Wide-field auroral imager onboard the Fengyun satellite

doi:10.1038/s41377-019-0157-7

CORC > 地质与地球物理研究所 > 中国科学院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

	Wide-field auroral imager onboard the Fengyun satellite
	Zhang, Xiao-Xin 1,2; Chen, Bo 3,4; He, Fei 5,6; Song, Ke-Fei 3,4; He, Ling-Ping 3,4; Liu, Shi-Jie 3,4; Guo, Quan-Feng 3; Li, Jia-Wei 1,2; Wang, Xiao-Dong 3; Zhang, Hong-Ji 3
刊名	LIGHT-SCIENCE & APPLICATIONS
	2019-05-22
卷号	8 页码:12
ISSN号	2047-7538
DOI	10.1038/s41377-019-0157-7
英文摘要	The newly launched Fengyun-3D (FY-3D) satellite carried a wide-field auroral imager (WAI) that was developed by Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences (CIOMP), which will provide a large field of view (FOV), high spatial resolution, and broadband ultraviolet images of the aurora and the ionosphere by imaging the N-2 LBH bands of emissions. The WAI consists of two identical cameras, each with an FOV of 68 degrees in the along-track direction and 10 degrees in the cross-track direction. The two cameras are tilted relative to each other to cover a fan-shaped field of size 130 degrees x 10 degrees. Each camera consists of an unobstructed four-mirror anastigmatic optical system, a BaF2 filter, and a photon-counting imaging detector. The spatial resolution of WAI is similar to 10 km at the nadir point at a reference height of 110 km above the Earth's surface. The sensitivity is >0.01 counts s(-1) Rayleigh(-1) pixel(-1) (140-180 nm) for both cameras, which is sufficient for mapping the boundaries and the fine structures of the auroral oval during storms/substorms. Based on the tests and calibrations that were conducted prior to launch, the data processing algorithm includes photon signal decoding, geometric distortion correction, photometric correction, flat-field correction, line-of-sight projection and correction, and normalization between the two cameras. Preliminarily processed images are compared with DMSP SSUSI images. The agreement between the images that were captured by two instruments demonstrates that the WAI and the data processing algorithm operate normally and can provide high-quality scientific data for future studies on auroral dynamics.
资助项目	National Science Foundation of China[41774152] ; National Science Foundation of China[41674155] ; Strategic Priority Research Program of Chinese Academy of Sciences[XDA17010201] ; Youth Innovation Promotion Association of the Chinese Academy of Sciences[2017258]
WOS关键词	ULTRAVIOLET IMAGER ; SPACECRAFT
WOS研究方向	Optics
语种	英语
出版者	NATURE PUBLISHING GROUP
WOS记录号	WOS:000469499000002
资助机构	National Science Foundation of China ; National Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; National Science Foundation of China ; National Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; National Science Foundation of China ; National Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; National Science Foundation of China ; National Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences
内容类型	期刊论文
源URL	[http://ir.iggcas.ac.cn/handle/132A11/92263]
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	Zhang, Xiao-Xin; Chen, Bo
作者单位	1.China Meteorol Adm, Natl Satellite Meteorol Ctr, Beijing, Peoples R China 2.China Meteorol Adm, Natl Ctr Space Weather, Key Lab Space Weather, Beijing, Peoples R China 3.Chinese Acad Sci, Changchun Inst Opt Fine Mech & Phys, Changchun, Jilin, Peoples R China 4.Chinese Acad Sci, State Key Lab Appl Opt, Changchun, Jilin, Peoples R China 5.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China 6.Chinese Acad Sci, Inst Earth Sci, Beijing, Peoples R China
推荐引用方式 GB/T 7714	Zhang, Xiao-Xin,Chen, Bo,He, Fei,et al. Wide-field auroral imager onboard the Fengyun satellite[J]. LIGHT-SCIENCE & APPLICATIONS,2019,8:12.
APA	Zhang, Xiao-Xin.,Chen, Bo.,He, Fei.,Song, Ke-Fei.,He, Ling-Ping.,...&Wang, Jin-Song.(2019).Wide-field auroral imager onboard the Fengyun satellite.LIGHT-SCIENCE & APPLICATIONS,8,12.
MLA	Zhang, Xiao-Xin,et al."Wide-field auroral imager onboard the Fengyun satellite".LIGHT-SCIENCE & APPLICATIONS 8(2019):12.