Optical testing of the Far-Ultraviolet Spectroscopic Explorer primary mirrors and predicted on-orbit performance

Details Optical testing of the Far-Ultraviolet Spectroscopic Explorer primary mirrors and predicted on-orbit performance Optical testing of the Far-Ultraviolet Spectroscopic Explorer primary mirrors and predicted on-orbit performance

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spie.3765..482o&link_type=abstract

Proc. SPIE Vol. 3765, p. 482-494, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy X, Oswald H. Siegmund; Kathryn A. Flan

Astronomy and Astrophysics

Astronomy

Scientific paper

The FUSE is an astrophysics satellite designed to provide high resolution spectra with large effective area over the interval 90.5-118.7 nm. The FUSE instrument consists of four co-aligned, normal incidence, off-axis parabolic primary mirrors which illuminate separate Rowland circle spectrograph channels equipped with holographic gratings and delay line microchannel plate detectors.

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