• Acta Optica Sinica
  • Vol. 44, Issue 3, 0304001 (2024)
Hanhui Cao1、2, Hongyao Chen2、*, Wenxin Huang2, and Jiawei Li2
Author Affiliations
  • 1University of Science and Technology of China, Hefei 230026, Anhui, China
  • 2Key Laboratory of Optical Calibration and Characterization, Anhui Institute of Optics and Fine Mechanics, HFIPS, Chinese Academy of Sciences, Hefei 230031, Anhui, China
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    DOI: 10.3788/AOS231501 Cite this Article Set citation alerts
    Hanhui Cao, Hongyao Chen, Wenxin Huang, Jiawei Li. Response Nonlinear Calibration of Solar Blind Phototube Detection System Using Indirect Method[J]. Acta Optica Sinica, 2024, 44(3): 0304001 Copy Citation Text show less
    Linear measurement device of solar blind phototube detection system
    Fig. 1. Linear measurement device of solar blind phototube detection system
    Response nonlinear calibration results of solar blind phototube detection system
    Fig. 2. Response nonlinear calibration results of solar blind phototube detection system
    Change of relative spectral radiance of xenon lamp light source with time
    Fig. 3. Change of relative spectral radiance of xenon lamp light source with time
    Linear fitting results of response photocurrents of reference detector and detector to be tested
    Fig. 4. Linear fitting results of response photocurrents of reference detector and detector to be tested
    Correlated coefficient, original response photocurrent, and relative error of response photocurrents of detector to be tested and reference detector. (a) Correlated coefficient; (b) original response photocurrent values; (c) relative error
    Fig. 5. Correlated coefficient, original response photocurrent, and relative error of response photocurrents of detector to be tested and reference detector. (a) Correlated coefficient; (b) original response photocurrent values; (c) relative error
    Experimental results of reference detector and light source current changes. (a) Linear fitting result; (b) response nonlinear calibration results; (c) current change of light source over time
    Fig. 6. Experimental results of reference detector and light source current changes. (a) Linear fitting result; (b) response nonlinear calibration results; (c) current change of light source over time
    ParameterS2281R6800U-11
    Spectral response range /nm190 to 1100160 to 350
    Photocathode materialSiCs-Te
    Dark current /pA50@VR=10 mV and 25 ℃1
    Recommended operating voltage /V15
    Ambient temperature /℃-10 to 60-80 to 50
    Radiant sensitivity /(A/W)0.12@200 nm and 25 ℃0.02@254 nm and 25 ℃
    Input window materialQuartzQuartz
    Active area size /mm11.38
    Table 1. Parameters of Si photodiode S2281 and phototube R6800U-11[25-26]
    Range5¹/₂ digit default resolutionAccuracy(1YR)±(% RDG.+ offset)18-28 °C,0-70% RHTypical RMS noise

    Analog rise time

    (10% to 90%)

