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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ACPD</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics Discussions</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACPD</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7375</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/acpd-10-23197-2010</article-id>
<title-group>
<article-title>Aura MLS observations of the westward-propagating &lt;i&gt;s&lt;/i&gt;=1, 16-day planetary wave in the middle atmosphere: climatology and cross-equatorial propagation</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Day</surname>
<given-names>K. 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>Hibbins</surname>
<given-names>R. E.</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>Mitchell</surname>
<given-names>N. J.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Centre for Space, Atmospheric and Oceanic Science, Department of Electronic and Electrical  Engineering, The University of Bath, BA2 7AY, UK</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>British Antarctic Survey, Cambridge, CB3 0ET, UK</addr-line>
</aff>
<pub-date pub-type="epub">
<day>07</day>
<month>10</month>
<year>2010</year>
</pub-date>
<volume>10</volume>
<issue>10</issue>
<fpage>23197</fpage>
<lpage>23227</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>
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<self-uri xlink:href="http://www.atmos-chem-phys-discuss.net/10/23197/2010/acpd-10-23197-2010.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys-discuss.net/10/23197/2010/acpd-10-23197-2010.pdf</self-uri>
<abstract>
<p>The Microwave Limb Sounder (MLS) on the Aura satellite has been used to measure temperatures
   in the stratosphere, mesosphere and lower thermosphere (MLT). The data used here are from
   August 2004 to June 2010 and latitudes 75&amp;deg; S to 75&amp;deg; N. The temperature
   data reveal the persistent presence of a westward propagating 16-day planetary wave with
   zonal wavenumber 1. The wave amplitude maximises in winter in the stratosphere and MLT at
   middle to high latitudes, where monthly-mean amplitudes can be as large as ~8 K. 
   Significant wave amplitudes are observed in the summer-time MLT and at lower
   stratospheric heights of up to ~20 km at middle to high latitudes. Wave amplitudes in
   the Northern Hemisphere approach values twice as large as those in the Southern
   Hemisphere. Wave amplitudes are also closely related to climatological zonal winds and are
   largest in regions of strongest eastward flow. There is a~reduction in wave amplitudes at
   the stratopause. No significant wave amplitude is observed near the equator or in the
   strongly westward background winds of the atmosphere in summer. This behaviour is
   interpreted as a consequence of wave/mean-flow interactions. It has been suggested that the
   summer-time 16-day wave in the MLT is ducted across the equator from the winter hemisphere
   and that this ducting is modulated by the equatorial Quasi-Biennial Oscillation (QBO) in the
   westerly phase. Here we observe that the QBO modulates the 16-day wave in the polar
   summer-time MLT in the Northern Hemisphere as previously observed, but this modulation is
   not seen in the Southern Hemisphere.</p>
</abstract>
<counts><page-count count="31"/></counts>
</article-meta>
</front>
<body/>
<back>
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