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<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" article-type="research-article" dtd-version="3.0" xml:lang="en">
<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>GÃ¶ttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-8-4997-2008</article-id>
<title-group>
<article-title>Laboratory studies of H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;/H&lt;sub&gt;2&lt;/sub&gt;O binary homogeneous nucleation from the SO&lt;sub&gt;2&lt;/sub&gt;+OH reaction: evaluation of the experimental setup and preliminary results</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Young</surname>
<given-names>L. H.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Benson</surname>
<given-names>D. R.</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>Kameel</surname>
<given-names>F. R.</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>Pierce</surname>
<given-names>J. R.</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>Junninen</surname>
<given-names>H.</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>Kulmala</surname>
<given-names>M.</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>Lee</surname>
<given-names>S.-H.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Kent State University, Department of Chemistry, Kent, OH, USA</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>NASA Goddard Space Flight Center, MD, USA</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>University of Helsinki, Department of Physical Sciences, Helsinki, Finland</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>now at: China Medical University, Department of Occupational Safety and Health, Taichung, Taiwan</addr-line>
</aff>
<pub-date pub-type="epub">
<day>28</day>
<month>08</month>
<year>2008</year>
</pub-date>
<volume>8</volume>
<issue>16</issue>
<fpage>4997</fpage>
<lpage>5016</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/8/4997/2008/acp-8-4997-2008.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/8/4997/2008/acp-8-4997-2008.pdf</self-uri>
<abstract>
<p>Binary homogeneous nucleation (BHN) of sulphuric acid and water
(H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;/H&lt;sub&gt;2&lt;/sub&gt;O) is one of the most important atmospheric
nucleation processes, but laboratory observations of this nucleation process
are very limited and there are also large discrepancies between different
laboratory studies. The difficulties associated with these experiments
include wall loss of H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt; and uncertainties in estimation of
H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt; concentration ([H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;]) involved in nucleation.
We have developed a new laboratory nucleation setup to study
H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;/H&lt;sub&gt;2&lt;/sub&gt;O BHN kinetics and provide relatively constrained
[H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;] needed for nucleation. H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt; is produced from
the SO&lt;sub&gt;2&lt;/sub&gt;+OHâ†’HSO&lt;sub&gt;3&lt;/sub&gt; reaction and OH radicals are produced
from water vapor UV absorption. The residual [H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;] were measured
at the end of the nucleation reactor with a chemical ionization mass
spectrometer (CIMS). Wall loss factors (WLFs) of H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt; were
estimated by assuming that wall loss is diffusion limited and these
calculated WLFs were in good agreement with simultaneous measurements of the
initial and residual [H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;] with two CIMSs. The nucleation zone
was estimated from numerical simulations based on the measured aerosol sizes
(particle diameter, &lt;i&gt;D&lt;/i&gt;&lt;sub&gt;&lt;i&gt;p&lt;/i&gt;&lt;/sub&gt;) and [H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;]. The measured BHN rates
(&lt;i&gt;J&lt;/i&gt;) ranged from 0.01â€“220 cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt; s&lt;sup&gt;&amp;minus;1&lt;/sup&gt; at the initial and residual
[H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;] from 10&lt;sup&gt;8&lt;/sup&gt;&amp;minus;10&lt;sup&gt;10&lt;/sup&gt; cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt;, a temperature of 288 K
and relative humidity (RH) from 11â€“23%; &lt;i&gt;J&lt;/i&gt; increased with increasing
[H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;] and RH. &lt;i&gt;J&lt;/i&gt; also showed a power dependence on
[H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;] with the exponential power of 3â€“8. These power dependences
are consistent with other laboratory studies under similar [H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;]
and RH, but different from atmospheric field observations which showed that
particle number concentrations are often linearly dependent on
[H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;]. These results, together with a higher [H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;]
threshold (10&lt;sup&gt;8&lt;/sup&gt;â€“10&lt;sup&gt;9&lt;/sup&gt; cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt;) needed to produce the unit &lt;i&gt;J&lt;/i&gt; measured
from the laboratory studies compared to the atmospheric conditions
(10&lt;sup&gt;6&lt;/sup&gt;â€“10&lt;sup&gt;7&lt;/sup&gt; cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt;), imply that H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;/H&lt;sub&gt;2&lt;/sub&gt;O BHN
alone is insufficient to explain atmospheric aerosol formation and growth.
Particle growth rates estimated from the measured aerosol size
distributions, residence times (&lt;i&gt;t&lt;/i&gt;&lt;sub&gt;&lt;i&gt;r&lt;/i&gt;&lt;/sub&gt;), and [H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;] were
100â€“500 nm h&lt;sup&gt;&amp;minus;1&lt;/sup&gt;, much higher than those seen from atmospheric field
observations, because of the higher [H&lt;sub&gt;2&lt;/sub&gt;SO&lt;sub&gt;4&lt;/sub&gt;] used in our study.</p>
</abstract>
<counts><page-count count="20"/></counts>
</article-meta>
</front>
<body/>
<back>
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