Design and Study of a High Resolution Vacuum Ultraviolet Imaging Spectrometer Carried by Satellite
YU Lei1,2, LIN Guan-yu1, QU Yi1, WANG Shu-rong1*,WANG Long-qi1
1. Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China 2. Graduate University of Chinese Academy of Sciences, Beijing 100049, China
Abstract:A high resolution vacuum ultraviolet imaging spectrometer prototype carried by satellite applied to the atmosphere detection of particles distribution in 115~300 nm was developed for remote sensing. First, based on the analysis of advanced loads, the optical system including an off-axis parabolic mirror as the telescope and Czerny-Turner structure as the imaging spectrometer was chosen. Secondly, the 2-D photon counting detector with MCP was adopted for the characteristic that the radiation is weak in vacuum ultraviolet waveband. Then the geometric method and 1st order differential calculation were introduced to improve the disadvantages that aberrations in the traditional structure can not be corrected homogeneously to achieve perfect broadband imaging based on the aberration theory. At last, an advanced example was designed. The simulation and calculation of results demonstrate that the modulation transfer function (MTF) of total field of view is more than 0.6 in the broadband, and the spectral resolution is 1.23 nm. The structure is convenient and predominant. It proves that the design is feasible.
于 磊1,2,林冠宇1,曲 艺1,王淑荣1*,汪龙祺1 . 高分辨率星载真空紫外成像光谱仪设计与研究[J]. 光谱学与光谱分析, 2011, 31(12): 3417-3422.
YU Lei1,2, LIN Guan-yu1, QU Yi1, WANG Shu-rong1*,WANG Long-qi1 . Design and Study of a High Resolution Vacuum Ultraviolet Imaging Spectrometer Carried by Satellite. SPECTROSCOPY AND SPECTRAL ANALYSIS, 2011, 31(12): 3417-3422.
[1] Lü Da-ren, CHEN Ze-yu, BIAN Jian-chun,et al(吕达仁,陈泽宇,卞建春,等). Chinese J. Atmospheric Sciences(大气科学), 2008, 32(4): 782. [2] ZHENG Yu-quan, WANG Hui, WANG Yi-fan(郑玉权,王 慧,王一凡). Optics and Precision Engineering(光学精密工程), 2009, 17(11): 2629. [3] David J Sahnow, Charles D Keyes, Thomas B Ake,et al. Proc. SPIE, 2010, 7731: 39. [4] Robert P McCoy, Kenneth F Dymond, Gilbert G Fritz, et al. Optical Engineering, 1994, 33(2): 423. [5] Paxton L J, Christensen A B, Morrison D, et al. Proc. of SPIE, 2004, 5660: 228. [6] Larry J Paxton, Ching I Meng, Glen H Fountain, et al. Proc. SPIE, 1992, 1764: 161. [7] Goldsten J O, Humm D C, Paxton L J, et al.. Proc. SPIE, 1998, 3765: 408. [8] Arthur B Shafer, Lawrence R Megill, Leann Droppleman. J. Opt. Soc. Am., 1964, 54: 879. [9] Xu Li, Chen Kexin, He Qingsheng, et al. Applied Optics, 2009, 48(15): 2871. [10] Austin D R, Witting T, Walmsley lan A. Appl. Opt. 2009, 48, 3846. [11] YU Lei, QU Yi, LIN Guan-yu, et al(于 磊, 曲 艺, 林冠宇, 等). Acta Optica Sinica(光学学报), 2011, 1(1): 0112011. [12] XUE Qing-sheng, WANG Shu-rong, LI Fu-tian,et al(薛庆生,王淑荣,李福田,等). Optics and Precision Engineering(光学精密工程), 2010, 18(4): 823.