Data accompanying the paper: Can a combination of convective and magmatic heat transport in the mantle explain Io's volcanic pattern?

Data accompanying the publication Steinke et al. 2020 - "Can a combination of convective and magmatic heat transport in the mantle explain Io's volcanic pattern?", JGR Planets. For more information see the README. Please contact Teresa Steinke with any questions.

PART A

Two sets including Io's volcanic features locations adopted from previous publications, fitted and filtered in order to be suitable for the comparision with Io's interior dynamics.

PART B

Solution spaces in three-dimensional parameter space spanned by the viscosity, the thickness and the heat flux fraction of Io's upper convective layer (Figure 3, 4, 5, and A1)