<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "journalpub-oasis3.dtd">
<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0"><?xmltex \makeatother\@nolinetrue\makeatletter?>
  <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-11-4583-2018</article-id><title-group><article-title><inline-formula><mml:math id="M1" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and HCHO measurements in Korea from 2012 to 2016 from Pandora
spectrometer instruments compared with OMI retrievals and with aircraft
measurements during the KORUS-AQ campaign</article-title><alt-title><inline-formula><mml:math id="M2" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and HCHO measurements in Korea from 2012 to 2016</alt-title>
      </title-group><?xmltex \runningtitle{{$\chem{NO_{{2}}}$} and HCHO measurements in Korea from 2012 to 2016}?><?xmltex \runningauthor{J. Herman et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Herman</surname><given-names>Jay</given-names></name>
          <email>jay.r.herman@nasa.gov</email>
        <ext-link>https://orcid.org/0000-0002-9146-1632</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Spinei</surname><given-names>Elena</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Fried</surname><given-names>Alan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Kim</surname><given-names>Jhoon</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1508-9218</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Kim</surname><given-names>Jae</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Kim</surname><given-names>Woogyung</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0445-4806</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Cede</surname><given-names>Alexander</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Abuhassan</surname><given-names>Nader</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7 aff8">
          <name><surname>Segal-Rozenhaimer</surname><given-names>Michal</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>JCET, University of Maryland Baltimore County, Baltimore, MD, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Virginia Polytechnic Institute and State University, Blacksburg, Virginia, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Institute of Arctic &amp; Alpine Research, University of Colorado, Boulder, Colorado, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Dept. of Atmospheric Sciences, Yonsei University, Seoul, Korea</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Atmospheric Science, Pusan University, Busan, Korea</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Goddard Earth Sciences Technology &amp; Research (GESTAR) Columbia, Columbia, Maryland, USA</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Earth Science Division, NASA Ames, Mountain View, California, USA</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>Bay Area Environmental Research Institute, Petaluma, California, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Jay Herman (jay.r.herman@nasa.gov)</corresp></author-notes><pub-date><day>8</day><month>August</month><year>2018</year></pub-date>
      
      <volume>11</volume>
      <issue>8</issue>
      <fpage>4583</fpage><lpage>4603</lpage>
      <history>
        <date date-type="received"><day>21</day><month>February</month><year>2018</year></date>
           <date date-type="rev-request"><day>3</day><month>April</month><year>2018</year></date>
           <date date-type="rev-recd"><day>12</day><month>June</month><year>2018</year></date>
           <date date-type="accepted"><day>10</day><month>July</month><year>2018</year></date>
      </history>
      <permissions>
        
        
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018.html">This article is available from https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018.html</self-uri><self-uri xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018.pdf">The full text article is available as a PDF file from https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018.pdf</self-uri>
      <abstract>
    <p id="d1e222">Nine Pandora
spectrometer instruments (PSI) were installed at eight sites in
South Korea as part of the KORUS-AQ (Korea U.S.-Air Quality) field study
integrating information from ground, aircraft, and satellite measurements
for validation of remote sensing air-quality studies. The PSI made
direct-sun measurements of total vertical column <inline-formula><mml:math id="M3" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M4" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, with
high precision (0.05 DU, where 1 DU <inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.69</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molecules cm<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>)
and accuracy (0.1 DU) that were retrieved using spectral fitting techniques.
Retrieval of formaldehyde C(HCHO) total column amounts were also obtained at
five sites using the recently improved PSI optics. The C(HCHO) retrievals have
high precision, but possibly lower accuracy than for <inline-formula><mml:math id="M7" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> because of
uncertainty about the optimum spectral window for all ground-based and
satellite instruments. PSI direct-sun retrieved values for <inline-formula><mml:math id="M8" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and
C(HCHO) are always significantly larger than OMI (AURA satellite Ozone
Monitoring Instrument) retrieved <inline-formula><mml:math id="M9" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and C(HCHO) for the OMI
overpass local times (<inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mi mathvariant="normal">KST</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">13.5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> h). In urban areas, PSI
<inline-formula><mml:math id="M11" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> 30-day running averages are at least a factor of two larger than
OMI averages. Similar differences are seen for C(HCHO) in Seoul and nearby
surrounding areas. Late afternoon values of C(HCHO) measured by PSI are even
larger, implying that OMI early afternoon measurements underestimate the
effect of poor air quality on human health. The primary cause of OMI
underestimates is the large OMI field of view (FOV) that includes regions
containing low values of pollutants. In relatively clean areas, PSI and OMI
are more closely in agreement. C(HCHO) amounts were obtained for five sites,
Yonsei University in Seoul, Olympic Park, Taehwa Mountain, Amnyeondo, and Yeoju.
Of these, the largest amounts of C(HCHO) were observed at Olympic Park and
Taehwa Mountain, surrounded by significant amounts of vegetation.
Comparisons of PSI C(HCHO) results were made with the Compact Atmospheric
Multispecies Spectrometer CAMS during overflights on the DC-8 aircraft for
Taehwa Mountain and Olympic Park. In all cases, PSI measured substantially more
C(HCHO) than obtained from integrating the CAMS altitude profiles. PSI
C(HCHO) at Yonsei University in Seoul frequently reached 0.6 DU and
occasionally exceeded 1.5 DU. The semi-rural site, Taehwa Mountain, frequently
reached 0.9 DU and occasionally exceeded 1.5 DU. Even at the cleanest site,
Amnyeondo, C(HCHO) occasionally exceeded 1 DU.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<?pagebreak page4584?><sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e368">The purpose of this paper is to present the retrieved total column amounts
of nitrogen dioxide and formaldehyde, <inline-formula><mml:math id="M12" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and C(HCHO), obtained from
Pandora spectrometer instruments (PSI) direct-sun observations during the
KORUS-AQ campaign (Korea US Air Quality: May–June 2016). Quoting from a
NASA website:<disp-quote>
  <p id="d1e389">Korea U.S.-Air Quality (KORUS-AQ) is a joint field study
between NASA and the Republic of Korea to advance the ability to monitor air
pollution from space. The campaign will assess air quality across urban,
rural, and coastal South Korea using observations from aircraft, ground
sites, ships, and satellites to test air quality models and remote sensing
methods. Findings will help develop observing systems using models and data
to improve air quality assessments for decision makers.</p>
</disp-quote>A thorough
description of the KORUS-AQ campaign and its motivations is given in a
pre-campaign white paper, <uri>https://espo.nasa.gov/korus-aq/content/KORUS-AQ_White_Paper</uri> (last access: 31 July 2018).</p>
      <p id="d1e397">Assessing air quality in South Korea is of interest because of the levels of
pollution arising from high densities of population and intense industrial
activity associated with the production of <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. Recent measurements
of surface concentrations of <inline-formula><mml:math id="M14" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and comparisons with satellite
data demonstrate the need for high quality ground-based measurements to
augment satellite observations (Kim et al., 2017; Jung et al., 2017). The
driving reason behind the interest is the effect of elevated levels of
<inline-formula><mml:math id="M15" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in Korea on human health (Kim and Song, 2017 and references
therein). Measurements of <inline-formula><mml:math id="M16" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from aircraft have been used to
obtain altitude profiles to compare with data obtained from fixed site
measurements and to obtain a national scale estimate of pollutant exposure
(Lee et al., 2016; Kim and Song, 2017).</p>
      <p id="d1e444">In addition to <inline-formula><mml:math id="M17" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, PSI measurements were used to assess the amount
of formaldehyde (HCHO) present in the air. This is important because of
HCHO's potential impact on health (Zhang et al., 2013; Zhu et al., 2017) and
because it plays a strong role in tropospheric reactions leading to the
formation of boundary layer ozone. Sources of HCHO are from atmospheric
reactions with volatile organic compounds (VOC) emitted from ground sources
and industrial activities (Lei at al., 2009). A previous paper describes HCHO
retrievals from a PSI located at Yonsei University in Seoul using a similar
spectral fitting retrieval algorithm used in the current study (Park et al.,
2018), but using a different wavelength fitting range, 335–358 nm instead
of 332–359 nm used in this study. The choice of spectral fitting window is
discussed in Spinei et al. (2018).</p>
      <p id="d1e458">As part of the KORUS-AQ campaign, a network of nine PSI was installed in
Korea at eight locations (Fig. 1 and Table 1). Five of the sites were
selected to be “down-wind” from Seoul, an area of very high <inline-formula><mml:math id="M18" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
pollution. The intent of the network was to integrate direct-sun column
density observations of <inline-formula><mml:math id="M19" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and HCHO into a multi-perspective
framework of observations including ground-based, satellite, and airborne
measurements of air quality. Viewing air quality through these multiple
perspectives is important for connecting observations from future
geostationary satellites to air quality networks such that
conditions, both at the surface and
aloft, can be better understood and
represented across unmonitored areas. The data are especially important for
computer models used for forecasts and decision making. Five of the KORUS-AQ
PSI had recently improved optics that permitted retrieval of total vertical
column formaldehyde (C(HCHO)). Part of the network was installed in April
2015, a year before the start of the campaign. Three PSI continue to operate
in Korea, one each, in Busan and Seoul since 2012, and one in Gwangju
operating since April 2015.</p>
      <p id="d1e484">Measurements of daytime total columns in Dobson Units, where 1 DU <inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.69</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molecules cm<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, <inline-formula><mml:math id="M22" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M23" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, and C(HCHO) are
obtained every 80 s, which enables the PSI to show rapid short term
(minutes to hours) variations in most locations with significant pollution
(e.g., <inline-formula><mml:math id="M24" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M25" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.2 DU). PSI measurements of the visible and
UV wavelengths are obtained separately (40 s each). A visible
wavelength blocking filter, U340, reduces stray light for UV measurements
originating from the much brighter visible wavelength range.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p id="d1e577">KORUS-AQ sites for nine Pandora instruments at eight sites.</p></caption>
        <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f01.png"/>

      </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><caption><p id="d1e589">KORUS-AQ locations (south to north).</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Locations</oasis:entry>
         <oasis:entry colname="col2">Alt(m)</oasis:entry>
         <oasis:entry colname="col3">Latitude</oasis:entry>
         <oasis:entry colname="col4">Longitude</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Gwangju</oasis:entry>
         <oasis:entry colname="col2">33</oasis:entry>
         <oasis:entry colname="col3">35.2260<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N</oasis:entry>
         <oasis:entry colname="col4">126.8430<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Busan</oasis:entry>
         <oasis:entry colname="col2">228</oasis:entry>
         <oasis:entry colname="col3">35.2353<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N</oasis:entry>
         <oasis:entry colname="col4">129.0825<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Anmyeondo</oasis:entry>
         <oasis:entry colname="col2">41</oasis:entry>
         <oasis:entry colname="col3">36.5380<inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N</oasis:entry>
         <oasis:entry colname="col4">126.3300<inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Taehwa Mountain</oasis:entry>
         <oasis:entry colname="col2">160</oasis:entry>
         <oasis:entry colname="col3">37.3123<inline-formula><mml:math id="M32" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N</oasis:entry>
         <oasis:entry colname="col4">127.3106<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Yeoju-1 &amp; 2</oasis:entry>
         <oasis:entry colname="col2">90</oasis:entry>
         <oasis:entry colname="col3">37.3385<inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N</oasis:entry>
         <oasis:entry colname="col4">127.4895<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Songchon</oasis:entry>
         <oasis:entry colname="col2">49</oasis:entry>
         <oasis:entry colname="col3">37.4100<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N</oasis:entry>
         <oasis:entry colname="col4">127.5600<inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Olympic Park</oasis:entry>
         <oasis:entry colname="col2">26</oasis:entry>
         <oasis:entry colname="col3">37.5232<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N</oasis:entry>
         <oasis:entry colname="col4">127.1260<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Seoul</oasis:entry>
         <oasis:entry colname="col2">181</oasis:entry>
         <oasis:entry colname="col3">37.5644<inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N</oasis:entry>
         <oasis:entry colname="col4">126.9340<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e892">Details on the Pandora spectrometer instrument can be found in Herman et
al. (2009, 2015) as well as a NASA Pandora website
<uri>https://avdc.gsfc.nasa.gov/pub/DSCOVR/Pandora/Web_Pandora/index.html</uri>
(last access: 31 July 2018) and the data used are available from
<uri>https://avdc.gsfc.nasa.gov/pub/DSCOVR/Pandora/DATA/KORUS-AQ/</uri> (last
access: 31 July 2018).</p>
      <p id="d1e901">The PSI consists of a small Avantes low stray light spectrometer
(280–525 nm with 0.6 nm spectral resolution with 4 times oversampling)
connected to an optical head by a 400 <inline-formula><mml:math id="M42" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m single strand fiber optic
cable. The spectrometer is temperature stabilized at 20 <inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
(68 <inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>F) inside of two weather resistant containers. The optical head
consists of a collimator and lens giving rise to a 1.6<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> FOV (field of
view) FWHM (Full Width Half Maximum) with light passing through two<?pagebreak page4585?> filter
wheels containing diffusers, a UV340 filter (blocks visible light), neutral
density filters, and an opaque position (dark current measurement). When the
diffuser is used, the FOV is increased to over 2<inline-formula><mml:math id="M46" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and becomes less
sensitive to the sun's exact position in the FOV. The optical head is
connected to a small suntracker capable of accurately following the sun's
center using software running on a small computer-data logger contained in a
weatherproof outer box along with the spectrometer in a second inner
temperature controlled box. The PSI is capable of obtaining <inline-formula><mml:math id="M47" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>,
C(HCHO), and <inline-formula><mml:math id="M48" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts sequentially over a period of 80 s
including two dark current determinations. The integration time for
<inline-formula><mml:math id="M49" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in bright sun is about 4 ms that is repeated and averaged for
20 s (up to 4000 measurements) to obtain very high signal to noise ratios
and very high precision (precision <inline-formula><mml:math id="M50" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.01 DU). Similar comments apply to
<inline-formula><mml:math id="M51" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, but not to C(HCHO), as formaldehyde absorption spectrum is
mixed in with absorption from <inline-formula><mml:math id="M52" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M53" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and BrO (when
present). This causes cross-correlation effects in the retrieval algorithm
that make C(HCHO) retrievals sensitive to the selection of the wavelength
range. The main source of noise in the measurement comes from the presence of
clouds or haze in the FOV, which increases the exposure time and reduces the
number of measurements in 20 s.</p>
      <p id="d1e1041"><?xmltex \hack{\newpage}?>The retrieval algorithm is based a direct-sun spectral fitting method similar
to the well-accepted DOAS (Differential Optical Absorption Spectroscopy,
Platt et al., 1979 and Platt, 1994). <inline-formula><mml:math id="M54" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> absorption cross sections
were obtained from the laboratory measurements of Vandaele et al. (1998), and
HCHO cross sections from Meller and Moortgat (2000). For ozone, the PSI
reference solar spectrum is constructed from a high resolution
extraterrestrial spectrum (270 to 1000 nm) merged from different sources
(Bernhard et al., 2004; Herman et al., 2015). For <inline-formula><mml:math id="M55" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and HCHO, the
reference spectrum is obtained from a Modified Langley Extrapolation method
(Herman et al., 2009; Spinei et al., 2018). One of the advantages of using
direct-sun observations is the accurate conversion to vertical column based
on a geometric calculation of the slant path air mass factor AMF for a known
solar zenith angle SZA with a slight correction to the function secant (SZA)
(Herman et al., 2009, Eq. 3). A complete description of the retrieval
algorithms and PSI operations are given in the PSI software manual (Cede,
2017). Accuracy in the DOAS-type retrieval is obtained using careful
measurements of the spectrometer's slit function, wavelength calibration,
knowledge of atmospheric absorption cross sections, and the solar spectrum at
the top of the atmosphere. Accuracy for <inline-formula><mml:math id="M56" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> has been estimated
to be <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula> DU. A recent addition of anti-reflection coatings to the
PSI optics has improved accuracy and precision by reducing the residuals
associated with spectral fitting using trace gas absorption cross sections.
The reduced residuals are necessary for the retrieval of formaldehyde and
bromine oxide that absorb in spectral regions dominated by ozone and
<inline-formula><mml:math id="M58" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. Other DOAS-type measurements have been made in Korea based on
observations of sky radiance ratios (e.g., multi axis MAX-DOAS: Kanaya, et
al., 2014) and direct-sun DOAS using a PSI in Seoul, Korea (Park et al.,
2018).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p id="d1e1107"><bold>(a)</bold> <inline-formula><mml:math id="M59" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts from Pandora 27 and 35 in
Yeoju, Korea during 3 June 2016 and their difference
<inline-formula><mml:math id="M60" display="inline"><mml:mo>|</mml:mo></mml:math></inline-formula>Pan35–Pan27<inline-formula><mml:math id="M61" display="inline"><mml:mo>|</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M62" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.05 DU. <bold>(b)</bold> Pandora 35 estimate of cloud
or aerosol reduced measured counts s<inline-formula><mml:math id="M63" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> at approximately 500 nm.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f02.png"/>

