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A P-wave velocity model of the upper crust of the Sannio region (Southern Apennines, Italy)

1998-10, Iannaccone, G., Improta, L., Capuano, P., Zollo, A., Biella, G., De Franco, R., Deschamps, A., Cocco, M., Mirabile, L., Romeo, R., Iannaccone, G.; Osservatorio Vesuviano, Ercolano, Napoli, Italy, Improta, L.; Dipartimento di Scienze Fisiche, Universitá di Napoli, Capuano, P.; Osservatorio Vesuviano, Ercolano, Napoli, Italy, Zollo, A.; Dipartimento di Scienze Fisiche, Universitá di Napoli, Biella, G.; Istituto per le Ricerche sul Rischio Sismico, Milano, Italy, De Franco, R.; Istituto per le Ricerche sul Rischio Sismico, Milano, Italy, Deschamps, A.; Institut de Geodynamique, CNRS, Université de Nice, Sophia-Antipolis, France, Cocco, M.; Istituto Nazionale di Geofisica, Roma, Italy, Mirabile, L.; Istituto di Oceanologia, Istituto Universitario Navale, Napoli, Italy, Romeo, R.; Servizio Sismico Nazionale, Roma, Italy, Osservatorio Vesuviano, Ercolano, Napoli, Italy, Dipartimento di Scienze Fisiche, Universitá di Napoli, Osservatorio Vesuviano, Ercolano, Napoli, Italy, Dipartimento di Scienze Fisiche, Universitá di Napoli, Istituto per le Ricerche sul Rischio Sismico, Milano, Italy, Istituto per le Ricerche sul Rischio Sismico, Milano, Italy, Institut de Geodynamique, CNRS, Université de Nice, Sophia-Antipolis, France, Istituto Nazionale di Geofisica, Roma, Italy, Istituto di Oceanologia, Istituto Universitario Navale, Napoli, Italy, Servizio Sismico Nazionale, Roma, Italy

This paper describes the results of a seismic refraction profile conducted in October 1992 in the Sannio region, Southern Italy, to obtain a detailed P-wave velocity model of the upper crust. The profile, 75 km long, extended parallel to the Apenninic chain in a region frequently damaged in historical time by strong earthquakes. Six shots were fired at five sites and recorded by a number of seismic stations ranging from 41 to 71 with a spacing of 1-2 km along the recording line. We used a two-dimensional raytracing technique to model travel times and amplitudes of first and second arrivals. The obtained P-wave velocity model has a shallow structure with strong lateral variations in the southern portion of the profile. Near surface sediments of the Tertiary age are characterized by seismic velocities in the 3.0-4.1 km/s range. In the northern part of the profile these deposits overlie a layer with a velocity of 4.8 km/s that has been interpreted as a Mesozoic sedimentary succession. A high velocity body, corresponding to the limestones of the Western Carbonate Platform with a velocity of 6 km/s, characterizes the southernmost part of the profile at shallow depths. At a depth of about 4 km the model becomes laterally homogeneous showing a continuous layer with a thickness in the 3-4 km range and a velocity of 6 km/s corresponding to the Meso-Cenozoic limestone succession of the Apulia Carbonate Platform. This platform appears to be layered, as indicated by an increase in seismic velocity from 6 to 6.7 km/s at depths in the 6-8 km range, that has been interpreted as a lithological transition from limestones to Triassic dolomites and anhydrites of the Burano formation. A lower P-wave velocity of about 5.0-5.5 km/s is hypothesized at the bottom of the Apulia Platform at depths ranging from 10 km down to 12.5 km; these low velocities could be related to Permo-Triassic siliciclastic deposits of the Verrucano sequence drilled at the bottom of the Apulia Platform in the Apulia Foreland.

