of China(41231065 ; National Important Basic Research Project of China(2012CB825604) ; National Important Basic Research Project of China(2012CB825604) ; National Important Basic Research Project of China(2012CB825604) ; National Important Basic Research Project of China(2012CB825604) ; 41621063) ; 41621063) ; 41621063) ; 41621063) ; National Natural Science Foundation of China(41231065 ; National Natural Science Foundation of China(41231065 ; National Natural Science Foundation of China(41231065 ; National Natural Science Foundation of China(41231065 ; National Important Basic Research Project of China(2012CB825604) ; National Important Basic Research Project of China(2012CB825604) ; National Important Basic Research Project of China(2012CB825604) ; National Important Basic Research Project of China(2012CB825604) ; 41621063) ; 41621063) ; 41621063) ; 41621063) ; National Natural Science Foundation of China(41231065 ; National Natural Science Foundation of China(41231065 ; National Natural Science Foundation of China(41231065 ; National Natural Science Foundation of China(41231065 ; National Important Basic Research Project of China(2012CB825604) ; National Important Basic Research Project of China(2012CB825604) ; National Important Basic Research Project of China(2012CB825604) ; National Important Basic Research Project of China(2012CB825604) ; 41621063) ; 41621063) ; 41621063) ; 41621063) |
源URL | [http://ir.iggcas.ac.cn/handle/132A11/82504] ![]() |
专题 | 中国科学院地质与地球物理研究所 |
通讯作者 | Liu, Libo |
作者单位 | 1.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China 2.Chinese Acad Sci, Inst Earth Sci, Beijing, Peoples R China 3.Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing, Peoples R China 4.Univ Chinese Acad Sci, Coll Earth Sci, Beijing, Peoples R China 5.Nanjing Univ Aeronaut & Astronaut, Coll Astronaut, Nanjing, Jiangsu, Peoples R China |
推荐引用方式 GB/T 7714 | Zhang, Ruilong,Liu, Libo,Le, Huijun,et al. The Storm Time Evolution of the Ionospheric Disturbance Plasma Drifts[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2017,122(11):11665-11676. |
APA | Zhang, Ruilong,Liu, Libo,Le, Huijun,Chen, Yiding,&Kuai, Jiawei.(2017).The Storm Time Evolution of the Ionospheric Disturbance Plasma Drifts.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,122(11),11665-11676. |
MLA | Zhang, Ruilong,et al."The Storm Time Evolution of the Ionospheric Disturbance Plasma Drifts".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 122.11(2017):11665-11676. |
入库方式: OAI收割
来源:地质与地球物理研究所
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