Wide-field optical design for a 60 m submillimeter telescope

被引:6
|
作者
Lou, Zheng [1 ,2 ]
Zuo, Ying-xi [1 ,2 ]
Yao, Qi-jun [1 ,2 ]
Shi, Sheng-cai [1 ,2 ]
Yang, Ji [1 ,2 ]
Chen, Xue-peng [1 ,2 ]
机构
[1] Chinese Acad Sci, Purple Mt Observ, 10 Yuanhua Rd, Nanjing 210033, Peoples R China
[2] Chinese Acad Sci, Key Lab Radio Astron, 10 Yuanhua Rd, Nanjing 210033, Peoples R China
基金
中国国家自然科学基金;
关键词
ABERRATIONS;
D O I
10.1364/AO.388320
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
We present a practical wide-field optical design for a 60 m aperture submillimeter telescope, which is currently under conceptual design study in China. The telescope is specified to operate over a wavelength range of 0.65-3mm and provide a wide field of view (FOV) of 1 degrees in diameter. We designed an F/6 Ritchey Chretien (RC) system with a quasi-planar tertiary corrector, which cancels all spherical, coma, and astigmatism aberrations. It also achieves a good balance among the mirror sizes, central obscuration, and focal-plane curvature. The problems of focal surface curvature and nontelecentricity are treated in the subfield instrumental design, which employs a simple silicon wedge prism to obtain flat and telecentric focal planes for each subfield instrument module. Our studies show that by such a design, more than 10(5) detector pixels can be efficiently and uniformly fed at the shortest wavelength band with Strehl ratios above 0.85 across the entire 1 degrees FOV. Several practical issues related to the telescope optics are also discussed. (C) 2020 Optical Society of America
引用
收藏
页码:3353 / 3359
页数:7
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