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<front>
<journal-meta>
<journal-id journal-id-type="publisher">NHESS</journal-id>
<journal-title-group>
<journal-title>Natural Hazards and Earth System Sciences</journal-title>
<abbrev-journal-title abbrev-type="publisher">NHESS</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Nat. Hazards Earth Syst. Sci.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1684-9981</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/nhess-3-197-2003</article-id>
<title-group>
<article-title>Exalting in atmospheric tides as earthquake precursor</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Biagi</surname>
<given-names>P. F.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Piccolo</surname>
<given-names>R.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Capozzi</surname>
<given-names>V.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ermini</surname>
<given-names>A.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Martellucci</surname>
<given-names>S.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Bellecci</surname>
<given-names>C.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Department of Physics-INFM, University of Bari, Via Amendola, 173, 70126 Bari, Italy</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Medicin Faculty-INFM, University of Foggia, Via L. Pinto, 71100 Foggia, Italy</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Department of Physics and Energy Science and Technology, University of Roma &quot;Tor Vergata&quot;, Via di Tor Vergata, 00133 Rome, Italy</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>INFM, University of Roma “Tor Vergata&quot;, Italy</addr-line>
</aff>
<pub-date pub-type="epub">
<day>31</day>
<month>08</month>
<year>2003</year>
</pub-date>
<volume>3</volume>
<issue>3/4</issue>
<fpage>197</fpage>
<lpage>201</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2003 P. F. Biagi et al.</copyright-statement>
<copyright-year>2003</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Generic License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by-nc-sa/2.5/">https://creativecommons.org/licenses/by-nc-sa/2.5/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://nhess.copernicus.org/articles/3/197/2003/nhess-3-197-2003.html">This article is available from https://nhess.copernicus.org/articles/3/197/2003/nhess-3-197-2003.html</self-uri>
<self-uri xlink:href="https://nhess.copernicus.org/articles/3/197/2003/nhess-3-197-2003.pdf">The full text article is available as a PDF file from https://nhess.copernicus.org/articles/3/197/2003/nhess-3-197-2003.pdf</self-uri>
<abstract>
<p>During February–March
      1998, we observed a significant increase (6–8 dB) in the electric field
      of the CZE (&lt;i&gt;f&lt;/i&gt; = 270 kHz, Czech Republic) broadcasting station at a site
      named AS and located in central Italy. On 13 March 1998 an earthquake (&lt;i&gt;M&lt;/i&gt; =
      5.2) occurred in Slovenia, starting a strong seismic crisis (&lt;i&gt;M&lt;/i&gt; = 6.0 on 12
      April, &lt;i&gt;M&lt;/i&gt; = 5.1 on 6 May). The distances of the epicentres from the radio
      receiver were over 400 km, but the epicentres are located in a zone that
      is in the middle of the CZE-AS path. Previously, we advanced the
      hypothesis that the increase of radio-signal electric field detected could
      be a precursor of the Slovenia seismic crisis. At the purpose to precise
      the connection between this radio anomaly and the preparatory phase of the
      earthquakes, we analysed in detail the data collected. At first we carried
      out a FFT on the data and clear harmonic components with period 0.5d, 1d,
      14d, 28d and 365d were revealed. These periods are characteristic of
      gravity tides and therefore, it seems reasonable to consider the previous
      harmonics in the electric field of the radio signal as components related
      to tides of the atmosphere, assuming as tides of the atmosphere only the
      linear action of gravity tides on atmosphere. Then, we carried out band
      pass filters on our data and we discovered that the February–March 1998
      increase is mainly related to an exalting of the harmonics with period
      0.5d, 1d, 14d and 28d, i.e. of the (semi)monthly and (semi)diurnal
      atmospheric tidal components in the radio signal. Supposing that this
      exalting is produced by a corresponding exalting of the atmospheric tides
      we propose a model able to explain the production of such an effect during
      the preparatory phase of the Slovenia earthquakes.</p>
</abstract>
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