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Geodynamically corrected Pliocene shoreline elevations in Australia consistent with midrange projections of Antarctic ice loss

dc.contributor.authorRichards, Fred D
dc.contributor.authorCoulson, Sophie
dc.contributor.authorHoggard, Mark
dc.contributor.authorAustermann, J
dc.contributor.authorDyer, Blake
dc.contributor.authorMitrovica, Jerry X.
dc.date.accessioned2024-08-15T02:21:42Z
dc.date.available2024-08-15T02:21:42Z
dc.date.issued2023
dc.date.updated2024-05-12T08:15:49Z
dc.description.abstractThe Mid-Pliocene represents the most recent interval in Earth history with climatic conditions similar to those expected in the coming decades. Mid-Pliocene sea level estimates therefore provide important constraints on projections of future ice sheet behavior and sea level change but differ by tens of meters due to local distortion of paleoshorelines caused by mantle dynamics. We combine an Australian sea level marker compilation with geodynamic simulations and probabilistic inversions to quantify and remove these post-Pliocene vertical motions at continental scale. Dynamic topography accounts for most of the observed sea level marker deflection, and correcting for this effect and glacial isostatic adjustment yields a Mid-Pliocene global mean sea level of +16.0 (+10.4 to +21.5) m (50th/16th to 84th percentiles). Recalibration of recent high-end sea level projections using this revised estimate implies a more stable Antarctic Ice Sheet under future warming scenarios, consistent with midrange forecasts of sea level rise that do not incorporate a marine ice cliff instability.
dc.description.sponsorshipF.D.R. acknowledges support from the Schmidt Science Fellows program, in partnership with the Rhodes Trust, and the Imperial College Research Fellowship Scheme. S.L.C. is supported by a Los Alamos National Laboratory Director’s Postdoctoral Fellowship. M.J.H. acknowledges support from Geoscience Australia and the Australian Research Council’s Discovery Early Career Researcher Award DE220101519. J.A. acknowledges support from the Vetlesen Foundation. Wethank the Computational Infrastructure for Geodynamics (geodynamics.org), which is fundedby the NSF under award EAR-0949446 and EAR-1550901 for supporting the development of ASPECT and the Imperial College Research Computing Service (https://doi.org/10.14469/hpc/2232) for providing computational resources
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn2375-2548
dc.identifier.urihttps://hdl.handle.net/1885/733714643
dc.language.isoen_AUen_AU
dc.provenanceDistributedunder a CreativeCommons AttributionLicense 4.0 (CC BY)
dc.publisherAmerican Association for the Advancement of Science
dc.relationhttp://purl.org/au-research/grants/arc/DE220101519
dc.rightsCopyright © 2023 The Authors, some rights reserved;exclusive licenseeAmerican Association for the Advancementof Science. No claim tooriginal U.S. Government Works.
dc.rights.licenseCreative Commons Attribution License
dc.rights.urihttp://creativecommons.org/licenses/by/4.0
dc.sourceScience Advances
dc.titleGeodynamically corrected Pliocene shoreline elevations in Australia consistent with midrange projections of Antarctic ice loss
dc.typeJournal article
dcterms.accessRightsOpen Access
local.bibliographicCitation.issue46
local.bibliographicCitation.lastpage14
local.bibliographicCitation.startpage1
local.contributor.affiliationRichards, Fred D, Imperial College London
local.contributor.affiliationCoulson, Sophie, Los Alamos National Laboratory
local.contributor.affiliationHoggard, Mark, College of Science, ANU
local.contributor.affiliationAustermann, J, Columbia University
local.contributor.affiliationDyer, Blake, University of Victoria
local.contributor.affiliationMitrovica, Jerry X., Harvard University
local.contributor.authoruidHoggard, Mark, u1093374
local.description.notesImported from ARIES
local.identifier.absfor370609 - Seismology and seismic exploration
local.identifier.absfor370604 - Geodynamics
local.identifier.absfor370603 - Geodesy
local.identifier.ariespublicationa383154xPUB45352
local.identifier.citationvolume9
local.identifier.doi10.1126/sciadv.adg3035
local.identifier.scopusID2-s2.0-85177432422
local.publisher.urlhttps://www.science.org/doi/10.1126/sciadv.adg3035
local.type.statusPublished Version
publicationvolume.volumeNumber9

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