Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/11353
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dc.date.accessioned2018-03-21T09:45:52Zen
dc.date.available2018-03-21T09:45:52Zen
dc.date.issued2006en
dc.identifier.urihttp://hdl.handle.net/2122/11353en
dc.description.abstractThe Colli Albani is a quiescent Volcanic District, located almost 20 Km southeast of Rome. It has been active since at least 600 ka and it belongs to the potassic and ultrapotassic Roman Magmatic Province, a northwest-trending chain of volcanoes that developed along the Tyrrhenian Sea Margin of Italy during middle and late Pleistocene time. The Albano maar (< 70 ka) represents the most recent activity of the hydromagmatic phase and cannot be considered extinguished yet. First Gravimetric map of Colli Albani Volcanic District was made by the Italian Geological Service from the 1:100,000 Gravimetric Map of Italy (Maino et al., 1969) and later some new gravity interpretations were performed by Di Filippo & Toro (1980, 1995). This paper gives preliminary gravity results in the northen and eastern side of the Volcanic District in order to obtain a detailed gravity map of Colli Albani Volcanic District. A broad area N of lake Albano (Rome, Ciampino-Marino) is the most one strongly characterized by the occurence of geochimical manifestation of a still-active subvolcanic system which are hazardous factors for the resident population. In eastern side of the volcano the previous studies showed that some areas are completely missing gravity stations. In this study the mesh interval between each gravity station are 500 m2 on average; in the previous was 2 km2 on average. A new Residual anomaly map has been prepared by substracting the first order Regional Field from Bouguer anomalies. The Residual anomaly map is very detailed and represents the most suitable picture for understanding the structure of the prevolcanic substratum. Residual anomaly map shows a maximium gravity value of Ciampino High, spatially continuous along the major NW-SE axis, corresponds to where the high distribution of radon and CO2 was observed. Another maximum value is located in the southern part of the Ciampino High relative to Rocca di Papa, where the second activity of the volcano took place.A minimum region gravity is located in the eastern part of the Ciampino High. The map shows faults obtained by gravity interpretations. The superficial geological data, the drill log data, and metamorphic xenoliths from the eruption of Colli Albani (Funiciello & Parotto, 1978) and gravity data have been analyzed all together in order to know sub-surface structure of this area and make a bi-dimensional gravity model. In order to define the heterogeneity of the lithotypes some sections have been prepared by gravity model.en
dc.language.isoengen
dc.relation.ispartofEUG 3th General Assemblyen
dc.subjectColli Albanien
dc.subjectRoman Magmatic Provinceen
dc.subjectRomeen
dc.subjectItalyen
dc.subjectgravity surveyen
dc.subject3D density modelen
dc.subjectcalderaen
dc.titleNew gravity interpretations in the northern and eastern side of the Colli Albani Volcanic District: first resultsen
dc.typeConference paperen
dc.description.statusPublisheden
dc.identifier.URLhttps://meetings.copernicus.org/egu2006/en
dc.description.ConferenceLocationVienna, Austria, 02-07 April 2006en
dc.description.obiettivoSpecifico1V. Storia eruttivaen
dc.description.obiettivoSpecifico2V. Struttura e sistema di alimentazione dei vulcanien
dc.description.obiettivoSpecifico6V. Pericolosità vulcanica e contributi alla stima del rischioen
dc.description.obiettivoSpecifico2SR. VULCANI - Servizi e ricerca per la Societàen
dc.contributor.authorDi Filippo, Micheleen
dc.contributor.authorDi Nezza, Mariaen
dc.contributor.authorToro, Beniaminoen
dc.contributor.departmentDipartimento di Scienze della Terra Università Sapienza di Romaen
dc.contributor.departmentDipartimento di Scienze della Terra Università Sapienza di Romaen
dc.contributor.departmentDipartimento di Scienze della Terra Università Sapienza di Romaen
item.fulltextWith Fulltext-
item.openairetypeConference paper-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextopen-
item.cerifentitytypePublications-
item.languageiso639-1en-
crisitem.author.deptCNR-IGAG-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptDipartimento di Scienze della Terra Università Sapienza di Roma-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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