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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-25-689-2007</article-id>
<title-group>
<article-title>On the location and structure of the artificial 630-nm airglow patch over Sura facility</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Grach</surname>
<given-names>S. M.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kosch</surname>
<given-names>M. J.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</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>Yashnov</surname>
<given-names>V. A.</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>Sergeev</surname>
<given-names>E. N.</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>Atroshenko</surname>
<given-names>M. A.</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>Kotov</surname>
<given-names>P. V.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Radiophysics Faculty, State University of Nizhny Novgorod,  Russia</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Radiophysical Research Institute, Nizhny Novgorod,  Russia</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Communication Systems, Lancaster University, Lancaster LA1 4WA, UK</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Honorary Research Fellow, University of Kwazulu-Natal, Durban 4001, South Africa</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Currently at Space Vehicles Directorate, Air Force Research Laboratory, Hanscom Air Force Base, MA, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>29</day>
<month>03</month>
<year>2007</year>
</pub-date>
<volume>25</volume>
<issue>3</issue>
<fpage>689</fpage>
<lpage>700</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2007 S. M. Grach et al.</copyright-statement>
<copyright-year>2007</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/25/689/2007/angeo-25-689-2007.html">This article is available from https://angeo.copernicus.org/articles/25/689/2007/angeo-25-689-2007.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/25/689/2007/angeo-25-689-2007.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/25/689/2007/angeo-25-689-2007.pdf</self-uri>
<abstract>
<p>Results are presented of the artificial optical emission of the atomic oxygen red line
(the radiation of level O(&lt;sup&gt;1&lt;/sup&gt;D) with a wavelength of 630 nm) from the
HF-pumped ionosphere, obtained in September 2004 at the SURA heating facility situated
near Nizhny Novgorod, Russia. For vertical pumping the airglow patch was increasingly
displaced to the north, up to 7&amp;ndash;8&amp;deg;, with increasing reflection altitude. For
large brightness of the emission, the airglow patch started to develop at the northern
edge of the pump beam and later expanded to the south. These effects  are attributed to
the precipitation of supra-thermal electrons from the pump wave upper hybrid resonance
altitude to lower altitudes where excitation of the O(&lt;sup&gt;1&lt;/sup&gt;D) level is  more
effective due to the larger density of atomic oxygen, and the O(&lt;sup&gt;1&lt;/sup&gt;D) lifetime
is shorter. For a pump beam inclination of 12&amp;deg; to the south, the optical spot was
displaced by 4&amp;ndash;5&amp;deg; to the south relative to the straight-line projection of the
pump beam onto the sky. This exceeds that expected from the ray tracing and may be
related, most probably, to the so-called &quot;magnetic zenith&quot; effect.  In addition,
mid-scale (1&amp;ndash;10 km) magnetic field-aligned structures were observed in the pumped
volume of the ionosphere. The east-west motions of the airglow patches are also analyzed.</p>
</abstract>
<counts><page-count count="12"/></counts>
</article-meta>
</front>
<body/>
<back>
<ref-list>
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