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        <rdf:li resource="http://hdl.handle.net/2122/8511" />
        <rdf:li resource="http://hdl.handle.net/2122/8510" />
        <rdf:li resource="http://hdl.handle.net/2122/8478" />
        <rdf:li resource="http://hdl.handle.net/2122/8469" />
        <rdf:li resource="http://hdl.handle.net/2122/8455" />
        <rdf:li resource="http://hdl.handle.net/2122/8335" />
        <rdf:li resource="http://hdl.handle.net/2122/8328" />
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    <dc:date>2013-05-21T12:54:44Z</dc:date>
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  <item rdf:about="http://hdl.handle.net/2122/8691">
    <title>Intersection of exogenous, endogenous and anthropogenic factors in the Holocene landscape: A study of the Naples coastline during the last 6000 years</title>
    <link>http://hdl.handle.net/2122/8691</link>
    <description>Title: Intersection of exogenous, endogenous and anthropogenic factors in the Holocene landscape: A study of the Naples coastline during the last 6000 years
Authors: Romano, P.; Dipartimento di Scienze della Terra, dell’Ambiente e delle Risorse, Università di Napoli Federico II, Largo S. Marcellino 10, 80138 Naples, Italy; Di Vito, M. A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia; Giampaola, D.; Soprintendenza Speciale ai Beni Archeologici di Napoli e Pompei, Museo Archeologico Nazionale, Naples, Italy; Cinque, A.; Dipartimento di Scienze della Terra, dell’Ambiente e delle Risorse, Università di Napoli Federico II, Largo S. Marcellino 10, 80138 Naples, Italy; Bartoli, C.; Soprintendenza Speciale ai Beni Archeologici di Napoli e Pompei, Museo Archeologico Nazionale, Naples, Italy; Boenzi, G.; Soprintendenza Speciale ai Beni Archeologici di Napoli e Pompei, Museo Archeologico Nazionale, Naples, Italy; Detta, F.; Dipartimento di Scienze della Terra, dell’Ambiente e delle Risorse, Università di Napoli Federico II, Largo S. Marcellino 10, 80138 Naples, Italy; Di Marco, M.; Soprintendenza Speciale ai Beni Archeologici di Napoli e Pompei, Museo Archeologico Nazionale, Naples, Italy; Giglio, M.; Soprintendenza Speciale ai Beni Archeologici di Napoli e Pompei, Museo Archeologico Nazionale, Naples, Italy; Iodice, S.; Soprintendenza Speciale ai Beni Archeologici di Napoli e Pompei, Museo Archeologico Nazionale, Naples, Italy; Liuzza, V.; Dipartimento di Scienze della Terra, dell’Ambiente e delle Risorse, Università di Napoli Federico II, Largo S. Marcellino 10, 80138 Naples, Italy; Ruello, M. R.; Dipartimento di Scienze della Terra, dell’Ambiente e delle Risorse, Università di Napoli Federico II, Largo S. Marcellino 10, 80138 Naples, Italy; Schiano di Cola, C.; Soprintendenza Speciale ai Beni Archeologici di Napoli e Pompei, Museo Archeologico Nazionale, Naples, Italy
Abstract: New data on the ancient landscape of Naples (southern Italy) during the middle and late Holocene from&#xD;
geo-archaeological excavations associated with public transport works were used to reconstruct the hill&#xD;
and coastal environment to the west of the ancient Graeco-Roman polis, where remains of human settlements&#xD;
date to the late Neolithic. The rich stratigraphic and archaeological records that emerged from&#xD;
the digs and from previous boreholes were measured and analysed by combining sedimentary facies&#xD;
analysis, tephrostratigraphy and archaeological data. Between the 5th and 4th millennia BP, a rocky&#xD;
profile with a wave-cut platform cutting across pyroclastites emplaced from the surrounding volcanoes&#xD;
was predominant in the coastal landscape. During the 3rd millennium BP, this rocky coast was progressively&#xD;
replaced by a sandy littoral environment primarily due to marine deposition, with a coastline&#xD;
located some hundred meters inland with respect to the modern one. The sedimentary record of the&#xD;
Greek and Roman periods indicates short-term fluctuations of the coastline, leading to the establishment&#xD;
of a backshore environment towards the end of the 6th century AD, when prograding river mouths and&#xD;
lobes of debris flows contributed to the advancing trend of the shoreline. The frequent archaeological&#xD;
remains from these periods indicate a stable settled area since Roman times. The shoreline was still&#xD;
subject to short-lived fluctuations between the 12th and 16th centuries, and attained its present position&#xD;
during the modern era with man-made reshaping of its profile. The construction of Relative Sea Level&#xD;
curves for two coastal sites reveals that the persistence of the foreshore environment in the Naples&#xD;
coastal strip during the 5th and 4th millennia BP was controlled by the counterbalancing effect of either&#xD;
