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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>8</volume_number>
		<issue_number>2</issue_number>
		<publication_year>2008</publication_year>
	</journal>
	<doi>10.5194/acpd-8-5901-2008</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/8/5901/2008/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/8/5901/2008/acpd-8-5901-2008.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/8/5901/2008/acpd-8-5901-2008.pdf</fulltext_pdf>
	<start_page>5901</start_page>
	<end_page>5917</end_page>
	<publication_date>2008-03-20</publication_date>
	<article_title content_type="html">Odin/OSIRIS observations of stratospheric NO&lt;sub&gt;3&lt;/sub&gt; through sunrise and sunset</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>C. A. McLinden</name>
			<email>Chris.McLinden@ec.gc.ca</email>
		</author>
		<author numeration="2" affiliations="2">
			<name>C. S. Haley</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Environment Canada, Toronto, ON, M3H 5T4, Canada</affiliation>
		<affiliation numeration="2" content_type="html">Centre for Research in Earth and Space Science, York Univ., Toronto, ON, M3J 1P3, Canada</affiliation>
	</affiliations>
	<abstract content_type="html">The nitrate radical (NO&lt;sub&gt;3&lt;/sub&gt;) has been detected in visible limb-scattered spectra measured by the Optical Spectrograph
and InfraRed Imager System (OSIRIS) on-board the Odin satellite when observing at large solar zenith angles
(91&amp;ndash;97&amp;deg;).  Apparent slant column densities of NO&lt;sub&gt;3&lt;/sub&gt; at tangent heights between 10 and 45 km are derived via
spectral fitting in the 590&amp;ndash;680 nm window.  Using observations from multiple scans spanning solar zenith angles of
91&amp;ndash;97&amp;deg;, the rapid evolution of NO&lt;sub&gt;3&lt;/sub&gt; through sunrise and sunset can be traced.  Slant column densities
are found to be consistent with those simulated using a radiative transfer model with coupled photochemistry.
In addition, a strong dependence of NO&lt;sub&gt;3&lt;/sub&gt; with temperature is observed.
These results indicate that OSIRIS possesses signal-to-noise sufficient to make useful measurements of scattered sunlight
out to solar zenith angles
of 96&amp;ndash;97&amp;deg; and suggests the possibility of retrieving profile information for NO&lt;sub&gt;3&lt;/sub&gt; and other species at large
solar zenith angles.</abstract>
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</article>

