Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9196
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dc.contributor.authorallSpada, G.; Dip.to di Scienze di Base e Fondamenti, Università di Urbino, Urbino, Italyen
dc.contributor.authorallGalassi, G.; Dipartimento di Scienze di Base e Fondamenti, Urbino University “Carlo Bo”en
dc.contributor.authorallOlivieri, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italiaen
dc.date.accessioned2014-12-29T15:10:33Zen
dc.date.available2014-12-29T15:10:33Zen
dc.date.issued2015en
dc.identifier.urihttp://hdl.handle.net/2122/9196en
dc.description.abstractWe use the Empirical Mode Decomposition (EMD) method to study the decadal variations in polar motion and its long-term trend since year 1900. The existence of the so-called “Markowitz wobble”, a multidecadal fluctuation of the mean pole of rotation whose nature has long been debated since its discovery in 1960, is confirmed. In the EMD approach, the Markowitz wobble naturally arises as an empirical oscillatory term in polar motion, showing significant amplitude variations and a period of approximately 3 decades. The path of the time-averaged, non-cyclic component of polar motion matches the results of previous investigations based on classical spectral methods. However, our analysis also reveals previously unnoticed steep variations (change points) in the rate and the direction of secular polar motion.en
dc.language.isoEnglishen
dc.publisher.namePlenum Pressen
dc.relation.ispartofStudia Geophysica et Geodaeticaen
dc.relation.ispartofseries/59(2015)en
dc.subjectsecular polar motionen
dc.subjectmarkowitz wobbleen
dc.titleEmpirical mode decomposition of long-term polar motion observationen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber200–211en
dc.identifier.URLhttp://www.bo.ingv.it/~olivieri/publications/Empirical_Polar_Motion_Spada_Galassi_Olivieri.pdfen
dc.subject.INGV04. Solid Earth::04.03. Geodesy::04.03.02. Earth rotationen
dc.identifier.doi10.1007/s11200-014-1151-4en
dc.description.obiettivoSpecifico1T. Geodinamica e interno della Terraen
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.relation.issn0039-3169en
dc.relation.eissn1573-1626en
dc.contributor.authorSpada, G.en
dc.contributor.authorGalassi, G.en
dc.contributor.authorOlivieri, M.en
dc.contributor.departmentDip.to di Scienze di Base e Fondamenti, Università di Urbino, Urbino, Italyen
dc.contributor.departmentDipartimento di Scienze di Base e Fondamenti, Urbino University “Carlo Bo”en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextreserved-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptInsitute of Physics, University of Urbino, Italy-
crisitem.author.deptDipartimento di Scienze di Base e Fondamenti, Urbino University “Carlo Bo”-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Bologna, Bologna, Italia-
crisitem.author.orcid0000-0002-7333-8809-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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