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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>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-10-3901-2010</article-id>
<title-group>
<article-title>Technical Note: Using a high finesse optical resonator to provide a long light path for differential optical absorption spectroscopy: CE-DOAS</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Meinen</surname>
<given-names>J.</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>Thieser</surname>
<given-names>J.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</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>Platt</surname>
<given-names>U.</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>Leisner</surname>
<given-names>T.</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-group><aff id="aff1">
<label>1</label>
<addr-line>Institute for Meteorology and Climate Research, Aerosols and Heterogeneous Chemistry in the Atmosphere (IMK-AAF), Karlsruhe Institute of Technology (KIT), Germany</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Institut for Environmental Physics (IUP), Atmosphere and Remote Sensing, Ruprecht-Karls-Universität Heidelberg, Germany</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>now at: Department of Atmospheric Chemistry, Max Planck Institute for Chemistry, Mainz Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>27</day>
<month>04</month>
<year>2010</year>
</pub-date>
<volume>10</volume>
<issue>8</issue>
<fpage>3901</fpage>
<lpage>3914</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/10/3901/2010/acp-10-3901-2010.html">This article is available from http://www.atmos-chem-phys.net/10/3901/2010/acp-10-3901-2010.html</self-uri>
<self-uri xlink:href="http://www.atmos-chem-phys.net/10/3901/2010/acp-10-3901-2010.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/10/3901/2010/acp-10-3901-2010.pdf</self-uri>
<abstract>
<p>Cavity enhanced methods in absorption spectroscopy have seen a considerable
increase in popularity during the past decade. Especially Cavity Enhanced
Absorption Spectroscopy (CEAS) established itself in atmospheric trace gas
detection by providing tens of kilometers of effective light path length
using a cavity as short as 1 m. In this paper we report on the construction
and testing of a compact and power efficient light emitting diode based
broadband Cavity Enhanced Differential Optical Absorption Spectrometer
(CE-DOAS) for in situ observation of atmospheric NO&lt;sub&gt;3&lt;/sub&gt;. This device
combines the small size of the cavity with the advantages of the DOAS
approach in terms of sensitivity, specificity and insensivity to intensity
fluctuations of the light source. In particular, no selective removal of the
analyte (here NO&lt;sub&gt;3&lt;/sub&gt;) is necessary for calibration of the instrument if
appropriate corrections are applied to the CEAS theory. Therefore the
CE-DOAS technique can – in principle – measure any gas detectable by DOAS.
We will discuss the advantages of using a light emitting diode (LED) as
light source particularly the precautions which have to be considered for
the use of LEDs with a broad wavelength range. The instrument was tested in
the lab by detecting NO&lt;sub&gt;3&lt;/sub&gt; formed by mixing of NO&lt;sub&gt;2&lt;/sub&gt; and O&lt;sub&gt;3&lt;/sub&gt; in
air. It was then compared to other trace gas detection techniques in an
intercomparison campaign in the atmosphere simulation chamber SAPHIR at
Forschungszentrum Jülich at NO&lt;sub&gt;3&lt;/sub&gt; concentrations as low as 6.3 ppt.</p>
</abstract>
<counts><page-count count="14"/></counts>
</article-meta>
</front>
<body/>
<back>
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</article>