scholarly journals The Boundary between the Cone-crown Telescope System and the Magnetic Attachment

2004 ◽  
Vol 48 (2) ◽  
pp. 154-158
Author(s):  
Kohei Kimura ◽  
Taro Kanno
1992 ◽  
Vol 36 (3) ◽  
pp. 471-480 ◽  
Author(s):  
Yoshinobu Tanaka ◽  
Eiichi Bando ◽  
Naoki Nagamachi ◽  
Atsushi Suzuki ◽  
Yasuo Kishimoto ◽  
...  

1984 ◽  
Vol 79 ◽  
pp. 607-616
Author(s):  
R. R. Shannon

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.


2021 ◽  
Vol 11 (3) ◽  
pp. 1200
Author(s):  
Junliu Fan ◽  
Quanying Wu ◽  
Baohua Chen ◽  
Lin Liu ◽  
Lei Chen

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.


1984 ◽  
Vol 51 (4) ◽  
pp. 450-455 ◽  
Author(s):  
H. Sasaki ◽  
Y. Kinouchi ◽  
H. Tsutsui ◽  
Y. Yoshida ◽  
T. Ushita
Keyword(s):  

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

2017 ◽  
Vol 55 (1) ◽  
pp. 53 ◽  
Author(s):  
Yu Jin Lee ◽  
Richard Leesungbok ◽  
Suk Won Lee ◽  
Su Jung Park ◽  
Su Jin Ahn

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

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