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  5. High frequency strong ground motion modelling in the Catania area associated to the Ibleo-Maltese fault system
 
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High frequency strong ground motion modelling in the Catania area associated to the Ibleo-Maltese fault system

Author(s)
Zollo, A.  
Dipartimento di Scienze Fisiche, Università di Napoli, Napoli, Italy  
Emolo, A.  
Dipartimento di Scienze Fisiche, Università di Napoli, Napoli, Italy  
Herrero, A.  
Dipartimento di Scienze Fisiche, Università di Napoli, Napoli, Italy  
Improta, L.  
Dipartimento di Scienze Fisiche, Università di Napoli, Napoli, Italy  
Language
English
Status
Published
Peer review journal
Yes
Journal
Journal of Seismology  
Issue/vol(year)
3(3)
Pages (printed)
279-288
Date Issued
March 11, 1999
URI
https://www.earth-prints.org/handle/2122/2026
Subjects
04. Solid Earth::04.06. Seismology::04.06.04. Ground motion  
Subjects

complex source models...

Abstract
A hybrid statistical-deterministic approach has been applied to estimate strong ground motion parameters (PGA, spectral ordinates) in South-Eastern Sicily for a M = 7 earthquake. A number of 100 different rupture processes has been simulated along a composite fault system representing two segments of the Ibleo-Maltese fault scarp. Map at regional scale of mean PGA in the 0.5–20 Hz frequency band shows highest values (0.4–0.5 g) nearby and North of Catania, due to a dominant directivity effect. The COV parameter, which expresses the variability of PGA values as a function of source complexity, is higher in the region nearby and South of the town of Augusta, where, depending on the rupture history, rather large PGA values can be observed (> 0:4 g). PGA attenuation curves suggest that an azimuthal variation could be related to the source extent and directivity. The response and pseudo acceleration spectra are computed for different sites in the town of Catania including an approximate 1D site response. Ground motion amplification effects at high frequency (5–20 Hz) are produced by thin shallow layer of soft clay, loose pyroclastites and fill. We observe small amplification effects, in the frequency ranges 2–3 Hz and 5–10 Hz, in sites where recent alluvia reach a thickness of some tens of meters. Otherwise, sites located on outcrops of massive lavas show moderate attenuation
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rome library|catania library|milano library|napoli library|pisa library|palermo library
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