Paper
22 January 1993 AURA, an experiment to measure ultraviolet radiation of the earth's atmosphere from space
Michael E. Gangl, John H. Middlestadt, Richard W. Eastes
Author Affiliations +
Abstract
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.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael E. Gangl, John H. Middlestadt, and Richard W. Eastes "AURA, an experiment to measure ultraviolet radiation of the earth's atmosphere from space", Proc. SPIE 1764, Ultraviolet Technology IV, (22 January 1993); https://doi.org/10.1117/12.140870
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Ultraviolet radiation

Spectroscopy

Telescopes

Sensors

Space operations

Space telescopes

Back to Top