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THE SOUTHERN TYRRHENIAN SEA MARGIN                               501

           Separate data analyses have been performed first for
        each technique (VLBI, GPS and SLR) and then the solu-
        tions were combined. In fact, once the geodetic solutions
        have been obtained, it is important to define a common
        reference frame prior to comparing and combining the
        results. Therefore the different solutions have been trans-
        formed and combined within the ITRF97 reference frame
        (BOUCHER et  alii,  1999).  Then  residual  velocities  with
        respect to the Eurasian block have been computed sub-
        tracting the rigid motion of Eurasia defined by 13 ITRF97
        stable sites located in central Europe and expressed in the
        ITRF97 reference frame (DEVOTI et alii, 2002).
           The last step in the analysis is the computation of the
        strain tensor (fig. 6) by using the residual horizontal veloci-
        ties  at  the  summit  of  triangles  (e.g.  Cagliari,  Noto  and
        Cosenza).  These  horizontal  velocity  components  can  be
        post-processed to evaluate the horizontal velocity gradient
        tensor at the barycentre of the triangle, elected as reference
        point. The strain rate tensor (fig. 6) provides a measure of
        internal deformation within the region and the rotation rate
        tensor gives the rigid body rotation about the local vertical
        (DEVOTI et alii, 2002). In the southern Tyrrhenian basin the
        three stations used to estimate the strain tensor are Cagliari,
        Cosenza  and  Noto.  The  results  show  a  NW-SE  directed
        shortening and a coeval SW-NE directed extension (fig. 6).


                            DISCUSSION

           The  results  of  space  geodesy  data  analysis,  inte-
        grated  with  available  geophysical  information,  indicate  Fig. 6 - Map of the Southern Tyrrhenian Sea, showing the strain tensor
        that  the  present-day  deformation  field  of  the  southern  computed from space geodesy measurements (modified after DEVOTI
                                                              et alii, 2002).
        Tyrrhenian Sea margin is characterised by a mean NW-  – Carta semplificata del Mare Tirreno Meridionale: gli assi principali
        SE direction of contraction, and a mean SW-NE direction  dalla deformazione sono stati calcolati attraverso la raccolta e l’elabo-
        of  extension.  Independent  structural  data  from  Plei -  razione di dati provenienti dalle tecniche di analisi di geodesia spaziale
        stocene or younger faults exposed onshore northern Sicily  (da DEVOTI et alii, 2002, con modifiche).
        are broadly consistent with geodetic and geophysical evi-
        dence,  and  suggest  that  the  inferred  NW-SE  directed
        shortening field remained in a constant orientation dur-  geodetic and structural analyses may represent a key for a
        ing the last 2 Ma (GUARNIERI, 2004). Our multidisciplinal  better understanding of the recent central Mediterranean
        approach provides a key for the interpretation of struc-  geodynamics. In particular, the data from space geodesy
        tures in the central Mediterranean area, whose kinemat-  and fault-slip analyses provide new evidence to help con-
        ics is still poorly constrained. Hereafter we discuss the  strain  the  kinematics  and  magnitude  of  displacements
        main  implications  of  findings  in  the  light  of  existing  accommodated by structures of the southern Tyrrhenian
        models,  contrasting  extensional  versus  strike-slip  inter-  Sea margin.
        pretations.  An  original  model  for  the  structures  of  the  Recent  investigation  of  offshore  extensional  basins
        southern Tyrrhenian Sea margin follows.               through  detailed  seismic  profiles  has  provided  relevant
                                                              controls on the geometry of evolving normal fault systems
                                                              worldwide (e.g. the Viking Graben in the North Sea: see
        STRIKE-SLIP VS.  EXTENSIONAL INTERPRETATION OF THE
                                                              YOUNG et alii, 2001, and references therein). On the other
           STRUCTURES OF NORTHERN SICILY AND ADJACENT AREAS
                                                              hand, the kinematics of offshore structures cannot always
           The  southern  boundary  of  the  Tyrrhenian  Sea  has  be well defined in seismic profile images. The kinematics
        alternatively been interpreted as a passive, i.e. extensional  of some offshore structures whose along-strike continua-
        continental  margin  (KASTENS et  alii,  1988;  KASTENS &  tions are accessible to direct investigation inland, instead,
        MASCLE, 1990; SARTORI, 1990; PEPE et alii, 2000, among  can  easily  be  inferred  from  simple  fault  slip  analysis
        many others), or as a transform, i.e. strike-slip dominated  (e.g. see ROBERTS & HOLDSWORTH, 1999). The southern
        zone  (RÉHAULT et  alii,  1984;  GUEGUEN et  alii,  1998;  Tyrrhenian  Sea  margin  provides  a  further,  excellent
        LENTINI et alii, 2006). The reasons for these different inter-  example of how the kinematics of offshore structures may
        pretations may in part reflect differences in the analytical  be constrained by analysis of their exposed counterparts.
        approaches used. For example, the extensional model is  Based  on  interpretation  of  deep  seismic  reflection  pro-
        mainly derived from interpretation of deep seismic pro-  files, PEPE et alii (2000) recognised prominent EW trend-
        files (e.g; see PEPE et alii, 2000), whereas the strike-slip  ing, mainly N-dipping faults that affect a Meso-Cenozoic
        model largely relies on palaeogeographic reconstructions  substratum  and  overlying  Miocene  sediments.  These
        (e.g. see GUEGUEN et alii, 1998 and references therein). In  authors  inferred  a  dip-slip  kinematic  character  from
        the framework of this ongoing debate, the results of our  analysis of fault separation in the Meso-Cenozoic substra-
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