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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>9</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/acpd-9-13943-2009</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/9/13943/2009/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/9/13943/2009/acpd-9-13943-2009.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/9/13943/2009/acpd-9-13943-2009.pdf</fulltext_pdf>
	<start_page>13943</start_page>
	<end_page>13997</end_page>
	<publication_date>2009-06-26</publication_date>
	<article_title content_type="html">Daytime SABER/TIMED observations of water vapor in the mesosphere: retrieval  approach and first results</article_title>
	<authors>
		<author numeration="1" affiliations="1,2">
			<name>A. G. Feofilov</name>
			<email>artem-feofilov@cua-nasa-gsfc.info</email>
		</author>
		<author numeration="2" affiliations="1,2">
			<name>A. A. Kutepov</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>W. D. Pesnell</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>R. A. Goldberg</name>
		</author>
		<author numeration="5" affiliations="3">
			<name>B. T. Marshall</name>
		</author>
		<author numeration="6" affiliations="3">
			<name>L. L. Gordley</name>
		</author>
		<author numeration="7" affiliations="4">
			<name>M. García-Comas</name>
		</author>
		<author numeration="8" affiliations="4">
			<name>M. López-Puertas</name>
		</author>
		<author numeration="9" affiliations="5">
			<name>R. O. Manuilova</name>
		</author>
		<author numeration="10" affiliations="5">
			<name>V. A. Yankovsky</name>
		</author>
		<author numeration="11" affiliations="6">
			<name>S. V. Petelina</name>
		</author>
		<author numeration="12" affiliations="7">
			<name>J. M. Russell III</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">The Catholic University of America, 620 Michigan Ave., Washington D.C. 20064, USA</affiliation>
		<affiliation numeration="2" content_type="html">NASA Goddard Space Flight Center, Mailcode 674, Greenbelt Rd.,  Greenbelt,  MD 20771, USA</affiliation>
		<affiliation numeration="3" content_type="html">GATS Inc., 1164 Canon Blvd., Suite 101, Newport News, VA 23606, USA</affiliation>
		<affiliation numeration="4" content_type="html">Instituto de Astrofísica de Andalucía (CSIC), C/Camino Bajo de Huetor, 50, Granada 18008, Spain</affiliation>
		<affiliation numeration="5" content_type="html">Institute for Physics, St. Petersburg State University, Ulianovskaja,  1,  St. Petersburg, 198904, Russia</affiliation>
		<affiliation numeration="6" content_type="html">La Trobe University, Victoria, 3086, Australia</affiliation>
		<affiliation numeration="7" content_type="html">Hampton University, Hampton, VA 23668, USA</affiliation>
	</affiliations>
	<abstract content_type="html">This paper describes a methodology for water vapor retrieval using
      6.6 &amp;mu;m daytime broadband emissions measured by SABER, the
      limb scanning infrared radiometer on board the TIMED
      satellite. Particular attention is given to accounting for the
      non-local thermodynamic equilibrium (non-LTE) nature of the
      H&lt;sub&gt;2&lt;/sub&gt;O 6.6 &amp;mu;m emission in the mesosphere and lower
      thermosphere (MLT). The non-LTE H&lt;sub&gt;2&lt;/sub&gt;O (&amp;nu;&lt;sub&gt;2&lt;/sub&gt;) vibrational
      level populations responsible for this emission depend on energy
      exchange processes within the H&lt;sub&gt;2&lt;/sub&gt;O vibrational system as well
      as on interactions with vibrationally excited states of the
      O&lt;sub&gt;2&lt;/sub&gt;, N&lt;sub&gt;2&lt;/sub&gt;, and CO&lt;sub&gt;2&lt;/sub&gt; molecules. The paper
      analyzes current H&lt;sub&gt;2&lt;/sub&gt;O non-LTE models and, based on
      comparisons with the ACE-FTS satellite solar occultation measurements,
      suggests an update to the rate coefficients of the three most
      important processes that affect the H&lt;sub&gt;2&lt;/sub&gt;O(&amp;nu;&lt;sub&gt;2&lt;/sub&gt;)
      populations in the MLT: a) the vibrational-vibrational (V–V) exchange
      between the H&lt;sub&gt;2&lt;/sub&gt;O and O&lt;sub&gt;2&lt;/sub&gt; molecules; b) the
      vibrational-translational (V–T) process of the O&lt;sub&gt;2&lt;/sub&gt;(1) level
      quenching by collisions with atomic oxygen, and c) the V–T process of
      the H&lt;sub&gt;2&lt;/sub&gt;O(010) level quenching by collisions with
      N&lt;sub&gt;2&lt;/sub&gt;, O&lt;sub&gt;2&lt;/sub&gt;, and O. We demonstrate that applying the
      updated H&lt;sub&gt;2&lt;/sub&gt;O non-LTE model to the SABER radiances makes the
      retrieved H&lt;sub&gt;2&lt;/sub&gt;O vertical profiles in 50–85 km region
      consistent with climatological data and model predictions.</abstract>
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