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    <title>DSpace Community: Editorial Initiatives</title>
    <link>http://hdl.handle.net/2122/583</link>
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      <title>The Community's search engine</title>
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      <link>http://www.earth-prints.org/simple-search</link>
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      <title>Effects of transient water mass redistribution associated with a tsunami wave on Earth’s pole path</title>
      <link>http://hdl.handle.net/2122/4060</link>
      <description>Title: Effects of transient water mass redistribution associated with a tsunami wave on Earth’s pole path
&lt;br/&gt;
&lt;br/&gt;Authors: Pisani, A. R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Piersanti, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Melini, D.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Piatanesi, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Soldati, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia
&lt;br/&gt;
&lt;br/&gt;Abstract: We have quantified the effects of a water mass redistribution associated with the propagation of a tsunami wave&#xD;
on the Earth’s pole path and on the Length-Of-Day (LOD) and applied our modeling results to the tsunami following&#xD;
the 2004 giant Sumatra earthquake. We compared the result of our simulations on the instantaneous rotational&#xD;
axis variations with the preliminary instrumental evidence on the pole path perturbation (which has not&#xD;
been confirmed) registered just after the occurrence of the earthquake. The detected perturbation in the pole path&#xD;
showed a step-like discontinuity that cannot be attributed to the effect of a seismic dislocation. Our results show&#xD;
that the tsunami induced instantaneous rotational pole perturbation is indeed characterized by a step-like discontinuity&#xD;
compatible with the observations but its magnitude is almost one hundred times smaller than the detected&#xD;
one. The LOD variation induced by the water mass redistribution turns out to be not significant because the&#xD;
total effect is smaller than current measurements uncertainties.</description>
      <pubDate>Fri, 28 Sep 2007 22:58:59 GMT</pubDate>
    </item>
    <item>
      <title>Cavola experiment site: geophysical investigations and deployment of a dense seismic array on a landslide</title>
      <link>http://hdl.handle.net/2122/4059</link>
      <description>Title: Cavola experiment site: geophysical investigations and deployment of a dense seismic array on a landslide
&lt;br/&gt;
&lt;br/&gt;Authors: Bordoni, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia; Haines, J.; Bullard Laboratories, Department of Earth Sciences, University of Cambridge, U.K.; Di Giulio, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Milana, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Augliera, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Milano-Pavia, Milano, Italia; Cercato, M.; Dipartimento di Idraulica Trasporti e Strade (DITS), Facoltà di Ingegneria, Università degli Studi di Roma «La Sapienza», Roma, Italy; Martelli, L.; Regione Emilia Romagna, Servizio Geologico Sismico e dei Suoli, Bologna, Italy; Cara, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia; Cavola Experiment Team; 0
&lt;br/&gt;
&lt;br/&gt;Abstract: Geophysical site investigations have been performed in association with deployment of a dense array of 95 3-component&#xD;
seismometers on the Cavola landslide in the Northern Apennines. The aim of the array is to study propagation&#xD;
of seismic waves in the heterogeneous medium through comparison of observation and modelling. The small-aperture&#xD;
array (130 m×56 m) operated continuously for three months in 2004. Cavola landslide consists of a clay body&#xD;
sliding over mudstone-shale basement, and has a record of historical activity, including destruction of a small village&#xD;
in 1960. The site investigations include down-hole logging of P- and S-wave travel times at a new borehole drilled&#xD;
within the array, two seismic refraction lines with both P-wave profiling and surface-wave analyses, geo-electrical&#xD;
profiles and seismic noise measurements. From the different approaches a consistent picture of the depths and seismic&#xD;
velocities for the landslide has emerged. Their estimates agree with resonance frequencies of seismic noise, and&#xD;
also with the logged depths to basement of 25 m at a new borehole and of 44 m at a pre-existing borehole. Velocities&#xD;
for S waves increase with depth, from 230 m/s at the surface to 625 m/s in basement immediately below the landslide.</description>
      <pubDate>Fri, 28 Sep 2007 22:58:59 GMT</pubDate>
    </item>
    <item>
      <title>Morphology of F-region vertical E×B drifts in the African sector using ionosonde measurements</title>
      <link>http://hdl.handle.net/2122/4058</link>
      <description>Title: Morphology of F-region vertical E×B drifts in the African sector using ionosonde measurements
&lt;br/&gt;
&lt;br/&gt;Authors: Oyekola, O. S.; Department of Physics, College of Science and Technology, Covenant University, Canaanland, Ota, Ogun State, Nigeria; Oluwafemi, C. C.; Department of Physics, College of Science and Technology, Covenant University, Canaanland, Ota, Ogun State, Nigeria
&lt;br/&gt;
&lt;br/&gt;Abstract: F-region vertical velocities are derived from the ground-based ionosonde data for Ibadan (7.4°N, 3.9°E; dip 6°S:&#xD;
an equatorial station in the African zone), to study the general characteristics of electrodynamics of equatorial&#xD;
ionosphere, such as their variation with season, solar cycle, and magnetic activity at different local time sectors.&#xD;
The results show profound seasonal and geomagnetic effects. Except for equinoctial period, there is an excellent&#xD;
consistency in the magnitudes (nearly 20 m/s) and patterns of upward daytime F-region drifts at low and high&#xD;
solar activity periods. Evening F-region exhibits strong motion with absolute mean value for quiet-time (15 m/s)&#xD;
greater than on disturbed-time (10 m/s). The average downward quiet midnight-early morning hours sector value&#xD;
is well below than 10 m/s. The evening reversal time is earliest and latest during solstitial periods. Prereversal&#xD;
peak is season dependent and varies strongly with magnetic activity. We show that prereversal peak, daytime,&#xD;
and nighttime maximum drifts saturate at particular values of F10.7 cm solar radio flux index, effects not noticed&#xD;
with corresponding sunspot number. Our observations confirm several previous results from other equatorial&#xD;
sites utilizing different experimental techniques.</description>
      <pubDate>Fri, 28 Sep 2007 22:58:59 GMT</pubDate>
    </item>
    <item>
      <title>Historical earthquakes and damage patterns in Potenza (Basilicata, Southern Italy)</title>
      <link>http://hdl.handle.net/2122/4057</link>
      <description>Title: Historical earthquakes and damage patterns in Potenza (Basilicata, Southern Italy)
&lt;br/&gt;
&lt;br/&gt;Authors: Gizzi, F. T.; Istituto per i Beni Archeologici e Monumentali, CNR, Area della Ricerca di Potenza, Tito Scalo (PZ), Italy; Masini, N.; Istituto per i Beni Archeologici e Monumentali, CNR, Area della Ricerca di Potenza, Tito Scalo (PZ), Italy
&lt;br/&gt;
&lt;br/&gt;Abstract: This paper analyzes three historical seismic damage patterns in Potenza, the main town of the Basilicata Region,&#xD;
in Southern Italy. We refer to the 1826, 1857 and 1930 earthquakes, which hit the town with intensities ranging&#xD;
from VI-VII to VIII-IX MCS. In order to depict the seismic effects, we analyzed original documents, most of&#xD;
them never consulted before. The events have been located on an urban map of Potenza dating back to 1875.&#xD;
This research represents the starting point for further investigations, with the goal of highlighting the causes of&#xD;
the ‘anomalies’ in the distribution of the effects.</description>
      <pubDate>Fri, 28 Sep 2007 22:58:59 GMT</pubDate>
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