中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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
出版日期2017-11-01
卷号122期号:11页码:11665-11676
ISSN号2169-9380
DOI10.1002/2017JA024637
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/132A11/82506]  
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.

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来源:地质与地球物理研究所

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