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  <channel>
    <title>DSpace Collection:</title>
    <link>http://hdl.handle.net/2122/172</link>
    <description />
    <pubDate>Fri, 24 May 2013 14:52:17 GMT</pubDate>
    <dc:date>2013-05-24T14:52:17Z</dc:date>
    <item>
      <title>Strengthening of the hydrological cycle in future scenarios: atmospheric energy and water balance perspective</title>
      <link>http://hdl.handle.net/2122/8581</link>
      <description>Title: Strengthening of the hydrological cycle in future scenarios: atmospheric energy and water balance perspective
Authors: Alessandri, A.; ENEA; Fogli, P. G.; CMCC; Vichi, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italia; Zeng, N.; University of Mariland
Abstract: Future climate scenarios experiencing global warming are expected to strengthen the hydrological cycle during the 21st century (21C). We analyze the strengthening of the global-scale increase in precipitation from the perspective of changes in whole atmospheric water and energy balances. By combining energy and water equations for the whole atmosphere, we obtain constraints for the changes in surface fluxes and partitioning at the surface between sensible and latent components. We investigate the differences in the strengthening of the hydrological cycle in two centennial simulations performed with an Earth system model forced with specified atmospheric concentration pathways. Alongside the Special Report on Emissions Scenario (SRES) A1B, which is a medium-high non-mitigation scenario, we consider a new aggressive-mitigation scenario (E1) with reduced fossil fuel use for energy production aimed at stabilizing global warming below 2 K.&#xD;
&#xD;
Our results show that the mitigation scenario effectively constrains the global warming with a stabilization below 2 K with respect to the 1950–2000 historical period. On the other hand, the E1 precipitation does not follow the temperature field toward a stabilization path but continues to increase over the mitigation period. Quite unexpectedly, the mitigation scenario is shown to strengthen the hydrological cycle even more than SRES A1B till around 2070. We show that this is mostly a consequence of the larger increase in the negative radiative imbalance of atmosphere in E1 compared to A1B. This appears to be primarily related to decreased sulfate aerosol concentration in E1, which considerably reduces atmospheric absorption of solar radiation compared to A1B.&#xD;
&#xD;
The last decades of the 21C show a marked increase in global precipitation in A1B compared to E1, despite the fact that the two scenarios display almost the same overall increase of radiative imbalance with respect to the 20th century. Our results show that radiative cooling is weakly effective in A1B throughout the 21C. Two distinct mechanisms characterize the diverse strengthening of the hydrological cycle in the middle and end- 21C. It is only through a very large perturbation of surface fluxes that A1B achieves a larger increase in global precipitation in the last decades of the 21C. Our energy/water budget analysis shows that this behavior is ultimately due to a bifurcation in the Bowen ratio change between the two scenarios.&#xD;
&#xD;
This work warns that mitigation policies that promote aerosol abatement, may lead to an unexpected stronger intensification of the hydrological cycle and associated changes that may last for decades after global warming is effectively mitigated. On the other hand, it is also suggested that predictable components of the radiative forcing by aerosols may have the potential to effectively contribute to the decadal-scale predictability of changes in the hydrological strength.</description>
      <pubDate>Sat, 31 Dec 2011 23:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/2122/8581</guid>
      <dc:date>2011-12-31T23:00:00Z</dc:date>
    </item>
    <item>
      <title>Investigating the impact of surface wave breaking on modeling the trajectories of drifters in the northern Adriatic Sea during a wind-storm event</title>
      <link>http://hdl.handle.net/2122/8191</link>
      <description>Title: Investigating the impact of surface wave breaking on modeling the trajectories of drifters in the northern Adriatic Sea during a wind-storm event
Authors: Carniel, S.; CNR-ISMAR; Warner, J. C.; USGS; Sclavo, M.; CNR-ISMAR; Chigiato, J.; NURC
Abstract: An accurate numerical prediction of the oceanic upper layer velocity is a demanding requirement for&#xD;
many applications at sea and is a function of several near-surface processes that need to be incorporated&#xD;
in a numerical model. Among them, we assess the effects of vertical resolution, different vertical mixing&#xD;
parameterization (the so-called Generic Length Scale –GLS– set of k–e, k–x, gen, and the Mellor–Yamada),&#xD;
and surface roughness values on turbulent kinetic energy (k) injection from breaking waves.&#xD;
