Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/16272
Authors: Magrini, Fabrizio* 
Diaferia, Giovanni* 
Fadel, Islam* 
Cammarano, Fabio* 
van der Meijde, Mark* 
Boschi, Lapo* 
Title: 3-D shear wave velocity model of the lithosphere below the Sardinia–Corsica continental block based on Rayleigh-wave phase velocities
Journal: Geophysical Journal International 
Series/Report no.: /220 (2020)
Publisher: Oxford University Press - The Royal Astronomical Society
Issue Date: 2020
DOI: 10.1093/gji/ggz555
URL: https://academic.oup.com/gji/article-abstract/220/3/2119/5686723?login=false
Abstract: Rayleigh-wave dispersion curves from both ambient noise and teleseismic events allow us to provide the first high-resolution 3-D shear wave velocity (VS) model of the crust and upper mantle below the Sardinia–Corsica microplate, an important continental block for understanding the evolution of the central-western Mediterranean. For a wide range of periods (from 3 to ∼30 s), the phase velocities of the study area are systematically higher than those measured within the Italian peninsula, in agreement with a colder geotherm. Relative and absolute variations in the VS allow us to detect a very heterogeneous upper crust down to 8 km, as opposed to a relatively homogeneous middle and lower crust. The isosurface at 4.1 km s−1 is consistent with a rather flat Moho at a depth of 28.0 ± 1.8 km (2σ). The lithospheric mantle is relatively cold, and we constrain the thermal lithosphere–asthenosphere boundary at ∼100 km. We find our estimate consistent with a continental geotherm based on a surface heat flow of 60 mW m−2. Our results suggest that most of the lithosphere endured the complex history of deformation experienced by the study area and imply, in general, that deep tectonic processes do not easily destabilize the deeper portion of the continental lithosphere, despite leaving a clear surface signature.
Description: This article has been accepted for publication in Geophysical Journal International ©:The Author(s) 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. All rights reserved.
Appears in Collections:Article published / in press

Files in This Item:
File Description SizeFormat
ggz555.pdf5.08 MBAdobe PDFView/Open
Show full item record

Page view(s)

34
checked on Apr 17, 2024

Download(s)

10
checked on Apr 17, 2024

Google ScholarTM

Check

Altmetric