RTE-RRTMGP
ExplanationsHow-to guidesConventions, technical documentationTutorials

How-to guides

  • Installation from conda-forge
  • How to build and test
  • Migrating from RRTMG

RTE-RRTMGP

  • RTE-RRTMGP
  • rrtmgp@aer.com
  • earth-system-radiation

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.