First, we modified the GLS turbulence closure formulation in the Regional Ocean Modeling System&#xD;
(ROMS) to incorporate the surface flux of turbulent kinetic energy due to wave breaking. Then, we&#xD;
applied the model to idealized test cases, exploring the sensitivity to the above mentioned factors. Last,&#xD;
the model was applied to a realistic situation in the Adriatic Sea driven by numerical meteorological forcings&#xD;
and river discharges. In this case, numerical drifters were released during an intense episode of Bora&#xD;
winds that occurred in mid-February 2003, and their trajectories compared to the displacement of satellite-&#xD;
tracked drifters deployed during the ADRIA02-03 sea-truth campaign.&#xD;
Results indicted that the inclusion of the wave breaking process helps improve the accuracy of the&#xD;
numerical simulations, subject to an increase in the typical value of the surface roughness z0. Specifically,&#xD;
the best performance was obtained using aCH = 56,000 in the Charnok formula, the wave breaking parameterization&#xD;
activated, k–e as the turbulence closure model. With these options, the relative error with&#xD;
respect to the average distance of the drifter was about 25% (5.5 km/day). The most sensitive factors in&#xD;
the model were found to be the value of aCH enhanced with respect to a standard value, followed by&#xD;
the adoption of wave breaking parameterization and the particular turbulence closure model selected.</description>
      <pubDate>Wed, 31 Dec 2008 23:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/2122/8191</guid>
      <dc:date>2008-12-31T23:00:00Z</dc:date>
    </item>
    <item>
      <title>Dissolved gases in brackish thermal waters: an improved analytical method</title>
      <link>http://hdl.handle.net/2122/7954</link>
      <description>Title: Dissolved gases in brackish thermal waters: an improved analytical method
Authors: Liotta, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; Martelli, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia
Abstract: An improved method based on equilibrium partitioning between water samples and an inert host gas, introduced&#xD;
after sampling, is proposed for determining multiple species of dissolved gases in brackish water. The method&#xD;
itself, and the most convenient equations for describing gas solubilities in brackish waters, is described in detail.&#xD;
The method allows the rapid characterization of several sites and represents a useful tool for geochemical surveys.&#xD;
A comparison between replicate samples analyzed using different procedures demonstrates the efficiency of the&#xD;
method and indicates that the abundances of the main dissolved gases can be obtained, which can then be used&#xD;
to determine underlying geochemical processes. A Microsoft Excel worksheet is provided to easily calculate the&#xD;
concentration of dissolved gas species.</description>
      <pubDate>Sat, 31 Dec 2011 23:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/2122/7954</guid>
      <dc:date>2011-12-31T23:00:00Z</dc:date>
    </item>
    <item>
      <title>Atmospheric sources and sinks of volcanogenic elements in a basaltic volcano (Etna, Italy)</title>
      <link>http://hdl.handle.net/2122/7189</link>
      <description>Title: Atmospheric sources and sinks of volcanogenic elements in a basaltic volcano (Etna, Italy)
Authors: Calabrese, S.; Università di Palermo, Dipartimento DiSTeM; Aiuppa, A.; Università di Palermo, Dipartimento DiSTeM; Allard, P.; Institut de Physique du Globe, Paris, France; Bagnato, E.; Università di Palermo, Dipartimento DiSTeM; Bellomo, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; Brusca, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; D'Alessandro, W.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; Parello, F.; Università di Palermo, Dipartimento DiSTeM
Abstract: This study reports on the first quantitative assessment of the geochemical cycling of volcanogenic elements, from their atmospheric release to their deposition back to the ground. Etna’s emissions and atmospheric depositions were characterised for more than 2 years, providing data on major and trace element abundance in both volcanic aerosols and bulk depositions. Volcanic aerosols were collected from 2004 to 2007, at the summit vents by conventional filtration techniques. Precipitation was collected, from 2006 to 2007, in five rain gauges, at various altitudes around the summit craters. Analytical results for volcanic aerosols showed that the dominant anions were S, Cl, and F, and that the most abundant metals were K, Ca, Mg, Al, Fe, and Ti (1.5–50 lg m 3). Minor and trace element concentrations ranged from about 0.001 to 1 lg m 3. From such analysis, we derived an aerosol mass flux ranging from 3000 to 8000 t a 1. Most analysed elements had higher concentrations close to the emission vent, confirming the prevailing volcanic contribution to bulk deposition. Calculated deposition rates