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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</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/acp-19-8863-2019</article-id><title-group><article-title>Using satellite observations of tropospheric <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> columns to infer long-term trends in US <inline-formula><mml:math id="M2" 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> emissions: the importance of accounting for
the free tropospheric <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> background</article-title><alt-title>Using satellite observations of tropospheric <inline-formula><mml:math id="M4" 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> columns to infer long-term trends</alt-title>
      </title-group><?xmltex \runningtitle{Using satellite observations of tropospheric {$\chem{NO_{{2}}}$} columns to infer long-term trends}?><?xmltex \runningauthor{R. F. Silvern et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Silvern</surname><given-names>Rachel F.</given-names></name>
          <email>rsilvern@g.harvard.edu</email>
        <ext-link>https://orcid.org/0000-0002-6683-3238</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Jacob</surname><given-names>Daniel J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Mickley</surname><given-names>Loretta J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Sulprizio</surname><given-names>Melissa P.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff10">
          <name><surname>Travis</surname><given-names>Katherine R.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-1628-0353</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Marais</surname><given-names>Eloise A.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5 aff6">
          <name><surname>Cohen</surname><given-names>Ronald C.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6617-7691</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5 aff11">
          <name><surname>Laughner</surname><given-names>Joshua L.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8599-4555</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Choi</surname><given-names>Sungyeon</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7 aff8">
          <name><surname>Joiner</surname><given-names>Joanna</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4278-1020</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8 aff9">
          <name><surname>Lamsal</surname><given-names>Lok N.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Department of Earth and Planetary Sciences, Harvard University,
Cambridge, MA, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>School of Engineering and Applied Sciences, Harvard University,
Cambridge, MA, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Department of Civil and Environmental Engineering, Massachusetts
Institute of Technology, Cambridge, MA, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Department of Physics and Astronomy, University of Leicester,
Leicester, UK</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Chemistry, University of California, Berkeley, CA, USA</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Department of Earth and Planetary Science, University of California,
Berkeley, CA, USA</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Science Systems and Applications Inc., Lanham, MD, USA</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>NASA Goddard Space Flight Center, Greenbelt, MD, USA</institution>
        </aff>
        <aff id="aff9"><label>9</label><institution>Goddard Earth Sciences Technology and Research, Universities Space
Research Association, Columbia, MD, USA</institution>
        </aff>
        <aff id="aff10"><label>a</label><institution>now at: NASA Langley Research Center, Hampton, VA, USA</institution>
        </aff>
        <aff id="aff11"><label>b</label><institution>now at: Division of Geological and Planetary Sciences, California
Institute of Technology, Pasadena, CA, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Rachel F. Silvern (rsilvern@g.harvard.edu)</corresp></author-notes><pub-date><day>12</day><month>July</month><year>2019</year></pub-date>
      
