Figure A1: Comparison to the model of Rafikov & Garmilla (2012).
Comparing the temperature dependence of sublimative mass flux in these models for both iron and olivine (or olivine species forsterite and fayalite). These models agree to within two orders of magnitude. For iron, these two models agree closely when the T0 parameter in the Rafikov and Gamilla (2012) model is changed to match the Steckloff et al. model.
