Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/3348
DC FieldValueLanguage
dc.contributor.authorallBlanco-Montenegro, I.; Dep. de Física, Escuela Politécnica Superior, Universidad de Burgos, Avda. de Cantabriaen
dc.contributor.authorallDe Ritis, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallChiappini, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.date.accessioned2007-12-14T14:35:28Zen
dc.date.available2007-12-14T14:35:28Zen
dc.date.issued2007en
dc.identifier.urihttp://hdl.handle.net/2122/3348en
dc.description.abstractIn this paper, we present a magnetic model of the subsurface structure of Vulcano island based on highresolution aeromagnetic data. Three profiles across the most intense magnetic anomalies over the Piano and Fossa calderas were selected for the magnetic modelling, which was constrained by structural and volcanological data, previous geophysical models, paleomagnetic data, and borehole stratigraphy obtained from two deep wells. The interpretation of the magnetic sources represents a significant contribution to the understanding of the Piano and Fossa calderas’ underlying structure, providing us with evidence of the lateral discontinuity between them at depth. We propose that the positive magnetic anomalies in the Piano caldera area are caused by: (a) the remnants of an early submarine volcano; (b) an outcropping dyke swarm related to the feeding system of the Primordial Vulcano phase (beneath Mt. Saraceno); and (c) the presence of a non-outcropping dyke system intruded along a NE–SWoriented intra-caldera fault (beneath the eastern part of the Piano caldera). Offshore, to the west, the magnetic anomaly map suggests the presence of a submarine volcanic structure, not revealed by bathymetric data, which represent the eruptive centre, the presence of which has been indirectly deduced from the outcrop of eastern-dipping lavas on the western seashore. Magnetic modelling of the Fossa caldera points to the presence of a highly magnetized cone-like body inside the Fossa cone, centred beneath the oldest crater rims. We interpret this body as a pile of tephritic lavas emplaced in an early phase of activity of the Fossa cone, suggesting that the volume of mafic lavas that erupted at the beginning of the construction of the Fossa edifice was more significant than has previously been deduced. Furthermore, the presence of a magnetized body inside the Fossa cone implies that high temperatures are contained in very limited spaces, do not affect its bulk inner structure, and are restricted to fumarolic conduits and vents. In addition, structures beneath the western and northern part of the Fossa caldera are revealed to have null or low magnetization, which can be ascribed to the presence of pyroclasts and hyaloclastites in this area as well as to a large volume of hydrothermally altered materials. This suggests that the hydrothermal system, with a very limited extension at present, affected a larger area in the past, especially beneath the western part of the caldera.en
dc.language.isoEnglishen
dc.publisher.nameSpringer-Verlagen
dc.relation.ispartofBullettin of Volcanologyen
dc.relation.ispartofseries6/69 82007)en
dc.subjectHigh-resolution aeromagnetic dataen
dc.subjectCrustal imagingen
dc.subjectCalderasen
dc.subjectVolcanic islandsen
dc.subjectVulcanoen
dc.subjectAeolian Islandsen
dc.titleImaging and modelling the subsurface structure of volcanic calderas with high-resolution aeromagnetic data at Vulcano (Aeolian Islands, Italy)en
dc.typearticleen
dc.description.statusPublisheden
dc.description.pagenumber643-659en
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.04. Magnetic anomaliesen
dc.identifier.doi10.1007/s00445-006-0100-7en
dc.description.obiettivoSpecifico3.8. Geofisica per l'ambienteen
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorBlanco-Montenegro, I.en
dc.contributor.authorDe Ritis, R.en
dc.contributor.authorChiappini, M.en
dc.contributor.departmentDep. de Física, Escuela Politécnica Superior, Universidad de Burgos, Avda. de Cantabriaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
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.deptDepartamento de Física, Universidad de Burgos, Burgos, Spain.-
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.orcid0000-0003-1771-0132-
crisitem.author.orcid0000-0001-7433-9435-
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-
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
BlancoMontenegro et al_BOV.pdf874.01 kBAdobe PDF
Show simple item record

WEB OF SCIENCETM
Citations

37
checked on Feb 10, 2021

Page view(s) 20

364
checked on Apr 17, 2024

Download(s)

39
checked on Apr 17, 2024

Google ScholarTM

Check

Altmetric