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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>5</volume_number>
		<issue_number>5</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-10369-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/10369/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/10369/2005/acpd-5-10369-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/10369/2005/acpd-5-10369-2005.pdf</fulltext_pdf>
	<start_page>10369</start_page>
	<end_page>10408</end_page>
	<publication_date>2005-10-24</publication_date>
	<article_title content_type="html">The heterogeneous chemical kinetics of N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; on CaCO&lt;sub&gt;3&lt;/sub&gt; and other atmospheric mineral dust surrogates</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>F. Karagulian</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>C. Santschi</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>M. J. Rossi</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Ecole Polytechnique Fédérale de Lausanne, Laboratoire de Pollution Atmosphérique et Sol (EPFL, LPAS), Bâtiment CH H5, Station 6, CH-1015 Lausanne, Switzerland</affiliation>
	</affiliations>
	<abstract content_type="html">Uptake experiments of N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; on several mineral dust powder samples
were carried out under continuous molecular flow conditions at 298&amp;plusmn;2 K.
At [N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt;]&lt;sub&gt;0&lt;/sub&gt;=(4.0&amp;plusmn;1.0)&amp;times;10&lt;sup&gt;11&lt;/sup&gt; cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt; we
have found &amp;gamma;&lt;sub&gt;&lt;i&gt;ss&lt;/i&gt;&lt;/sub&gt; values ranging from (3.5&amp;plusmn;1.1)&amp;times;10&lt;sup&gt;&amp;minus;2&lt;/sup&gt;
for CaCO&lt;sub&gt;3&lt;/sub&gt; to (0.20&amp;plusmn;0.05) for Saharan Dust with &amp;gamma;&lt;sub&gt;&lt;i&gt;ss&lt;/i&gt;&lt;/sub&gt;
decreasing as [N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt;]&lt;sub&gt;0&lt;/sub&gt; increased. We have observed delayed
production of HNO&lt;sub&gt;3&lt;/sub&gt; upon uptake of N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; for every investigated
sample owing to hydrolysis of N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; with surface-adsorbed H&lt;sub&gt;2&lt;/sub&gt;O.
At high and low [N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt;] Arizona Test Dust and Kaolinite turned out
to be the samples to produce the largest amount of gas phase HNO&lt;sub&gt;3&lt;/sub&gt; with
respect to N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; taken up. In contrast, the yield of HNO&lt;sub&gt;3&lt;/sub&gt; for
Saharan Dust and CaCO&lt;sub&gt;3&lt;/sub&gt; are lower. On CaCO&lt;sub&gt;3&lt;/sub&gt; the disappearance of
N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; was also accompanied by the formation of CO&lt;sub&gt;2&lt;/sub&gt;. For
CaCO&lt;sub&gt;3&lt;/sub&gt; sample masses ranging from 0.33 to 2.0 g, the yield of CO&lt;sub&gt;2&lt;/sub&gt;
was approximately 42&amp;ndash;50% with respect to the total number of
N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; molecules taken up. The reaction of N&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;5&lt;/sub&gt; with
mineral dust and the subsequent production of gas phase HNO&lt;sub&gt;3&lt;/sub&gt; leads to a
decrease in [NO&lt;sub&gt;x&lt;/sub&gt;] which may have a significant effect on global ozone.</abstract>
	<references>
	</references>
</article>

