<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd">
<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>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acp-4-549-2004</article-id>
<title-group>
<article-title>Growth of upper tropospheric aerosols due to uptake of HNO&lt;sub&gt;3&lt;/sub&gt;</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Romakkaniemi</surname>
<given-names>S.</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>Kokkola</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>Petzold</surname>
<given-names>A.</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>Laaksonen</surname>
<given-names>A.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>University of Kuopio, Department of Applied Physics, Kuopio, Finland</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Deutsches Zentrum für Luft und Raumfahrt Oberpfaffenhofen, Institut für Physik der Atmosphäre, Wessling, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>03</month>
<year>2004</year>
</pub-date>
<volume>4</volume>
<issue>2</issue>
<fpage>549</fpage>
<lpage>556</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/4/549/2004/acp-4-549-2004.html">This article is available from http://www.atmos-chem-phys.net/4/549/2004/acp-4-549-2004.html</self-uri>
<self-uri xlink:href="http://www.atmos-chem-phys.net/4/549/2004/acp-4-549-2004.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys.net/4/549/2004/acp-4-549-2004.pdf</self-uri>
<abstract>
<p>The effect of nitric acid on the equilibrium size
distributions of upper tropospheric
aerosols is calculated as a function of relative humidity.
It is shown that HNO&lt;sub&gt;3&lt;/sub&gt; concentrations above a few tenths of a ppb can
cause substantial increases in haze mode particle concentrations
at relative humidities at about 60% and above. The effect can be
strongly magnified when letovicite particles are present in addition
to sulfuric acid aerosols. Letovicite particles are less acidic than
the sulfuric acid particles and so more nitric acid can be absorbed.
This effect can be seen even at RH below 50% due to the lowering of the
deliquescence RH of letovicite in the presence of gaseous nitric acid
at low temperatures. We have also compared equilibrium calculations
of the HNO&lt;sub&gt;3&lt;/sub&gt; effect with observations of increased
haze mode concentrations at relative humidities above 50%
(Petzold et al., 2000). Nitric acid
mixing ratios on the order of 0.5-2ppb may explain
the observed increase of haze mode particles at
least partially.</p>
</abstract>
<counts><page-count count="8"/></counts>
</article-meta>
</front>
<body/>
<back>
</back>
</article>