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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. |
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Giampiccolo_et_al_GJI_2021.pdf | Paper | 11.93 MB | Adobe PDF | View/Open |
Giampiccolo_et_al_2021_submitted_version.pdf | Open Access submitted article | 7.41 MB | Adobe PDF | View/Open |
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