the concurrent eustatic sea level rise or subsidence. On the other hand, the morpho-stratigraphic record&#xD;
for the last two millennia shows a significant correlation between sedimentation rate and settlement&#xD;
history, accounting for the dominant role of the anthropogenic forcing-factor in late Holocene landscape&#xD;
history. In particular, land mismanagement during Late Antiquity seems to have triggered a slope&#xD;
disequilibrium phase, exacerbating soil erosion and increasing the sediment accumulation rate in both&#xD;
foothill and coastal areas. Nonetheless, the environmental changes of the Chiaia coast during the last&#xD;
2000 years clearly show volcanicetectonic perturbations influencing coastline development up to the&#xD;
modern era.</description>
    <dc:date>2012-12-31T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/8511">
    <title>Human colonization and volcanic activity in the eastern Campania Plain (Italy) between the Eneolithic and Late Roman periods</title>
    <link>http://hdl.handle.net/2122/8511</link>
    <description>Title: Human colonization and volcanic activity in the eastern Campania Plain (Italy) between the Eneolithic and Late Roman periods
Authors: Di Vito, M. A; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia; Castaldo, N.; Soprintendenza Speciale per i Beni Archeologici di Napoli e Pompei, Naples, Italy; De Vita, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia; Bishop, J.; CAL srl, Contrada delle Bassiche 54, 25122 Brescia, Italy; Vecchio, G.; Soprintendenza Speciale per i Beni Archeologici di Napoli e Pompei, Naples, Italy
Abstract: Archaeological and volcanological studies conducted in the Naples area have revealed that numerous&#xD;
high-intensity explosive eruptions that occurred in the past 10 ka caused damage and victims in the&#xD;
human communities living in the plain surrounding the Neapolitan volcanoes. These catastrophic events&#xD;
were interspersed by hundred to thousand year long periods of quiescence, usually exceeding a human&#xD;
life-time.&#xD;
During the Early Bronze Age in particular, the Campania Plain was densely inhabited due to favourable&#xD;
climatic conditions and soil fertility. The archaeological and volcanological investigation of the sequences&#xD;
found in archaeological excavations has permitted the detailed reconstruction of the effects of eruptions&#xD;
and deposition mechanisms of their products on settlements. This paper discusses the example of Nola-&#xD;
Palma Campania during a most interesting, though poorly known, period of activity bracketed by the&#xD;
Vesuvian Pomici di Avellino (Early Bronze Age) and Pollena (AD 472) Plinian eruptions. Through this timespan&#xD;
the Plainwas variably inhabited, crossed by long-lived roads and subject to agricultural exploitation.&#xD;
Eruptions caused significant breaks in the occupation of the area, but also maintained the plain’s extraordinary&#xD;
fertility. During this period, at least eight other eruptions occurred: the Pomici di Pompei Plinian&#xD;
event (AD 79), two sub-Plinian to phreato-Plinian events, and five violent Strombolian to Vulcanian events.&#xD;
Thin and poorly developed to thicker and mature palaeosols or erosional unconformities separate the&#xD;
various pyroclastic deposits. Almost all the eruptions and related phenomena interacted with human&#xD;
settlements in the Campania Plain, and in their sequences many traces of the displacement of people&#xD;
during the eruptions may be seen, as well as land reclamation and re-utilization soon afterwards.&#xD;
Despite the various kinds of hazard posed by volcanic and related phenomena, humans nevertheless&#xD;
found good reasons for settlement in the Campania Plain and flourished there. A multidisciplinary&#xD;
approach has yielded detailed information regarding the evolution of the area and the effects of eruptions&#xD;
on settlements. These data are of paramount importance for an improved understanding of past&#xD;
events and in evaluating the hazard of eruptions and related phenomena</description>
    <dc:date>2012-12-31T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/8510">
    <title>The impact of the Ischia Porto Tephra eruption (Italy) on the Greek colony of Pithekoussai</title>
    <link>http://hdl.handle.net/2122/8510</link>
    <description>Title: The impact of the Ischia Porto Tephra eruption (Italy) on the Greek colony of Pithekoussai
Authors: de Vita, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia; Di Vito, M. A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia; Gialanella, C.; Soprintendenza Speciale per i Beni Archeologici di Napoli e Pompei; Sansivero, F.