      </fig>

      <p id="d1e1172">This paper discusses the distribution of <inline-formula><mml:math id="M64" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and C(HCHO) over
Korea at the sites where the PSI were located (Fig. 1). Section 2 shows the
amounts of <inline-formula><mml:math id="M65" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> observed by PSIs at the eight KORUS-AQ sites.
Section 3 discusses the diurnal variation of <inline-formula><mml:math id="M66" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. Section 4 looks
at longer term changes in <inline-formula><mml:math id="M67" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> obtained from PSIs that were deployed
before the beginning of the KORUS-AQ campaign. Section 5 evaluates the
disagreement with Ozone Monitoring Instrument (OMI) satellite
<inline-formula><mml:math id="M68" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> retrievals (Kramer et al., 2008). Section 6 compared PSI
<inline-formula><mml:math id="M69" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> retrievals with the aircraft overpass retrievals from the
4STAR instrument (Segal-Rozenhaimer et al., 2014). Section 6 discusses
retrievals of C(HCHO) amounts for five PSI sites, the diurnal variation of
C(HCHO), and comparisons with the Compact Atmospheric Multispecies
Spectrometer CAMS (Richter et al., 2015) from DC-8 aircraft overflights of
five PSI sites.</p>
</sec>
<?pagebreak page4586?><sec id="Ch1.S2">
  <?xmltex \opttitle{{$\protect\chem{NO_{{2}}}$} during the KORUS-AQ campaign (May--June 2016)}?><title><inline-formula><mml:math id="M70" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> during the KORUS-AQ campaign (May–June 2016)</title>
      <p id="d1e1277">An example of <inline-formula><mml:math id="M71" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> retrieval from two independently calibrated Pandoras,
which were initially located at the same site (Yeoju, Korea, 37.3385<inline-formula><mml:math id="M72" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
127.4895<inline-formula><mml:math id="M73" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W), are compared in Fig. 2a showing that the differences in
<inline-formula><mml:math id="M74" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts are less than 0.05 DU, even in the presence of thin
afternoon clouds (Fig. 2b) that decrease the measured solar irradiance by
more than a factor of 2. Though Yeoju is a relatively clean site in Korea
(located to the southeast of Seoul, 37.5644<inline-formula><mml:math id="M75" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 126.934<inline-formula><mml:math id="M76" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W), <inline-formula><mml:math id="M77" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts frequently reach
moderately high values (e.g., 1 DU on 3 June 2016), and occasionally even
higher (2–3 DU). However, Yeoju has much less <inline-formula><mml:math id="M78" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> compared to Seoul,
less than 30 km distant, where PSI measurements were found to reach over 3 DU (Fig. 3) during the campaign period from mid-April to early June, 2016.
Typical <inline-formula><mml:math id="M79" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts are 0.3 to 0.5 DU in polluted regions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p id="d1e1398">Frequency distributions of <inline-formula><mml:math id="M80" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> across the KORUS-AQ PSI
network: 20 April to 6 June 2016, except as labeled. The axes vary for
different sites.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f03.png"/>

      </fig>

      <p id="d1e1424">In a manner similar to Fig. 2a, <inline-formula><mml:math id="M81" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts can show large
variability from day-to-day and intra-day, as well as between different
sites. The largest amounts of <inline-formula><mml:math id="M82" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> are in the north (Seoul and
Olympic Park) associated with the largest population and industry
concentrations, while the southern cities of Busan and Gwangju have smaller
amounts of <inline-formula><mml:math id="M83" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. The smallest <inline-formula><mml:math id="M84" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts are at Anmyeondo
(an island on west coast of Korea 42 km south of Seoul, usually not downwind
of Seoul), and Songchon to the east of Seoul.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p id="d1e1498"><inline-formula><mml:math id="M85" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> time series vs. day of the year (DOY) and diurnal
variability (daily vertical extent) at nine Pandora sites. Notice the very
high <inline-formula><mml:math id="M86" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> amounts in Seoul and nearby Olympic Park. The black curves
are approximate weekly least squares running averages. Note that the vertical
scales are different for each site to show the daily variability relative to
the running average.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f04.png"/>

      </fig>

      <p id="d1e1528">Figure 2b shows the effect of thin clouds in terms of reduced measured count
rates for a single spectrometer pixel near 500 nm showing a near noon count
rate of <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.26</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> counts s<inline-formula><mml:math id="M88" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> followed by a reduced count rate as
clouds move in front of the sun. The cloud plus aerosol cover estimate is
from the same date 3 June 2016 as the <inline-formula><mml:math id="M89" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts shown in Fig. 2a.
The effect of thin clouds for <inline-formula><mml:math id="M90" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> retrieval (Fig. 2a) is increased
noise (reduced precision) with a very small impact on accuracy. There are
two effects on PSI observations to consider in association with thin clouds.
First, is multiple scattering within the cloud affecting the optical path
and effective air mass factor AMF. This has a very small effect on AMF,
as most of the <inline-formula><mml:math id="M91" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is near the surface well below the clouds.
Second, is the reduction in the number of measurements during a fixed 20 s measuring period causing a decrease in the signal to noise ratio. The
weather during the campaign was occasionally very cloudy, which caused some
missing <inline-formula><mml:math id="M92" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M93" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> data. However, most of the cloudy days were
light to moderate cloud cover, which permitted <inline-formula><mml:math id="M94" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts to be
determined, but with lower precision compared to clear-sky direct sun
measurements (e.g., Fig. 2a and b). When the cloud cover becomes
sufficiently thick, precision is reduced (increased point-to-point scatter)
and the spectral fitting error increases. A small percentage of data points
with high retrieval error, <inline-formula><mml:math id="M95" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">Error</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M96" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.1 DU, have been
removed from the data set.</p>
      <p id="d1e1669">Figures 3 and 4 summarize all of the Pandora <inline-formula><mml:math id="M97" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> data obtained
during the KORUS-AQ campaign. Figure 3 presents histograms in percent
frequency of occurrence for all nine sites. All of the sites located within
or downwind of major cities have production of <inline-formula><mml:math id="M98" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> mainly
from transportation and power generation as its major sources. The ratio of
transportation <inline-formula><mml:math id="M99" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> production is a factor of 3 larger
compared to all other sources (Kim et al., 2013). Of these sites, the
Anmyeondo PSI frequently (40 %) retrieves values of <inline-formula><mml:math id="M100" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> that
are close to the typical stratospheric values of <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.1</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula> DU. Other
sites occasionally have clean days with similarly low values.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p id="d1e1742"><inline-formula><mml:math id="M102" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> amounts vs. day of the year (DOY) and local
time (KST) for six sites as labeled in
each panel. Day 120 is 29 April, Day 130 is 9 May, Day 140 is 19 May, Day 150
is 29 May, Day 160 is 8 June, Day 170 is 18 June.</p></caption>
        <?xmltex \igopts{width=327.206693pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f05.jpg"/>

      </fig>

      <p id="d1e1761">The Seoul site frequently has amounts of <inline-formula><mml:math id="M103" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> greater than 2 DU. The
same is true of Olympic Park, located in the eastern part of the Seoul
metropolitan area. For locations increasingly distant from Seoul, the amount
of <inline-formula><mml:math id="M104" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> decreases in response to smaller local emissions, as the
short chemical lifetime of <inline-formula><mml:math id="M105" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> normally precludes long-distance
transport. Compared to Seoul, the two smaller southern cities, Gwangju and
Busan, have relatively low levels of <inline-formula><mml:math id="M106" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> on most days, with the most
typical values ranging<?pagebreak page4587?> from 0.3 to 0.5 DU, although high values exceeding 2
DU can occur on rare occasions.</p>
      <p id="d1e1827">Figure 4 shows the same data as Fig. 3, but in the form of a time series
covering the KORUS-AQ period. The daily variation (at least one point every
2 min) is shown in the vertical extent corresponding to each day's data.
Figures 3 and 4 show that sites near the Seoul metropolitan (e.g., Olympic
Park) area have larger amounts of pollution compared to those further away
(Taehwa, Songchon, and Yeoju). Even though average <inline-formula><mml:math id="M107" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts
are much lower at Songchon and Yeoju, there are times when the pollution
levels are quite high (<inline-formula><mml:math id="M108" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M109" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 2 DU, Figs. 4 and 5). There
are days when the amount of <inline-formula><mml:math id="M110" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> gets close to 4 DU in Seoul,
3 DU in Olympic Park and Busan, and 4 DU for one day in Yeoju (27 April).
The southern cities, Busan and Gwangju are much less polluted on average,
which results in a much smaller effect on adjacent regions. Busan is located
on the southeastern coastline, so that some of its <inline-formula><mml:math id="M111" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pollution
dissipates over the ocean, except for occasional days when very high amounts
(3 DU) occur. Anmyeondo is quite clean, as it is located on the western
coast well south of Seoul. The most frequently occurring <inline-formula><mml:math id="M112" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
value at Anmyeondo is 0.15–0.2 DU, which means that the measured
<inline-formula><mml:math id="M113" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> amount are partly from the stratosphere (<inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.1</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula> DU)
with very little tropospheric or boundary layer <inline-formula><mml:math id="M115" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. There are
occasional <inline-formula><mml:math id="M116" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> plumes that could be from industrial activity to
the north, and, perhaps, from China. Transport of <inline-formula><mml:math id="M117" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from China
occurs episodically in significant amounts (Lee et al., 2014).</p>
</sec>
<sec id="Ch1.S3">
  <?xmltex \opttitle{Diurnal variation of {$\protect\chem{C(NO_{{2}})}$}}?><title>Diurnal variation of <inline-formula><mml:math id="M118" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula></title>
      <?pagebreak page4588?><p id="d1e2002">Grouping the diurnal variation together from multiple days (Fig. 5) reveals a
pattern to <inline-formula><mml:math id="M119" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions and accumulation related to the main
<inline-formula><mml:math id="M120" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emission sources (automobiles and power generation) for the
three largest cities in Korea: Seoul (Pan40), Busan (Pan17), and Gwangju
(Pan26). For Seoul, the amounts of <inline-formula><mml:math id="M121" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> during the morning (1 DU
at 10:00 KST; all times are specified as Korean standard time (KST) in this paper) are much lower than
later in the afternoon (over 2–3 DU at 16:00) on almost every day with
values occasionally reaching as high as 6 DU. Even the relatively low
morning values of <inline-formula><mml:math id="M122" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> represent a significant amount of
pollution. The 6 DU <inline-formula><mml:math id="M123" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amount in Seoul is unusual, but
coincides with the peak values frequently occurring in the late afternoon.
<inline-formula><mml:math id="M124" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> behavior at nearby Olympic Park to the east of Seoul is very
similar to Yonsei University in the heart of Seoul, even though Olympic
Park's traffic density is lower than Seoul. Olympic Park is close enough to
the metropolitan Seoul area for the transport of <inline-formula><mml:math id="M125" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> combined with
local production from traffic to produce a very similar diurnal pattern. The
moderately large city of Busan also has high values of <inline-formula><mml:math id="M126" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>,
occasionally reaching 3 DU in the afternoon. Busan has relatively low values
of <inline-formula><mml:math id="M127" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the morning, having peaks in the mid-afternoon and
declining in the late afternoon. Gwangju, located in the southwest, is a
smaller city with less pollution (peak values <inline-formula><mml:math id="M128" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.6 DU) and does not
have as distinct an afternoon maximum.</p>
      <p id="d1e2136">The panels in Fig. 5 for Taehwa Mountain and Anmyeondo show regions outside the
Seoul metropolitan area that still show substantial amounts of <inline-formula><mml:math id="M129" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.
Compared to Seoul, the Taehwa site is a semi-rural location with only a
modest amount of car traffic in the immediate area. However, there are major
highways about 6 km from the site that are close enough to permit transport
of <inline-formula><mml:math id="M130" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to the Taehwa Mountain site. All of the sites showed a tendency
to have peak <inline-formula><mml:math id="M131" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> occur in the late afternoon. Anmyeondo on the west
central coast of Korea shows <inline-formula><mml:math id="M132" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts that are quite low with
occasional plumes arriving from the north or the west (China).</p>
      <p id="d1e2189">The basic daily pattern of <inline-formula><mml:math id="M133" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in urban Korea arises from large
amounts of automobile traffic and power plants emitting <inline-formula><mml:math id="M134" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
(for modern automobiles, roughly 99 % NO and 1 % <inline-formula><mml:math id="M135" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>). An
FTIR analysis of automobile exhaust shows that NO is emitted at 127 ppm,
<inline-formula><mml:math id="M136" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> at 1.6 ppm, HCHO at 39 ppm, and <inline-formula><mml:math id="M137" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:math></inline-formula> at 139 ppm
as part of the main emissions containing <inline-formula><mml:math id="M138" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> (144 ppm) and
<inline-formula><mml:math id="M139" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (122 ppm)
(<uri>https://tools.thermofisher.com/content/sfs/brochures/D10248~.pdf</uri>, last
access: 31 July 2018; see also Walters et al., 2015).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p id="d1e2286">Approximately 1 year of daily column <inline-formula><mml:math id="M140" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amount
data <bold>(a, d)</bold> and the monthly running average amount (dark plot in
panels <bold>a</bold> and <bold>d</bold>). The data are from GIST at Gwangju and
Amnyeondo. Panels <bold>(a)</bold> and <bold>(d)</bold> are the original time series
with one data point every 80 s, panels <bold>(b)</bold> and <bold>(e)</bold> are the
deseasonalized time series. Panels <bold>(c)</bold> and <bold>(f)</bold> are an
expanded scale of the monthly running averages <inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M142" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
that are identical to the solid lines in panels <bold>(a)</bold>
and <bold>(d)</bold>. The vertical extent <bold>(a, b, d, e)</bold> on a given day is
the range of diurnal variation from early morning to late afternoon.</p></caption>
        <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f06.jpg"/>