    2 nA10 fA0.4%+400 fA20 fA8 ms
    20 nA100 fA0.4%+1 pA100 fA8 ms
    200 nA1 pA0.2%+10 pA1 pA500 μs
    2 μA10 pA0.15%+100 pA10 pA500 μs
    20 μA100 pA0.1%+1 nA100 pA500 μs
    200 μA1 nA0.1%+10 nA1 nA500 μs
    2 mA10 nA0.1%+100 nA10 nA500 μs
    20 mA100 nA0.1%+1 μA100 nA500 μs
    Table 2. Characteristic parameters of 6485 picoammeter (Keithley)[27]
    Measurement pointResponse photocurrent of S2281 /AResponse photocurrent of R6800U-11 /ARelative responsivityRelative error /%
    19.314×10-121.384×10-120.149-1.056
    24.641×10-116.374×10-120.1376.591
    32.053×10-102.806×10-110.1377.062
    42.128×10-92.965×10-100.1395.268
    51.207×10-81.718×10-90.1423.210
    64.863×10-87.034×10-90.1451.639
    71.369×10-71.979×10-80.1451.676
    82.662×10-73.934×10-80.148-0.505
    93.719×10-75.484×10-80.147-0.270
    104.308×10-76.330×10-80.1470.073
    114.500×10-76.610×10-80.1470.122
    Table 3. Relative response values and relative error at each measurement point
    Measurement pointMeasured value of R6800U-11 /%Measured value of S2281 /%
    1180.97961.7538
    239.29550.3520
    38.92550.0795
    40.84480.0070
    50.14580.0012
    60.03280.0012
    70.01170.0004
    80.00670.0002
    90.00480.0002
    100.00420.0001
    110.00400.0001
    Table 4. Influence of dark background noise on measured values of each measurement point
    Measurement pointMeasured value of R6800U-11 /%Measured value of S2281 /%
    1146.8041.850
    220.0550.700
    35.1310.573
    41.0730.473
    50.4640.418
    60.3600.361
    70.3130.285
    80.2080.205
    90.1700.165
    100.1620.158
    110.1570.152
    Table 5. Influence of noise on measured values of each measurement point
    Measurement pointRoot mean square value of R6800U-11 /ARoot mean square value of S2281 /A
    12.032×10-121.723×10-13
    21.278×10-123.246×10-13
    31.440×10-121.176×10-12
    43.181×10-121.006×10-11
    57.967×10-125.043×10-11
    62.534×10-111.754×10-10
    76.184×10-113.896×10-10
    88.168×10-115.457×10-10
    99.301×10-116.147×10-10
    101.027×10-106.812×10-10
    111.036×10-106.853×10-10
    Table 6. Root mean square values of noise at each measuring point
    Photo current /ANonlinear correction factorRelative standard deviation /%
    Group 1Group 2Group 3Group 4Group 5Group 6Group 7Group 8
    1.239×10-90.9930.9930.9900.9970.9930.9940.9900.9950.222
    7.087×10-91.0000.9970.9950.9980.9971.0080.9940.9970.422
    2.873×10-81.0010.9981.0020.9981.0001.0011.0050.9950.296
    7.833×10-81.0011.0001.0020.9981.0001.0031.0031.0010.158
    1.527×10-71.0031.0011.0011.0011.0031.0011.0001.0010.108
    2.140×10-70.9981.0001.0021.0001.0020.9990.9991.0010.151
    2.494×10-71.0010.9981.0010.9991.0011.0021.0001.0000.127
    2.647×10-70.9971.0010.9990.9990.9991.0011.0030.9970.212
    Table 7. Data of nonlinear correction factor for various response photo current
    Measurement pointNonlinear correction factorRelative standard deviation /%
    Group 1Group 2Group 3Group 4Group 5Group 6Group 7Group 8
    11.1800.9340.7521.1480.6701.4250.9281.04924.107
    20.9780.9130.8980.9710.9330.9010.9493.471
    30.9300.9270.9270.9340.9200.9460.9270.9290.826
    40.9490.9460.9460.9490.9480.9490.9480.9480.139
    50.9680.9670.9680.9700.9690.9690.9690.9680.098
    60.9820.9830.9840.9860.9850.9850.9850.9840.123
    70.9810.9840.9850.9850.9840.9850.9840.9840.129
    81.0011.0041.0061.0071.0071.0081.0071.0070.242
    90.9981.0011.0031.0041.0051.0051.0051.0050.256
    100.9950.9981.0001.0011.0021.0021.0021.0010.259
    110.9940.9980.9991.0001.0011.0011.0011.0010.241
    Table 8. Data of nonlinear correction factor for each measurement point
    Influence factorUncertainty /%
    Surface nonuniformity(integrating sphere)0.800
    Angle nonuniformity(integrating sphere)0.500
    Standard detector0.422
    Repeatability0.259
    Dark background0.845
    Standard transfer process0.473
    Detection system to be tested(phototube,picoammeter,source meter)1.073
    Combined uncertainty1.795
    Expanded uncertainty(confidence factor k=2)3.591
    Table 9. Combined uncertainty of measurement system
    Hanhui Cao, Hongyao Chen, Wenxin Huang, Jiawei Li. Response Nonlinear Calibration of Solar Blind Phototube Detection System Using Indirect Method[J]. Acta Optica Sinica, 2024, 44(3): 0304001
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