A spherical catadioptric telescope system based on Cooke corrector group

2009 ◽  
Author(s):  
Jian Zhang ◽  
Yusi Kang ◽  
Weiqi Liu
Keyword(s):  
Telescope System

scholarly journals Recent Developments in Coatings, Gratings, and Reflective Components

1984 ◽  
Vol 79 ◽  
pp. 607-616
Author(s):  
R. R. Shannon
Keyword(s):  
State Of The Art ◽  
New Technology ◽  
The State ◽  
Current Technology ◽  
Large Size ◽  
Incoming Radiation ◽  
Recent Developments ◽  
Electronic Sensors ◽  
Large Primary ◽  
Telescope System

The requirements on gratings and coatings for astronomical use differ from the general industrial requirements primarily in the scale of the components to be fabricated. Telescopes have large primary mirrors which require large coating plants to handle the components. Dispersive elements are driven by the requirement to be efficient in the presence of large working apertures, and usually optimize to large size in order to efficiently use the incoming radiation. Beyond this, there is a “new” technology of direct electronic sensors that places specific limits upon the image scale that can be used at the output of a telescope system, whether direct imagery or spectrally divided imagery is to be examined. This paper will examine the state of the art in these areas and suggest some actions and decisions that will be required in order to apply current technology to the predicted range of large new telescopes.

scholarly journals Optical Design of the Goaly3 Multi-Mirror Telescope System with a Wide Field of View

2021 ◽  
Vol 11 (3) ◽  
pp. 1200
Author(s):  
Junliu Fan ◽  
Quanying Wu ◽  
Baohua Chen ◽  
Lin Liu ◽  
Lei Chen
Keyword(s):  
Fill Factor ◽  
Optical Design ◽  
Tolerance Analysis ◽  
Field Of View ◽  
Wide Field ◽  
Aspheric Surfaces ◽  
The Monte Carlo Method ◽  
Wide Field Of View ◽  
Mirror Telescope ◽  
Telescope System

A Golay3 multi-mirror telescope (MMT) system is designed in this paper. The fill factor of the Golay3 MMT is derived from the angular resolution of the telescope. An initial configuration is established according to the paraxial optical theory. A three-element aspheric corrector group is designed and placed in the converging light cone to enlarge the field of view (FOV) of the Golay3 MMT. The tolerance analysis for each surface of the Golay3 MMT is conducted using the Monte Carlo method. The design results show the FOV of the Golay3 MMT system can be increased to 1.5° with the insertion of a three-element aspheric corrector group. The results of the tolerance analysis indicate that most tolerances are loose, while some decenter tolerances relating with the aspheric surfaces are relatively tight, but still within an acceptable range.

scholarly journals Comparison and analysis on Polarization aberration in Pehan prisms and the Telescope system including Pehan prisms

2011 ◽  
Vol 19 ◽  
pp. 436-441
Author(s):  
Lu Jinjun ◽  
Li Xiangyang ◽  
Yuan Qiao ◽  
Sun Xueping ◽  
Guo Xiaochuan
Keyword(s):  
Comparison And Analysis ◽  
Telescope System

New type optical Cassegrain antenna with lenses telescope system

Optik ◽  
2010 ◽  
Vol 121 (6) ◽  
pp. 521-525 ◽  
Author(s):  
Liuping Xiao ◽  
Huajun Yang ◽  
Xiaojing Liu ◽  
Quan Xu ◽  
Xinqiang Xiong
Keyword(s):  
Cassegrain Antenna ◽  
New Type ◽  
Telescope System

Polarization Analysis of the Telescope System Used for Space Target Polarization Detection

2014 ◽  
Vol 34 (12) ◽  
pp. 1211003
Author(s):  
王国聪 Wang Guocong ◽  
王建立 Wang Jianli ◽  
张振铎 Zhang Zhenduo ◽  
明名 Ming Ming ◽  
张斌 Zhang Bin ◽  
...  
Keyword(s):  
Polarization Analysis ◽  
Target Polarization ◽  
Polarization Detection ◽  
Telescope System ◽  
Space Target

Design of Golay 3 telescope system

2011 ◽  
Vol 19 (12) ◽  
pp. 2877-2883 ◽  
Author(s):  
范君柳 FAN Jun-liu ◽  
吴泉英 WU Quan-ying ◽  
王福亮 WANG Fu-liang ◽  
沈婷婷 SHEN Ting-ting
Keyword(s):  
Telescope System
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