Paper
23 July 2008 Free-forms optics into astronomical use: the case of an all-mirror anamorphic collimator
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Abstract
Up to now, optical design of astronomical instrumentation has been based onto "classical" surfaces, i.e. plano surfaces, spherical surfaces, and some classes of aspheric surfaces. More complex surfaces (like cylinders), are used from time to time to correct for aberrations. A new class of more general surfaces, i.e. non-rotationally symmetrical and completely "free-form" surfaces have been recently introduced. Their use in astronomy, however, has not widely used so far. We propose a new layout for an anamorphic collimator based onto two "free-form" cylinder surfaces, giving diffraction limited images. This collimator can be used to create an elliptical pupil, and allows reducing size of optical systems, too. Two interesting cases of application in astronomy are shown: a very-high resolution spectrograph for large telescopes, and an interferometer cavity to test large plano optics.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Paolo Spanò "Free-forms optics into astronomical use: the case of an all-mirror anamorphic collimator", Proc. SPIE 7018, Advanced Optical and Mechanical Technologies in Telescopes and Instrumentation, 701840 (23 July 2008); https://doi.org/10.1117/12.789183
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Cited by 4 scholarly publications.
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KEYWORDS
Collimators

Interferometers

Mirrors

Astronomy

Spectrographs

Surface finishing

Image quality

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