Published July 8, 2017 | Version v1
Software Open

Source Code for Simulation of the Origin of Mantle Volatiles

  • 1. Royal Holloway University of London
  • 2. University of Minnesota, Twin Cities



This README would normally document whatever steps are necessary to get your application up and running. Please note that there won't be any additional support available for running these codes. They are provided as-is.

What is this repository for?

  • This repository contains scilab files and data for a numerical modelof magma ocean crystallization

How do I get set up?

  • To run the simulations, you will need scilab installed in your computer. The file hmh.sce is the central file for creating data. It's major dependency is on module.sce.
  • To generate figures, run post_process_MO.sce
  • In the data folder, there will be three series folders (corresponding to the three different H:C ratios). Within each folder there are ten different folders mass 1- 10, which have different starting masses for the volatiles. You need to create this directory tree prior to running scilab
  • Within each massX folder the data is in .dat files. Each row contains iterations in time. The column contents are given by file name. See the main code for definition of contents.


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