A simulation of convection within the solar convection zone. The code is written in IDL and is dependent on the SSW IDL code repository.
This repository contains a directory of IDL code attempting to perform the simulation, and is incomplete.
The Python directory contains code written by Sean Blake and used for his 4th year Physics/Astro project at TCD. -See the README.md file in the ./python directory.
For the static solar model used in the code, see the README.md in the ./solar_model directory.