Absolute line intensities in CO2 bands near 4.8 microns

Details Absolute line intensities in CO2 bands near 4.8 microns Absolute line intensities in CO2 bands near 4.8 microns

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apopt..25.1204r&link_type=abstract

Applied Optics (ISSN 0003-6935), vol. 25, April 1, 1986, p. 1204-1214. USAF-supported research.

Physics

Optics

29

Carbon Dioxide, Infrared Spectra, Molecular Spectra, Remote Sensing, Atmospheric Pressure, Fourier Transformation, Tables (Data)

Scientific paper

Absolute intensities for 726 unblended lines in 20 bands of C-12(O-16)2, C-13(O-16)2, O-16C-12O-18, and O-16C-12O-17 in the 4.8-micron spectral region have been determined using a natural sample of ultrahigh-purity CO2. Spectral data were recorded at low pressure (less than 10 torr) and room temperature with the Fourier transform spectrometer in the McMath solar telescope complex on Kitt Peak. Derived vibrational band intensities and coefficients of the F factor for each band were compared to values of the 1982 Air Force Geophysics Laboratory line parameters compilation. The present work fills out the CO2 lines in the 5-micron band systems. Lines in the strongest of these measured bands are being used to infer atmospheric pressure from high-resolution stratospheric spectra recorded during the Spacelab 3 Atmospheric Trace Molecule Spectroscopy experiment.

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