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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ACPD</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics Discussions</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACPD</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7375</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/acpd-8-10665-2008</article-id>
<title-group>
<article-title>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>
</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), Forschungszentrum Karlsruhe GmbH, 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>
<pub-date pub-type="epub">
<day>04</day>
<month>06</month>
<year>2008</year>
</pub-date>
<volume>8</volume>
<issue>3</issue>
<fpage>10665</fpage>
<lpage>10695</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>
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<self-uri xlink:href="http://www.atmos-chem-phys-discuss.net/8/10665/2008/acpd-8-10665-2008.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys-discuss.net/8/10665/2008/acpd-8-10665-2008.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 field observation of atmospheric NO&lt;sub&gt;3&lt;/sub&gt;. This device
combines the small size of the cavity with the enormous advantages of the
DOAS approach in terms of sensitivity and specificity. In particular, no
selective removal of the analyte (here NO&lt;sub&gt;3&lt;/sub&gt;) is necessary, thus the
CE-DOAS technique can &amp;ndash; in principle &amp;ndash; 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 satisfied for the
use of LEDs. The instrument was tested in the lab by detecting NO&lt;sub&gt;3&lt;/sub&gt; in a
mixture 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 NO&lt;sub&gt;3&lt;/sub&gt; concentrations as low as 6.3 ppt.</p>
</abstract>
<counts><page-count count="31"/></counts>
</article-meta>
</front>
<body/>
<back>
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</article>