MagIC is a high-performance code that solves the magneto-hydrodynamics equations in rotating spherical shells
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Updated
May 29, 2024 - Fortran
MagIC is a high-performance code that solves the magneto-hydrodynamics equations in rotating spherical shells
A 1D radiative-convective model for the atmospheres of hot terrestrial planets.
A simple Java library that computes ECAPE values and parcel paths.
A simple Python package that computes ECAPE values and parcel paths. Also includes irreversible adiabatic parcels, which are significantly different and more accurate than pseudoadiabatic parcels.
PAK-KTM (Program for Structural Analysis - Kojic Transport Model) is high-performance software for finite element analysis (FEA) of gradient-driven smeared physical fields, developed at the University of Kragujevac and the Research and Development Center for Bioengineering, BioIRC.
An OpenFOAM solver to model enhancement of mixed convection heat transfer due to electrohydrodynamic (EHD) flow.
Utility MATLAB scripts that I used when working on the braking system of the Formula Student race car from Squadra Corse Polito, in 2018, and when writing my MSc thesis, in 2019
Thermoregulated Airflow Cooling for Indoor Cycling
Project dedicated to borehole modilisation and command using Julia
Finite volume toolbox for Matlab/Octave
SOFTBALL: SOlidification, Flow, and Thermodynamics in Binary ALLoys. A code for simulating convection in mushy layers with Adaptive Mesh Refinement.
Turbulent convection in a vertical column of PPD
Python code for 1D Steady State Convection Diffusion
Prediction of convecition cell initialization 1 hr before
A Shallow Water model with convective parameterization built on top of Oceananigans.jl
To address some of the failure modes in training of physics informed neural networks, a Lagrangian architecture is designed to conform to the direction of travel of information in convection-diffusion equations, i.e., method of characteristic; The repository includes a pytorch implementation of PINN and proposed LPINN with periodic boundary cond…
Solves advection-diffusion equation for a low Prandt number medium
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
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