
RTE+RRTMGP is a set of codes for computing radiative fluxes in planetary atmospheres. RRTMGP uses a k-distribution to provide an optical description (absorption and possibly Rayleigh optical depth) of the gaseous atmosphere, along with the relevant source functions, on a pre-determined spectral grid given temperatures, pressures, and gas concentration. RTE computes fluxes given spectrally-resolved optical descriptions and source functions. The fluxes are normally summarized or reduced via a user extensible class.
If you use this software, please cite it using these metadata.
research, radiative transfer, RTE+RRTMGP, atmospheric radiation, climate model
research, radiative transfer, RTE+RRTMGP, atmospheric radiation, climate model
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