留言板

尊敬的读者、作者、审稿人, 关于本刊的投稿、审稿、编辑和出版的任何问题, 您可以本页添加留言。我们将尽快给您答复。谢谢您的支持!

姓名
邮箱
手机号码
标题
留言内容
验证码

基于 掩星吸收光谱的二氧化碳探测技术

王玉诏,陶宇亮,孙海青,杨超

downloadPDF
王玉诏, 陶宇亮, 孙海青, 杨超. 基于 掩星吸收光谱的二氧化碳探测技术[J]. , 2021, 14(3): 634-642. doi: 10.37188/CO.2020-0201
引用本文: 王玉诏, 陶宇亮, 孙海青, 杨超. 基于 掩星吸收光谱的二氧化碳探测技术[J]. , 2021, 14(3): 634-642.doi:10.37188/CO.2020-0201
WANG Yu-Zhao, TAO Yu-Liang, SUN Hai-Qing, YANG Chao. Carbon dioxide detection technology based on the laser occultation absorption spectrum[J]. Chinese Optics, 2021, 14(3): 634-642. doi: 10.37188/CO.2020-0201
Citation: WANG Yu-Zhao, TAO Yu-Liang, SUN Hai-Qing, YANG Chao. Carbon dioxide detection technology based on the laser occultation absorption spectrum[J].Chinese Optics, 2021, 14(3): 634-642.doi:10.37188/CO.2020-0201

基于 掩星吸收光谱的二氧化碳探测技术

doi:10.37188/CO.2020-0201
基金项目:民用航天十三五预研项目资助(No. D040105)
详细信息
    作者简介:

    王玉诏(1984—),男,河北南宫人,博士,高级工程师,2011年于北京理工大学获得工学博士学位,主要研究领域为 雷达、 遥感. E-mail:zz0525wyz@163.com

  • 中图分类号:P407.5, P412.27

Carbon dioxide detection technology based on the laser occultation absorption spectrum

Funds:Supported by Civil Aerospace 13 th Five-Year Pre-research Project (No. D040105)
More Information
  • 摘要:本文分析了固定波长 掩星差分吸收技术的优点和不足,介绍了可调谐 直接吸收光谱技术测量原理。分析了最优波长透过率与信噪比的关系以及测量误差与背景光干扰的关系。根据高灵敏度探测器的工作波长范围,选择了6310.915 cm −1、6310.893 cm −1、6310.890 cm −1、6310.8834 cm −1作为吸收的工作波长,同时选择6310.15 cm −1作为参考波长,并对各波长的探测能力进行了仿真分析。通过仿真结果可知,在1 km垂直分辨率下,在5~35 km内CO 2浓度探测误差优于0.9%,7~42 km范围内的探测误差优于0.4%。该技术降低了系统成本和复杂度,有利于星载产品的设计和实现。

  • 图 1直接吸收光谱 掩星探测原理

    Figure 1.Detection principle of laser occultation direct absorption spectroscopy

    图 2信噪比SNR与透过率关系

    Figure 2.The relationship ofSNRand transmissionT

    图 3(a)背景光谱与(b)CO2光谱对比(波数ν范围5882 cm−1~7143 cm−1,高度5 km)

    Figure 3.Comparison of (a) background spectrum and (b) CO2spectrum (The range of wave numberνis 5882 cm−1~7143 cm−1and the height is 5 km.)

    图 4背景光谱干扰误差

    Figure 4.Error caused by background spectral interference

    (λonis 6310.915 cm−1@ 5~10 km, 6310.893 cm−1@ 11~18 km, 6310.890 cm−1@ 19~26 km, 6310.8834 cm−1@ 27~39 km, andλoffis 6310.15 cm−1)

    图 5探测信噪比仿真结果

    Figure 5.Simulation results of detectionSNR

    图 6累积次数的高度分布

    Figure 6.Height distribution of cumulative times

    图 7探测误差随高度分布

    Figure 7.Distribution of detection error varying with height

    表 1系统仿真参数

    Table 1.System simulation parameters

    System parameter Value Unit
    Orbit altitude of laser transmitter 500 km
    Orbit altitude of laser receiver 600 km
    repetition rate 40 Hz
    Laser power 1 W
    Laser wavenumber 6309.8834~6311.8834 cm−1
    Absorption wavenumber 6310.915@5~10 km, 6310.893@11~18 km,
    6310.890@19~26 km, 6310.8834 @27~39 km
    cm−1
    Reference wavenumber 6310.15 cm−1
    Laser line width 10 MHz
    Laser beam divergence 0.3 mrad
    Telescope diameter 0.3 m
    System optical efficiency 0.5 1
    Detector responsivity (InGaAs-APD,
    C30662, 1584.6 nm)
    10.3 A/W
    Nominal gain 10 1
    Noise factor 5.5 1
    Dark current 45 nA
    Spectral noise current 0.7 pA/rt (Hz)
    Bandwidth 3000 Hz
    下载: 导出CSV
  • [1] IPCC.Climate Change 2014:Impacts,Adaptation,and Vulnerability[M]. Cambridge: Cambridge University Press, 2014.
    [2] 熊伟. 高分五号卫星大气主要温室气体监测仪优化设计及数据分析[J]. 上海航天,2019,36(S2):167-172.

