Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/2445
AuthorsCultrera, G.* 
Rovelli, A.* 
Mele, G.* 
Azzara, R.* 
Caserta, A.* 
Marra, F.* 
TitleAzimuth-dependent amplification of weak and strong ground motions within a fault zone (Nocera Umbra, central Italy)
Issue Date2003
Series/Report no./108 (2003)
DOI10.1029/2002JB001929
URIhttp://hdl.handle.net/2122/2445
Keywordssite effects
fault zone
Subject Classification04. Solid Earth::04.06. Seismology::04.06.04. Ground motion 
AbstractDuring three moderate-magnitude earthquakes occurred in September–October 1997 in the central Apennines, Italy, accelerations larger than 0.5 g were recorded in the town of Nocera Umbra, 10 to 15 km N-NW of the epicenters. The accelerograph is sited in a fault zone, close to a N30 E tectonic contact. Six temporary seismological stations installed across the fault recorded 82 aftershocks occurred in two seismogenic zones: the Colfiorito-Sellano area, S-SE of the array, and the Gualdo Tadino area, to the north. The array data reveal large variations in terms of both peak ground motions and spectral amplitudes. Within the fault zone, amplifications show a strong dependence on the source azimuth. At the accelerograph site, the effects are particularly large for events from S-SE: peak ground motions are a factor of 14 larger than those of a reference site and conventional spectral ratios attain amplitudes as large as 50 at 7 Hz along the N30 E direction of motion, parallel to the strike of the fault. Nineteen strong motion accelerograms were then used to compare ground motion properties between weak and strong events up to M0 = 1.2 1025 dyn cm. A particle motion analysis shows that the directional effect is also present in the strongest motions, even though the amplification of peak ground motion decreases when M0 increases. Results from stochastic simulations indicate that such a behavior is not due to nonlinearity: applying the empirical weak motion transfer functions in a purely linear model the observed peak ground motions of the largest events are fit satisfactorily.
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