First thing would be to normalise the black line relative to the 'Zeng_2019/massradiusEarthlikeRocky.txt' at current radius. The water line should be normalised to, for example, 'Zeng_2019/massradius_100percentH2O_300K_1mbar.txt'. Optimally, the latter is tuned to the approx. T_eq of the planet.
Normalise mass-radius curves of the same radius of the planet at a particular time-step. Here are lots of M-R curves: https://drive.google.com/open?id=1M6MXZ0OscVtF713r86H3MoRRBj60IMUF&usp=drive_fs.
First thing would be to normalise the black line relative to the 'Zeng_2019/massradiusEarthlikeRocky.txt' at current radius. The water line should be normalised to, for example, 'Zeng_2019/massradius_100percentH2O_300K_1mbar.txt'. Optimally, the latter is tuned to the approx. T_eq of the planet.
_Originally posted by @timlichtenberg in https://github.com/FormingWorlds/PROTEUS/pull/214#discussion_r1807307834_