Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/966
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dc.contributor.authorallFaggioni, O.; Istituto di Geofisica Marina, Università di Pisa, Consorzio Universitario della Spezia, Italyen
dc.contributor.authorallBeverini, N.; Istituto di Geofisica Marina, Università di Pisa, Consorzio Universitario della Spezia, Italyen
dc.contributor.authorallCaratori Tontini, F.; Istituto di Geofisica Marina, Università di Pisa, Consorzio Universitario della Spezia, Italyen
dc.contributor.authorallCarmisciano, C.; Istituto di Geofisica Marina, Università di Pisa, Consorzio Universitario della Spezia, Italyen
dc.contributor.authorallNicolosi, I.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.date.accessioned2006-02-23T09:54:12Zen
dc.date.available2006-02-23T09:54:12Zen
dc.date.issued2003en
dc.identifier.urihttp://hdl.handle.net/2122/966en
dc.description.abstractThe aim of this work is the formulation of a 3D model of the Mt. Amiata volcanic complex (Southern Tuscany) by means of geomagnetic data. This work is shown not only as a real test to check the validity of the inversion algorithm, but also to add information about the structure of the volcanic complex. First, we outline briefly the theory of geomagnetic data inversion and we introduce the approach adopted. Then we show the 3D model of the Amiata volcano built from the inversion, and we compare it with the available geological information. The most important consideration regards the surface distribution of the magnetization that is in good agreement with rock samples from this area. Moreover, the recovered model orientation recall the extension of the lava flows, and as a last proof of validity, the source appears to be contained inside of the topographic contour level. The credibility of the inversion procedure drives the interpretation even for the deepest part of the volcano. The geomagnetic signal appears suppressed at a depth of about 2 km, but the most striking consequence is that sub-vertical structures are found even in different positions from the conduits shown in the geologic sections. The results are thus in good agreement with the information obtained from other data, but showing features that had not been identified, stressing the informative power of the geomagnetic signal when a meaningful inversion algorithm is used.en
dc.format.extent916647 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.publisher.nameINGVen
dc.relation.ispartofAnnals of Geophysicsen
dc.relation.ispartofseries3/46 (2003)en
dc.subjectmagnetic methoden
dc.subjectMt. Amiata volcanoen
dc.subjectpotential field inversionen
dc.titleA realistic inversion algorithm for magnetic anomaly data: the Mt. Amiata volcano testen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.04. Magnetic anomaliesen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorFaggioni, O.en
dc.contributor.authorBeverini, N.en
dc.contributor.authorCaratori Tontini, F.en
dc.contributor.authorCarmisciano, C.en
dc.contributor.authorNicolosi, I.en
dc.contributor.departmentIstituto di Geofisica Marina, Università di Pisa, Consorzio Universitario della Spezia, Italyen
dc.contributor.departmentIstituto di Geofisica Marina, Università di Pisa, Consorzio Universitario della Spezia, Italyen
dc.contributor.departmentIstituto di Geofisica Marina, Università di Pisa, Consorzio Universitario della Spezia, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
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.deptUNIPI-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0002-9772-3453-
crisitem.author.orcid0000-0002-2868-4235-
crisitem.author.orcid0000-0001-7357-2147-
crisitem.author.orcid0000-0002-0711-9923-
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-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
Appears in Collections:Annals of Geophysics
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