25.01.2015 Views

IASPEI - Picture Gallery

IASPEI - Picture Gallery

IASPEI - Picture Gallery

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

IUGG XXIV General Assembly July 2-13, 2007 Perugia, Italy<br />

(S) - <strong>IASPEI</strong> - International Association of Seismology and Physics of the Earth's<br />

Interior<br />

JSS002 Poster presentation 1822<br />

Constraints on the source of the 20th February 1743 tsunamigenic<br />

earthquake in Apulia, Italy, from numerical tsunami modelling and<br />

geological evidences<br />

Dr. Alberto Armigliato<br />

Dipartimento di Fisica, Settore Geofisica Universita di Bologna <strong>IASPEI</strong><br />

Stefano Tinti, Giuseppe Mastronuzzi, Paolo Sans, Gianluca Pagnoni<br />

According to the most recent version of the Italian Tsunami Catalogue, the 20th February 1743 tsunami<br />

was generated by a strong earthquake (M=6.9) which severely hit the Salento peninsula (Apulia) and<br />

the Greek Ionian Islands, and that was felt in a very large area, including Calabria, the Messina Straits<br />

and Naples. The maximum damage due to the earthquake was suffered by the towns of Nard and<br />

Francavilla Fontana in southern Apulia, where most buildings were ruined. The cities of Taranto and<br />

Brindisi were also heavily damaged. The earthquake was responsible for more than 160 victims.<br />

Historical accounts on the tsunami are scarce: the only available report describes some tsunami effects<br />

in the harbour of Brindisi, where the sea withdrew. On the other hand, the impact of the tsunami waves<br />

along the Ionian and Adriatic coasts of Apulia appears to be well documented from the geological point<br />

of view. A recent detailed study on large boulder accumulations along the southern Apulia coasts and on<br />

their depositional characteristics allowed not only to put them in relation to the 1743 event with a<br />

reasonable degree of confidence, but also to formulate some hypotheses on the possible source area<br />

(SSE of Apulia), on the direction of impact of the tsunami waves and on the highest tsunami runup (11<br />

m). Based on these results and on some basic information coming from local tectonics, we take into<br />

account a small number of seismic sources and for each of them we simulate numerically the ensuing<br />

tsunami. More specifically, for each studied fault we compute the coseismic deformation of the sea<br />

bottom and take it to be identical to the tsunami initial condition. The subsequent tsunami wave<br />

propagation is computed by means of a finite-element numerical code, UBO-TSUFE, developed at the<br />

Department of Physics of the University of Bologna, which implements and solves the Navier-Stokes<br />

equations in the shallow-water approximation. For each run, we compare the numerical results with the<br />

available geological and historical evidences: attention is posed especially on the tsunami wave<br />

propagation direction, on the polarity of the first wave arrivals in some selected coastal stations in<br />

southern Apulia and on the spatial distribution of the extreme water elevations along the coastlines. The<br />

results are discussed in order to draw some preliminary conclusions on the most probable source area<br />

and geometry for the 1743 tsunamigenic earthquake.<br />

Keywords: apulia, numerical modelling, tsunami deposits

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!