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<article language="en">
	<journal>
		<journal_title>Atmospheric Chemistry and Physics Discussions</journal_title>
		<journal_url>www.atmos-chem-phys-discuss.net</journal_url>
		<issn>1680-7367</issn>
		<eissn>1680-7375</eissn>
		<volume_number>3</volume_number>
		<issue_number>5</issue_number>
		<publication_year>2003</publication_year>
	</journal>
	<doi>10.5194/acpd-3-4701-2003</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/3/4701/2003/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/3/4701/2003/acpd-3-4701-2003.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/3/4701/2003/acpd-3-4701-2003.pdf</fulltext_pdf>
	<start_page>4701</start_page>
	<end_page>4753</end_page>
	<publication_date>2003-09-05</publication_date>
	<article_title content_type="html">Halogen cycling and aerosol pH in the Hawaiian marine boundary layer</article_title>
	<authors>
		<author numeration="1" affiliations="1,7">
			<name>A. A. P. Pszenny</name>
		</author>
		<author numeration="2" affiliations="2,3">
			<name>J. Moldanová</name>
		</author>
		<author numeration="3" affiliations="4">
			<name>W. C. Keene</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>R. Sander</name>
		</author>
		<author numeration="5" affiliations="4">
			<name>J. R. Maben</name>
		</author>
		<author numeration="6" affiliations="5">
			<name>M. Martinez</name>
		</author>
		<author numeration="7" affiliations="2,6">
			<name>P. J. Crutzen</name>
		</author>
		<author numeration="8" affiliations="2">
			<name>D. Perner</name>
		</author>
		<author numeration="9" affiliations="1">
			<name>R. G. Prinn</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Center for Global Change Science, Massachusetts Institute of Technology, Cambridge, MA, USA</affiliation>
		<affiliation numeration="2" content_type="html">Air Chemistry Division, Max Planck Institute for Chemistry, Mainz, Germany</affiliation>
		<affiliation numeration="3" content_type="html">Swedish Environmental Research Institute, G¨otheborg, Sweden</affiliation>
		<affiliation numeration="4" content_type="html">Department of Environmental Sciences, University of Virginia, Charlottesville, VA, USA</affiliation>
		<affiliation numeration="5" content_type="html">Department of Meteorology, Pennsylvania State University, University Park, PA, USA; now at 2 (above)</affiliation>
		<affiliation numeration="6" content_type="html">Scripps Institution of Oceanography, University of California at San Diego, La Jolla, CA, USA</affiliation>
		<affiliation numeration="7" content_type="html">Now at: Institute for the Study of Earth, Oceans and Space, University of New Hampshire, Durham, and Mount Washington Observatory, North Conway, NH, USA</affiliation>
	</affiliations>
	<abstract content_type="html">Halogen species (HCl* (primarily HCl), Cl* (including
      Cl&lt;sub&gt;2&lt;/sub&gt; and HOCl), BrO,  total gaseous inorganic Br and size-resolved particulate
      Cl&lt;sup&gt;&amp;minus;&lt;/sup&gt; and Br &lt;sup&gt;&amp;minus;&lt;/sup&gt;) and related chemical and physical parameters were measured in surface air at Oahu, Hawaii during September
      1999. Aerosol pH as a function of particle size was inferred from phase partitioning and
      thermodynamic properties of HCl. Mixing ratios of halogen compounds and aerosol pHs
      were simulated with a new version of the photochemical box model MOCCA that
      considers multiple aerosol size bins.&lt;br&gt;
      &lt;br&gt;
      Inferred aerosol pHs ranged from 4.5 to 5.4 (median 5.1, n=22) for super-&lt;font     face=&quot;Symbol&quot;&gt;m&lt;/font&gt;m (primarily
      sea-salt) size fractions and 2.6 to 5.3 (median 4.6) for sub-&amp;mu;m (primarily
      sulphate) fractions. Simulated pHs for most sea-salt size bins were within the range of inferred
      values.  However, simulated pHs for the largest size fraction in the model were somewhat
      higher (oscillating around 5.9) due to the rapid turnover rates and relatively larger
      infusions of sea-salt alkalinity associated with fresh aerosols.&lt;br&gt;
      &lt;br&gt;
      Measured mixing ratios of HCl* ranged from &amp;lt;30 to 250 pmol mol&lt;sup&gt;-1&lt;/sup&gt; and those for
      Cl* from &amp;lt;6 to 38 pmol mol&lt;sup&gt;-1&lt;/sup&gt;. Simulated HCl and Cl*
      (Cl+ClO+HOCl+Cl&lt;sub&gt;2&lt;/sub&gt;) mixing ratios ranged between 20 and 70 pmol
      mol&lt;sup&gt;&amp;minus;1&lt;/sup&gt; and 0.5 and 6 pmol mol&lt;sup&gt;&amp;minus;1&lt;/sup&gt;, respectively. Afternoon
      HCl* maxima occurred on some days but consistent diel cycles for HCl* and Cl* were
      not observed. Simulated HCl did vary diurnally, peaking before dusk and reaching a
      minimum at dawn. While individual components of Cl* varied diurnally in the
      simulations, their sum did not, consistent with the lack of a diel cycle in observed Cl*.&lt;br&gt;
      &lt;br&gt;
      Mixing ratios of total gaseous inorganic Br varied from &amp;lt;1.5 to 9 pmol
      mol&lt;sup&gt;&amp;minus;1&lt;/sup&gt; and particulate Br &lt;sup&gt;&amp;minus;&lt;/sup&gt; deficits varied from 1 to 6 pmol
      mol&lt;sup&gt;&amp;minus;1&lt;/sup&gt; with values for both tending to be greater during daytime. Simulated mixing ratios of Br species were consistent with those
      of observed total gaseous inorganic Br, however the diel cycle was reversed with higher
      values predicted at night. This may be due to cloud processing, which is not considered in
      the current version of MOCCA. Measured BrO was never above detection limit
      (~2 pmol mol&lt;sup&gt;-1&lt;/sup&gt;) during the experiment, however relative changes in the BrO signal during the 3-hour
      period ending at 11:00 local time were mostly negative, averaging &amp;minus;0.3 pmol
      mol&lt;sup&gt;&amp;minus;1&lt;/sup&gt;. Both of these results are consistent with MOCCA simulations of BrO mixing ratios.&lt;br&gt;
      &lt;br&gt;
      Increasing the sea-salt mixing ratio in MOCCA by ~25% (within observed range) led to a
      decrease in O&lt;sub&gt;3&lt;/sub&gt; of ~16%. The chemistry leading to this decrease is complex and is tied to
      NO&lt;sub&gt;x&lt;/sub&gt; removal by heterogeneous reactions of BrNO&lt;sub&gt;3&lt;/sub&gt; and
      ClNO&lt;sub&gt;3&lt;/sub&gt;. The sink of O&lt;sub&gt;3&lt;/sub&gt; due to the catalytic Cl-ClO and Br-BrO cycles was estimated at
      &amp;minus;1.0 to &amp;minus;1.5 nmol mol&lt;sup&gt;&amp;minus;1&lt;/sup&gt; day&lt;sup&gt;&amp;minus;1&lt;/sup&gt;, a range similar to that due to
      O&lt;sub&gt;3&lt;/sub&gt; photolysis in the MOCCA simulations.</abstract>
	<references>
	</references>
</article>

