Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/12796
Authors: Ciaccio, Maria Grazia* 
Chiarabba, Claudio* 
Title: Tomographic models and seismotectonies of the Reggio Emilia region, Italy
Journal: Tectonophysics 
Series/Report no.: /344 (2002)
Issue Date: 2002
DOI: 10.1016/S0040-1951(01)00275-X
Abstract: The aim of this study is to define the Vp and Vp/Vs structure of the fault zone ruptured by the ML 5.1 earthquake of October 15, 1996 which occurred near Reggio Emilia (central-northern Italy). A 1-month-long seismic sequence followed the main- shock and occurred in a small region along the outer border of the northern Apenninic belt, at depth ranging between 10 and 17 km. P- and S-wave arrival times from 304 aftershocks recorded by two local dense seismic arrays installed in the epicentral region have been inverted to obtain one- and three-dimensional velocity models by using state of the art local earthquake tomographic techniques. Velocity models and aftershock relocation help us to infer the seismotectonic of the region. Earth- quakes originated along a NW-dipping backthrust of a NE-trending main thrust, composing the western part of the broad Ferrara Arc. A main high Vp and high Vp/Vs region delineates a pop-up structure in the center of the area. The high Vp/Vs within the pop-up structure supports the presence of a zone with increased pore pressure. The hypocentral depth of both mainshock and aftershocks is greater than those usually found for the main seismogenic regions of the Apenninic belt. P-wave velocity values in the seismogenic area, obtained by tomography, are compatible with rocks of the Mesozoic cover and suggest that seismicity occurred within the Mesozoic units stack at present by compressional tectonics. D 2002 Elsevier Science B.V. All rights reserved.
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