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

<p>Data accompanying&nbsp;the publication Steinke et al.&nbsp;2020 - &quot;Can a combination of convective and magmatic heat transport in the mantle explain Io&#39;s volcanic pattern?&quot;,&nbsp;JGR Planets.&nbsp;For more information see the README.&nbsp;Please contact Teresa Steinke with any questions.</p> <p>PART&nbsp;A</p> <p>Two sets including&nbsp;Io&#39;s volcanic features locations adopted from previous publications, fitted and filtered in order to be suitable for the comparision with Io&#39;s interior dynamics.</p> <p>PART B</p> <p>Solution spaces in three-dimensional parameter space spanned by the viscosity, the thickness and the heat flux fraction of Io&#39;s upper convective layer (Figure 3, 4, 5, and A1)</p> <p>&nbsp;</p>