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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Pure and applied geophysics 151 (1998), S. 495-502 
    ISSN: 1420-9136
    Keywords: Key words: Seismic anisotropy, Pn waves, northern Apennines.
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract—Pn travel times recorded by the stations of the Italian seismic network have been used to image the azimuthal variations of seismic velocity in the uppermost mantle beneath the northern part of the Apennine chain. The azimuthal variation of Pn velocity is interpreted here in terms of seismic anisotropy. We have found that about 5% anisotropy characterizes the uppermost mantle of the studied area, and that the fastest direction of Pn follows the arcuate trend of the chain. This suggests that seismic anisotropy is strongly related to the tectonic regime that originated the northern Apennine arc.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2017-04-04
    Description: A geomorphologic survey was performed along the shoreline extending for about 3 km between the beache of Santa Maria del Focallo and Porto Ulisse, on the southeastern coast of Sicily. The study area belongs to the territory of Ispica, within the Ragusa province. This area is characterized by anthropic activities due to the agricultural and turistic use of the territory. Here the coastline is featured by cliffs made of calcarenitic breccia and sandy levels with Strombus coronatus (Upper Pliocene). The maximum elevation of the cliffs is 12 m a.s.l.. At the base of the cliffs are a number of caves caused by marine erosion. This process causes rockfalling and the formation of small, short-living sandy beaches. Further, the presence of several stacks is evidence of a progressive and fast coastline retreat. An interesting phenomenon can be observed at the artificial harbour of Punta Cirica, where marine erosion has excavated small caves along pre-existing fault planes. In some of these caves the partial collapse of the roof has caused the formation of sink holes.
    Description: Unpublished
    Description: Rimini, Italia
    Description: open
    Keywords: geomorphology ; Ispica ; 05. General::05.03. Educational, History of Science, Public Issues::05.03.99. General or miscellaneous
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Poster session
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  • 3
    Publication Date: 2017-04-04
    Description: We have studied four mud volcano fields located in eastern Sicily, around the Mt. Etna edifice. Three of them are located on the southern flank of Etna, between the Paternò and Belpasso villages and, based of their location, are named “Salinelle dei Cappuccini”, “Salinelle del Fiume” and “Salinelle del Vallone Salato”. Their genesis is connected with a structural trap formed by a brachyanticline of Pleistocene clays that form the Etna basement. The fourth one is located on the farest north-eastern part of Etna, along the Ionian coastline, and it is named “Salsa di Fondachello” after the name of the closest village. Geologic surveys and drilling data allow us to say that in “Salinelle dei Cappuccini” and “Salinelle del Fiume” fluids uprise through pre-existing volcanic necks, while in “Salinelle del Vallone Salato” fluids presumably uprise through a fault plane. The morphological evolution of these mud volcano fields depends mainly on the density of the emitted muds and secondarily on preexisting features of the ground surface. Chemical analyses revealed that the water coming out from the mud volcanoes is a fossil marine water hosted in the Miocene sedimentary rocks of the Mt. Etna basement. CO2 is the most abundant escaping gas, and it is mainly of magmatic origin: its amount and rate could be related to movements of the deep Etna magma. The activity of the “Salsa di Fondachello” mud volcano started on January 11th, 1693, associated with the destructive Val di Noto earthquake. The mud volcano was again active from 1795 to 1832. At the end of its last activity, started in March 1847, an earthquake occurred and the mud volcano collapsed. Today only a weak methane emission is evidence of endogenous activity.
    Description: Unpublished
    Description: Rimini, Italia
    Description: open
    Keywords: mud volcanoes ; Etna ; 05. General::05.03. Educational, History of Science, Public Issues::05.03.99. General or miscellaneous
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Poster session
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  • 4
    Publication Date: 2017-04-04
    Description: Mount Etna is the largest active volcano of Europe and the highest mountain (about 3,330 m a.s.l.) of peninsular and insular Italy; moreover, during the Last Glacial Maximum (LGM, 25,000 ÷ 14,000 years BP) it was some hundreds meters higher than today. Since other mountains of the Apennines were covered by glaciers during the Upper Pleistocene, several authors hypothesized that a glacial cover could have been also present on Mount Etna during the LGM, being the estimated limit of perpetual snow around 2,500 m a.s.l. at that time and latitude. We have carried out a morphological survey in a portion of the volcanic edifice where rocks older than the LGM outcrop. This portion includes Punta Lucia, on the NW slope, and Serra delle Concazze, on the NE slope. Along the upper part of the northeastern slope of Etna we have found a small valley, about 170 m long, 15 m wide and 7 m deep, characterized by a clear U-shaped section, that we interpreted to be of glacial origin. The search for moraine deposits that could be ascribed to the activity of the hypothesized glacier was unsuccessful so far and is also complicated by the presence of vegetation and recent lava and tephra deposits covering the volcano flanks. We are aware that this valley should be considered as a possible geomorphosite to guarantee its preservation and further study.
    Description: Submitted
    Description: Paris, France
    Description: open
    Keywords: glacial morphology ; geomorphosite ; Mt Etna volcano ; 05. General::05.03. Educational, History of Science, Public Issues::05.03.99. General or miscellaneous
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Extended abstract
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  • 5
    Publication Date: 2017-04-04
    Description: Geosites are valuable natural resources of a territory and represent the geologic heritage of a region. In southeastern Sicily several localities in the Ragusa area can be considered and exploited as possible geosites. The area that we propose in this study belongs to the calcareous Hyblean foreland that is part of the Pelagian block, in turn belonging to the northern continental margin of the African plate. The neogenic units of the Apennine-Maghrebide orogen are thrusted onto the Hyblean foreland from the north, while to the east the Hyblean foreland is bounded by the Hyblean-Maltese Escarpment toward the Ionian Sea. Among the active tectonic structures of the study area is the Ispica normal fault system that displaces the sector to the east by 80-100 m, forming the depression of Ispica-Capo Passero. The Ispica area is characterized by deep gorges, locally called “cave”, which origin is due to fluvio-karstic processes that acted along pre-existing structural discontinuities. In this work we describe in particular the Cava d’Ispica, a 13-km long valley extending in the NW-SE direction within the territory of Modica, Ispica and Rosolini. It is an area of relevant interest both for the beauty of the landscape and for its historical and archaeological importance. Inside the Cava d’Ispica is a number of caves of different size where the first inhabitants of the area used to live (the first settlings are dated 2000 b.C.). These caves also hosted the Sicilians escaping from the nearby coastal areas after the arrival of the Greek settlers. In the IV-V centuries hundreds of these caves were used as a cemetery complex, while during the barbaric invasions and the following Byzantin age (VI-IX centuries) they were mostly utilized by local people as shelters. At the entrance of the valley is the archeologic park called “Parco della Forza”, whose name derives from the latin word “Fortilitium” because of the presence of a fortress. In the northern part of the park is the unique and spectacular Centoscale, a well carved in the calcareous rock that, with its 250 steps, reaches the bottom of the valley located 60 m below. In 1972 the Soprintendenza ai Beni Culturali started an excavation in the Cava d’Ispica area and the archaeological findings are now exhibited within the Antiquarium museum of the park.
    Description: Unpublished
    Description: Rimini, Italia
    Description: 1.8. Osservazioni di geofisica ambientale
    Description: open
    Keywords: geosite ; Cava d'Ispica ; Ragusa ; 05. General::05.03. Educational, History of Science, Public Issues::05.03.99. General or miscellaneous
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Conference paper
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