Joe Renaud
Joe Renaud
Kamata et al. (2015) has the two starting solutions for `RadialSolver` k^2 +/- (see their Eq. B13) implying that solution 1 uses the + version and solution 2 uses the...
The recrusision formula shown in TS72 and KMN15 (See TS72 Eq. 97) does not reproduce the full version of this function (TS72 Eq. 96). I am finding it to be...
An earlier version of TidalPy used the full definition of Takeuchi & Saito (1972)'s starting conditions in the radial function. However, testing revealed that there were issues matching the limiting...
Add a function to quickly build common systems (instantiate and return the orbit class for each system): - [ ] Jovian system - [ ] Earth-Moon system - [ ]...
Please read the style.md before making new doc strings. _Docstrings should be concise_ **Sub-Packages** - [ ] burnman_interface - [ ] cooling - [ ] dynamics - [ ] integration...
The beginnings of this were implemented in version 0.2.1, but the sphinx documentation is sparse compared to the older markdown files. - [ ] Rewrite old markdown files into new...
Ctrl-f "TODO" and "OPT" throughout the project and make a new issue for each item. It is okay if you don't know what exactly to put (labels, comments, etc.). Just...
Currently, to change a configuration on a planet you need to A). know a potentially complex series of configuration keys and B). make a separate call to the planet's reinit()....
This will be easy to do for silicates (see the equations 21 and 22 in Shoji & Kurita 2014). Run these equations at layer initialization (TidalPy does not allow for...
Currently, the base temperature of a layer is equal to its average temperature (layer.temperature_lower = layer.temperature). In reality, this temperature will be higher. Generally, this is found via an assumed...