Optics and Precision Engineering, Volume. 29, Issue 12, 2763(2021)

Analysis of signal-to-noise ratio for space-based optical surveillance of asteroids

Xin-tao WANG1...2, Jian-hua ZHENG1,2, and Ming-tao LI12,* |Show fewer author(s)
Author Affiliations
  • 1National Space Science Center, Chinese Academy of Sciences, Beijing0499, China
  • 2University of Chinese Academy of Sciences, Beijing100049, China
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    Figures & Tables(19)
    Solar spectrum radiant exitance
    Irradiance of Lambert disced radiator
    Spectrum radiant exitance of black body
    Brightness in zodiacal light
    Brightness in galactic light
    Orbits of target asteroid and visible telescope deployed on Earth-leading heliocentric orbit
    Distance of the target asteroid relative to the visible telescope deployed on Earth-leading heliocentric orbit
    SNR of target asteroid relative to visible telescope deployed on Earth-leading heliocentric orbit
    Apparent magnitude of target asteroid relative to visible telescope deployed on Earth-leading heliocentric orbit
    Maximum surveillance distance of visible telescope deployed on Sun-Earth L1 point
    Maximum surveillance distance of visible telescope deployed on Earth-leading heliocentric orbit
    SNR and apparent magnitude vs. asteroid's visual albedo
    SNR and apparent magnitude vs. asteroid's temperature
    SNR and apparent magnitude vs. asteroid's visual emissivity
    • Table 1. 转换系数在不同波长处的取值

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      Table 1. 转换系数在不同波长处的取值

      λ/μmcf
      0.361.37×10-8
      0.442.17×10-8
      0.502±0.0121.55×10-8
      0.530±0.003 51.33×10-8
      0.551.18×10-8
      0.647.40×10-9
      0.705.70×10-9
      0.794.02×10-9
      0.902.73×10-9
      1.259.89×10-10
      1.653.69×10-10
      2.21.29×10-10
      3.52.26×10-11
      3.81.60×10-11
      4.86.50×10-12
      8.48.09×10-13
      103.94×10-13
      10.63.15×10-13
      121.91×10-13
      202.56×10-14
      212.10×10-14
      251.06×10-14
    • Table 2. Orbital elements of target asteroid

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      Table 2. Orbital elements of target asteroid

      a/AUei/(°)Ω/(°)ω/(°)F/(°)
      10.05101030165
    • Table 3. Physical parameters of target asteroid

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      Table 3. Physical parameters of target asteroid

      参 数数 值
      温度Tobj/K300
      发射率ε0.9
      反照率α0.142
      直径D/m100
    • Table 4. Performance parameters of telescope

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      Table 4. Performance parameters of telescope

      参 数数 值
      口径D0/m0.7
      焦距f/m5
      光学透过率τopt0.8
    • Table 5. Performance parameters of detector

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      Table 5. Performance parameters of detector

      参 数数 值
      光电增益G1
      量子效率η0.7
      图像帧数N1
      暗电流ND/(e-·s-1·pixel-10.6
      读出噪声NR0.35e-RMS@500 kHz
      逆增益GI105/214
      工作波段λ/nm380-800
      像元尺寸a/μm10
      积分时间tint/s10
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    Xin-tao WANG, Jian-hua ZHENG, Ming-tao LI. Analysis of signal-to-noise ratio for space-based optical surveillance of asteroids[J]. Optics and Precision Engineering, 2021, 29(12): 2763

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    Paper Information

    Category: Modern Applied Optics

    Received: Apr. 29, 2021

    Accepted: --

    Published Online: Jan. 20, 2022

    The Author Email: LI Ming-tao (limingtao@nssc.ac.cn)

    DOI:10.37188/OPE.20212912.2763

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