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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-12-5319-2012</article-id>
<title-group>
<article-title>An isotopic analysis of ionising radiation as a source of sulphuric acid</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Enghoff</surname>
<given-names>M. B.</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>Bork</surname>
<given-names>N.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</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>Hattori</surname>
<given-names>S.</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>Meusinger</surname>
<given-names>C.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Nakagawa</surname>
<given-names>M.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Pedersen</surname>
<given-names>J. O. P.</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>Danielache</surname>
<given-names>S.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ueno</surname>
<given-names>Y.</given-names>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Johnson</surname>
<given-names>M. S.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Yoshida</surname>
<given-names>N.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Svensmark</surname>
<given-names>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>National Space Institute, Technical University of Denmark, 2100, Copenhagen Ø, Denmark</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Division of Atmospheric Science, Department of Physics, P.O. Box 64, 00014 University of Helsinki, Finland</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Department of Environmental Science and Technology, Interdisciplinary Graduate School of Science and Engineering, Tokyo Institute of Technology, Yokohama, 226-8502, Japan</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>University of Copenhagen, Department of Chemistry, 2100, Copenhagen Ø, Denmark</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Department of Environmental Chemistry and Engineering, Interdisciplinary Graduate School of Science and Engineering, Tokyo Institute of Technology, Yokohama, 226-8502, Japan</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>Department of Earth and Planetary Science, Tokyo Institute of Technology, Meguro-ku, Tokyo, 152-8551, Japan</addr-line>
</aff>
<pub-date pub-type="epub">
<day>19</day>
<month>06</month>
<year>2012</year>
</pub-date>
<volume>12</volume>
<issue>12</issue>
<fpage>5319</fpage>
<lpage>5327</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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<abstract>
<p>Sulphuric acid is an important factor in aerosol nucleation and growth. It
has been shown that ions enhance the formation of sulphuric acid aerosols,
but the exact mechanism has remained undetermined. Furthermore some studies
have found a deficiency in the sulphuric acid budget, suggesting a missing
source. In this study the production of sulphuric acid from SO&lt;sub&gt;2&lt;/sub&gt; through a
number of different pathways is investigated. The production methods are
standard gas phase oxidation by OH radicals produced by ozone photolysis with
UV light, liquid phase oxidation by ozone, and gas phase oxidation initiated
by gamma rays. The distributions of stable sulphur isotopes in the products
and substrate were measured using isotope ratio mass spectrometry. All
methods produced sulphate enriched in &lt;sup&gt;34&lt;/sup&gt;S and we find an enrichment factor (&amp;delta;&lt;sup&gt;34&lt;/sup&gt;S)
of 8.7 ± 0.4&amp;permil; (1 standard deviation) for the
UV-initiated OH reaction. Only UV light (Hg emission at 253.65 nm) produced a
clear non-mass-dependent excess of &lt;sup&gt;33&lt;/sup&gt;S. The pattern of isotopic
enrichment produced by gamma rays is similar, but not equal, to that produced
by aqueous oxidation of SO&lt;sub&gt;2&lt;/sub&gt; by ozone. This, combined with the relative
yields of the experiments, suggests a mechanism in which ionising radiation
may lead to hydrated ion clusters that serve as nanoreactors for S(IV) to
S(VI) conversion.</p>
</abstract>
<counts><page-count count="9"/></counts>
</article-meta>
</front>
<body/>
<back>
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