Abstract: The island of Ischia is an active volcanic field, whose activity dates back to more than 150 ka. From Neolithic times it experienced a complex history of human colonization and volcanic eruptions that destroyed settlements and drove away the population. Recent archaeological and volcanological research has demonstrated that humans have periodically had to face volcanic and related hazardous phenomena since at least the Greek foundation of Pithekoussai (8th century BC).&#xD;
&#xD;
During the 5th century BC a telluric event is reported by the historian Strabo to have caused the abandonment of a Syracusan military outpost on the island. In the volcanological literature the Ischia Porto Tephra eruption has been identified as the most likely culprit. The eruption formed a crater lake in the north-eastern corner of the island and emplaced a poorly dispersed pyroclastic deposit, composed of a sequence of magmatic and phreatomagmatic scoria- and pumice-fallout beds, interlayered with minor pyroclastic density current deposits. Recent excavations furnished clear evidence of the impact of this eruption on a settlement located on S. Pietro Hill, to the east of Ischia’s harbour.&#xD;
&#xD;
The archaeological finds include mounds of building materials, pieces of decorative terracotta panels and a few terracotta antefix fragments. The spatial distribution of the material found, the presence of stacks of tiles and other building materials and the absence of any structural remains, suggest that this was a building site for the construction of a temple. As written sources confirm, although the site and the military garrison were abandoned, the colony survived.</description>
    <dc:date>2013-01-01T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/8478">
    <title>Integrating new and traditional approaches for the estimate of slip-rates of active faults: examples from the Mw 6.3, 2009 L’Aquila earthquake area, Central Italy</title>
    <link>http://hdl.handle.net/2122/8478</link>
    <description>Title: Integrating new and traditional approaches for the estimate of slip-rates of active faults: examples from the Mw 6.3, 2009 L’Aquila earthquake area, Central Italy
Authors: Civico, Riccardo; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia
Abstract: This thesis developed a multidisciplinary and multi-scale investigation strategy based on the integration of traditional and innovative approaches aimed at improving the normal faults seismogenic identification and characterization, focusing mainly on slip-rate estimate as a measure of the fault activity. &#xD;
The L’Aquila Mw 6.3 April 6, 2009 earthquake causative fault was used as a test site for the application, testing, and refinement of traditional and/or innovative approaches, with the aim to 1) evaluate their strength or limitations 2) develop a reference approach useful for extending the investigation to other active faults in the area and 3) translate the results of the methodological approaches into new inputs to local seismic hazard. &#xD;
The April 6, 2009 L’Aquila earthquake occurred on a so far poorly known tectonic structure, considered having a limited seismic potential, the Paganica - San Demetrio fault system (PSDFS), and thus has highlighted the need for a detailed knowledge in terms of location, geometry, and characterization of the active faults that are the potential sources for future earthquakes.&#xD;
To fill the gap of knowledge enhanced by the occurrence of the 2009 L’Aquila earthquake, we developed a multidisciplinary and multiscale‐based strategy consisting of paleoseismological investigations, detailed geomorphological and geological field studies, as well as shallow geophysical imaging and an innovative methodology that uses, as an alternative paleoseismological tool, core sampling and laboratory analyses but also in situ measurements of physical properties. &#xD;
The integration of geomorphology, geology as well as shallow geophysics, was essential to produce a new detailed geomorphological and geological map of the PSDFS and to define its tectonic style, arrangement, kinematics, extent, geometry and internal complexities.&#xD;
Our investigations highlighted that the PSDFS is a 19 km-long tectonic structure characterized by a complex structural setting at the surface and that is arranged in two main sectors: the Paganica sector to the NW and the San Demetrio sector to SE. The Paganica sector is characterized by a narrow deformation zone, with a relatively small (but deep) Quaternary basin affected by few fault splays. The San Demetrio sector is characterized by a strain distribution at the surface that is accommodated by several tectonic structures, with the system opening into a set of parallel, km-spaced fault traces that exhume and dissect the Quaternary basin.&#xD;
