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dc.date.accessioned2022-09-11T15:09:10Z
dc.date.available2022-09-11T15:09:10Z
dc.date.created2022-09-06T18:16:24Z
dc.date.issued2022
dc.identifier.citationGallo, Leandro Cesar Domeier, Mathew Michael sapienza, facundo . An optimization method for paleomagnetic Euler pole analysis. Computers & Geosciences. 2022
dc.identifier.urihttp://hdl.handle.net/10852/96560
dc.description.abstractOwing to the axial symmetry of the Earth’s magnetic field, paleomagnetic data only directly record the latitudinal and azimuthal positions of crustal blocks in the past, and paleolongitude cannot be constrained. An ability to overcome this obstacle is thus of fundamental importance to paleogeographic reconstruction. Paleomagnetic Euler pole (PEP) analysis presents a unique means to recover such information, but prior implementations of the PEP method have incorporated subjective decisions into its execution, undercutting its fidelity and rigor. Here we present an optimization approach to PEP analysis that addresses some of these deficiencies—namely the objective identification of change-points and small-circle arcs that together approximate an apparent polar wander path. We elaborate on our novel methodology and conduct some experiments with synthetic data to demonstrate its performance. We furthermore present implementations of our methods both as adaptable, stand-alone scripts in Python and as a streamlined interactive workflow that can be operated through a web browser.
dc.languageEN
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleAn optimization method for paleomagnetic Euler pole analysis
dc.title.alternativeENEngelskEnglishAn optimization method for paleomagnetic Euler pole analysis
dc.typeJournal article
dc.creator.authorGallo, Leandro Cesar
dc.creator.authorDomeier, Mathew Michael
dc.creator.authorsapienza, facundo
cristin.unitcode185,15,22,40
cristin.unitnameSenter for Jordens utvikling og dynamikk
cristin.ispublishedfalse
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin2049286
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Computers & Geosciences&rft.volume=&rft.spage=&rft.date=2022
dc.identifier.jtitleComputers & Geosciences
dc.identifier.volume166
dc.identifier.doihttps://doi.org/10.1016/j.cageo.2022.105150
dc.identifier.urnURN:NBN:no-99067
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0098-3004
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/96560/1/gallo-sapienza-domeier_2022_An%2Boptimization%2Bmethod%2Bfor%2Bpaleomagnetic%2BEuler%2Bpole%2Banalysis.pdf
dc.type.versionPublishedVersion
cristin.articleid105150


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