ktrinh20
PhD Candidate || Icy moons | Computer models | Geodynamics | Geochemistry
Arizona State UniversityTempe, AZ
Pinned Repositories
ktrinh20.github.io
Kevin's personal academic profile.
MeteoriteCompositions
I will use this repository to store scripts used to handle meteorite compositions. Feel free to let me know if you want to contribute and share ownership of this repository!
MoonInteriorStructure
Codes that I use to model the interior structure of moons. Though, these codes should apply to any small icy body (e.g., Pluto). Models are constrained by mass, radius, and normalized moment of inertia (MoI).
numerical-methods-demos
I wrote code to demonstrate various numerical methods.
ThermalEvolution1D
This code (ThermalEvolution1D.cpp) models the thermal evolution of small planetary bodies, particularly icy moons. I solve the 1-D heat diffusion equation assuming only conduction. Heat sources include short- and long-lived radioactive isotopes and tidal heating. Heat sinks include silicate dehydration.
ktrinh20's Repositories
ktrinh20/ktrinh20.github.io
Kevin's personal academic profile.
ktrinh20/MeteoriteCompositions
I will use this repository to store scripts used to handle meteorite compositions. Feel free to let me know if you want to contribute and share ownership of this repository!
ktrinh20/MoonInteriorStructure
Codes that I use to model the interior structure of moons. Though, these codes should apply to any small icy body (e.g., Pluto). Models are constrained by mass, radius, and normalized moment of inertia (MoI).
ktrinh20/numerical-methods-demos
I wrote code to demonstrate various numerical methods.
ktrinh20/ThermalEvolution1D
This code (ThermalEvolution1D.cpp) models the thermal evolution of small planetary bodies, particularly icy moons. I solve the 1-D heat diffusion equation assuming only conduction. Heat sources include short- and long-lived radioactive isotopes and tidal heating. Heat sinks include silicate dehydration.