A solar radiation model for use in climate studies

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Abstract

It includes the absorption and scattering due to ozone, water vapor, oxygen, carbon dioxide, clouds, and aerosols. Rayleigh scattering is also included. The UV and visible region (λ<0.69 μm) is grouped into four bands. An effective coefficeint for ozone absorption and an effective cross section for Rayleigh scattering are computed for each band. In the near-infrared region (λ>0.69 μm), the broadband parameterization is used to compute the absorption by water vapor in a clear atmosphere, and the k-distribution method is applied to compute fluxes in a scattering atmosphere. The reflectivity and transmissivity of a scattering layer are computed analytically using the delta-four-stream discrete-ordinate approximation. The two-stream adding method is then applied to compute fluxes for a composite of clear and scattering layers. Compared to the results of high spectral resolution and detailed multiple-scattering calculations, fluxes and heating rate are accurately computed to within a few percent. -from Author

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Ming-Dah Chou. (1992). A solar radiation model for use in climate studies. Journal of the Atmospheric Sciences, 49(9), 762–772. https://doi.org/10.1175/1520-0469(1992)049<0762:asrmfu>2.0.co;2

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