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Proceedings Paper

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

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.

Paper Details

Date Published: 22 October 1999
PDF: 13 pages
Proc. SPIE 3765, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy X, (22 October 1999); doi: 10.1117/12.366527
Show Author Affiliations
Raymond G. Ohl, Johns Hopkins Univ. and Univ. of Virginia (United States)
Scott D. Friedman, Johns Hopkins Univ. (United States)
Timo T. Saha, NASA Goddard Space Flight Ctr. (United States)
Robert H. Barkhouser, Johns Hopkins Univ. (United States)
Henry W. Moos, Johns Hopkins Univ. (United States)


Published in SPIE Proceedings Vol. 3765:
EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy X
Oswald H. W. Siegmund; Kathryn A. Flanagan, Editor(s)

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