    XIONG W. Optimum design and data analysis of greenhouse gases monitoring instrument on GF-5satellite[J].Aerospace Shanghai, 2019, 36(S2): 167-172. (in Chinese)
    [3] FRANKENBERG C, POLLOCK R, LEE R A M,et al. The Orbiting Carbon Observatory (OCO-2): spectrometer performance evaluation using pre-launch direct sun measurements[J].Atmospheric Measurement Techniques, 2015, 8(1): 301-313.doi:10.5194/amt-8-301-2015
    [4] 谢杨易, 刘继桥, 姜佳欣, 等. 使CO2浓度测量误差减小的星载 雷达波长优化[J]. 红外与 工程,2014,43(1):88-93.doi:10.3969/j.issn.1007-2276.2014.01.015

    XIE Y Y, LIU J Q, JIANG J X,et al. Wavelengths optimization to decrease error for a space-borne lidar measuring CO2concentration[J].Infrared and Laser Engineering, 2014, 43(1): 88-93. (in Chinese)doi:10.3969/j.issn.1007-2276.2014.01.015
    [5] 宗雪梅. 大气红外辐射超高光谱探测仪临边探测—污染气体的反演精度和光谱通道评估[J]. 环境科学学报,2020,40(4):1410-1421.

    ZONG X M. Inversion accuracy and spectral channel evaluation of atmospheric polluted gases of atmospheric infrared radiation ultra-high detector under limb sounding[J].Acta Scientiae Circumstantiae, 2020, 40(4): 1410-1421. (in Chinese)
    [6] 王雅鹏, 李小英, 陈良富, 等. 红外临边探测发展现状[J]. 遥感学报,2016,20(4):513-527.

    WANG Y P, LI X Y, CHEN L F,et al. Overview of infrared limb sounding[J].Journal of Remote Sensing, 2016, 20(4): 513-527. (in Chinese)
    [7] KIRCHENGAST G. ACCURATE-Climate benchmark profiling of greenhouse gases and thermo-dynamic variables and wind from space, ESA Earth Explorer Opportunity Mission EE8 Proposal, Scientific Report 36-2010[R]. Graz, Austria: Wegener Center Verlag, 2010.
    [8] 李文冬, 刘继桥, 朱亚丹, 等. LEO-LEO红外 掩星CO2浓度测量技术研究[J]. 中国 ,2019,46(8):0810001.doi:10.3788/CJL201946.0810001

    LI W D, LIU J Q, ZHU Y D,et al. LEO-LEO infrared laser occultation technique to measure atmospheric carbon dioxide concentration[J].Chinese Journal of Lasers, 2019, 46(8): 0810001. (in Chinese)doi:10.3788/CJL201946.0810001
    [9] MOTTINI S, LOESCHER A, AGUIRRE M. A new approach to climatology from space: laser occultation[J].Proceedings of SPIE, 2010, 10565: 1056565.
    [10] 苏俊宏, 尚小燕, 弥谦. 光电技术基础[M]. 北京: 国防工业出版社, 2011.

    SU J H, SHANG X Y, MI Q.Fundamentals of Photoelectric Technology[M]. Beijing: National Defense Industry Press, 2011. (in Chinese)
    [11] 王玉诏, 陶宇亮, 杨超, 等. 一种基于可调谐 的掩星大气密度廓线测量系统及方法: 中国, 201911032531.8[P]. 2019-10-28.

    WANG Y ZH, TAO Y L, YANG CH,et al.. Occultation atmospheric density profile measurement system and method based on tunable laser: CN, 201911032531.8[P]. 2019-10-28. (in Chinese)
    [12] C30659 Series-900/1060/1550/1550E[R]. Excelitas Technologies, 2012.
    [13] WERLE P. Tunable diode laser absorption spectroscopy: recent findings and novel approaches[J].Infrared Physics&Technology, 1996, 37(l): 59-66.
    [14] 屈东胜, 洪延姬, 王广宇, 等. 基于波长调制光谱的多参数测量方法研究[J]. 红外与毫米波学报,2016,35(4):470-476.doi:10.11972/j.issn.1001-9014.2016.04.015

    QU D SH, HONG Y J, WANG G Y,et al. Measurement of multi-parameters of gas based on the wavelength modulation spectroscopy[J].Journal of Infrared and Millimeter Waves, 2016, 35(4): 470-476. (in Chinese)doi:10.11972/j.issn.1001-9014.2016.04.015
    [15] 王玉诏. 基于matlab的 掩星大气探测仿真系统[C]. 第三十一届全国空间探测学术研讨会. 银川: 中国空间科学学会, 2018: 47-55.

    WANG Y ZH. Laser occultation detection simulation system based on matlab[C].The 31th National Conference on Space Exploration. Yinchuan: Chinese Society of Space Research, 2018. (in Chinese)
    [16] 饶瑞中. 现代大气光学[M]. 北京: 科学出版社, 2012.

    RAO R ZH.Modern Atmospheric Optics[M]. Beijing: Science Press, 2012. (in Chinese)
  • 加载中
图(7)/ 表(1)
计量
  • 文章访问数:883
  • HTML全文浏览量:421
  • PDF下载量:59
  • 被引次数:0
出版历程
  • 收稿日期:2020-12-28
  • 修回日期:2021-01-08
  • 网络出版日期:2021-03-27
  • 刊出日期:2021-05-14

目录

    /

      返回文章
      返回
        Baidu
        map