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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-10-2879-2010</article-id>
<title-group>
<article-title>Toward real-time measurement of atmospheric mercury concentrations using cavity ring-down spectroscopy</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Faïn</surname>
<given-names>X.</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>Moosmüller</surname>
<given-names>H.</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>Obrist</surname>
<given-names>D.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Division of Atmospheric Sciences, Desert Research Institute, 2215 Raggio Parkway, Reno, NV 89512, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>26</day>
<month>03</month>
<year>2010</year>
</pub-date>
<volume>10</volume>
<issue>6</issue>
<fpage>2879</fpage>
<lpage>2892</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.net/10/2879/2010/acp-10-2879-2010.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/10/2879/2010/acp-10-2879-2010.pdf</self-uri>
<abstract>
<p>Cavity ring-down spectroscopy (CRDS) is a direct absorption technique that
utilizes path lengths up to multiple kilometers in a compact absorption cell
and has a significantly higher sensitivity than conventional absorption
spectroscopy. This tool opens new prospects for study of gaseous elemental
mercury (Hg&lt;sup&gt;0&lt;/sup&gt;) because of its high temporal resolution and reduced sample
volume requirements (&amp;lt;0.5 l of sample air). We developed a new sensor
based on CRDS for measurement of (Hg&lt;sup&gt;0&lt;/sup&gt;) mass concentration. Sensor
characteristics include sub-ng m&lt;sup&gt;&amp;minus;3&lt;/sup&gt; detection limit and high temporal
resolution using a frequency-doubled, tuneable dye laser emitting pulses at
~253.65 nm with a pulse repetition frequency of 50 Hz. The dye laser
incorporates a unique piezo element attached to its tuning grating allowing
it to tune the laser on and off the Hg&lt;sup&gt;0&lt;/sup&gt; absorption line on a
pulse-to-pulse basis to facilitate differential absorption measurements.
Hg&lt;sup&gt;0&lt;/sup&gt; absorption measurements with this CRDS laboratory prototype are highly
linearly related to Hg&lt;sup&gt;0&lt;/sup&gt; concentrations determined by a Tekran 2537B
analyzer over an Hg&lt;sup&gt;0&lt;/sup&gt; concentration range from 0.2 ng m&lt;sup&gt;&amp;minus;3&lt;/sup&gt; to
573 ng m&lt;sup&gt;&amp;minus;3&lt;/sup&gt;, implying excellent linearity of both instruments. The
current CRDS instrument has a sensitivity of 0.10 ng Hg&lt;sup&gt;0&lt;/sup&gt; m&lt;sup&gt;&amp;minus;3&lt;/sup&gt; at
10-s time resolution. Ambient-air tests showed that background Hg&lt;sup&gt;0&lt;/sup&gt; levels
can be detected at low temporal resolution (i.e., 1 s), but also highlight a
need for high-frequency (i.e., pulse-to-pulse) differential on/off-line
tuning of the laser wavelength to account for instabilities of the CRDS
system and variable background absorption interferences. Future applications
may include ambient Hg&lt;sup&gt;0&lt;/sup&gt; flux measurements with eddy covariance techniques,
which require measurements of Hg&lt;sup&gt;0&lt;/sup&gt; concentrations with sub-ng m&lt;sup&gt;&amp;minus;3&lt;/sup&gt;
sensitivity and sub-second time resolution.</p>
</abstract>
<counts><page-count count="14"/></counts>
</article-meta>
</front>
<body/>
<back>
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</article>