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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-9-7313-2009</article-id>
<title-group>
<article-title>Error correlation between CO&lt;sub&gt;2&lt;/sub&gt; and CO as constraint for CO&lt;sub&gt;2&lt;/sub&gt; flux inversions using satellite data</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Wang</surname>
<given-names>H.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Jacob</surname>
<given-names>D. J.</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>Kopacz</surname>
<given-names>M.</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>Jones</surname>
<given-names>D. B. A.</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>Suntharalingam</surname>
<given-names>P.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Fisher</surname>
<given-names>J. 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>Nassar</surname>
<given-names>R.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Pawson</surname>
<given-names>S.</given-names>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Nielsen</surname>
<given-names>J. E.</given-names>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>School of Engineering and Applied Sciences, Harvard University, Cambridge, MA, USA</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Smithsonian Astrophysical Observatory, Cambridge, MA, USA</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Department of Physics, University of Toronto, Toronto, Ontario, Canada</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>School of Environmental Sciences, University of East Anglia, Norwich, UK</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Department of Geography, University of Toronto, Toronto, Ontario, Canada</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>NASA Goddard Space Flight Center, Global Modeling and Assimilation Office, Greenbelt, MD, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>02</day>
<month>10</month>
<year>2009</year>
</pub-date>
<volume>9</volume>
<issue>19</issue>
<fpage>7313</fpage>
<lpage>7323</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2009 H. Wang et al.</copyright-statement>
<copyright-year>2009</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/9/7313/2009/acp-9-7313-2009.html">This article is available from https://acp.copernicus.org/articles/9/7313/2009/acp-9-7313-2009.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/9/7313/2009/acp-9-7313-2009.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/9/7313/2009/acp-9-7313-2009.pdf</self-uri>
<abstract>
<p>Inverse modeling of CO&lt;sub&gt;2&lt;/sub&gt; satellite observations to better quantify
carbon surface fluxes requires a chemical transport model (CTM) to
relate the fluxes to the observed column concentrations. CTM transport error
is a major source of uncertainty. We show that its effect can be reduced by
using CO satellite observations as additional constraint in a joint
CO&lt;sub&gt;2&lt;/sub&gt;-CO inversion. CO is measured from space with high precision, is
strongly correlated with CO&lt;sub&gt;2&lt;/sub&gt;, and is more sensitive than CO&lt;sub&gt;2&lt;/sub&gt; to
CTM transport errors on synoptic and smaller scales. Exploiting this
constraint requires statistics for the CTM transport error correlation
between CO&lt;sub&gt;2&lt;/sub&gt; and CO, which is significantly different from the
correlation between the concentrations themselves. We estimate the error
correlation globally and for different seasons by a paired-model method
(comparing GEOS-Chem CTM simulations of CO&lt;sub&gt;2&lt;/sub&gt; and CO columns using
different assimilated meteorological data sets for the same meteorological
year) and a paired-forecast method (comparing 48- vs. 24-h GEOS-5 CTM
forecasts of CO&lt;sub&gt;2&lt;/sub&gt; and CO columns for the same forecast time). We find
strong error correlations (&lt;i&gt;r&lt;/i&gt;&lt;sup&gt;2&lt;/sup&gt;&gt;0.5) between CO&lt;sub&gt;2&lt;/sub&gt; and CO columns
over much of the extra-tropical Northern Hemisphere throughout the year, and
strong consistency between different methods to estimate the error
correlation. Application of the averaging kernels used in the retrieval for
thermal IR CO measurements weakens the correlation coefficients by 15% on
average (mostly due to variability in the averaging kernels) but preserves
the large-scale correlation structure. We present a simple inverse modeling
application to demonstrate that CO&lt;sub&gt;2&lt;/sub&gt;-CO error correlations can indeed
significantly reduce uncertainty on surface carbon fluxes in a joint
CO&lt;sub&gt;2&lt;/sub&gt;-CO inversion vs. a CO&lt;sub&gt;2&lt;/sub&gt;-only inversion.</p>
</abstract>
<counts><page-count count="11"/></counts>
</article-meta>
</front>
<body/>
<back>
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