      <volume>19</volume>
      <issue>13</issue>
      <fpage>8863</fpage><lpage>8878</lpage>
      <history>
        <date date-type="received"><day>18</day><month>February</month><year>2019</year></date>
           <date date-type="rev-request"><day>25</day><month>February</month><year>2019</year></date>
           <date date-type="rev-recd"><day>24</day><month>May</month><year>2019</year></date>
           <date date-type="accepted"><day>3</day><month>June</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 </copyright-statement>
        <copyright-year>2019</copyright-year>
      <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://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e285">The National Emission Inventory (NEI) of the US Environmental
Protection Agency (EPA) reports a steady decrease in US <inline-formula><mml:math id="M5" 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> emissions
over the 2005–2017 period at a rate of 0.1 Tg N a<inline-formula><mml:math id="M6" 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> (53 % decrease
over the period), reflecting sustained efforts to improve air quality.
Tropospheric <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> columns observed by the satellite-based Ozone
Monitoring Instrument (OMI) over the US show a steady decrease until 2009
but a flattening afterward, which has been attributed to a flattening of
<inline-formula><mml:math id="M8" 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> emissions, contradicting the NEI. We show here that the
steady 2005–2017 decrease in <inline-formula><mml:math id="M9" 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> emissions reported by the NEI is in
fact largely consistent with observed network trends of surface <inline-formula><mml:math id="M10" 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
ozone concentrations. The OMI <inline-formula><mml:math id="M11" 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> trend is instead similar to that
observed for nitrate wet deposition fluxes, which is weaker than that for
anthropogenic <inline-formula><mml:math id="M12" 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> emissions, due to a large and increasing relative
contribution of non-anthropogenic background sources of <inline-formula><mml:math id="M13" 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
lightning and soils). This is confirmed by contrasting OMI <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> trends
in urban winter, where the background is low and OMI <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> shows a
2005–2017 decrease consistent with the NEI, and rural summer, where the
background is high and OMI <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> shows no significant 2005–2017 trend. A
GEOS-Chem model simulation driven by NEI emission trends for the 2005–2017
period reproduces these different trends, except for the post-2009 flattening
of OMI <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>, which we attribute to a model underestimate of free
tropospheric <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>. Better understanding is needed of the factors
controlling free tropospheric <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> in order to relate satellite
observations of tropospheric <inline-formula><mml:math id="M20" 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> columns to the underlying <inline-formula><mml:math id="M21" 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>
emissions and their trends. Focusing on urban winter conditions in the
satellite data minimizes the effect of this free tropospheric background.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e487">Nitrogen oxide radicals (<inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow><mml:mo>≡</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow><mml:mo>+</mml:mo><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:mrow></mml:math></inline-formula>) emitted by fuel
combustion harm air quality by catalyzing ozone production and by producing
nitrate particulate matter. They also contribute to acid and nitrogen
deposition. Starting in the early<?pagebreak page8864?> 2000s, the US Environmental Protection
Agency (EPA) implemented increasingly stringent <inline-formula><mml:math id="M23" 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 controls
targeted principally at improving ozone air quality. The EPA National
Emission Inventory (NEI) reports a steady decrease in US <inline-formula><mml:math id="M24" 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> emissions
over the 2005–2017 period at a rate of 0.10 Tg N a<inline-formula><mml:math id="M25" 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> or 53 % overall
(EPA, 2018). However, Jiang et al. (2018) showed that tropospheric <inline-formula><mml:math id="M26" 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>
columns observed by the OMI satellite instrument over the US stopped
decreasing after 2009, and they concluded that <inline-formula><mml:math id="M27" 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> emissions have been
decreasing much less than reported by the NEI. Here we show that the
flattening of the OMI <inline-formula><mml:math id="M28" 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> trend is in fact not inconsistent with the
sustained decrease in <inline-formula><mml:math id="M29" 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> emissions reported by the NEI and that the
NEI emission trend is consistent with other atmospheric observations of
<inline-formula><mml:math id="M30" 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 ozone trends. Our results demonstrate the importance of
accounting for the free tropospheric <inline-formula><mml:math id="M31" 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> background when using
satellite observations of <inline-formula><mml:math id="M32" 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> columns to infer <inline-formula><mml:math id="M33" 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> emissions and
their trends.</p>
      <p id="d1e639">The Ozone Monitoring Instrument (OMI) aboard the US National Aeronautics and
Space Administration (NASA) Aura satellite has been making continuous daily
global observations of <inline-formula><mml:math id="M34" 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> since late 2004 (Levelt et al., 2006, 2018).
The <inline-formula><mml:math id="M35" 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 (Boersma et al., 2011; Bucsela et al., 2013) involves
spectral fitting of measured nadir solar backscatter at 400–500 nm, yielding
“slant” <inline-formula><mml:math id="M36" 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> columns along the line of sight from which the
contribution from the stratosphere is removed (Martin et al., 2002; Richter
and Burrows, 2002; Bucsela et al., 2013). The slant tropospheric columns are
then converted to actual tropospheric <inline-formula><mml:math id="M37" 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> columns by accounting for
surface and atmospheric scattering, and assuming a vertical distribution of
<inline-formula><mml:math id="M38" 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> within the column (“shape factor”). In polluted regions with high
<inline-formula><mml:math id="M39" 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> emissions, most of the information in the <inline-formula><mml:math id="M40" 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> tropospheric
column is presumed to originate from the boundary layer. Thus, the column is
commonly viewed as a proxy for <inline-formula><mml:math id="M41" 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> emissions.</p>
      <p id="d1e731">Satellite observations of tropospheric <inline-formula><mml:math id="M42" 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> columns have been used
extensively to infer <inline-formula><mml:math id="M43" 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> emissions and their trends (Leue et al., 2001;
Martin et al., 2003; Richter et al., 2005; Boersma et al., 2008). OMI
<inline-formula><mml:math id="M44" 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> observations from the early part of the record showed decreasing
trends over the US consistent with the decreases in <inline-formula><mml:math id="M45" 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> emissions
reported by the NEI (Russell et al., 2012; Duncan et al., 2013, 2016; Streets et
al., 2013; de Foy et al., 2015;  Krotkov et al., 2016)
and also consistent with trends in <inline-formula><mml:math id="M46" 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 observed from
surface networks (Kharol et al., 2015; Lamsal et al., 2015; Lu et al., 2015;
Tong et al., 2015; Zhang et al., 2018). Several studies reported a
steepening of the OMI <inline-formula><mml:math id="M47" 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> decrease during the Great Recession of
2007–2009 and a subsequent flattening attributed to economic recovery
(Russell et al., 2012; Tong et al., 2015; de Foy et al., 2016). However, the
analysis of the 2005–2015 record by Jiang et al. (2018) shows that the
post-2009 flattening of the <inline-formula><mml:math id="M48" 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> trend extends well beyond the initial
economic recovery period.</p>
      <p id="d1e812">The NEI is a “bottom-up” national inventory compiled by the EPA every 3 years using continuous emission monitoring systems (CEMS) for large point
sources, and estimates derived from activity data and emission factors
(<inline-formula><mml:math id="M49" 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> emitted per unit of activity) for smaller and distributed sources.
Emissions in 2017 estimated by EPA (2018) included 35 % from on-road
mobile sources, 25 % from off-road mobile sources, 12 % from industrial
point sources, and 27 % from electricity generating units (EGUs). Mobile
emissions are estimated with the Motor Vehicle Emission Simulator (MOVES)
model using vehicle population, vehicle miles traveled (VMT), and
operating modes as inputs. Long-term trends in <inline-formula><mml:math id="M50" 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> emissions are recomputed with
each new NEI release using updated emission models so that national trends
are self-consistent for a given NEI version.</p>
      <p id="d1e838">Many recent studies using near-source, urban, and regional observations of
atmospheric <inline-formula><mml:math id="M51" 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> have found that the NEI greatly overestimates US
<inline-formula><mml:math id="M52" 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> emissions (Castellanos et al., 2011; Brioude et al., 2013; Anderson
et al., 2014; Goldberg et al., 2016; Souri et al., 2016; Travis et al.,
2016). CEMS measurements of point sources are considered reliable but tunnel
and roadside measurements show that the MOVES inventory for mobile sources
may be too high (Fujita et al., 2012). Fuel-based approaches for estimating
emissions from mobile sources appear to be more reliable than the MOVES VMT
approach (Dallmann and Harley, 2010; McDonald et al., 2012; Kim et al.,
2016). McDonald et al. (2018) showed that on-road gasoline <inline-formula><mml:math id="M53" 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
factors used by NEI are a factor of 2 too high compared to roadside
observations and their fuel-based inventory. All these studies were
conducted under summertime or warm conditions. By contrast, atmospheric
observations of <inline-formula><mml:math id="M54" 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 related species during the WINTER campaign over
the northeastern US during February–March 2015 showed good agreement with the
NEI (Jaeglé et al., 2018; Salmon et al., 2018).</p>
      <p id="d1e885">The uncertainty regarding NEI <inline-formula><mml:math id="M55" 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> emissions suggests that the trend in
these emissions could be uncertain as well. However, a flattening out of US
<inline-formula><mml:math id="M56" 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> emissions over the past decade, as inferred by Jiang et al. (2018)
from the OMI data, would be difficult to reconcile with observations of
steady improvement in ozone air quality (Astitha et al., 2017; Chang et al.,
2017), which has been attributed specifically to <inline-formula><mml:math id="M57" 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 controls
(Hidy and Blanchard, 2015; Simon et al., 2015; Strode et al., 2015; Xing et
al., 2015; Blanchard and Hidy, 2018; Li et al., 2018). Here we conduct a
more comprehensive analysis of 2005–2017 trends in US <inline-formula><mml:math id="M58" 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> emissions
by using the GEOS-Chem chemical transport model (Travis et al., 2016) to
concurrently interpret the trends observed in OMI <inline-formula><mml:math id="M59" 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> columns, nitrogen
wet deposition fluxes, and surface observations of <inline-formula><mml:math id="M60" 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 ozone.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><?xmltex \opttitle{The 2005--2017 trends of OMI tropospheric {$\protect\chem{NO_{2}}$} columns}?><title>The 2005–2017 trends of OMI tropospheric <inline-formula><mml:math id="M61" 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> columns</title>
      <?pagebreak page8865?><p id="d1e975">Figure 1 shows the 2005–2017 trends of OMI tropospheric <inline-formula><mml:math id="M62" 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> columns
averaged spatially and annually over the contiguous US. The observations are
from the NASA operational retrieval (level 2, version 3.0; Krotkov et al., 2017)
after removing cloudy scenes (cloud radiance fraction <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula>),
bright surfaces (surface reflectivity <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula>), and observations
affected by the so-called row anomaly (Dobber et al., 2008). OMI is in a
sun-synchronous orbit with overpass at 13:30 LT. It measures
backscattered solar radiation in the nadir and off-track, with <inline-formula><mml:math id="M65" 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="M66" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> nadir pixel resolution and global daily coverage. The retrieval
fits the backscattered radiance spectrum to obtain the total slant <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>
column along the line of sight from the Sun to the satellite. The
stratospheric contribution to the total slant column is estimated using OMI
observations over clean background and cloudy areas and applying an
interpolating–filtering–smoothing algorithm (Bucsela et al., 2013). The
remaining tropospheric slant column is then converted to a vertical column
with an air mass factor (AMF; Palmer et al., 2001) that convolves the
altitude-dependent sensitivity from atmospheric scattering (scattering
weights) with the local relative vertical distribution of <inline-formula><mml:math id="M68" 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 the
Global Modeling Initiative (GMI) model (shape factor). Over continental
source regions, the AMF dominates the overall retrieval error due to
uncertainties in a priori <inline-formula><mml:math id="M69" 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> profiles, surface albedo, and
aerosol and cloud parameters (Kleipool et al., 2008; Boersma et al., 2011;
Lamsal et al., 2014; Lorente et al., 2017). We recomputed the AMFs using
GEOS-Chem rather than GMI shape factors and found little difference in the
mean (Fig. 1).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e1066">The 2005–2017 trends in tropospheric <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> columns and <inline-formula><mml:math id="M71" 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>
emissions over the contiguous US. Panel <bold>(a)</bold> shows OMI observations
averaged over the contiguous US and the corresponding GEOS-Chem simulation.
The OMI observations are from the NASA retrieval (Krotkov et al., 2017) with
air mass factors (AMFs) computed from the original GMI model <inline-formula><mml:math id="M72" 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 profiles or GEOS-Chem vertical profiles. Panel <bold>(b)</bold> shows
percent changes in tropospheric <inline-formula><mml:math id="M73" 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> columns relative to 2005. Panel <bold>(c)</bold> shows 2005–2017 annual total <inline-formula><mml:math id="M74" 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> emissions from the GEOS-Chem
model, including anthropogenic fuel combustion emissions from the National
Emission Inventory (NEI), with a 60 % decrease for non-EGU sources (see
text and Appendix).</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/8863/2019/acp-19-8863-2019-f01.png"/>

