000000094 001__ 94 000000094 005__ 20230824003255.0 000000094 0247_ $$a10.7936/77ps-1s85$$2DOI 000000094 037__ $$aRDM 000000094 041__ $$aeng 000000094 245__ $$aA Global Catalog of Volcanoes and Shield Fields on Venus [Version 1] 000000094 251__ $$a1 000000094 269__ $$a2022-03-29 000000094 270__ $$mh.rebeccahahn@wustl.edu$$pHahn, Rebecca M 000000094 300__ $$a5223 KB 000000094 336__ $$aDataset 000000094 518__ $$d2019-08-15/2020-08-15$$oCollected 000000094 520__ $$aVenus is home to thousands of volcanic landforms that range in size from less than 5 km in diameter to well over 100 km in diameter, and their extrusive materials comprise ~80% of the surface. With the NASA Magellan SAR (synthetic aperture radar) FMAP (full-resolution radar map) left- and right-look global mosaics at 75 meter-per-pixel (m/px) resolution, we created a global catalog of volcanic edifices on Venus that contains ~85,000 features, ~99% of which are volcanoesAdditionally, we developed an automated approach to grouping volcanoes into "shield fields": areas with relatively high spatial concentrations of shield- or dome-like volcanic edifices that are ≤20 km in diameter. This global dataset can be used as a tool to investigate the morphological, spatial, and temporal properties of volcanoes on Venus. 000000094 540__ $$aCreative Commons Attribution (CC BY) 4.0 International$$uhttps://creativecommons.org/licenses/by/4.0/ 000000094 650__ $$aPhysical sciences 000000094 6531_ $$aVolcano 000000094 6531_ $$aVenus 000000094 6531_ $$aGIS 000000094 6531_ $$aShield Fields 000000094 655__ $$aTabular 000000094 7001_ $$aHahn, Rebecca M$$1https://orcid.org/0000-0002-4425-434X$$uWashington University in St. Louis$$4https://ror.org/01yc7t268$$5ROR 000000094 7001_ $$aByrne, Paul K$$1https://orcid.org/0000-0002-5644-7069$$uWashington University in St. Louis$$4https://ror.org/01yc7t268$$5ROR 000000094 791__ $$tHahn, Rebecca M. and Byrne, Paul K., "A Global Catalog of Volcanoes and Shield Fields on Venus." [Dataset Version 2]. Washington University in St. Louis (2022). $$aDataset$$eIsPreviousVersionOf$$whttps://doi.org/10.7936/8xy0-x885$$2DOI 000000094 8564_ $$99d3e5089-d8d2-4aa5-b3ef-688b2fbe8764$$s5334366$$uhttps://data.library.wustl.edu/record/94/files/doi10793677ps1s85_hahn_dip.zip$$ePublic$$24be4d4f6c0d1451eb9b3ade2a3f17e6d$$01 000000094 8564_ $$9ccb3ff3d-e616-44e1-b73f-80eeb331e03a$$s27799$$uhttps://data.library.wustl.edu/record/94/files/doi10793677ps1s85_hahn_readme.txt$$yReadme file$$ePublic$$2385d4e82b865f8b5b87a3b3af31ba3c5$$02 000000094 904__ $$apaul.byrne@wustl.edu 000000094 909CO $$ooai:data.library.wustl.edu:94$$pdataset 000000094 974__ $$aVenus 000000094 980__ $$aWashU Researcher Data