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碳卫星高光谱CO_2探测仪发射前光谱定标
引用本文:蔺超,李诚良,王龙,毕研盟,郑玉权.碳卫星高光谱CO_2探测仪发射前光谱定标[J].光学精密工程,2017,25(8):2064-2075.
作者姓名:蔺超  李诚良  王龙  毕研盟  郑玉权
作者单位:1. 中国科学院 长春光学精密机械与物理研究所, 吉林 长春 130033;2. 国家卫星气象中心, 北京 100081
基金项目:国家863高技术发展计划资助项目
摘    要:为了完成碳卫星高光谱CO_2探测仪的发射前光谱定标,建立了光谱定标系统,并对定标系统设计、所采用的自动化数据采集和数据处理算法等进行了研究。根据CO_2探测仪的探测原理介绍了载荷的光谱性能要求,描述了定标系统的设计与所采用的仪器设备,说明了采用自动化数据采集、旋转积分球、功率校正与暗背景校正等改进的定标方法。最后,介绍了光谱定标的数据处理方法。发射前定标结果表明:载荷三个波段的ILS能量集中度分别大于0.80,0.81和0.78;FWHM分别为0.039 2~0.042 4nm,0.123~0.128nm和0.157~0.168nm;光谱采样率区间分别为2.12~2.95、1.97~2.27和1.92~2.26。对发射后实测太阳夫朗禾费光谱进行了评估,结果表明:中心波长偏差小于0.0013,0.058和0.065nm。CO_2探测仪整体的光谱性能指标能够达到系统设计要求。

关 键 词:光学遥感  碳卫星  二氧化碳探测仪  光谱定标  线形函数
收稿时间:2017-03-27

Preflight spectral calibration of hyperspectral carbon dioxide spectrometer of TanSat
LIN Chao,LI Cheng-liang,WANG Long,BI Yan-meng,ZHENG Yu-quan.Preflight spectral calibration of hyperspectral carbon dioxide spectrometer of TanSat[J].Optics and Precision Engineering,2017,25(8):2064-2075.
Authors:LIN Chao  LI Cheng-liang  WANG Long  BI Yan-meng  ZHENG Yu-quan
Affiliation:1. Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, ChangChun 130033, China;2. National Satellite Meteorological Center, Beijing 100081, China
Abstract:In order to realize spectral calibration for TanSat''s hyperspectral Carbon Dioxide Spectrometer (CDS), a calibration system was established and relevant methodology such as design of the system, data acquisition and algorithms of data processing and etc was investigated.Based on the sounding principle, CDS''s spectral requirements were presented.Design of calibration system and the adopted equipments was described.Then after the scheme of Orbiting Carbon Observatory''s spectral calibration was compared, the modified methods such as automatic data acquisition, rotatable integrating sphere, power and dark calibration was analyzed.Finally, the methods of data processing were described as well.Experimental results indicate that the ILS concentration radios of CDS are more than 0.80, 0.81, 0.78 respectively and the intervals of FWHM are 0.039 2-0.042 4 nm, 0.123-0.128 nm, 0.157-0.168 nm respectively.The intervals of spectral sampling are 2.12-2.95, 1.97-2.27, 1.92-2.26 respectively.The comparison of on-orbit solar spectra indicate that the difference of central wavelength are less than 0.001 3, 0.058, 0.065 nm respectively.It can satisfy the system requirements of CDS.
Keywords:remote sensing  TanSat  carbon dioxide spectrometer  spectral calibration  instrument line shape(ILS)
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