Wang Qian, Yang Zhongdong, Bi Yanmeng. Spectral parameters and signal-to-noise ratio requirement for CO2 hyper spectral remote sensor. J Appl Meteor Sci, 2014, 25(5): 600-609.
Citation: Wang Qian, Yang Zhongdong, Bi Yanmeng. Spectral parameters and signal-to-noise ratio requirement for CO2 hyper spectral remote sensor. J Appl Meteor Sci, 2014, 25(5): 600-609.

Spectral Parameters and Signal-to-noise Ratio Requirement for CO2 Hyper Spectral Remote Sensor

  • Received Date: 2013-08-29
  • Rev Recd Date: 2014-07-24
  • Publish Date: 2014-09-30
  • With the stable increase of carbon dioxide (CO2) concentrations, space based measurement of CO2 concentration in lower atmosphere by reflected sunlight in near infrared band has become a hot research topic. Recently, instruments sensitive to total CO2 column data in near-surface have become available through the SCIAMACHY instrument on ENVISAT and TANSO-FTS on GOSAT. The developing hyper spectral CO2 detector in China carried by TANSAT is going to be launched in 2015. Hyper spectral CO2 detector is designed to provide global measurements of CO2 in lower troposphere, employing high resolution spectra of reflected sunlight taken simultaneously in near-infrared CO2 (1.61 μm and 2.06 μm) and O2 (0.76 μm) bands.Associated with climate change and observation requirements of carbon sources and sinks, the feasibility of making CO2 column concentration measurements with high-resolution and high-precision is studied by high resolution atmosphere radiation transfer model. In consideration of the application requirements, effects of key specifications of the hyper spectral CO2 detector such as spectral resolution, sampling ratio and sign-to-noise ratio (SNR) on CO2 detection are analyzed.Typical characteristics of hyper spectral CO2 detector on TANSAT are grating spectrometer and array-based detector. To achieve the column averaged atmospheric CO2 dry air mole fraction (XCO2) precision requirements of 1×10-6-4×10-6, hyper spectral CO2 detector should provide high resolution at first to resolve CO2 absorption lines from continuous spectra of reflected sunlight. Compared to a variety of simulated spectral resolutions, the spectral resolution of hyper spectral CO2 detector on TANSAT can resolve CO2 spectral features and maintain the moderate radiance sensitivity. Since small size array detector-based instruments may suffer from undersampling of the spectra, influences of spectral undersampling to CO2 absorption spectra are studied, indicating that sampling ratio should exceed 2 pixels/FWHM to ensure the accuracy of CO2 spectrum.SNR is one of the most important parameters of hyper spectral CO2 detectors to ensure the reliability. SNR requirements of CO2 detector to different detection precisions are explored based on the radiance sensitivity factors. Results show that it is difficult to achieve SNR to detect 1×10-6-4×10-6 CO2 concentration change in the boundary layer by solar shortwave infrared passive remote sensing, limited by the instrument development condition and level at present. However, the instrument SNR to detect 1% change in the CO2 column concentration is attainable. These results are not only conductive to universal applications and guides on developing grating spectrometer, but also helpful to better understand the complexity of CO2 retrieval.
  • Fig. 1  Transmittance spectra for three spectral resolutions

    Fig. 2  Transmittance spectra for three spectral resolutions and sampling ratios

    Fig. 3  Transmittance spectra for two spectral resolutions of two detectors

    Fig. 4  Transmittance spectra for two detectors under the sampling ratios listed in Table 2

    Fig. 5  Transmittance relative errors for two detectors under two spectral resolutions

    Table  1  Simulation conditions of LBLRTM

    模拟条件 参数
    大气模型 美国标准大气
    扫描函数 三角型函数
    波数范围/cm-1 6237~6242
    光谱分辨率/cm-1 0.0014, 0.07, 0.312, 0.5
    FWHM内光谱采样数 1, 2, 4
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    Table  2  Sampling spacing and sampling ratio for two spectral resolutions of detectors

    探测器 采样间隔/cm-1 采样率
    FWHM为0.312 cm-1 FWHM为0.468 cm-1
    A 0.234 1.33 2
    B 0.117 2.67 4
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    Table  3  Transmittance average errors for two detectors under two spectral resolutions, referred to those under the baseline in the absorption channels between 6235-6245 cm-1

    探测器 FWHM为0.312 cm-1 FWHM为0.468 cm-1
    A 2.41% 0.92%
    B 0.57% 0
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    Table  4  Simulation conditions of SCIATRAN

    模拟条件 参数
    背景CO2浓度 373.6×10-6
    气溶胶条件 晴空无气溶胶
    太阳天顶角 60°
    地表反照率 0.15
    狭缝函数类型 高斯型
    光谱分辨率 0.08 nm
    光谱范围 1594~1624 nm
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    Table  5  SNR requirements of detecting CO2 concentration variation in boundary layer

    CO2浓度变化 f/% 信噪比
    1×10-6 -0.0524 1900
    2×10-6 -0.1048 950
    3×10-6 -0.1571 640
    4×10-6 -0.3252 300
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    Table  6  SNR requirements of detecting CO2 concentration variation in the whole column

    CO2柱浓度变化 f/% 信噪比
    1×10-6 -0.1219 820
    2×10-6 -0.2441 410
    3×10-6 -0.3580 280
    4×10-6 -0.4874 200
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    • Received : 2013-08-29
    • Accepted : 2014-07-24
    • Published : 2014-09-30

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