Line-By-Line Radiative Transfer Model by Atmospheric and Environmental Research
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Updated
Dec 3, 2024 - Fortran
Line-By-Line Radiative Transfer Model by Atmospheric and Environmental Research
RTE+RRTMGP is a set of codes for computing radiative fluxes in planetary atmospheres.
(REOS) Radar and ElectroOptical Simulation Framework written in Fortran.
MCFOST radiative transfer code
A line-by-line longwave radiation code for planetary atmospheres.
TenStream - a 3D radiative transfer solver for earth system models
RRTM for GCMs, ShortWave domain
The 3D version of C2-Ray for multiple sources, hydrogen only
A Python library for spectral modelling and RADEX
RRTM for GCMs, LongWave domain
A line-by-line radiation code for planetary atmospheres. Now with shortwave radiative transfer.
C2-Ray radiative transfer / photo-ionziation code, version with helium, combining 1D and 3D
Binary Line File Generator by Atmospheric and Environmental Research
Cloud-J is multi-scattering eight-stream radiative transfer model for solar radiation based on Fast-J. It was originally developed by Michael J. Prather.
A base repository for light scattering calculations
A neutron transport mini-app with both diamond-difference and linear-discontinuous finite element spatial discretisation options
A dynamical model to simulate turbulence. Licensed under the MIT License.
a simplified model for line-by-line calculation of gas absorption, with absorption lines extracted from HiTRAN database.
Fortran engine to couple neural network based Mie emulator, called MieAI, with ICON-ART.
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