<?xml version="1.0" encoding="UTF-8"?>
<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns="http://purl.org/rss/1.0/" xmlns:slash="http://purl.org/rss/1.0/modules/slash/" xmlns:sy="http://purl.org/rss/1.0/modules/syndication/" xmlns:g-core="http://base.google.com/ns/1.0" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:taxo="http://purl.org/rss/1.0/modules/taxonomy/" xmlns:content="http://purl.org/rss/1.0/modules/content/">
  <channel rdf:about="http://hdl.handle.net/2122/254">
    <title>DSpace Collection:</title>
    <link>http://hdl.handle.net/2122/254</link>
    <description />
    <items>
      <rdf:Seq>
        <rdf:li resource="http://hdl.handle.net/2122/8669" />
        <rdf:li resource="http://hdl.handle.net/2122/8185" />
        <rdf:li resource="http://hdl.handle.net/2122/7104" />
        <rdf:li resource="http://hdl.handle.net/2122/5952" />
        <rdf:li resource="http://hdl.handle.net/2122/4704" />
        <rdf:li resource="http://hdl.handle.net/2122/3252" />
        <rdf:li resource="http://hdl.handle.net/2122/2695" />
        <rdf:li resource="http://hdl.handle.net/2122/2694" />
        <rdf:li resource="http://hdl.handle.net/2122/876" />
        <rdf:li resource="http://hdl.handle.net/2122/376" />
      </rdf:Seq>
    </items>
    <dc:date>2013-05-23T09:31:35Z</dc:date>
  </channel>
  <item rdf:about="http://hdl.handle.net/2122/8669">
    <title>Curie isotherm depth from aeromagnetic data constraining shallow heat source depths in the central Aeolian Ridge (Southern Tyrrhenian Sea, Italy)</title>
    <link>http://hdl.handle.net/2122/8669</link>
    <description>Title: Curie isotherm depth from aeromagnetic data constraining shallow heat source depths in the central Aeolian Ridge (Southern Tyrrhenian Sea, Italy)
Authors: De Ritis, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia; Ravat, D.; Department of Earth and Environmental Sciences, University of Kentucky; Ventura, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Chiappini, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia
Abstract: The Salina, Lipari, and Vulcano volcanic ridge&#xD;
and the surrounding sea sectors (Aeolian Archipelago,&#xD;
Southern Tyrrhenian Sea, Italy) are characterized by vents&#xD;
responsible for a recent (&lt;40 ka—1889/1890 AD) effusive&#xD;
and explosive subareal activity and repeated, 56 to 7 ka in&#xD;
age, submarine explosive eruptions from source areas located&#xD;
between Lipari and Vulcano. A spectral depth estimation of&#xD;
the magnetic bottom using a fractal method on aeromagnetic&#xD;
data from Vulcano, Lipari, and Salina volcanic ridge allows us&#xD;
to constrain the Curie isotherm depth. The elevated portion of&#xD;
the isotherm is between 2 and 3 km below Salina and Vulcano&#xD;
and about 1 km below Lipari. The Curie depth results in the&#xD;
context of other geological and geophysical evidence suggest&#xD;
that the rise of the Curie isotherm is mainly due to the&#xD;
occurrence of shallow heat sources such as magma ponds&#xD;
and associated hydrothermal systems. The short-wavelength&#xD;
magnetic anomaly field reflects magnetic contrasts from&#xD;
highly magnetized volcanic bodies, low-magnetization&#xD;
sediments, and hydrothermally altered rocks. Borehole temperature&#xD;
data verify the Curie temperature derived from the&#xD;
magnetic methods on the island of Vulcano.We conclude that&#xD;
the whole Vulcano, Lipari, and Salina volcanic ridge is active&#xD;
and should be monitored.</description>
    <dc:date>2013-03-19T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/8185">
    <title>Night Thermal Gradient: A New Potential Tool for Earthquake Precursors Studies. An Application to the Seismic Area of L'Aquila (Central Italy)</title>
    <link>http://hdl.handle.net/2122/8185</link>
    <description>Title: Night Thermal Gradient: A New Potential Tool for Earthquake Precursors Studies. An Application to the Seismic Area of L'Aquila (Central Italy)
Authors: Piroddi, L.; Università degli Studi di Cagliari; Ranieri, G.; Università degli Studi di Cagliari
Abstract: Relations between ground surface warming-up and earthquakes are presented by means of the analysis of thermal data detected by Meteosat satellite.  The analysis has been carried out on the basis of Land Surface Temperature  (LST) data, by the application of algorithms for two purposes: the reduction of the effect of cloud coverage and daily weather variability and the improvement in resolution of  thermal maps.&#xD;
The main case study has been L’Aquila earthquake on 6th April 2009 with two different observation timeframes: one in absence of significant seismic activity (October 2008), one right before and straight after the same earthquake (January-May 2009).&#xD;
The detected thermal anomalies reveal the possibility to associate surface thermal phenomena to the imminent manifestation of seismic events.
