Baranov, Y. I., and W. J. Lafferty (2011), The water‐vapor continuum and selective absorption in the 3 to 5 μm spectral region at temperatures from 311 to 363K, J. Quant. Spectrosc. Radiat. Transfer, 112, 1304–1313, doi:10.1016/j.jqsrt.2011.01.024.
n most near‐infrared atmospheric windows, absorption of solar radiation is dominated by the water vapor self‐continuum, and yet there is a paucity of measurements in these windows. We report new laboratory measurements of the self‐continuum absorption at temperatures between 293 and 472 K and pressures from 0.015 to 5 atm in four near‐infrared windows between 1 and 4 μm (10000–2500 cm−1); the measurements are made over a wider range of wavenumbers, temperatures, and pressures than any previous measurements. They show that the self‐continuum in these windows is typically one order of magnitude stronger than given in representations of the continuum widely used in climate and weather prediction models. These results are also not consistent with current theories attributing the self‐continuum within windows to the far wings of strong spectral lines in the nearby water vapor absorption bands; we suggest that they are more consistent with water dimers being the major contributor to the continuum. The calculated global average clear‐sky atmospheric absorption of solar radiation is increased by ∼0.75 W/m2 (which is about 1% of the total clear‐sky absorption) by using these new measurements as compared to calculations with the MT_CKD‐2.5 self‐continuum model.
JGR-Atmospheres includes physics and chemistry of the atmosphere, as well as the atmospheric-biospheric, lithospheric, and hydrospheric interface.
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The pure water-vapor continuum absorption in the 2.88 to 5.18 μm spectral region has been measured using a Fourier-transform infrared spectrometer at a resolution of 0.1 cm−1. The sample temperatures and pressures varied from 311 to 363 K and from 2.8 kPa (21 Torr) to 34.5 kPa (259 Torr), respectively. The path lengths used in the study ranged from 68 to 116 m. Under these conditions, the continuum absorption in the middle of the 4 μm window is quite detectable reaching as high as 4%. The spectral processing included calculations to fit and remove the H2O ro-vibrational structure. In the region around 5 μm, the absorption coefficients obtained are in good agreement with those of the commonly used MT_CKD continuum model. However at shorter wavelengths, the observed values significantly deviate from the model. Inspection of the present data as well as that of previous measurements leads to the conclusion that the MT_CKD model despite the latest updates significantly underestimates the rate of the continuum temperature dependence over the 4 μm atmospheric window. Line strengths for 189 H2O transitions were obtained from the spectral processing. The deviation of these measured intensities from those listed in the HITRAN database is randomly scattered around zero to within several percents and no systematic trends were detected.
