• Journal of Infrared and Millimeter Waves
  • Vol. 41, Issue 1, 2021106 (2022)
Wen-Long FAN1、2、3, Xiao-Xian HUANG1、2、*, and Yu-Tian FU1、2
Author Affiliations
  • 1Key Laboratory of Infrared System Detection an Imaging Technology,Chinese Academy of Sciences,Shanghai 200083,China
  • 2Shanghai Institute of Technical Physics,Chinese Academy of Sciences,Shanghai 200083,China
  • 3University of Chinese Academy of Sciences,Beijing 100049,China
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    DOI: 10.11972/j.issn.1001-9014.2022.01.031 Cite this Article
    Wen-Long FAN, Xiao-Xian HUANG, Yu-Tian FU. Analysis of radiation reference anomaly of HY-1B COCTS and research on the repair algorithm[J]. Journal of Infrared and Millimeter Waves, 2022, 41(1): 2021106 Copy Citation Text show less
    Imaging diagram of COCTS
    Fig. 1. Imaging diagram of COCTS
    Scanning period of COCTS
    Fig. 2. Scanning period of COCTS
    Cold space signal in sunshine area
    Fig. 3. Cold space signal in sunshine area
    Cold space signal of different frame
    Fig. 4. Cold space signal of different frame
    Blackbody signal in sunshine area
    Fig. 5. Blackbody signal in sunshine area
    Schematic of the experiment
    Fig. 6. Schematic of the experiment
    Blackbody signal
    Fig. 7. Blackbody signal
    Cold space signal
    Fig. 8. Cold space signal
    Integrating sphere signal
    Fig. 9. Integrating sphere signal
    The influence of multi-layer dressings
    Fig. 10. The influence of multi-layer dressings
    The influence on HY-1B COCTS of the sun glitter
    Fig. 11. The influence on HY-1B COCTS of the sun glitter
    Diagram of the glitter influence
    Fig. 12. Diagram of the glitter influence
    The relationship between the glitter energy and zenith angle for HY-1C COCTS
    Fig. 13. The relationship between the glitter energy and zenith angle for HY-1C COCTS
    The theoretical output code of CH41A of HY-1B COCTS
    Fig. 14. The theoretical output code of CH41A of HY-1B COCTS
    The actual output code of CH41A of HY-1B COCTS
    Fig. 15. The actual output code of CH41A of HY-1B COCTS
    Code correction quantity
    Fig. 16. Code correction quantity
    Image curve before and after correction(No.1164 pixel)(a)channel 1~4,(b)channel 5~8
    Fig. 17. Image curve before and after correction(No.1164 pixel)(a)channel 1~4,(b)channel 5~8
    Image curve before and after correction(No.1840 frame)(a)channel 1~4,(b)channel 5~8
    Fig. 18. Image curve before and after correction(No.1840 frame)(a)channel 1~4,(b)channel 5~8
    Image correction(a)image before correction,(b)image after correction
    Fig. 19. Image correction(a)image before correction,(b)image after correction
    Image correction of the Bohai Sea and the Yellow Sea area(a)image before correction,(b)image after correction
    Fig. 20. Image correction of the Bohai Sea and the Yellow Sea area(a)image before correction,(b)image after correction
    Image code distribution(a)channel 1~4,(b)channel 5~8
    Fig. 21. Image code distribution(a)channel 1~4,(b)channel 5~8
    技术指标C/D星水色仪MODIS
    轨道高度(km)782705
    轨道类型太阳同步太阳同步
    轨道周期(分钟)100.698.8
    地球覆盖周期(日)0.5~11~2
    谱段范围(μm)0.4~12.50.4~14.4
    地面分辨率(m)1 100250~1 000
    幅宽(km)2 9002 330
    设计寿命(年)55~6
    Table 1. Main performance of COCTS and MODIS
    通道谱段(μm)应用对象
    10.402~0.422黄色物质、水体污染
    20.433~0.453叶绿素吸收
    30.480~0.500叶绿素、海水光学、海冰、污染、浅海地形
    40.510~0.530叶绿素、水深、污染、低含量泥沙
    50.555~0.575叶绿素、低含量泥沙
    60.660~0.680中高含量泥沙、大气校正、污染、气溶胶
    70.734~0.754大气校正、高含量泥沙
    80.845~0.885大气校正、高含量泥沙
    Table 2. VNIR spectral range of COCTS
    开灯数量灯功率(W)

    第4谱段光谱辐亮度

    (mW∙cm-2∙μm-1∙Sr-1

    000
    11501.416
    2150+502.727
    3150+50+1005.999
    4150+50+100+20011.146
    5150+50+100+200+30021.511
    Table 3. Energy level of integrating sphere
    探测元响应系数αB暗电平βB相关系数
    CH11A73.152 8915.347 480.993 9
    CH11B73.421 4415.352 420.994
    CH21A73.637 717.268 040.993 3
    CH21B73.529 4117.235 290.993 4
    CH31A79.428 1214.670 370.993 1
    CH31B80.064 0514.675 740.993 2
    CH41A79.554 4916.618 930.992 9
    CH41B79.808 4616.600 160.993
    CH51A83.472 4518.305 510.991 7
    CH51B82.781 4618.278 150.991 7
    CH61A92.592 5917.481 480.992 4
    CH61B92.764 3817.467 530.992 5
    CH71A97.943 1914.681 680.993 7
    CH71B98.135 4314.671 250.993 8
    CH81A170.76517.486 340.996 5
    CH81B170.998 617.458 960.996 5
    Table 4. System response coefficient of HY-1B COCTS
    通道斜率k截距b相关系数
    1-3.448 5786.301 199-0.675 223
    2-4.269 9477.101 911-0.708 497
    3-5.756 9098.673 079-0.740 943
    4-6.828 9839.679 126-0.739 072
    5-8.133 14510.919 994-0.741 929
    6-9.904 32612.693 466-0.738 442
    7-10.365 13412.987 391-0.744 667
    8-11.085 59913.601 824-0.742 428
    Table 5. Regression coefficient of the glitter of HY-1C COCTS
    探测元能量修复系数
    斜率αB"截距NB"相关系数
    CH11A57.95-188.4860.843
    CH11B58.591-195.2590.842
    CH21A63.424-297.4070.849
    CH21B63.602-300.9080.849
    CH31A73.859-333.9640.893
    CH31B75.369-345.690.89
    CH41A77.7-279.3890.905
    CH41B78.153-280.3320.905
    CH51A82.999-237.1050.912
    CH51B83.294-243.6940.911
    CH61A93.763-164.480.923
    CH61B94.816-170.7590.922
    CH71A173.544-154.9080.967
    CH71B174.693-160.5890.965
    CH81A354.823-161.2010.982
    CH81B356.442-168.4270.981
    Table 6. 1st pixel’s repair coefficient of 8 channels of HY-1B COCTS
    Wen-Long FAN, Xiao-Xian HUANG, Yu-Tian FU. Analysis of radiation reference anomaly of HY-1B COCTS and research on the repair algorithm[J]. Journal of Infrared and Millimeter Waves, 2022, 41(1): 2021106
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