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The earth's mesospheric carbon monoxide was observed in absorption against the moon in early December 1979 at a wavelength of 1.3 mm and in early December 1980 at a wavelength of 2.6 mm. These wavelengths correspond to the respective rotational transitions of CO, J = 1 → 2 and J = 0 → 1. No significant change in the column density of CO above ∼65 km is found between the 1979 and 1980 observations. Inversion of the spectra did not provide unique CO mixing ratio profiles for a direct quantitative comparision of December 1979 and 1980 profiles, due to limited signal‐to‐noise ratios. Comparison with other published spectra of mesospheric CO suggests a large seasonal variation (about a factor of 2–3) in the column density of CO above 65 km, with a maximum in winter and a minimum in summer.
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Clancy et al. (1982) studied this question.
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