      </fig>

      <p id="d1e2381">NO quickly converts into <inline-formula><mml:math id="M143" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the presence of ozone and volatile
organic compounds VOCs in the atmosphere and can convert back to NO by solar
photolysis. KORUS-AQ results frequently show increasing <inline-formula><mml:math id="M144" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> during the
day with peaks in the afternoon. For these days the measurements imply that
the amount of locally produced <inline-formula><mml:math id="M145" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and conversion into <inline-formula><mml:math id="M146" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
dominates the losses of <inline-formula><mml:math id="M147" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> through photolysis and transport out of the
region. Other days occasionally show a different behavior, with <inline-formula><mml:math id="M148" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
peaks in the morning and a decline thereafter suggesting transport out of
the region.</p>
</sec>
<?pagebreak page4589?><sec id="Ch1.S4">
  <?xmltex \opttitle{Longer-term changes in {$\protect\chem{C(NO_{{2}})}$}}?><title>Longer-term changes in <inline-formula><mml:math id="M149" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula></title>
      <p id="d1e2474">Some of the sites used for the KORUS-AQ campaign (Gwangju and Amnyeondo) had
PSIs set up in April 2015, about 1 year before the start of the campaign.
Two other sites (Seoul and Busan) have PSI <inline-formula><mml:math id="M150" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> data starting in
2012. The extended data sets for Seoul and Busan provide the opportunity to
estimate 5-year changes in <inline-formula><mml:math id="M151" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amount and seasonal dependence.</p>
      <p id="d1e2511">In Fig. 6, the daily variation over one year at Gwangju and Anmyeondo are
evaluated to estimate one year secular trends. The vertical extent in the
time series is not noise or uncertainty, but rather the 80 s per data
point variability throughout each day (e.g., see Fig. 2). Before calculating
linear least squares slopes, the unadjusted time series (grey data points in
panels a and d) were deseasonalized (grey data points in panels b and e) by
subtracting a function with zero slope derived from a 30 day running average
(dark line in panels a and d or the identical curves in panels c and f). The
running average curves in panels (a) and (d) are shown with expanded scale in
panels (c) and (f) to clearly show the seasonal variation. The “zero slope
functions” ZM(<inline-formula><mml:math id="M152" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>) are obtained by subtracting a linear least squares fit
<inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:mi>L</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> to monthly running average curves <inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in panels (c) and (f) to form zero
slope functions <inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:mi mathvariant="normal">ZM</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi>M</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mi>L</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. The results ZM(<inline-formula><mml:math id="M156" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>) are functions that
look similar to the <inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> plots in panels (c) and (f), but with zero slopes. The
resulting ZM(<inline-formula><mml:math id="M158" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>) are then subtracted from the respective original time series
(grey circles) in panels (a) and (d). The results are the grey circles in panels (b) and (e). Similar monthly running means are shown in panels (b) and (e) that have
almost no monthly variations (see Appendix Fig. A1).</p>
      <?pagebreak page4590?><p id="d1e2613">The linear trends in Fig. 6b and e suggest that there was an increase in
pollution levels in Gwangju and Anmyeondo over the period of observation. The
southern city of Gwangju (Pan 26) has higher average <inline-formula><mml:math id="M159" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
amounts, <inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.34</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.19</mml:mn></mml:mrow></mml:math></inline-formula> DU, compared to the relatively clean coastal site
Amnyeondo, <inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.26</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.14</mml:mn></mml:mrow></mml:math></inline-formula> DU. Gwangju seasonal cycle has a minimum in
<inline-formula><mml:math id="M162" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amount in September–October and a very broad maximum from
December to May. The Gwangju PSI is located away from major city traffic on a
university campus (Gwangju Institute of Science and Technology, GIST) so that
the average amount of <inline-formula><mml:math id="M163" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (about 0.34 DU) is moderate with some
days reaching 1.5 DU. The slopes are statistically significant at the
2-standard deviation level (<inline-formula><mml:math id="M164" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>) and imply that <inline-formula><mml:math id="M165" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> was
increasing at a substantial rate. However, the period of observation was too
short to estimate multi-year long-term trends. Additional long-term
monitoring of these sites would be desirable for air quality purposes.</p>
      <p id="d1e2715">The PSI on Anmyeondo was located away from a commercial area with moderate
traffic and very near the shore of the Yellow Sea at a regional Global
Atmosphere Watch (GAW) station. For Amnyeondo there is a clear seasonal
cycle similar to that in Gwangju with a minimum in September–October and a
broad maximum during the winter–spring months. Amnyeondo had an average
amount of 0.25 DU, which is lower than observed at Gwangju.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><caption><p id="d1e2721"><bold>(a)</bold> <inline-formula><mml:math id="M166" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> time series at Yonsei University in
Seoul <inline-formula><mml:math id="M167" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>(grey) and <bold>(b)</bold> deseasonalized time series.
Combined slope <inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.001</mml:mn></mml:mrow></mml:math></inline-formula> DU yr<inline-formula><mml:math id="M169" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> and mean <inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.2</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.8</mml:mn></mml:mrow></mml:math></inline-formula> DU or the decrease is <inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.08</mml:mn></mml:mrow></mml:math></inline-formula> % yr<inline-formula><mml:math id="M172" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. Seoul has no
clear seasonal cycle.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f07.jpg"/>

      </fig>

      <p id="d1e2832">Figures 7 and 8 each contain an approximately 5-year daily time series (grey)
for Seoul (Yonsei University) and Busan (Pusan University) and a linear fit
to a deseasonalized version of the time series. As the observations at both
sites had an extended period of missing data, the slopes were estimated
separately for each segment and for the combined time series. Both Seoul and
Busan show a steady reduction in <inline-formula><mml:math id="M173" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> air pollution with an average
reduction of about <inline-formula><mml:math id="M174" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4 %<?pagebreak page4591?> per year. A recent paper by Duncan et
al. (2016) estimated a decrease in <inline-formula><mml:math id="M175" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> for Seoul in about a <inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:mn mathvariant="normal">10</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> km box of about <inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.6</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.4</mml:mn></mml:mrow></mml:math></inline-formula> % per year over the 2004 to
2013 period based on a 2014 average <inline-formula><mml:math id="M178" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amount of 0.6 DU, or
about half of the average value <inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.8</mml:mn></mml:mrow></mml:math></inline-formula> DU observed by the PSI. The
larger reduction in <inline-formula><mml:math id="M180" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> measured by the PSI is caused by a
reduction in higher than average afternoon <inline-formula><mml:math id="M181" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts that are
rarely observed by OMI overpass at 13:30 KST. OMI is a polar orbiting push broom hyperspectral instrument
(300–500 nm with a spectral resolution of 0.45 nm in the UV and 1 nm in
the visible, and a spatial resolution of <inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:mn mathvariant="normal">13</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">24</mml:mn></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M183" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>) onboard
the AURA satellite. The high observed late afternoon values are not
restricted to Seoul, but occur for all of the urban areas where the PSI has
been deployed. The high late afternoon values do not regularly occur in
remote rural areas such as Amnyeondo.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><caption><p id="d1e2981"><bold>(a)</bold> Pusan University in Busan <inline-formula><mml:math id="M184" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> daily time
series (grey) and <bold>(b)</bold> deseasonalized time series with linear
trends.</p></caption>
        <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f08.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p id="d1e3014"><bold>(a)</bold> Comparisons between the daily values of
<inline-formula><mml:math id="M185" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> for OMI (black) and PSI (red) at Seoul and Busan for a
5-year period. Solid lines show the average seasonal variation (Lowess(0.1)),
see also panel <bold>(b)</bold>. Linear interpolation is used where there are
missing data points. <bold>(b)</bold> Comparisons between the seasonal averages
for <inline-formula><mml:math id="M186" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> from OMI (black) and PSI (red) at Seoul and Busan for a
5-year period. The lower panels show the seasonal difference between the PSI
and OMI. The individual data points are shown derived from a Lowess(0.1)
smoothing, approximately a 3-month running averages of the daily data.
Interpolation has been used where there are missing data
points.</p></caption>
        <?xmltex \igopts{width=327.206693pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f09.png"/>

      </fig>

      <p id="d1e3065">Seoul and Busan <inline-formula><mml:math id="M187" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> measurements are remarkable for the large peak
amounts that are seen on many days compared to the 1.5 to 2 DU peak values
for Gwangju and Amnyeondo. For Yonsei, the peak values range above 5 to 6 DU
in the years 2012 to 2015, but decrease somewhat in 2015 to 2016. In 2015–2016, the decrease appears to be large, but is only 0.2 DU relative to a
mean of about 1.2 DU. A smaller decrease appears for Busan (Fig. 8) relative
to a mean of about 0.6 DU. All of the PSI measurements show very high values
of <inline-formula><mml:math id="M188" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> during almost every day when measurements were possible. As
the <inline-formula><mml:math id="M189" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations represented by these large column amounts are
probably in the boundary layer near the sources of <inline-formula><mml:math id="M190" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, there is a
strong effect on local air quality.</p>
</sec>
<sec id="Ch1.S5">
  <title>Comparison with OMI satellite overpass data</title>
      <p id="d1e3125">Seoul and Busan have 5-year PSI data records (Fig. 9a and b), and Gwangju has
a 1-year data record (Figs. 6 and 10) spanning the KORUS-AQ campaign. The PSI
<inline-formula><mml:math id="M191" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> can be matched in time (<inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula> min) with the overpass time
from OMI onboard the AURA satellite (mid-day overpass times <inline-formula><mml:math id="M193" display="inline"><mml:mrow><mml:mn mathvariant="normal">13</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">30</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">90</mml:mn></mml:mrow></mml:math></inline-formula> min). Figure 9a shows the <inline-formula><mml:math id="M194" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> daily variation at the OMI
overpass time with far more high values of <inline-formula><mml:math id="M195" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> from the PSI than
observed by OMI. The solid lines represent the seasonal dependence, which are
shown separately in Fig. 9b along with the <inline-formula><mml:math id="M196" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> differences, PSI
- OMI. The result is that the average PSI values are double those observed by
OMI's large FOV (OMI Version 03:
<uri>https://avdc.gsfc.nasa.gov/index.php?site=666843934&amp;id=13</uri>, last access:
31 July 2018).</p>
      <p id="d1e3226">The seasonal dependence (Fig. 9b) of <inline-formula><mml:math id="M197" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> from OMI for both Seoul and
Busan is fairly regular, with maxima in January of each year and minima in
July–August. The seasonal behavior of <inline-formula><mml:math id="M198" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> obtained from the PSI in
Seoul varies with high values extending from January into the summer months
and with minima varying from August in 2012, September–October in 2013,
missing in 2014, July in 2015, and June in 2016. For Busan, the maxima occur
in the spring for 2013 and 2014, October for 2015, and in the spring for
2016. The minima are also variable. The difference between OMI and PSI
retrievals depends on local conditions for PSI and on an area average for
OMI.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><caption><p id="d1e3265"><inline-formula><mml:math id="M199" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> time series from Pandora (red) and OMI (black) for
GIST University in Gwangju Korea and their differences. The comparison is
formed from time coincidences between Pandora and OMI.</p></caption>
        <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f10.png"/>

