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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-6-735-2006</article-id>
<title-group>
<article-title>On variations of &lt;i&gt;fo&lt;/i&gt;F2 and F-spread before strong earthquakes in Japan</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Liperovskaya</surname>
<given-names>E. V.</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>Parrot</surname>
<given-names>M.</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>Bogdanov</surname>
<given-names>V. V.</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>Meister</surname>
<given-names>C.-V.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Rodkin</surname>
<given-names>M. V.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Liperovsky</surname>
<given-names>V. A.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Institute for Physics of the Earth, 123995 Moscow, Russia</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>L.P.C.E./C.N.R.S., 3A, Avenue de la Recherche Scientifique, 45071 Orléans Cedex 2, France</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Inst. of Cosmophysical Research and Radio Wave Propagation, Far Eastern Branch of RAS, 684034 P-Kamchatsky, Russia</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>High School and Science Programme Brandenburg/Potsdam, Project &quot;Physics of Stellar and Planetary Atmospheres&quot;, 14482 Potsdam, Germany</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>World Geophysical Data Center, Molodejnaya 3, 117296 Moscow,  Russia</addr-line>
</aff>
<pub-date pub-type="epub">
<day>22</day>
<month>08</month>
<year>2006</year>
</pub-date>
<volume>6</volume>
<issue>5</issue>
<fpage>735</fpage>
<lpage>739</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2006 E. V. Liperovskaya et al.</copyright-statement>
<copyright-year>2006</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/6/735/2006/nhess-6-735-2006.html">This article is available from https://nhess.copernicus.org/articles/6/735/2006/nhess-6-735-2006.html</self-uri>
<self-uri xlink:href="https://nhess.copernicus.org/articles/6/735/2006/nhess-6-735-2006.pdf">The full text article is available as a PDF file from https://nhess.copernicus.org/articles/6/735/2006/nhess-6-735-2006.pdf</self-uri>
<abstract>
<p>The statistical analysis  of the variations of the dayly-mean frequency of the
maximum ionospheric electron density &lt;i&gt;fo&lt;/i&gt;F2 is performed in connection with the
occurrence of (more than 60) earthquakes with magnitudes &lt;i&gt;M&lt;/i&gt;&amp;gt;6.0, depths
&lt;i&gt;h&lt;/i&gt;&amp;lt;80 km and distances from the vertical sounding station &lt;i&gt;R&lt;/i&gt;&amp;lt;1000 km. For
the study, data of the Tokyo sounding station are used, which were registered
every hour in the years 1957&amp;ndash;1990.  It is shown that, on the average, &lt;i&gt;fo&lt;/i&gt;F2
decreases before the earthquakes. One day before the shock the decrease
amounts to about 5%. The statistical reliability of this phenomenon
is obtained to be better than 0.95.

&lt;P&gt;

Further, the variations of the occurrence probability of the turbulization of
the F-layer (F spread) are investigated for (more than 260) earthquakes with
&lt;i&gt;M&lt;/i&gt;&amp;gt;5.5, &lt;i&gt;h&lt;/i&gt;&amp;lt;80 km, &lt;i&gt;R&lt;/i&gt;&amp;lt;1000 km. For the analysis, data of the Japanese
station  Akita from 1969&amp;ndash;1990 are used, which were  obtained every hour.
It is found that before the earthquakes the occurrence probability of F spread
decreases. In the week before the event, the decrease has values of more than
10%. The statistical reliability of this phenomenon
is also larger than 0.95. Examining the seismo-ionospheric effects, here
periods
of time with weak heliogeomagnetic disturbances are considered.
For the &lt;i&gt;fo&lt;/i&gt;F2 analysis, the Wolf
number is less than 100 and the index &amp;Sigma;&lt;i&gt;K&lt;sub&gt;p&lt;/sub&gt;&lt;/i&gt; is smaller than 30, and
in case of the F-spread study a Wolf
number less than 80 and &amp;Sigma;&lt;i&gt;K&lt;sub&gt;p&lt;/sub&gt;&lt;/i&gt;  smaller than 17 are chosen.</p>
</abstract>
<counts><page-count count="5"/></counts>
</article-meta>
</front>
<body/>
<back>
<ref-list>
<title>References</title>
<ref id="ref1">
<label>1</label><mixed-citation publication-type="other" xlink:type="simple"> Hobara, Y. and Parrot, M.: Ionospheric perturbations linked to a very powerful seismic event, J. Atmos. Terr. Phys., 67, 677&amp;ndash;685, 2005.  </mixed-citation>
</ref>
<ref id="ref2">
<label>2</label><mixed-citation publication-type="other" xlink:type="simple"> Liperovsky, V. A., Pokhotelov, O. A., and Shalimov, S. L.: Ionospheric precursors of earthquakes, Nauka, Moscow, 1992.  </mixed-citation>
</ref>
<ref id="ref3">
<label>3</label><mixed-citation publication-type="other" xlink:type="simple"> Liu, J. Y., Chen, Y. I., Chuo, Y. J., and Chen, C. S.: A statistical investigation of preearthquake ionospheric anomaly, J. Geophys. Res., 111, A05304, https://doi.org/10.1029/2005JA011333, 2006. </mixed-citation>
</ref>
<ref id="ref4">
<label>4</label><mixed-citation publication-type="other" xlink:type="simple"> Ondoh, T.: Seismo-ionospheric phenomena, Adv. Space Res., 26(8), 1267&amp;ndash;1272, 2000. </mixed-citation>
</ref>
<ref id="ref5">
<label>5</label><mixed-citation publication-type="other" xlink:type="simple"> Pulinets, S. A. and Boyarchuk, K. A.: Ionospheric precursors of earthquakes, Springer, Berlin, 2004. </mixed-citation>
</ref>
<ref id="ref6">
<label>6</label><mixed-citation publication-type="other" xlink:type="simple"> Rios, V. H., Kim, V. P., and Hegai, V. V.: Abnormal perturbations in the F2 region ionosphere observed prior to the great San Juan earthquake of 23 November 1977, Adv. Space Res., 33, 323&amp;ndash;327, 2004. </mixed-citation>
</ref>
<ref id="ref7">
<label>7</label><mixed-citation publication-type="other" xlink:type="simple"> Singh, B., Kushwah, V., Singh, O. P., Lakshmi, D. R., and Reddy, B. M.: Ionospheric perturbations caused by some major earthquakes in India, Phys. Chem. Earth, 29, 537&amp;ndash;550, 2004. </mixed-citation>
</ref>
</ref-list>
</back>
</article>