Compact catadioptric optical system with long focal length large relative aperture and large field of view

Author(s):  
Yang Shen ◽  
WANG Hu ◽  
XUE Yaoke ◽  
JIE Yongjie ◽  
LIN Shangmin ◽  
...  
2014 ◽  
Vol 7 (4) ◽  
pp. 631-637
Author(s):  
白玉琢 BAI Yu-zhuo ◽  
木锐 MU Rui ◽  
马琳 MA Lin ◽  
贾钰超 JIA Yu-chao ◽  
普群雁 PU Qun-yan ◽  
...  

2015 ◽  
Vol 44 (1) ◽  
pp. 122001
Author(s):  
孟庆宇 MENG Qing-yu ◽  
董吉洪 DONG Ji-hong ◽  
曲洪丰 QU Hong-feng ◽  
王维 WANG Wei ◽  
曹智睿 CAO Zhi-rui

2014 ◽  
Vol 51 (5) ◽  
pp. 052203
Author(s):  
孙明哲 Sun Mingzhe ◽  
张红鑫 hang Hongxin ◽  
卢振武 Lu Zhenwu ◽  
卜和阳 Bu Heyang ◽  
马俊林 Ma Junlin ◽  
...  

2014 ◽  
Vol 51 (5) ◽  
pp. 052202
Author(s):  
陈启梦 Chen Qimeng ◽  
张国玉 Zhang Guoyu ◽  
王哲 Wang Zhe ◽  
张健 Zhang Jian

Sensors ◽  
2020 ◽  
Vol 20 (19) ◽  
pp. 5501
Author(s):  
Yang Bai ◽  
Jianlin Li ◽  
Rongwei Zha ◽  
Ying Wang ◽  
Guangzhi Lei

The optical system is one of the core components for star sensors, whose imaging quality directly influences the performance of star sensors for star detection, thereby determining the attitude control accuracy of spacecrafts. Here, we report a new type of optical system with a catadioptric structure and a large entrance pupil diameter for a 15-magnitude star sensor. It consists of an improved Cassegrain system (R-C system), an aperture correction spherical lens group and a field of view correction spherical lens group. By embedding the secondary mirror of the R-C system into the output surface of the negative spherical lens of the aperture correction spherical lens group, the blocking of incident light is eliminated from the secondary mirror holder. After the structure optimization, the catadioptric optical system (COS) had a spectral range of 450 nm–950 nm, an entrance pupil diameter of 250 mm, a half-diagonal field of view of 1.4° and a focal length of 390 mm. By using theoretical calculations and experimental measurements, it was verified that the COS, with the ability to correct astigmatism, lateral color and distortion, can fulfill the detection of 15-magnitude dark stars.


Author(s):  
Yuanlin Zhao ◽  
Xiangyang Peng ◽  
Shengli Chang ◽  
Wuming Wu

2007 ◽  
Vol 364-366 ◽  
pp. 550-554
Author(s):  
Jun Chang ◽  
Zhi Cheng Weng ◽  
Yong Tian Wang ◽  
De Wen Cheng ◽  
Hui Lin Jiang

In this paper, we are presenting a design method and its results for a space optical system with high resolution and wide field of view. This optical system can be used both in infrared and visible configurations. The designing of this system is based on an on-axis three-mirror anastigmatic (TMA) system. Here the on-axis concept allows wide field of view (FOV) enabling a diversity of designs available for the Multi-Object Spectrometer instruments optimized for low scattered and low emissive light. The available FOVs are upto 1º in both spectrum ranges, whereas the available aperture range is F/15 - F/10. The final optical system is a three-mirror telescope with two on-axis and one off-axis segment and its resolution is 0.3m or even lower. The distinguished feature of this design is that it maintains diffraction-limited image at wide wavelengths. The technological developments in the field of computer generated shaping of large-sized optical surface details with diffraction-limited imagery have opened new avenues towards the designing techniques. Such techniques permit us to expand these technological opportunities to fabricate the aspherical off-axis mirrors for a complex configuration.


2018 ◽  
Vol 47 (9) ◽  
pp. 922003
Author(s):  
李旭阳 LI Xu-yang ◽  
倪栋伟 NI Dong-wei ◽  
杨明洋 YANG Ming-yang ◽  
任志广 REN Zhi-guang

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