OSAC analysis of the Far Ultraviolet Spectroscopic Explorer (FUSE) telescope

Details OSAC analysis of the Far Ultraviolet Spectroscopic Explorer (FUSE) telescope OSAC analysis of the Far Ultraviolet Spectroscopic Explorer (FUSE) telescope

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986spie..640...79s&link_type=abstract

IN: Grazing incidence optics; Proceedings of the Meeting, Orlando, FL, Apr. 3, 4, 1986 (A87-42701 19-74). Bellingham, WA, Societ

Physics

Optics

Far Uv Spectroscopic Explorer, Optical Correction Procedure, Surface Properties, Ultraviolet Telescopes, Computer Programs, Mirrors

Scientific paper

An investigation is made of the sensitivity of the image quality for the proposed FUSE telescope to mirror misalignments and a wide spatial frequency range of figure errors. Representative figure error data was obtained for the analysis from measurements made on the SEUTS (Solar Extreme Ultraviolet Telescope Spectrograph) telescope mirrors. The tolerancing analysis was carried out with the aid of the Optical Surface Analysis Code (OSAC) program.

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