<?xml version="1.0" encoding="UTF-8"?>
<rss xmlns:slash="http://purl.org/rss/1.0/modules/slash/" xmlns:apple-wallpapers="http://www.apple.com/ilife/wallpapers" xmlns:itunes="http://www.itunes.com/dtds/podcast-1.0.dtd" xmlns:g-custom="http://base.google.com/cns/1.0" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:creativeCommons="http://backend.userland.com/creativeCommonsRssModule" xmlns:taxo="http://purl.org/rss/1.0/modules/taxonomy/" xmlns:content="http://purl.org/rss/1.0/modules/content/" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:g-core="http://base.google.com/ns/1.0" xmlns:cc="http://web.resource.org/cc/" xmlns:media="http://search.yahoo.com/mrss/" xmlns:opensearch="http://a9.com/-/spec/opensearch/1.1/" xmlns:georss="http://www.georss.org/georss" xmlns:geo="http://www.w3.org/2003/01/geo/wgs84_pos#" version="2.0">
  <channel>
    <title>DSpace Collection:</title>
    <link>http://hdl.handle.net/2122/171</link>
    <description />
    <pubDate>Sat, 18 May 2013 08:08:56 GMT</pubDate>
    <dc:date>2013-05-18T08:08:56Z</dc:date>
    <item>
      <title>GEMS: Underwater spectrometer for long-term radioactivity measurements</title>
      <link>http://hdl.handle.net/2122/6116</link>
      <description>Title: GEMS: Underwater spectrometer for long-term radioactivity measurements
Authors: L.Sartini; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia
Abstract: GEMS (Gamma Energy Marine Spectrometer) is a prototype of an autonomous radioactivity sensor for underwater&#xD;
measurements, developed in the framework of the KM3NeT Design Study (DS) EC project. The spectrometer is&#xD;
sensitive to gamma rays produced by 40K decays and it is also able to detect other natural (e.g., 238U, 232Th) and&#xD;
anthropogenic radionuclides (e.g. 137Cs). The decay of 40K, contained in sea salt, particulate and sediments, is one&#xD;
of the main sources of photon background in the underwater environment.&#xD;
GEMS was first calibrated in the laboratory using known sources, also in order to evaluate the performance of&#xD;
the instrument. In November 2008 GEMS was deployed at a depth of 3200 m in the area of Capo Passero (in the&#xD;
Ionian Sea) to acquire data autonomously. After recovery of the spectrometer six months later (May 2009) it was&#xD;
found that the instrument had worked within the specifications and acquired data over the full deployment period.&#xD;
These data allowed us to investigate over a long period the possible variations of activity at the Capo Passero site.&#xD;
GEMS is suitable to be used either in autonomous mode or as payload of seafloor observatories or vehicles.</description>
      <pubDate>Mon, 03 May 2010 22:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/2122/6116</guid>
      <dc:date>2010-05-03T22:00:00Z</dc:date>
    </item>
    <item>
      <title>The ocean wave dynamo: a source of magnetic field fluctuations</title>
      <link>http://hdl.handle.net/2122/1461</link>
      <description>Title: The ocean wave dynamo: a source of magnetic field fluctuations
Authors: Watermann, J.; NATO SACLANT Undersea Research Centre, La Spezia, Italy; Magunia, A.; Institut für Meteorologie und Geophysik, J.-W.-Goethe-Universitat, Frankfurt/Main, Germany; Gambetta, M.; Dipartimento di Scienze della Terra, Universitá di Genova, Italy; Bozzo, E.; Dipartimento di Scienze della Terra, Universitá di Genova, Italy
Abstract: The alternating magnetic dynamo field of sea surface waves, a consequence of their Lorentz electric field, has been observed with a pair of simultaneously operated, closely spaced tri-axial magnetometers. Measurements from a magnetometer located in the centre of a tiny, uninhabited island served to compensate measurements from a near-shore magnetometer for magnetic pulsations of ionospheric origin, leaving the ocean wave dynamo field, effective close to shore only, as the dominant residual magnetic field. Amplitude and frequency of waves and swell were recorded with a vertical accelerometer (wave rider buoy) floating nearby on the sea surface. A spectral analysis was performed on ten nighttime intervals of three hours length each, and for every interval, the peak power of the surface waves (obtained from the wave rider) was compared with the peak power of the residual horizontal magnetic field (after the background field had been removed). The results suggest that the dual-sensor magnetic field observations yield, within the limits of statistical significance, a good quantitative description of the amplitude and frequency of sea surface waves and swell.</description>
      <pubDate>Fri, 31 Jul 1998 22:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/2122/1461</guid>
      <dc:date>1998-07-31T22:00:00Z</dc:date>
    </item>
  </channel>
</rss>

