Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10165
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dc.contributor.authorallPavón-Carrasco, F. J.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallOsete, M. L.; Univ. Complutense Madrid (Spain)en
dc.contributor.authorallCampuzano, S. A.; Univ. Complutense Madrid (Spain)en
dc.contributor.authorallMcIntosh, G.; Canterbury Univ. (UK)en
dc.contributor.authorallMartín-Hernández, F.; Univ. Complutense Madrid (Spain)en
dc.contributor.editorallEppelbaum, L. V.; Telaviv Univ. (Israel)en
dc.date.accessioned2015-09-16T14:05:41Zen
dc.date.available2015-09-16T14:05:41Zen
dc.date.issued2015-09en
dc.identifier.isbn978-1-63483-129-1en
dc.identifier.urihttp://hdl.handle.net/2122/10165en
dc.description.abstractSince the pioneering studies in archeomagnetism in the second half of the 20th century, the number of archeomagnetic studies has increased exponentially. The huge density of archeomagnetic data collected during these years allows us to describe the past spatial and temporal evolution of the Earth’s magnetic field during the last millennia. Most of the data are located in the Northern Hemisphere, but currently, thanks to the strong effort of the paleomagnetic community, new collections of data are coming from the Southern Hemisphere, homogenizing the present database. Although the data distribution presents some epochs and locations where the data are still very scarce, they describe, to a greater or lesser degree of accuracy, the past behavior of the geomagnetic field. At regional scales, the use of archeomagnetic data permits the construction of paleosecular variation curves for the geomagnetic field elements: declination, inclination, and intensity. These curves describe the evolution of the elements at different times for the last millennia. During the last five years novel techniques, such as Bayesian statistics, bootstrap algorithms, or the Markov chain Monte Carlo method, have been applied to extract the most useful information from archeomagnetic data to build accurate and reliable curves. The accuracy of these curves can be exploited as a tool for archeomagnetic dating, assigning possible ages to archeological artifacts or volcanic lava flows with unknown age. At global scales, archeomagnetic data are jointly treated with other paleomagnetic data to generate continuous geomagnetic field models, reconstructing the past evolution of the geomagnetic field not only at the Earth’s surface, but also at the core-mantle boundary, shedding light on the past evolution of complex geodynamo processes.en
dc.language.isoEnglishen
dc.relation.ispartofNew Developments in Paleomagnetism Researchen
dc.relation.isversionofhttps://www.novapublishers.com/catalog/product_info.php?products_id=55345&osCsid=3234607ea9a1e9049b2124b9bb959746en
dc.subjectArcheomagnetismen
dc.subjectPaleomagnetismen
dc.titleRecent developments in Archeomagnetism: the story of the Earth's past magnetic fielden
dc.title.alternativeRecent developments in Archeomagnetismen
dc.typebook chapteren
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber99-158en
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.02. Geomagnetic field variations and reversalsen
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.03. Global and regional modelsen
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.05. Main geomagnetic fielden
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.06. Paleomagnetismen
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.07. Rock magnetismen
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.08. Instruments and techniquesen
dc.description.obiettivoSpecifico1A. Geomagnetismo e Paleomagnetismoen
dc.publisherNova Science Publishersen
dc.description.fulltextrestricteden
dc.contributor.authorPavón-Carrasco, F. J.en
dc.contributor.authorOsete, M. L.en
dc.contributor.authorCampuzano, S. A.en
dc.contributor.authorMcIntosh, G.en
dc.contributor.authorMartín-Hernández, F.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentUniv. Complutense Madrid (Spain)en
dc.contributor.departmentUniv. Complutense Madrid (Spain)en
dc.contributor.departmentCanterbury Univ. (UK)en
dc.contributor.departmentUniv. Complutense Madrid (Spain)en
dc.contributor.editorEppelbaum, L. V.en
dc.contributor.editordepartmentTelaviv Univ. (Israel)en
item.openairetypebook chapter-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptUniv. Complutense Madrid (Spain)-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptCanterbury Univ. (UK)-
crisitem.author.deptUniv. Complutense Madrid (Spain)-
crisitem.author.orcid0000-0001-7047-5704-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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