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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-30-929-2012</article-id>
<title-group>
<article-title>Electron radiation belt data assimilation with an ensemble Kalman filter relying on the Salammbô code</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Bourdarie</surname>
<given-names>S. 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>Maget</surname>
<given-names>V. F.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>ONERA the French Aerospace lab, Toulouse, France</addr-line>
</aff>
<pub-date pub-type="epub">
<day>08</day>
<month>06</month>
<year>2012</year>
</pub-date>
<volume>30</volume>
<issue>6</issue>
<fpage>929</fpage>
<lpage>943</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2012 S. A. Bourdarie</copyright-statement>
<copyright-year>2012</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/30/929/2012/angeo-30-929-2012.html">This article is available from https://angeo.copernicus.org/articles/30/929/2012/angeo-30-929-2012.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/30/929/2012/angeo-30-929-2012.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/30/929/2012/angeo-30-929-2012.pdf</self-uri>
<abstract>
<p>In this study we implement a data assimilation tool using a 3-D radiation
belt model and an ensemble Kalman filter approach. High time and space
reanalysis of the electron radiation belt fluxes is obtained over the time
period 5 October to 25 October 1990 by combining sparse
observations with the Salammbô 3-D model in an optimal way. The
convergence of the ensemble Kalman filter is analyzed carefully. The risk of
using a biased physical model is discussed and relative consequences are
highlighted. Finally, a validation against CRRES data and major improvements
compared to pure physics based model are presented.</p>
</abstract>
<counts><page-count count="15"/></counts>
</article-meta>
</front>
<body/>
<back>
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