Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/15115
Authors: Giampiccolo, Elisabetta* 
Del Pezzo, Edoardo* 
Tuvè, Tiziana* 
Di Grazia, Giuseppe* 
Ibanez, Jesús M* 
Title: 3-D Q-coda attenuation structure at Mt. Etna (Italy)
Journal: Geophysical Journal International 
Series/Report no.: 1/227 (2021)
Publisher: Oxford University Press
Issue Date: 2021
DOI: 10.1093/gji/ggab235
Abstract: Three dimensional attenuation images of Mt Etna volcano obtained by the analysis of Q-coda from local volcano-tectonic earthquakes are presented in this work. Seismic sources are confined inside the Etna structure with a maximum focal depth of 35 km below the sea level. The space distribution of the attenuation values was calculated by using 3-D weighting functions derived by the sensitivity kernels of Pacheco & Snieders and approximated by a polynomial interpolation, represented in the maps by using a backprojection method. Data were analyzed in four bands with central frequency placed at 1.5, 3, 6 and 12 Hz, respectively. We observed a frequency dependence of Q-coda with values that range from 55 at 1.5 Hz to 218 at 12 Hz. Q-coda space distribution in the Etna area shows almost uniformity in the average attenuation in the first 35 km below the surface. The images were derived with a resolution of 5 km. We observe as one of our main conclusions that Q-coda attenuation space anomalies are correlated with the areas of highest structural heterogeneities and are distributed along the well-known tectonic structures which characterize the crust in Mt Etna region. Previous and numerous velocity and attenuation images describing the structure of Mt Etna support our main conclusion: high Q-coda volumes almost coincide with the zones marked by high velocity and relative low total attenuation for direct waves.
Description: This article has been accepted for publication in Geophysical Journal International ©: The Authors 2021. 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.
This article has been accepted for publication in Geophysical Journal International ©:The Author(s) 2021. 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.
Appears in Collections:Article published / in press

Files in This Item:
File Description SizeFormat
Giampiccolo_et_al_GJI_2021.pdfPaper11.93 MBAdobe PDFView/Open
Giampiccolo_et_al_2021_submitted_version.pdfOpen Access submitted article7.41 MBAdobe PDFView/Open
Show full item record

Page view(s)

201
checked on Apr 24, 2024

Download(s)

144
checked on Apr 24, 2024

Google ScholarTM

Check

Altmetric