Description: The article shows a new algorithm for the processing of geostationary night data useful for environmental monitoring.  Application to thermal earthquake precursors studies is proposed with the case study of L'Aquila 2009 earthquake.</description>
    <dc:date>2012-01-31T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/7104">
    <title>Societal need for improved understanding of climate change, anthropogenic impacts, and geo-hazard warning drive development of ocean observatories in European Seas</title>
    <link>http://hdl.handle.net/2122/7104</link>
    <description>Title: Societal need for improved understanding of climate change, anthropogenic impacts, and geo-hazard warning drive development of ocean observatories in European Seas
Authors: Ruhl, H. A.; NOCS; Andrè, M.; UPC; Beranzoli, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia; Çagatay, M. N.; ITU; Colaço, A.; Univ. Azores; Cannat, M.; IPGP; Dañobeitia, J. J.; CSIC-UTM; Favali, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia; Géli, L.; IFREMER; Gillooly, M.; IMI; Greinert, J.; NIOZ; Hall, P. O. J.; Univ. Goteborg; Huber, R.; MARUM; Karstensen, J.; Univ. Kiel; Lampitt, R. S.; NOCS; Larkin, K. E.; NOCS; Lykousis, V.; HCMR; Mienert, J.; Univ. Tromsø; Miranda, J. M.; Univ. Lisboa; Person, R.; IFREMER; Priede, I. G.; Univ. Aberdeen; Puillat, I.; IFREMER; Thomsen, L.; Jacobs Univ. Bremen; Waldmann, C.; MARUM
Abstract: Society’s needs for a network of in situ ocean observing systems cross many areas of earth and marine&#xD;
science. Here we review the science themes that benefit from data supplied from ocean observatories.&#xD;
Understanding from existing studies is fragmented to the extent that it lacks the coherent long-term&#xD;
monitoring needed to address questions at the scales essential to understand climate change and&#xD;
improve geo-hazard early warning. Data sets from the deep sea are particularly rare with long-term data&#xD;
available from only a few locations worldwide. These science areas have impacts on societal health and&#xD;
well-being and our awareness of ocean function in a shifting climate.&#xD;
Substantial efforts are underway to realise a network of open-ocean observatories around European&#xD;
Seas that will operate over multiple decades. Some systems are already collecting high-resolution data&#xD;
from surface, water column, seafloor, and sub-seafloor sensors linked to shore by satellite or cable connection&#xD;
in real or near-real time, along with samples and other data collected in a delayed mode. We&#xD;
expect that such observatories will contribute to answering major ocean science questions including:&#xD;
How can monitoring of factors such as seismic activity, pore fluid chemistry and pressure, and gas&#xD;
hydrate stability improve seismic, slope failure, and tsunami warning? What aspects of physical oceanography,&#xD;
biogeochemical cycling, and ecosystems will be most sensitive to climatic and anthropogenic&#xD;
change? What are natural versus anthropogenic changes? Most fundamentally, how are marine processes&#xD;
that occur at differing scales related?&#xD;
The development of ocean observatories provides a substantial opportunity for ocean science to evolve&#xD;
in Europe. Here we also describe some basic attributes of network design. Observatory networks provide the means to coordinate and integrate the collection of standardised data capable of bridging measurement&#xD;
scales across a dispersed area in European Seas adding needed certainty to estimates of future oceanic&#xD;
conditions. Observatory data can be analysed along with other data such as those from satellites,&#xD;
drifting floats, autonomous underwater vehicles, model analysis, and the known distribution and abundances&#xD;
of marine fauna in order to address some of the questions posed above. Standardised methods for&#xD;
information management are also becoming established to ensure better accessibility and traceability of&#xD;
these data sets and ultimately to increase their use for societal benefit. The connection of ocean observatory&#xD;
effort into larger frameworks including the Global Earth Observation System of Systems (GEOSS) and&#xD;
the Global Monitoring of Environment and Security (GMES) is integral to its success. It is in a greater integrated&#xD;
framework that the full potential of the component systems will be realised.</description>
    <dc:date>2010-12-31T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/5952">
    <title>Physical-Mathematical modeling and numerical simulations of stress-strain state in seismic and volcanic regions</title>
    <link>http://hdl.handle.net/2122/5952</link>
    <description>Title: Physical-Mathematical modeling and numerical simulations of stress-strain state in seismic and volcanic regions
