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<article language="en">
	<journal>
		<journal_title>Atmospheric Measurement Techniques Discussions</journal_title>
		<journal_url>www.atmos-meas-tech-discuss.net</journal_url>
		<eissn>1867-8610</eissn>
		<volume_number>2</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/amtd-2-1419-2009</doi>
	<article_url>http://www.atmos-meas-tech-discuss.net/2/1419/2009/</article_url>
	<abstract_html>http://www.atmos-meas-tech-discuss.net/2/1419/2009/amtd-2-1419-2009.html</abstract_html>
	<fulltext_pdf>http://www.atmos-meas-tech-discuss.net/2/1419/2009/amtd-2-1419-2009.pdf</fulltext_pdf>
	<start_page>1419</start_page>
	<end_page>1452</end_page>
	<publication_date>2009-06-15</publication_date>
	<article_title content_type="html">Use of O&lt;sub&gt;2&lt;/sub&gt; airglow for calibrating direct atomic oxygen measurements from sounding rockets</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. Hedin</name>
			<email>jonash@misu.su.se</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>J. Gumbel</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>J. Stegman</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>G. Witt</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Department of Meteorology, Stockholm University, 10691 Stockholm, Sweden</affiliation>
	</affiliations>
	<abstract content_type="html">Accurate knowledge about the distribution of atomic oxygen is crucial
      for many studies of the mesosphere and lower thermosphere. Direct
      measurements of atomic oxygen by the resonance fluorescence technique
      at 130 nm have been made from many sounding rocket payloads in
      the past. This measurement technique yields atomic oxygen profiles
      with good sensitivity and altitude resolution. However, accuracy is
      a problem as calibration and aerodynamics make the quantitative
      analysis challenging. In general, accuracies better than a factor 2
      are not to be expected from direct atomic oxygen measurements. As an
      example, we present results from the NLTE (non local thermodynamic
      equilibrium) sounding rocket campaign at Esrange, Sweden, in 1998,
      with simultaneous O&lt;sub&gt;2&lt;/sub&gt; airglow and O resonance fluorescence
      measurements. O number densities are found to be consistent with the
      nightglow analysis, but only within the uncertainty limits of the
      resonance fluorescence technique. Based on these results, we here
      describe how better atomic oxygen number densities can be obtained by
      calibrating direct techniques with complementary airglow photometer
      measurements and detailed aerodynamic analysis. Night-time direct O
      measurements can be complemented by photometric detection of the
      O&lt;sub&gt;2&lt;/sub&gt; (&lt;I&gt;b&lt;/I&gt;&lt;sup&gt;1&lt;/sup&gt;&amp;Sigma;&lt;sub&gt;&lt;I&gt;g&lt;/I&gt;&lt;/sub&gt;&lt;sup&gt;+&lt;/sup&gt;&amp;minus;&lt;I&gt;X&lt;/I&gt;&lt;sup&gt;3&lt;/sup&gt;&amp;Sigma;&lt;sub&gt;&lt;I&gt;g&lt;/I&gt;&lt;/sub&gt;&lt;sup&gt;&amp;minus;&lt;/sup&gt;)
      atmospheric band at 762 nm, while during daytime the
      O&lt;sub&gt;2&lt;/sub&gt; (&lt;I&gt;a&lt;/I&gt;&lt;sup&gt;1&lt;/sup&gt;&amp;Delta;&lt;sub&gt;&lt;I&gt;g&lt;/I&gt;&lt;/sub&gt;&amp;minus;&lt;I&gt;X&lt;/I&gt;&lt;sup&gt;3&lt;/sup&gt;&amp;Sigma;&lt;sub&gt;&lt;I&gt;g&lt;/I&gt;&lt;/sub&gt;&lt;sup&gt;&amp;minus;&lt;/sup&gt;) infrared
      atmospheric band at 1.27 μm can be used. The combination of
      a photometer and a rather simple resonance fluorescence probe can
      provide atomic oxygen profiles with both good accuracy and good height
      resolution.</abstract>
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