IGGCAS OpenIR  > 地球与行星物理院重点实验室
Solar Dependence of Equatorial F Region Irregularities Observed by COSMIC Radio Occultations
Yu, Tao1,2; Miyoshi, Yasunobu2; Xia, Chunliang1; Zuo, Xiaomin1; Yan, Xiangxiang1; Yang, Na1; Sun, Yangyi1; Yue, Xinan3; Mao, Tian4
2018-11-01
Source PublicationJOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
ISSN2169-9380
Volume123Issue:11Pages:9775-9787
AbstractWith an improved method for retrieving the equatorial F region irregularities (EFIs) from radio occultation measurements, a huge amount of S4 index profiles from Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) satellites is employed to study the solar cycle variation of global EFIs during the period of 2007 to 2017. This full solar cycle data show that impacts of the solar activity on the occurrence rates and heights of EFIs are notable and complex. The occurrence rates of EFIs at higher altitude (greater than 500 km) increase with increasing the solar activity. The mean heights ((h) over tilde) and heights standard deviation (sigma(h)) of EFIs at higher altitudes do not show clearly the solar activity dependence. On the other hand, the occurrence rates of EFIs at entire altitudes (from 150 to 800 km) do not have clear relation with the solar activity. The (h) over tilde and sigma(h) of EFIs at entire altitudes increase with increasing the solar activity. Moreover, the dependence of the occurrence rates of EFIs on the solar activity are the strongest in the equinoxes, weaker in winter and weakest in summer. The electric fields and corresponding seasonal variation can account for the EFIs occurrence and height variation versus solar activities, and the EFIs at low altitudes seem to be related to the seed associated with atmospheric gravity wave.
DOI10.1029/2018JA025936
Funding OrganizationStrategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Exchange Program of National Institute of Information and Communications (NICT) ; International Exchange Program of National Institute of Information and Communications (NICT) ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Exchange Program of National Institute of Information and Communications (NICT) ; International Exchange Program of National Institute of Information and Communications (NICT) ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Exchange Program of National Institute of Information and Communications (NICT) ; International Exchange Program of National Institute of Information and Communications (NICT) ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Exchange Program of National Institute of Information and Communications (NICT) ; International Exchange Program of National Institute of Information and Communications (NICT)
WOS KeywordIONOSPHERIC PLASMA BUBBLES ; SPREAD-F ; LONGITUDINAL VARIABILITY ; GLOBAL CLIMATOLOGY ; CYCLE ; DMSP ; SCINTILLATION ; RELEVANT ; GPS/MET
Language英语
Funding ProjectStrategic Priority Research Program of Chinese Academy of Sciences[XDA17010207] ; National Natural Science Foundation of China[41574147] ; National Natural Science Foundation of China[41774164] ; International Exchange Program of National Institute of Information and Communications (NICT)
Funding OrganizationStrategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Exchange Program of National Institute of Information and Communications (NICT) ; International Exchange Program of National Institute of Information and Communications (NICT) ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Exchange Program of National Institute of Information and Communications (NICT) ; International Exchange Program of National Institute of Information and Communications (NICT) ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Exchange Program of National Institute of Information and Communications (NICT) ; International Exchange Program of National Institute of Information and Communications (NICT) ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; International Exchange Program of National Institute of Information and Communications (NICT) ; International Exchange Program of National Institute of Information and Communications (NICT)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000453227400059
PublisherAMER GEOPHYSICAL UNION
Citation statistics
Document Type期刊论文
Identifierhttp://ir.iggcas.ac.cn/handle/132A11/90296
Collection地球与行星物理院重点实验室
Corresponding AuthorYan, Xiangxiang
Affiliation1.China Univ Geosci, Inst Geophys & Geomat, Hubei Subsurface Multiscale Imaging Key Lab, Wuhan, Hubei, Peoples R China
2.Kyushu Univ, Dept Earth & Planetary Sci, Fukuoka, Fukuoka, Japan
3.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
4.China Meteorol Adm, Key Lab Space Weather, Natl Ctr Space Weather, Beijing, Peoples R China
Recommended Citation
GB/T 7714
Yu, Tao,Miyoshi, Yasunobu,Xia, Chunliang,et al. Solar Dependence of Equatorial F Region Irregularities Observed by COSMIC Radio Occultations[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2018,123(11):9775-9787.
APA Yu, Tao.,Miyoshi, Yasunobu.,Xia, Chunliang.,Zuo, Xiaomin.,Yan, Xiangxiang.,...&Mao, Tian.(2018).Solar Dependence of Equatorial F Region Irregularities Observed by COSMIC Radio Occultations.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,123(11),9775-9787.
MLA Yu, Tao,et al."Solar Dependence of Equatorial F Region Irregularities Observed by COSMIC Radio Occultations".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 123.11(2018):9775-9787.
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