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A New Method for Deriving Equatorial Plasma Bubble Velocity by Tracing OI 630 nm All-Sky Images
Yu, Tao1,2; Li, Mingyuan1; Xia, Chunliang1; Zuo, Xiaomin1; Liu, Zhizhao2; Zhao, Biqiang3,4
2018-11-01
Source PublicationJOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
ISSN2169-9380
Volume123Issue:11Pages:9619-9633
AbstractA new method for estimating the equatorial plasma bubbles (EPBs) motions from airglow emission all-sky images is presented in this paper. This method, which is called cloud motion wind (CMW) and widely used in satellite observation of wind, could reasonably derive zonal and meridional velocity vectors of EPBs drift by tracking a series of successive airglow images. Airglow emission images data are available from all-sky airglow camera in Hainan Fuke (19.5 degrees N, 109.2 degrees E) supported by China Meridional Project, which can receive the 630.0 nm emission from ionosphere F region at low latitudes to observe plasma bubbles. A series of pretreatment technology is utilized to preprocess the raw observation. Then the regions of plasma bubble extracted from the images are divided into several small tracing windows, and each tracing window can find a target window in the searching area in following image, which is considered as the position tracing window moved to. According to this, velocity of each tracing window was calculated by CMW. The maximum correlation coefficient is adopted to analyze the velocity of plasma bubbles due to its better performance than histogram of oriented gradient. All-sky images from Hainan Fuke, an example on 17 September 2014, are analyzed to investigate the plasma bubble drift velocities using CMW. For comparison and validation, EPBs motions obtained from three traditional methods are also investigated. The advantages and disadvantages of using CMW are discussed. The results of CMW are compared with slant total electron contents data and show a good consistency, but some errors are also discussed.
DOI10.1029/2018JA025332
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 ; 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 ; 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 ; 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
WOS KeywordDRIFT
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[41231065] ; National Natural Science Foundation of China[4154145]
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 ; 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 ; 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 ; 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
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000453227400049
PublisherAMER GEOPHYSICAL UNION
Citation statistics
Document Type期刊论文
Identifierhttp://ir.iggcas.ac.cn/handle/132A11/90270
Collection地球与行星物理院重点实验室
Corresponding AuthorYu, Tao
Affiliation1.China Univ Geosci, Hubei Subsurface Multiscale Imaging Key Lab, Inst Geophys & Geomat, Wuhan, Hubei, Peoples R China
2.Hong Kong Polytech Univ PolyU, Dept Land Surveying & Geoinformat, Kowloon, Hong Kong, Peoples R China
3.Chinese Acad Sci, Key Lab Earth & Planetary Phys, Inst Geol & Geophys, Beijing, Peoples R China
4.Univ Chinese Acad Sci, Coll Earth Sci, Beijing, Peoples R China
Recommended Citation
GB/T 7714
Yu, Tao,Li, Mingyuan,Xia, Chunliang,et al. A New Method for Deriving Equatorial Plasma Bubble Velocity by Tracing OI 630 nm All-Sky Images[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2018,123(11):9619-9633.
APA Yu, Tao,Li, Mingyuan,Xia, Chunliang,Zuo, Xiaomin,Liu, Zhizhao,&Zhao, Biqiang.(2018).A New Method for Deriving Equatorial Plasma Bubble Velocity by Tracing OI 630 nm All-Sky Images.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,123(11),9619-9633.
MLA Yu, Tao,et al."A New Method for Deriving Equatorial Plasma Bubble Velocity by Tracing OI 630 nm All-Sky Images".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 123.11(2018):9619-9633.
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