Fortran engine to couple neural network based Mie emulator, called MieAI, with ICON-ART.
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Updated
Dec 14, 2023 - Fortran
Fortran engine to couple neural network based Mie emulator, called MieAI, with ICON-ART.
Radiative transfer and synthetic radio imaging of ionised jets from young forming stars
Analytic 1-D radiative transfer model of blue-asymmetric spectral line profiles from infalling molecular clouds. The model is presented in the paper, "Molecular Line Profile Fitting with Analytic Radiative Transfer Models" by De Vries & Myers (2005).
High-performance Julia re-implementation of RADEX
Computes spectral energy distributions from radiatively inefficient accretion flows around black holes. GPU-accelerated, CUDA (alpha, unstable)
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.
Find systems using 4-pixels connectivity in 3d data cube from a radiative transfer simulation
Compressed representations of opacity for radiative transfer!
This repository includes the training and testing of the Neural Network model proposed in the article titled "Quantification of Shortwave Surface Albedo Feedback using a Neural Network Approach".
My IDL libraries covering various topics related to spectroscopy, radiative transfer, theory of stellar atmospheres and numerical methods in general.
MOCASSIN - MOnte CArlo SimulationS of Ionized Nebulae on Voronoi Meshes
MOCASSIN - MOnte CArlo SimulationS of Ionized Nebulae, Version 2.0
Compute linear polarization of the radiation emitted from the molecular cloud in magnetic field using LVG approximation.
Reference solar irradiance spectrum datasets manager
fluorescence ultrasound modulated optical tomography with radiative transport equation.
Obtaining sky brightness temperatures for stratocumulus clouds based on soundings at NKX
Process maps of artificial night sky radiance with .kmz extension
C2-Ray radiative transfer / photo-ionziation code, version with helium, combining 1D and 3D
MOCASSIN - MOnte CArlo SimulationS of Ionized Nebulae, Version 3.0
Train and use neural networks to quickly approximate polarized synchrotron radiative transfer coefficients
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