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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ANGEO</journal-id>
<journal-title-group>
<journal-title>Annales Geophysicae</journal-title>
<abbrev-journal-title abbrev-type="publisher">ANGEO</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Ann. Geophys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1432-0576</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/angeo-22-2643-2004</article-id>
<title-group>
<article-title>Cluster observations of ELF/VLF signals generated by modulated heating of the lower ionosphere with the HAARP HF transmitter</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Platino</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>Inan</surname>
<given-names>U. S.</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>Bell</surname>
<given-names>T. 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>Pickett</surname>
<given-names>J.</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>Kennedy</surname>
<given-names>E. J.</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>Trotignon</surname>
<given-names>J. G.</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>Rauch</surname>
<given-names>J. L.</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>Canu</surname>
<given-names>P.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Space, Telecommunications and Radioscience (STAR) Laboratory, Stanford University, Stanford, CA 94305, USA</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Dept. of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, USA</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Naval Research Laboratory, 4555 Overlook Ave. SW, Washington D.C. 20375, USA</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Laboratoire de Physique et Chimie de l’Environnement, Centre National de la Recherche Scientifique, 3 A avenue de la Recherche Scientifique, F-45071 Orléans cedex 02, France</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Centre d’Etudes des Environnements Terrestres et Planétaires, Centre National de la Recherche Scientifique, Université Versailles Saint-Quentin-en-Yvelines, 10 avenue de l’Europe, F-78140, Vélizy Villacoublay, France</addr-line>
</aff>
<pub-date pub-type="epub">
<day>14</day>
<month>07</month>
<year>2004</year>
</pub-date>
<volume>22</volume>
<issue>7</issue>
<fpage>2643</fpage>
<lpage>2653</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2004 M. Platino et al.</copyright-statement>
<copyright-year>2004</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://angeo.copernicus.org/articles/22/2643/2004/angeo-22-2643-2004.html">This article is available from https://angeo.copernicus.org/articles/22/2643/2004/angeo-22-2643-2004.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/22/2643/2004/angeo-22-2643-2004.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/22/2643/2004/angeo-22-2643-2004.pdf</self-uri>
<abstract>
<p>It is now well known that amplitude modulated HF
transmissions into the ionosphere can be used to generate ELF/VLF signals
using the so-called &quot;electrojet antenna&quot;. Although most observations of the
generated ELF/VLF signals have been made on the ground, several low and
high-altitude satellite observations have also been reported (James et al., 1990). One of
the important unknowns in the physics of ELF/VLF wave generation by
ionospheric heating is the volume of the magnetosphere illuminated by the
ELF/VLF waves. In an attempt to investigate this question further,
ground-satellite conjunction experiments have recently been conducted using
the four Cluster satellites and the HF heater of the High-Frequency Active
Auroral Research Program (HAARP) facility in Gakona, Alaska. Being located
on largely closed field lines at &lt;i&gt;L&lt;/i&gt;&amp;asymp;4.9, HAARP is currently also
being used for ground-to-ground type of ELF/VLF wave-injection experiments,
and will be increasingly used for this purpose as it is now being upgraded
for higher power operation. In this paper, we describe the HAARP
installation and present recent results of the HAARP-Cluster experiments.
We give an overview of the detected ELF/VLF signals at Cluster, and a
possible explanation of the spectral signature detected, as well as the
determination of the location of the point of injection of the HAARP ELF/VLF
signals into the magnetosphere using ray tracing.</p>
</abstract>
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