Authors: Scandura, Danila
Abstract: The strain-stress state generated by faulting or cracking and influenced by the strong heterogeneity of the internal earth structure precedes and accompanies volcanic and seismic activity. Particularly, volcanic eruptions are the culmination of long and complex geophysical processes and physical processes which involve the generation of magmas in the mantle or in the lower crust, its ascent to shallower levels, its storage and differentiation in shallow crustal chambers, and, finally, its eruption at the Earth’s surface. Instead, earthquakes are a frictional stick-slip instability arising along pre-existing faults within the brittle crust of the Earth. Long-term tectonic plate motion causes stress to accumulate around faults until the frictional strength of the fault is exceeded. &#xD;
The study of these processes has been traditionally carried out through different geological disciplines, such as petrology, structural geology, geochemistry or sedimentology. Nevertheless, during the last two decades, the development of physical of earth as well as the introduction of new powerful numerical techniques has progressively converted geophysics into a multidisciplinary science. Nowadays, scientists with very different background and expertises such as geologist, physicists, chemists, mathematicians and engineers work on geophysics. As any multidisciplinary field, it has been largely benefited from these collaborations. The different ways and procedures to face the study of volcanic and seismic phenomena do not exclude each other and should be regarded as complementary.&#xD;
Nowadays, numerical modeling in volcanology covers different pre-eruptive, eruptive and post-eruptive aspects of the general volcanic phenomena. Among these aspects, the pre-eruptive process, linked to the continuous monitoring, is of special interest because it contributes to evaluate the volcanic risk and it is crucial for hazard assessment, eruption prediction and risk mitigation at volcanic unrest.&#xD;
large faults. The knowledge of the actual activity state of these sites is not only an academic topic but it has crucial importance in terms of public security and eruption and earthquake forecast. &#xD;
However, numerical simulation of volcanic and seismic processes have been traditionally developed introducing several simplifications: homogeneous half-space, flat topography and elastic rheology. These simplified assumptions disregards effects caused by topography, presence of medium heterogeneity and anelastic rheology, while they could play an important role in Moreover, frictional sliding of a earthquake generates seismic waves that travel through the earth, causing major damage in places nearby to the modeling procedure&#xD;
This thesis presents mathematical modeling and numerical simulations of volcanic and seismic processes. The subject of major interest has been concerned on the developing of mathematical formulations to describe seismic and volcanic process. The interpretation of geophysical parameters requires numerical models and algorithms to define the optimal source parameters which justify observed variations. In this work we use the finite element method that allows the definition of real topography into the computational domain, medium heterogeneity inferred from seismic tomography study and the use of complex rheologies. Numerical forward method have been applied to obtain solutions of ground deformation expected during volcanic unrest and post-seismic phases, and an automated procedure for geodetic data inversion was proposed for evaluating slip distribution along surface rupture.</description>
    <dc:date>2008-12-31T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/4704">
    <title>RECONSTRUCTION OF POROSITY PROFILE IN AN OFFSHORE WELL</title>
    <link>http://hdl.handle.net/2122/4704</link>
    <description>Title: RECONSTRUCTION OF POROSITY PROFILE IN AN OFFSHORE WELL
Authors: Montegrossi, G.; CNR-IGG; Vaselli, O.; Dip. Sci. della Terra Firenze; Cantucci, B.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Quattrocchi, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia
Abstract: We presents the results of a new approach for the reconstruction of thermo-physical properties of deep well from the well log and  mineralogical analisys of the outcrops formation. This kind of procedure are generally new, and they are useful for creating the background data for reservoir engeneers and geochemist for modelling a well in order to asses its properties prior of re-opening the well itself for industrial use, such as CO2 sequestration. We used the temperature profile obtained from the well log and the bulk mineralogy analysed from the corresponding formation outcrops. The profile of thermal capacity and conductivity, and porosity and permeability as well, result well constrained and detaile for further use.</description>
