This study finds a 30% difference between modeled and observed solar energy absorbed by the atmosphere.
Juan Du, Li Huang, Qilong Min, Lei Zhu. The influence of water vapor absorption in the 290-350 nm region on solar radiance: Laboratory studies and model simulation. Geophysical Research Letters. DOI: 10.1002/grl.50935
Water vapor is an important greenhouse gas in the earth’s atmosphere. Absorption of the solar radiation by water vapor in the near UV region may partially account for the up to 30% discrepancy between the modeled and the observed solar energy absorbed by the atmosphere. But the magnitude of water vapor absorption in the near UV region at wavelengths shorter than 384 nm is not known. We have determined absorption cross sections of water vapor at 5 nm intervals in the 290-350 nm region, by using cavity ring-down spectroscopy. Water vapor cross section values range from 2.94 × 10-24 to 2.13 × 10-25 cm2/molecule in the wavelength region studied. The effect of the water vapor absorption in the 290-350 nm region on the modeledradiation flux at the ground level has been evaluated using radiative transfer model.
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