Long Path Atmospheric Ozone Absorption in the 9–10-μ Region Observed from a Balloon-Borne Spectrometer
- 1 March 1970
- journal article
- Published by Optica Publishing Group in Applied Optics
- Vol. 9 (3), 565-580
- https://doi.org/10.1364/ao.9.000565
Abstract
A balloon-borne spectrometer was used to measure the atmospheric absorption of solar radiation in the 9–10-μ region as a function of altitude. Among the numerous spectra recorded, several were made with very long optical paths above the troposphere obtained from floating altitude (~30 km) while the sun set. When the experimental results are compared with calculated spectra, based on line by line parameters of the ν3 and ν1 fundamentals of ordinary ozone, 16O3, combined with the Curtis-Godson approximation, large discrepancies are found for the long path spectra. It is shown that the hot bands ν3 + ν2 − ν2 and ν3 + ν3 − ν3 of the 16O3, and the ν3 fundamentals of the isotopic species 16O18O16O and 16O16O18O, can contribute significant absorption for long paths such as obtained in this experiment. Such long paths also give rise to significant absorptions by the ν3 − ν1 and the ν3 − 2ν2° bands of CO2. Including these weak bands in the calculated spectra leads to good agreement with the observed data.This publication has 12 references indexed in Scilit:
- Variation of the Infrared Solar Spectrum Between 700 cm^−1 and 2240 cm^−1 with AltitudeApplied Optics, 1969
- A Comparison Between Statistical Model and Line by Line Calculation with Application to the 96-μ Ozone and the 27-μ Water Vapor BandsApplied Optics, 1968
- Nitric Acid and Nitric Oxide in the Lower StratosphereNature, 1968
- The infrared spectrum of ozoneJournal of Molecular Spectroscopy, 1968
- A Balloon-Borne Grating SpectrometerApplied Optics, 1967
- The computation of infra‐red cooling rate in planetary atmospheresQuarterly Journal of the Royal Meteorological Society, 1966
- A Study of the Solar Spectrum from 7 μ to 400 μApplied Optics, 1965
- Attenuation by Ozone and the Earth’s Albedo in the Middle UltravioletApplied Optics, 1964
- Structure of Ozone from the Microwave Spectrum between 9000 and 45 000 McThe Journal of Chemical Physics, 1956
- The Solar Spectrum from 7 μ to 13 μ.The Astrophysical Journal, 1952