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.
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
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.
Quarto source code for my master's thesis "Remote Sensing of Foliar Nitrogen in Californian Almonds" (2023)
This is a read-only mirror of https://gitlab.com/pytools4dart/pytools4dart.
Line-By-Line Radiative Transfer Model by Atmospheric and Environmental Research
DIRTY: 3D dust radiative transfer for dusty astrophysical sources
TenStream - a 3D radiative transfer solver for earth system models
Retrieves 3D cloud properties from multi-angle images of reflected solar radiation
Numerical solver for system of PDEs modelling radiative transfer
pyOSOAA is a python interface for the Ocean Successive Orders with Atmosphere - Advanced (OSOAA) radiative transfer.
Soil VIS-NIR reflectance spectra simulation based on generative model. PROSAIL model is integrated..
Leaf and canopy radiative transfer modeling tools built on PROSPECT-D and SAIL
A Python-backend for radiative transfer model inversion for crop trait retrieval
Radiative transfer and synthetic radio imaging of ionised jets from young forming stars
Computational framework for solving the radiative transfer equation in one spatial dimension using a Godunov-type finite volume method with piecewise linear reconstruction of the solution within each cell of the computational domain.
Using radiative transfer models to investigate indirect methods for measuring protostellar luminosity.
Fast tool for 1D Non-LTE stellar parameter determination via Equivalent Width method
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.
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
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