Paper
21 August 2009 A spherical catadioptric telescope system based on Cooke corrector group
Jian Zhang, Yusi Kang, Weiqi Liu
Author Affiliations +
Abstract
To obtain a number of advantages in fabrication, testing and alignment, many designs in which spherical mirrors replace classical Cassegrain-form aspheric mirrors are present in the literature. However, spherical mirrors suffer from substantial spherical aberration and thereby require some form of corrector group. But in this case, the question encountered is that of making the basic optical configuration more complex. In this paper, a new design based on Cooke corrector group is presented for eliminating spherical aberration, which is believed to provide higher performance with less complexity than previous approaches. Besides, the cost and fabrication period will be extremely decreased. The telescope system using corrector group here can achieve good optical performance with f# of 10, full field of 0.5°, obscuration of 1/3 and MTF (Modulation Transfer Function) of 0.48 corresponding to 50@lp/mm.
© (2009) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jian Zhang, Yusi Kang, and Weiqi Liu "A spherical catadioptric telescope system based on Cooke corrector group", Proc. SPIE 7429, Novel Optical Systems Design and Optimization XII, 74290T (21 August 2009); https://doi.org/10.1117/12.825562
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KEYWORDS
Mirrors

Spherical lenses

Telescopes

Monochromatic aberrations

Combined lens-mirror systems

Aspheric optics

Modulation transfer functions

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