Detailed crustal structure in the area of the southern Apennines–Calabrian Arc border from local earthquake tomography
Introduction
The western Mediterranean area, located at the contact belt between the slowly convergent African and Eurasian plates (Calais et al., 2003, Nocquet and Calais, 2004, Serpelloni et al., 2007), has been the site of a continental-scale lithospheric subduction process, the evolution of which in the last 30 million years is marked by the eastward migration of the retreating subduction hinge (Fig. 1a; Wortel and Spakman, 2000). Most of the subduction system has already undergone detachment of the subducting lithosphere with the exception of the central, most arcuate portion of the system, the Calabrian Arc in southern Italy (Fig. 1b; Neri et al., 2009 and references therein). Different states of the subduction process can be related to the progressive change of lithospheric structure near the retreating trench zone and to strong lithospheric heterogeneity between the Calabrian Arc and the marginal tectonic units of Sicily and southern Apennines, where detachment has already occurred (Cimini and Marchetti, 2006, Faccenna et al., 2005, Lucente et al., 2006, Montuori et al., 2007, Neri et al., 2009, Spakman and Wortel, 2004). According to Govers and Wortel (2005) this scenario, characterized by a progressive detachment of a retreating lithospheric slab, may have led to the generation of a Subduction-Transform Edge Propagator (STEP) fault that laterally decouples subducting lithosphere from non-subducting lithosphere in a scissor type of fashion.
The lithosphere and mantle setting of the southern Apennines–Calabrian Arc border region has been deeply investigated in the last decades by means of regional and local seismic analyses reported in several previous papers (Barberi et al., 2004, Chiarabba et al., 2008, Chironi et al., 2000, Giacomuzzi et al., 2012, Montuori et al., 2007, Neri et al., 2002, Neri et al., 2009, Steckler et al., 2008). Different velocity patterns have been identified, providing evidences for first order crustal and sub-crustal heterogeneities and boundaries between the main crustal domains of Southern Apennines, Calabrian, and Tyrrhenian regions (Fig. 1b). High velocity pattern at crustal depth beneath the Tyrrhenian Sea is commonly interpreted with the thinning of the Tyrrhenian crust and incipient oceanization (Barberi et al., 2004, Chiarabba et al., 2008, Finetti, 2005a, Finetti, 2005b, Orecchio et al., 2011, Pepe et al., 2000). At greater depths, tomographic analysis evidenced that the Ionian subducting slab is in-depth continuous only beneath the central part of the Arc in southern Calabria while detachment has already occurred at the northern and southwestern edges of the arc itself, e.g. northern Calabria and northeastern Sicily, respectively (Fig. 1b; Neri et al., 2009). Beneath the southern Apennines lack of subcrustal seismicity and of high-velocity anomalies down to 200 km depth, together with a southwestward dipping high-velocity body at greater depths have been detected (Cimini, 1999, Cimini and Marchetti, 2006, Wortel and Spakman, 2000). In this framework the Calabrian Arc, a curved structure characterized by very heterogeneous seismotectonic regimes along its length (Cristofolini et al., 1985, Montone et al., 2004), together with the adjacent southern Apennines sector, has been the site of destructive, magnitude class 6 and 7 earthquakes that have occurred both in recent and historical times (Fig. 1b; Galli et al., 2008, Neri et al., 2006).
In the junction area between the Southern Apennines and the Calabrian Arc domains (e.g. at the northern edge of the Calabrian subduction zone, gray box in Fig. 1b), the Pollino Mts. area shows a structural and seismotectonic setting quite intricate, representing a highly deformed, very complex sector of great geodynamic interest and still not fully understood (see e.g. Bonini et al., 2011, Frepoli et al., 2011, Neri et al., 2012, Spina et al., 2011). Furthermore, in this sector a seismic gap was previously hypothesized by paleoseismological evidences associated with the lack of major earthquakes in historical catalogs (Cinti et al., 2002, Michetti et al., 2000). Since spring 2010 to 2013, this area has been affected by a seismic sequence with more than four thousands of small to moderate earthquakes (black dots in Fig. 1b). The strongest events occurred on May 28th 2012 (Ml 4.3) and on October 25th 2012 (Ml 5.0), respectively. Seismic activity has shown a fairly regular increase in number and energy since the onset of activity (Totaro et al., 2013). Epicentral distribution of the 2010–2013 sequence and the relative focal mechanism solutions evidenced two main clusters with a faint NNW-SSE-trend, showing predominantly normal faulting mechanisms with NE extension. The recent seismic activity has been interpreted as a seismic deformation occurring inside the southern Apennines extensional domain, specifically at its southern tip (Totaro et al., 2013).
In order to better characterize the crustal structures of this peculiar region of southern Italy, which includes the Pollino Mts. area, we performed a local earthquake tomography by applying the LOTOS code (Koulakov, 2009), drawing also benefit from the large amount of data coming from the 2010–2013 seismic activity. The use of the LOTOS code, that represents the first application of this algorithm in the southern Italy crustal studies, allowed us to obtain highly resolved results strongly reducing the grid spacing with respect to previous investigations carried out in the region, and also to furnish a detailed Vp/Vs model not previously available for the study area.
Section snippets
Tectonic settings
The large Calabrian Arc is a Cenozoic–Quaternary curved orogen (Fig. 1a) running from the NW–SE-trending Southern Apennines to the E–W-trending Sicilian Maghrebides (Carminati et al., 2012, Catalano et al., 1996, Lavecchia et al., 2007, Malinverno and Ryan, 1986, Minelli and Faccenna, 2010, Polonia et al., 2011, Rosenbaum and Lister, 2004). The central part of the Arc is characterized by the presence of a narrow subduction zone, which appears to be the only site of residual active subduction in
Data and method
In order to increase the detail of our analysis with respect to previous study carried out in the same sector (Barberi et al., 2004, Calò et al., 2013, Chiarabba et al., 2008, Orecchio et al., 2011), we performed a tomographic inversion by applying the LOTOS algorithm (Koulakov, 2009). We used the data of local seismicity occurred in the study region and collected from the available national and local networks managed by INGV (www.ingv.it) and University of Calabria, respectively. We selected
Results and discussion
In order to estimate a possible effect of noise on the resolution as well as the optimal values of inversion parameters, we performed several synthetic tests. In particular, in Fig. 3 we present three different checkerboard tests. In these models we defined periodic positive and negative velocity anomalies of different sizes and empty spacing between them: 20–10 km for Model 1, 15–7 km for Model 2 and 10–5 km for Model 3. Anomalies always had amplitude equal to 5% and opposite signs for P- and
Conclusions
The present study represents the first application of the LOTOS algorithm to crustal analyses in southern Italy. This code allowed us to obtain a new highly resolved seismic velocity model for the southern Apennines–Calabrian Arc border region furnishing also a detailed Vp/Vs model not previously available for the study area.
The tomographic results for P- and S anomalies at the upper crust layer show a fairly good correlation between velocity patterns and the main geological features of the
Acknowledgments
This research has been supported by Istituto Nazionale di Geofisica e Vulcanologia and Dipartimento della Protezione Civile (DPC) through the INGV-DPC 2014 S1 Project and by the Project of National Interest PRIN 2010-2011 “Geodinamica attiva e recente dell’Arco Calabro e del complesso di accrezione nel Mar Ionio”, funded by Ministero Istruzione Università e Ricerca (MIUR).
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