The integration of all the fault displacement data and age constraints (radiocarbon dating, optically stimulated luminescence (OSL) and tephrochronology) resulting from paleoseismological, geomorphological, geophysical and geological investigations played a primary role in the estimate of the slip-rate of the PSDFS. Slip-rates were estimated for different time intervals in the Quaternary, from Early Pleistocene (1.8 Ma) to Late Holocene (last 5 ka), yielding values ranging between 0.09 and 0.58 mm/yr and providing an average Quaternary slip-rate representative for the PSDFS of 0.27 - 0.48 mm/yr.&#xD;
We contributed also to the understanding of the PSDFS seismic behavior and of the local seismic hazard by estimating the max expected magnitude for this fault on the basis of its length (ca. 20 km) and slip per event (up to 0.8 m), and identifying the two most active fault splays at present. Our multidisciplinary results converge toward the possibility of the occurrence of past surface faulting earthquakes characterized by a moment magnitude between 6.3 and 6.8, notably larger than the 2009 event, but compatible with the M range observed in historical earthquakes in the area. The slip-rate distribution over time and space and the tectonic style of the PSDFS suggested the occurrence of strain migration through time in the southern sector, from the easternmost basin-bounding fault splay toward the southwestern splays. This topic has a significant implication in terms of surface faulting hazard in the area, because it can contribute defining the fault splays that have a higher potential to slip during future earthquakes along the PSDFS.&#xD;
By a methodological point of view, the multidisciplinary and multiscale‐based investigation strategy emphasizes the advantages of the joint application of different approaches and methodologies for active faults identification and characterization. &#xD;
Our work suggests that each approach alone may provide sufficient information but only the application of a multidisciplinary strategy is effective in providing robust results and in defining a proper framework of active faults.</description>
    <dc:date>2011-12-31T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/8469">
    <title>Orbital variations in planktonic foraminifera assemblages from the Ionian Sea during the Middle Pleistocene Transition</title>
    <link>http://hdl.handle.net/2122/8469</link>
    <description>Title: Orbital variations in planktonic foraminifera assemblages from the Ionian Sea during the Middle Pleistocene Transition
Authors: Incarbona, A.; Università degli Studi di Palermo, Dipartimento di Scienze della Terra e del Mare, Via Archirafi 22, 90134 Palermo, Italy; Dinarès-Turell, J.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia; Di Stefano, E.; Università degli Studi di Palermo, Dipartimento di Scienze della Terra e del Mare, Via Archirafi 22, 90134 Palermo, Italy; Ippolito, G.; Università degli Studi di Palermo, Dipartimento di Scienze della Terra e del Mare, Via Archirafi 22, 90134 Palermo, Italy; Pelosi, N.; Consiglio Nazionale delle Ricerche, Istituto per l'Ambiente Marino Costiero, Calata Porto di Massa, Interno Porto di Napoli, 80133, Naples, Italy; Sprovieri, R.; Università degli Studi di Palermo, Dipartimento di Scienze della Terra e del Mare, Via Archirafi 22, 90134 Palermo, Italy
Abstract: The Middle Pleistocene Transition (1.2-0.7 Ma) is the most recent re-organization of the global climate system which includes variations in the frequency and&#xD;
amplitude of glacial/interglacial cycles, increased ice sheet volume, sea surface&#xD;
temperature cooling and a significant drop in the CO2 atmospheric levels. Here we&#xD;
present high-resolution planktonic foraminifera data (mean sampling resolution of about 780 years) from core LC10 recovered in the Ionian Sea (eastern Mediterranean), between 1.2 and 0.9 Ma. Selected taxa, among them G. ruber, T. quinqueloba and G. bulloides, show significant periodicities that can be associated to orbital cycles, mainly precession and obliquity. The planktonic foraminifera based paleoclimatic curve exhibits a cooling linear trend that can be associated to similar phenomena observed in the North Atlantic. On the other hand, we refer to the influence of the North African Monsoon the occurrence of two peaks of the low-salinity tolerant species G. quadrilobatus that fall in coincidence of sapropel layers. Finally, we discuss the&#xD;
distribution pattern of N. pachyderma sinistral coiling, with peaks up to about 20%&#xD;
between MIS 30 and 28, and compare it to middle-late Quaternary records of the&#xD;
