Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/8920
DC FieldValueLanguage
dc.contributor.authorallPavón-Carrasco, F. J.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallTorta, J. M.; Observatori de l'Ebre (Spain)en
dc.contributor.authorallOsete, M. L.; Universidad Complutense Madrid (Spain)en
dc.contributor.authorallDe Santis, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.date.accessioned2014-02-10T11:29:24Zen
dc.date.available2014-02-10T11:29:24Zen
dc.date.issued2014-02en
dc.identifier.urihttp://hdl.handle.net/2122/8920en
dc.description.abstractWe propose a new geomagnetic field model for the Holocene period based on archaeomagnetic and lava flow data, avoiding the use of lake sediment data. The source of data comes from the GEOMAGIA50v2 database which has been updated with the new archaeomagnetic and volcanic studies published during the last 3 years. The model, called SHA.DIF.14k, allows us to analyse the behaviour of the geomagnetic field for the last 14000 years: from 12000 BC to 1900 AD. For the model construction we use the spherical harmonic analysis in space and the penalized cubic B-splines in time. Both spatial and temporal regularization norms are used to constrain the inversion problem and applied at the core-mantle boundary (CMB) to assure the convergence of the model. For the last 3ka, the model predictions agree with those given by the global model ARCH3k.1 and the European model SCHA.DIF.3k. For older epochs, the new model presents a clear improvement in field resolution with respect to other current models of the geomagnetic field for the Holocene. For the last 9ka, the time evolution of the dipolar moment obtained from the dipole field shows a clear minimum between 5500 BC and 3000 BC, and the well-known continuous decreasing trend of the geomagnetic field strength for the last millennium and half. A general view of the time-average evolution of the geomagnetic field flux lobes at the CMB for the northern hemisphere suggests a marked lobe of positive magnetic flux when the dipole moment was maximum. This lobe vanishes when the dipolar field is decreasing. The north polar wander paths of both north magnetic dip and geomagnetic poles were obtained showing an average rate of motion of 5.1 km/yr and 3.7 km/yr respectively. The model shows that the geomagnetic field can be averaged as axial dipolar in ~2000 years within an error of 5º, the typical uncertainty of the palaeomagnetic studies. Finally, and following the recent definition of archaeomagnetic jerks, we found 8 critical events in the time-evolution of the geomagnetic field for the last 8ka characterized by a maximum in the hemispheric asymmetry of the proposed model. The model is available in the Earth Ref Digital Archive at http://earthref.org/ERDA/1897/.en
dc.language.isoEnglishen
dc.publisher.nameElsevier Science Limiteden
dc.relation.ispartofEarth and planetary science lettersen
dc.relation.ispartofseries/388 (2014)en
dc.subjectgeomagnetismen
dc.subjectarchaeomagnetismen
dc.subjectgeomagnetic field modelen
dc.subjectsecular variationen
dc.subjectholoceneen
dc.titleA geomagnetic field model fo the Holocene based on archaeomagnetic and lava flow dataen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber98-109en
dc.identifier.URLhttp://earthref.org/ERDA/1897/en
dc.identifier.URLhttp://pc213fis.fis.ucm.es/sha.dif.14k/index.htmlen
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.01. Dynamo theoryen
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.identifier.doi10.1016/j.epsl.2013.11.046en
dc.description.obiettivoSpecifico1A. Geomagnetismo e Paleomagnetismoen
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0012-821Xen
dc.relation.eissn1385-013Xen
dc.contributor.authorPavón-Carrasco, F. J.en
dc.contributor.authorTorta, J. M.en
dc.contributor.authorOsete, M. L.en
dc.contributor.authorDe Santis, A.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentObservatori de l'Ebre (Spain)en
dc.contributor.departmentUniversidad Complutense Madrid (Spain)en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptObservatori de l’Ebre, CSIC - URL, Horta Alta 38, 43520 Roquetes, Spain-
crisitem.author.deptUniv. Complutense Madrid (Spain)-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0002-3941-656X-
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.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
Appears in Collections:Article published / in press
Files in This Item:
File Description SizeFormat Existing users please Login
Pavón-Carrasco et al., 2014.pdfMain Article3.91 MBAdobe PDF
Show simple item record

WEB OF SCIENCETM
Citations 50

189
checked on Feb 7, 2021

Page view(s) 5

507
checked on Apr 24, 2024

Download(s) 50

123
checked on Apr 24, 2024

Google ScholarTM

Check

Altmetric