Data for Glacial isostatic adjustment reveals Mars' interior viscosity structure

<p>Present-day Martian interior models used in Broquet et al. (2024). All models use the following naming convention: Profile_NorthPole_Mars-TAYAK-dc-rho_south[-rho_north], where dc is the crustal thickness at the InSight landing site in km, rho_north and rho_south are the bulk density of the northern and southern hemisphere crust in g cm^-3. If added, XGRS provides the crustal heat producing element enrichment factor (X) with respect to the nominal Gamma Ray measured average of 49 pW kg^-1.&nbsp;</p> <p>Files with _60deg provide quantities averaged over the northern regions (&gt;60&deg;N) and _AVG give averages for the whole planet. Models with case numbers are from Plesa et al. (2018) [https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2018GL080728].&nbsp;</p> <p>Data Columns:<br>------------------------------<br>Column 1: Radius [m]<br>Column 2: Temperature [K]<br>Column 3: Viscosity [Pa s]<br>Column 4: Shear Velocity [m/s]<br>Column 5: Density [kg/m3]<br>Column 6: Shear Modulus [Pa]</p>