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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
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.
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…
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.
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.
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
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.