<?xml version="1.0" encoding="utf-8" standalone="no"?>
<!DOCTYPE article SYSTEM "http://www.atmos-chem-phys.net/inc/acp/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>Atmospheric Chemistry and Physics</journal_title>
		<journal_url>www.atmos-chem-phys.net</journal_url>
		<issn>1680-7316</issn>
		<eissn>1680-7324</eissn>
		<volume_number>4</volume_number>
		<issue_number>1</issue_number>
		<publication_year>2004</publication_year>
	</journal>
	<doi>10.5194/acp-4-147-2004</doi>
	<article_url>http://www.atmos-chem-phys.net/4/147/2004/</article_url>
	<abstract_html>http://www.atmos-chem-phys.net/4/147/2004/acp-4-147-2004.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys.net/4/147/2004/acp-4-147-2004.pdf</fulltext_pdf>
	<start_page>147</start_page>
	<end_page>168</end_page>
	<publication_date>2004-02-03</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, Göteborg, 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;-&lt;/sup&gt; and Br &lt;sup&gt;-&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-&lt;font face=&quot;Symbol&quot;&gt;m&lt;/font&gt;m (primarily
      sulphate) fractions. Inferred daytime pHs tended to be slightly lower than those at night, although
      daytime median values did not differ statistically from nighttime medians. 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;-1&lt;/sup&gt; and 0.5 and 6 pmol mol&lt;sup&gt;-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;-1&lt;/sup&gt; and particulate Br &lt;sup&gt;-&lt;/sup&gt; deficits varied from 1 to
      6 pmol mol&lt;sup&gt;-1&lt;/sup&gt; with values for both tending to be greater during daytime.  Simulated
      Br&lt;sub&gt;t&lt;/sub&gt; and Br &lt;sup&gt;-&lt;/sup&gt; mixing ratios and enrichment factors (EFBr) were similar to those observed, with early
      morning maxima and dusk minima.  However, the diel cycles differed in detail among the various simulations. In low-salt simulations, halogen
      cycling was less intense, Br &lt;sup&gt;-&lt;/sup&gt; accumulated and Br&lt;sub&gt;t&lt;/sub&gt; and
      EFBr increased slowly overnight. In higher-salt simulations with more intense halogen cycling,
      Br &lt;sup&gt;-&lt;/sup&gt; and EFBr decreased and Br&lt;sub&gt;t&lt;/sub&gt; increased rapidly after dusk. Cloud processing, which is not
      considered in this version of MOCCA, may also affect these diel cycles (von Glasow et al., 2003).  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 -0.3 pmol mol&lt;sup&gt;-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 -1.0 to -1.5 nmol mol&lt;sup&gt;-1&lt;/sup&gt; day&lt;sup&gt;-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>