      </fig>

      <p id="d1e1140">The OMI data show an evident flattening of <inline-formula><mml:math id="M75" 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> columns after 2009, as
pointed out by Jiang et al. (2018), who also find the same flattening in
alternative OMI <inline-formula><mml:math id="M76" 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 produced by KNMI (Boersma et al., 2011) and UC Berkeley (Laughner et al., 2018). <inline-formula><mml:math id="M77" 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> tropospheric columns decrease at a mean rate of <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:mn mathvariant="normal">6</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M79" 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> over the 2005–2009 period but then do not change significantly post-2009. We find that data for the western, central, northeastern, and southeastern US all show similar
trends. Hence, we focus our analysis on the mean trends over the contiguous
US, following Jiang et al. (2018).</p>
      <p id="d1e1201">Also shown in Fig. 1 are trends from a 13-year simulation (2005–2017) with
the GEOS-Chem global chemical transport model at 0.5<inline-formula><mml:math id="M80" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M81" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M82" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> nested horizontal resolution over North America. The model is
driven by NEI <inline-formula><mml:math id="M83" 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> emissions for fuel combustion, decreased by 60 %
for non-EGU sources following Travis et al. (2016). It also includes
<inline-formula><mml:math id="M84" 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> emissions from background (nonfuel combustion) sources, including
open fires (Darmenov and da Silva, 2013), lightning (Murray et al., 2012),
and soil and fertilizer (Hudman et al., 2012). Further details on the model
are in the Appendix. The model <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> column averages 28 % lower than
observed, due to both an underestimate in background <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>, discussed
below, and because the Travis et al. (2016) correction to the NEI is
excessive, which we will address in a separate paper. More to the point
here, the model shows a sustained decrease, averaging <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.1</mml:mn></mml:mrow></mml:math></inline-formula> % a<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> over the 2005–2017 period, at odds with the OMI observations,
though lower than the NEI reported decrease of 5.9 % a<inline-formula><mml:math id="M89" 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> over the
same period. Here and throughout this paper we derive linear trends by
ordinary regression and express them in units of percent per annum (% a<inline-formula><mml:math id="M90" 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>) relative to
the mean over the data period, following Jiang et al. (2018). We compute
uncertainty using the bootstrapping method as the error standard deviation
of the linear trend.</p>
      <p id="d1e1322">The weaker relative trend in the model compared to the NEI is because of the
contribution from background <inline-formula><mml:math id="M91" 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> sources. Figure 1c
shows the annual total US <inline-formula><mml:math id="M92" 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> emissions for 2005–2017 in the GEOS-Chem
simulation. Anthropogenic emissions from fuel combustion decrease at a rate
of 5.9 % a<inline-formula><mml:math id="M93" 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>, following the NEI trend. But these emissions account
for only 61 % of total US emissions in 2005 and 42 % in 2017. Natural
emissions from lightning and soils play a relatively increasing role as
anthropogenic emissions decrease. They have interannual variability but no
significant 2005–2017 trend. The trend of total US <inline-formula><mml:math id="M94" 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> emissions for
2005–2017 in GEOS-Chem is <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3.5</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M96" 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>, closely matching the simulated
<inline-formula><mml:math id="M97" 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 trend.</p>
      <p id="d1e1404">Trends in the <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> chemical lifetime over the 2005–2017 period would
affect the relationship between trends in <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> emissions and atmospheric
<inline-formula><mml:math id="M100" 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>. Many factors could contribute to a trend in <inline-formula><mml:math id="M101" 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> lifetime
(Laughner, 2018; Laughner and Cohen, 2018). We find in GEOS-Chem that the
daily tropospheric <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> column lifetime over the contiguous US is 8.1 h
in 2005 (annual mean) and 7.7 h in 2017. In the model at least, the trend in
<inline-formula><mml:math id="M103" 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> lifetime is much weaker than the trend in emissions, so that the
trend in concentrations mainly follows that of emissions.</p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>The 2005–2017 trends of surface observations</title>
      <?pagebreak page8866?><p id="d1e1482">Long-term records of surface <inline-formula><mml:math id="M104" 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 over the US are
available at a large number of monitoring sites from the US EPA Air Quality
System (AQS) (<uri>https://www.epa.gov/aqs</uri>, last access: 4 September 2018; Demerjian, 2000)
and at additional sites in the southeast from the Southeastern Aerosol
Research and Characterization Study (SEARCH) network (<uri>https://www.dropbox.com/sh/o9hxoa4wlo97zpe/AACbm6LetQowrpUgX4vUxnoDa?dl=0</uri>, last access: 27 July 2018; Hansen et al., 2003; Edgerton et al., 2006). AQS sites are mainly urban
and measure <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> with a chemiluminescence analyzer equipped with a
molybdenum converter, known to have positive interferences from <inline-formula><mml:math id="M106" 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>
oxidation products including peroxyacetyl nitrate (PAN) and nitric acid
(<inline-formula><mml:math id="M107" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>; Dunlea et al., 2007; Steinbacher et al., 2007; Reed et al.,
2016). SEARCH sites are both urban and rural and use a more specific
photolytic converter instrument in which broadband photolysis of <inline-formula><mml:math id="M108" 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
followed by chemiluminescence detection of the NO product with accuracy
better than 10 % (Ryerson et al., 2000; Pollack et al., 2010).<?xmltex \hack{\newpage}?></p>
      <p id="d1e1548">Figure 2a–d show annual average trends in daily
surface <inline-formula><mml:math id="M109" 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 at the 132 AQS sites with continuous
yearlong records for 2005–2017 and the 2 rural SEARCH sites (Centreville, AL,
and Yorkville, GA) with continuous records for 2005–2016 (SEARCH was
discontinued in 2017). Also shown for the AQS sites are the values corrected
for interferences based on local GEOS-Chem monthly mean <inline-formula><mml:math id="M110" 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>, alkyl
nitrate, PAN, and <inline-formula><mml:math id="M111" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations and following the correction
factor in Lamsal et al. (2008). The AQS data show decreasing trends
throughout the 2005–2017 period, generally consistent with the NEI. The
rural SEARCH sites also show a steady decrease but are more noisy (only two sites). One would expect the trend in the urban AQS data to be most
indicative of the trend in anthropogenic <inline-formula><mml:math id="M112" 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> emissions from fuel
combustion. GEOS-Chem underestimates the AQS observations because of the
urban nature of the sites, but the model relative decreases agree closely
with observations for both the AQS and the SEARCH data. This is in sharp
contrast to the OMI <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> data.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e1608">The 2005–2017 trends in annual mean surface <inline-formula><mml:math id="M114" 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
and nitrate wet deposition fluxes over the contiguous US. Observations are
compared to GEOS-Chem model values sampled at the corresponding sites. The
map in the right panel <bold>(g)</bold> shows the observation sites for the AQS, SEARCH, and NADP
measurements networks with continuous annual records for 2005–2017 (2016 for
SEARCH). Panels <bold>(a)</bold> and <bold>(b)</bold> show surface <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> observed at AQS sites (mainly
urban). The measurements are affected by positive interference from <inline-formula><mml:math id="M116" 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>
oxidation products and the gray line shows the data corrected as in Lamsal
et al. (2008). Panels <bold>(c)</bold> and <bold>(d)</bold> show surface <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> at the two rural SEARCH
sites in the southeastern US. Panels <bold>(e)</bold> and <bold>(f)</bold> shows nitrate wet deposition
fluxes at NADP sites. Panels <bold>(b)</bold>, <bold>(d)</bold> and <bold>(f)</bold> show trends relative to 2005 values
and the mean <inline-formula><mml:math id="M118" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> standard deviation percent change per year is shown
inset. All trends shown are statistically significant.</p></caption>
        <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/8863/2019/acp-19-8863-2019-f02.png"/>

