Reassessment of the volumes of sediment sources and sinks on Venus: Supporting Datasets

This repository contains the supporting materials associated with Ganey et al. (2023), published in Planetary Science Journal (https://doi.org/10.3847/PSJ/aca521) - it includes: <br> [visible_parabolas.shp] – Shapefiles (and auxiliary files) for the radar-dark visible parabolas identified in Campbell et al. (1992) [doi: 10.1029/92JE01634]. [modeled_parabolas.shp] – Shapefiles (and auxiliary files) for the parabolas modeled after Basilevsky et al. (2004) [doi: 10.1029/2004JE002307]. [sed_fields.shp] – Shapefiles (and auxiliary files) for the known aeolian feature fields (dunes, microdunes and yardangs). They were first identified in Greeley et al. (1992) [doi: 10.1029/92JE00980] and Weitz et al. (1994) [doi: 10.1006/icar.1994.1181]. [Sum_Thickness.tif] – Global impact-generated sediment thickness (4.6 km per pixel). [Sum_Volume.tif] – Global impact-generated sediment volume (4.6 km per pixel). [Craters.xlsx] – List of craters used for this study with visible and modeled parabolas.