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Looking inside mt. vesuvius

1998, Gasparini, Paolo, Zollo, Aldo, Auger, Emanuel, Bobbio, Antonella, Emolo, Antonio, Frattini, M, Herrero, André, Iannaccone, Giovanni, Improta, Luigi, Nielsen, Stefan, Simini, S M, Achauer, U., Jordan, M., Chiarabba, Claudio, Ciaccio, Maria Grazia, Lucente, Francesco Pio, de Franco, Roberto, Biella, G., Del Pezzo, Edoardo, De Matteis, Raffaella, La Rocca, Mario, De Natale, Giuseppe, Capuano, Paolo, Godano, C., Martini, Marcello, Pingue, Folco, Troise, Claudia, Dietrich, M., Coutant, O., Moinet, F, Guerra, Ignazio, Kissling, Edi, Marsella, Ennio, Milana, Giuliano, Gorini, A., Marcucci, A, Zambonelli, E., Mirabile, L., Buonocore, Berardino, Nowack, R, Scarpa, Roberto, De Luca, G, Filippi, L., Solarino, Stefano, Eva, Elena, Virieux, J., Bertrand, Etienne, Charvis, P., Deschamps, Anne, Deverchere, J, Lomax, Anthony, Montelli, R, Bongiovanni, G, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#, #PLACEHOLDER_PARENT_METADATA_VALUE#

Italy's Mt.Vesuvius has been slumbering for a long time, but its silence could preface an eruption with potentially disastrous ef­fects for 600,000 people living on the vol­cano's slopes. To assess the scenario of the next eruption, the National Group of Vol-canology (GNV) of the Italian National Coun­cil of Researches (CNR) has fostered research aimed at mitigating eruption risk to the densely populated area. In this framework, researchers have gathered high-resolution seismic tomography data to better under­stand the internal structure of Mt. Vesuvius. The experiments were carried out during the last 4 years. The data will be used in three-dimen­sional modeling of the structure of Mt. Vesu­vius and underlying upper crust. Seismic velocities and attenuation and density con­trasts will be calculated, with special empha­sis on the delineation of significant magma reservoirs of more than 1 km in diameter. In modeling Mt. Vesuvius, tools are being devel­oped for using seismogram information to ob­tain high-quality seismic imaging of heterogeneous structures such as volcanoes

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2D seismic tomography of Somma- Vesuvius. Description of the experiment and preliminary results.

1996-05, Zollo, A., Gasparini, P., Biella, G., de Franco, R., Buonocore, B., Mirabile, L., De Natale, G., Milano, G., Pingue, F., Vilardo, G., Bruno, P. P., De Matteis, R., Le Meur, H., Iannaccone, G., Deschamps, A., Virieux, J., Nardi, A., Frepoli, A., Hunstad, I., Guerra, I., Zollo, A.; Dipartimento di Geofisica e Vulcanologia, Napoli, Italy, Gasparini, P.; Dipartimento di Geofisica e Vulcanologia, Napoli, Italy, Biella, G.; Istituto per lo Studio del Rischio Sismico, C.N.R., Milano, Italy, de Franco, R.; Istituto per lo Studio del Rischio Sismico, C.N.R., Milano, Italy, Buonocore, B.; Istituto di Oceanologia, Istituto Universitario Navale, Napoli, Italy, Mirabile, L.; Istituto di Oceanologia, Istituto Universitario Navale, Napoli, Italy, De Natale, G.; Osservatorio Vesuviano, Ercolano, Napoli, Italy, Milano, G.; Osservatorio Vesuviano, Ercolano, Napoli, Italy, Pingue, F.; Osservatorio Vesuviano, Ercolano, Napoli, Italy, Vilardo, G.; Osservatorio Vesuviano, Ercolano, Napoli, Italy, Bruno, P. P.; Dipartimento di Geofisica e Vulcanologia, Napoli, Italy, De Matteis, R.; Dipartimento di Geofisica e Vulcanologia, Napoli, Italy, Le Meur, H.; Dipartimento di Geofisica e Vulcanologia, Napoli, Italy, Iannaccone, G.; Dipartimento di Geofisica e Vulcanologia, Napoli, Italy, Deschamps, A.; Institut Geodynamique, CNRS, Sophia-Antipolis, France, Virieux, J.; Institut Geodynamique, CNRS, Sophia-Antipolis, France, Nardi, A.; Istituto Nazionale di Geofisica, Roma, Italy, Frepoli, A.; Istituto Nazionale di Geofisica, Roma, Italy, Hunstad, I.; Istituto Nazionale di Geofisica, Roma, Italy, Guerra, I.; Dipartimento di Scienze della Terra, Cosenza, Italy, Dipartimento di Geofisica e Vulcanologia, Napoli, Italy, Dipartimento di Geofisica e Vulcanologia, Napoli, Italy, Istituto per lo Studio del Rischio Sismico, C.N.R., Milano, Italy, Istituto per lo Studio del Rischio Sismico, C.N.R., Milano, Italy, Istituto di Oceanologia, Istituto Universitario Navale, Napoli, Italy, Istituto di Oceanologia, Istituto Universitario Navale, Napoli, Italy, Osservatorio Vesuviano, Ercolano, Napoli, Italy, Osservatorio Vesuviano, Ercolano, Napoli, Italy, Osservatorio Vesuviano, Ercolano, Napoli, Italy, Osservatorio Vesuviano, Ercolano, Napoli, Italy, Dipartimento di Geofisica e Vulcanologia, Napoli, Italy, Dipartimento di Geofisica e Vulcanologia, Napoli, Italy, Dipartimento di Geofisica e Vulcanologia, Napoli, Italy, Dipartimento di Geofisica e Vulcanologia, Napoli, Italy, Institut Geodynamique, CNRS, Sophia-Antipolis, France, Institut Geodynamique, CNRS, Sophia-Antipolis, France, Istituto Nazionale di Geofisica, Roma, Italy, Istituto Nazionale di Geofisica, Roma, Italy, Istituto Nazionale di Geofisica, Roma, Italy, Dipartimento di Scienze della Terra, Cosenza, Italy