      </fig>

      <p id="d1e1701">Jiang et al. (2018) reported AQS surface <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> trends of <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6.6</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.4</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M121" 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> for 2005–2009 and <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.6</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M123" 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> for
2011–2015, indicating a significant weakening of the trend with time. But
they used all AQS sites in that analysis including those with incomplete
records. We find that when using only sites with continuous records, the
slope is steeper for the latter time period. Specifically, we find the AQS
trend to be <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6.6</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.2</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M125" 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> for 2005–2009 and <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4.5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.7</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M127" 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> for 2011–2015. In comparison, the NEI emission trend is
<inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6.4</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M129" 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> for 2005–2009 and <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5.3</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M131" 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> for 2011–2015. Thus,
the surface data suggest a slight weakening of the <inline-formula><mml:math id="M132" 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 trend
relative to the NEI but not the flattening implied by the OMI data. Jiang et
al. (2018) presented an alternative fuel-based <inline-formula><mml:math id="M133" 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
to the NEI, featuring a slowdown in the trend of US <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> emissions after
2009 due to a slower rate of reduction for industrial, off-road mobile, and
on-road diesel sources as well as a smaller relative contribution of on-road
gasoline. That inventory shows a <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.9</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M136" 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> trend for 2011–2015. The
AQS trend is in somewhat better agreement with the NEI inventory but could
accommodate either inventory within its error standard deviation.</p>
      <p id="d1e1921">Figure 2e–f show observed and simulated trends in nitrate
(<inline-formula><mml:math id="M137" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) wet deposition fluxes for the 138 National Acid Deposition
Program (NADP; <uri>https://nadp.slh.wisc.edu/data/NTN/</uri>, last access: 14 August 2018) sites with
continuous yearlong records for 2005–2017. Nitric acid gas and nitrate
aerosol are both efficiently scavenged by precipitation and the lifetime of
<inline-formula><mml:math id="M138" 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> is sufficiently short that nitrate wet deposition fluxes should
relate to total <inline-formula><mml:math id="M139" 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> emissions. The relationship is not one-to-one
because of competition from dry deposition but one would not expect a
long-term trend in the wet/dry deposition ratio. GEOS-Chem model values for
individual years are corrected for precipitation bias using the
high-resolution PRISM precipitation data (<uri>http://prism.oregonstate.edu</uri>, last access: 14 August 2018; Di Luzio et al., 2008), as described by
Paulot et al. (2014) and Travis et al. (2016). Model values average 17 %
lower than observed values, again because the model may underestimate emissions,
but the trends are consistent. The fluxes show a decrease over the 2005–2017
time period (averaging <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.7</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M141" 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> observed, <inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.9</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M143" 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> modeled), weaker than for surface <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> concentrations.
After 2012, there is still a significant decrease in nitrate wet deposition,
though it is less than during the earlier time period (averaging <inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.9</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M146" 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> observed and <inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.7</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M148" 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> modeled).</p>
      <p id="d1e2074">Nitrate wet deposition is more sensitive to background (nonfuel combustion)
influences than <inline-formula><mml:math id="M149" 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 because (1) the wet deposition sites
are prevailingly rural and (2) precipitation scavenges a deeper column. Indeed,
in GEOS-Chem, the mean nitrate wet deposition trend is more consistent with
the <inline-formula><mml:math id="M150" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3.5</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M151" 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> trend of total <inline-formula><mml:math id="M152" 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> emissions (including lightning
and soils) than that of emissions from fuel combustion (<inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5.9</mml:mn></mml:mrow></mml:math></inline-formula>% a<inline-formula><mml:math id="M154" 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>).</p>
      <?pagebreak page8867?><p id="d1e2144">The relative contribution from background sources to nitrate wet deposition
would be expected to increase over time as fuel combustion emissions
decrease. In order to quantify this, we performed GEOS-Chem sensitivity
simulations for 2005 and 2017 with only background <inline-formula><mml:math id="M155" 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> emissions
(shutting off <inline-formula><mml:math id="M156" 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> emissions from US fuel combustion). We find that
background contributed 50 % of nitrate wet deposition at NADP sites in
2005 but 69 % in 2017. In contrast, background only contributed 5 % to
surface <inline-formula><mml:math id="M157" 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 AQS sites in 2005 and 10 % in 2017.</p>
      <p id="d1e2180">Figure 3 shows summertime ozone trends for 2005–2017 as further evidence of
a sustained decrease in anthropogenic <inline-formula><mml:math id="M158" 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> emissions. Data are from the
AQS and Clean Air Status and Trends Network (CASTNET; <uri>https://www.epa.gov/castnet</uri>, last access: 27 July 2018) networks. We show records for the 47 CASTNET
and 427 AQS sites with continuous summertime records for 2005–2017. The
trends are for the 95th percentiles in the maximum daily 8 h average
(MDA8) values determined at individual sites and then averaged across all
sites for each summer. We excluded high-elevation (<inline-formula><mml:math id="M159" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> km)
CASTNET sites in the western US because they have different trends driven in
part by the larger influence from background ozone (Cooper et al., 2011; Lin
et al., 2017; Jaffe et al., 2018). Much of the interannual variability in
ozone concentrations in Fig. 3 can be explained by surface temperatures,
including the 2012 peak in ozone in the observations and captured by
GEOS-Chem, which is due to anomalously high temperatures (Fiore et al.,
2015; Jia et al., 2016; Lin et al., 2017). Nonetheless, the surface
observations do show overall decreases over the 2005–2017 time period. On a
national scale, the observations show declines of <inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.11</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.08</mml:mn></mml:mrow></mml:math></inline-formula> ppb a<inline-formula><mml:math id="M161" 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> (CASTNET) and <inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.04</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.03</mml:mn></mml:mrow></mml:math></inline-formula> ppb a<inline-formula><mml:math id="M163" 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> (AQS), with no indication of a post-2009 flattening. The GEOS-Chem model shows similar
trends. The sustained (post-2009) decrease in ozone pollution over the past
decade provides additional evidence of a continued decrease in anthropogenic
<inline-formula><mml:math id="M164" 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> emissions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e2270">Summertime surface ozone trends for 2005–2017 at the CASTNET and
AQS networks in the contiguous US. The trends are for the 95th
percentile of the maximum daily 8 h average (MDA8) ozone concentrations
computed for individual sites (shown in the map on the right) and then
averaged over all sites from the network. High-elevation (<inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> km) CASTNET sites in the western US are excluded. The slope and standard
deviation of the linear regressions are shown inset, and all trends shown
are statistically significant.</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/8863/2019/acp-19-8863-2019-f03.png"/>