      </fig>

      <p id="d1e3290">Figure 9b shows that the PSI has a mean difference compared to OMI in Busan
of 0.35 DU and peak values (up to 2.5 DU at 13:30 and 4 DU in the late
afternoon). The differences are important when considering pollution effects
on human health (Krafta et al., 2005; Latza et al., 2009). Even larger
differences are observed in Seoul, where the mean difference is 0.58 DU
between Pandora and OMI at the satellite overpass time. The results from PSI
suggest that local ground-based monitoring of pollution is important for
estimating their impact on human health, particularly as amounts of
<inline-formula><mml:math id="M200" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> occurring later in the afternoon exceed the amounts at the time
of the satellite overpass.</p>
      <?pagebreak page4592?><p id="d1e3311">A comparison with Lowess(0.1) fits (Locally Weighted least squares fit to 0.1
of the data points; Cleveland, 1981) to the matched Pandora vs. OMI overpass
data (about 3-month averages) shows that PSI <inline-formula><mml:math id="M201" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is larger than
OMI measured <inline-formula><mml:math id="M202" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> mostly because of its much smaller 2<inline-formula><mml:math id="M203" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
field of view (a circle of 35 m diameter at 1 km altitude) compared to
OMI's FOV of <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:mn mathvariant="normal">13</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">24</mml:mn></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M205" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> at nadir, which may encompass areas
outside of the city or the adjacent ocean areas. For example, the center of
Seoul is about 48 km from the Yellow Sea, while the OMI overpass file lists
FOV center distances of over 60 km from Seoul. Another possible reason for
the differences is that OMI <inline-formula><mml:math id="M206" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> retrievals use <inline-formula><mml:math id="M207" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
vertical profile shape factors from the low resolution (<inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">110</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">110</mml:mn></mml:mrow></mml:math></inline-formula> km) Global Model Initiative (GMI) model simulation to calculate air
mass factors that are used to determine observed tropospheric <inline-formula><mml:math id="M209" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
vertical columns, while much finer resolution profiles are needed to more
accurately represent highly polluted urban areas such as Seoul. Increases in
OMI retrieved tropospheric column <inline-formula><mml:math id="M210" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> up to 160 % are found
when using model derived <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.33</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1.33</mml:mn></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M212" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> profile shape factors
(Goldberg et al., 2017). The effect of moderate amounts of cloud or aerosol
have little effect on the PSI direct -sun spectral fitting retrieval of
<inline-formula><mml:math id="M213" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> as shown in Fig. 2. OMI and MAXDOAS retrievals are sensitive
to the presence of aerosols and clouds (Kanaya et al., 2014), which may
contribute to the underestimate of <inline-formula><mml:math id="M214" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> by OMI even after
corrections are made for retrieved aerosol and cloud amounts (Chimot et al.,
2016).</p>
      <p id="d1e3499">The implications for assessing clean air indices suggest that OMI
underestimates the human health effect from trace gases such as <inline-formula><mml:math id="M215" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>,
especially in highly populated urban areas. Figure 5 gives a much clearer
picture of the degree of pollution than is possible with just the 13:30 OMI
comparison measurements, as the late afternoon is the time of maximum
pollution.</p>
      <p id="d1e3513">The city of Gwangju is much smaller than Busan, with less industrial
activity, especially automobiles. PSI observations at GIST show much closer
agreement with OMI (Fig. 10), especially as GIST is located within the
city boundaries, but in an area with much less concentrated industrial
activity compared to the center of Gwangju. The large OMI FOV over a
relatively clean area reduce the OMI difference in measured <inline-formula><mml:math id="M216" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> amount
compared to the PSI <inline-formula><mml:math id="M217" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts. OMI still measures less than the
PSI (<inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.12</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.15</mml:mn></mml:mrow></mml:math></inline-formula> DU), but the mean difference is not statistically
significant. However, OMI clearly misses the high values of <inline-formula><mml:math id="M219" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> that
are present in the PSI observations.</p>
<?pagebreak page4593?><sec id="Ch1.S5.SSx1" specific-use="unnumbered">
  <title>Comparison with 4STAR DC-8 overpass data</title>
      <p id="d1e3578"><inline-formula><mml:math id="M220" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> results were obtained by the Spectrometer for Sun-tracking
Sky-Scanning Atmospheric Research (4STAR) flown on-board the DC-8 during
KORUS-AQ and compared with the PSI (Fig. 11). The 4STAR is an airborne
sunphotometer, capable of measuring total <inline-formula><mml:math id="M221" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M222" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>,
water vapor and AOD columns in its direct-sun mode (Segal-Rozenhaimer et al.,
2014; Shinozuka et al., 2013), which is similar to the mode used by the PSI
network.</p>
      <p id="d1e3631">A detailed description of 4STAR is given in Dunagan et al. (2013). In brief,
the instrument has two structurally rigid grating array spectrometers that
are combined to yield continuous spectra between 300 and 700 nm. The
instrument sampling rate is 1 Hz, and the nominal integration time used for
<inline-formula><mml:math id="M223" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> retrievals is 50 ms (with six spectra averaged per one
sampling period). Dark counts are measured every 20 min using a shutter
mechanism. The 4STAR light collection system has fiber optic bundle
foreoptics that is connected to the spectrometers. A two axis motion control
system with analog feedback provides active tracking of the solar disk. The
instrument full field of view (FOV) is <inline-formula><mml:math id="M224" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.25</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M225" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. <inline-formula><mml:math id="M226" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
is retrieved following a method described in Segal-Rozenhaimer et al. (2014),
but using the 460–490 nm spectral range. A series of 4STAR columnar
<inline-formula><mml:math id="M227" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> values above aircraft (for legs below 300 m) taken from DC-8
“missed approach” maneuvers flying over Olympic Park PSI station, within a
radius of 5 km, are shown in Fig. 11. There is a relatively good correlation
(<inline-formula><mml:math id="M228" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula>), with a slight positive bias of 4STAR compared with the PSI
values. This might result from higher noise effects (i.e., small amount of
spectra averages) for 4STAR during the fast change of altitude when the
aircraft performs its “missed approach” overpasses over the PSI stations.
Relaxing the altitude constraint to include legs below 500 m showed good
agreement with the PSI station at Taehwa Mountain, but with an overall lower
correlation coefficient (<inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.54</mml:mn></mml:mrow></mml:math></inline-formula>), which is expected due to averaging of
larger vertical range. As with PSI, 4STAR shows better agreement with OMI
<inline-formula><mml:math id="M230" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> for low values of <inline-formula><mml:math id="M231" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, but considerable
differences over polluted areas (Segal-Rozenhaimer et al., 2018), when 4STAR
<inline-formula><mml:math id="M232" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values are averaged within each of the OMI pixels
corresponding to the flight path for each of the days.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><caption><p id="d1e3781">A correlation plot of <inline-formula><mml:math id="M233" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> from 4STAR onboard the DC-8
compared to the <inline-formula><mml:math id="M234" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amount measured by the PSI at Olympic Park
on nine different days. The solid black line is the 1 : 1 line drawn for
reference. The dashed line represents the data linear fit, with a slope of
1.05, and a correlation coefficient <inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula>, as shown on the plot.</p></caption>
          <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f11.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><caption><p id="d1e3842">C(HCHO) from PSI at Olympic Park for 6 days in June 2016. C(HCHO) on
2 June 2016 has a peak value of 2.3 DU at 14:30 KST.</p></caption>
          <?xmltex \igopts{width=298.753937pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f12.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S6">
  <title>Formaldehyde from five Korus-AQ sites</title>
      <p id="d1e3858">PSI makes two sets of direct-sun measurements every 80 s. One set is
for measurements in the visible range (380–525 nm used for <inline-formula><mml:math id="M236" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) and
the other is for the UV range (290–380 nm with a filter, U340, which
blocks visible light). Formaldehyde is derived from the same set of spectral
measurements used for ozone (i.e., with a U340 blocking filter), but using
the spectral range 332–359 nm. Sources of error in the C(HCHO) retrieval
arise from the selection of the fitting window and the amount of C(HCHO)
remaining in the reference spectrum after application of the modified
Langley estimation (MLE) method of calibration (Herman et al., 2009; Spinei
et al., 2018). The MLE extrapolation to zero C(HCHO) could have an offset
error of 0.1 to 0.2 DU. Selecting different fitting windows can also cause
the C(HCHO) retrievals to differ. For example, a wider alternate fitting
window, 324–360 nm, retrieves HCHO values that are about 8 % higher
because of different amounts of interference from overlapping absorption by
<inline-formula><mml:math id="M237" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M238" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and BrO at the spectral resolution of 0.5 to 0.6 nm
currently in use. Absolute offset errors do not affect the retrieval
precision (relative column amounts), which is approximately 0.1 DU. A
detailed analysis of the algorithms and uncertainties is discussed by Spinei
et al. (2018).</p>
      <?pagebreak page4594?><p id="d1e3894"><?xmltex \hack{\newpage}?>The Olympic Park area has much more vegetation than central Seoul for the
production of isoprene (<uri>http://www.olympicpark.co.kr</uri>, last access:
31 July 2018), which is a significant source of the chemicals needed for
formaldehyde production in the atmosphere (Luecken et al., 2012).
Observations from PSI show that C(HCHO) starts out every day at low levels
0.6 DU at about 08:00 and increases to over 2 DU until 18:00 (Figs. 12 and
13). Most HCHO arises from photochemical production, while a significant
fraction is chemically derived from automotive emissions in densely populated
urban areas (Friedfeld et al., 2002; Garcia et al., 2006; Lei et al., 2009;
Liteplo et al., 2010). Regardless of the precursor source, HCHO forms in the
atmosphere primarily though photochemistry, which causes HCHO to usually be
at a minimum early in the day, increase into the afternoon, and decline
towards evening. The PSI C(HCHO) observations (Figs. 12 and 13) support this
pattern of daily variation.</p>
      <p id="d1e3901">A summary of the daily time dependence of C(HCHO) at Olympic Park during the
entire KORUS-AQ campaign is shown in Fig. 13. As in Fig. 12, minimum values
are observed in the morning (06:00–08:00) before the chemical and direct
sources of HCHO are significant. There is strong buildup during the day that
reached a maximum between 15:00 to 16:00, and then diminished towards
sunset. As with <inline-formula><mml:math id="M239" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, the daily pattern of late afternoon peaking of
HCHO amounts presents a problem for polar orbiting satellite observations
(e.g., OMI observations at 13:30) assessing air quality.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13"><caption><p id="d1e3917">Pandora measured formaldehyde amounts vs. day of the year and local
time for 29 April 2016 to 11 June 2016 in Olympic Park.</p></caption>
        <?xmltex \igopts{width=184.942913pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f13.jpg"/>

      </fig>

      <p id="d1e3927">Figure 14 shows two altitude profiles acquired by the Compact Atmospheric
Multispecies Spectrometer (CAMS) (Richter et al., 2015) onboard the DC-8
aircraft as it spiraled over the Olympic Park area on 4 May 2016 in the
morning and at midday. Quoting from Richter et al. (2015):<disp-quote>
  <p id="d1e3931">CAMS is a multi-species spectrometer configured for the simultaneous
detection of ethane (<inline-formula><mml:math id="M240" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) and formaldehyde (<inline-formula><mml:math id="M241" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>).
The spectrometer utilizes a tunable, fiber optically pumped difference
frequency generation laser source in combination with a Herriott type
multi-pass absorption cell with an effective path length of 89.6 m.</p>
</disp-quote></p>
      <p id="d1e3964">The morning integrated amount on 4 May was <inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.02</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molecules cm<inline-formula><mml:math id="M243" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (0.38 DU) and the afternoon amount
was <inline-formula><mml:math id="M244" display="inline"><mml:mrow><mml:mn mathvariant="normal">6.95</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molecules cm<inline-formula><mml:math id="M245" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (0.26 DU), both substantially less than the PSI measured values of
0.48 and 0.42 DU, respectively. There were no surface measurements of
HCHO mixing ratio on 4 May at Olympic Park. On 2 June at 11:40 there was a
surface measurement 3.94 ppb. Including the surface measurement in the
profile integral yields Integ(0.026, 7.2 km) <inline-formula><mml:math id="M246" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.55 DU, while PSI measured
1.2 DU, which is<?pagebreak page4595?> consistent with the differences shown in Fig. 14. The
notation in Fig. 14 is <inline-formula><mml:math id="M247" display="inline"><mml:mrow><mml:mi mathvariant="normal">Integ</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi>z</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∫</mml:mo><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:munderover><mml:mrow class="chem"><mml:mi mathvariant="normal">HCHO</mml:mi></mml:mrow><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> for the altitudes <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M249" display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M250" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> is in km.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14"><caption><p id="d1e4109">HCHO altitude profile measured by CAMS onboard the DC-8 on 4 May at
07:54 KST <bold>(a)</bold> and
11:54 KST <bold>(b)</bold> over Olympic Park, Korea.
<bold>(c)</bold> PSI measurements of total column HCHO. Vertical
bars <bold>(c)</bold> mark the DC-8 flight duration for the profiles yielding
altitude integrated column amounts of 0.38 and 0.26 DU.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f14.jpg"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F15" specific-use="star"><caption><p id="d1e4132">DC-8 CAMS HCHO mixing ratio measurements over Olympic Park on
4 June. The continuous blue profiles show the 1 s HCHO data while the black
points with error bars show the 10 s average and standard deviation of this
data at points of closest approach above the Olympic Park site.</p></caption>
        <?xmltex \igopts{width=327.206693pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f15.png"/>

      </fig>

      <p id="d1e4141">The profiles used data for lower altitudes obtained from aircraft “missed
approach” maneuvers at a nearby Seoul Airbase, 8.5 km from Olympic Park,
(Fig. 15). When available, a single surface altitude point was added using
ground-based volume mixing ratio measurements obtained from US Environmental
Protection Agency measurements using quantum cascade laser instruments (Fried
et al., 2008; Hottle et al., 2009; Richter et al., 2015; Spinei et al., 2018
and references therein). The DC-8 minimum altitude exactly over Olympic Park
was typically around 0.4 km above the surface (black circles Fig. 15). Large
vertical CAMS retrieved HCHO gradients were observed as the DC-8 descended to
lower altitudes over Seoul Airbase. A comparison of 10 s DC-8 HCHO averages
at the points of closest spatial approach to the Olympic Park (black circles)
site on 4 June, for example, to peak HCHO measurements during missed
approaches at the nearby Seoul Airbase (20–40 m above the ground) revealed
ratios in the observed HCHO (black circles) ranging between 75 % to
83 % of the maximum values near the surface. As Olympic Park DC-8
overpasses miss significant near-surface HCHO amounts, the profiles shown in
Figs. 14 and 16 incorporate the HCHO amounts down to the surface at an
altitude of 0.026 km a.s.l (above sea level) derived from the “missed
approach” at Seoul airbase. HCHO measurements above the maximum altitude
over Olympic Park (see Figs. 14 and 16) were taken from the closest time over
the Taewha Mountain site, 28 km from Olympic Park. The assumption is that
the horizontal gradients above 2.2 km (Fig. 15) can be neglected.</p>
      <p id="d1e4145">After conversion from mixing ratio to molecules cm<inline-formula><mml:math id="M251" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> using the measured
atmospheric density, the resulting profile data were integrated from the
minimum (0.026 km asl, Table 1) to the maximum heights indicated in Fig. 14.
The result is 0.38 DU at 07:54 and 0.26 DU at 11:54 compared to the
measurements from the Pandora instrument 0.48 and 0.38 DU The derived
vertical HCHO columns from the DC-8 data in Fig. 14a and b are 79 % of
PSI measured C(HCHO) in the morning and 68 % of PCI C(HCHO) at midday
(Fig. 14c).</p>
      <p id="d1e4160">A similar comparison is shown in Fig. 16 for 5 June 2016 where the amount of
C(HCHO) is much larger than on 4 May. Integration of the measured profiles
yields column densities of 0.60 and 0.82 DU at 08:30 and 15:21 h. For
this case, at both times the CAMS DC-8 values are about 77 % and 63 %
of the PSI measured column amounts, 0.78 and 1.3 DU. For both cases in Figs. 14 and 15 the 23 % to 37 % differences are outside of the expected
error from PSI fitting window selection and from residual HCHO included in
the MLE calibration method.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F16"><caption><p id="d1e4165">HCHO altitude profiles measured by CAMS onboard the DC-8 on 5 June
at 08:30 KST <bold>(a)</bold> and
15:21 KST <bold>(b)</bold> over Olympic Park, Korea. <bold>(c)</bold> PSI
measurements of total column HCHO. Vertical bars mark the DC-8 flight
duration for the profiles yielding column amounts of 0.60 and 0.82 DU.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f16.jpg"/>

