High-Resolution Optical Telescope For Ultraviolet (UV) Radiation Field

Wahe W. Karayan

doi:10.1117/12.957955

15 November 1979 High-Resolution Optical Telescope For Ultraviolet (UV) Radiation Field

Wahe W. Karayan

Proceedings Volume 0196, Measurements of Optical Radiations; (1979) https://doi.org/10.1117/12.957955
Event: 23rd Annual Technical Symposium, 1979, San Diego, United States

Abstract

Design techniques are discussed for all-reflecting optics from first-order system considerations and applications currently utilized in the field of astronomical optics. The solution to the Dall-Karkham design problem is described, showing the advantage of inexpensive construction as compared with higher order surfaces. The design process reported here is a F/5 collecting system which quickly mates directly with the spectrometer; it is capable of achieving desired high resolution and sensitivity requirements. The theoretical limit of aberration tolerances is achieved with less than 1/8 of a wavelength at final focus (OPD). The design of spectrometer for ultra-violet (UV) radiation and its mechanism is included in this study.

Citation Download Citation

Wahe W. Karayan "High-Resolution Optical Telescope For Ultraviolet (UV) Radiation Field", Proc. SPIE 0196, Measurements of Optical Radiations, (15 November 1979); https://doi.org/10.1117/12.957955

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KEYWORDS

Mirrors

Ultraviolet radiation

Monochromatic aberrations

Spectroscopy

Optical testing

Diffraction gratings

Spectral resolution

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