Acta Optica Sinica, Volume. 43, Issue 8, 0822018(2023)
Design of Geostationary Full-Spectrum Wide-Swath High-Fidelity Imaging Spectrometer and Development of Its Spectrometers
Fig. 1. Working principle diagram of GeoFWHIS. (a) Layout diagram; (b) pointing to different coverages by turning the platform
Fig. 2. Afocal three-mirror system. (a) Coaxial three-mirror; (b) off-axis three-mirror; (c) zigzag-axis three-mirror
Fig. 3. Off-axis three-mirror imaging systems. (a) Two-mirror system; (b) three-mirror system with intermediate image; (c) three-mirror system without intermediate image
Fig. 4. Optical path of fore-optics system. (a) 3D model of fore-optics system; (b) optical path with scanning mirror at edge position of -2.56°; (c) optical path with scanning mirror at edge position of +2.56°
Fig. 5. MTF curves and spot diagrams of fore-optics system in B2 band. (a)-(c) MTF curves with scanning angle of -2.56°, 0°, and +2.56°; (d)-(f) sport diagrams with scanning angle of -2.56°, 0°, and +2.56°
Fig. 8. Optical path of spectrometers in GeoFWHIS. (a) B1 band; (b) B2 band; (c) B3 band; (d) B4 band; (e) B5 band
Fig. 9. SRF of optical splitting systems for each band. (a) B1 band; (b) B2 band; (c) B3 band; (d) B4 band; (e) B5 band
Fig. 11. SNR curves for B2 band in cloudless environment when observation zenith angle is 35° and integration time is 80 ms
Fig. 12. Silicon long slits. (a) Slit for B1 and B2 bands with length of 61.44 mm and width of 15 μm; (b) slit for B3 and B4 bands with length of 49.16 mm and width of 24 μm; (c) slit for B5 band with length of 24.58 mm and width of 24 μm
Fig. 13. Micrograph of slit for B2. (a) 10× micrograph; (a) test result of slit width
Fig. 14. Convex blazed gratings and their groove shapes, the lower right corner shows AFM test results of groove shapes. (a) B1 band, groove density is 312.1 lp/mm and blazed angle is 3.8°; (b) B2 band, groove density is 210.1 lp/mm and blazed angle is 4.75°; (c) B3 band, groove density is 68.5 lp/mm and blazed angle is 3.1°; (d) B4 band, groove density is 19.1 lp/mm and blazed angle is 2.8°; (e) B5 band, groove density is 8.8 lp/mm and blazed angle is 2.8°
Fig. 15. Diffraction efficiency curves of gratings at B1-B5 bands. (a) B1 band; (b) B2 band; (c) B3 band; (d) B4 band; (e) B5 band
Fig. 16. Alignment of the spectrometer by utilizing a point source microscope. (a) Self-developed point source microscope; (b) alignment of two separated meniscus in B3 spectrometer with point source microscope; (c) star images of two spherical surfaces in field of view of point source microscope
Fig. 17. Full-spectrum spectrometer prototypes. (a) B1 band; (b) B2 band; (c) B3 band; (d) B4 band; (e) B5 band
Fig. 18. Test device and test results of B2 spectrometer. (a) Test device of spectral property; (b) spectral lines; (c) SRF of 546.1 nm spectral line; (d) scatter diagram of 546.1 nm spectral line and its fitting curve
Fig. 19. Test device and spectral lines of B5 spectrometer. (a) Test device; (b) spectral lines
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Jiacheng Zhu, Zhicheng Zhao, Quan Liu, Xinhua Chen, Huan Li, Shaofan Tang, Weimin Shen. Design of Geostationary Full-Spectrum Wide-Swath High-Fidelity Imaging Spectrometer and Development of Its Spectrometers[J]. Acta Optica Sinica, 2023, 43(8): 0822018
Category: Optical Design and Fabrication
Received: Oct. 26, 2022
Accepted: Nov. 25, 2022
Published Online: Apr. 6, 2023
The Author Email: Liu Quan (liuquan@suda.edu.cn), Shen Weimin (swm@suda.edu.cn)