Building and testing using examples Example compiler flags RTE+RRTMGP documentation RTE+RRTMGP - Explanations Tutorials How-to guides Reference (technical documentation)Working with optical properties and spectral discretizations RTE - fluxes RTE - optical properties RTE - solvers

How-to guides

How to build and test

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.