Earth-prints repository, logo   DSpace

About DSpace Software
|earth-prints home page | roma library | bologna library | catania library | milano library | napoli library | palermo library
Please use this identifier to cite or link to this item:

Authors: Piana Agostinetti, N.*
Chiarabba, C.*
Title: Seismic Structure Beneath Mt. Vesuvius From Receiver Function Analysis and Local Earthquakes Tomography: Evidences for Location and Geometry of the Magma Chamber
Title of journal: Geophys. J. Int.
Series/Report no.: 3/175 (2008)
Publisher: Blackwell publishing
Issue Date: 30-Jun-2008
DOI: 10.1111/j.1365-246X.2008.03868.x
Keywords: Receiver Function
Magma Chamber
Local Earthquake tomography
Abstract: The recognition and localisation of magmatic fluids are pre-requisites for evaluating the volcano hazard of the highly urbanized area of Mt. Vesuvius. Here we show evidence and constraints for the volumetric estimation of magmatic fluids underneath this sleeping volcano. We use Receiver Functions for teleseismic data recorded at a temporary broad band station installed on the volcano to constrain the S-wave velocity structure in the crust. Receiver Functions are analyzed and inverted using the Neighbourhood Algorithm approach. The 1D S-velocity profile is jointly interpreted and discussed with a new Vp and Vp/Vs image obtained by applying double difference tomographic techniques to local earthquakes. Seismologic data define the geometry of an axial, cylindrical high Vp, high Vs body consisting of a shallow solidified materials, probably the remnants of the caldera, and ultramafic rocks paving the crustal magma chamber. Between these two anomalies, we find a small region where the shear wave velocity drops, revealing the presence of magma at relatively shallow depths. The volume of fluids (30 km3) is sufficient to contribute future explosive eruptions.
Appears in Collections:04.06.08. Volcano seismology
Papers Published / Papers in press

Files in This Item:

File Description SizeFormatVisibility
piana_gji_manuscript_revised.texAccepted paper45.83 kBTeXView/Open

This item is licensed under a Creative Commons License
Creative Commons

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.

Share this record




Stumble it!



Valid XHTML 1.0! ICT Support, development & maintenance are provided by CINECA. Powered on DSpace Software. CINECA