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Yuanhe Tang, Xiaodong Duan, Haiyang Gao, et all.. Ground-based airglow imaging interferometer. Part 2: forward model and inverse method. Applied Optics, 53(11): 2273-2282, 2014.
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Ground-based airglow imaging interferometer. Part 2: forward model and inverse method


×÷Õß:Tang, YH (Tang, Yuanhe)[ 1 ] ; Duan, XD (Duan, Xiaodong)[ 1 ] ; Gao, HY (Gao, Haiyang)[ 1,2,3 ] ; Qu, OY (Qu, Ouyang)[ 1 ] ; Jia, QJ (Jia, Qijie)[ 1 ] ; Cao, XG (Cao, Xiangang)[ 1 ] ; Wei, SN (Wei, Shenni)[ 1 ] ; Yang, R (Yang, Rui)[ 1 ]




APPLIED OPTICS



¾í: 53

ÆÚ: 11

Ò³: 2273-2282

DOI: 10.1364/AO.53.002273

³ö°æÄê: APR 10 2014

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The ground-based airglow imaging interferometer (GBAII) observes the nighttime airglow of the O-2(0-1) 867.7 nm line, peaked at 94 km altitude, to measure the upper atmospheric wind and temperature field. Its forward model, a code package in interactive data language (IDL), is developed to simulate the expected imaging interference fringes. It includes eight modules to simulate the light source, the atmospheric radiation transmission, the wide- angle Michelson interferometer, the interference filter, the optical system decay function, the responsivity, the imaging CCD, and the noises. The inverse method is also developed for obtaining the rest phase calibration, temperature, and wind. By means of both theoretical tools, we carry out a comparison of theoretical results with a field observation case. The apparent quantities J(1-p) from the forward model has the deviation of 1.5%-2.5% compared with that from the observation image. The temperature falls mainly in the range of 167-196 K with the precision of 2 K. The zonal and meridional winds are mainly in the region of 5.1 to 46.5 m/s and 12.5 to 48.3 m/s respectively, with errors of 13.2 to 21.5 m/s. The consistent trends between the observation results and standard models (MSISE90 and HWM93) suggest that the forward model and inverse method are suitable for GBAII. (C) 2014 Optical Society of America


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KeyWords Plus:ANGLE MICHELSON INTERFEROMETER; GRAVITY-WAVES; TEMPERATURE; INSTRUMENT; IMAGER; SATELLITE; EMISSION; WINDS


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ͨѶ×÷ÕßµØÖ·: Tang, YH (ͨѶ×÷Õß)





Xian Univ Technol, Sch Sci, 5 South Jinhua Rd, Xian 710048, Peoples R China.





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[ 1 ] Xian Univ Technol, Sch Sci, Xian 710048, Peoples R China







[ 2 ] Xian Univ Technol, Sch Mech & Precis Instrument Engn, Xian 710048, Peoples R China







[ 3 ] Nanjing Univ Informat Sci & Technol, Sch Atmospher Phys, Nanjing 210044, Peoples R China





µç×ÓÓʼþµØÖ·:ltp1801@163.com


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National Natural Science Foundation of China


10874138

41027004

61275185

41304124



Education Office of Shaanxi Province


09JK653



Excellent Doctoral Dissertation Fund of Xi'an University of Technology


101211104

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OPTICAL SOC AMER, 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA


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ÎÄÏ×ÀàÐÍ:Article

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Èë²ØºÅ: WOS:000334165100002

ISSN: 1559-128X

µç×Ó ISSN: 2155-3165


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