Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9472
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dc.contributor.authorallOsete, M. L.; Facultad de Ciencias Físicas, Universidad Complutense de Madrid, Avda Complutense s/n, 28040 Madrid, Spainen
dc.contributor.authorallCatanzariti, G.; Facultad de Ciencias Físicas, Universidad Complutense de Madrid, Avda Complutense s/n, 28040 Madrid, Spainen
dc.contributor.authorallChauvin, A.; Géosciences-Rennes, CNRS, UMR 6118, Université de Rennes 1, Campus de Beaulieu, 35042 Rennes, Cedex, Franceen
dc.contributor.authorallPavón-Carrasco, F. J.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallRoperch, P.; Géosciences-Rennes, CNRS, UMR 6118, Université de Rennes 1, Campus de Beaulieu, 35042 Rennes, Cedex, Franceen
dc.contributor.authorallFernández, V. M.; Departamento de Prehistoria, Universidad Complutense de Madrid, 28040 Madrid. Spainen
dc.date.accessioned2015-04-03T08:53:18Zen
dc.date.available2015-04-03T08:53:18Zen
dc.date.issued2015-03-11en
dc.identifier.urihttp://hdl.handle.net/2122/9472en
dc.description.abstractFirst archaeointensity determinations have been obtained from Ethiopia. Seven bricks (34 specimens) from the Däbsan archaeological remains were subjected to archaeointensity determination by means of classical Thellier–Thellier experiment including tests for magnetic anisotropy and magnetic cooling rate dependency. The age of the Däbsan Palace is well controlled by historical information: between 1603, when land grants were conceded to the Jesuits and the Catholicism was established as the official religion in Ethiopia, and the age of the Palace foundation in 1626–27. Successful archaeointensity determinations were obtained in 27 specimens from five individual bricks revealing an average field value of 33.5 ± 1.1 lT, which is 11–26% lower than expected values from global geomagnetic models based on historical and archaeomagnetic data. Global models for 1615 AD predict a low in central-southern Africa related to past location of the present Southern Atlantic Anomaly (SAA). Our results suggest that the field intensity in central Africa may have been slightly lower than global model predictions. This would indicate that the low could be probably more extended towards central-eastern Africa (or more intense) than previously considered. Further data from this region are especially welcome to delineate the evolution of the SAA.en
dc.language.isoEnglishen
dc.publisher.nameElsevier Science Limiteden
dc.relation.ispartofPhysics of the Earth and Planetary Interiorsen
dc.relation.ispartofseries/242(2015)en
dc.subjectPaleomagnetic secular variationen
dc.subjectArcheomagnetismen
dc.subjectPaleointensityen
dc.subjectCentral Africaen
dc.subjectGeomagnetic modelsen
dc.subjectSouth Atlantic Anomalyen
dc.titleFirst archaeomagnetic field intensity data from Ethiopia, Africa (1615 ± 12 AD)en
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber24 - 35en
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.06. Paleomagnetismen
dc.identifier.doi10.1016/j.pepi.2015.03.003en
dc.description.obiettivoSpecifico1A. Geomagnetismo e Paleomagnetismoen
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0031-9201en
dc.relation.eissn1872-7395en
dc.contributor.authorOsete, M. L.en
dc.contributor.authorCatanzariti, G.en
dc.contributor.authorChauvin, A.en
dc.contributor.authorPavón-Carrasco, F. J.en
dc.contributor.authorRoperch, P.en
dc.contributor.authorFernández, V. M.en
dc.contributor.departmentFacultad de Ciencias Físicas, Universidad Complutense de Madrid, Avda Complutense s/n, 28040 Madrid, Spainen
dc.contributor.departmentFacultad de Ciencias Físicas, Universidad Complutense de Madrid, Avda Complutense s/n, 28040 Madrid, Spainen
dc.contributor.departmentGéosciences-Rennes, CNRS, UMR 6118, Université de Rennes 1, Campus de Beaulieu, 35042 Rennes, Cedex, Franceen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentGéosciences-Rennes, CNRS, UMR 6118, Université de Rennes 1, Campus de Beaulieu, 35042 Rennes, Cedex, Franceen
dc.contributor.departmentDepartamento de Prehistoria, Universidad Complutense de Madrid, 28040 Madrid. Spainen
item.openairetypearticle-
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.deptFacultad de Ciencias Físicas, Universidad Complutense de Madrid, Avda Complutense s/n, 28040 Madrid, Spain-
crisitem.author.deptGeosciences-Rennes, CNRS, UMR 6118, Universite de Rennes 1, Campus de Beaulieu, Rennes, Cedex, France-
crisitem.author.deptGéosciences-Rennes, CNRS, UMR 6118, Université de Rennes 1, Campus de Beaulieu, 35042 Rennes, Cedex, France-
crisitem.author.deptDepartamento de Prehistoria, Universidad Complutense de Madrid, 28040 Madrid. Spain-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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