Repository logo
  • English
  • Italiano
Log In
New user? Click here to register.Have you forgotten your password?
  1. Home
  2. Affiliation
  3. INGV
  4. Article published / in press
  5. A first 3-D shear wave velocity model of the Ischia Island (Italy) by HVSR inversion
 
  • Details

A first 3-D shear wave velocity model of the Ischia Island (Italy) by HVSR inversion

Author(s)
Manzo, Roberto  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia  
Nardone, Lucia  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia  
Gaudiosi, Guido  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia  
Martino, Claudio  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia  
Galluzzo, Danilo  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia  
Bianco, Francesca  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia  
Di Maio, Rosa  
Language
English
Obiettivo Specifico
2V. Struttura e sistema di alimentazione dei vulcani
Status
Published
JCR Journal
JCR Journal
Journal
Geophysical Journal International  
Issue/vol(year)
/230 (2022)
ISSN
0956-540X
Publisher
Oxford University Press - The Royal Astronomical Society
Pages (printed)
2056–2072
Date Issued
2022
DOI
10.1093/gji/ggac157
URI
https://www.earth-prints.org/handle/2122/16289
Subjects

Inverse theory

Seismic noise

Volcano seismology

Calderas

Abstract
Following the Mw 3.9 earthquake that occurred in the Ischia island (Naples, southern Italy) on 21 August 2017, the local monitoring seismic network was significantly improved in terms of both number of stations and instrumentation performance. Due to the huge amount of collected seismic ambient noise data, in this paper we present a first 3-D shear wave velocity model of the island retrieved from the inversion of horizontal-to-vertical spectral ratio curves by fixing the shear wave velocities (Vs) and modifying the thicknesses to get the corresponding 1-D Vs models. We are confident about the robustness of the attained models since the inversion process provided a good convergence towards the best-fitting solutions. Then, a first 3-D velocity model was obtained by contouring all the 1-D models obtained for the selected seismic stations to highlight possible lateral variations of the layer thicknesses and to reconstruct the morphology of the deeper interface characterized by a high-impedance contrast. A good correspondence between the 3-D Vs model and the geological features of the island was observed, especially in the northern sector where most of the stations are installed. In particular, the top of the high-impedance contrast interface appears deeper in the northern coastal areas and shallower in the central sector. This result agrees with the structural settings of the island likely due to the resurgence of Mount Epomeo.
Description
This article has been accepted for publication in Geophysical Journal International ©:The Author(s) 2022. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.Uploaded in accordance with the publisher's self-archiving policy.
All rights reserved.
Type
article
File(s)
Loading...
Thumbnail Image
Name

ggac157.pdf

Size

7.68 MB

Format

Adobe PDF

Checksum (MD5)

192606c290839b6d40602a454d0b405e

rome library|catania library|milano library|napoli library|pisa library|palermo library
Explore By
  • Research Outputs
  • Researchers
  • Organizations
Info
  • Earth-Prints Open Archive Brochure
  • Earth-Prints Archive Policy
  • Why should you use Earth-prints?
Earth-prints working group
⚬Anna Grazia Chiodetti (Project Leader)
⚬Gabriele Ferrara (Technical and Editorial Assistant)
⚬Massimiliano Cascone
⚬Francesca Leone
⚬Salvatore Barba
⚬Emmanuel Baroux
⚬Roberto Basili
⚬Paolo Marco De Martini

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback