The Earth’s Clear-Sky Radiation Budget and Water Vapor Absorption in the Far Infrared

Ashok Sinha Space and Atmospheric Physics Group, Blackett Laboratory, Imperial College of Science, Technologyand Medicine, London, United Kingdom

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John E. Harries Space and Atmospheric Physics Group, Blackett Laboratory, Imperial College of Science, Technologyand Medicine, London, United Kingdom

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Abstract

Detailed observational data are used to simulate the sensitivity of clear-sky outgoing longwave radiation (OLR) to water vapor perturbations in order to investigate the effect of uncertainties in water vapor measurements and spectroscopic parameters. Seasonal, geographical, and spectral variations in the clear-sky OLR, and of zonal mean clear-sky atmospheric cooling rate profiles are calculated for this purpose. Outside of deep convective regions, when only water vapor is varied, it is found that the 20–30-μm waveband of the far infrared (FIR) is the most substantial influence on the clear-sky OLR change. By contrast, the largest contribution to the clear-sky OLR variation in deep convective areas is from the continuum. Similarly, seasonal clear-sky infrared cooling rates are largely determined by contributions from the FIR and continuum, with a systematic variation in these contributions with latitude and altitude. The results presented reinforce the conclusions of recent studies that the lack of validation of FIR model line parameters under atmospheric conditions may have serious implications for the accuracy of simulations of clear-sky OLR variability. FIR parameterizations in climate models should be therefore validated by observational programs.

Corresponding author address: Dr. Ashok Sinha, Blackett Laboratory, Imperial College of Science, Technology and Medicine, London SW7 2BZ, United Kingdom.

Abstract

Detailed observational data are used to simulate the sensitivity of clear-sky outgoing longwave radiation (OLR) to water vapor perturbations in order to investigate the effect of uncertainties in water vapor measurements and spectroscopic parameters. Seasonal, geographical, and spectral variations in the clear-sky OLR, and of zonal mean clear-sky atmospheric cooling rate profiles are calculated for this purpose. Outside of deep convective regions, when only water vapor is varied, it is found that the 20–30-μm waveband of the far infrared (FIR) is the most substantial influence on the clear-sky OLR change. By contrast, the largest contribution to the clear-sky OLR variation in deep convective areas is from the continuum. Similarly, seasonal clear-sky infrared cooling rates are largely determined by contributions from the FIR and continuum, with a systematic variation in these contributions with latitude and altitude. The results presented reinforce the conclusions of recent studies that the lack of validation of FIR model line parameters under atmospheric conditions may have serious implications for the accuracy of simulations of clear-sky OLR variability. FIR parameterizations in climate models should be therefore validated by observational programs.

Corresponding author address: Dr. Ashok Sinha, Blackett Laboratory, Imperial College of Science, Technology and Medicine, London SW7 2BZ, United Kingdom.

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