Paper
1 September 1991 Analysis of atmospheric trace constituents from high-resolution infrared balloon-borne and ground-based solar absorption spectra
Aaron Goldman, Frank J. Murcray, Curtis P. Rinsland, Ronald D. Blatherwick, F. H. Murcray, David G. Murcray
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Abstract
Results of ongoing studies of high-resolution solar absorption spectra aimed at the identification and quantification of trace constituents of importance in the chemistry of the stratosphere and upper troposphere are presented. An analysis of balloon-borne and ground-based spectra obtained at 0.0025/cm covering the 700-2200/cm interval is presented. The 0.0025/cm spectra, along with corresponding laboratory spectra, improves the spectral line parameters, and thus the accuracy of quantifying trace constituents. Results for COF2, F22, SF6, and other species are presented. The retrieval methods used for total column density and altitude distribution for both ground-based and balloon-borne spectra are also discussed.
© (1991) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Aaron Goldman, Frank J. Murcray, Curtis P. Rinsland, Ronald D. Blatherwick, F. H. Murcray, and David G. Murcray "Analysis of atmospheric trace constituents from high-resolution infrared balloon-borne and ground-based solar absorption spectra", Proc. SPIE 1491, Remote Sensing of Atmospheric Chemistry, (1 September 1991); https://doi.org/10.1117/12.46662
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Cited by 3 scholarly publications.
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KEYWORDS
Absorption

Gases

Infrared radiation

Spectroscopic atmospheric monitoring techniques

Atmospheric monitoring

Spectral resolution

Spectroscopy

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