      </fig>

</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Comparative analysis of trends</title>
      <p id="d1e2297">Figure 4 combines the relative trends since 2005 of NEI
<inline-formula><mml:math id="M166" 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> emissions, OMI tropospheric <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> columns, surface <inline-formula><mml:math id="M168" 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, and nitrate wet deposition fluxes into a single plot. Observed surface <inline-formula><mml:math id="M169" 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 follow the NEI emissions trend, showing consistency with a
sustained<?pagebreak page8868?> decline of emissions over the 2005–2017 time period. This behavior
is well captured by GEOS-Chem, which confirms the <inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> relationship expected
between surface <inline-formula><mml:math id="M171" 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 and <inline-formula><mml:math id="M172" 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> emissions. Nitrate wet
deposition observations show a much weaker trend, which we attributed in
Sect. 3 to a larger contribution of the background. The GEOS-Chem trend
for nitrate wet deposition and tropospheric <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> columns is similarly
weaker than for surface <inline-formula><mml:math id="M174" 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>, reflecting the influence of the
background, but shows a steeper decrease than observed after 2009. This
suggests that GEOS-Chem may underestimate the background contribution.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e2403">Relative trends since 2005 of NEI <inline-formula><mml:math id="M175" 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> emissions and relevant
atmospheric quantities averaged over the contiguous US. Panel <bold>(a)</bold> shows
observations and <bold>(b)</bold> shows the GEOS-Chem simulation. NEI
<inline-formula><mml:math id="M176" 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> emissions are the same in both panels. The SEARCH network was
discontinued in 2017.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/8863/2019/acp-19-8863-2019-f04.png"/>

      </fig>

      <p id="d1e2440">Satellite-based tropospheric <inline-formula><mml:math id="M177" 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> columns show trends remarkably similar
to those of nitrate wet deposition fluxes, both in the OMI observations and
in GEOS-Chem, suggesting that the post-2009 flattening of the OMI trend is
due to a large and increasing relative influence of the background rather
than to a leveling of US <inline-formula><mml:math id="M178" 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> emissions.<?xmltex \hack{\newpage}?></p>
</sec>
<sec id="Ch1.S5">
  <label>5</label><?xmltex \opttitle{Background contribution to OMI {$\protect\chem{NO_{2}}$} trends}?><title>Background contribution to OMI <inline-formula><mml:math id="M179" 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> trends</title>
      <p id="d1e2487">We showed in Sect. 4 that the 2005–2017 trend of OMI <inline-formula><mml:math id="M180" 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> columns over
the US is similar to that of nitrate wet deposition and much weaker than
that of surface <inline-formula><mml:math id="M181" 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, pointing to the importance of
background in affecting the <inline-formula><mml:math id="M182" 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. To further examine this effect,
we segregated the OMI observations into winter and summer as well as urban and rural. Urban
conditions are defined as the top 10 % <inline-formula><mml:math id="M183" 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>-emitting 0.5<inline-formula><mml:math id="M184" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M185" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M186" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid squares in the US according to the NEI. We
expect background influences to be relatively higher at rural than urban
sites, and higher in summer (lightning, soil, intercontinental transport;
Fischer et al., 2014) than in winter. Thus, background influences should be
at a minimum in winter urban conditions and a maximum under summer rural
conditions.</p>
      <p id="d1e2560">Figure 5 shows the results. OMI <inline-formula><mml:math id="M187" 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> observations in urban winter show a
steady decline at a mean rate of <inline-formula><mml:math id="M188" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M189" 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>, with no
post-2009 flattening, though there is some suggestion of a slightly weaker
trend after 2009 when compared to GEOS-Chem driven by NEI. By contrast, the
OMI <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> observations in rural summer show no significant trend over the
2005–2017 period. GEOS-Chem for rural summer shows a significant decreasing
trend for 2005–2017 but weaker than for urban winter and become
insignificant for the 2009–2017 period. The winter rural and summer urban
conditions in Fig. 5 show trends that are intermediate between these two limiting
cases. The ability of GEOS-Chem to capture the observed post-2009 weakening
of the trend in the summer urban case argues against a seasonal flattening
of emissions that would affect summer but not winter.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e2611">OMI tropospheric <inline-formula><mml:math id="M191" 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 trends over the contiguous US
relative to 2005, separated into urban and rural as well as summer (JJA) and winter (DJF).
OMI observations are shown in black, the standard GEOS-Chem model simulation
with EPA National Emission Inventory (NEI) trends (EPA, 2018) is in red, and
the GEOS-Chem sensitivity simulation with additional <inline-formula><mml:math id="M192" 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> background (50 ppt above 5 km in winter and above 10 km in summer, up to the local
tropopause) is shown in blue. Slopes and standard deviation of the linear
regressions are shown inset. Urban conditions are defined as the top 10 %
<inline-formula><mml:math id="M193" 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>-emitting 0.5<inline-formula><mml:math id="M194" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M195" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M196" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid squares in
the NEI.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/8863/2019/acp-19-8863-2019-f05.png"/>

