Line-By-Line Radiative Transfer Model by Atmospheric and Environmental Research

TenStream - a 3D radiative transfer solver for earth system models

RTE+RRTMGP is a set of codes for computing radiative fluxes in planetary atmospheres. This fork uses neural networks for the gas optics computations and optimized code for the radiative transfer.

pyOSOAA is a python interface for the Ocean Successive Orders with Atmosphere - Advanced (OSOAA) radiative transfer.

RRTM for GCMs, LongWave domain

R package dedicated to the PROSAIL canopy reflectance model. The package allows running PROSAIL in direct and inverse modes, with various inversion strategies. A tutorial can be found on the gitlab website

RRTM for GCMs, ShortWave domain

Retrieves 3D cloud properties from multi-angle images of reflected solar radiation

Discrete Ordinates Solver for the (1D) Radiative Transfer Equation in a single or multi-layer plane-parallel atmosphere. Coded entirely in Python 3. Based on Stamnes' FORTRAN DISORT (see references in the Jupyter Notebook) and has its main features. This repository also includes our F2PY-wrapped Stamnes' DISORT (version 4.0.99).

Fast tool for 1D Non-LTE stellar parameter determination via Equivalent Width method

PyRTlib is an attractive educational software to simulate observations from ground-based, airborne, and satellite microwave sensors. It provides a flexible and user-friendly tool to broadly simulate how electromagnetic radiation travels through the atmosphere as it interacts with atmospheric constituents.

Leaf and canopy radiative transfer modeling tools built on PROSPECT-D and SAIL

DIRTY: 3D dust radiative transfer for dusty astrophysical sources

This python notebook reformats a series of Hydrolight-generated m-files (radiative transfer outputs) into hdf5 files. This enables easier access to data for investigators, who can work with structured variables inside the hdf5 files rather than unweildy ascii files, which are difficult to utilize on a large scale. See GitHub readme for more deta…

Re-configures data from Hydrolight m-files into MAT files using HDF5 based format.

This is a read-only mirror of https://gitlab.com/pytools4dart/pytools4dart.

Quantifying accuracy drawbacks across various 1d and 0d methods of modelling large-scale Earth systems and interpreting results through the lens of spectroscopy, radiative transfer and thermodynamics.

Atmospheric temperature profile generated by a highly simplified radiative transfer model. It calculates the temperature at a range of points (initially three) from the Earth's surface to the top of the atmosphere. The input parameters are the percentage of planetary cloud cover, the emissitivity/absorptivity of the two atmospheric layer

Quarto source code for my master's thesis "Remote Sensing of Foliar Nitrogen in Californian Almonds" (2023)