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29 June 1992 UVSTAR, an imaging spectrograph with telescope for the Shuttle Hitchhiker-M platform
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Abstract
The Ultraviolet Spectrograph Telescope for Astronomical Research (UVSTAR), is an EUV spectral imager for solar system and stellar astronomy that covers the 500-1250 A wavelength range with sufficient spectral resolution to distinguish atomic emission lines and form spectrally resolved images of extended plasma sources. UVSTAR employs a pair of telescopes and concave-grating spectrographs that cover the overlapping 500-900 A and 850-1250 A spectral ranges.
© (1992) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Bill R. Sandel, A. Lyle Broadfoot, and Roberto Stalio "UVSTAR, an imaging spectrograph with telescope for the Shuttle Hitchhiker-M platform", Proc. SPIE 1745, Instrumentation for Planetary and Terrestrial Atmospheric Remote Sensing, (29 June 1992); https://doi.org/10.1117/12.60620
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