were integrated over the whole Etna area, to provide a first estimate of the total deposition fluxes for several major and trace elements. These calculated deposition fluxes ranged from 20 to 80 t a 1 (Al, Fe, Si) to 0.01–0.1 t a 1 (Bi, Cs, Sc, Th, Tl, and U). Comparison between volcanic emissions and atmospheric deposition showed that the amount of trace elements scavenged from the plume in the surrounding of the volcano ranged from 0.1% to 1% for volatile elements such as As, Bi, Cd, Cs, Cu, Tl, and from 1% to 5% for refractory elements such as Al, Ba, Co, Fe, Ti, Th, U, and V. Consequently, more than 90% of volcanogenic trace elements were dispersed further away, and may cause a regional scale impact. Such a large difference between deposition and emission fluxes at Mt. Etna pointed to relatively high stability and long residence time of aerosols in the plume.</description>
      <pubDate>Wed, 30 Nov 2011 23:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/2122/7189</guid>
      <dc:date>2011-11-30T23:00:00Z</dc:date>
    </item>
    <item>
      <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>
      <pubDate>Fri, 31 Dec 2010 23:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/2122/7104</guid>
      <dc:date>2010-12-31T23:00:00Z</dc:date>
    </item>
    <item>
      <title>Rainwater-induced leaching of selenium, arsenic and vanadium from Etnean volcanic soils</title>
      <link>http://hdl.handle.net/2122/5114</link>
      <description>Title: Rainwater-induced leaching of selenium, arsenic and vanadium from Etnean volcanic soils
Authors: Floor, G.H.; University of Girona, Spain; Calabrese, S.; Dip. CFTA, Università di Palermo; Roman-Ross, G.; University of Girona, Spain; D'Alessandro, W.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; Aiuppa, A.; Dip. CFTA, Università di Palermo
Abstract: Active volcanoes emit considerable amounts of&#xD;
contaminants such as As, Se and V. Mount Etna is the biggest&#xD;
volcano of Europe and an excellent geochemical site to study&#xD;
water-soil processes. Due to its volcanic activity, the rainwater&#xD;
has a strong compositional gradient, both in time and space.&#xD;
At present, the behaviour of trace elements in the soils around&#xD;
Mt Etna is poorly understood. To determine the influence of&#xD;
the rainwater pH on the potential mobilization of geogenic&#xD;
pollutants, batch experiments have been performed with&#xD;
synthetic rainwater for 25 soils collected along the flanks of&#xD;
the volcano. Our results show that:&#xD;
i) The maximum concentrations in the leaching solutions are&#xD;
higher for acid rain than for neutral rain (e.g. 7.7 vs 1.3&#xD;
mg/L for Se).&#xD;
ii) With neutral rain conditions the soils upwind from the&#xD;
volcano have higher concentrations of Se than those&#xD;
downwind (up to 1.3 mg/L compared to ≤0.3 mg/L for&#xD;
the other samples). This trend is less clear for As and V.&#xD;
iii) For soils collected from 2 to 10 km downwind of the&#xD;
craters, Se concentrations in acid rain leachates decrease&#xD;
one order of magnitude with increasing distance. A&#xD;
similar pattern is also observed upwind from the&#xD;
volcano. For As and V no clear relationship between&#xD;
concentrations and location with respect to the volcanic&#xD;
craters is observed.&#xD;
Both i) and ii) result in a low pH dependence for samples&#xD;
upwind from the volcano. The biggest difference between acid&#xD;
and neutral leaching for As and V is observed for a sample 2&#xD;
km downwind from the craters. The observed patterns are&#xD;
influenced by potential controlling factors, such as organic&#xD;
matter content, total concentrations, mineralogy, influence of&#xD;
the volcanic plume, etc. Our results have implications for the&#xD;
chemical composition of the Etnean aquifer, the only water&#xD;
resource to the one million inhabitants around Mt Etna, as well&#xD;
as for the bioavailability and potential toxicity through&#xD;
agricultural activities, essential to the local economy.</description>
      <pubDate>Sat, 20 Jun 2009 22:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/2122/5114</guid>
      <dc:date>2009-06-20T22:00:00Z</dc:date>
    </item>
    <item>
      <title>Bacterial and archaeal populations at two shallow hydrothermal vents off Panarea Island (Eolian Islands, Italy)</title>
      <link>http://hdl.handle.net/2122/5064</link>
      <description>Title: Bacterial and archaeal populations at two shallow hydrothermal vents off Panarea Island (Eolian Islands, Italy)
Authors: Maugeri, T.; Dipartimento di Biologia Animale ed Ecologia Marina, Universita` di Messina; Lentini, V.; Dipartimento di Biologia Animale ed Ecologia Marina, Universita` di Messina; Gugliandolo, C.; Dipartimento di Biologia Animale ed Ecologia Marina, Universita` di Messina; Italiano, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; Cousin, S.; Deutsche Sammlung von Mikroorganismen und Zellkulturen GmbH,; Stackebrandt, E.