      </fig>

      <p id="d1e4183">Another Olympic Park case on 9 June 2016 shows CAMS <inline-formula><mml:math id="M252" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.79 vs.
PSI <inline-formula><mml:math id="M253" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1 DU at 08:06, CAMS <inline-formula><mml:math id="M254" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.74 vs. PSI <inline-formula><mml:math id="M255" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.3 DU at 12:12, and
CAMS <inline-formula><mml:math id="M256" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.13 vs. PSI <inline-formula><mml:math id="M257" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.9 DU, or the CAMS measurements on the DC-8
are 79 % and 57 % less than the PSI total column HCHO. All of the
remaining comparisons of CAMS DC-8 profile results with PSI C(HCHO) show
similar results. The reasons for the disagreement between C(HCHO) measured by
direct sun observations (PSI) and the integrated column density from aircraft
measurements of HCHO VMR are not known. Contributions to the differences
include the selection of the PSI wavelength window (332–359 nm) and
possible interference from overlapping <inline-formula><mml:math id="M258" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M259" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
absorption that are not properly included, and, more likely, the use of CAMS
measured volume mixing ratios at the lowest altitudes from the nearby Seoul
airbase, 8.5 km from Olympic Park, where spatial variation may affect the
calculation of C(HCHO). The use of Taehwa Mountain data for higher altitudes over
Olympic Park contributes 25 % for 3 of the above cases and 50 % for
4 May 2016 at 07:54 (Fig. 14a). This is probably not the reason for the
disagreement between CAMS and PSI, as the percent underestimate for CAMS
over Taewha is about the same magnitude (Table 2) as over Olympic Park.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2"><caption><p id="d1e4254">Taehwa Mountain. DC-8 compared to PSI measurements in Fig. 18.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Date KST</oasis:entry>
         <oasis:entry colname="col2">DC-8 HCHO DU</oasis:entry>
         <oasis:entry colname="col3">PSI HCHO</oasis:entry>
         <oasis:entry colname="col4">%</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">11 May 08:25:19</oasis:entry>
         <oasis:entry colname="col2">0.4</oasis:entry>
         <oasis:entry colname="col3">0.6</oasis:entry>
         <oasis:entry colname="col4">67</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">18 May 08:34:26</oasis:entry>
         <oasis:entry colname="col2">0.4</oasis:entry>
         <oasis:entry colname="col3">0.5</oasis:entry>
         <oasis:entry colname="col4">80</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">30 May 12:05:00</oasis:entry>
         <oasis:entry colname="col2">0.5</oasis:entry>
         <oasis:entry colname="col3">0.9</oasis:entry>
         <oasis:entry colname="col4">56</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">10 June 08:22:45</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">1.16</oasis:entry>
         <oasis:entry colname="col4">86</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">10 June 12:22:53</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">1.5</oasis:entry>
         <oasis:entry colname="col4">67</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">10 June 15:46:03</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">1.3</oasis:entry>
         <oasis:entry colname="col4">77</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e4384">PSI measurements show that Olympic Park produces more HCHO almost every day
than observed at the Yonsei University in Seoul and Taehwa Mountain sites
(Figs. 12, 17, 18). The hourly variations observed during the KORUS-AQ
campaign at the Yonsei University in Seoul and at Taehwa Mountain sites are
similar to Olympic Park even though most of the HCHO is locally produced by
photochemistry, but has a relatively short lifetime of a few hours in
polluted air where there is significant ozone and OH. However, at typical
wind speeds of 10–20 km h<inline-formula><mml:math id="M260" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> and a chemical lifetime of 2.5 h (Dufour
et al., 2009), HCHO can be transported about 25–50 km, which<?pagebreak page4596?> is far
enough for some transport of HCHO between the PSI sites at Yonsei, Olympic
Park, and Taewha Mountain DC-8 CAMS results over the Taehwa Mountain site compared
to PSI are given in Table 2 with differences similar to Olympic Park.</p>
      <p id="d1e4399">Figure 19a and b summarizes all of the C(HCHO) data obtained during KORUS-AQ
at the five sites. The graphs on the left show all of the data points (light
gray circles) as a function of the local time and a Lowess(0.1) fit to the
data showing the average hourly behavior. The spread of the data about the
Lowess(0.1) fit represents the day-to-day variation at a given local time. On
average, Mt. Taehwa tends to increase throughout each day, while Yonsei and
Olympic Park show maxima at 14:00 and 15:30 KST, respectively. Similarly, in
Fig. 18b Yeogju increases during the day having a maximum at 17:42 KST while
Anmyeondo has a broad peak with maxima at 12:00 and 13:42 KST.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F17"><caption><p id="d1e4404">Total column HCHO from Pandora Yonsei University, Seoul for 6 days
in June 2016. C(HCHO) on 2 June 2016 has a peak value of 1.2 DU at 13:30.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f17.jpg"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F18"><caption><p id="d1e4415">Total column HCHO from Pandora Taehwa Mountain for 6 days in June
2016. C(HCHO) on 2 June 2016 has a peak value of 1.2 DU at 12:45. <inline-formula><mml:math id="M261" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>
are DC-8 CAMS measurements on 10 June.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f18.jpg"/>

      </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F19" specific-use="star"><caption><p id="d1e4434"><bold>(a)</bold> Summary of total column HCHO for the stated dates
during the KORUS-AQ campaign. The solid line is a Lowess(0.1) fit to the
data. The sharp cutoffs in panels <bold>(a)</bold>, <bold>(b)</bold>, and
<bold>(c)</bold> were caused obstructions of the direct sun from the PSI FOV in
the afternoon. <bold>(b)</bold> Summary of total column HCHO for the stated dates
during the KORUS-AQ campaign. Panels <bold>(a)</bold> and <bold>(b)</bold> represent
the daily variation at a given local time. The solid line is a Lowess(0.1)
fit to the data. Panels <bold>(c)</bold> and <bold>(d)</bold> show the frequency of
occurrence (%) for different amounts of C(HCHO).</p></caption>
        <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f19.jpg"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F20" specific-use="star"><caption><p id="d1e4472">The springtime change in C(HCHO) over about a 40 day period
depending on the site. The “vertical bars” are the diurnal variation within
each day of data. The thicker red curve is a Lowess(0.3) fit to the data,
while the thin red line is a linear least squares fit. The Lowess(0.3) fit is
approximately a 10-day local least-squares average.</p></caption>
        <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f20.png"/>

      </fig>

      <p id="d1e4481">The histograms on the right side of Fig. 19 represent the percent frequency
of occurrence of C(HCHO) in 0.1 DU bins. C(HCHO) at Mt. Taehwa and Seoul
rarely exceeds 1.5 DU compared to Olympic Park where C(HCHO) <inline-formula><mml:math id="M262" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 2 DU for a significant fraction of time. The most frequent values are 0.6 DU
for Seoul, 0.9 DU for Mt. Taehwa, and over 1 DU for Olympic Park. Olympic
Park also has a broader distribution towards higher values of C(HCHO) than
other sites.</p>
      <?pagebreak page4597?><p id="d1e4491"><?xmltex \hack{\newpage}?>The general intra-day C(HCHO) time dependence and C(HCHO) percent occurrence
are shown for two additional sites (Fig. 19b), Yeogju and Amnyeondo. Yeogju
shows an increase in C(HCHO) from morning to a peak value of 0.85 DU at
14:42 KST, which then declines after 16:00 KST. In contrast, Amnyeondo is
almost symmetric with the sun position, having a maximum of about 0.77 DU
near 12:00 and 13:42 KST.</p>
      <p id="d1e4495">The average change in C(HCHO) during the spring campaign at the five sites
is summarized in Fig. 20. Of the sites, Olympic Park showed the largest
change rate, 58 % month<inline-formula><mml:math id="M263" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> followed by Amnyeondo at 50 % month<inline-formula><mml:math id="M264" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, then
Taehwa (33 % month<inline-formula><mml:math id="M265" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>), Yonsei Seoul (25 % month<inline-formula><mml:math id="M266" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>), and Yeogju (<inline-formula><mml:math id="M267" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>13 % month<inline-formula><mml:math id="M268" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). Amnyeondo tends to have lower C(HCHO) amounts because of its
relatively isolated coastal location. These 2-month trends include seasonal
increases during the campaign months May and June, 2016.</p>
      <p id="d1e4567">It is difficult to compare PSI C(HCHO) with OMI for the KORUS-AQ period,
as OMI overpass C(HCHO) data for 2016 have some missing days (Fig. 21).
For days with matching data points over Seoul, PSI C(HCHO) (approximately
0.8 DU) is almost always larger than the OMI values (0.2 DU) plus a few very
high PSI values and two high OMI values. The general day-to-day variations
are similar.</p>
</sec>
<sec id="Ch1.S7" sec-type="conclusions">
  <title>Summary</title>
      <p id="d1e4576">Nine Pandora Spectrometer Instruments, PSI, were installed at eight sites in
South Korea as part of the KORUS-AQ ground, aircraft, and satellite
measurements for air-quality studies. The measurements made during the
months of April to June by PSI showed very high amounts of urban pollution
from <inline-formula><mml:math id="M269" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and HCHO, and more moderate, but still high values in Mt
Taewha and Yeogju, which are some distance from the major urban centers,.
The urban areas show minimum values in the morning that rise rapidly
throughout the day, peaking in the late afternoon for both <inline-formula><mml:math id="M270" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and
C(HCHO). An exceptionally clean location was Amnyeondo, which is located on
a western coastal island adjacent to the Yellow Sea about 100 km south of
Seoul.</p>
      <p id="d1e4607">PSI direct-sun retrieved values of <inline-formula><mml:math id="M271" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and C(HCHO) are always larger
than OMI retrieved <inline-formula><mml:math id="M272" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and C(HCHO) for the OMI overpass times (<inline-formula><mml:math id="M273" display="inline"><mml:mrow><mml:mn mathvariant="normal">13.5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> h). In urban areas, PSI <inline-formula><mml:math id="M274" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> averages are at least a
factor of two larger than OMI averages. Similar differences are seen for
C(HCHO) in Seoul. However, late afternoon values measured by PSI are even
larger, implying that OMI measurements underestimate the effect of poor air
quality on human health. The primary cause of the OMI underestimate at its
overpass time is the large OMI FOV that includes regions containing low
values of pollutants. In relatively clean areas, PSI and OMI are more
closely in agreement.</p>
      <?pagebreak page4599?><p id="d1e4673">PSI retrieved <inline-formula><mml:math id="M275" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts for Seoul frequently exceed 2 DU and
occasionally reach 6 DU. Other urban centers in the south, Busan and
Gwangju, have smaller <inline-formula><mml:math id="M276" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts, but exhibit a similar strong
diurnal pattern, namely low values in the morning and high values later
during midday. This behavior is expected because of the large number of
urban automobiles and concentrated industry. Urban areas downwind from Seoul
show high <inline-formula><mml:math id="M277" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts, but also show daily minimum amounts in the
morning that increase later in the day. Two of the sites, Seoul and Busan,
have long-term <inline-formula><mml:math id="M278" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> data records, 2012–2016, that suggest a
gradual decrease in <inline-formula><mml:math id="M279" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> amounts in Korea. When compared with OMI,
both ground-based PSI's and the 4STAR aircraft instrument onboard the DC-8
show that the correlation is best for small values of <inline-formula><mml:math id="M280" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in the
troposphere and stratosphere, and worst for high values that are usually in
the boundary layer near their local sources. In Olympic Park, the
measurements of significant values of C(HCHO) and high values of <inline-formula><mml:math id="M281" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
in the afternoon suggest that there are also increased boundary layer
amounts of ozone.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F21"><caption><p id="d1e4798">Compare PSI (bullet) and OMI (red circles) retrievals of C(HCHO) at
<inline-formula><mml:math id="M282" display="inline"><mml:mrow><mml:mn mathvariant="normal">13.30</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> KST. OMI overpass data, V03, are from
<uri>https://avdc.gsfc.nasa.gov/index.php?site=1113974256&amp;id=81</uri> (last
access: 31 July 2018).</p></caption>
        <?xmltex \igopts{width=184.942913pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f21.jpg"/>

      </fig>

      <p id="d1e4823">C(HCHO) amounts were obtained for five sites, Yonsei University in Seoul,
Olympic Park,<?xmltex \hack{\vadjust{\newpage}}?> Taehwa Mountain, Amnyeondo, and Yeoju.
Of these the largest amounts of C(HCHO) were observed at Olympic Park, and
Taehwa Mountain, both surrounded by significant amounts of vegetation.
Comparisons of PSI results were made with overflights on the DC-8 aircraft
for Taehwa Mountain and Olympic Park showing a significant difference in
total column HCHO. In all cases, PSI measured substantially more C(HCHO) than
obtained from integrating the altitude profiles measured from the DC-8
overflights.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability">

      <p id="d1e4832">OMI Formaldehyde HCHO Version 03 data are available from:
<uri>https://avdc.gsfc.nasa.gov/index.php?site=1113974256&amp;id=81</uri> (last
access: 31 July 2018); OMI Nitrogen Dioxide <inline-formula><mml:math id="M283" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> Version 03 data are
available from:
<uri>https://avdc.gsfc.nasa.gov/index.php?site=666843934&amp;id=13</uri> (last access:
31 July 2018); Pandora KORUS-AQ <inline-formula><mml:math id="M284" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and HCHO data are available
from: <uri>https://avdc.gsfc.nasa.gov/pub/DSCOVR/Pandora/DATA/KORUS-AQ/</uri>
(last access: 31 July 2018). The OMI data were prepared by the Goddard Space
Flight Center OMI processing team located in Greenbelt, Maryland, USA. The
Pandora KORUS-AQ data were prepared by Elena Spinei and by Jay Herman.</p>
  </notes><?xmltex \hack{\clearpage}?><app-group>

<?pagebreak page4600?><app id="App1.Ch1.S1">
  <title/>
      <p id="d1e4874">Figure A1 illustrates the deseasonalization of the time series in Fig. 6. Panel (a) reproduces the solid black curve in Fig. 6a or c in the inset.
Panel (b) reproduces the solid curve in Fig. 6b and is magnified in
the inset. The seasonal dependence in the panel (a) inset is almost
non-existent in the panel (b) inset.</p>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.F1"><caption><p id="d1e4879">An illustration of the deseasonalization <bold>(b)</bold> of the monthly
running average of <inline-formula><mml:math id="M285" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> for the Gwangju site <bold>(a)</bold> shown in
Fig. 6. The insets are magnifications of the main plots.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://amt.copernicus.org/articles/11/4583/2018/amt-11-4583-2018-f22.png"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>
  </app-group><notes notes-type="authorcontribution">

      <p id="d1e4913">JH wrote most of the paper and performed the analysis and
comparisons with the DC-8 aircraft measurements.
ES derived the formaldehyde altitude profiles suitable for
comparison with Pandora data.
AF obtained the HCHO profile data from the DC-8 CAMS instrument.
JhK provided support for the installation of Pandora instruments in
Korea.
JaK provided support for the Pandora located in Busan.
WK provided support in installing the Pandoras and analyzing the
raw data.
AC provided calibration and data analysis support.
NA provided Pandora setup in Korea and provided the
maintenance of calibration.
MSR provided the 4STAR <inline-formula><mml:math id="M286" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> data from the DC-8
flights and the comparison with Pandora.</p>
  </notes><notes notes-type="competinginterests">

      <p id="d1e4930">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e4937">The author would like to thank the Pandora project for support in completing
this study as well as financial support from the KORUS-AQ project
NNH15ZDA001N-KORUS. Jae Kim and Jhoon Kim are supported by Korea
Ministry of Environment as Public Technology Program based on Environmental
Policy (2017000160001).<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: Michel Van Roozendael<?xmltex \hack{\newline}?>
Reviewed by: two anonymous referees</p></ack><ref-list>
    <title>References</title>

