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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>Springer Verlag</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.1007/s00585-000-0215-7</article-id>
<title-group>
<article-title>Irregular structures observed below 71 km in the night-time polar D-region</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Thrane</surname>
<given-names>E. V.</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="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Blix</surname>
<given-names>T. A.</given-names>
</name>
<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="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Svenes</surname>
<given-names>K. R.</given-names>
</name>
<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="aff4">
<sup>4</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Norwegian Defence Research Establishment, P O Box 25, NO-2027 Kjeller, Norway</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>E-mail: eivind-wilhelm.thrane@ffi.no</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Institute of Physics, University in Oslo, P O Box 1048, Blindern, NO-0316 Oslo, Norway</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>&lt;i&gt;Correspondence to:&lt;/i&gt; E. V. Thrane</addr-line>
</aff>
<pub-date pub-type="epub">
<day>29</day>
<month>02</month>
<year>2000</year>
</pub-date>
<volume>18</volume>
<issue>2</issue>
<fpage>215</fpage>
<lpage>222</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2000 E. V. Thrane et al.</copyright-statement>
<copyright-year>2000</copyright-year>
<license license-type="open-access">
<license-p>© European Geosciences Union 2000</license-p>
</license>
</permissions>
<self-uri xlink:href="https://angeo.copernicus.org/articles/18/215/2000/angeo-18-215-2000.html">This article is available from https://angeo.copernicus.org/articles/18/215/2000/angeo-18-215-2000.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/18/215/2000/angeo-18-215-2000.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/18/215/2000/angeo-18-215-2000.pdf</self-uri>
<abstract>
<p>A new rocket range, SvalRak, was opened in
November 1997 at Ny-Ålesund (79°N) in the Svalbard archipelago. The first
instrumented rocket was launched on 20 November, 1997, at 1730 UT during
geomagnetically quiet conditions. The payload was instrumented to measure plasma
parameters in the mesosphere and lower thermosphere, but the payload only
reached an altitude of 71 km. This resulted in a very flat trajectory through
the lower D-region. The positive ion concentrations were larger than expected,
and some unexpected plasma irregularities were observed below 71 km. The
irregularities were typically 100 m in spatial extent, with plasma densities a
factor of two to five above the ambient background. In the dark polar night the
plasma below 71 km must consist mainly of positive and negative ions and the
only conceivable ionising radiation is a flux of energetic particles.
Furthermore only relativistic electrons have the large energies and the small
gyro radii required in order to explain the observed spatial structure. The
source of these electrons is uncertain.&lt;/p&gt;
&lt;p  style=&quot;line-height: 20px;&quot;&gt;&lt;b&gt;Key words: &lt;/b&gt;Ionosphere (ionospheric irregularities;
ionization mechanisms) - Magnetospheric physics (polar cap phenomena)</p>
</abstract>
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