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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-8-135-2008</article-id>
<title-group>
<article-title>Detection of ionospheric perturbations associated with Japanese earthquakes on the basis of reception of LF transmitter signals on the satellite DEMETER</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Muto</surname>
<given-names>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>Yoshida</surname>
<given-names>M.</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>Horie</surname>
<given-names>T.</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>Hayakawa</surname>
<given-names>M.</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>Molchanov</surname>
<given-names>O. A.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Department of Electronic Engineering and Research Station on Seismo Electromagnetics, University of Electro-Communications, Chofu Tokyo, Japan</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>LPCE/CNRS, Orleans, France</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Institute of Physics of the Earth, Moscow, Russia</addr-line>
</aff>
<pub-date pub-type="epub">
<day>26</day>
<month>02</month>
<year>2008</year>
</pub-date>
<volume>8</volume>
<issue>1</issue>
<fpage>135</fpage>
<lpage>141</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2008 F. Muto et al.</copyright-statement>
<copyright-year>2008</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/8/135/2008/nhess-8-135-2008.html">This article is available from https://nhess.copernicus.org/articles/8/135/2008/nhess-8-135-2008.html</self-uri>
<self-uri xlink:href="https://nhess.copernicus.org/articles/8/135/2008/nhess-8-135-2008.pdf">The full text article is available as a PDF file from https://nhess.copernicus.org/articles/8/135/2008/nhess-8-135-2008.pdf</self-uri>
<abstract>
<p>There have been recently reported a lot of electromagnetic phenomena
associated with earthquakes (EQs). Among these, the ground-based reception
of subionospheric waves from VLF/LF transmitters, is recognized as a
promising tool to investigate the ionospheric perturbations associated with
EQs. This paper deals with the corresponding whistler-mode signals in the
upper ionosphere from those VLF/LF transmitters, which is the counterpart of
subionospheric signals. The whistler-mode VLF/LF transmitter signals are
detected on board the French satellite, DEMETER launched on 29 June 2004.
We have chosen several large Japanese EQs including the Miyagi-oki EQ (16
August 2005; M=7.2, depth=36 km), and the target transmitter is a Japanese
LF transmitter (JJY) whose transmitter frequency is 40 kHz. Due to large
longitudinal separation of each satellite orbit (2500 km), we have to adopt
a statistical analysis over a rather long period (such as 3 weeks or one
month) to have reliable data set. By analyzing the spatial distribution of
JJY signal intensity (in the form of signal to noise ratio SNR) during a
period of 4 months including the Miyagi-oki EQ, we have found significant
changes in the intensity; generally the SNR is significantly depleted before
the EQ, which is considered to be a precursory ionospheric signature of the
EQ. This abnormal effect is reasonably explained in terms of either (1)
enhanced absorption of whistler-mode LF signals in the lower ionosphere due
to the lowering of the lower ionosphere, or (2) nonlinear wave-wave
scattering. Finally, this analysis suggests an important role of satellite
observation in the study of lithosphere-atmosphere-ionosphere coupling.</p>
</abstract>
<counts><page-count count="7"/></counts>
</article-meta>
</front>
<body/>
<back>
<ref-list>
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</back>
</article>