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<!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>3</volume_number>
		<issue_number>5</issue_number>
		<publication_year>2003</publication_year>
	</journal>
	<doi>10.5194/acp-3-1709-2003</doi>
	<article_url>http://www.atmos-chem-phys.net/3/1709/2003/</article_url>
	<abstract_html>http://www.atmos-chem-phys.net/3/1709/2003/acp-3-1709-2003.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys.net/3/1709/2003/acp-3-1709-2003.pdf</fulltext_pdf>
	<start_page>1709</start_page>
	<end_page>1723</end_page>
	<publication_date>2003-10-14</publication_date>
	<article_title content_type="html">On the relationship between acetone and carbon monoxide in different air masses</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>M. de Reus</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>H. Fischer</name>
		</author>
		<author numeration="3" affiliations="3">
			<name>F. Arnold</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>J. de Gouw</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>R. Holzinger</name>
		</author>
		<author numeration="6" affiliations="2">
			<name>C Warneke</name>
		</author>
		<author numeration="7" affiliations="1">
			<name>J. Williams</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Max Planck Institute for Chemistry, Airchemistry Department, Mainz, Germany</affiliation>
		<affiliation numeration="2" content_type="html">National Oceanic and Atmospheric Administration (NOAA), Aeronomy Laboratory, Boulder, USA</affiliation>
		<affiliation numeration="3" content_type="html">Max Planck Institute for Nuclear Physics, Atmospheric Physics Division, Heidelberg, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">Carbon monoxide and acetone measurements are presented for five aircraft
      measurement campaigns at mid-latitudes, polar and tropical regions in the northern hemisphere. Throughout all campaigns, free tropospheric air
      masses, which were influenced by anthropogenic emissions, showed a similar
      linear relation between acetone and CO, with a slope of 21-25 ppt&lt;sub&gt;v&lt;/sub&gt;
      acetone/ppb&lt;sub&gt;v&lt;/sub&gt; CO. Measurements in the anthropogenically influenced marine
      boundary layer revealed a slope of 13-16 ppt&lt;sub&gt;v&lt;/sub&gt; acetone/ppb&lt;sub&gt;v&lt;/sub&gt; CO. The different
      slopes observed in the marine boundary layer and the free troposphere indicate that acetone is emitted by the ocean in relatively clean air masses
      and taken up by the ocean in polluted air masses. In the lowermost stratosphere, a good correlation between acetone and CO was observed as
      well, however, with a much smaller slope (~5 ppt&lt;sub&gt;v&lt;/sub&gt; acetone/ppb&lt;sub&gt;v&lt;/sub&gt; CO)
      compared to the troposphere. This is caused by the longer photochemical lifetime of CO compared to acetone in the lower stratosphere, due to the
      increasing photolytic loss of acetone and the decreasing OH concentration with altitude. No significant correlation between acetone and CO was
      observed over the tropical rain forest due to the large direct and indirect
      biogenic emissions of acetone.&lt;br&gt;
      &lt;br&gt;
      The common slopes of the linear acetone-CO relation in various layers of the
      atmosphere, during five field experiments, makes them useful for model calculations. Often a single observation of the acetone-CO correlation,
      determined from stratospheric measurements, has been used in box model applications. This study shows that different slopes have to be considered for
      marine boundary layer, free tropospheric and stratospheric air masses, and
      that the acetone-CO relation cannot be used for air masses which are strongly
      influenced by biogenic emissions.</abstract>
	<references>
	</references>
</article>

