During the Eighties and the Nineties a lot of effort has been devoted by Academic Institutions to understand the geodynamic evolution of the continental margins of the South-western European block. Multichannel seismic data collected in this area (Sartori et al., 1994; Torelli et al., 1997: AR92 lines in Fig. 1) gave a new insight of the tectonic structure of the South-western Iberian margin. One of these seismic lines (AR-9210 in Fig. 1) shows a large compressive structure located offshore Cape San Vincente (Portugal), called Marquês de Pombal, whose motion probably caused the famous 1755 earthquake (Zitellini et al., 1999). Following this discovery the European Community funded the project BIGSETS (Big Sources of Earthquakes and Tsunami in SW Iberia) and an MCS survey (multichannel seismic survey) has been carried out to better investigate this structure (BIGSETS lines in Fig. 1).
The BIGSETS survey confirmed that the Marquês de Pombal is the likely source of the 1755 event (Zitellini et al., 2001). The deformed area, associated to the emplacement of Marquês de Pombal structure, is at least 100 km long, 5 km wide, the maximum up-lift is of about 1100 m and is located where the thrust fault emerges at the surface with a strike of N20E. The BIGSETS survey has shown that beside the Marquês the Pombal, other active, compressive, tectonic structures of regional significance are present: the Horseshoe fault (HSF), the Guadalquivir Bank (GB) and a large hill of tectonic origin (A) (Fig. 1). Besides the Marquês the Pombal structure the other above mentioned tectonic structures are poorly known and the VOLTAIRE campaign was designed to investigate them. This new set of data will point to a re-evaluation of the potential tsunami hazards in this very highly populated area and can constitute a firm basis both for more elaborated geodynamic models in the whole region and to assess seismic and tsunami risk associated with the largest events in Western Europe and North-western Africa.
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