Supporting Information for "Evidence for a Locally Thinned Lithosphere Associated with Recent Volcanism at Aramaiti Corona, Venus"

e#_output_##.dat:

Data and modeled results containing the topographic profiles and axisymmetric flexure modeling corresponding to figures 3a, 4a, and 5a. Two files for each profile exist corresponding to E = 5, 65 GPa.
Columns are as follows:
-    profile #
-    distance from beginning of profile (m)
-    detrended stereo elevation (m)
-    best fit he (km)
-    modeled deflection outboard of load (m)
-    radial flexural stress (Pa)

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fig3b_profile5.dat:

Data corresponding to figure 3b, he vs RMS misfit for different combinations of r1 and r2 for profile 5. Columns are as follows:
-    he (km)
-    r1 (km)
-    r2 (km)
-    RMS misfit (m)

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fig_4b_all.dat:

Data corresponding to figure 4b, he vs RMS misfit for all profiles. Columns are as follows:
-    profile #
-    he (km)
-    RMS misfit (m)

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swath2_narina_clip.zip:

- clip of the stereo-derived topography used for flexural modeling in this study

- the zipfile contains a geotiff (geolocated tiff file for use in GIS software) and auxiliary files.

- References below. Full documentation of the processing applied is now available at the PDS https://pds-geosciences.wustl.edu/mgn/urn-nasa-pds-magellan_stereo_topography/document/magellan_stereo_topography_description.pdf

Herrick, R. R., Stahlke, D. L., & Sharpton, V. L. (2012). Fine‐scale Venusian topography from Magellan stereo data. Eos, Transactions American Geophysical Union, 93(12), 125-126. doi:10.1029/2012EO120002

Herrick, R. R. (2020). MGN RDRS Magellan Stereo-Derived Topography Mosaic (Derived Data). NASA Planetary Data System. doi:10.17189/1519332