Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/2285
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dc.contributor.authorallSperanza, F.; Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy.en
dc.contributor.authorallBranca, S.; Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy.en
dc.contributor.authorallColtelli, M.; Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy.en
dc.contributor.authorallCaracciolo, F.; Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy.en
dc.contributor.authorallVigliotti, L.; Istituto di Scienze Marine, Consiglio Nazionale delle Ricerche,en
dc.date.accessioned2007-07-03T09:04:27Zen
dc.date.available2007-07-03T09:04:27Zen
dc.date.issued2006en
dc.identifier.urihttp://hdl.handle.net/2122/2285en
dc.description.abstractIn the last years, paleomagnetism has been increasingly used to provide emplacement ages of loosely dated volcanics. Dating is achieved by comparison of paleomagnetic directions with a given reference curve of the paleosecular variation (PSV) of the geomagnetic field. Recently, a debate has developed on the achievable precision (the a95 value) of the paleomagnetic directions and hence on the accuracy that ‘‘paleomagnetic dating’’ can yield. At 39 different sites from Etna we paleomagnetically investigated 13 flows (four ‘‘test flows’’ with known age, and nine loosely dated flows), emplaced between 122 B.C. and 1865 A.D. We systematically drilled 12 cores per flow spaced in three (far from each other) sites and demagnetized one specimen per core by alternating field cleaning. Results from the four test flows yield age windows effectively encompassing the respective true flow ages, when dating based on Bayesian statistics at a 95% confidence level is adopted. We find a95 values for the flow mean directions ranging between 3.3 and 5.7 (4.5 on average), which translate into accuracies of age determinations of 136–661 years (307 years on average). Such dating uncertainty is likely underestimated, as we disregarded several kinds of errors that might affect both the fidelity of paleomagnetic recording and the PSV reference curve. The strong magnetization of both the underlying terrain and the cooling flow itself and mineral magnetic variations across the flows are the most likely sources for the scatter characterizing the recording process of the magnetic field in volcanic rocks.en
dc.format.extent1525569 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.relation.ispartofJOURNAL OF GEOPHYSICAL RESEARCH,en
dc.relation.ispartofseriesB12/111(2006)en
dc.subjectpaleomagneticen
dc.subjectMount Etnaen
dc.titleHow accurate is ‘‘paleomagnetic dating’’? New evidence from historical lavas from Mount Etnaen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumberS33en
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.06. Paleomagnetismen
dc.identifier.doidoi:10.1029/2006JB004496en
dc.description.fulltextreserveden
dc.contributor.authorSperanza, F.en
dc.contributor.authorBranca, S.en
dc.contributor.authorColtelli, M.en
dc.contributor.authorCaracciolo, F.en
dc.contributor.authorVigliotti, L.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Rome, Italy.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Rome, Italy.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Rome, Italy.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Rome, Italy.en
dc.contributor.departmentIstituto di Scienze Marine, Consiglio Nazionale delle Ricerche,en
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Bologna, Bologna, Italia-
crisitem.author.orcid0000-0001-5492-8670-
crisitem.author.orcid0000-0002-4971-4528-
crisitem.author.orcid0000-0001-7868-3946-
crisitem.author.orcid0000-0003-3148-8216-
crisitem.author.orcid0000-0002-4160-8958-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
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