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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-20-1167-2002</article-id>
<title-group>
<article-title>Imaging radar observations and nonlocal theory of large-scale plasma waves in the equatorial electrojet</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Hysell</surname>
<given-names>D. L.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Chau</surname>
<given-names>J. L.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Department of Physics and Astronomy, Clemson University, Clemson, South Carolina, USA</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>On leave at the Radio Science Center for Space and Atmosphere, Kyoto University, Uji, Kyoto 611–011, Japan</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Now at the Department of Earth and Atmospheric Sciences, Cornell University, Ithaca, New York, USA</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Radio Observatorio de Jicamarca, Instituto Geof´isico del Per´u, Lima, Peru</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Correspondence to: D. L. Hysell; (daveh@geology.cornell.edu)</addr-line>
</aff>
<pub-date pub-type="epub">
<day>31</day>
<month>08</month>
<year>2002</year>
</pub-date>
<volume>20</volume>
<issue>8</issue>
<fpage>1167</fpage>
<lpage>1179</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2002 D. L. Hysell</copyright-statement>
<copyright-year>2002</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>
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<self-uri xlink:href="https://angeo.copernicus.org/articles/20/1167/2002/angeo-20-1167-2002.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/20/1167/2002/angeo-20-1167-2002.pdf</self-uri>
<abstract>
<p>Large-scale (&lt;font face=&quot;Symbol&quot;&gt;l&lt;/font&gt;
 ~ 1 km) waves in the daytime and night-time equatorial electrojet are
 studied using coherent scatter radar data from Jicamarca. Images of plasma
 irregularities within the main beam of the radar are formed using
 interferometry with multiple baselines. These images are analyzed according to
 nonlocal gradient drift instability theory and are also compared to nonlinear
 computer simulations carried out recently by Ronchi et al. (1991) and Hu and
 Bhattacharjee (1999). In the daytime, the large-scale waves assume a non-steady
 dynamical equilibrium state characterized by the straining and destruction of
 the waves by shear and diffusion followed by spontaneous regeneration as
 predicted by Ronchi et al. (1991). At night, when steep plasma density
 gradients emerge, slowly propagating large-scale vertically extended waves
 predominate. Eikonal analysis suggests that these waves are trapped (absolutely
 unstable) or are nearly trapped (convectively unstable) and are able to tunnel
 between altitude regions which are locally unstable. Intermediate-scale waves
 are mainly transient (convectively stable) but can become absolutely unstable
 in narrow altitude bands determined by the background density profile. These
 characteristics are mainly consistent with the simulations presented by Hu and
 Bhattacharjee (1999). A new class of large-scale primary waves is found to
 occur along bands that sweep westward and downward from high altitudes through
 the E-region at twilight.&lt;br&gt;&lt;br&gt;&lt;b&gt;Key words. &lt;/b&gt;Ionosphere (equatorial
 ionosphere; ionospheric irregularities; plasma waves and instabilities)</p>
</abstract>
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