A multidisciplinary project for the investigation of Mt. Vesuvius Structure was started in 1993. The core of the project is represented by a high resolution seismic tomography study by using controlled and natura1 sources. The main research objective is to investigate the feeding system of the vo1cano and to retrieve details of the upper crustal structure in the area. A first 2D using seismic experiment was performed in May 1994, with the aim of studing the feasibility of lIsing tomographic techniques for exploring the vo1cano interiors. Particularly, this experiment was designed to obtain information on the optimal sources-receivers configuration and on the depth extension of the volume sampled by shot-generated seismic waves. 66 three-component seismic stations and 16 single-component analogue instruments were installed by several Italian and French groups to record signals generated by three on-land, underground explosions. Sources and geophones were deployed along a 30-km NW-SE profile passing through the volcano crater. Receivers were placed at an average spacing of 250 m in the middle of the recording line and at 500 m outside. The arrival time data base was complemented by first P and S readings of micro earthquakes which occurred in the recent past within the volcano. The first arrival data set was preliminary used to determine the shallow structure of the volcano by applying Thurber's (1983) tomographic inversion technique. This analysis shows evidence for a high-velocity body which extends vertically from about 400 m below the crater down to at least 3000 m and for a shallow 300-500 m thick low-velocity cover which borders the edifice. Data from the distant shot show evidence for arrivals of deep reflected/converted phases and provide information on the deeper structure under the volcano. The results from the interpretation of 2D data are used for planning a 3D tomographic survey which will be cauied out in 1996.

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A study of local site effects in Benevento(Southern Italy) by the analysis of seismic records of explosions

1995-09, Iannaccone, G., Improta, L., Biella, G., Castellano, M., Deschamps, A., De Franco, R., Malagnini, L., Mirabile, L., Romeo, R., Zollo, A., Iannaccone, G.; Dipartimento di Geofisica e Vulcanologia, Università di Napoli, Italy, Improta, L.; Dipartimento di Geofisica e Vulcanologia, Università di Napoli, Italy, Biella, G.; Istituto per le Ricerche sul Rischio Sismico, Milano, Italy, Castellano, M.; Osservatorio Vesuviano, Ercolano, Napoli, Italy, Deschamps, A.; Institut de Geodynamique, C.N.R.S., Universite de Nice, Sophia-Antipolis, France, De Franco, R.; Istituto per le Ricerche sul Rischio Sismico, Milano, Italy, Malagnini, L.; Istituto Nazionale di Geofisica, Roma, Italy, Mirabile, L.; Istituto di Oceanologia, Istituto Universitario Navale, Napoli, Italy, Romeo, R.; Servizio Sismico Nazionale, Roma, Italy, Zollo, A.; Dipartimento di Geofisica e Vulcanologia, Università di Napoli, Italy, Dipartimento di Geofisica e Vulcanologia, Università di Napoli, Italy, Dipartimento di Geofisica e Vulcanologia, Università di Napoli, Italy, Istituto per le Ricerche sul Rischio Sismico, Milano, Italy, Osservatorio Vesuviano, Ercolano, Napoli, Italy, Institut de Geodynamique, C.N.R.S., Universite de Nice, Sophia-Antipolis, France, Istituto per le Ricerche sul Rischio Sismico, Milano, Italy, Istituto Nazionale di Geofisica, Roma, Italy, Istituto di Oceanologia, Istituto Universitario Navale, Napoli, Italy, Servizio Sismico Nazionale, Roma, Italy, Dipartimento di Geofisica e Vulcanologia, Università di Napoli, Italy

