The materials uploaded here contain the shapefiles for: 1) the major units; and 2) the flow units used to create the two geomorphological maps in Elysium Planitia on Mars; as well as 3) the depth maps derived from SHARAD of the flow units. The "MajorUnits" and "FlowUnits" files include shapefile format readable in GIS. The major units were digitized at 1:100,000-scale and flow units at 1:80,000, both datasets were mapped based on CTX images (see methods section in Voigt et al. (2023)). The "Depth_maps" file include all SHARAD derived depth maps from Voigt et al. (2023) in a .txt file format.
For inquiries regarding the contents of this dataset, please contact the Corresponding Author listed in the README.txt file. Administrative inquiries (e.g., removal requests, trouble downloading, etc.) can be directed to data-management@arizona.edu
Funding
This work was supported by NASA’s FINESST program Grant number 80NSSC20K1373
DECIPHERING EFFUSIVE ERUPTION STYLES THROUGHOUT ELYSIUM PLANITIA, MARS: LINKING LAVA EMPLACEMENT DYNAMICS WITH MAGMATIC STORAGE CONDITIONS