• Acta Photonica Sinica
  • Vol. 51, Issue 11, 1111003 (2022)
Kaisheng ZHANG1、2、*, Xiuqin SU1, and Zhilong YE3
Author Affiliations
  • 1Xi'an Institute of Optics and Precision Mechanics,Chinese Academy of Sciences,Xi'an 710119,China
  • 2University of Chinese Academy of Sciences,Beijing 100049,China
  • 3Shanghai Aerospace Control Technology Research Institute,Shanghai 201109,China.
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    DOI: 10.3788/gzxb20225111.1111003 Cite this Article
    Kaisheng ZHANG, Xiuqin SU, Zhilong YE. Large Relative Aperture Optical System Design for All Day Star Sensor[J]. Acta Photonica Sinica, 2022, 51(11): 1111003 Copy Citation Text show less
    Radiation at different temperatures and its derivative curves
    Fig. 1. Radiation at different temperatures and its derivative curves
    Optical lens design results
    Fig. 2. Optical lens design results
    Optical lens structure diagram
    Fig. 3. Optical lens structure diagram
    MTF of optical system at different pressure and temperature
    Fig. 4. MTF of optical system at different pressure and temperature
    Cromatic distortion curve of optical system
    Fig. 5. Cromatic distortion curve of optical system
    Dispersion spot of optical system at different temperature under defocusing condition.
    Fig. 6. Dispersion spot of optical system at different temperature under defocusing condition.
    Envelope energy of optical system at different temperature under defocusing condition
    Fig. 7. Envelope energy of optical system at different temperature under defocusing condition
    tolerance curve of optical system
    Fig. 8. tolerance curve of optical system
    Optical system modeling
    Fig. 9. Optical system modeling
    Stray light analysis results in the field of view
    Fig. 10. Stray light analysis results in the field of view
    Out-of-field PST analysis results
    Fig. 11. Out-of-field PST analysis results
    Fixed star(3:00 PM,along the direction of light)
    Fig. 12. Fixed star(3:00 PM,along the direction of light)
    Fixed star(3:00 PM,against the light,30°solar angle)
    Fig. 13. Fixed star(3:00 PM,against the light,30°solar angle)
    3D energy map of stars(3:00 PM,against the light,30°solar angle)
    Fig. 14. 3D energy map of stars(3:00 PM,against the light,30°solar angle)
    fixed star(4:00 PM,against the light,10°solar angle)
    Fig. 15. fixed star(4:00 PM,against the light,10°solar angle)
    3D energy map of stars(4:00 PM,against the light,10°solar angle)
    Fig. 16. 3D energy map of stars(4:00 PM,against the light,10°solar angle)
    Optical parameterValue
    Focal length84 mm
    Field of view≥8°
    Relative aperture1/1.4
    Spectral range1.1~1.4 μm
    System transmittance80%
    Energy concentration30 μm uniform concentration of more than 85% energy
    Primary wavelength1.25 μm
    Operating temperature-40~+60 ℃
    Table 1. Optical parameters
    Material nameThermal expansion coefficient/(×10-7·K-1Temperature coefficient of refractive/(×10-6·℃-1
    HLAF3803.2
    HZF52A845.0
    HFK611676.5
    Table 2. Optical material properties
    Optical parameterIndicator requirementsValue
    Focal length84 mm84 mm
    Field of view≥8°8.4°
    Relative aperture1/1.41/1.4
    Spectral range1.1~1.4 μm1.1~1.4 μm
    System transmittance≥80%≥86%
    Energy concentration30 μm uniform concentration of more than 85% energy30 μm uniform concentration of more than 95% energy
    Primary wavelength1.25 μm1.25 μm
    Operating temperature-40~+60 ℃-40~+60 ℃
    Table 3. Comparison of optical design results and analysis parameters
    Kaisheng ZHANG, Xiuqin SU, Zhilong YE. Large Relative Aperture Optical System Design for All Day Star Sensor[J]. Acta Photonica Sinica, 2022, 51(11): 1111003
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