Abstract: The aim of this study was to investigate the&#xD;
microbial community thriving at two shallow hydrothermal&#xD;
vents off Panarea Island (Italy). Physico-chemical characteristics&#xD;
of thermal waters were examined in order to&#xD;
establish the effect of the vents on biodiversity of both&#xD;
Bacteria and Archaea. Water and adjacent sediment samples&#xD;
were collected at different times from two vents,&#xD;
characterised by different depth and temperature, and&#xD;
analysed to evaluate total microbial abundances, sulphuroxidising&#xD;
and thermophilic aerobic bacteria. Total microbial&#xD;
abundances were on average of the order of&#xD;
105 cells ml-1, expressed as picoplanktonic size fraction.&#xD;
Picophytoplanktonic cells accounted for 0.77–3.83% of the&#xD;
total picoplanktonic cells. The contribution of bacterial and&#xD;
archaeal taxa to prokaryotic community diversity was&#xD;
investigated by PCR–DGGE fingerprinting method. The&#xD;
number of bands derived from bacterial DNA was highest&#xD;
in the DGGE profiles of water sample from the warmest&#xD;
and deepest site (site 2). In contrast, archaeal richness was&#xD;
highest in the water of the coldest and shallowest site (site&#xD;
1). Sulphur-oxidising bacteria were detected by both culture-&#xD;
dependent and -independent methods. The primary&#xD;
production at the shallow hydrothermal system of Panarea&#xD;
is supported by a complex microbial community composed&#xD;
by phototrophs and chemolithotrophs.</description>
      <pubDate>Wed, 31 Dec 2008 23:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/2122/5064</guid>
      <dc:date>2008-12-31T23:00:00Z</dc:date>
    </item>
    <item>
      <title>Geosystemics</title>
      <link>http://hdl.handle.net/2122/5017</link>
      <description>Title: Geosystemics
Authors: De Santis, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia
Editors: Trilling, L.; Massachussets Institute of Technology (MIT), USA; Perkins, D.; Harvard University, USA; Dionysiou, D. D.; University of Cincinnati, USA; Perlovsky, L.; Harvard University, USA; Davey, K.; IEEE Fellow, Editor IEEE Trans. on Magnetics, Austin, TX, USA; Landgrebe, D.; Purdue University, USA; Marino, M. A.; Civil &amp; Environmental Eng., and Biological &amp; Agricultural Engineering, University of California, CA, USA; Russell, D.L.; Virginia Tech., USA; Collicott, S. H.; School of Aeronautics and Astronautics, Univ. West Lafayette, USA; Ceccarelli, M.; University of Cassino, IT; Lund, G. W.; Oregon Institute of Technology, USA
Abstract: For Geosystemics we define the science that studies the Earth system from a holistic point of view. Earth is thus considered as a whole and unique far-from-the equilibrium complex system, formed by numerous different parts (sub-systems), which do not act independently but interact each other continuously. Most interactions are nonlinear, so that we can usually say that “resultant is more than the sum of the parts”. Interactions are not only in terms of contrasts but, and mostly, cooperative and mutual organizations. We will see some aspects and properties of this approach with a few examples.</description>
      <pubDate>Mon, 23 Feb 2009 23:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/2122/5017</guid>
      <dc:date>2009-02-23T23:00:00Z</dc:date>
    </item>
    <item>
      <title>Geogenic element behaviour in soil-rainwater interaction at Mt Etna, Sicily: preliminary results</title>
      <link>http://hdl.handle.net/2122/4222</link>
      <description>Title: Geogenic element behaviour in soil-rainwater interaction at Mt Etna, Sicily: preliminary results
Authors: Floor, G.; University of Girona Department of Chemistry; Calabrese, S.; Università di Palermo, Dipartimento CFTA; Roman-Ross, G.; University of Girona Department of Chemistry; D'Alessandro, W.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; Aiuppa, A.; Università di Palermo, Dipartimento CFTA
Abstract: Active volcanoes emit considerable amounts of contaminants such as As, Se and V. Previous&#xD;
studies have shown that the volcanic activity at Mt Etna (Sicily) has a strong influence on local&#xD;
rainwater compositions. However to date, the behaviour of trace elements in the soils around&#xD;
Mt Etna is poorly understood. 4-hr batch experiments have been performed with 1:5 soil&#xD;
solutions of air-dried soil (fraction &lt;2 mm) and synthetic (acid) rainwater (using either&#xD;
deionized water with a pH of ~6 or a ~500 ppm of sulphuric acid solution with a pH of ~2). In&#xD;
