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. Seismic anisotropy time variations at Mt Etna
 
  • Details

Seismic anisotropy time variations at Mt Etna

Author(s)
Nardone, Lucia  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia  
Bianco, Francesca  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia  
Zaccarelli, Lucia  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Bologna, Bologna, Italia  
Patanè, Domenico  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia  
Language
English
Obiettivo Specifico
2V. Struttura e sistema di alimentazione dei vulcani
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Journal
Geophysical Journal International  
Issue/vol(year)
1/ 220 (2020)
Pages (printed)
450-460
Date Issued
January 2020
DOI
10.1093/gji/ggz460
URI
https://www.earth-prints.org/handle/2122/12920
Subjects

Seismic anisotropy

Volcano monitoring

Volcano seismology

Abstract
The aim of this paper is to study the temporal variations in the seismic wavefield associated with the stress changes in the dynamic features of the Mt Etna volcanic activity. We used shear wave splitting analysis on a huge data set of local earthquakes, in order to identify changes of the local stress field at Mt Etna during the time interval from 2006 to 2011. This analysis allows us to obtain two parameters: the polarization direction of the fast shear wave (φ) and the time delay of the slow shear wave (Td,time delay between the split shear waves). Orientation of φ generally provides information about the anisotropic symmetry and stress direction whereas Td provide information about the average crack density along the ray path.

Based on our findings it is possible to divide Etna Volcano in three different sectors, each one distinguished by typical fast wave polarization direction. We find that the western part of the volcano is controlled by the regional tectonic stress field having a NS and EW directions. Instead, the eastern part of the volcano is mainly controlled by the local volcanic stress, particularly an EW local stress field in the NE sector (Pernicana), and a quasi NS local stress field in the SE sector (Mascalucia, Timpe), where previous studies evidenced: (i) some low-Qp anomaly regions between 0 and about 6 km depth, probably associated with high pore pressure and the intense faulting and (ii) by magnetotelluric surveys, several high conductivity zones, up to 8 km depth, related to a diffuse presence of hydrothermal activity and fluid circulation. Temporal variations in time delay, mostly before the 2008–2009 lateral eruption, can be interpreted as stress accumulation increase with a consequent release of stress due to coalescing of microcracks in the conduit for the eruption of magma.
Description
This article has been accepted for publication in Geophysical Journal International ©: The Authors 2020. 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.
Type
article
File(s)
Loading...
Thumbnail Image
Name

Etna_Anisotropia_Nardone_2019.pdf

Size

4.97 MB

Format

Adobe PDF

Checksum (MD5)

96ea32e1982cd9c8128d2d9a87eed277

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