Sicily Channel and western Mediterranean.</description>
    <dc:date>2012-12-31T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/8455">
    <title>A photographic dataset of the coseismic geological effects induced on the environment by the 2012 Emilia (Northern Italy) earthquake sequence</title>
    <link>http://hdl.handle.net/2122/8455</link>
    <description>Title: A photographic dataset of the coseismic geological effects induced on the environment by the 2012 Emilia (Northern Italy) earthquake sequence
Authors: Alessio, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia; Alfonsi, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia; Brunori, C. A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Burrato, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Casula, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italia; Cinti, F. R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Civico, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Colini, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia; Cucci, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; De Martini, P. M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Falcucci, E.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Galadini, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Gaudiosi, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia; Gori, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Mariucci, M. T.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Montone, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Moro, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia; Nappi, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia; Nardi, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia; Nave, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia; Pantosti, D.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Patera, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Pesci, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italia; Pignone, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia; Pinzi, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Pucci, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Vannoli, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Venuti, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia; Villani, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; EMERGEO, Working Group; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia
Abstract: We present a collection of pictures of the coseismic secondary geological effects produced on the&#xD;
environment by the 2012 Emilia seismic sequence in northern Italy. The May-June 2012 sequence struck a&#xD;
broad area located in the Po Plain region, causing 26 deaths and hundreds of injured, 15.000 homeless,&#xD;
severe damage of historical centres and industrial areas, and an estimated economic toll of ~2 billion of&#xD;
euros. The sequence included two mainshocks (Figure 1): the first one, with ML 5.9, occurred on May 20&#xD;
between Finale Emilia, S. Felice sul Panaro and S. Martino Spino; the second one, with ML 5.8, occurred 12&#xD;
km southwest of the previous mainshock on May 29. Both the mainshocks occurred on about E-W trending,&#xD;
S dipping blind thrust faults; the whole aftershocks area extends in an E-W direction for more than 50 km&#xD;
and includes five ML≥5.0 events and more than 1800 ML&gt;1.5 events. Ground cracks and liquefactions were&#xD;
certainly the most relevant coseismic geological effects observed during the Emilia sequence. In particular,&#xD;
extensive liquefaction was observed over an area of ~1200 km2 following the May 20 and May 29 events.&#xD;
We collected all the coseismic geological evidence through field survey, helicopter and powered hang-glider&#xD;
trike survey, and reports from local people directly checked in the field. On the basis of their morphologic&#xD;
and structural characteristics the 1362 effects surveyed were grouped into three main categories: a)&#xD;
liquefactions related to overpressure of aquifers, occurring through several aligned vents forming coalescent&#xD;
flat cones (485 effects); b) liquefactions with huge amounts of liquefied sand and fine sand ejected from&#xD;
fractures tens of meters long (768); c) extensional fractures with small vertical throws, apparently organized&#xD;
in an en-echelon pattern, with no effects of liquefaction (109). The photographic dataset consists of 99&#xD;
pictures of coseismic geological effects observed in 17 localities concentrated in the epicentral area. The&#xD;
pictures are sorted and presented by locality of observation; each photo reports several information such as&#xD;
