Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/4531
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dc.contributor.authorallFedi, M.; Dipartimento di Scienze Della Terra, Universit degli Studi di Napoli Federico II, Largo San Marcellino 10, 80138 Napoli, Italyen
dc.contributor.authorallCascone, L.; Dipartimento di Scienze Della Terra, Università degli Studi di Napoli “Federico II”, Largo San Marcellino 10, 80138 Napoli, Italyen
dc.contributor.authorallDel Negro, C.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallLa Manna, M.; Dipartimento di Scienze Della Terra, Università degli Studi di Napoli “Federico II”, Largo San Marcellino 10, 80138 Napoli, Italyen
dc.date.accessioned2008-12-09T10:36:14Zen
dc.date.available2008-12-09T10:36:14Zen
dc.date.issued2008en
dc.identifier.urihttp://hdl.handle.net/2122/4531en
dc.description.abstractVolcanomagnetic anomalies have been mostly observed during strong eruptions. Our aim is to improve the geomagnetic data analysis to evidence the anomalies occurring in a larger time span, especially in the phases preceding the eruptive events. We developed a time variant statistical approach and applied it to the 20002002 Etna geomagnetic temporal series. It is based on an algorithm that statistically predicts the geomagnetic field at the station on the volcanic edifice by that recorded at the remote one. In such a way a number of significant changes in the time series (called statistical innovations), marking the local magnetic field change, were detected. The distribution of such statistical innovations accurately describes the Etna volcanic evolution: we note a progressive increase of the innovation occurrence as the eruptive cycles were approaching and only few and weak innovations at times between the various eruptive cycles. The significance of this analysis is further confirmed by the close agreement among the mean square prediction error, strain release and the volcanic activity behavior. On the contrary, the geomagnetic field at a single station or its difference at two stations do not have any clear correlation with other measured physical quantities. The complex pattern of the prediction error was also investigated by a multifractal analysis. We found that the Holder regularity increases with the intensification of the volcanic activity, implying that innovations tend to be less sporadic and correlated during the major volcanic phases.en
dc.language.isoEnglishen
dc.publisher.nameelsevieren
dc.relation.ispartofEarth and Planetary Science Lettersen
dc.relation.ispartofseries/269 (2008)en
dc.subjectEtna volcanoen
dc.subjectgeomagnetic methoden
dc.subjectvolcanic monitoringen
dc.subjectpredictive analysisen
dc.titleTime variant analysis of geomagnetic signals describes the volcanic activityen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber155-163en
dc.subject.INGV04. Solid Earth::04.02. Exploration geophysics::04.02.04. Magnetic and electrical methodsen
dc.identifier.doi10.1016/j.epsl.2008.02.016en
dc.description.obiettivoSpecifico2.6. TTC - Laboratorio di gravimetria, magnetismo ed elettromagnetismo in aree attiveen
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorFedi, M.en
dc.contributor.authorCascone, L.en
dc.contributor.authorDel Negro, C.en
dc.contributor.authorLa Manna, M.en
dc.contributor.departmentDipartimento di Scienze Della Terra, Universit degli Studi di Napoli Federico II, Largo San Marcellino 10, 80138 Napoli, Italyen
dc.contributor.departmentDipartimento di Scienze Della Terra, Università degli Studi di Napoli “Federico II”, Largo San Marcellino 10, 80138 Napoli, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentDipartimento di Scienze Della Terra, Università degli Studi di Napoli “Federico II”, Largo San Marcellino 10, 80138 Napoli, Italyen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptDipartimento di Geofisica e Vulcanologia, L.go S. Marcellino 10, 80138 Napoli, Italy-
crisitem.author.deptDipartimento di Scienze Della Terra, Università degli Studi di Napoli “Federico II”, Largo San Marcellino 10, 80138 Napoli, Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptDepartment of Earth, Environment and Resources Science, University Federico II, Complesso di Monte S. Angelo, Via Cintia, Edifice L, I-80126 Naples, Italy-
crisitem.author.orcid0000-0002-2145-2271-
crisitem.author.orcid0000-0001-5734-9025-
crisitem.author.orcid0000-0003-1260-4277-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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