      <ref id="bib1.bib1"><label>1</label><mixed-citation>Bernhard, G., Booth, C. R., and Ehramjian, J. C.: Version 2 data of the
National Science Foundation's ultraviolet radiation monitoring network: South
Pole, J. Geophys. Res.-Atmos., 109, D21207, <ext-link xlink:href="https://doi.org/10.1029/2004JD004937" ext-link-type="DOI">10.1029/2004JD004937</ext-link>, 2004.</mixed-citation></ref>
      <ref id="bib1.bib2"><label>2</label><mixed-citation>Cede, A.: Manual for Blick Software Suite1.3 Version 7, 20 April 2017,
available at:
<uri>https://avdc.gsfc.nasa.gov/pub/DSCOVR/Pandora/Documents/BlickSoftwareSuite_Manual_v7.pdf</uri>
(last access: 31 July 2018), 2017.</mixed-citation></ref>
      <ref id="bib1.bib3"><label>3</label><mixed-citation>Chimot, J., Vlemmix, T., Veefkind, J. P., de Haan, J. F., and Levelt, P. F.:
Impact of aerosols on the OMI tropospheric <inline-formula><mml:math id="M287" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> retrievals over
industrialized regions: how accurate is the aerosol correction of cloud-free
scenes via a simple cloud model?, Atmos. Meas. Tech., 9, 359–382,
<ext-link xlink:href="https://doi.org/10.5194/amt-9-359-2016" ext-link-type="DOI">10.5194/amt-9-359-2016</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bib4"><label>4</label><mixed-citation>Cleveland, W. S.: LOWESS: A program for smoothing scatterplots by robust
locally weighted regression, Am. Stat., 35, 2683591, <ext-link xlink:href="https://doi.org/10.2307/2683591" ext-link-type="DOI">10.2307/2683591</ext-link>,
1981.</mixed-citation></ref>
      <ref id="bib1.bib5"><label>5</label><mixed-citation>Dufour, G., Wittrock, F., Camredon, M., Beekmann, M., Richter, A., Aumont,
B., and Burrows, J. P.: SCIAMACHY formaldehyde observations: constraint for
isoprene emission estimates over Europe?, Atmos. Chem. Phys., 9, 1647–1664,
<ext-link xlink:href="https://doi.org/10.5194/acp-9-1647-2009" ext-link-type="DOI">10.5194/acp-9-1647-2009</ext-link>, 2009.</mixed-citation></ref>
      <ref id="bib1.bib6"><label>6</label><mixed-citation>Dunagan, S. E., Johnson, R., Zavaleta, J., Russell, P. B., Schmid, B., Flynn,
C., Redemann, J., Shinozuka, Y., Livingston, J., and Segal-Rosenhaimer, M.:
4STAR spectrometer for sky-scanning Sun-tracking atmospheric research:
Instrument technology, Remote Sens., 5, 3872–3895, <ext-link xlink:href="https://doi.org/10.3390/rs5083872" ext-link-type="DOI">10.3390/rs5083872</ext-link>,
2013.</mixed-citation></ref>
      <ref id="bib1.bib7"><label>7</label><mixed-citation>Duncan, B. N., Lamsal, L. N., Thompson, A. M., Yoshida, Y., Lu, Z., Streets,
D. G., Hurwitz, M. M., and Pickering, K. E.: A space-based, high-resolution
view of notable changes in urban <inline-formula><mml:math id="M288" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> pollution around the
world (2005–2014), J. Geophys. Res. Atmos., 121, 976–996,
<ext-link xlink:href="https://doi.org/10.1002/2015JD024121" ext-link-type="DOI">10.1002/2015JD024121</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bib8"><label>8</label><mixed-citation>Fried, A., Walega, J. G., Olson, J. R., Crawford, J. H., Chen, G., Weibring,
P., Richter, D., Roller, C., Tittel, F. K., Heikes, B. G., Snow, J. A., Shen,
H., O'Sullivan, D. W., Porter, M., Fuelberg, H., Halland, J., and Millet, D.
B.: Formaldehyde over North America and the North Atlantic during the summer
2004 INTEX campaign: Methods, observed distributions, and measurement-model
comparisons, J. Geophys. Res., 113, D10302, <ext-link xlink:href="https://doi.org/10.1029/2007JD009185" ext-link-type="DOI">10.1029/2007JD009185</ext-link>, 2008.</mixed-citation></ref>
      <ref id="bib1.bib9"><label>9</label><mixed-citation>
Friedfeld,S., Fraser, M., Ensor, K., Tribble, S., Rehle, D., Leleux, D., and
Tittel, F.: Statistical analysis of primary and secondary atmospheric
formaldehyde, Atmos. Environ., 36, 4767–4775, 2002.</mixed-citation></ref>
      <ref id="bib1.bib10"><label>10</label><mixed-citation>Garcia, A. R., Volkamer, R., Molina, L. T., Molina, M. J., Samuelson, J.,
Mellqvist, J., Galle, B., Herndon, S. C., and Kolb, C. E.: Separation of
emitted and photochemical formaldehyde in Mexico City using a statistical
analysis and a new pair of gas-phase tracers, Atmos. Chem. Phys., 6,
4545–4557, <ext-link xlink:href="https://doi.org/10.5194/acp-6-4545-2006" ext-link-type="DOI">10.5194/acp-6-4545-2006</ext-link>, 2006.</mixed-citation></ref>
      <ref id="bib1.bib11"><label>11</label><mixed-citation>Goldberg, D. L., Lamsal, L. N., Loughner, C. P., Swartz, W. H., Lu, Z., and
Streets, D. G.: A high-resolution and observationally constrained OMI
<inline-formula><mml:math id="M289" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> satellite retrieval, Atmos. Chem. Phys., 17, 11403–11421,
<ext-link xlink:href="https://doi.org/10.5194/acp-17-11403-2017" ext-link-type="DOI">10.5194/acp-17-11403-2017</ext-link>, 2017.</mixed-citation></ref>
      <ref id="bib1.bib12"><label>12</label><mixed-citation>Herman, J., Cede, A., Spinei, E., Mount, G., Tzortziou, M., and Abuhassan,
N.: <inline-formula><mml:math id="M290" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> Column Amounts from Ground-based Pandora and MFDOAS
Spectrometers using the Direct-Sun DOAS Technique: Intercomparisons and
Application to OMI Validation, J. Geophys. Res., 114, D13307,
<ext-link xlink:href="https://doi.org/10.1029/2009JD011848" ext-link-type="DOI">10.1029/2009JD011848</ext-link>, 2009.</mixed-citation></ref>
      <ref id="bib1.bib13"><label>13</label><mixed-citation>Herman, J., Evans, R., Cede, A., Abuhassan, N., Petropavlovskikh, I., and
McConville, G.: Comparison of ozone retrievals from the Pandora spectrometer
system and Dobson spectrophotometer in Boulder, Colorado, Atmos. Meas. Tech.,
8, 3407–3418, <ext-link xlink:href="https://doi.org/10.5194/amt-8-3407-2015" ext-link-type="DOI">10.5194/amt-8-3407-2015</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bib14"><label>14</label><mixed-citation>Hottle, J. R., Huisman, A. J., DiGangi, J. P., Kammrath, A., Galloway, M. M.,
Coens, K. L., and Keutsch, F. N.: A Laser Induced Fluorescence-Based
Instrument for In-Situ Measurements of Atmospheric Formaldehyde, Environ.
Sci. Technol., 43, 790–795, <ext-link xlink:href="https://doi.org/10.1021/es801621f" ext-link-type="DOI">10.1021/es801621f</ext-link>, 2009.</mixed-citation></ref>
      <ref id="bib1.bib15"><label>15</label><mixed-citation>Jung, J., Lee, J., Kim, B., and Oh, S.: Seasonal variations in the
<inline-formula><mml:math id="M291" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> artifact from chemiluminescence measurements with a molybdenum
converter at a suburban site in Korea (downwind of the Asian continental
outflow) during 2015–2016, Atmos. Environ., 165, 290–300, 2017.</mixed-citation></ref>
      <?pagebreak page4602?><ref id="bib1.bib16"><label>16</label><mixed-citation>Kanaya, Y., Irie, H., Takashima, H., Iwabuchi, H., Akimoto, H., Sudo, K., Gu,
M., Chong, J., Kim, Y. J., Lee, H., Li, A., Si, F., Xu, J., Xie, P.-H., Liu,
W.-Q., Dzhola, A., Postylyakov, O., Ivanov, V., Grechko, E., Terpugova, S.,
and Panchenko, M.: Long-term MAX-DOAS network observations of <inline-formula><mml:math id="M292" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
in Russia and Asia (MADRAS) during the period 2007–2012: instrumentation,
elucidation of climatology, and comparisons with OMI satellite observations
and global model simulations, Atmos. Chem. Phys., 14, 7909–7927,
<ext-link xlink:href="https://doi.org/10.5194/acp-14-7909-2014" ext-link-type="DOI">10.5194/acp-14-7909-2014</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bib17"><label>17</label><mixed-citation>Kim, D., Lee, H., Hong, H., Choi, W., Lee, Y. G., and Park, J.: Estimation of
Surface <inline-formula><mml:math id="M293" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> Volume Mixing Ratio in Four Metropolitan Cities in
Korea Using Multiple Regression Models with OMI and AIRS Data, Remote Sens.,
9, 627, <ext-link xlink:href="https://doi.org/10.3390/rs9060627" ext-link-type="DOI">10.3390/rs9060627</ext-link>, 2017.</mixed-citation></ref>
      <ref id="bib1.bib18"><label>18</label><mixed-citation>Kim, N. K., Kim, Y. P., Morino, Y., Kurokawa, J., and Ohara, T.: Verification
of <inline-formula><mml:math id="M294" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emission inventory over South Korea using sectoral
activity data and satellite observation of <inline-formula><mml:math id="M295" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> vertical column
densities, Atmos. Environ., 77, 496–508, 2013.</mixed-citation></ref>
      <ref id="bib1.bib19"><label>19</label><mixed-citation>Kim, S. Y. and Song, I.: National-scale exposure prediction for long-term
concentrations of particulate matter and nitrogen dioxide in South Korea,
Environ. Pollut., 226, 21–29, <ext-link xlink:href="https://doi.org/10.1016/j.envpol.2017.03.056" ext-link-type="DOI">10.1016/j.envpol.2017.03.056</ext-link>, 2017.</mixed-citation></ref>
      <ref id="bib1.bib20"><label>20</label><mixed-citation>
Kraft, M., Eikmann, T., Kappos, A., Künzli, N., Rapp, R., Schneider, K.,
Seitz, H., Voss, J.-U., and Wichmann, H.-E.: The German view: Effects of
nitrogen dioxide on human health – derivation of health-related short-term
and long-term values, Int. J. Hyg. Envir. Heal., 208, 305–318, 2005.</mixed-citation></ref>
      <ref id="bib1.bib21"><label>21</label><mixed-citation>Kramer, L., Leigh, R. J., Remedios, J. J., and Monks, P. S.: Comparison of
OMI and Ground-Based in situ and MAXDOAS Measurements of Tropospheric
Nitrogen Dioxide in An Urban Area, J. Geophys. Res., 113, D16S39,
<ext-link xlink:href="https://doi.org/10.1029/2007JD009168" ext-link-type="DOI">10.1029/2007JD009168</ext-link>, 2008.</mixed-citation></ref>
      <ref id="bib1.bib22"><label>22</label><mixed-citation>Latza, U., Gerdes, S., and Baur, X.: Effects of nitrogen dioxide on human
health: Systematic review of experimental and epidemiological studies
conducted between 2002 and 2006, Int. J. Hyg. Envir. Heal., 212, 271–287,
<ext-link xlink:href="https://doi.org/10.1016/j.ijheh.2008.06.003" ext-link-type="DOI">10.1016/j.ijheh.2008.06.003</ext-link>, 2009.</mixed-citation></ref>
      <ref id="bib1.bib23"><label>23</label><mixed-citation>
Lee, G., Oh, H.-R., Ho, C.-H., Kim, J., Song, C.-K., Chang, L.-S., Lee,
J.-B., and Lee, S.: Airborne Measurements of High Pollutant Concentration
Events in the Free Troposphere over the West Coast of South Korea between
1997 and 2011, Aerosol Air Qual. Res., 16, 1118–1130, 2016.</mixed-citation></ref>
      <ref id="bib1.bib24"><label>24</label><mixed-citation>Lee, H.-J., Kim, S.-W., Brioude, J., Cooper, O. R., Frost, G. J., Kim, C.-H.,
Park, R. J., Trainer, M., and Woo, J.-H.: Transport of <inline-formula><mml:math id="M296" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
in East Asia identified by satellite and in situ measurements and Lagrangian
particle dispersion model simulations, J. Geophys. Res., 119, 2574–2596,
<ext-link xlink:href="https://doi.org/10.1002/2013JD021185" ext-link-type="DOI">10.1002/2013JD021185</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bib25"><label>25</label><mixed-citation>Lei, W., Zavala, M., de Foy, B., Volkamer, R., Molina, M. J., and Molina, L.
T.: Impact of primary formaldehyde on air pollution in the Mexico City
Metropolitan Area, Atmos. Chem. Phys., 9, 2607–2618,
<ext-link xlink:href="https://doi.org/10.5194/acp-9-2607-2009" ext-link-type="DOI">10.5194/acp-9-2607-2009</ext-link>, 2009.</mixed-citation></ref>
      <ref id="bib1.bib26"><label>26</label><mixed-citation>Liteplo, R. G., Beauchamp, R., Meek, M. E., and Chénier, R.:
Formaldehyde, International Programme on Chemical Safety, Geneva,
Switzerland, 2002, Concise International Chemical Assessment Document 40,
available at: <uri>http://www.who.int/ipcs/publications/cicad/en/cicad40.pdf</uri>
(last access: 31 July 2018), 2010.</mixed-citation></ref>
      <ref id="bib1.bib27"><label>27</label><mixed-citation>Luecken, D. J., Hutzell, W. T., Strum, M. L., and Pouliot, G. A.: Regional
sources of atmospheric formaldehyde and acetaldehyde, and implications for
atmospheric modeling, Atmos. Environ., 47, 477–490,
<ext-link xlink:href="https://doi.org/10.1016/j.atmosenv.2011.10.005" ext-link-type="DOI">10.1016/j.atmosenv.2011.10.005</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bib28"><label>28</label><mixed-citation>Meller, R. and Moortgat, G. K.: Temperature dependence of the absorption
cross sections of formaldehyde between 223 and 323 k in the wavelength range
225–375 nm, J. Geophys. Res.-Atmos., 105, 7089–7101,
<ext-link xlink:href="https://doi.org/10.1029/1999JD901074" ext-link-type="DOI">10.1029/1999JD901074</ext-link>, 2000.</mixed-citation></ref>
      <ref id="bib1.bib29"><label>29</label><mixed-citation>Park, J., Lee, H., Kim, J., Herman, J., Kim, W., Hong, H., Choi, W., Yang,
J., and Kim, D.: HCHO column density retrieval using Pandora measurements in
Seoul, Korea: Temporal characteristics and comparison with OMI measurement,
Remote Sens., 10, 173, <ext-link xlink:href="https://doi.org/10.3390/rs10020173" ext-link-type="DOI">10.3390/rs10020173</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bib30"><label>30</label><mixed-citation>
Platt, U.: Differential optical absorption spectroscopy (DOAS), Air
monitoring by Spectroscopic Techiques, edited by: Sigrist, M., John Wiley
&amp; Sons, Inc., 27–84, 1994.</mixed-citation></ref>
      <ref id="bib1.bib31"><label>31</label><mixed-citation>Platt, U., Perner, D., and Pätz, H. W.: Simultaneous measurements of
atmospheric <inline-formula><mml:math id="M297" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M298" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M299" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> by differential
optical absorption, J. Geophys. Res., 84, 6329–6335, 1979.</mixed-citation></ref>
      <ref id="bib1.bib32"><label>32</label><mixed-citation>Richter, D., Weibring, P., Walega, J. G., Fried, A., Spuler, S. M., and
Taubman, M. S.: Compact highly sensitive multi-species airborne mid-IR
spectrometer, Appl. Phys. B, 119, 119–131, <ext-link xlink:href="https://doi.org/10.1007/s00340-015-6038-8" ext-link-type="DOI">10.1007/s00340-015-6038-8</ext-link>,
2015.</mixed-citation></ref>
      <ref id="bib1.bib33"><label>33</label><mixed-citation>Segal-Rosenheimer, M., Russell, P. B., Schmid, B., Redemann, J., Livingston,
J. M., Flynn, C. J., Johnson, R. R., Dunagan, S. E., Shinozuka, Y., Herman,
J., Cede, A., Abuhassan, N., Comstock, J. M., Hubbe, J. M., Zelenyuk, A., and
Wilson, J.: Tracking elevated pollution layers with a newly developed
hyperspectral Sun/Sky spectrometer(4STAR): Results from the TCAP 2012 and
2013 campaigns, J. Geophys. Res.-Atmos., 119, 2611–2628,
<ext-link xlink:href="https://doi.org/10.1002/2013JD020884" ext-link-type="DOI">10.1002/2013JD020884</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bib34"><label>34</label><mixed-citation>
Segal-Rozenhaimer, M., Goldberg, D. L., Kacenelbogen, M., LeBlanc, S., Flynn,
C., Redemann, J., Herman, J., Cede, A., Abuhassan, N., and Lamsal, L. N.:
Assessing how aerosols effect OMI NO2 retrievals during KORUS-AQ, AOGS
2–8 June 2018, Honolulu, HI, USA, 2018.</mixed-citation></ref>
      <ref id="bib1.bib35"><label>35</label><mixed-citation>Shinozuka, Y., Johnson, R. R., Flynn, C. J., Russell, P. B., Schmid, B.,
Redemann, J., Dunagan, S. E., Kluzek, C. D., Hubbe, J. M., Segal-Rosenheimer,
M., Livingston, J. M., Eck, T. F., Wagener, R., Gregory, L., Chand, D., Berg,
L. K., Rogers, R. R., Ferrare, R. A., Hair, J. W., Hostetler, C. A., and
Burton, S. P.: Hyperspectral aerosol optical depths from TCAP flights, J.
Geophys. Res.-Atmos., 118, 12180–12194, <ext-link xlink:href="https://doi.org/10.1002/2013JD020596" ext-link-type="DOI">10.1002/2013JD020596</ext-link>, 2013.</mixed-citation></ref>
      <ref id="bib1.bib36"><label>36</label><mixed-citation>Spinei, E., Whitehill, A., Fried, A., Tiefengraber, M., Knepp, T. N.,
Herndon, S., Herman, J. R., Müller, M., Abuhassan, N., Cede, A.,
Weibring, P., Richter, D., Walega, J., Crawford, J., Szykman, J., Valin, L.,
Williams, D. J., Long, R., Swap, R. J., Lee, Y., Nowak, N., and Poche, B.:
The First Evaluation of Formaldehyde Column Observations by Pandora
Spectrometers during the KORUS-AQ Field Study, Atmos. Meas. Tech. Discuss.,
<ext-link xlink:href="https://doi.org/10.5194/amt-2018-57" ext-link-type="DOI">10.5194/amt-2018-57</ext-link>, in review, 2018.</mixed-citation></ref>
      <ref id="bib1.bib37"><label>37</label><mixed-citation>Vandaele, A. C., Hermans, C., Simon, P. C., Carleer, M., Colin, R., Fally,
S., Mérienne, M. F., Jenouvrier, A., and Coquart, B.: Measurements of the
<inline-formula><mml:math id="M300" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> absorption cross-section from 42,000 cm<inline-formula><mml:math id="M301" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1 to 10,000 cm<inline-formula><mml:math id="M302" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1
(238–1000 nm) at 220 K and 294 K, J. Quant. Spectrosc. Ra., 59, 171–184,
<ext-link xlink:href="https://doi.org/10.1016/S0022-4073(97)00168-4" ext-link-type="DOI">10.1016/S0022-4073(97)00168-4</ext-link>, 1998.</mixed-citation></ref>
      <ref id="bib1.bib38"><label>38</label><mixed-citation>Walters, W., Goodwin, S., and Michalski, G.: The Nitrogen Stable Isotope
Composition (<inline-formula><mml:math id="M303" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>15N) of Vehicle Emitted <inline-formula><mml:math id="M304" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, Environ.
Sci. Technol., 49, 2278–2285, <ext-link xlink:href="https://doi.org/10.1021/es505580v" ext-link-type="DOI">10.1021/es505580v</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bib39"><label>39</label><mixed-citation>Zhang, H., Li, J., Ying, Q., Guven, B. B., and Olaguer, E. P.: Source
apportionment of formaldehyde during TexAQS 2006 using a source-oriented
chemical transport model, J. Geophys. Res., 118, 1525–1535,
<ext-link xlink:href="https://doi.org/10.1002/jgrd.50197" ext-link-type="DOI">10.1002/jgrd.50197</ext-link>, 2013.</mixed-citation></ref>
      <?pagebreak page4603?><ref id="bib1.bib40"><label>40</label><mixed-citation>Zhu, L., Jacob, D. J., Keutsch, F. N., Mickley, L. J., Scheffe, R., Strum,
M., Abad, G. G., Chance, K., Yang, K., Rappenglück, B., Millet, D. B.,
Baasandorj, M., Jaeglé, L., and Shah, V.: Formaldehyde (HCHO) As a
Hazardous Air Pollutant: Mapping Surface Air Concentrations from Satellite
and Inferring Cancer Risks in the United States, Environ. Sci. Technol., 51,
5650–5657, <ext-link xlink:href="https://doi.org/10.1021/acs.est.7b01356" ext-link-type="DOI">10.1021/acs.est.7b01356</ext-link>, 2017.</mixed-citation></ref>

