Volume 43 Issue 9
Oct.  2014
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Li Hongzhuang, Zhao Yongzhi, Wang Guoqiang, Liu Xinyue. Design of refractive optical system with large relative aperture and long focal length[J]. Infrared and Laser Engineering, 2014, 43(9): 2954-2958.
Citation: Li Hongzhuang, Zhao Yongzhi, Wang Guoqiang, Liu Xinyue. Design of refractive optical system with large relative aperture and long focal length[J]. Infrared and Laser Engineering, 2014, 43(9): 2954-2958.

Design of refractive optical system with large relative aperture and long focal length

  • Received Date: 2014-01-10
  • Rev Recd Date: 2014-02-25
  • Publish Date: 2014-09-25
  • The aberration characteristics of refractive optical system with large relative aperture and long focal length were analyzed. And a lens with 300 mm diameter, 540 mm focal length, 500 -850 nm operating wavelength range, and 2field of view was designed. First, as the secondary spectrum was the most prominent aberration, the Petzval form was chose as the initial configuration, and after complication, the configuration with three components with large air space was used, which was good for aberration correction and element size reduction. Then the partial dispersion and abbe number of typical glasses were recalculated and modified for the used wavelength, and P-V map is draw, then the glasses with some secondary spectrum correction ability and fine optical performance were chose. Finally the secondary spectrum of the system is reduced to 0.06 mm, which show that the system is apochromat. The design results demonstrate that the MTF of all field of view at Nyquist frequency 39 lp/mm is higher than 0.8, and 80% energy of the system encircled in 8um, which is less than a pixel size, and the distortion is less than 0.1%. All indexes satisfy the commands of system.
  • [1] Wang Meiqin, Wang Zhonghou, Bai Jiaguang. Removing secondary spectrum in wide spectrum optical system [J].Journal of Applied Optics, 2010, 31(3): 360-364. (in Chinese)王美钦, 王忠厚, 白加光. 宽谱段光学系统消二级光谱的设计[J]. 应用光学. 2010, 31(3): 360-364.
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    [3] Yang Qinghua, Zhao Baochang, Zhou Renkui. Correction ofsecondary spectrum based on normal dispersion glass [J].Acta Phoutonica Sinica, 2008, 37(4): 772-775. (in Chinese)杨庆化, 赵葆常, 周任魁. 基于正常色散玻璃二级光谱的校正[J]. 光子学报, 2008, 37(4): 772-775.
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    [5] Huang Lei, Hu Wenwen, Yang Zhiwen. Optical design ofwide bands and long focal length collimating lens [J].Infrared and Laser Engineering, 2007, 36(S): 125-127. (inChinese)黄雷, 胡雯雯, 杨志文. 宽光谱、长焦距准直物镜光学设计[J]. 红外与激光工程, 2007, 36(S): 125-127.
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    [7] Wu Di, Li Lijuan, Shen Jiwei. Optical system design ofaerial camera simulator with wide spectrum and wide-viewfield [J]. Journal of Xi' an Technological University, 2012,32(12): 991-999. (in Chinese)吴迪, 李丽娟, 沈继伟. 宽光谱大视场航空相机模拟器光学系统设计[J]. 西安工业大学学报, 2012, 32(12): 991-999.
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    [10] Sun Xin, Bai Jiaguang, Wang Zhonghou, et al. Opticalsystem design of an airborne multi-spectral camera [J]. ActaPhoutonica Sinica, 2009, 38(12):3160-3164. (in Chinese)孙鑫, 白加光, 王忠厚, 等. 一种机载多光谱相机的光学系统设计[J]. 光子学报,2009, 38(12): 3160-3164.
    [11] Martha Rosete-Aguilar. Correction of secondary spectrumusing standard glasses[C]//SPIE, 1996, 2774: 378-386.
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Design of refractive optical system with large relative aperture and long focal length

  • 1. Changchun Institute of Optics,Fine Mechanics and Physics,Chinese Academy of Sciences,Changchun 130033,China

Abstract: The aberration characteristics of refractive optical system with large relative aperture and long focal length were analyzed. And a lens with 300 mm diameter, 540 mm focal length, 500 -850 nm operating wavelength range, and 2field of view was designed. First, as the secondary spectrum was the most prominent aberration, the Petzval form was chose as the initial configuration, and after complication, the configuration with three components with large air space was used, which was good for aberration correction and element size reduction. Then the partial dispersion and abbe number of typical glasses were recalculated and modified for the used wavelength, and P-V map is draw, then the glasses with some secondary spectrum correction ability and fine optical performance were chose. Finally the secondary spectrum of the system is reduced to 0.06 mm, which show that the system is apochromat. The design results demonstrate that the MTF of all field of view at Nyquist frequency 39 lp/mm is higher than 0.8, and 80% energy of the system encircled in 8um, which is less than a pixel size, and the distortion is less than 0.1%. All indexes satisfy the commands of system.

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