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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>
</journal-title-group>
<issn pub-type="epub">1680-7324</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>GÃ¶ttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-6-3517-2006</article-id>
<title-group>
<article-title>Measuring atmospheric CO&lt;sub&gt;2&lt;/sub&gt; from space using Full Spectral Initiation (FSI) WFM-DOAS</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Barkley</surname>
<given-names>M. P.</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>FrieÃŸ</surname>
<given-names>U.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Monks</surname>
<given-names>P. S.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>EOS, Space Research Centre, Department of Physics &amp; Astronomy, University of Leicester, Leicester, LE1 7RH, UK</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Department of Chemistry, University of Leicester, Leicester, LE1 7RH, UK</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>now at: Institute of Environmental Physics, Heidelberg, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>08</month>
<year>2006</year>
</pub-date>
<volume>6</volume>
<issue>11</issue>
<fpage>3517</fpage>
<lpage>3534</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/6/3517/2006/acp-6-3517-2006.html">This article is available from http://www.atmos-chem-phys.net/6/3517/2006/acp-6-3517-2006.html</self-uri>
<self-uri xlink:href="http://www.atmos-chem-phys.net/6/3517/2006/acp-6-3517-2006.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/6/3517/2006/acp-6-3517-2006.pdf</self-uri>
<abstract>
<p>Satellite measurements of atmospheric CO&lt;sub&gt;2&lt;/sub&gt; concentrations are a
rapidly evolving area of scientific research which  can help reduce
the uncertainties in the global carbon cycle fluxes and provide
insight into surface sources and sinks. One of the emerging CO&lt;sub&gt;2&lt;/sub&gt;
measurement techniques is a relatively new retrieval algorithm
called Weighting Function Modified Differential Optical Absorption
Spectroscopy (WFM-DOAS) that has been developed by
Buchwitz et al. (2000). This algorithm is designed to
measure the total columns of CO&lt;sub&gt;2&lt;/sub&gt; (and other greenhouse gases)
through the application to spectral measurements in the near
infrared (NIR), made by the SCIAMACHY instrument on-board ENVISAT.
The algorithm itself is based on fitting the logarithm of a model
reference spectrum and its derivatives to the logarithm of the ratio
of a measured nadir radiance and solar irradiance spectrum. In this
work, a detailed error assessment of this technique has been
conducted and it has been found necessary to include suitable a
priori information within the retrieval in order to minimize the
errors on the retrieved CO&lt;sub&gt;2&lt;/sub&gt; columns. Hence, a more flexible
implementation of the retrieval technique, called Full Spectral
Initiation (FSI) WFM-DOAS, has been developed which generates a
reference spectrum for each individual SCIAMACHY observation using
the estimated properties of the atmosphere and surface at the time
of the measurement. Initial retrievals over Siberia during the
summer of 2003 show that the measured CO&lt;sub&gt;2&lt;/sub&gt; columns are not biased
from the input a priori data and that whilst the monthly averaged
CO&lt;sub&gt;2&lt;/sub&gt; distributions contain a high degree of variability, they also
contain interesting spatial features.</p>
</abstract>
<counts><page-count count="18"/></counts>
</article-meta>
</front>
<body/>
<back>
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