      </fig>

      <?pagebreak page8869?><p id="d1e2680">It thus appears that the post-2009 flattening of the OMI <inline-formula><mml:math id="M197" 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> trend over
the US is due to increasing relative importance of the <inline-formula><mml:math id="M198" 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> background,
rather than to flattening of US <inline-formula><mml:math id="M199" 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> emissions. Satellite observations
of tropospheric <inline-formula><mml:math id="M200" 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> columns are more sensitive to the free troposphere
than to the boundary layer because of atmospheric scattering; the
sensitivity increases by a factor of 3 from the surface to the upper
troposphere for clear sky and by much more for a cloudy atmosphere (Martin
et al., 2002). For the OMI <inline-formula><mml:math id="M201" 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 set used here, the sensitivity
increases by over a factor of 4 from the surface to the upper
troposphere on average, as given by the scattering weights (Krotkov et al., 2017). The
AMF is intended to correct for this effect but relies on an assumed model
vertical distribution of <inline-formula><mml:math id="M202" 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> that may not correctly account for free
tropospheric levels or for the changing ratio between the free troposphere
and the boundary layer as anthropogenic <inline-formula><mml:math id="M203" 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> emissions decrease.</p>
      <p id="d1e2761">There is indeed evidence that free tropospheric <inline-formula><mml:math id="M204" 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> makes a large
contribution to OMI <inline-formula><mml:math id="M205" 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> columns and that models underestimate this
contribution. Measurements of <inline-formula><mml:math id="M206" 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 profiles during the
SEAC<inline-formula><mml:math id="M207" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula>RS aircraft campaign over the southeastern US in August–September 2013 showed a median concentration of 300 ppt near the surface, dropping to a
50 ppt background in the free troposphere at 2–10 km, and rising back to 130 ppt at the 12 km aircraft ceiling (Silvern et al., 2018). By applying OMI
scattering weights to this median vertical profile, most representative of a
rural profile, Travis et al. (2016) found that the boundary layer below 1.5 km contributed only 19 %–28 % of the OMI <inline-formula><mml:math id="M208" 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> tropospheric column. A
GEOS-Chem simulation of the SEAC<inline-formula><mml:math id="M209" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula>RS conditions matched the observed 50 ppt background (mostly from lightning) but could not reproduce the
enhancement above 10 km (Travis et al., 2016; Silvern et al., 2018). The GMI
model used to compute AMFs in the NASA OMI <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> retrievals also has
little <inline-formula><mml:math id="M211" 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 upper troposphere (Lamsal et al., 2014). Measurements
of <inline-formula><mml:math id="M212" 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 upper troposphere are prone to positive interferences
because of inlet decomposition of labile reservoirs (Reed et al., 2016), but
the measurements in SEAC<inline-formula><mml:math id="M213" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula>RS were designed to minimize and correct for
these interferences (Thornton et al., 2000; Day et al., 2002; Wooldridge et
al., 2010; Nault et al., 2015). Silvern et al. (2018) suggested that errors
in the kinetics of NO–<inline-formula><mml:math id="M214" 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="M215" 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> cycling reactions could explain model
underestimates of <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> concentrations in the upper troposphere.</p>
      <p id="d1e2903">Choi et al. (2014) and Belmonte Rivas et al. (2015) used the so-called
cloud-slicing method to isolate the upper tropospheric contribution to the
OMI <inline-formula><mml:math id="M217" 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> observations by comparing neighboring cloudy scenes with cloud
tops at different altitudes. They report in this manner partial <inline-formula><mml:math id="M218" 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>
columns at 6–10 km altitude. Marais et al. (2018) evaluated these data in
comparison with aircraft observations and found large uncertainties but
concluded that GEOS-Chem underestimates <inline-formula><mml:math id="M219" 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 6–10 km over North
America by 20–30 ppt in winter with no significant bias in summer. The good
agreement in summer is consistent with the comparison to SEAC<inline-formula><mml:math id="M220" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula>RS
observations, which shows, however, a low model bias above 10 km.</p>
      <p id="d1e2948">We conducted a sensitivity test, adding 50 ppt of background <inline-formula><mml:math id="M221" 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
GEOS-Chem vertical profiles above 5 km altitude in winter and above 10 km in
summer, up to the local tropopause. The resulting normalized vertical
profiles (shape factors) were convolved with the vertical distribution of
sensitivities (scattering weights) provided by the NASA retrieval to
recompute the AMFs. The implications for the model trends are shown in
Fig. 5 as the blue lines. The effect is large for winter rural conditions,
where the added free tropospheric background is particularly important and
largely reconciles the model trend with the OMI observations. It is much
less in summer, where the addition is only above 10 km and there is already
substantial background <inline-formula><mml:math id="M222" 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> present. The<?pagebreak page8870?> discrepancy between the model and the
observations in summer is largely driven by the uptick in the summer
rural observations for 2016–2017.</p>
      <p id="d1e2973">It is possible that additional background <inline-formula><mml:math id="M223" 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> missing from the model in
summer could be present in the tropopause region and lower stratosphere. The
deepest convection in summertime over the US can reach 17 km in the
lowermost stratosphere (Randel et al., 2012; Huntrieser et al., 2016b;
Anderson et al., 2017; Herman et al., 2017; Smith et al., 2017). Such a deep
convective injection could conceivably deliver substantial lightning
<inline-formula><mml:math id="M224" 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> above the tropopause. Although delivered above the tropopause, this
<inline-formula><mml:math id="M225" 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> would be counted as tropospheric in retrievals because it would
represent an enhancement above background <inline-formula><mml:math id="M226" 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> columns in the
stratospheric separation. It could have a particularly important effect on
the AMF by being delivered above clouds. High <inline-formula><mml:math id="M227" 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> mixing ratios in the
lowermost stratosphere were observed over the central and southeastern US
during the DC3 aircraft campaign in May–June 2012 and were attributed to
lightning (Huntrieser et al., 2016a, b), and higher
lightning flash rates have been observed in tropopause-penetrating
above-anvil cirrus plumes (Bedka et al., 2018). There is suggestive evidence
that convective injection into the lowermost stratosphere over the US may
have increased during the 2004–2013 period (Cooney et al., 2018), which
could further affect the OMI <inline-formula><mml:math id="M228" 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 trend, although the Lightning
Imaging Sensor (LIS) satellite data do not show a 2003–2012 trend in total
lightning over the US (Koshak et al., 2015). While tropopause heights in the
GEOS MERRA-2 meteorological data driving GEOS-Chem agree well with
SEAC<inline-formula><mml:math id="M229" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula>RS observations of water vapor and ozone (Kuang et al., 2017;
Smith et al., 2017), models in general do not properly capture the observed
convective injections into the lowermost stratosphere (Smith et al., 2017;
Anderson et al., 2019). The 0.5<inline-formula><mml:math id="M230" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M231" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M232" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
resolution of the MERRA-2 meteorological data would be too coarse to resolve
convective overshoots.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusions</title>