general trace element concentrations are more enriched in soil solutions with low pH (e.g.&#xD;
enrichment factor (EF) acid compared to neutral soil solution is up to 4.3x102 for V, 2.5x102&#xD;
for As and 50 for Se). However, it seems that the EF especially for As and V has a correlation&#xD;
with the distance to the crater. Additional, some soils located downwind of the volcano have&#xD;
EFs smaller than 1 (i.e. the elements are more enriched in neutral rainwater), for several&#xD;
elements like V, As and Se. For As and V the EF seems to be vary with distance to the crater.&#xD;
Some possible explanations for these trends will be discussed. These results might have&#xD;
important implications for the chemical composition of the Etnean aquifer, the only water&#xD;
resource to the one million inhabitants around Mt Etna, as well as the bioavailability and&#xD;
therefore potential toxicity through agricultural activities, essential to the local economy.</description>
      <pubDate>Sat, 18 Oct 2008 22:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/2122/4222</guid>
      <dc:date>2008-10-18T22:00:00Z</dc:date>
    </item>
    <item>
      <title>Mount Etna the major point source of metals in the Mediterranean basin: impact on atmospheric precipitation</title>
      <link>http://hdl.handle.net/2122/4214</link>
      <description>Title: Mount Etna the major point source of metals in the Mediterranean basin: impact on atmospheric precipitation
Authors: Calabrese, S.; Università di Palermo, Dipartimento CFTA; Parello, F.; Università di Palermo, Dipartimento CFTA; D'Alessandro, W.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italia; Aiuppa, A.; Università di Palermo, Dipartimento CFTA
Editors: Di Stefano, A.; Università di Catania - Dip. Scienze Geologiche; Maniscalco, R.; Università di Catania - Dip. Scienze Geologiche; Sturiale, G.; Università di Catania - Dip. Scienze Geologiche
Abstract: Mount Etna is a huge volcano in the Mediterranean basin and is located in the eastern part of&#xD;
Sicily. It is considered to be, on the long-term average, the major atmospheric point source of&#xD;
many environmental harmful compounds. Their emission occurs either through continuous&#xD;
passive degassing from open-conduit activity or through sporadic paroxysmal eruptive&#xD;
activity, in the form of gases, aerosols or particulate. Volcanic volatiles and aerosol emitted&#xD;
into the atmosphere fall on the Earth’s surface as wet or dry deposition, and can influence&#xD;
the environment both at local and regional scale.&#xD;
To estimate the environmental impact of magma-derived trace metals and their depositions&#xD;
processes, bulk deposition samples have been collected approximately fortnightly, using a&#xD;
network of 5 rain gauges located at various altitudes on the upper flanks close to the summit&#xD;
craters, from April 2006 to December 2007. Samples were analyzed for the main chemicalphysical&#xD;
parameters (electric conductivity and pH) and for major and trace elements&#xD;
concentrations.&#xD;
The data obtained clearly show that the volcanic contribution is always prevailing in the&#xD;
sampling site closest to the summit craters (∼1.5 km). In the distal sites (5.5-10 km from the&#xD;
summit) and downwind of the summit craters, the volcanic contribution is also detectable&#xD;
but often overwhelmed by anthropogenic or other natural (seawater spray, geogenic dust)&#xD;
contributions. Volcanogenic contribution may derive from both dry and wet deposition of&#xD;
gases and aerosols from the volcanic plume, but sometimes also from leaching of freshly&#xD;
emitted volcanic ashes. In fact, in our background site (7.5 km in the upwind direction), after&#xD;
an ash deposition event high concentration of lithophiles elements (Si, Al, Fe, Ti) have been&#xD;
measured.&#xD;
Sulphur, Chlorine and Fluorine, represent the main constituents that characterize the&#xD;
volcanic contribution in the bulk deposition on Mt. Etna, although high concentrations of&#xD;
many trace elements (Si, Al, Fe, Ti, Cu, As, Rb, Pb, Tl, Cd, Cr, U and Ag) display, in the site&#xD;
most exposed to the volcanic emissions, average concentrations of about two orders of&#xD;
magnitude higher than those measured in the background site (Mount Intraleo).</description>
      <pubDate>Mon, 02 Jun 2008 22:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/2122/4214</guid>
      <dc:date>2008-06-02T22:00:00Z</dc:date>
    </item>
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