The two-mirror telescopes/cameras that have no coma, no spherical aberration and arbitrarily fast focal ratios form a two-parameter (s, K) family of exact optical designs analytically derived earlier. We explore the full range of these designs in the s-K plane. Here s is the mirror separation/focal length and K is the distance from secondary to focus/focal length. Besides perfect-focus analogues of most well-known telescope designs, there are families of spectrograph cameras, X-ray telescopes and solar furnaces. Systems with s = 2 have minimum astigmatism and have exceptionally good images.
CITATION STYLE
Willstrop, R. V., & Lynden-Bell, D. (2003). Exact optics - II. Exploration of designs on- and off-axis. Monthly Notices of the Royal Astronomical Society, 342(1), 33–49. https://doi.org/10.1046/j.1365-8711.2003.06434.x
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