污染气体扫描成像红外被动遥测系统实时数据处理研究

焦洋; 徐亮; 高闽光; 金岭; 童晶晶; 李胜; 魏秀丽

doi:10.7498/aps.62.140705

摘要

使用红外被动遥测技术可实现污染气体的远程监控和预警. 该技术应用过程中, 获取背景辐射是进行定量解析的关键, 在已有的应用中, 多采用同条件测量法和上风口测量方法获取背景光谱和环境光谱, 但这些方法均需要提前或者同时测量无目标物的背景光谱, 难以在实际应用中满足快速响应的需求. 本文基于红外辐射传输模型分析, 通过研究在800–1200 cm-1波段内的实测光谱中同时包含目标、背景和环境辐射的基本原理, 采用了一种不需要事先测量背景的目标特征的背景光谱实时提取算法, 通过将该方法应用于自主研制的污染气体扫描成像红外被动遥测系统, 以六氟化硫为示踪气体, 开展了遥测验证实验. 将获取的浓度数据与应用同条件测量法获取的数据进行了比较, 结果显示两者的相关系数平方值达到0.99, 表明该方法切实可行, 可有效提高系统的响应速度和适用范围.

关键词:

Abstract

Infrared passive remote sensing allows remote monitoring and early warning of air pollution. The key to the quantitative resolution is to obtain the background radiation in application process. The existing methods (such as measuring the background and atmosphere radiance spectrum in the same condition or uptake) need in advance or at the same time to measure the background spectrum without target. So, they are difficult to satisfy the demand for rapid response in the practical application. According to the infrared radiation transmission model analysis and by studying the principle of measured spectrum in the 800-1200 cm-1 band containing the target, background and environmental radiation, we propose a real-time spectrum extraction algorithm that does not require to measure the background target feature. The method is applied to the developed polluting gas scanning imaging passive FTIR system. The remote sensing of SF6 is done. Concentration data and the data obtained by the method at the same condition are compared, and the results show that the correlation coefficient squared value reaches 0.99, indicating that the method is feasible, which can effectively improve the response speed of the system and the scope of application.

Keywords:

Fourier transform infrared spectroscopy /
passive remote sensing /
real-time spectrum extraction algorithm

作者及机构信息

1.
中国科学院安徽光学精密机械研究所, 中国科学院环境光学与技术重点实验室, 合肥 230031

基金项目: 中国科学院战略性先导科技专项(B类)(批准号: XDB05040500)和国家自然科学基金(批准号: 40905011)资助的课题.

Authors and contacts

1.
Key Laboratory of Environment Optics and Technology, Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031 China

Funds: Project supported by the Strategic Priority Research Program(B) of the Chinese Academy of Sciences (Grant No. XDB05040500) and the National Natural Science Foundation of China (Grant No. 40905011).

参考文献

[1]	Zander R, Roland G, Delbouille L, Sauval A, Farmer C B, Norton R H 1987 J. Atmosph. Chem. 5 395
[2]	Flanigan D F 1986 Appl. Opt. 25 4253
[3]	Liu X, Murcray F J, Murcray D G, Russell J M 1996 J. Geophys. Res. 101 10175
[4]	Liu Z M, Liu W Q, Gao M G, Tong J J, Zhang T S, Xu L, Wei X L, Jin L, Wang Y P, Chen J 2010 Acta Phys. Sin. 59 5397 (in Chinese) [刘志明, 刘文清, 高闽光, 童晶晶, 张天舒, 徐亮, 魏秀丽, 金岭, 王亚萍, 陈军 2010 物理学报 59 5397]
[5]	Herget W F, Brasher J D 1980 Opt. Eng. 19 508
[6]	Heland J, Schäfer K 1997 Appl. Opt. 36 4922
[7]	Worden H, Beer R, Rinsland C P 1997 J. Geophys. Res. 102 1287
[8]	Theriault J, Puckrin E, Lavoie H, Turcotte C S, Bouffard F, Dube D 2004 Proc. SPIE 5584 100
[9]	Flanigan D F 1996 Appl. Opt. 35 6090
[10]	Wayne F, Evans J, Puckrin E, McMaster D 2002 Proc. SPIE 4574 44
[11]	Gao M G, Liu W Q, Zhang T S 2006 Spectrosc. Spec. Anal. 26 47 (in Chinese) [高闽光, 刘文清, 张天舒 2006 光谱学与光谱分析 26 47]
[12]	Cao T T, Luo S R, Zhao X Y, Liang H M, Wang H B, Yang J G 2007 Acta Phys. Sin. 56 5554 (in Chinese)［曹婷婷, 罗时荣, 赵晓艳, 梁慧敏, 王宏波, 杨经国 2007 物理学报 56 5554]
[13]	Jiao Y, Xu L, Gao M G, Feng M C, Jin L, Tong J J, Li S 2012 Spectrosc. Spec. Anal. 32 1754 (in Chinese) [焦洋, 徐亮, 高闽光, 冯明春, 金岭, 童晶晶, 李胜 2012 光谱学与光谱分析 32 1754]
[14]	Liu Z M, Liu W Q, Gao M G, Tong J J, Zhang T S, Xu L, Wei X L 2008 Chin. Phys. B 17 4184
[15]	Feng M C, Xu L, Gao M G, Jiao Y, Li X X, Jin L, Cheng S Y, Tong J J, Wei X L, Li S 2012 Infrared Technology 34 366 (in Chinese) [冯明春, 徐亮, 高闽光, 焦洋, 李相贤, 金岭, 程巳阳, 童晶晶, 魏秀丽, 李胜 2012 红外技术 34 366]

