中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
首页 机构 成果 学者
  
  1. CAS IR Grid
  2. 地质与地球物理研究所
  3. 中国科学院地质与地球物理研究所
  4. 中国科学院地球与行星物理重点实验室
Statistical characteristics of locally generated ESF during equinoctial months over Sanya

文献类型：期刊论文

作者Meng, Xing1; Fang, Hanxian1; Li, Guozhu2,3; Weng, Libin1
刊名ADVANCES IN SPACE RESEARCH
出版日期2018-05-01
卷号61期号:9页码:2227-2233
关键词Equatorial spread-F Local generation rate S4 and ROTI
ISSN号0273-1177
DOI10.1016/j.asr.2017.11.040
文献子类Article
英文摘要Understanding the local generation rate of equatorial spread-F (ESF) is important for forecasting ionospheric scintillation. Using the GPS ionospheric scintillation/TEC and VHF radar data during March-April and September-October from 2010 to 2014, the occurrence of ionospheric scintillation, TEC fast fluctuation, and backscatter plume were studied. Through analyzing the simultaneous occurrence of ionospheric scintillation, TEC fast fluctuation and backscatter plume, the local generation rate of ESF over Sanya was investigated. The results show that the monthly generation rate varies between 0% and 68%. A significant equinoctial asymmetry of local generation rate of ESF can be found in 2010, 2013 and 2014. The local generation rate of ESF increases from 2010 to 2014 during March-April, while it does not have similar trend during September-October. The plasma vertical drift influenced by solar activity has a significant impact on the monthly generation rate. The equinoctial asymmetry of plasma vertical drift may contribute a lot to the equinoctial asymmetry of the generation rate of ESF. (C) 2017 Published by Elsevier Ltd on behalf of COSPAR.
WOS关键词EQUATORIAL F-REGION ; F/PLASMA BUBBLE IRREGULARITIES ; FIELD-ALIGNED IRREGULARITIES ; SPREAD-F ; ATMOSPHERE RADAR ; BACKSCATTER PLUMES ; PLASMA BUBBLES ; SOLAR-CYCLE ; VHF RADAR ; DEPLETIONS
WOS研究方向Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences
语种英语
WOS记录号WOS:000430903800001
出版者ELSEVIER SCI LTD
资助机构Natural Science Foundation of China(40505005) ; Natural Science Foundation of China(40505005) ; Natural Science Foundation of China(40505005) ; Natural Science Foundation of China(40505005) ; Natural Science Foundation of China(40505005) ; Natural Science Foundation of China(40505005) ; Natural Science Foundation of China(40505005) ; Natural Science Foundation of China(40505005)
源URL[http://ir.iggcas.ac.cn/handle/132A11/88318]  
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Fang, Hanxian
作者单位1.Natl Univ Def Technol, Inst Meteorol & Oceanog, Nanjing 211101, Jiangsu, Peoples R China
2.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
3.Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing, Peoples R China
推荐引用方式
GB/T 7714		 Meng, Xing,Fang, Hanxian,Li, Guozhu,et al. Statistical characteristics of locally generated ESF during equinoctial months over Sanya[J]. ADVANCES IN SPACE RESEARCH,2018,61(9):2227-2233.
APA Meng, Xing,Fang, Hanxian,Li, Guozhu,&Weng, Libin.(2018).Statistical characteristics of locally generated ESF during equinoctial months over Sanya.ADVANCES IN SPACE RESEARCH,61(9),2227-2233.
MLA Meng, Xing,et al."Statistical characteristics of locally generated ESF during equinoctial months over Sanya".ADVANCES IN SPACE RESEARCH 61.9(2018):2227-2233.

入库方式： OAI收割

来源：地质与地球物理研究所

浏览0
下载0
收藏0
其他版本

除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。