Overview of environment simulation device for large aperture optical imaging quality test

2021 ◽  
Author(s):  
Jiang Di ◽  
Yarong Shao ◽  
Shuang Wang ◽  
Hexin Li ◽  
Bo Li
2016 ◽  
Vol 24 (5) ◽  
pp. 1118-1127 ◽  
Author(s):  
朱俊青 ZHU Jun-qing ◽  
沙 巍 SHA Wei ◽  
陈长征 CHEN Chang-zheng ◽  
张星祥 ZHANG Xing-xiang ◽  
任建岳 REN Jian-yue

2007 ◽  
Vol 364-366 ◽  
pp. 1231-1236 ◽  
Author(s):  
Li Rong Zhu ◽  
Wei Min Shen

Four-mirror systems with a very large aperture and a long focal length were investigated and designed. Their design idea is given. Through the derivation of primary aberration formula, the aberration properties were analyzed and discussed, and the method to determine its initial structure is reported. As examples, two four-mirror systems with spherical and parabolic primary mirror, 100m focal length, and 10m entrance pupil were optimally designed. Their imaging quality approaches diffraction limit within field of view of 0.4 and 0.5 degrees respectively.


2015 ◽  
Vol 150 ◽  
pp. 79-87 ◽  
Author(s):  
Aysegul Cumurcu ◽  
Jordi Diaz ◽  
Ian D. Lindsay ◽  
Sissi de Beer ◽  
Joost Duvigneau ◽  
...  

1991 ◽  
Author(s):  
Pascal O. Rol ◽  
Dominik Beck ◽  
Peter F. Niederer

2012 ◽  
Vol 516 ◽  
pp. 181-185
Author(s):  
Yang Lin Peng ◽  
Yi Fan Dai ◽  
Shan Yong Chen

The surface figure of the primary mirror in a large aperture telescope is one of the key factors influencing imaging quality. Space telescopes are used in weightless environments, which is different from the ground environment for optical machining and testing. Therefore the effect of the deformation induced by gravity on the imaging quality is not negligible and the mirror support is to be carefully designed to unload the gravity during the course of machining and testing. In this paper, finite element analysis software is adopted to simulate and compare the deformation induced by gravity of a metre-scale aspheric lightweight primary mirror with different support methods and different working conditions. The results are then imported into MetroPro software supplied by ZYGO Corporation, to remove the tilts and rigid body motion of the mirror and calculate the primary aberrations from the deformation. Finally, sensitivity analysis of support deformation is implemented and the principles of mirror support design are summarized. The research is instructive for design, machining and testing of large aperture mirrors.


2006 ◽  
Author(s):  
Xinhua Niu ◽  
Yao Zhu ◽  
Qingbo Zheng

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