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• W1917384098 startingPage "17497" @default.
• W1917384098 abstract "Thermal emission from the deep atmosphere of Venus can be detected on the nightside around 2.3 μm. The analysis of this radiation requires a reliable knowledge of the absorption in the far wings of the nearby allowed CO 2 bands and of the absorption due to collision‐induced bands. We measured absorption coefficients for pure CO 2 at pressures varying from 30 to 60 bars in the frequency range 3910–4570 cm −1 at 297.5 K. Values between 1.0 and 1.6 × 10 −7 cm −1 amagat −2 are found in the 4100–4500 cm −1 interval where emission from the Venus nightside occurs. The comparison of experimental results with synthetic spectra calculated from a line by line code demonstrates that the Lorentzian line shape strongly overestimates the observed absorption, whereas the use of a χ factor extrapolated from the 3800–4000 cm −1 region does not provide enough opacity." @default.
• W1917384098 created "2016-06-24" @default.
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• W1917384098 date "1991-09-25" @default.
• W1917384098 modified "2023-09-27" @default.
• W1917384098 title "Measurements of pure CO₂absorption at high densities near 2.3 μm" @default.
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• W1917384098 doi "https://doi.org/10.1029/91je01680" @default.
• W1917384098 hasPublicationYear "1991" @default.
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