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Peking University
- Beijing, China
- https://danielkoll.github.io
Stars
Correlated-k radiative-transfer modelling package for exoplanet atmosphere GCMs.
2D spectral-core shallow-water exoplanet atmosphere model
This repository contains all of the code necessary to run simulations, save and load data, and make figures as in Teixeira et al. 2023, "The Carbon-Deficient Evolution of TRAPPIST-1c".
Code for stellar properties, rotation, and activity evolution
A Python package for helping to compute input arrays to DISORT.
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…
Scripts for computing analytical clearsky longwave spectral feedbacks (Koll, Jeevanjee, Lutsko 2023 JAS)
Fortran 2003 code to generate molecular spectra, partition functions, lifetimes, cooling functions etc using ExoMol line lists
Non-grey, picket fence, two-stream RT methods code collection package.
FMS-idealized moist GCM of O'Gorman and Schneider 2008 and dry GCM of Schneider and Walker 2006
On a 3D radiative transfer code for charaterize transiting planet
Exoplanet transit model with Monte Carlo light scattering.
Semi-grey, two stream RT code collection package.
3D Monte Carlo Radiative Transfer for exoplanet atmospheres using GPUs.
Julia implementation of MARGO, an idealized climate-economic modelling framework for Optimizing trade-offs between emissions Mitigation, Adaptation, carbon dioxide Removal, and solar Geoengineering.
RTE+RRTMGP is a set of codes for computing radiative fluxes in planetary atmospheres.
Python code for Planetary Atmosphere, Crust, and MANtle (PACMAN) geochemical evolution model applied to Venus, as described in Krissansen-Totton et al. (2021; Planetary Science Journal)
Scripts for transforming GCM output into a tidally locked coordinate system.
A line-by-line radiation code for planetary atmospheres. Now with shortwave radiative transfer.
A simple finite difference scheme for the Rayleigh-Bernard equations (buoyancy driven convection).
The Simple Dynamical Core Lab is a personal project to explore some numerical algorithms involved in primitive equations models of atmospheric dynamics in a simplified setting
ethankruse / exoplots
Forked from elisaquintana/exoplotsPresentation-ready, interactive plots of all known exoplanets — updated daily
Julia code for analytic and numeric solutions of the GIll Matsuno Circulation
Line-By-Line Radiative Transfer Model by Atmospheric and Environmental Research
Binary Line File Generator by Atmospheric and Environmental Research
Various tools used with the SOCRATES GCM radiation scheme package (https://code.metoffice.gov.uk/trac/socrates).