Peak height of OH airglow derived from simultaneous observations a Fabry-Perot interferometer and a meteor radar
Yu, Tao1; Zuo, Xiaomin1; Xia, Chunliang1; Li, Mingyuan1; Huang, Cong2; Mao, Tian2; Zhang, Xiaoxin2; Zhao, Biqiang3,4; Liu, Libo3,4
刊名JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
2017-04-01
卷号122期号:4页码:4628-4637
ISSN号2169-9380
DOI10.1002/2016JA023743
文献子类Article
英文摘要A new method for estimating daily averaged peak height of the OH airglow layer from a ground-based meteor radar (MR) and a Fabry-Perot interferometer (FPI) is presented. The first results are derived from 4 year simultaneous measurements of winds by a MR and a FPI at two adjacent stations over center China and are compared with observations from the Thermosphere Ionosphere Mesosphere Energetics and Dynamics/Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument. The OH airglow peak heights, which are derived by using correlation analysis between winds of the FPI and MR, are found to generally peak at an altitude of 87 km and frequently varied between 80 km and 90 km day to day. In comparison with SABER OH 1.6 mu m observations, reasonable similarity of airglow peak heights is found, and rapid day-to-day variations are also pronounced. Lomb-Scargle analysis is used to determine cycles of temporal variations of airglow peak heights, and there are obvious periodic variations both in our airglow peak heights and in the satellite observations. In addition to the annual, semiannual, monthly, and three monthly variations, the shorter time variations, e.g., day-to-day and several days' variations, are also conspicuous. The day-to-day variations of airglow height obviously could reduce observation accuracy and lead to some deviations in FPI measurements. These FPI wind deviations arising from airglow height variations are also estimated to be about 3-5 m/s from 2011 to 2015, with strong positive correlation with airglow peak height variation. More attention should be paid to the wind deviations associated with airglow height variation when using and interpreting winds measured by FPI.
WOS关键词UPPER-ATMOSPHERE RESEARCH ; WIND IMAGING INTERFEROMETER ; NIGHTGLOW EMISSIONS ; RESEARCH SATELLITE ; TEMPERATURE ; IMAGERS ; CHINA ; INSTRUMENT ; ALTITUDE ; O(S-1)
WOS研究方向Astronomy & Astrophysics
语种英语
出版者AMER GEOPHYSICAL UNION
WOS记录号WOS:000401340800054
资助机构National Natural Science Foundation of China(41574147 ; National High-tech R&D Program of China (863 Program)(2014AA123503/2014AA123501) ; 41231065 ; 41574145) ; National Natural Science Foundation of China(41574147 ; National High-tech R&D Program of China (863 Program)(2014AA123503/2014AA123501) ; 41231065 ; 41574145) ; National Natural Science Foundation of China(41574147 ; National High-tech R&D Program of China (863 Program)(2014AA123503/2014AA123501) ; 41231065 ; 41574145) ; National Natural Science Foundation of China(41574147 ; National High-tech R&D Program of China (863 Program)(2014AA123503/2014AA123501) ; 41231065 ; 41574145)
内容类型期刊论文
源URL[http://ir.iggcas.ac.cn/handle/132A11/52914]  
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Yu, Tao
作者单位1.China Univ Geosci, Inst Geophys & Geomat, Hubei Subsurface Multiscale Imaging Key Lab, Wuhan, Peoples R China
2.China Meteorol Adm, Natl Ctr Space Weather, Key Lab Space Weather, Beijing, Peoples R China
3.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
4.Univ Chinese Acad Sci, Coll Earth Sci, Beijing, Peoples R China
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GB/T 7714
Yu, Tao,Zuo, Xiaomin,Xia, Chunliang,et al. Peak height of OH airglow derived from simultaneous observations a Fabry-Perot interferometer and a meteor radar[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2017,122(4):4628-4637.
APA Yu, Tao.,Zuo, Xiaomin.,Xia, Chunliang.,Li, Mingyuan.,Huang, Cong.,...&Liu, Libo.(2017).Peak height of OH airglow derived from simultaneous observations a Fabry-Perot interferometer and a meteor radar.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,122(4),4628-4637.
MLA Yu, Tao,et al."Peak height of OH airglow derived from simultaneous observations a Fabry-Perot interferometer and a meteor radar".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 122.4(2017):4628-4637.
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