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
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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 |
DOI | 10.1186/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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