  </ref-list></back>
    <!--<article-title-html>NO<sub>2</sub> and HCHO measurements in Korea from 2012 to 2016 from Pandora spectrometer instruments compared with OMI retrievals and with aircraft measurements during the KORUS-AQ campaign</article-title-html>
<abstract-html><p>Nine Pandora
spectrometer instruments (PSI) were installed at eight sites in
South Korea as part of the KORUS-AQ (Korea U.S.-Air Quality) field study
integrating information from ground, aircraft, and satellite measurements
for validation of remote sensing air-quality studies. The PSI made
direct-sun measurements of total vertical column NO<sub>2</sub>, C(NO<sub>2</sub>), with
high precision (0.05&thinsp;DU, where 1&thinsp;DU&thinsp; = 2.69×10<sup>16</sup>&thinsp;molecules&thinsp;cm<sup>−2</sup>)
and accuracy (0.1&thinsp;DU) that were retrieved using spectral fitting techniques.
Retrieval of formaldehyde C(HCHO) total column amounts were also obtained at
five sites using the recently improved PSI optics. The C(HCHO) retrievals have
high precision, but possibly lower accuracy than for NO<sub>2</sub> because of
uncertainty about the optimum spectral window for all ground-based and
satellite instruments. PSI direct-sun retrieved values for C(NO<sub>2</sub>) and
C(HCHO) are always significantly larger than OMI (AURA satellite Ozone
Monitoring Instrument) retrieved C(NO<sub>2</sub>) and C(HCHO) for the OMI
overpass local times (KST = 13.5±0.5&thinsp;h). In urban areas, PSI
C(NO<sub>2</sub>) 30-day running averages are at least a factor of two larger than
OMI averages. Similar differences are seen for C(HCHO) in Seoul and nearby
surrounding areas. Late afternoon values of C(HCHO) measured by PSI are even
larger, implying that OMI early afternoon measurements underestimate the
effect of poor air quality on human health. The primary cause of OMI
underestimates is the large OMI field of view (FOV) that includes regions
containing low values of pollutants. In relatively clean areas, PSI and OMI
are more closely in agreement. C(HCHO) amounts were obtained for five sites,
Yonsei University in Seoul, Olympic Park, Taehwa Mountain, Amnyeondo, and Yeoju.
Of these, the largest amounts of C(HCHO) were observed at Olympic Park and
Taehwa Mountain, surrounded by significant amounts of vegetation.
Comparisons of PSI C(HCHO) results were made with the Compact Atmospheric
Multispecies Spectrometer CAMS during overflights on the DC-8 aircraft for
Taehwa Mountain and Olympic Park. In all cases, PSI measured substantially more
C(HCHO) than obtained from integrating the CAMS altitude profiles. PSI
C(HCHO) at Yonsei University in Seoul frequently reached 0.6&thinsp;DU and
occasionally exceeded 1.5&thinsp;DU. The semi-rural site, Taehwa Mountain, frequently
reached 0.9&thinsp;DU and occasionally exceeded 1.5&thinsp;DU. Even at the cleanest site,
Amnyeondo, C(HCHO) occasionally exceeded 1&thinsp;DU.</p></abstract-html>
<ref-html id="bib1.bib1"><label>1</label><mixed-citation>
Bernhard, G., Booth, C. R., and Ehramjian, J. C.: Version 2 data of the
National Science Foundation's ultraviolet radiation monitoring network: South
Pole, J. Geophys. Res.-Atmos., 109, D21207, <a href="https://doi.org/10.1029/2004JD004937" target="_blank">https://doi.org/10.1029/2004JD004937</a>, 2004.
</mixed-citation></ref-html>
<ref-html id="bib1.bib2"><label>2</label><mixed-citation>
Cede, A.: Manual for Blick Software Suite1.3 Version 7, 20 April 2017,
available at:
<a href="https://avdc.gsfc.nasa.gov/pub/DSCOVR/Pandora/Documents/BlickSoftwareSuite_Manual_v7.pdf" target="_blank">https://avdc.gsfc.nasa.gov/pub/DSCOVR/Pandora/Documents/BlickSoftwareSuite_Manual_v7.pdf</a>
(last access: 31 July 2018), 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib3"><label>3</label><mixed-citation>
Chimot, J., Vlemmix, T., Veefkind, J. P., de Haan, J. F., and Levelt, P. F.:
Impact of aerosols on the OMI tropospheric NO<sub>2</sub> retrievals over
industrialized regions: how accurate is the aerosol correction of cloud-free
scenes via a simple cloud model?, Atmos. Meas. Tech., 9, 359–382,
<a href="https://doi.org/10.5194/amt-9-359-2016" target="_blank">https://doi.org/10.5194/amt-9-359-2016</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib4"><label>4</label><mixed-citation>
Cleveland, W. S.: LOWESS: A program for smoothing scatterplots by robust
locally weighted regression, Am. Stat., 35, 2683591, <a href="https://doi.org/10.2307/2683591" target="_blank">https://doi.org/10.2307/2683591</a>,
1981.
</mixed-citation></ref-html>
<ref-html id="bib1.bib5"><label>5</label><mixed-citation>
Dufour, G., Wittrock, F., Camredon, M., Beekmann, M., Richter, A., Aumont,
B., and Burrows, J. P.: SCIAMACHY formaldehyde observations: constraint for
isoprene emission estimates over Europe?, Atmos. Chem. Phys., 9, 1647–1664,
<a href="https://doi.org/10.5194/acp-9-1647-2009" target="_blank">https://doi.org/10.5194/acp-9-1647-2009</a>, 2009.
</mixed-citation></ref-html>
<ref-html id="bib1.bib6"><label>6</label><mixed-citation>
Dunagan, S. E., Johnson, R., Zavaleta, J., Russell, P. B., Schmid, B., Flynn,
C., Redemann, J., Shinozuka, Y., Livingston, J., and Segal-Rosenhaimer, M.:
4STAR spectrometer for sky-scanning Sun-tracking atmospheric research:
Instrument technology, Remote Sens., 5, 3872–3895, <a href="https://doi.org/10.3390/rs5083872" target="_blank">https://doi.org/10.3390/rs5083872</a>,
2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib7"><label>7</label><mixed-citation>
Duncan, B. N., Lamsal, L. N., Thompson, A. M., Yoshida, Y., Lu, Z., Streets,
D. G., Hurwitz, M. M., and Pickering, K. E.: A space-based, high-resolution
view of notable changes in urban NO<sub><i>x</i></sub> pollution around the
world (2005–2014), J. Geophys. Res. Atmos., 121, 976–996,
<a href="https://doi.org/10.1002/2015JD024121" target="_blank">https://doi.org/10.1002/2015JD024121</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib8"><label>8</label><mixed-citation>
Fried, A., Walega, J. G., Olson, J. R., Crawford, J. H., Chen, G., Weibring,
P., Richter, D., Roller, C., Tittel, F. K., Heikes, B. G., Snow, J. A., Shen,
H., O'Sullivan, D. W., Porter, M., Fuelberg, H., Halland, J., and Millet, D.
B.: Formaldehyde over North America and the North Atlantic during the summer
2004 INTEX campaign: Methods, observed distributions, and measurement-model
comparisons, J. Geophys. Res., 113, D10302, <a href="https://doi.org/10.1029/2007JD009185" target="_blank">https://doi.org/10.1029/2007JD009185</a>, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib9"><label>9</label><mixed-citation>
Friedfeld,S., Fraser, M., Ensor, K., Tribble, S., Rehle, D., Leleux, D., and
Tittel, F.: Statistical analysis of primary and secondary atmospheric
formaldehyde, Atmos. Environ., 36, 4767–4775, 2002.
</mixed-citation></ref-html>
<ref-html id="bib1.bib10"><label>10</label><mixed-citation>
Garcia, A. R., Volkamer, R., Molina, L. T., Molina, M. J., Samuelson, J.,
Mellqvist, J., Galle, B., Herndon, S. C., and Kolb, C. E.: Separation of
emitted and photochemical formaldehyde in Mexico City using a statistical
analysis and a new pair of gas-phase tracers, Atmos. Chem. Phys., 6,
4545–4557, <a href="https://doi.org/10.5194/acp-6-4545-2006" target="_blank">https://doi.org/10.5194/acp-6-4545-2006</a>, 2006.
</mixed-citation></ref-html>
<ref-html id="bib1.bib11"><label>11</label><mixed-citation>
Goldberg, D. L., Lamsal, L. N., Loughner, C. P., Swartz, W. H., Lu, Z., and
Streets, D. G.: A high-resolution and observationally constrained OMI
NO<sub>2</sub> satellite retrieval, Atmos. Chem. Phys., 17, 11403–11421,
<a href="https://doi.org/10.5194/acp-17-11403-2017" target="_blank">https://doi.org/10.5194/acp-17-11403-2017</a>, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib12"><label>12</label><mixed-citation>
Herman, J., Cede, A., Spinei, E., Mount, G., Tzortziou, M., and Abuhassan,
N.: NO<sub>2</sub> Column Amounts from Ground-based Pandora and MFDOAS
Spectrometers using the Direct-Sun DOAS Technique: Intercomparisons and
Application to OMI Validation, J. Geophys. Res., 114, D13307,
<a href="https://doi.org/10.1029/2009JD011848" target="_blank">https://doi.org/10.1029/2009JD011848</a>, 2009.
</mixed-citation></ref-html>
<ref-html id="bib1.bib13"><label>13</label><mixed-citation>
Herman, J., Evans, R., Cede, A., Abuhassan, N., Petropavlovskikh, I., and
McConville, G.: Comparison of ozone retrievals from the Pandora spectrometer
system and Dobson spectrophotometer in Boulder, Colorado, Atmos. Meas. Tech.,
8, 3407–3418, <a href="https://doi.org/10.5194/amt-8-3407-2015" target="_blank">https://doi.org/10.5194/amt-8-3407-2015</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib14"><label>14</label><mixed-citation>
Hottle, J. R., Huisman, A. J., DiGangi, J. P., Kammrath, A., Galloway, M. M.,
Coens, K. L., and Keutsch, F. N.: A Laser Induced Fluorescence-Based
Instrument for In-Situ Measurements of Atmospheric Formaldehyde, Environ.
Sci. Technol., 43, 790–795, <a href="https://doi.org/10.1021/es801621f" target="_blank">https://doi.org/10.1021/es801621f</a>, 2009.
</mixed-citation></ref-html>
<ref-html id="bib1.bib15"><label>15</label><mixed-citation>
Jung, J., Lee, J., Kim, B., and Oh, S.: Seasonal variations in the
NO<sub>2</sub> artifact from chemiluminescence measurements with a molybdenum
converter at a suburban site in Korea (downwind of the Asian continental
outflow) during 2015–2016, Atmos. Environ., 165, 290–300, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib16"><label>16</label><mixed-citation>
Kanaya, Y., Irie, H., Takashima, H., Iwabuchi, H., Akimoto, H., Sudo, K., Gu,
M., Chong, J., Kim, Y. J., Lee, H., Li, A., Si, F., Xu, J., Xie, P.-H., Liu,
W.-Q., Dzhola, A., Postylyakov, O., Ivanov, V., Grechko, E., Terpugova, S.,
and Panchenko, M.: Long-term MAX-DOAS network observations of NO<sub>2</sub>
in Russia and Asia (MADRAS) during the period 2007–2012: instrumentation,
elucidation of climatology, and comparisons with OMI satellite observations
and global model simulations, Atmos. Chem. Phys., 14, 7909–7927,
<a href="https://doi.org/10.5194/acp-14-7909-2014" target="_blank">https://doi.org/10.5194/acp-14-7909-2014</a>, 2014.
</mixed-citation></ref-html>
<ref-html id="bib1.bib17"><label>17</label><mixed-citation>
Kim, D., Lee, H., Hong, H., Choi, W., Lee, Y. G., and Park, J.: Estimation of
