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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-10-7265-2010</article-id>
<title-group>
<article-title>Observations of OH and HO&lt;sub&gt;2&lt;/sub&gt; radicals over West Africa</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Commane</surname>
<given-names>R.</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>Floquet</surname>
<given-names>C. F. A.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</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>Ingham</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 contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Stone</surname>
<given-names>D.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Evans</surname>
<given-names>M. J.</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>Heard</surname>
<given-names>D. E.</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>School of Chemistry, University of Leeds, Leeds, UK</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>National Centre for Atmospheric Science, University of Leeds, Leeds, UK</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Institute for Climate And Atmospheric Science, School of Earth &amp; Environment, University of Leeds, Leeds, UK</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>now at: School of Engineering &amp; Applied Sciences, Harvard University, Cambridge, USA</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>now at: National Oceanography Centre, University of Southampton, Southampton, UK</addr-line>
</aff>
<pub-date pub-type="epub">
<day>18</day>
<month>03</month>
<year>2010</year>
</pub-date>
<volume>10</volume>
<issue>3</issue>
<fpage>7265</fpage>
<lpage>7322</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-discuss.net/10/7265/2010/acpd-10-7265-2010.html">This article is available from http://www.atmos-chem-phys-discuss.net/10/7265/2010/acpd-10-7265-2010.html</self-uri>
<self-uri xlink:href="http://www.atmos-chem-phys-discuss.net/10/7265/2010/acpd-10-7265-2010.pdf">The full text article is available as a PDF file from http://www.atmos-chem-phys-discuss.net/10/7265/2010/acpd-10-7265-2010.pdf</self-uri>
<abstract>
<p>The hydroxyl radical (OH) plays a key role in the oxidation of trace gases in
the troposphere. However, observations of OH and the closely related
hydroperoxy radical (HO&lt;sub&gt;2&lt;/sub&gt;) have been sparse, especially in the tropics.
Based on a low-pressure laser-induced fluorescence technique (FAGE –
Fluorescence Assay by Gas Expansion), an instrument has been developed to
measure OH and HO&lt;sub&gt;2&lt;/sub&gt; aboard the Facility for Airborne Atmospheric
Measurement (FAAM) BAe-146 research aircraft. The instrument is described and
the calibration method is discussed. During the African Monsoon
Multidisciplinary Analyses (AMMA) campaign, observations of OH and HO&lt;sub&gt;2&lt;/sub&gt;
(HO&lt;sub&gt;x&lt;/sub&gt;) were made in the boundary layer and free troposphere over West
Africa on 13 flights during July and August 2006. Mixing ratios of both OH
and HO&lt;sub&gt;2&lt;/sub&gt; were found to be highly variable but followed a diurnal cycle,
with a median HO&lt;sub&gt;2&lt;/sub&gt;/OH ratio of 95. Daytime OH observations were compared
with the primary production rate of OH from ozone photolysis in the presence
of water vapour. Daytime HO&lt;sub&gt;2&lt;/sub&gt; observations were generally reproduced by a
simple steady-state HO&lt;sub&gt;x&lt;/sub&gt; calculation, where HO&lt;sub&gt;x&lt;/sub&gt; was assumed
to be formed from the primary production of OH and lost through HO&lt;sub&gt;2&lt;/sub&gt;
self-reaction. Deviations between the observations and this simple model were
found to be grouped into a number of specific cases: (a) in the presence of
high levels of isoprene in the boundary layer, (b) within a biomass burning
plume and (c) within cloud. In the forested boundary layer, HO&lt;sub&gt;2&lt;/sub&gt; was
underestimated at altitudes below 500 m but overestimated between 500 m and
2 km. In the biomass burning plume, OH and HO&lt;sub&gt;2&lt;/sub&gt; were both significantly
reduced compared to calculations. HO&lt;sub&gt;2&lt;/sub&gt; was sampled in and around cloud,
with significant short-lived reductions of HO&lt;sub&gt;2&lt;/sub&gt; observed. HO&lt;sub&gt;2&lt;/sub&gt;
observations were better reproduced by a steady state calculation with
heterogeneous loss of HO&lt;sub&gt;2&lt;/sub&gt; onto cloud droplets included. Up to 9 pptv of
HO&lt;sub&gt;2&lt;/sub&gt; was observed at night, increasing early in the morning. Potential
sources of high altitude HO&lt;sub&gt;2&lt;/sub&gt; at night are also discussed.</p>
</abstract>
<counts><page-count count="58"/></counts>
</article-meta>
</front>
<body/>
<back>
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