Project Overview
This project analysed the temperature profile across spacecraft heat shield tiles using Finite Differencing Methods (FDM). The objective was to determine optimal tile thickness, assess stability and accuracy of numerical methods, and model realistic damage scenarios. Enhancements included automated plot scanning and a graphical user interface to improve usability and data extraction.
Tools & Technologies
Project Details
Implemented 1D thermal models of spacecraft heat shield tiles to analyse temperature distribution across tile thickness during re-entry.
Compared Forward, Backward, Du Fort-Frankel, and Crank-Nicolson methods for stability and accuracy; Crank-Nicolson proved most accurate and stable across selected timesteps and spatial steps.
Determined optimal tile thickness of 54.7 mm using the shooting method to ensure aluminium skin temperatures remained below 180°C, balancing weight and safety.
Extended modelling to 2D scenarios simulating damaged and missing tiles to evaluate heat penetration and structural risk during re-entry.
Developed a GUI for automated plot scanning of NASA thermocouple data to extract time-temperature points efficiently, reducing human error.