the name of the site, the geographical coordinates and the type of effect observed. Figure 1 shows a map of&#xD;
the pictures sites along with the location of the two mainshocks; Figure 2 shows a detail of the distribution of&#xD;
the liquefactions in the area of S. Carlo. The complete description of the coseismic geological effects&#xD;
induced by the Emilia sequence, their relation with the aftershock area, the InSAR deformation area and the&#xD;
I&gt;6 EMS felt area, along with the description of the technologies used for data sourcing and processing are&#xD;
shown in Emergeo Working Group [2012a and 2012b].</description>
    <dc:date>2012-09-30T22:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/8335">
    <title>The Palaeocene ‘‘top chron C27n’’ transient greenhouse episode: evidence from marine pelagic Atlantic and peri-Tethyan sections</title>
    <link>http://hdl.handle.net/2122/8335</link>
    <description>Title: The Palaeocene ‘‘top chron C27n’’ transient greenhouse episode: evidence from marine pelagic Atlantic and peri-Tethyan sections
Authors: Dinarès-Turell, J.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia; Pujalte, V.; Department of Stratigraphy and Paleontology, Fac. Science and Technology, University of the Basque Country UPV⁄EHU, PO Box 644, Bilbao E-48080, Spain; Stoykova, K.; Department of Paleontology and Stratigraphy, Geological Institute, Bulgarian Academy of Science, Sofia BG-1113, Bulgaria; Baceta, J. I.; Department of Stratigraphy and Paleontology, Fac. Science and Technology, University of the Basque Country UPV⁄EHU, PO Box 644, Bilbao E-48080, Spain; Ivanov, M.; Department of Geology and Paleontology, University of Sofia, Sofia BG-1000, Bulgaria
Abstract: The early Cenozoic, which is punctuated by several negative carbon isotope excursions (CIEs), was a time of climatic and&#xD;
oceanographic transition from ’Greenhouse’ to ’Icehouse’ conditions. The occurrence of a  0.5&amp; CIE starting at the top of Chron C27n (TC27N) is reconfirmed with stable isotope data from Zumaia (Spain) and Bjala (Bulgaria)&#xD;
localities. Spectral analysis on respective carbonate ⁄magnetic susceptibility proxy records substantiates the orbital&#xD;
cyclostratigraphy allowing correlation to a high-resolution benthic foraminifera isotope record from ODP Pacific Site 1209, that indicates a coeval 2  C transient warming. The hyperthermal event lasts  200 ka, contrasting with other short-lived events from the Eocene, and displays a relatively&#xD;
rapid onset and a longer tailing back to pre-event values similar to the Palaeocene–Eocene Thermal Maximum (PETM), though lower in amplitude. That a causal trigger for the&#xD;
TC27N event may be the onset of volcanism in the North Atlantic Igneous Province (NAIP) can be inferred from a 200-m-thick lava pile erupted during C27n ⁄ C26r polarity&#xD;
transition in the E Greenland margin.</description>
    <dc:date>2011-12-31T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/8328">
    <title>Gli eventi alluvionali: cronologia ed effetti sui resti archeologici</title>
    <link>http://hdl.handle.net/2122/8328</link>
    <description>Title: Gli eventi alluvionali: cronologia ed effetti sui resti archeologici
Authors: Galadini, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Falcucci, E.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Fubelli, G.; Università degli Studi Roma Tre; Gori, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia
Editors: Modadori Electa
Abstract: Field investigations performed at the Marco Nonio Macrino mausoleum, located along the ancient Flaminia road, in the northern sector of Rome (Italy), as well as the analysis of the archaeological stratigraphy allowed the reconstruction of the geological history of the archaeological site during the past centuries. Our investigations defined that, after the collapse of the mausoleum, the area was affected by at least five alluvial episodes of the Tiber river that interfingered with human activities at the site that were mainly focused on the recovery and re-use of the marble composing the architectonic elements of the building.</description>
    <dc:date>2011-12-31T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/8325">
    <title>Integrated stratigraphy for the Late Quaternary in the eastern Tyrrhenian Sea</title>
    <link>http://hdl.handle.net/2122/8325</link>
    <description>Title: Integrated stratigraphy for the Late Quaternary in the eastern Tyrrhenian Sea
