Design of stigmatic grazing incidence telescopes with non-parabolic primaries

Details Design of stigmatic grazing incidence telescopes with non-parabolic primaries Design of stigmatic grazing incidence telescopes with non-parabolic primaries

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979spie..184..223w&link_type=abstract

In: Space optics: Imaging X-ray optics workshop; Proceedings of the Seminar, Huntsville, Ala., May 22-24, 1979. (A80-17469 05-89

Computer Science

Performance

Design Analysis, Grazing Incidence Telescopes, X Ray Telescopes, Aberration, Mirrors, Optimization, Performance Prediction

Scientific paper

A two-mirror grazing-incidence telescope having a non-parabolic primary, and designed to be free of spherical aberration has been investigated. A method for determining the second surface equation is described, when the surface equation for one mirror is given. Application to grazing incidence systems such as used in X-ray and planed for EUV astronomy is discussed. Of special interest is the design of a secondary mirror when the hyperboloid of a conventional Wolter type I system is taken as the primary.

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