Surface NO<sub>2</sub> Volume Mixing Ratio in Four Metropolitan Cities in
Korea Using Multiple Regression Models with OMI and AIRS Data, Remote Sens.,
9, 627, <a href="https://doi.org/10.3390/rs9060627" target="_blank">https://doi.org/10.3390/rs9060627</a>, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib18"><label>18</label><mixed-citation>
Kim, N. K., Kim, Y. P., Morino, Y., Kurokawa, J., and Ohara, T.: Verification
of NO<sub><i>x</i></sub> emission inventory over South Korea using sectoral
activity data and satellite observation of NO<sub>2</sub> vertical column
densities, Atmos. Environ., 77, 496–508, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib19"><label>19</label><mixed-citation>
Kim, S. Y. and Song, I.: National-scale exposure prediction for long-term
concentrations of particulate matter and nitrogen dioxide in South Korea,
Environ. Pollut., 226, 21–29, <a href="https://doi.org/10.1016/j.envpol.2017.03.056" target="_blank">https://doi.org/10.1016/j.envpol.2017.03.056</a>, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib20"><label>20</label><mixed-citation>
Kraft, M., Eikmann, T., Kappos, A., Künzli, N., Rapp, R., Schneider, K.,
Seitz, H., Voss, J.-U., and Wichmann, H.-E.: The German view: Effects of
nitrogen dioxide on human health – derivation of health-related short-term
and long-term values, Int. J. Hyg. Envir. Heal., 208, 305–318, 2005.
</mixed-citation></ref-html>
<ref-html id="bib1.bib21"><label>21</label><mixed-citation>
Kramer, L., Leigh, R. J., Remedios, J. J., and Monks, P. S.: Comparison of
OMI and Ground-Based in situ and MAXDOAS Measurements of Tropospheric
Nitrogen Dioxide in An Urban Area, J. Geophys. Res., 113, D16S39,
<a href="https://doi.org/10.1029/2007JD009168" target="_blank">https://doi.org/10.1029/2007JD009168</a>, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib22"><label>22</label><mixed-citation>
Latza, U., Gerdes, S., and Baur, X.: Effects of nitrogen dioxide on human
health: Systematic review of experimental and epidemiological studies
conducted between 2002 and 2006, Int. J. Hyg. Envir. Heal., 212, 271–287,
<a href="https://doi.org/10.1016/j.ijheh.2008.06.003" target="_blank">https://doi.org/10.1016/j.ijheh.2008.06.003</a>, 2009.
</mixed-citation></ref-html>
<ref-html id="bib1.bib23"><label>23</label><mixed-citation>
Lee, G., Oh, H.-R., Ho, C.-H., Kim, J., Song, C.-K., Chang, L.-S., Lee,
J.-B., and Lee, S.: Airborne Measurements of High Pollutant Concentration
Events in the Free Troposphere over the West Coast of South Korea between
1997 and 2011, Aerosol Air Qual. Res., 16, 1118–1130, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib24"><label>24</label><mixed-citation>
Lee, H.-J., Kim, S.-W., Brioude, J., Cooper, O. R., Frost, G. J., Kim, C.-H.,
Park, R. J., Trainer, M., and Woo, J.-H.: Transport of NO<sub><i>x</i></sub>
in East Asia identified by satellite and in situ measurements and Lagrangian
particle dispersion model simulations, J. Geophys. Res., 119, 2574–2596,
<a href="https://doi.org/10.1002/2013JD021185" target="_blank">https://doi.org/10.1002/2013JD021185</a>, 2014.
</mixed-citation></ref-html>
<ref-html id="bib1.bib25"><label>25</label><mixed-citation>
Lei, W., Zavala, M., de Foy, B., Volkamer, R., Molina, M. J., and Molina, L.
T.: Impact of primary formaldehyde on air pollution in the Mexico City
Metropolitan Area, Atmos. Chem. Phys., 9, 2607–2618,
<a href="https://doi.org/10.5194/acp-9-2607-2009" target="_blank">https://doi.org/10.5194/acp-9-2607-2009</a>, 2009.
</mixed-citation></ref-html>
<ref-html id="bib1.bib26"><label>26</label><mixed-citation>
Liteplo, R. G., Beauchamp, R., Meek, M. E., and Chénier, R.:
Formaldehyde, International Programme on Chemical Safety, Geneva,
Switzerland, 2002, Concise International Chemical Assessment Document 40,
available at: <a href="http://www.who.int/ipcs/publications/cicad/en/cicad40.pdf" target="_blank">http://www.who.int/ipcs/publications/cicad/en/cicad40.pdf</a>
(last access: 31 July 2018), 2010.
</mixed-citation></ref-html>
<ref-html id="bib1.bib27"><label>27</label><mixed-citation>
Luecken, D. J., Hutzell, W. T., Strum, M. L., and Pouliot, G. A.: Regional
sources of atmospheric formaldehyde and acetaldehyde, and implications for
atmospheric modeling, Atmos. Environ., 47, 477–490,
<a href="https://doi.org/10.1016/j.atmosenv.2011.10.005" target="_blank">https://doi.org/10.1016/j.atmosenv.2011.10.005</a>, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib28"><label>28</label><mixed-citation>
Meller, R. and Moortgat, G. K.: Temperature dependence of the absorption
cross sections of formaldehyde between 223 and 323&thinsp;k in the wavelength range
225–375&thinsp;nm, J. Geophys. Res.-Atmos., 105, 7089–7101,
<a href="https://doi.org/10.1029/1999JD901074" target="_blank">https://doi.org/10.1029/1999JD901074</a>, 2000.
</mixed-citation></ref-html>
<ref-html id="bib1.bib29"><label>29</label><mixed-citation>
Park, J., Lee, H., Kim, J., Herman, J., Kim, W., Hong, H., Choi, W., Yang,
J., and Kim, D.: HCHO column density retrieval using Pandora measurements in
Seoul, Korea: Temporal characteristics and comparison with OMI measurement,
Remote Sens., 10, 173, <a href="https://doi.org/10.3390/rs10020173" target="_blank">https://doi.org/10.3390/rs10020173</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib30"><label>30</label><mixed-citation>
Platt, U.: Differential optical absorption spectroscopy (DOAS), Air
monitoring by Spectroscopic Techiques, edited by: Sigrist, M., John Wiley
&amp; Sons, Inc., 27–84, 1994.
</mixed-citation></ref-html>
<ref-html id="bib1.bib31"><label>31</label><mixed-citation>
Platt, U., Perner, D., and Pätz, H. W.: Simultaneous measurements of
atmospheric CH<sub>2</sub>, O<sub>3</sub> and NO<sub>2</sub> by differential
optical absorption, J. Geophys. Res., 84, 6329–6335, 1979.
</mixed-citation></ref-html>
<ref-html id="bib1.bib32"><label>32</label><mixed-citation>
Richter, D., Weibring, P., Walega, J. G., Fried, A., Spuler, S. M., and
Taubman, M. S.: Compact highly sensitive multi-species airborne mid-IR
spectrometer, Appl. Phys. B, 119, 119–131, <a href="https://doi.org/10.1007/s00340-015-6038-8" target="_blank">https://doi.org/10.1007/s00340-015-6038-8</a>,
2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib33"><label>33</label><mixed-citation>
Segal-Rosenheimer, M., Russell, P. B., Schmid, B., Redemann, J., Livingston,
J. M., Flynn, C. J., Johnson, R. R., Dunagan, S. E., Shinozuka, Y., Herman,
J., Cede, A., Abuhassan, N., Comstock, J. M., Hubbe, J. M., Zelenyuk, A., and
Wilson, J.: Tracking elevated pollution layers with a newly developed
hyperspectral Sun/Sky spectrometer(4STAR): Results from the TCAP 2012 and
2013 campaigns, J. Geophys. Res.-Atmos., 119, 2611–2628,
<a href="https://doi.org/10.1002/2013JD020884" target="_blank">https://doi.org/10.1002/2013JD020884</a>, 2014.
</mixed-citation></ref-html>
<ref-html id="bib1.bib34"><label>34</label><mixed-citation>
Segal-Rozenhaimer, M., Goldberg, D. L., Kacenelbogen, M., LeBlanc, S., Flynn,
C., Redemann, J., Herman, J., Cede, A., Abuhassan, N., and Lamsal, L. N.:
Assessing how aerosols effect OMI NO2 retrievals during KORUS-AQ, AOGS
2–8 June 2018, Honolulu, HI, USA, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib35"><label>35</label><mixed-citation>
Shinozuka, Y., Johnson, R. R., Flynn, C. J., Russell, P. B., Schmid, B.,
Redemann, J., Dunagan, S. E., Kluzek, C. D., Hubbe, J. M., Segal-Rosenheimer,
M., Livingston, J. M., Eck, T. F., Wagener, R., Gregory, L., Chand, D., Berg,
L. K., Rogers, R. R., Ferrare, R. A., Hair, J. W., Hostetler, C. A., and
Burton, S. P.: Hyperspectral aerosol optical depths from TCAP flights, J.
Geophys. Res.-Atmos., 118, 12180–12194, <a href="https://doi.org/10.1002/2013JD020596" target="_blank">https://doi.org/10.1002/2013JD020596</a>, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib36"><label>36</label><mixed-citation>
Spinei, E., Whitehill, A., Fried, A., Tiefengraber, M., Knepp, T. N.,
Herndon, S., Herman, J. R., Müller, M., Abuhassan, N., Cede, A.,
Weibring, P., Richter, D., Walega, J., Crawford, J., Szykman, J., Valin, L.,
Williams, D. J., Long, R., Swap, R. J., Lee, Y., Nowak, N., and Poche, B.:
The First Evaluation of Formaldehyde Column Observations by Pandora
Spectrometers during the KORUS-AQ Field Study, Atmos. Meas. Tech. Discuss.,
<a href="https://doi.org/10.5194/amt-2018-57" target="_blank">https://doi.org/10.5194/amt-2018-57</a>, in review, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib37"><label>37</label><mixed-citation>
Vandaele, A. C., Hermans, C., Simon, P. C., Carleer, M., Colin, R., Fally,
S., Mérienne, M. F., Jenouvrier, A., and Coquart, B.: Measurements of the
NO<sub>2</sub> absorption cross-section from 42,000&thinsp;cm−1 to 10,000&thinsp;cm−1
(238–1000&thinsp;nm) at 220&thinsp;K and 294&thinsp;K, J. Quant. Spectrosc. Ra., 59, 171–184,
<a href="https://doi.org/10.1016/S0022-4073(97)00168-4" target="_blank">https://doi.org/10.1016/S0022-4073(97)00168-4</a>, 1998.
</mixed-citation></ref-html>
<ref-html id="bib1.bib38"><label>38</label><mixed-citation>
Walters, W., Goodwin, S., and Michalski, G.: The Nitrogen Stable Isotope
Composition (<i>δ</i>15N) of Vehicle Emitted NO<sub><i>x</i></sub>, Environ.
Sci. Technol., 49, 2278–2285, <a href="https://doi.org/10.1021/es505580v" target="_blank">https://doi.org/10.1021/es505580v</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib39"><label>39</label><mixed-citation>
Zhang, H., Li, J., Ying, Q., Guven, B. B., and Olaguer, E. P.: Source
apportionment of formaldehyde during TexAQS 2006 using a source-oriented
chemical transport model, J. Geophys. Res., 118, 1525–1535,
<a href="https://doi.org/10.1002/jgrd.50197" target="_blank">https://doi.org/10.1002/jgrd.50197</a>, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib40"><label>40</label><mixed-citation>
Zhu, L., Jacob, D. J., Keutsch, F. N., Mickley, L. J., Scheffe, R., Strum,
M., Abad, G. G., Chance, K., Yang, K., Rappenglück, B., Millet, D. B.,
Baasandorj, M., Jaeglé, L., and Shah, V.: Formaldehyde (HCHO) As a
Hazardous Air Pollutant: Mapping Surface Air Concentrations from Satellite
and Inferring Cancer Risks in the United States, Environ. Sci. Technol., 51,
5650–5657, <a href="https://doi.org/10.1021/acs.est.7b01356" target="_blank">https://doi.org/10.1021/acs.est.7b01356</a>, 2017.
</mixed-citation></ref-html>--></article>
