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Chinese Academy of Sciences Institutional Repositories Grid
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CAS IR Grid
机构
长春光学精密机械与物... [4]
南京天文光学技术研究... [2]
西安光学精密机械研究... [1]
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OAI收割 [7]
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会议论文 [7]
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2022 [1]
2011 [2]
2010 [2]
2009 [1]
2006 [1]
学科主题
天文望远镜::郭守敬... [2]
天文技术与方法::主... [1]
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Research on selection of high intensity laser beam expanding system
会议论文
OAI收割
Kunming, China, 2021-12-07
作者:
Gao, Na
;
Zhang, XiangHui
;
Liu, Jie
;
Shen, ZeYi
;
Xin, Wei
  |  
收藏
  |  
浏览/下载:49/0
  |  
提交时间:2022/04/27
beam expander
reflecting system
refraction system
off-axis,coaxial
Design of reimaging F/1.0 long-wavelength infrared optical system (EI CONFERENCE)
会议论文
OAI收割
International Symposium on Photoelectronic Detection and Imaging 2011: Advances in Infrared Imaging and Applications, May 24, 2011 - May 24, 2011, Beijing, China
作者:
Zhang X.
;
Zhang X.
;
Zhang X.
收藏
  |  
浏览/下载:35/0
  |  
提交时间:2013/03/25
A reimaging F/1.0 long-wavelength infrared optical system is proposed. The design has a flexible opto-mechanical layout. The design process is as follows. Firstly
the catadioptric reimaging system consists of two reflecting mirrors and a relay lenses. Two reflecting mirrors make up of the first imaging system and are therefore free of chromatic aberrations
while low dispersion lenses were used in the reimaging system
so the optical system do not need achromatic design for a high image quality. Then
to correct high-order aberrations resulting from large relative aperture
more parameters need to be used with aspheric or diffractive surfaces due to modern optic technology development. Here
aspheric is selected for easily manufacture. Finally
the design is completed with the help of ZEMAX software. The effective focal length of the objective is 120mm and the field of view (FOV) is 4. The simulated final design shows adequate image quality and the modulation transfer function (MTF) is close to diffraction limit. The effect of the surrounding environmental temperature is analyzed using the concept of thermal defocusing
and the thermal compensation is discussed. 2011 Copyright Society of Photo-Optical Instrumentation Engineers (SPIE).
Design of visible, infrared dual-channel optical system for space target detection (EI CONFERENCE)
会议论文
OAI收割
2011 International Conference on Electronics and Optoelectronics, ICEOE 2011, July 29, 2011 - July 31, 2011, Dalian, China
Zhang X. Y.
收藏
  |  
浏览/下载:22/0
  |  
提交时间:2013/03/25
This paper designs a total of 250mm dual-channel optical system
including visible (0.5m0.8m)
infrared (3m5m). The main system is a three-reflection system
and the primary mirror is designed as the first and the third reflecting surface with different figuring. The cooling infrared detector was choiced in infrared channel and achieves 100% cool shield efficiency of luminescence through the second imaging. The main benefits of this design are the large corrected and unvignetted FOV
an easily baffling of stray light
small encumbrance and an easy handing. 2011 IEEE.
The optical performance of LAMOST telescope
会议论文
OAI收割
San Diego, California, USA, 2010-6-27
作者:
Yong Zhang
;
Guoping Li
;
Xiangqun Cui
;
Genrong Liu
;
Yeping Li
收藏
  |  
浏览/下载:37/0
  |  
提交时间:2014/01/06
Wide field telescope
Reflecting Schmidt system
Active optics
Segmented mirror
Southern LAMOST for all sky spectroscopic survey
会议论文
OAI收割
San Diego, California, USA, 2010-6-27
作者:
Guoping Li
;
Xiangqun Cui
;
Ding-qiang Su
;
Ya-nan Wang
收藏
  |  
浏览/下载:30/0
  |  
提交时间:2014/01/05
Wide field telescope
Spectroscopic observation
All sky survey
Multi-fiber spectroscopy
Active optics
Reflecting Schmidt system
Segmented mirror
Optical design of reflecting telescope with large field (EI CONFERENCE)
会议论文
OAI收割
4th International Symposium on Advanced Optical Manufacturing and Testing Technologies: Large Mirrors and Telescopes, November 19, 2008 - November 21, 2008, Chengdu, China
作者:
Gong D.
;
Tian T.-Y.
;
Wang H.
收藏
  |  
浏览/下载:23/0
  |  
提交时间:2013/03/25
Reflecting telescopes have been widely used for many outstanding advantages. But the field of a common reflecting system is too small to meet the needs nowadays. When a correcting lens is inserted at the rear of R-C system
the off-axis image quality is significantly improved. After optimizing with CODE V optical design software
a new design scheme of reflecting telescope with large field of view is achieved. 2009 SPIE.
Method for computer-aided alignment of complex optical system (EI CONFERENCE)
会议论文
OAI收割
2nd International Symposium on Advanced Optical Manufacturing and Testing Technologies: Optical Test and Measurement Technology and Equipment, November 2, 2005 - November 5, 2005, Zian, China
作者:
Yu J.
收藏
  |  
浏览/下载:27/0
  |  
提交时间:2013/03/25
For making complex optical system meet the design requirement
such as the space camera used in remote sensing and UVX lithophotography
especially for off-axis all-reflecting optical system
alignment technology is so necessary. In this paper
a method is presented. Based on the ideas of linearity instead of non-linearity and difference quotient instead of differential quotient
a mathematical model for computer-aided alignment is proposed. This model included the characteristics of the optical system
wavefront difference of its exit pupil and its misalignment of the misaligned optical system. Then comparing self-compiled software with alignment package of CODE V
as a result
this self-compiled software is much more valid than alignment package of CODE V. For a large aperture
long focal length and off-axis three-mirror optical system
computer-aided alignment is successful. Finally
the wavefront error of the middle field is 0.094 waves RMS and the wavefront error of +0.7 field is 0.106 waves RMS and the wavefront error of -0.7 field is 0.125 waves RMS at =632.8nm are obtained.