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dc.date.accessioned2024-03-02T16:43:41Z
dc.date.available2024-03-02T16:43:41Z
dc.date.created2023-07-10T08:50:25Z
dc.date.issued2023
dc.identifier.citationGallo, Leandro Cesar Domeier, Mathew Michael Sapienza, F. Swanson-Hysell, N. L. Vaes, B. Zhang, Y. Arnould, Maelis Rose Marie Eyster, A. Gürer, D. Kiraly, Agnes Robert, Boris Rolf, Tobias Shephard, Grace van der Boon, Annique . Embracing Uncertainty to Resolve Polar Wander: A Case Study of Cenozoic North America. Geophysical Research Letters. 2023, 50(11)
dc.identifier.urihttp://hdl.handle.net/10852/108926
dc.description.abstractAbstract Our understanding of Earth's paleogeography relies heavily on paleomagnetic apparent polar wander paths (APWPs), which represent the time‐dependent position of Earth's spin axis relative to a given block of lithosphere. However, conventional approaches to APWP construction have significant limitations. First, the paleomagnetic record contains substantial noise that is not integrated into APWPs. Second, parametric assumptions are adopted to represent spatial and temporal uncertainties even where the underlying data do not conform to the assumed distributions. The consequences of these limitations remain largely unknown. Here, we address these challenges with a bottom‐up Monte Carlo uncertainty propagation scheme that operates on site‐level paleomagnetic data. To demonstrate our methodology, we present an extensive compilation of site‐level Cenozoic paleomagnetic data from North America, which we use to generate a high‐resolution APWP. Our results demonstrate that even in the presence of substantial noise, polar wandering can be assessed with unprecedented temporal and spatial resolution.
dc.languageEN
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleEmbracing Uncertainty to Resolve Polar Wander: A Case Study of Cenozoic North America
dc.title.alternativeENEngelskEnglishEmbracing Uncertainty to Resolve Polar Wander: A Case Study of Cenozoic North America
dc.typeJournal article
dc.creator.authorGallo, Leandro Cesar
dc.creator.authorDomeier, Mathew Michael
dc.creator.authorSapienza, F.
dc.creator.authorSwanson-Hysell, N. L.
dc.creator.authorVaes, B.
dc.creator.authorZhang, Y.
dc.creator.authorArnould, Maelis Rose Marie
dc.creator.authorEyster, A.
dc.creator.authorGürer, D.
dc.creator.authorKiraly, Agnes
dc.creator.authorRobert, Boris
dc.creator.authorRolf, Tobias
dc.creator.authorShephard, Grace
dc.creator.authorvan der Boon, Annique
cristin.unitcode185,15,22,91
cristin.unitnameSenter for planetær beboelighet
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin2161591
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Geophysical Research Letters&rft.volume=50&rft.spage=&rft.date=2023
dc.identifier.jtitleGeophysical Research Letters
dc.identifier.volume50
dc.identifier.issue11
dc.identifier.pagecount12
dc.identifier.doihttps://doi.org/10.1029/2023GL103436
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0094-8276
dc.type.versionPublishedVersion
cristin.articleide2023GL103
dc.relation.projectEC/H2020/101025975
dc.relation.projectEC/HEU/101043844
dc.relation.projectNFR/326238
dc.relation.projectNFR/314742
dc.relation.projectNFR/323531
dc.relation.projectSIGMA2/NS9010k
dc.relation.projectNFR/276032
dc.relation.projectSIGMA2/NN9010k


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Attribution 4.0 International
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