中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Simulated east–west differences in F-region peak electron density at Far East mid-latitude region

文献类型:期刊论文

作者Ren,Zhipeng1,2,3,4; Zhao,Biqiang1,2,3,4; Wan,Weixing1,2,3,4; Liu,Libo1,2,3,4; Li,Xing5,6; Yu,Tingting1,2,3,4
刊名Earth, Planets and Space
出版日期2020-04-15
卷号72期号:1
关键词Ionospheric east–west difference Ionospheric longitudinal variation Ionospheric region anomalies Mid-latitude ionosphere Ionosphere–thermosphere coupling
DOI10.1186/s40623-020-01175-5
英文摘要AbstractUsing TIME3D-IGGCAS model, we simulated the east–west differences in F-region peak electron density (NmF2) in the Far East mid-latitude region near the longitudinal sectors with very clear zonal variations of geomagnetic declination, and mainly analyzed the influence of the geomagnetic field configuration on the east–west differences. We found that, after removing the longitudinal variations of neutral parameters, TIME3D-IGGCAS can better represent the observed relative east–west difference (Rew) features. Rew is mainly negative (West NmF2?>?East NmF2) at noon and positive (East NmF2?>?West NmF2) at evening–night. The magnitude of daytime negative Rew is weaker in winter and stronger in summer, and the daytime Rew shows two negative peaks around two equinoxes. With the increasing solar flux level, the magnitude of Rew mainly becomes larger, and the two daytime negative peaks slightly shift to June Solstice. With the decreasing geographical latitude, Rew mainly becomes positive, and the two daytime negative peaks slightly shift to June Solstice. Our simulation also suggested that the thermospheric zonal wind plays an important role in the formation of the ionospheric east–west differences in the Far East mid-latitude region. The observed solar activity dependency of the ionospheric EW differences may be driven primarily by corresponding zonal wind changes with solar activity, whereas the observed latitudinal dependency of the differences is associated with primarily zonal wind and secondarily meridional wind latitudinal variations.
语种英语
WOS记录号BMC:10.1186/S40623-020-01175-5
出版者Springer Berlin Heidelberg
源URL[http://ir.iggcas.ac.cn/handle/132A11/94043]  
专题地质与地球物理研究所_中国科学院地球与行星物理重点实验室
通讯作者Ren,Zhipeng
作者单位1.Chinese Academy of Sciences; Beijing National Observatory of Space Environment, Institute of Geology and Geophysics
2.University of the Chinese Academy of Sciences; College of Earth and Planetary Sciences
3.Chinese Academy of Sciences; Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics
4.Chinese Academy of Sciences; Innovation Academy for Earth Science
5.Ministry of Industry and Information Technology; Key Laboratory of Space Environment Monitoring and Information Processing
6.Beihang University; School of Space and Environment
推荐引用方式
GB/T 7714
Ren,Zhipeng,Zhao,Biqiang,Wan,Weixing,et al. Simulated east–west differences in F-region peak electron density at Far East mid-latitude region[J]. Earth, Planets and Space,2020,72(1).
APA Ren,Zhipeng,Zhao,Biqiang,Wan,Weixing,Liu,Libo,Li,Xing,&Yu,Tingting.(2020).Simulated east–west differences in F-region peak electron density at Far East mid-latitude region.Earth, Planets and Space,72(1).
MLA Ren,Zhipeng,et al."Simulated east–west differences in F-region peak electron density at Far East mid-latitude region".Earth, Planets and Space 72.1(2020).

入库方式: OAI收割

来源:地质与地球物理研究所

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