• Acta Optica Sinica
  • Vol. 40, Issue 7, 0722002 (2020)
Fuzhen Yang1、2, Xinhua Chen1、2、*, Zhicheng Zhao1、2, Quan Liu1、2, and Weimin Shen1、2
Author Affiliations
  • 1Key Laboratory of Modern Optical Technologies of Ministry of Education of China, School of Optoelectronic Science and Engineering, Soochow University, Suzhou, Jiangsu 215006, China
  • 2Key Laboratory of Advanced Optical Manufacturing Technologies of Jiangsu Province, School of Optoelectronic Science and Engineering, Soochow University, Suzhou, Jiangsu 215006, China
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    DOI: 10.3788/AOS202040.0722002 Cite this Article Set citation alerts
    Fuzhen Yang, Xinhua Chen, Zhicheng Zhao, Quan Liu, Weimin Shen. Visible-Infrared Imaging Spectrometer for the Exploration of Asteroids[J]. Acta Optica Sinica, 2020, 40(7): 0722002 Copy Citation Text show less
    VNIR-SWIR reflection spectra of Kaolinite, Halloysite and Montmorillonite. (a) Typical spectral curve; (b) local enlarged drawing of the selected area in Fig. 1(a)
    Fig. 1. VNIR-SWIR reflection spectra of Kaolinite, Halloysite and Montmorillonite. (a) Typical spectral curve; (b) local enlarged drawing of the selected area in Fig. 1(a)
    VNIR-SWIR reflection spectra of HEDs. (a) Spectral curve of HEDs from different regions; (b) local enlarged drawing of the selected area in Fig. 2(a)
    Fig. 2. VNIR-SWIR reflection spectra of HEDs. (a) Spectral curve of HEDs from different regions; (b) local enlarged drawing of the selected area in Fig. 2(a)
    Diagram of the partitioned diffraction gratings
    Fig. 3. Diagram of the partitioned diffraction gratings
    Imaging diagram of Rowland circles on meridional image locations
    Fig. 4. Imaging diagram of Rowland circles on meridional image locations
    Steps to calculate the initial structure
    Fig. 5. Steps to calculate the initial structure
    Optical layout of the designed optical system
    Fig. 6. Optical layout of the designed optical system
    Spot diagram of designed optical system
    Fig. 7. Spot diagram of designed optical system
    Curve of the smile versus the normalized field of view
    Fig. 8. Curve of the smile versus the normalized field of view
    Curve of the keystone versus the normalized field of view
    Fig. 9. Curve of the keystone versus the normalized field of view
    Diffraction efficiency of gratings in VNIR band. (a) Diffraction efficiency at different blaze angles; (b) combined diffraction efficiency with different area ratios
    Fig. 10. Diffraction efficiency of gratings in VNIR band. (a) Diffraction efficiency at different blaze angles; (b) combined diffraction efficiency with different area ratios
    Diffraction efficiency of gratings in SWIR band
    Fig. 11. Diffraction efficiency of gratings in SWIR band
    Partitioned grating and the prototype of the designed optical system. (a) Partitioned grating; (b) prototype of the designed optical system
    Fig. 12. Partitioned grating and the prototype of the designed optical system. (a) Partitioned grating; (b) prototype of the designed optical system
    Photo of the spectrum performance measurement device for the VNIR band
    Fig. 13. Photo of the spectrum performance measurement device for the VNIR band
    Spectral image and intensity distribution curves in the VNIR band
    Fig. 14. Spectral image and intensity distribution curves in the VNIR band
    Photo of the spectrum performance measurement device for the SWIR band
    Fig. 15. Photo of the spectrum performance measurement device for the SWIR band
    Spectral image and intensity distribution curves at 1900 nm
    Fig. 16. Spectral image and intensity distribution curves at 1900 nm
    ParameterVNIRSWIR
    Spectral range /nm400--10001000--2700
    Spectral resolution /nm≤5≤10
    F number63
    Pixel size /μm25
    Slit length /mm10
    Smile and keystone /pixel<10%
    Table 1. Main parameters of the system
    VNIRSWIR
    ParameterValue /mmParameterValue /mmParameterValue /mmParameterValue /mm
    R1-136.31071/g0.0083R1-165.82631/g0.022
    R2-69.4444dCO33.5520R2-81.1111dCO25.0754
    R3-133.3195dCIM27.7187R3-155.7172dCIM32.3754
    Table 2. Initial structural parameters of the system
    Field of view /mmVNIRSWIR
    0.4 μm0.7 μm1.0 μm1.0 μm1.85 μm2.7 μm
    (0,0)0.930.860.800.770.700.51
    (3.7,0)0.930.870.800.740.700.53
    (5,0)0.930.870.790.720.700.54
    (-3.7,0)0.940.870.800.740.700.53
    (-5,0)0.930.870.790.720.700.54
    Table 3. MTF at the Nyquist frequency (20 lp/mm)
    Wavelength /nm4005507008501000
    Spectral resolution /nm3.503.753.713.633.54
    Smile /pixel7.57%7.34%7.39%7.33%7.86%
    Max keystone /pixel3.43%
    Table 4. Measurement results of the spectral resolution, smile and keystone in VNIR band
    Wavelength /nm11001300150017001900
    Spectral resolution /nm9.599.619.359.779.89
    Smile /pixel8.6%7.90%6.83%7.33%8.35%
    Maxkeystone /pixel5.61%
    Table 5. Measurement results of the spectral resolution, smile and keystone in SWIR band
    Fuzhen Yang, Xinhua Chen, Zhicheng Zhao, Quan Liu, Weimin Shen. Visible-Infrared Imaging Spectrometer for the Exploration of Asteroids[J]. Acta Optica Sinica, 2020, 40(7): 0722002
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