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SAGE III test model: ground-based coincident measurements with the SAGE III flight instruments and field characterization measurements (Proceedings Paper)

Author(s): Robert E. Veiga; Brian N. Wenny; Gary M. Hansen; Patricia L. Lucker; William P. Chu
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Optical Spectroscopic Techniques, Remote Sensing, and Instrumentation for Atmospheric and Space Research IV, Allen M. Larar; Martin G. Mlynczak, Editors, pp.135-141

Date: 30 January 2002

Paper Abstract

Five functional UV-VIS-NIR spectrometer/telescopes were built for the Stratospheric Aerosol and Gas Experiment III (SAGE III) satellite instrument project. Three will be on satellite platforms in the early part of the decade, and a fourth, the SAGE III Test Model (TM) is functioning as a ground-based instrument. The fifth is used as a software test-bed to support Mission Operations for the space instruments. The SAGE III instrument is spatially scanning UV-VIS-NIR holographic grating spectrometer using a co
DOI: 10.1117/12.454244
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