      <p id="d1e3085">US emissions of nitrogen oxides (<inline-formula><mml:math id="M233" display="inline"><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow><mml:mo>≡</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow><mml:mo>+</mml:mo><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:mrow></mml:math></inline-formula>) from
fuel combustion steadily declined over 2005–2017 at a mean rate
of 5.9 % a<inline-formula><mml:math id="M234" 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> according to the National Emission Inventory (NEI) of
the US EPA. Tropospheric <inline-formula><mml:math id="M235" 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> columns over the US observed by OMI aboard the Aura satellite instead show a leveling off after 2009, leading to
the suggestion that the NEI emission trend is in error and that related air
quality gains have halted. Here we re-examined this issue by using trends in
surface observations together with a 2005–2017 GEOS-Chem chemical transport
model simulation to better understand the relationship between satellite
<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> observations, <inline-formula><mml:math id="M237" 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> emissions, and their trends.</p>
      <p id="d1e3158">We started by comparing the 2005–2017 GEOS-Chem simulation driven by NEI
emission trends to the OMI observations. The model shows a sustained
decrease in the tropospheric <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> column at a mean rate of <inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.1</mml:mn></mml:mrow></mml:math></inline-formula> % a<inline-formula><mml:math id="M240" 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> over the period. The rate is less than the NEI trend
because of natural <inline-formula><mml:math id="M241" 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> emissions (mainly from lightning and soils) that
account in GEOS-Chem for 58 % of total <inline-formula><mml:math id="M242" 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> emissions over the US by
2017. Nevertheless, the GEOS-Chem simulation cannot capture the post-2009
flattening in the OMI observations.</p>
      <p id="d1e3218">We then examined 2005–2017 US trends in surface observations of <inline-formula><mml:math id="M243" 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 and nitrate wet deposition fluxes from surface networks (AQS,
SEARCH, NADP). Surface <inline-formula><mml:math id="M244" 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 measured by the AQS (urban)
and SEARCH (rural) surface networks show a decline over the 2005–2017 time
period that closely follows the NEI emissions trend, and the same is found
in GEOS-Chem. Some deviation between AQS <inline-formula><mml:math id="M245" 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 NEI towards the
later part of the time period suggests that the rate of decrease in
emissions may have slowed slightly. Nitrate wet deposition shows a much
weaker 2005–2017 trend than surface <inline-formula><mml:math id="M246" 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 NEI emissions, both in the
observations and the model, reflecting a large and increasing relative
contribution from background sources (69 % in the model in 2017) as
anthropogenic emissions decrease. Surface ozone concentrations from the
CASTNET and AQS networks show sustained 2005–2017 decreases, consistent with
the model; such sustained decreases would be hard to reconcile with a
flattening of <inline-formula><mml:math id="M247" 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> emissions.</p>
      <p id="d1e3276">Bringing together these observed trends, we see two different patterns: (1) a 2005–2017 decrease in surface <inline-formula><mml:math id="M248" 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> that supports the steady decrease
in <inline-formula><mml:math id="M249" 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> emissions reported by the EPA NEI and (2) a weaker trend and
post-2009 flattening of OMI <inline-formula><mml:math id="M250" 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 nitrate wet deposition that
reflects a growing influence from the background, rather than large error in
NEI <inline-formula><mml:math id="M251" 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> emissions.</p>
      <?pagebreak page8871?><p id="d1e3324">We confirmed the importance of background <inline-formula><mml:math id="M252" 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 driving the post-2009
flattening of OMI <inline-formula><mml:math id="M253" 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> trends over the US by segregating the OMI
observations into urban and rural as well as winter and summer. There is a steady 2005–2017
decrease in the urban winter data where background influence is lowest. By
contrast, there is no significant 2005–2017 trend in rural summer (where
background influence is highest). The failure of GEOS-Chem to reproduce the
observed post-2009 flattening then points to a model underestimate of the
<inline-formula><mml:math id="M254" 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> background. Cloud-sliced OMI <inline-formula><mml:math id="M255" 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 indicate a GEOS-Chem
underestimate of the upper tropospheric background in winter. Deep
convective injections of lightning <inline-formula><mml:math id="M256" 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> above the tropopause might add
to the <inline-formula><mml:math id="M257" 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> background in summer. Observations from the NASA
SEAC<inline-formula><mml:math id="M258" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula>RS aircraft campaign show lower NO <inline-formula><mml:math id="M259" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M260" 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> ratios than
simulated by GEOS-Chem, which could reflect errors in the kinetics of
NO–<inline-formula><mml:math id="M261" 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="M262" 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> chemical cycling (Silvern et al., 2018). While such
errors would be most important in summertime, chemistry important for
wintertime <inline-formula><mml:math id="M263" 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> not being comprehensively included in models may help to
explain the winter background <inline-formula><mml:math id="M264" 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> underestimate. Observations of
short-chained alkyl nitrates show higher concentrations in the northern
extratropical free troposphere in winter than captured by GEOS-Chem and may
represent an increasing reservoir of background <inline-formula><mml:math id="M265" 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> (Fisher et al.,
2018). Measurements from the WINTER campaign suggest models may also
overestimate <inline-formula><mml:math id="M266" 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> loss via <inline-formula><mml:math id="M267" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> hydrolysis (Jaeglé et al.,
2018; Kenagy et al., 2018; McDuffie et al., 2018), and recent laboratory data
suggest that models using the recommended NASA-JPL kinetics for the
<inline-formula><mml:math id="M268" 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:mo>+</mml:mo><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:math></inline-formula> reaction may overestimate <inline-formula><mml:math id="M269" 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> loss at cold temperatures
(Amedro et al., 2019).</p>
      <p id="d1e3531">We conclude that the sustained 2005–2017 decrease in US <inline-formula><mml:math id="M270" 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> emissions
reported by the EPA is supported by observations and that better
understanding of the free tropospheric background is needed to interpret
satellite observations of <inline-formula><mml:math id="M271" 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> tropospheric columns in terms of their
implications for <inline-formula><mml:math id="M272" 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> emissions and their trends. The concern is minor
in highly polluted areas where <inline-formula><mml:math id="M273" 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> emissions are sufficiently high to
dominate over the background influence. In the US, however, <inline-formula><mml:math id="M274" 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>
emissions have now decreased to the point that <inline-formula><mml:math id="M275" 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> columns over
nonurban areas are mostly contributed by the free tropospheric background.
Accounting for this poorly understood background will become increasingly
important as <inline-formula><mml:math id="M276" 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> emissions continue to decrease in the developed world
and in tropical regions that are undergoing rapid development but have a
deep troposphere and intense lightning.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e3616">OMI <inline-formula><mml:math id="M277" 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> observations are available from <uri>https://mirador.gsfc.nasa.gov/</uri> (last access: 31 January 2019).</p>

