Acta Optica Sinica, Volume. 45, Issue 18, 1828011(2025)
Scientific Mission Design for Ultraviolet Hyperspectral Detection of Venus Cloud Layers (Invited)
Fig. 2. MTF curves of channel 1 spectrometer at different wavelengths. (a) 190 nm; (b) 320 nm; (c) 450 nm
Fig. 3. Optical layout of ultraviolet ultra-high-resolution spectrometer and its overall structure
Fig. 4. MTF of the imaging system in channel 2 of ultraviolet ultra-high-resolution spectrometer. (a) 370 nm; (b) 385 nm; (c) 400 nm
Fig. 5. MTF of the imaging system in channel 3 of ultraviolet ultra-high-resolution spectrometer. (a) 275 nm; (b) 290 nm; (c) 305 nm
Fig. 6. MTF of the imaging system in channel 4 of ultraviolet ultra-high-resolution spectrometer. (a) 190 nm; (b) 205 nm; (c) 220 nm
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Tao Li, Xin Fang, Liujun Zhong, Dexin Lai, Bo Li, Yamin Wang, Yonghe Zhang, Xin Ye. Scientific Mission Design for Ultraviolet Hyperspectral Detection of Venus Cloud Layers (Invited)[J]. Acta Optica Sinica, 2025, 45(18): 1828011
Category: Remote Sensing and Sensors
Received: May. 27, 2025
Accepted: Aug. 28, 2025
Published Online: Sep. 19, 2025
The Author Email: Xin Fang (xinf@ustc.edu.cn)
CSTR:32393.14.AOS251150