In this paper we evalllate the seismic amplification effects in the town of Benevento llsing records of an explo- sion of 500 kg fired at abollt 7 km. Seismic records were obtained at 43 selected sites in the city by digital three-component stations. A data selection performed on the signal-to-noise ratio reduced the available data to 26 stations. We used the spectral ratio techniques to evaluate the amplification effects of each recording site compared both to the average spectrum calculated over 26 stations and to a reference seismic station. The shapes of the spectral ratios were classified according to the geological characteristics of the site. A characteristic shape of the spectral ratio was observed to be related to the specific structure of the subsoil. In particular, the sites on basin sediments (Lagonegro Unit) and Middle Pleistocene conglomerates failed to show amplification effects; the sites on thick alluvial deposits showed amplification in the 5-9 Hz range; finally, sites on alluvial-lacustrine deposits amplified the seismic signal at frequencies depending on the characteristics and the thickness of the deposit. In addition, damage distribution caused by the 1688 earthquake in Benevento was related to the thickness of the surface layers in the ancient built-up area of the town. The study of the spectral ra- tios showed that these deposits amplify ground motion at frequencies between 9 and 12 Hz, i.e. frequencies close to the natural period of the most widespread buildings at that time in Benevento. Geological and seismic data were jointly used to carry out a zonation of the urban area of Benevento on the basis of homogeneous seismic responses. The validity of this analysis is limited to the main frequency band and amplitude of ground motion produced by the explosions.

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Caratterizzazione della risposta sismica nella città di Benevento.

1994-12, Iannaccone, G., Improta, L., Romeo, R., Biella, G., De Franco, R., Basili, A., Castellano, M., Deschamps, A., Iannaccone, G.; Università di Napoli "Federico II", Improta, L.; Università di Napoli "Federico II", Romeo, R.; Servizio Sismico Nazionale, Roma, Biella, G.; Istituto di Ricerca sul Rischio Sismico, CNR, Milano, De Franco, R.; Istituto di Ricerca sul Rischio Sismico, CNR, Milano, Basili, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia, Castellano, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia, Deschamps, A.; Institut de Géodynamique, Valbonne, Università di Napoli "Federico II", Università di Napoli "Federico II", Servizio Sismico Nazionale, Roma, Istituto di Ricerca sul Rischio Sismico, CNR, Milano, Istituto di Ricerca sul Rischio Sismico, CNR, Milano, Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia, Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia, Institut de Géodynamique, Valbonne

L'ampiezzà de1 moto del suolo, ed il suo contenuto in frequenza, alla súpeúcie della TerIa dípede dale caratte stiche della, sorgente sismica e dalle proprietà meccaniche del úezzo in cui si propagano le onde sismiche. In pa.rtico lare, gli strati pmssimi alla superficie possono modifrcare in modo sigdficativo il segnale sismlco. InJatti la presenza, di uno strato con un fo e contraato di im pedenza, spetto ad un basarnento sottostànte prÌò indurc etretti di risonanza alterando sensibilmente il livelo di anpiezza, il conterùto in Îrequenza e la, durata delle oscilla.zioni del suolo. Un esempio estîemo di questo fenomeno è stato evidenziatoi n occasiored el terremoto di Michoacan,M essico,d el 1985.Q uesto evento, pur essendo a-r.venuto ad alcune centinaia di chilometri da.lla capitale, ha, eccitato con il pe.iodo proprio di oscillnzioÈe( cilca 2 secondi)i depositi di riempimento di un antico lago prosciugato, su cui è costruita parte di Città, del Messico, pmvocaùdo iI crollo di nurerosi edifici e misliaia di morti (Singh et al., 1988