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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-24-1281-2006</article-id>
<title-group>
<article-title>A high-resolution study of mesospheric fine structure with the Jicamarca MST radar</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sheth</surname>
<given-names>R.</given-names>
</name>
<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>Kudeki</surname>
<given-names>E.</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>Lehmacher</surname>
<given-names>G.</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>Sarango</surname>
<given-names>M.</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>Woodman</surname>
<given-names>R.</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>Chau</surname>
<given-names>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>Guo</surname>
<given-names>L.</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>Reyes</surname>
<given-names>P.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>University of Illinois at Urbana-Champaign, IL 61801, USA</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Clemson University, Clemson, SC 29634, USA</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Jicamarca Radio Observatory, Lima 13, Peru</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>now at: Lincoln Laboratories, Lexington, MA 02420, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>03</day>
<month>07</month>
<year>2006</year>
</pub-date>
<volume>24</volume>
<issue>5</issue>
<fpage>1281</fpage>
<lpage>1293</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2006 R. Sheth et al.</copyright-statement>
<copyright-year>2006</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/24/1281/2006/angeo-24-1281-2006.html">This article is available from https://angeo.copernicus.org/articles/24/1281/2006/angeo-24-1281-2006.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/24/1281/2006/angeo-24-1281-2006.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/24/1281/2006/angeo-24-1281-2006.pdf</self-uri>
<abstract>
<p>Correlation studies performed on data from recent mesospheric experiments
conducted with the 50-MHz Jicamarca radar in May 2003 and July 2004
are reported. The study is based on signals detected from a combination
of vertical and off-vertical beams. The nominal height resolution
was 150 m and spectral estimates were obtained after ~1 min integration. Spectral widths and backscattered power generally
show positive correlations at upper mesospheric heights in agreement
with earlier findings (e.g., Fukao et al., 1980) that upper mesospheric
echoes are dominated by isotropic Bragg scatter. In many instances
in the upper mesosphere, a weakening of positive correlation away
from layer centers (towards top and bottom boundaries) was observed
with the aid of improved height resolution. This finding supports
the idea that layer edges are dominated by anisotropic turbulence. The data
also suggests that negative correlations observed at lower mesospheric
heights are caused by scattering from anisotropic structures rather
than reflections from sharp vertical gradients in electron density.</p>
</abstract>
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