      <p id="d1e3633">AQS <inline-formula><mml:math id="M278" 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 ozone observations are available from <uri>https://www.epa.gov/aqs</uri>  (last access: 4 September 2018).</p>

      <p id="d1e3650">SEARCH <inline-formula><mml:math id="M279" 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> observations are available from <uri>https://www.dropbox.com/sh/o9hxoa4wlo97zpe/AACbm6LetQowrpUgX4vUxnoDa?dl=0</uri>  (last access: 27 July 2018).</p>

      <p id="d1e3667">NADP nitrate wet deposition observations are available from <uri>https://nadp.slh.wisc.edu/data/NTN/</uri>  (last access: 14 August 2018).</p>

      <p id="d1e3673">CASTNET ozone observations are available from <uri>https://www.epa.gov/castnet</uri>  (last access: 27 July 2018).</p>

      <p id="d1e3680">GEOS-Chem output from this work is available upon request.</p>
  </notes><?xmltex \hack{\clearpage}?><app-group>

<?pagebreak page8872?><app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title>The GEOS-Chem model</title>
      <p id="d1e3694">We conducted a 13-year simulation (2005–2017) with the GEOS-Chem global 3-D
chemical transport model version 11-02c (<uri>http://www.geos-chem.org</uri>, last access: 14 August 2018) using NASA MERRA-2 assimilated meteorological
data (Gelaro et al., 2017). We use the nested North American version of
GEOS-Chem at the native MERRA-2 0.5<inline-formula><mml:math id="M280" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M281" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M282" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
horizontal resolution over North America and adjacent oceans
(10–70<inline-formula><mml:math id="M283" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 140–40<inline-formula><mml:math id="M284" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W) with dynamic boundary conditions
from a global simulation with 4<inline-formula><mml:math id="M285" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M286" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 5<inline-formula><mml:math id="M287" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
horizontal resolution. The simulation includes detailed
<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>–hydrocarbon–aerosol chemistry as described in Travis et al. (2016),
Fisher et al. (2016) and Marais et al. (2016). US anthropogenic emissions
are distributed spatially following the NEI2011 inventory (EPA, 2018).
NEI2011 is scaled for individual years using national annual totals (EPA,
2018), and we decrease non-EGU <inline-formula><mml:math id="M289" 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> emissions by 60 %, as in Travis et
al. (2016), for all years. Open fire emissions are from the daily Quick Fire
Emissions Database (QFED; Darmenov and da Silva, 2013) with diurnal
variability from the Western Regional Air Partnership (Air Sciences, 2005).
Soil <inline-formula><mml:math id="M290" 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> emissions, including emissions from fertilizer application,
are computed according to Hudman et al. (2012), with a 50 % reduction in
the midwestern US for summertime based on a previous comparison with OMI
<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> observations (Vinken et al., 2014). Lightning <inline-formula><mml:math id="M292" 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> emissions
are described by Murray et al. (2012) with a horizontal distribution
matching climatological observations of lightning flashes, interannual
variability driven by MERRA-2 convection, and most of the release at the top
of convective updrafts (Ott et al., 2010). The <inline-formula><mml:math id="M293" 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> yield per flash is
260 mol to the south of 35<inline-formula><mml:math id="M294" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and 500 mol to the north (Hudman et
al., 2007; Huntrieser et al., 2008, 2009; Ott et al., 2010; Travis et al.,
2016).</p>
      <p id="d1e3845">The GEOS-Chem simulation of <inline-formula><mml:math id="M295" 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 related species over the US has
been evaluated in a number of recent papers including Zhang et al. (2012),
Ellis et al. (2013), and Lee et al. (2016) for nitrogen deposition; Travis
et al. (2016) for <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> concentrations over the southeastern US during the
SEAC<inline-formula><mml:math id="M297" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula>RS campaign; Fisher et al. (2016) for organic nitrates during that
same campaign; Jaeglé et al. (2018) for the WINTER campaign; and Fischer
et al. (2014) for the ensemble of PAN observations. These evaluations find
that the model is overall successful with no indication of systematic bias.</p><?xmltex \hack{\clearpage}?>
</app>
  </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e3884">DJJ, LJM, and RFS designed the study. RFS and MPS
conducted model simulations. RFS analyzed satellite, surface, and model
data. KRT contributed NEI emissions in GEOS-Chem and supported data
analysis. LJM, EAM, RCC, and JLL helped with scientific interpretation and
discussion. SC, JJ, and LNL provided OMI data and supporting guidance. RFS
and DJJ wrote the manuscript and all authors provided input on the paper for
revision before submission.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3890">The authors declare that they have no conflict of interest.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e3896">This study's contents are solely the responsibility of the grantee and do
not necessarily represent the official views of the US EPA. Further, US EPA
does not endorse the purchase of any commercial products or services
mentioned in the publication.</p>
  </notes><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e3902">This research has been supported by the US Environmental Protection Agency (grant no. 83587201). Daniel J. Jacob was supported by the NASA Earth Science
Division.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3909">This paper was edited by Qiang Zhang and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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    <!--<article-title-html>Using satellite observations of tropospheric NO<sub>2</sub> columns to infer long-term trends in US NO<sub><i>x</i></sub> emissions: the importance of accounting for the free tropospheric NO<sub>2</sub> background</article-title-html>
<abstract-html><p>The National Emission Inventory (NEI) of the US Environmental
Protection Agency (EPA) reports a steady decrease in US NO<sub><i>x</i></sub> emissions
over the 2005–2017 period at a rate of 0.1&thinsp;Tg&thinsp;N&thinsp;a<sup>−1</sup> (53&thinsp;% decrease
over the period), reflecting sustained efforts to improve air quality.
Tropospheric NO<sub>2</sub> columns observed by the satellite-based Ozone
Monitoring Instrument (OMI) over the US show a steady decrease until 2009
but a flattening afterward, which has been attributed to a flattening of
NO<sub><i>x</i></sub> emissions, contradicting the NEI. We show here that the
steady 2005–2017 decrease in NO<sub><i>x</i></sub> emissions reported by the NEI is in
fact largely consistent with observed network trends of surface NO<sub>2</sub> and
ozone concentrations. The OMI NO<sub>2</sub> trend is instead similar to that
observed for nitrate wet deposition fluxes, which is weaker than that for
anthropogenic NO<sub><i>x</i></sub> emissions, due to a large and increasing relative
contribution of non-anthropogenic background sources of NO<sub><i>x</i></sub> (mainly
lightning and soils). This is confirmed by contrasting OMI NO<sub>2</sub> trends
in urban winter, where the background is low and OMI NO<sub>2</sub> shows a
2005–2017 decrease consistent with the NEI, and rural summer, where the
background is high and OMI NO<sub>2</sub> shows no significant 2005–2017 trend. A
GEOS-Chem model simulation driven by NEI emission trends for the 2005–2017
period reproduces these different trends, except for the post-2009 flattening
of OMI NO<sub>2</sub>, which we attribute to a model underestimate of free
tropospheric NO<sub>2</sub>. Better understanding is needed of the factors
controlling free tropospheric NO<sub>2</sub> in order to relate satellite
observations of tropospheric NO<sub>2</sub> columns to the underlying NO<sub><i>x</i></sub>
emissions and their trends. Focusing on urban winter conditions in the
satellite data minimizes the effect of this free tropospheric background.</p></abstract-html>
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