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  • Articles  (5)
  • 04. Solid Earth::04.04. Geology::04.04.03. Geomorphology  (4)
  • 03. Hydrosphere::03.02. Hydrology::03.02.03. Groundwater processes
  • INGV  (3)
  • American Association for the Advancement of Science  (1)
  • Copernicus
  • 2010-2014  (5)
  • 1980-1984
  • 1965-1969
  • 1925-1929
Collection
  • Articles  (5)
Years
  • 2010-2014  (5)
  • 1980-1984
  • 1965-1969
  • 1925-1929
  • 2005-2009  (3)
Year
  • 1
    Publication Date: 2020-12-21
    Description: BREVIA
    Description: We report on the discovery in southern Egypt of an impact crater 45 m in diameter with a pristine rayed structure. Such pristine structures have been previously observed only on atmosphereless rocky or icy planetary bodies in the Solar System. This feature and the association with an iron meteorite impactor and shock metamorphism provides a unique picture of small-scale hypervelocity impacts on the Earth's crust. Contrary to current geophysical models, ground data indicate that iron meteorites with masses of the order of tens of tons can penetrate the atmosphere without significant fragmentation.
    Description: Published
    Description: 804
    Description: 1.8. Osservazioni di geofisica ambientale
    Description: 3.8. Geofisica per l'ambiente
    Description: JCR Journal
    Description: open
    Keywords: Impact crater ; Egypt ; geophysical exploration ; ataxite ; 04. Solid Earth::04.04. Geology::04.04.03. Geomorphology
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 2
    Publication Date: 2017-04-04
    Description: Etna volcano, Italy, hosts one of the major groundwater systems of the island of Sicily. Waters circulate within highly permeable fractured, mainly hawaiitic, volcanic rocks. Aquifers are limited downwards by the underlying impermeable sedimentary terrains. Thickness of the volcanic rocks generally does not exceed some 300 m, preventing the waters to reach great depths. This is faced by short travel times (years to tens of years) and low thermalisation of the Etnean groundwaters. Measured temperatures are, in fact, generally lower than 25 °C. But the huge annual meteoric recharge (about 0.97 kmˆ3) with a high actual infiltration coefficient (0.75) implies a great underground circulation. During their travel from the summit area to the periphery of the volcano, waters acquire magmatic heat together with volcanic gases and solutes through water-rock interaction processes. In the last 20 years the Etnean aquifers has been extensively studied. Their waters were analysed for dissolved major, minor and trace element, O, H, C, S, B, Sr and He isotopes, and dissolved gas composition. These data have been published in several articles. Here, after a summary of the obtained results, the estimation of the magmatic heat flux through the aquifer will be discussed. To calculate heat uptake during subsurface circulation, for each sampling point (spring, well or drainage gallery) the following data have been considered: flow rate, water temperature, and oxygen isotopic composition. The latter was used to calculate the mean recharge altitude through the measured local isotopic lapse rate. Mean recharge temperatures, weighted for rain amount throughout the year, were obtained from the local weather station network. Calculations were made for a representative number of sampling points (216) including all major issues and corresponding to a total water flow of about 0.315 kmˆ3/a, which is 40% of the effective meteoric recharge. Results gave a total energy output of about 140 MW/a the half of which is ascribable to only 13 sampling points. These correspond to the highest flow drainage galleries with fluxes ranging from 50 to 1000 l/s and wells with pumping rates from 70 to 250 l/s. Geographical distribution indicates that, like magmatic gas leakage, heat flow is influenced by structural features of the volcanic edifice. The major heat discharge through groundwater are all tightly connected either to the major regional tectonic systems or to the major volcanic rift zones along which the most important flank eruptions take place. But rift zones are much more important for heat upraise due to the frequent dikes injection than for gas escape because generally when dikes have been emplaced the structure is no more permeable to gases because it becomes sealed by the cooling magma.
