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- W2149019892 abstract "A grating spectrometer with a Ge/Cu detector was flown on several balloon flights during which the variation of the infrared solar spectrum in the 3- to 5-μ region was recorded. Atmospheric absorption spectra were obtained at various altitudes from ground through 30 km with a resolution of ∼0.3 cm−1. Intense CO lines from both P and R branches are observed in the 2150-cm−1 region. In particular, the R (2) and R (3) lines in the (1–0) fundamental ban are clearly isolated from the neighboring H2O and N2O lines, so that the vertical distribution of CO in the atmosphere can be determined from these lines. A line-by-line, layer-by-layer computer program has been developed that derives the CO amounts in a layered atmosphere where the layers are defined by the actual altitudes of observations. The resulting altitude profile shows that the CO concentration between 4 and 15 km is gradually decreasing from ∼8 × 10−2 ppm to ∼4 × 10−2 ppm." @default.
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- W2149019892 date "1973-08-20" @default.
- W2149019892 modified "2023-10-16" @default.
- W2149019892 title "Vertical distribution of CO in the atmosphere" @default.
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- W2149019892 doi "https://doi.org/10.1029/jc078i024p05273" @default.
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