Authors: Lirer, F.; Istituto per l’Ambiente Marino Costiero (IAMC) e CNR, Calata Porta di Massa, Interno Porto di Napoli, 80133 Napoli, Italy; Sprovieri, M.; Istituto per l’Ambiente Marino Costiero (IAMC) e CNR, Via del Faro 3, Torretta Granitola (Fraz. Campobello di Mazara, Tp) 91021, Italy; Ferraro, L.; Istituto per l’Ambiente Marino Costiero (IAMC) e CNR, Calata Porta di Massa, Interno Porto di Napoli, 80133 Napoli, Italy; Vallefuoco, M.; Istituto per l’Ambiente Marino Costiero (IAMC) e CNR, Calata Porta di Massa, Interno Porto di Napoli, 80133 Napoli, Italy; Capotondi, L.; Istituto Scienze Marine, ISMAR e CNR, Consiglio Nazionale delle Ricerche, Via Gobetti 101, 40129 Bologna, Italy; Cascella, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia; Petrosino, P.; Dipartimento di Scienze della Terra e Università degli Studi “Federico II” di Napoli. Largo S. Marcellino 10, 80138 Napoli, Italy; Insinga, D. D.; Istituto per l’Ambiente Marino Costiero (IAMC) e CNR, Calata Porta di Massa, Interno Porto di Napoli, 80133 Napoli, Italy; Pelosi, N.; Istituto per l’Ambiente Marino Costiero (IAMC) e CNR, Calata Porta di Massa, Interno Porto di Napoli, 80133 Napoli, Italy; Tamburrino, S.; Istituto per l’Ambiente Marino Costiero (IAMC) e CNR, Calata Porta di Massa, Interno Porto di Napoli, 80133 Napoli, Italy; Lubritto, C.; Dipartimento di Scienze Ambientali, Seconda Università di Napoli, Via Vivaldi 47, Caserta, Italy
Abstract: A high-resolution integrated stratigraphy is presented for the Late Quaternary in the southern-eastern Tyrrhenian Sea. It is based on calcareous plankton taxa (planktonic foraminifera and nannoplankton) distribution, d18OGlobigerinoides ruber record, tephrostratigraphy and radiometric dating methods (210Pb and 137Cs, AMS 14C) for a composite sediment core (from the top to the bottom, C90-1m, C90 and C836) from&#xD;
the continental shelf of the Salerno Gulf. High sedimentation rates from ca 1 cm/100 y for the early Holocene, to 3.45 cm/100 y for the middle Holocene to 8.78 cm/100 y from late Holocene and to 20 cm/100 y for the last 600 AD, make this area an ideal marine archive of secular paleoclimate changes.&#xD;
Quantitative distributional trend in planktonic foraminifera identify seven known (1Fe7F) eco-biozones, and several auxiliary bioevents of high potential for Mediterranean biostratigraphic correlation. Recognised&#xD;
were: the acme distribution of Neogloboquadrina pachyderma r.c. between 10.800   0.400 ka BP and 5.500   0.347 ka BP, a strong increase in abundance of Globorotalia truncatulinoides r.c. and l.c. at 5.500   0.347 ka BP and at 4.571   0.96 ka BP, respectively, an acme interval of Globigerinoides quadrilobatus&#xD;
(between 3.702   0.048 ka BP and 2.70   0.048 ka BP) and the acme/paracme intervals of&#xD;
T. quinqueloba (acme between 3.350   0.054 ka BP and 1.492   0.016 ka BP; paracme between&#xD;
1.492   0.016 ka BP and 0.657   0.025 ka BP; acme beginning 0.657   0.025 ka BP).&#xD;
These results, integrated with trends of selected calcareous nannofossil species (Florisphaera profunda, Brarudosphaera bigelowii, Gephyrocapsa oceanica and Emiliania huxleyi) and d18OG. ruber signature, are consistent with the most important pre-Holocene and early Holocene paleoclimatic and paleoceanographic phases i.e., the BöllingeAllerod, the Younger Dryas and the time interval of Sapropel S1 deposition in the eastern Mediterranean Sea. These features revealed the high potential of this shallow water environment for high-resolution stratigraphy and correlation for the western Mediterranean.&#xD;
In addition, the chemical characterization of seven tephra layers supplied further data about the age and the dispersal area of some well-known Campi Flegrei explosive events, inferring the possible occurrence of explosive activity at Vesuvius around the middle of the 6th century, and contributing to refine the tephrostratigraphic framework for the last 15 ka in the south-eastern Tyrrhenian Sea.</description>
    <dc:date>2012-12-31T23:00:00Z</dc:date>
  </item>
  <item rdf:about="http://hdl.handle.net/2122/8284">
    <title>Introduction: The ANDRILL McMurdo Ice Shelf (MIS) and Southern McMurdo Sound (SMS) Drilling Projects</title>
    <link>http://hdl.handle.net/2122/8284</link>
    <description>Title: Introduction: The ANDRILL McMurdo Ice Shelf (MIS) and Southern McMurdo Sound (SMS) Drilling Projects
Authors: Paulsen, T. S.; Department of Geology, University of Wisconsin Oshkosh, Oshkosh, Wisconsin 54901, USA; Pompilio, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Pisa, Pisa, Italia; Niessen, F.; Alfred Wegener Institute for Polar and Marine Research, D-27568 Bremerhaven, Germany; Panter, K.; Department of Geology, Bowling Green State University, Bowling Green, Ohio 43403-0218, USA; Jarrard, R. D.; Department of Geology and Geophysics, 383 FASB, University of Utah, 115 S. 1460 East, Salt Lake City, Utah 84112-0102, USA
Abstract: No Abstract</description>
    <dc:date>2012-05-31T22:00:00Z</dc:date>
  </item>
</rdf:RDF>

