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<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>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7324</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/acp-10-11439-2010</article-id>
<title-group>
<article-title>Stability of temperatures from TIMED/SABER v1.07 (2002–2009) and Aura/MLS v2.2 (2004–2009) compared with OH(6-2) temperatures observed at Davis Station, Antarctica</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>French</surname>
<given-names>W. J. R.</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>Mulligan</surname>
<given-names>F. J.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Australian Antarctic Division, Kingston, Tasmania, Australia</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>National University of Ireland Maynooth, Co. Kildare, Ireland</addr-line>
</aff>
<pub-date pub-type="epub">
<day>03</day>
<month>12</month>
<year>2010</year>
</pub-date>
<volume>10</volume>
<issue>23</issue>
<fpage>11439</fpage>
<lpage>11446</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2010 W. J. R. French</copyright-statement>
<copyright-year>2010</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://acp.copernicus.org/articles/10/11439/2010/acp-10-11439-2010.html">This article is available from https://acp.copernicus.org/articles/10/11439/2010/acp-10-11439-2010.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/10/11439/2010/acp-10-11439-2010.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/10/11439/2010/acp-10-11439-2010.pdf</self-uri>
<abstract>
<p>Temperature profiles from two satellite instruments – TIMED/SABER and
Aura/MLS – have been used to calculate hydroxyl-layer equivalent
temperatures for comparison with values measured from OH(6-2) emission lines
observed by a ground-based spectrometer located at Davis Station, Antarctica
(68° S, 78° E). The profile selection criteria – miss-distance
&lt;500 km from the ground station and solar zenith angles &gt;97° –
yielded a total of 2359 SABER profiles over 8 years (2002–2009) and 7407 MLS
profiles over 5.5 years (2004–2009). The availability of simultaneous OH
volume emission rate (VER) profiles from the SABER (OH-B channel) enabled an
assessment of the impact of several different weighting functions in the
calculation of OH-equivalent temperatures. The maximum difference between
all derived hydroxyl layer equivalent temperatures was less than 3 K.
Restricting the miss-distance and miss-time criteria showed little effect on
the bias, suggesting that the OH layer is relatively uniform over the
spatial and temporal scales considered. However, a significant trend was
found in the bias between SABER and Davis OH of ~0.7 K/year over the
8-year period with SABER becoming warmer compared with the Davis OH
temperatures. In contrast, Aura/MLS exhibited a cold bias of 9.9 &amp;plusmn; 0.4 K
compared with Davis OH, but importantly, the bias remained constant over the
2004–2009 year period examined. The difference in bias behaviour of the two
satellites has significant implications for multi-annual and long-term
studies using their data.</p>
</abstract>
<counts><page-count count="8"/></counts>
</article-meta>
</front>
<body/>
<back>
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</article>