施引文献

[1]	Zander R, Roland G, Delbouille L, Sauval A, Farmer C B, Norton R H 1987 J. Atmosph. Chem. 5 395
[2]	Flanigan D F 1986 Appl. Opt. 25 4253
[3]	Liu X, Murcray F J, Murcray D G, Russell J M 1996 J. Geophys. Res. 101 10175
[4]	Liu Z M, Liu W Q, Gao M G, Tong J J, Zhang T S, Xu L, Wei X L, Jin L, Wang Y P, Chen J 2010 Acta Phys. Sin. 59 5397 (in Chinese) [刘志明, 刘文清, 高闽光, 童晶晶, 张天舒, 徐亮, 魏秀丽, 金岭, 王亚萍, 陈军 2010 物理学报 59 5397]
[5]	Herget W F, Brasher J D 1980 Opt. Eng. 19 508
[6]	Heland J, Schäfer K 1997 Appl. Opt. 36 4922
[7]	Worden H, Beer R, Rinsland C P 1997 J. Geophys. Res. 102 1287
[8]	Theriault J, Puckrin E, Lavoie H, Turcotte C S, Bouffard F, Dube D 2004 Proc. SPIE 5584 100
[9]	Flanigan D F 1996 Appl. Opt. 35 6090
[10]	Wayne F, Evans J, Puckrin E, McMaster D 2002 Proc. SPIE 4574 44
[11]	Gao M G, Liu W Q, Zhang T S 2006 Spectrosc. Spec. Anal. 26 47 (in Chinese) [高闽光, 刘文清, 张天舒 2006 光谱学与光谱分析 26 47]
[12]	Cao T T, Luo S R, Zhao X Y, Liang H M, Wang H B, Yang J G 2007 Acta Phys. Sin. 56 5554 (in Chinese)［曹婷婷, 罗时荣, 赵晓艳, 梁慧敏, 王宏波, 杨经国 2007 物理学报 56 5554]
[13]	Jiao Y, Xu L, Gao M G, Feng M C, Jin L, Tong J J, Li S 2012 Spectrosc. Spec. Anal. 32 1754 (in Chinese) [焦洋, 徐亮, 高闽光, 冯明春, 金岭, 童晶晶, 李胜 2012 光谱学与光谱分析 32 1754]
[14]	Liu Z M, Liu W Q, Gao M G, Tong J J, Zhang T S, Xu L, Wei X L 2008 Chin. Phys. B 17 4184
[15]	Feng M C, Xu L, Gao M G, Jiao Y, Li X X, Jin L, Cheng S Y, Tong J J, Wei X L, Li S 2012 Infrared Technology 34 366 (in Chinese) [冯明春, 徐亮, 高闽光, 焦洋, 李相贤, 金岭, 程巳阳, 童晶晶, 魏秀丽, 李胜 2012 红外技术 34 366]

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