{"@attributes":{"xmlns:xsi":"http:\/\/www.w3.org\/2001\/XMLSchema-instance","xmlns":"http:\/\/datacite.org\/schema\/kernel-4","xsi:schemaLocation":"http:\/\/datacite.org\/schema\/kernel-4 http:\/\/schema.datacite.org\/meta\/kernel-4\/metadata.xsd"},"identifier":"10.24396\/ORDAR-170","creators":{"creator":[{"creatorName":"F\u00e9nisse Gabriel"},{"creatorName":"Bekaert David Vincent"},{"creatorName":"Blard Pierre-Henri","nameIdentifier":"0000-0002-8455-8014"},{"creatorName":"Duprat Jean"},{"creatorName":"Mattia Isabelle"},{"creatorName":"Genge Matthew"},{"creatorName":"Suttle Martin"},{"creatorName":"Barres Odile"},{"creatorName":"Engrand C\u00e9cile"},{"creatorName":"Marroccchi Yves"}]},"titles":{"title":"Supplementary material: data availability compiling the database and our analytical results"},"publisher":"OTELO","publicationYear":"2025-02-11","subjects":{"subject":"Geology"},"resourceType":"Dataset","language":"ENGLISH","version":"1","descriptions":{"description":"Files used in this study:\r\n\r\n(i) \"IDP_Neve_Concordia_CRPG_MNHN_GF\u00e9nisseEtAl_EPSL.xlsx\", a snow mass compilation from clean snow at the CONCORDIA station (Dome C, Antarctica);\r\n(ii) \"Calibration_of_He_concentration_inFurnace_GF\u00e9nisseEtAl_EPSL.xlsx\", the furnace calibration for He measurements;\r\n(iii) \"HeResults_IDPsMMs_GF\u00e9nisseEtAl_EPSL.xlsx\", the He isotopic compositions and total masses of cosmic dust, categorized by size range, from the CONCORDIA snow;\r\n(iv) \"ETMassFluxSynthesis_GF\u00e9nisseEtAl_EPSL.xlsx\", ET mass comparisons from collection, He method and CABMOD-ZoDy modeling.\r\n(v) \"Database_IDPs&MMs_He&Ne_GF\u00e9nisseEtAl_EPSL.xlsx\", an exhaustive database containing all published light noble gas data (\u00b3He, \u2074He, and \u00b2\u2070Ne) measured in IDPs and MMs collected in the stratosphere and Antarctica;\r\n(vi) \"ReferencesTable_3HeETFlux_GF\u00e9nisseEtAl_EPSL.xlsx\", a database of light noble gas measurements in Antarctica MMs. This dataset of He vs. MM mass is used here to convert \u00b3He concentrations into dust abundances."}}