There are 4 repositories under radiative-transfer-models topic.
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.
Retrieves 3D cloud properties from multi-angle images of reflected solar radiation
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.
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 details.
Re-configures data from Hydrolight m-files into MAT files using HDF5 based format.
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.
This is a read-only mirror of https://gitlab.com/pytools4dart/pytools4dart.
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)
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.
A Python implementation of the delta-fit phase function truncation algorithm by Hu et al. 2000.
Numerical solver for system of PDEs modelling radiative transfer
Radiative transfer and synthetic radio imaging of ionised jets from young forming stars
Soil VIS-NIR reflectance spectra simulation based on generative model. PROSAIL model is integrated..
Using radiative transfer models to investigate indirect methods for measuring protostellar luminosity.