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The coded aperture imaging spectrometer system based on the double-Amici-prism is designed in this paper, which includes the telescope objective, the coded template, the double-Amici-prism, the collimator lens and the imaging lens. This optical system can obtain a high diffraction efficiency. Compared to the imaging spectrometer system with a slit for this kind of system, the field of view is a two-dimensional spatial expansion, increasing the difficulty of design. For the subsequent data inversion algorithm, perfect imaging is needed, and based on this, the optical aberration of the system should be corrected carefully wildly. In this paper, we design and analyse the features of the imaging spectrometer system based on the double-Amici-prism, then the comple imaging spectrometer system. Telescope objective is designed to be telecentric, its MTF at 39 line pairs is 0.8, implying that good images can be obtained. Innovatively, an inverted telescope objective is used as a collimation system.The imaging spectrometer system's MTF at 39 line pairs is higher than 0.65. The imaging of the outdoor target scene, obtained by the coded aperture imaging spectrometer, proves that the design principle is feasible,the system is of high diffraction efficiency, the full-field imaging is of good quality, and the full spectrum of data is creditabe.
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Keywords:
- imaging spectrometer /
- optical system design /
- the double-Amici-prism
[1] Wang J Y, Shu R, Liu Y N, Ma Y H 2011 Introduction to the ImagingSpectrum Technology (1st Ed.) (Beijing: Science Press) p259-262[王建宇, 舒嵘, 刘银年, 马艳华2011成像光谱技术导论(第一版) (北京: 科学出版社)第259–262页]
[2] Yuan Y 2005 Ph. D. Dissertation (Beijing: Beijing University ofAeronautics and Astronautics) (in Chinese) [袁艳2005博士学位论文(北京: 北京航空航天大学)]
[3] WagadarikarA, John R, Willett R, Brady D 2008 Appl. Opt. 47 44
[4] Hagen N, Tkaczyk T S 2011 Appl. Opt. 50 4998
[5] Pei L L, Huang M, L Q B 2013 Acta Optica Sinica 33 122003 (in Chinese) [裴琳琳, 黄旻, 吕群波 2013 光学学报 33 122003]
[6] Sun Q, Yu B, Wang Z Q, Mu G G, Lu Z W 2004 Acta Phys. Sin. 53 756 (in Chinese) [孙强, 于斌, 王肇圻, 母国光, 卢振武 2004 物理学报 53 756]
[7] Song Y F, Shao X P, Xu J 2008 Acta Phys. Sin. 57 6298 (in Chinese) [宋岩峰, 邵晓鹏, 徐军 2008 物理学报 57 6298]
[8] Sun J X, Pan G Q, Liu Y 2013 Acta Phys. Sin. 62 094203
[9] Li D X, Lu Z W, Sun Q 2007 Acta Phys. Sin. 56 5766 (in Chinese) [李东熙, 卢振武, 孙强 2007 物理学报 56 5766]
[10] Dong K Y, Sun Q, Li Y D 2006 Acta Phys. Sin. 55 4602 (in Chinese) [董科研, 孙强, 李永大 2006 物理学报 55 4602]
[11] Liu Y J 2012 Ph. D. Dissertation (Changchun: The Changchun Institute ofOptics, Fine Mechanics and Physics, Chinese Academy of Science) (inChinese) [刘玉娟2012博士学位论文(长春: 中国科学院长春光学精密机械与物理研究所)]
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[1] Wang J Y, Shu R, Liu Y N, Ma Y H 2011 Introduction to the ImagingSpectrum Technology (1st Ed.) (Beijing: Science Press) p259-262[王建宇, 舒嵘, 刘银年, 马艳华2011成像光谱技术导论(第一版) (北京: 科学出版社)第259–262页]
[2] Yuan Y 2005 Ph. D. Dissertation (Beijing: Beijing University ofAeronautics and Astronautics) (in Chinese) [袁艳2005博士学位论文(北京: 北京航空航天大学)]
[3] WagadarikarA, John R, Willett R, Brady D 2008 Appl. Opt. 47 44
[4] Hagen N, Tkaczyk T S 2011 Appl. Opt. 50 4998
[5] Pei L L, Huang M, L Q B 2013 Acta Optica Sinica 33 122003 (in Chinese) [裴琳琳, 黄旻, 吕群波 2013 光学学报 33 122003]
[6] Sun Q, Yu B, Wang Z Q, Mu G G, Lu Z W 2004 Acta Phys. Sin. 53 756 (in Chinese) [孙强, 于斌, 王肇圻, 母国光, 卢振武 2004 物理学报 53 756]
[7] Song Y F, Shao X P, Xu J 2008 Acta Phys. Sin. 57 6298 (in Chinese) [宋岩峰, 邵晓鹏, 徐军 2008 物理学报 57 6298]
[8] Sun J X, Pan G Q, Liu Y 2013 Acta Phys. Sin. 62 094203
[9] Li D X, Lu Z W, Sun Q 2007 Acta Phys. Sin. 56 5766 (in Chinese) [李东熙, 卢振武, 孙强 2007 物理学报 56 5766]
[10] Dong K Y, Sun Q, Li Y D 2006 Acta Phys. Sin. 55 4602 (in Chinese) [董科研, 孙强, 李永大 2006 物理学报 55 4602]
[11] Liu Y J 2012 Ph. D. Dissertation (Changchun: The Changchun Institute ofOptics, Fine Mechanics and Physics, Chinese Academy of Science) (inChinese) [刘玉娟2012博士学位论文(长春: 中国科学院长春光学精密机械与物理研究所)]
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