    <dc:date>2008-09-23T22:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/3252">
    <title>Modeling of the thermal state of Mount Vesuvius from 1631 A.D. to present and the role of CO2 degassing on the volcanic conduit closure after the 1944 A.D. eruption</title>
    <link>http://hdl.handle.net/2122/3252</link>
    <description>Title: Modeling of the thermal state of Mount Vesuvius from 1631 A.D. to present and the role of CO2 degassing on the volcanic conduit closure after the 1944 A.D. eruption
Authors: Quareni, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italia; Moretti, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia; Piochi, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia; Chiodini, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia
Abstract: The last eruptive event at Mount Vesuvius occurred in 1944 A.D., ending a cycle&#xD;
of continuous eruptive activity started with the sub-Plinian event of 1631 A.D. The aim of&#xD;
this research is (1) to model the thermal evolution of the volcanic system from&#xD;
1631 A.D. up to the present and (2) to investigate the possible process leading the volcano&#xD;
to the current state of quiescence. A finite element software is employed to solve the&#xD;
time-dependent energy equation and obtain the thermal field in the volcanic edifice and&#xD;
the surrounding medium. Volcanological, petrological, and geophysical constraints are&#xD;
used to define the crustal structure beneath the volcanic edifice, the magma supply system&#xD;
active since 1631 A.D., and the physico-chemical conditions of magma. Thermodynamic&#xD;
properties of magma and wall rocks have been evaluated from well-established&#xD;
thermo-chemical compilations and data from the literature. It is shown that heat transfer&#xD;
due to magma degassing is required in addition to the heat conduction in order to obtain&#xD;
transient depth-temperature fields consistent with geochemical observations, high&#xD;
crustal magnetization, and rigid behavior of the shallow crust as indicated by geophysical&#xD;
data. Surface data of carbon dioxide soil flux coming out from the Mount Vesuvius crater&#xD;
are taken to constrain such an additional heat flux. The agreement between modeled&#xD;
and measured temperatures at the crater since 1944 A.D. proves the consistency of the&#xD;
model. It is concluded that the present state of quiescence of Mount Vesuvius is&#xD;
mostly a consequence of the absence of magma supply from the deep reservoir into the&#xD;
shallower system. This allows the cooling of residual magma left within the volcanic&#xD;
conduit and the transition from continuous eruptive activity to the condition of conduit&#xD;
obstruction. In this scenario, the hydrothermal system may have developed subsequent to&#xD;
the cooling of the magma within the conduit. Our findings are a direct consequence of the&#xD;
high concentration of CO2 in the most mafic Vesuvian magmas: The low solubility of&#xD;
CO2, with respect to H2O, enables a high mass flux of carbon dioxide through the volcanic&#xD;
edifice. The results of this study are relevant for hazard assessment at Vesuvius and&#xD;
indicate directions for further investigation, such as the role of the hydrothermal system on&#xD;
the thermal energy budget of the volcanic system and its relationships with fluids&#xD;
released by crustal structures likely to host the magmatic reservoir. In general, the role of&#xD;
the high concentration of carbon dioxide in magmas should be more questioned and&#xD;
investigated when studying the behavior of volcanic systems, particularly in south Italy&#xD;
volcanoes.</description>
    <dc:date>2007-02-28T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/2695">
    <title>Advances in the Prediction of Shear Events Induced From Mechanical Stimulation</title>
    <link>http://hdl.handle.net/2122/2695</link>
    <description>Title: Advances in the Prediction of Shear Events Induced From Mechanical Stimulation
Authors: Kohl, T.; Geowatt, Zurich, Switzerland; Mégel, T.; Geowatt, Zurich, Switzerland
Editors: Vinciguerra, Sergio; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Bernabé, Yves; MIT, USA
Abstract: see Abstract Volume</description>
    <dc:date>2007-09-24T22:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/2694">
    <title>Well path design and stimulation treatments at the geothermal research well GtGrSk4/05 in Groß Schönebeck</title>
    <link>http://hdl.handle.net/2122/2694</link>
    <description>Title: Well path design and stimulation treatments at the geothermal research well GtGrSk4/05 in Groß Schönebeck
