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<front>
<journal-meta>
<journal-id journal-id-type="publisher">AMT</journal-id>
<journal-title-group>
<journal-title>Atmospheric Measurement Techniques</journal-title>
<abbrev-journal-title abbrev-type="publisher">AMT</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Meas. Tech.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1867-8548</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/amt-6-3325-2013</article-id>
<title-group>
<article-title>Comparison of SMILES ClO profiles with satellite, balloon-borne and ground-based measurements</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sagawa</surname>
<given-names>H.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sato</surname>
<given-names>T. O.</given-names>
<ext-link>https://orcid.org/0000-0002-0123-9393</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Baron</surname>
<given-names>P.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Dupuy</surname>
<given-names>E.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff8">
<sup>8</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Livesey</surname>
<given-names>N.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Urban</surname>
<given-names>J.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>von Clarmann</surname>
<given-names>T.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>de Lange</surname>
<given-names>A.</given-names>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Wetzel</surname>
<given-names>G.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Connor</surname>
<given-names>B. J.</given-names>
</name>
<xref ref-type="aff" rid="aff7">
<sup>7</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kagawa</surname>
<given-names>A.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Murtagh</surname>
<given-names>D.</given-names>
<ext-link>https://orcid.org/0000-0003-1539-3559</ext-link>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kasai</surname>
<given-names>Y.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Applied Electromagnetic Research Institute, National Institute of Information and Communications Technology, Nukui-kita, Koganei, Tokyo 184-8795, Japan</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Tokyo Institute of Technology, Nagatsuta, Midori-ku, Yokohama, Kanagawa 226-8503, Japan</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Groove Drive, Pasadena, California 91109, USA</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Department of Earth and Space Sciences, Chalmers University of Technology, 41296 Gothenburg, Sweden</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Karlsruhe Institute of Technology, Institute for Meteorology and Climate Research, P.O. Box 3640, 76021 Karlsruhe, Germany</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>SRON-Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, the Netherlands</addr-line>
</aff>
<aff id="aff7">
<label>7</label>
<addr-line>BC Consulting, 6 Fairway Dr., Alexandra 9320, New Zealand</addr-line>
</aff>
<aff id="aff8">
<label>8</label>
<addr-line>now at: National Institute for Environmental Studies, Onogawa, Tsukuba, Ibaraki 305-8506, Japan</addr-line>
</aff>
<pub-date pub-type="epub">
<day>06</day>
<month>12</month>
<year>2013</year>
</pub-date>
<volume>6</volume>
<issue>12</issue>
<fpage>3325</fpage>
<lpage>3347</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2013 H. Sagawa et al.</copyright-statement>
<copyright-year>2013</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://amt.copernicus.org/articles/6/3325/2013/amt-6-3325-2013.html">This article is available from https://amt.copernicus.org/articles/6/3325/2013/amt-6-3325-2013.html</self-uri>
<self-uri xlink:href="https://amt.copernicus.org/articles/6/3325/2013/amt-6-3325-2013.pdf">The full text article is available as a PDF file from https://amt.copernicus.org/articles/6/3325/2013/amt-6-3325-2013.pdf</self-uri>
<abstract>
<p>We evaluate the quality of ClO profiles derived from the
Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the
International Space Station (ISS). Version 2.1.5 of the level-2 product
generated by the National Institute of Information and Communications
Technology (NICT) is the subject of this study. Based on sensitivity studies,
the systematic error was estimated as 5–10 pptv at the pressure
range of 80–20 hPa, 35 pptv at the ClO peak altitude
(~ 4 hPa), and 5–10 pptv at
pressures &amp;leq; 0.5 hPa for daytime mid-latitude conditions. For
nighttime measurements, a systematic error of 8 pptv was estimated
for the ClO peak altitude (~ 2 hPa). The SMILES NICT
v2.1.5 ClO profiles agree with those derived from another level-2
processor developed by the Japan Aerospace Exploration Agency (JAXA) within
the bias uncertainties, except for the nighttime measurements in the low and
middle latitude regions where the SMILES NICT v2.1.5 profiles have a negative
bias of ~ 30 pptv in the lower stratosphere. This bias is
considered to be due to the use of a limited spectral bandwidth in the
retrieval process of SMILES NICT v2.1.5, which makes it difficult to
distinguish between the weak ClO signal and wing contributions of spectral
features outside the bandwidth. In the middle and upper stratosphere outside
the polar regions, no significant systematic bias was found for the SMILES
NICT ClO profile with respect to data sets from other instruments such
as the Aura Microwave Limb Sounder (MLS), the Odin Sub-Millimetre Radiometer
(SMR), the Envisat Michelson Interferometer for Passive Atmospheric Sounding
(MIPAS), and the ground-based radiometer at Mauna Kea, which demonstrates the
scientific usability of the SMILES ClO data including the diurnal
variations. Inside the chlorine-activated polar vortex, the SMILES NICT v2.1.5
ClO profiles show larger volume mixing ratios by 0.4 ppbv
(30%) at 50 hPa compared to those of the JAXA processed
profiles. This discrepancy is also considered to be an effect of the limited
spectral bandwidth in the retrieval processing. We also compared the SMILES
NICT ClO profiles of chlorine-activated polar vortex conditions with
those measured by the balloon-borne instruments: Terahertz and submillimeter
Limb Sounder (TELIS) and the MIPAS-balloon instrument (MIPAS-B). In
conclusion, the SMILES NICT v2.1.5 ClO data can be used at
pressures &amp;leq; ~30 hPa for scientific analysis.</p>
</abstract>
<counts><page-count count="23"/></counts>
</article-meta>
</front>
<body/>
<back>
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