Eccentricity curve estimation from geological data using sinusoidal modeling

dc.contributor.authorZivanovic, Miroslav
dc.contributor.authorSinnesael, Matthias
dc.contributor.departmentIngeniería Eléctrica, Electrónica y de Comunicación
dc.contributor.departmentIngeniaritza Elektrikoa, Elektronikoa eta Telekomunikazio Ingeniaritza
dc.date.accessioned2025-02-19T09:03:50Z
dc.date.issued2025-01-16
dc.date.updated2025-02-19T08:56:22Z
dc.description.abstractThe estimation of eccentricity curves from geological data is important as it can be used as a basis for the construction of geological timescales, or making inferences of past orbital evolutions of the Solar System. Such estimation can be challenging for multiple reasons like age-depth distortions, non-linear responses to insolation and various other sources of perturbation. We present a novel approach to estimating the eccentricity waveform from geological time series by targeted modifications to the Astronomical Component Estimation model (ACEv.1). We show that analyzing individual precession components is highly beneficial in understanding the impact of perturbation on the estimator. It turns out that individual precession components are fairly stationary in noise-free environments. Although the presence of perturbation modifies the morphology of the corresponding waveforms, the root-mean-square of individual waveforms remains approximately unchanged. This finding allows for a simple adjustment of individual precession components, that renders them almost noise-free. Such an approach provides a high-fidelity precession waveform, from which we can estimate the eccentricity. Furthermore, we provide a benchmark study on both synthetic and real geological data, which assess the performance of the proposed method against three state-of-the-art methods from the literature. The modified ACEv.1 model - here named ACEv.2 - outperforms the reference methods in terms of goodness-of-fit to the known eccentricity solutions in the case of a known age-depth model and precession frequencies. Cyclostratigraphic studies often lack comparisons to other methods; therefore, we believe this study could enhance users' understanding of how the reference methods handle perturbations in geological signals.en
dc.description.sponsorshipWe thank Thomas Westerhold for constructive input on the ODP926 record. MS thanks the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (Advanced Grant AstroGeo-885250 awarded to Jacques Laskar) for financial support. This work was made possible thanks to the support of CycloNet (Research Foundation Flanders (FWO); Grant W000522N).
dc.embargo.lift2027-01-16
dc.embargo.terms2027-01-16
dc.format.mimetypeapplication/pdfen
dc.identifier.citationZivanovic, M., Sinnesael, M. (2025) Eccentricity curve estimation from geological data using sinusoidal modeling. Computers and Geosciences, 196, 1-16. https://doi.org/10.1016/j.cageo.2025.105866
dc.identifier.doi10.1016/j.cageo.2025.105866
dc.identifier.issn0098-3004
dc.identifier.urihttps://academica-e.unavarra.es/handle/2454/53470
dc.language.isoeng
dc.publisherElsevier
dc.relation.ispartofComputers and Geosciences, 196, 1-16
dc.relation.projectIDinfo:eu-repo/grantAgreement/European Commission/Horizon 2020 Framework Programme/885250/
dc.relation.publisherversionhttps://doi.org/10.1016/j.cageo.2025.105866
dc.rights© 2025 Elsevier Ltd. This manuscript version is made available under the CC-BY-NC-ND 4.0
dc.rights.accessRightsinfo:eu-repo/semantics/embargoedAccess
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/
dc.subjectBenchmark studyen
dc.subjectEccentricity estimateen
dc.subjectModel uncertaintyen
dc.subjectNarrow-band noiseen
dc.subjectNon-stationary sinusoidal modelingen
dc.titleEccentricity curve estimation from geological data using sinusoidal modelingen
dc.typeinfo:eu-repo/semantics/article
dc.type.versioninfo:eu-repo/semantics/acceptedVersion
dspace.entity.typePublication
relation.isAuthorOfPublicationdc2b0e94-3db8-470e-8912-58ae1b092ba7
relation.isAuthorOfPublication.latestForDiscoverydc2b0e94-3db8-470e-8912-58ae1b092ba7

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