Authors: Zimmermann, G.; GFZ, Potsdam, Germany; Reinicke, A.; GFZ, Potsdam, Germany; Blöcher, G.; GFZ, Potsdam, Germany; Milsch, H.; GFZ, Potsdam, Germany; Holl, H.-G.; GFZ, Potsdam, Germany; Moeck, I.; GFZ, Potsdam, Germany; Kranz, S.; GFZ, Potsdam, Germany; Brandt, W.; GFZ, Potsdam, Germany; Saadat, A.; GFZ, Potsdam, Germany; Huenges, E.; GFZ, Potsdam, Germany
Editors: Vinciguerra, Sergio; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Bernabé, Yves; MIT, USA
Abstract: see Abstract Volume</description>
    <dc:date>2007-09-24T22:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/876">
    <title>Heat and mass transfer from the mantle: heat flow and He-isotope constraints</title>
    <link>http://hdl.handle.net/2122/876</link>
    <description>Title: Heat and mass transfer from the mantle: heat flow and He-isotope constraints
Authors: Polyak, B. G.; Geological Institute, Russian Academy of Sciences, Moscow, Russia
Abstract: Terrestrial heat flow density, q, is inversely correlated with the age, t, of tectono-magmatic activity in the Earth's&#xD;
crust (Polyak and Smirnov, 1966; etc.). «Heat flow-age dependence» indicates unknown temporal heat sources in&#xD;
the interior considered a priori as the mantle-derived diapirs. The validity of this hypothesis is demonstrated by&#xD;
studying the helium isotope ratio, 3He/4He = R, in subsurface fluids. This study discovered the positive correlation&#xD;
between the regionally averaged (background) estimations of R- and q-values (Polyak et al., 1979a). Such a correlation&#xD;
manifests itself in both pan-regional scales (Norhtern Eurasia) and separate regions, e.g., Japan (Sano et al.,&#xD;
1982), Eger Graben (Polyak et al., 1985) Eastern China rifts (Du, 1992), Southern Italy (Italiano et al., 2000), and&#xD;
elsewhere. The R-q relation indicates a coupled heat and mass transfer from the mantle into the crust. From considerations&#xD;
of heat-mass budget this transfer can be provided by the flux consisting of silicate matter rather than He&#xD;
or other volatiles. This conclusion is confirmed by the correlation between 3He/ 4He and 87Sr/86Sr ratios in the products&#xD;
of the volcanic and hydrothermal activity in Italy (Polyak et al., 1979b; Parello et al., 2000) and other places.&#xD;
Migration of any substance through geotemperature field transports thermal energy accumulated within this substance,&#xD;
i.e. represents heat and mass transfer. Therefore, only the coupled analysis of both material and energy&#xD;
aspects of this transfer makes it possible to characterise the process adequately and to decipher an origin of terrestrial&#xD;
heat flow observed in upper parts of the earth crust. An attempt of such kind is made in this paper.</description>
    <dc:date>2004-12-31T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/376">
    <title>Active geodynamics of the central Mediterranean Sea: Tensional tectonic evidences in western Sicily from mantle-derived helium</title>
    <link>http://hdl.handle.net/2122/376</link>
    <description>Title: Active geodynamics of the central Mediterranean Sea: Tensional tectonic evidences in western Sicily from mantle-derived helium
Authors: Caracausi, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; Favara, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; Italiano, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; Nuccio, P. M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; Paonita, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; Rizzo, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia
Abstract: We report results on the measured high 3He/4He&#xD;
isotope ratio in western Sicily, interpreted together with the heat data. The study of this sector of the Europe-Africa interaction is crucial to a better understanding of the&#xD;
tectonics and the geodynamical evolution of the central Mediterranean area. The estimated mantle-derived helium fluxes in the investigated areas are up to 2–3 orders of magnitude greater than those of a stable continental area.&#xD;
The highest flux, found in the southernmost area near the Sicily Channel, where recent eruptions of the Ferdinandea Island occurred 20 miles out to sea off Sciacca, has been associated with a clear excess of heat flow. Our results indicate that there is an accumulation of magma below the&#xD;
continental crust of western Sicily that is possibly intruding and out-gassing through roughly N-S trending deep fault systems linked to the mantle, that have an extensional component. Although the identification of these faults is not&#xD;
sufficiently constrained by our data, they could possibly be linked to the pre-existing faults that originated during the Mesozoic extensional-transtensional tectonic phases.</description>
    <dc:date>2004-12-31T23:00:00Z</dc:date>
  </item>
</rdf:RDF>

