The Spartan-281 Far Ultraviolet Imaging Spectrograph

Details The Spartan-281 Far Ultraviolet Imaging Spectrograph The Spartan-281 Far Ultraviolet Imaging Spectrograph

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988spie..932...87c&link_type=abstract

IN: Ultraviolet technology II; Proceedings of the Meeting, Orlando, FL, Apr. 4, 5, 1988 (A89-29476 11-19). Bellingham, WA, Socie

Computer Science

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Far Ultraviolet Radiation, Spaceborne Astronomy, Spectrographs, Ultraviolet Astronomy, Ultraviolet Spectrometers, Comets, H Ii Regions, Interstellar Matter, Planetary Nebulae, Reflection Nebulae, Schmidt Telescopes, Sounding Rockets, Stellar Winds, Supernova Remnants

Scientific paper

The U.S. Naval Research Laboratory's Far Ultraviolet Imaging Spectrograph (FUVIS), currently under development for flight as a Spartan shuttle payload, is designed to perform spectroscopy of diffuse sources in the FUV with very high sensitivity and moderate spatial and spectral resolution. Diffuse nebulae, the general galactic background radiation, and artificially induced radiation associated with the Space Shuttle vehicle are sources of particular interest. The FUVIS instrument will cover the wavelength range of 970-2000 A with selectable resolutions of 5 and 30 A. It is a slit imaging spectrograph having 3 arcmin spatial resolution along its 2.7 deg long slit.

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