    Description: Published
    Description: Vienna, Austria
    Description: 1.2. TTC - Sorveglianza geochimica delle aree vulcaniche attive
    Description: open
    Keywords: groundwaters ; volcanic surveillance ; water chemistry ; dissolved gases ; 03. Hydrosphere::03.02. Hydrology::03.02.03. Groundwater processes ; 03. Hydrosphere::03.02. Hydrology::03.02.04. Measurements and monitoring ; 03. Hydrosphere::03.04. Chemical and biological::03.04.03. Chemistry of waters ; 03. Hydrosphere::03.04. Chemical and biological::03.04.05. Gases ; 03. Hydrosphere::03.04. Chemical and biological::03.04.06. Hydrothermal systems
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Oral presentation
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  • 3
    Publication Date: 2017-04-04
    Description: Vivere in un territorio vulcanico, fronteggiare giorno dopo giorno il pericolo che un’eruzione possa, nel volgere di poche ore, distruggere il lavoro di una vita intera e con esso la vita stessa, è una sfida che l’uomo continua ad accettare sin dagli albori della civiltà....
    Description: Published
    Description: 7-8
    Description: 3.5. Geologia e storia dei vulcani ed evoluzione dei magmi
    Description: N/A or not JCR
    Description: open
    Keywords: AIQUA 2013 ; eruzioni vulcaniche ; impatto sul territorio ; 04. Solid Earth::04.04. Geology::04.04.99. General or miscellaneous ; 04. Solid Earth::04.04. Geology::04.04.03. Geomorphology
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 4
    Publication Date: 2017-04-04
    Description: Gli studi archeologici e vulcanologici condotti nell’area napoletana, hanno evidenziato che le eruzioni del Somma-Vesuvio e della caldera dei Campi Flegrei hanno fortemente condizionato lo sviluppo e il declino degli insediamenti umani in quest’area sin dalla Preistoria [Laforgia et al., 2009; Di Lorenzo et al., 2013; Di Vito et al., 2013]. La lunga storia dell’interazione tra uomo e vulcano è dettagliatamente registrata nella stratigrafia della Piana Campana, dove gli studi condotti in concomitanza con l’esecuzione di indagini sistematiche o preventive ad opere pubbliche, hanno contribuito a definire il quadro degli insediamenti e delle attività umane tra il Tardo Neolitico e l’epoca storica attorno ai vulcani napoletani [Marzocchella, 2000; Albore Livadie et al., 2005; Laforgia et al., 2009]. Durante questo periodo di tempo la Piana Campana (Fig. 1) è stata intensamente frequentata, attraversata da vie di comunicazione di lunga persistenza temporale e soggetta a consistente sfruttamento agricolo. Le eruzioni vulcaniche del Vesuvio e dei Campi Flegrei hanno spesso determinato lunghi intervalli nella frequentazione di queste aree, ma hanno altresì contribuito alla straordinaria fertilità dei suoli, favorendone lo sfruttamento agricolo.Di seguito si riporta un esempio, di recente pubblicazione [Di Vito et al., 2013], di come l’approccio integrato geologico-archeologico abbia permesso di ricostruire l’evoluzione del territorio intorno al Vesuvio in un periodo di tempo tanto interessante quanto poco conosciuto, compreso tra l’eruzione pliniana delle Pomici di Avellino e quella sub-pliniana del 472 d.C. L’area è stata infatti interessata dalla deposizione dei prodotti di numerose eruzioni vulcaniche caratterizzate da diversa energia, effetti e durata; inoltre,l’accumulo lungo i versanti dei rilievi attorno alle piane vesuviane di grandi quantità di materiale piroclastico sciolto, depositato rapidamente nel corso delle eruzioni, ha favorito nel tempo la generazione di lahar, e di ripetuti episodi di alluvionamento che hanno frequentemente causato l’impaludamento e il seppellimento delle piane sotto spesse coltri detritiche [Di Vito et al., 1998; Zanchetta et al., 2004]. Nonostante ciò, l’area a nord-est del vulcano corrispondente al territorio di Nola, contraddistinta da un’eccellente posizione geografica e attraversata da importanti vie naturali di collegamento tra le aree interne irpine e beneventane e la costa tirrenica, ha partecipato a tutti gli stadi del popolamento umano, con l’avvicendarsi di genti alla ricerca continua di terreni fertili e risorse naturali dalle quali trarre il proprio sostentamento. In questo territorio l’uomo ha sempre trovato vantaggioso stabilire i suoi insediamenti, probabilmente grazie alla grande fertilità del suolo e alle favorevoli condizioni climatiche, ma anche in virtù dei lunghi intervalli di quiescenza tra le varie eruzioni, che generalmente hanno superato il tempo di una vita umana.
