21 results for “topic:atmosphere-model”
A Collection of Awesome Large Weather Models (LWMs) | AI for Earth (AI4Earth) | AI for Science (AI4Science)
Fork of E3SM used to develop exascale global atmosphere model written in C++ (aka SCREAM)
Implementation of an atmospheric scattering example found on ShaderToy, ported to URP and made to work with baked optical depth. Inspired by Sebastian Lague's series on Atmospheric Rendering
Radio-Frequency Engineering Modeling Toolkit (RF-EMT)
Python interface to the NRLMSIS codes for calculating atmospheric densities and constituents at satellite altitudes
TenStream - a 3D radiative transfer solver for earth system models
An open-source model for extreme atmospheres on rocky exoplanets.
Function to calculate GOST R 25645.166-2004 upper atmosphere model
Unofficial Mirror of NRLMSIS2.1 https://map.nrl.navy.mil/map/pub/nrl/NRLMSIS/NRLMSIS2.1/
U.S. Standard Atmosphere 1976
1976 Standard Atmosphere in Modern Fortran
Replication of Seager et al. (2019) Nat. Clim. Chan. They used a simple-as-possible coupled model to explain the bias in the nino3.4 trend in climate models (CMIP5). This repository replicates/reproduces their work, shows that it also applies to CMIP6, and varies some of the parameters.
Two-dimensional spatial filters, developed for application to ocean & atmosphere model output and gridded observations
An introductory course for earth scientists interested in learning ml/ai application and approaches with geophysical data
This is the code used in the can-sized satellite for team Idealite in the Canadian Satellite Design Challenge (CSDC).
A C++ port of Max Bernard's C# solution for calculating temperature, pressure and air density at a given altitude, according to the ISA.
Unofficial mirror of Horizontal Wind Model 2014
Modeling and analysis of the eclipsing binary star system KIC 2306740 using PHOEBE software
ACCESS Models Accessory Multitool Interface (AMAMI) is a Python package that bundles a set of commands to handle ACCESS models input and output files.
um-modify is a standalone Python module to modify the data of a UM file
Simulate the distribution and intensity of photon on the surface of a planet.