Physics
Scientific paper
Jan 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993spie.1764...50g&link_type=abstract
In: Ultraviolet technology IV; Proceedings of the Meeting, San Diego, CA, July 20, 21, 1992 (A93-34426 13-35), p. 50-60.
Physics
Atmospheric Radiation, Earth Observations (From Space), Imaging Techniques, Radiation Measurement, Ultraviolet Radiation, Earth Atmosphere, Ionospheric Electron Density, Remote Sensing
Scientific paper
The Atmospheric Ultraviolet Radiance Analyzer (AURA) has been designed to furnish global UV emissions measurements in the 115-175 nm range of sufficient sensitivity for observations of the weak emissions from the tropical arcs and the aurora from a nearly circular high-inclination orbit. Excellent S/N is obtained by AURA in the case of day airglow measurements. Two UV observation channels are available, each of which is based on a 1/8 Ebert-Fastie spectrometer and a telescope with a scanning mirror; each can furnish data in any one of three operational modes.
Eastes Richard Wayne
Gangl Michael E.
Middlestadt John H.
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