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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>3</issue_number>
		<publication_year>2003</publication_year>
	</journal>
	<doi>10.5194/acpd-3-2331-2003</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/3/2331/2003/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/3/2331/2003/acpd-3-2331-2003.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/3/2331/2003/acpd-3-2331-2003.pdf</fulltext_pdf>
	<start_page>2331</start_page>
	<end_page>2352</end_page>
	<publication_date>2003-05-12</publication_date>
	<article_title content_type="html">Sensitivity studies of the recent new data on O(&lt;sup&gt;1&lt;/sup&gt;&lt;i&gt;D&lt;/i&gt;) quantum yields in O&lt;sub&gt;3&lt;/sub&gt; Hartley band photolysis in the stratosphere</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>N. Taniguchi</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>S. Hayashida</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>K. Takahashi</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>Y. Matsumi</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Faculty of Science, Nara Women’s University, Kitauoya-Nishimachi, Nara, 630-8506, Japan</affiliation>
		<affiliation numeration="2" content_type="html">Solar-Terrestrial Environment Laboratory, Nagoya University, Honohara 3–13, Toyokawa, 442-8507, Japan</affiliation>
	</affiliations>
	<abstract content_type="html">The production yields of excited oxygen O(&lt;sup&gt;1&lt;/sup&gt;&lt;i&gt;D&lt;/i&gt;) atoms from the near ultraviolet
      O&lt;sub&gt;3&lt;/sub&gt; photolysis are essential quantities for atmospheric chemistry calculations because of its importance as
      major sources of hydroxyl (OH) radicals and nitric oxide (NO).  Recently, new
      O(&lt;sup&gt;1&lt;/sup&gt;&lt;i&gt;D&lt;/i&gt;)
      quantum yields from O&lt;sub&gt;3&lt;/sub&gt; photolysis between 230 and 305 nm in the Hartley band region were
      reported, which are almost independent of the photolysis wavelength
      (0.88-0.93) and smaller than NASA/JPL-2000 recommendation (0.95 between 240 and 300 nm).  In order to assess
      consequences of the new data of O(&lt;sup&gt;1&lt;/sup&gt;&lt;i&gt;D&lt;/i&gt;) quantum yields on the stratospheric chemistry, the
      changes in stratospheric chemical partitioning and O&lt;sub&gt;3&lt;/sub&gt; concentration are examined using a
      one-dimensional atmospheric model.  Our steady state model simulations for mid-latitude in
      March indicate that the smaller O(&lt;sup&gt;1&lt;/sup&gt;&lt;i&gt;D&lt;/i&gt;) quantum yields result in increases of stratospheric
      O&lt;sub&gt;3&lt;/sub&gt; (up to ~2% in the upper stratosphere), which are attributed to the changes in
      HO&lt;sub&gt;x&lt;/sub&gt;, NO&lt;sub&gt;x&lt;/sub&gt;, and ClO&lt;sub&gt;x&lt;/sub&gt; abundance and their catalyzed
      O&lt;sub&gt;3&lt;/sub&gt; loss rates.</abstract>
	<references>
	</references>
</article>

