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Simulation and application of the emission line O19P18 of O-2 (a(1)Delta(g) ) dayglow near 1.27 mu m for wind observations from limb-viewing satellites
Wu, Kuijun1; Fu, Di1; Feng, Yutao2; Li, Juan2; Hao, Xiongbo2; Li, Faquan1; Feng, YT (reprint author), Chinese Acad Sci, Xian Inst Opt & Precis Mech, Key Lab Spectral Imaging Technol, Xian 710119, Shaanxi, Peoples R China.
作者部门光谱成像技术实验室
2018-06-25
发表期刊OPTICS EXPRESS
ISSN1094-4087
卷号26期号:13页码:16984-16999
产权排序2
摘要

The O-2 (a(1)Delta(g)) emission near 1.27 gm has relatively bright signal and extended altitude coverage and provides an important means to remotely sense the compositional structures and dynamical features of the upper atmosphere globally. In this paper, we report the simulation and application of O-2 (a(1)Delta(g)) dayglow near 1.27 mu m for wind observations from limb-viewing satellites. A line by line radiative transfer model of the O-2 (a(1)Delta(g), v' = 0) -> O-2 (X-3 Sigma(g), v '' = 0) band is developed by taking both multiple scattering radiative transfer and nonlocal thermal equilibrium (non-LTE) models into account. The emission line O19P18 (7772.030 cm(-1)) with weak self-absorption, bright radiation intensity, and large spectral separation range is proved to be suitable for limb-viewing wind detection, due to its advantages of significantly lower cost, risk, and platform requirements. In order to ascertain the wind precision of O19P18, observations by a DASH-type (the Doppler asymmetric spatial heterodyne) instrument are simulated. The simulated results indicate a wind measurement precision of 1-2 m/s over an altitude range of 40 to 70 km in general, and possibly to 2-4 m/s due to a strong dependence on the spectral interference of the scattered sunlight background. (C) 2018 Optical Society of America under the terms of the OSA Open Access Publishing Agreement

学科领域Optics
DOI10.1364/OE.26.016984
收录类别SCI
语种英语
WOS研究方向Optics
WOS记录号WOS:000436226800075
引用统计
文献类型期刊论文
条目标识符http://ir.opt.ac.cn/handle/181661/30417
专题光谱成像技术实验室
通讯作者Feng, YT (reprint author), Chinese Acad Sci, Xian Inst Opt & Precis Mech, Key Lab Spectral Imaging Technol, Xian 710119, Shaanxi, Peoples R China.
作者单位1.Chinese Acad Sci, Wuhan Inst Phys & Math, Wuhan Natl Lab Optoelect, State Key Lab Magnet Resonance & Atom & Mol Phys, Wuhan 430071, Hubei, Peoples R China
2.Chinese Acad Sci, Xian Inst Opt & Precis Mech, Key Lab Spectral Imaging Technol, Xian 710119, Shaanxi, Peoples R China
推荐引用方式
GB/T 7714
Wu, Kuijun,Fu, Di,Feng, Yutao,et al. Simulation and application of the emission line O19P18 of O-2 (a(1)Delta(g) ) dayglow near 1.27 mu m for wind observations from limb-viewing satellites[J]. OPTICS EXPRESS,2018,26(13):16984-16999.
APA Wu, Kuijun.,Fu, Di.,Feng, Yutao.,Li, Juan.,Hao, Xiongbo.,...&Feng, YT .(2018).Simulation and application of the emission line O19P18 of O-2 (a(1)Delta(g) ) dayglow near 1.27 mu m for wind observations from limb-viewing satellites.OPTICS EXPRESS,26(13),16984-16999.
MLA Wu, Kuijun,et al."Simulation and application of the emission line O19P18 of O-2 (a(1)Delta(g) ) dayglow near 1.27 mu m for wind observations from limb-viewing satellites".OPTICS EXPRESS 26.13(2018):16984-16999.
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