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Spectral irradiance degradation model of halogen tungsten lamps at wavelength from 400 nm to 1300 nm

ZHANG Ya-chao,YE Xin,XIA Zhi-wei,SUI Long,FANG Wei

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张亚超, 叶新, 夏志伟, 隋龙, 方伟. 400~1300 nm波段的卤钨灯光谱辐照度衰减模型[J]. , 2022, 15(4): 825-834. doi: 10.37188/CO.EN.2021-0011
引用本文: 张亚超, 叶新, 夏志伟, 隋龙, 方伟. 400~1300 nm波段的卤钨灯光谱辐照度衰减模型[J]. , 2022, 15(4): 825-834.doi:10.37188/CO.EN.2021-0011
ZHANG Ya-chao, YE Xin, XIA Zhi-wei, SUI Long, FANG Wei. Spectral irradiance degradation model of halogen tungsten lamps at wavelength from 400 nm to 1300 nm[J]. Chinese Optics, 2022, 15(4): 825-834. doi: 10.37188/CO.EN.2021-0011
Citation: ZHANG Ya-chao, YE Xin, XIA Zhi-wei, SUI Long, FANG Wei. Spectral irradiance degradation model of halogen tungsten lamps at wavelength from 400 nm to 1300 nm[J].Chinese Optics, 2022, 15(4): 825-834.doi:10.37188/CO.EN.2021-0011

400~1300 nm波段的卤钨灯光谱辐照度衰减模型

详细信息
  • 中图分类号:TP394.1;TH691.9

Spectral irradiance degradation model of halogen tungsten lamps at wavelength from 400 nm to 1300 nm

doi:10.37188/CO.EN.2021-0011
Funds:Supported by National Key Research and Development Program (No. 2018YFB0504603)
More Information
    Author Bio:

    Zhang Ya-chao (1989—), Dcoctor, assistant professor, Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences. His research interests are on radiometric calibration of space optical remote sensor. E-mail:zhangyachao@ciomp.ac.cn

    Ye xin (1979—), Doctor, Professor. Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences. His research interests are on radiometric calibration of space optical remote sensor. E-mail:yexin@ciomp.ac.cn

    Corresponding author:yexin@ciomp.ac.cn
  • 摘要:

    卤钨灯光谱辐照度衰减会增加灯-板系统的光谱辐亮度不确定度,因此,有必要对卤钨灯的衰减特性展开研究,以提高灯-板系统光谱辐亮度精度。首先,根据黑体辐射定律和维尔斯特拉斯定理,在400~1300 nm波段,提出了一种包含待定阶数的卤钨灯光谱辐照度衰减模型。然后,实验测量卤钨灯的光谱辐照度衰减曲线,分别利用不同阶数的模型对其光谱辐照度衰减曲线进行最小二乘拟合。最后,以满足重建精度要求的最低阶数作为卤钨灯光谱照度模型的阶数。对于本文所用型号的卤钨灯,当模型阶数为二阶时卤钨灯光谱辐照度衰减曲线的重建精度优于0.25%。本文给出的光谱辐照度衰减模型为提高灯-板系统的光谱辐亮度精度奠定了理论基础。

  • Figure 1.Measurement scheme of the spectral irradiance degradation curve of the halogen tungsten lamp

    Figure 2.(a) Extra-atmospheric solar spectral irradiance and (b) spectral irradiance of tested halogen tungsten lamp

    Figure 3.Ratio of the spectral irradiance of the tested halogen tungsten lamp to the sun

    Figure 4.Spectral irradiance degradation curves of (a) 1# and (b) 2# halogen tungsten lamps

    Figure 5.Measurement uncertainty of the spectral irradiance degradation curve for (a) 1# and (b) 2# halogen tungsten lamps

    Figure 6.Measured spectral irradiance degradation curves and fitted results with the second-order model of (a) 1# and (b) 2# halogen tungsten lamps

    Figure 7.Relative standard deviations of the spectral irradiance degradation curves of (a) 1# and (b) 2# halogen tungsten lamps

    Figure 8.Relative errors between the fitted and measured spectral irradiance degradation curve of the two halogen tungsten lamps fitted by the second-order model. (a) 1# and (b) 2# halogen tungsten lamp

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出版历程
  • 收稿日期:2021-11-30
  • 录用日期:2022-02-22
  • 修回日期:2021-12-10
  • 网络出版日期:2022-02-22

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