Skip to content

Releases: vancesteven/PlanetProfile

Icy moon models across the solar system in Python

30 Jun 04:20
Compare
Choose a tag to compare

All of the major icy moons in the solar system now have default models in the Python version, as does Pluto.

Plotting extras now in Python version

20 Jun 02:31
Compare
Choose a tag to compare

The Python version now includes additional features copied over from the Matlab, including marking the models studied by Vance et al. (2021) on inductograms and plotting Fourier spectra of magnetic oscillations.

Complete plots in Python version

13 Jun 11:20
Compare
Choose a tag to compare

The Python version now contains all the major plotting functions available in the Matlab.

Python version

30 May 21:37
Compare
Choose a tag to compare

PlanetProfile now has a Python version. See the README for recommendations and instructions on running the software. Not all Matlab functionality is included yet--notably, a few types of plots and most PPBody files have not yet been created for the Python version.

For a description of capabilities and goals, see: https://doi.org/10.1002/essoar.10511365.1

Supplementary Data: Effects of Methane Clathrate Lids on Titan's Ice Shell and added TauP functionality

02 Mar 17:16
Compare
Choose a tag to compare

This release includes an update that allows users to model 10-20 km clathrate lids on a 100 km ice shell for Titan. It also allows users to generate TauP models and plot travel time curves.

Supplementary Data: Magnetic Induction Responses of Jupiter's Ocean Moons Including Effects from Adiabatic Convection

27 Sep 06:22
Compare
Choose a tag to compare

Computes the complex magnetic induction responses for spherically symmetric models of Europa, Ganymede, and Callisto. Generates most of the figures and tables from Vance et al. (under review).

v1.1.1 contains minor bug fixes from the 1.1.0 version.

Supplementary Data: Geophysical Investigations of Habitability in Icy Ocean Worlds

16 Aug 22:52
Compare
Choose a tag to compare

Models interiors of icy ocean worlds based on geophysical constraints. Considers seawater, water, MgSO4 (aq) and NH3 (aq) oceans; ices I, II, III, V, VI; rock mineralogies of chondrite and pyrite; metallic cores of gamma-iron and FeS rich iron including melts. Includes applications to Europa, Ganymede, Callisto, Enceladus, Titan.