    Description: Published
    Description: 9-13
    Description: 3.5. Geologia e storia dei vulcani ed evoluzione dei magmi
    Description: 3.10. Storia ed archeologia applicate alle Scienze della Terra
    Description: N/A or not JCR
    Description: open
    Keywords: eruzioni vulcaniche ; Campania ; interazione tra uomo e vulcano ; 04. Solid Earth::04.04. Geology::04.04.99. General or miscellaneous ; 04. Solid Earth::04.04. Geology::04.04.03. Geomorphology
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 5
    Publication Date: 2021-12-16
    Description: Sand boils, which are also known as sand blows or sand volcanoes, are among the most common superficial effects induced by high-magnitude earthquakes. These generally occur in or close to alluvial plains when a strong earthquake (M 〉5) strikes on a lens of saturated and unconsolidated sand deposits that are constrained between silt-clay layers [Ambraseys 1988, Carter and Seed 1988, Galli 2000, Tuttle 2001, Obermeier et al. 2005], where the sediments are converted into a fluid suspension. The liquefaction phenomena requires the presence of saturated and uncompacted sand, and a groundwater table near the ground surface. This geological– geomorphological setting is common and widespread for the Po Plain (Italy) [Castiglioni et al. 1997]. The Po Plain (ca. 46,000 km2) represents 15% of the Italian territory. It hosts a population of about 20 million people (mean density of 450 people/km2) and many infrastructures. Thus, the Po Plain is an area of high vulnerability when considering the liquefaction potential in the case of a strong earthquake. Despite the potential, such phenomena are rarely observed in northern Italy [Cavallin et al. 1977, Galli 2000], because strong earthquakes are not frequent in this region; e.g., historical data report soil liquefaction near Ferrara in 1570 (M 5.3) and in Argenta 1624 (M 5.5) [Prestininzi and Romeo 2000, Galli 2000]. In the Emilia quakes of May 20 and 29, 2012, the most widespread coseismic effects were soil liquefaction and ground cracks, which occurred over wide areas in the Provinces of Modena, Ferrara, Bologna, Reggio Emilia and Mantova (Figure 1). These were the causes of considerable damage to buildings and the infrastructure. The soil liquefaction and ground cracks were accompanied by sand boils, which are described in this report. The spatial distribution and geomorphological setting of sand boils and ground cracks are also described here. A detailed three-dimensional (3D) reconstruction of these features is also presented, which was carried out using terrestrial photogrammetry. Since archeological times, fluvial ridges, and in general sandy deposits on low plains have been the preferred sites for human infrastructure, colonial houses, roads, etc. Therefore, it is very important to understand how the local topography/ morphology interacts in the liquefaction processes. Numerous distinctive seismic landforms were generated by the May 2012 strong earthquakes (seven with M 〉5), and in particular, sand boils and ground fractures. The sand-boil landforms, also known as sand craters or sand volcanoes, are formed by low mounds of sand that have been extruded from fractures [Tuttle 2001]. The cone is a generally shortlived structure that naturally collapses, starting from the center holes that mark the water retreat back into the fracture. Sand boils also occurred along larger cracks (with decimetric lateral and vertical displacements). Here, the upper scarps block the formation of craters and allow the deposition of a sandy layer several centimeters thick (e.g. ca. 4 cm in the San Carlo crack), on the lower side of the steep slope. These landforms are highly vulnerable to erosion. After a few weeks, they are washed out by rain, destroyed by human activity, or masked by growing crops. Thus, ground surveys that investigate these events have to be carried out as soon as possible [Panizza et al. 1981]. In this report, we present preliminary results using methods to map the detailed micro-morphology of some representative liquefaction features (Figure 2) that normally disappear for the aforementioned reasons, or that are recorded only in qualitative terms.
    Description: Published
    Description: 727-733
    Description: 4.4. Scenari e mitigazione del rischio ambientale
    Description: JCR Journal
    Description: open
    Keywords: Sand boils, Digital elevation model, Liquefaction ; 04. Solid Earth::04.04. Geology::04.04.03. Geomorphology
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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