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<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" article-type="research-article" dtd-version="3.0" xml:lang="en">
<front>
<journal-meta>
<journal-id journal-id-type="publisher">ACP</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7324</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-4-685-2004</article-id>
<title-group>
<article-title>Aspect sensitivity of VHF echoes from field aligned irregularities in meteor trails and thin ionization layers</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Zhou</surname>
<given-names>Q. H.</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>Morton</surname>
<given-names>Y. 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>Mathews</surname>
<given-names>J. D.</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>Janches</surname>
<given-names>D.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Electrical and Computer Engineering Department, Miami University, Oxford, OH, USA</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>CSSL, Pennsylvania State University, University Park, PA, USA</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Arecibo Observatory, Arecibo, Puerto Rico</addr-line>
</aff>
<pub-date pub-type="epub">
<day>07</day>
<month>05</month>
<year>2004</year>
</pub-date>
<volume>4</volume>
<issue>3</issue>
<fpage>685</fpage>
<lpage>692</lpage>
<permissions>
<license xlink:type="simple">
<license-p>This is an open-access article ditributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.</license-p>
</license>
</permissions>
<self-uri xlink:href="http://www.atmos-chem-phys.net/4/685/2004/acp-4-685-2004.html">This article is available from http://www.atmos-chem-phys.net/4/685/2004/acp-4-685-2004.html</self-uri>
<self-uri xlink:href="http://www.atmos-chem-phys.net/4/685/2004/acp-4-685-2004.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/4/685/2004/acp-4-685-2004.pdf</self-uri>
<abstract>
<p>The aspect sensitivity of VHF echoes from field aligned irregularities (FAI)
within meteor trails and thin ionization layers is studied using numerical
models. Although the maximum power is obtained when a radar is pointed
perpendicular to the field line (&lt;IMG WIDTH=&quot;15&quot; HEIGHT=&quot;14&quot; ALIGN=&quot;BOTTOM&quot; BORDER=&quot;0&quot;
   src=&quot;acp-4-685-img1.gif&quot;  
 ALT=&quot;$bot$&quot;&gt;&lt;B&gt;B&lt;/B&gt;), substantial power can
be obtained off the &lt;IMG WIDTH=&quot;15&quot; HEIGHT=&quot;14&quot; ALIGN=&quot;BOTTOM&quot; BORDER=&quot;0&quot;
   src=&quot;acp-4-685-img1.gif&quot;  
 ALT=&quot;$bot$&quot;&gt;&lt;B&gt;B&lt;/B&gt; direction if the ionization
trail/layer is thin. When the FAI length along &lt;B&gt;B&lt;/B&gt; is 20 m, the power
observed 6&amp;deg; off &lt;IMG WIDTH=&quot;15&quot; HEIGHT=&quot;14&quot; ALIGN=&quot;BOTTOM&quot; BORDER=&quot;0&quot;
   src=&quot;acp-4-685-img1.gif&quot;  
 ALT=&quot;$bot$&quot;&gt;&lt;B&gt;B&lt;/B&gt; is about 10 db below that
perpendicular to the &lt;B&gt;B&lt;/B&gt; direction. Meteoric FAI echoes can
potentially be used to determine the diffusion rate in the mesopause region.
Based on the aspect sensitivity analysis, we conclude that the range spread
trail echoes far off &lt;IMG WIDTH=&quot;15&quot; HEIGHT=&quot;14&quot; ALIGN=&quot;BOTTOM&quot; BORDER=&quot;0&quot;
   src=&quot;acp-4-685-img1.gif&quot;  
 ALT=&quot;$bot$&quot;&gt;&lt;B&gt;B&lt;/B&gt; observed by powerful VHF radars are
likely due to overdense meteors. Our simulation also shows that ionospheric
FAI echoes can have an altitude smearing effect of about 4 km if the
vertical extension of a FAI-layer is around 100 m, which has often been
observed at Arecibo. The altitude smearing effect can account for the fact
that the Es-layers observed by the Arecibo incoherent scatter radar are
typically much narrower than FAI-layers and the occurrence of double
spectral peaks around the Es-layer altitude in FAI echoes.</p>
</abstract>
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