Comparison of near-room temperature measurements of the water vapour self-continuum cross-sections between 2000 and 7000 cm-1. [16] Y.I. Baranov, W.J. Lafferty, The water-vapor continuum and selective absorption in the 3–5 μm spectral region at temperatures from 311° to 363°K, J. Quant. Spectrosc. Radiat. Transfer 112 (2011) 1304–1313, http://dx.doi.org/10.1016/j.jqsrt.2011.01.024.
Spectroscopic catalogues, such as GEISA and HITRAN, do not yet include information on the water vapour continuum that pervades visible, infrared and microwave spectral regions. This is partly because, in some spectral regions, there are rather few laboratory measurements in conditions close to those in the Earth’s atmosphere; hence understanding of the characteristics of the continuum absorption is still emerging. This is particularly so in the near-infrared and visible, where there has been renewed interest and activity in recent years. In this paper we present a critical review focusing on recent laboratory measurements in two near-infrared window regions (centred on 4700 and 6300 cm−1) and include reference to the window centred on 2600 cm−1 where more measurements have been reported. The rather few available measurements, have used Fourier transform spectroscopy (FTS), cavity ring down spectroscopy, optical-feedback – cavity enhanced laser spectroscopy and, in very narrow regions, calorimetric interferometry. These systems have different advantages and disadvantages. Fourier Transform Spectroscopy can measure the continuum across both these and neighbouring windows; by contrast, the cavity laser techniques are limited to fewer wavenumbers, but have a much higher inherent sensitivity. The available results present a diverse view of the characteristics of continuum absorption, with differences in continuum strength exceeding a factor of 10 in the cores of these windows. In individual windows, the temperature dependence of the water vapour self-continuum differs significantly in the few sets of measurements that allow an analysis. The available data also indicate that the temperature dependence differs significantly between different near-infrared windows. These pioneering measurements provide an impetus for further measurements. Improvements and/or extensions in existing techniques would aid progress to a full characterisation of the continuum – as an example, we report pilot measurements of the water vapour self-continuum using a supercontinuum laser source coupled to an FTS. Such improvements, as well as additional measurements and analyses in other laboratories, would enable the inclusion of the water vapour continuum in future spectroscopic databases, and therefore allow for a more reliable forward modelling of the radiative properties of the atmosphere. It would also allow a more confident assessment of different theoretical descriptions of the underlying cause or causes of continuum absorption.
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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.