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THE SOUTHERN TYRRHENIAN SEA MARGIN                               497

        eastward  migration  of  the  Apenninic  arc  system  and
        related  back-arc  extension  induced  by  the  retreat  of  a
        steeply  west-dipping  subduction  zone  (RÉHAULT et  alii,
        1984; MALINVEMO & RYAN, 1986; GUEGUEN et alii, 1997,
        1998). In spite of an ongoing debate on the deep geometry
        and  physical  continuity  of  the  subducting  slab  (i.e.  the
        slab break-off model: WORTEL & SPAKMAN, 1991; CARMI-
        NATI et alii, 1998), recent geophysical and volcanological
        data (PECCERILLO, 1985; FINETTI & DEL BEN, 1986; SPAK-
        MAN, 1989; AMATO et alii, 1993; SELVAGGI & CHIARABBA,
        1995;  WILSON &  BIANCHINI,  1999)  further  support  the
        view of subduction as the dominant geodynamic process.
        The southernmost domains of the Apennine-Maghrebide
        subduction zone, i.e. the Sicilian and Tunisian segments,
        are deformed by the concomitant, slowly north-northwest
        moving  African  plate  (MALINVERNO &  RYAN,  1986;  DE
        METS et alii, 1994; GUEGUEN et alii, 1998). This interfer-
        ence of the subduction process with the slow northward
        drift of Africa is best seen in Sicily, which can therefore
        be considered a key-area for the study of the present-day
        and  recent  geodynamics  of  the  central  Mediterranean
        region (MANTOVANI et alii, 2009; VITI et alii, 2009).
           The arcuate shape of the Apennine-Maghrebide sys-
        tem  is  thought  to  reflect  primary  compositional  differ-
        ences  in  the  subducted  crustal  slabs,  with  the  Ionian
        basin,  floored  by  old  oceanic  crust  (DE VOGD et  alii,
        1992),  separating  the  Sicilian  and  Apulian  continental
        forelands. Because of this compositional difference, dur-
        ing the last 5 Ma the Calabrian arc continued to roll-back
        faster  than  the  adjacent  segments,  like  the  Southern
        Apennines where the eastward migration of the Apulian
        hinge slowed down by a factor of 6 in 10 Ma (GUEGUEN et
        alii, 1997, 1998).


        TECTONICS OF THE SOUTHERN TYRRHENIAN SEA MARGIN
           The tectonic setting of Sicily is characterised by the
        superposition of different tectonic units that were origi-  Fig. 1 - Structural sketch map of the Central Mediterranean showing
        nated at expense of distinct palaeogeographic domains of  the major structures and the main tectonic domains.
                                                              – Schema semplificato della regione centro-mediterranea, che illustra i
        the African mesozoic continental margin (OGNIBEN, 1960).  lineamenti tettonici di primo ordine e le principali strutture deformative.
        The main recognised units in central-northern Sicily are
        the basin-derived Sicilide and Imerese Units, and the plat-
        form-derived  Panormide  Unit.  From  Oligocene  time  ing the continental platform of Sardinia (RÉHAULT et alii,
        onwards, these units were piled along shallow thrusts and  1987;  BOCCALETTI et  alii,  1990).  Other  important  N-S
        translated  southwards  during  the  construction  of  the  trending  faults  extend  for  over  150  km  and  dip  west-
        Apennine-Maghrebide fold-and-thrust system (CATALANO  wards,  bounding  the  Paola  Basin  (BOCCALETTI et  alii,
        et  alii,  1984).  The  thrust  surfaces  have  been  offset  by  1990). The N-S trending faults are not laterally continu-
        recent structures related to the opening of the Tyrrhenian  ous, but rather appear segmented by E-W trending strike-
        Sea  during  Neogene-Quaternary  time  (MALINVERNO &  slip  faults.  The  northernmost  E-W  trending  faults  are
        RYAN, 1986). The opening involved significant anticlock-  characterised by dominantly left-lateral kinematics (fig. 1;
        wise rotations (RÉHAULT et alii, 1987; DEWEY et alii, 1989;  SELLI, 1985; LAVECCHIA, 1988). Southward, an important
        GUEGUEN et alii, 1997, 1998), and was controlled by faults  E-W trending fault zone, known as the Ustica-Eolie Line
        of different orientations (fig. 1; BOCCALETTI et alii, 1982,  (UEL: BOCCALETTI et alii, 1984) or Southern Tyrrhenian
        1984,  1990;  WEZEL,  1985).  The  most  important  recog-  Line  (BOCCALETTI et  alii,  1990),  lies  on  the  southern
        nised fault trends are: N-S, E-W and NW-SE (BOCCALETTI  Tyrrhenian Sea margin, where it extends for over 400 km.
        et  alii,  1982).  NE-SW  trending  faults,  although  present  BOCCALETTI & DAINELLI (1982) first inferred for this fault
        and  locally  important  in  the  central  Mediterranean  a right-lateral kinematic character. Towards the west the
        region, are poorly developed along the southern Tyrrhen-  UEL can be related to the North Balearic Fracture Zone
        ian Sea margin (e.g. see NIGRO et alii, 2000). N-S trending  (NBFZ, MAUFFRET, 1976; AUZENDE et alii, 1973) that rep-
        faults display a marked extensional character. Slip along  resents  the  southern  boundary  of  the  Liguro-Provençal
        these faults led to attenuation of the previously thickened  Basin and allowed the drift of the Corsica-Sardinia block
        continental lithosphere, and to creation of new oceanic  during the opening of the basin (AUZENDE et alii, 1973;
        floor (KASTENS et alii, 1987). The main recognised struc-  RÉHAULT et  alii,  1984;  GUEGUEN et  alii,  1998,  among
        tures extend for over 300 km and dip eastwards, bound-  many others). Right-lateral kinematic character of south-
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