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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ESSD</journal-id><journal-title-group>
    <journal-title>Earth System Science Data</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ESSD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Earth Syst. Sci. Data</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1866-3516</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/essd-13-2995-2021</article-id><title-group><article-title>Catalog of <inline-formula><mml:math id="M1" 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 point sources as derived from the divergence of the <inline-formula><mml:math id="M2" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> flux for TROPOMI</article-title><alt-title>Catalog of <inline-formula><mml:math id="M3" 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> point sources</alt-title>
      </title-group><?xmltex \runningtitle{Catalog of {$\chem{NO_{\mathit{x}}}$} point sources}?><?xmltex \runningauthor{S. Beirle et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Beirle</surname><given-names>Steffen</given-names></name>
          <email>steffen.beirle@mpic.de</email>
        <ext-link>https://orcid.org/0000-0002-7196-0901</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Borger</surname><given-names>Christian</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1128-3718</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Dörner</surname><given-names>Steffen</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5049-5692</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Eskes</surname><given-names>Henk</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8743-4455</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Kumar</surname><given-names>Vinod</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8405-3470</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>de Laat</surname><given-names>Adrianus</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Wagner</surname><given-names>Thomas</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Satellitenfernerkundung, Max-Planck-Institut für Chemie (MPI-C), Mainz, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Satellite Observations Department, Royal Netherlands Meteorological Institute (KNMI),<?xmltex \hack{\break}?> De Bilt, the Netherlands</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Steffen Beirle (steffen.beirle@mpic.de)</corresp></author-notes><pub-date><day>24</day><month>June</month><year>2021</year></pub-date>
      
      <volume>13</volume>
      <issue>6</issue>
      <fpage>2995</fpage><lpage>3012</lpage>
      <history>
        <date date-type="received"><day>17</day><month>September</month><year>2020</year></date>
           <date date-type="rev-request"><day>11</day><month>February</month><year>2021</year></date>
           <date date-type="rev-recd"><day>16</day><month>May</month><year>2021</year></date>
           <date date-type="accepted"><day>22</day><month>May</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2021 Steffen Beirle et al.</copyright-statement>
        <copyright-year>2021</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://essd.copernicus.org/articles/essd-13-2995-2021.html">This article is available from https://essd.copernicus.org/articles/essd-13-2995-2021.html</self-uri><self-uri xlink:href="https://essd.copernicus.org/articles/essd-13-2995-2021.pdf">The full text article is available as a PDF file from https://essd.copernicus.org/articles/essd-13-2995-2021.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e177">We present version 1.0 of a global catalog of <inline-formula><mml:math id="M4" 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 point sources, derived from TROPOspheric Monitoring Instrument (TROPOMI) measurements of tropospheric <inline-formula><mml:math id="M5" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> for 2018–2019.
The identification of sources and quantification of emissions are based on the divergence (spatial derivative) of the mean horizontal flux, which is highly sensitive for point sources like power plant exhaust stacks.</p>
    <p id="d1e202">The catalog lists 451 locations which could be clearly identified as <inline-formula><mml:math id="M6" 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> point sources by a fully automated algorithm, while ambiguous cases as well as area sources such as megacities are skipped.
A total of 242 of these point sources could be automatically matched to power plants.
Other <inline-formula><mml:math id="M7" 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> point sources listed in the catalog are metal smelters, cement plants, or industrial areas.
The four largest localized <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> emitters are all coal combustion plants in South Africa. About <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> of all detected point sources are located in the Indian subcontinent and are mostly associated with power plants.</p>
    <p id="d1e250">The catalog is incomplete, mainly due to persisting gaps in the TROPOMI <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> product at some coastlines, inaccurate or complex wind fields in coastal and mountainous regions, and high noise in the divergence maps for high background pollution.
The derived emissions are generally too low, lacking a factor of about 2 up to 8 for extreme cases.
This strong low bias results from combination of different effects, most of all a strong underestimation of near-surface <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> in TROPOMI <inline-formula><mml:math id="M12" 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.</p>
    <p id="d1e286">Still, the catalog has high potential for checking and improving emission inventories, as it provides accurate and independent up-to-date information on the location of 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> and thus also <inline-formula><mml:math id="M14" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
    <p id="d1e311">The catalog of <inline-formula><mml:math id="M15" 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 point sources is freely available at <uri>https://doi.org/10.26050/WDCC/Quant_NOx_TROPOMI</uri> <xref ref-type="bibr" rid="bib1.bibx4" id="paren.1"/>.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e340">Nitrogen oxides (<inline-formula><mml:math id="M16" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) are key species in air pollution and tropospheric chemistry <xref ref-type="bibr" rid="bib1.bibx27" id="paren.2"/>. For the prediction of air quality with regional atmospheric chemistry models, accurate and up-to-date <inline-formula><mml:math id="M17" 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 on high spatial resolution are essential <xref ref-type="bibr" rid="bib1.bibx5" id="paren.3"/>. Such data are often difficult to gain for countries with restrictive information policy. In addition, bottom-up emission inventories take several years to be compiled and are thus generally outdated for countries with quickly developing industrial activities.</p>
      <p id="d1e382">Spectrally resolved satellite measurements of solar backscattered radiation allow for the quantification of <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> and other trace gases absorbing in the UV–vis spectral range by their characteristic spectral absorption structures <xref ref-type="bibr" rid="bib1.bibx25 bib1.bibx26" id="paren.4"><named-content content-type="post">and references therein</named-content></xref>.
Tropospheric vertical column densities (TVCDs), i.e., concentrations of <inline-formula><mml:math id="M19" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> integrated vertically across the troposphere, can be derived by removing the stratospheric<?pagebreak page2996?> contribution and applying the so-called air mass factor (AMF)
that depends on the <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> profile shape as well as on viewing geometry, surface albedo, aerosols, and particularly on clouds.</p>
      <p id="d1e423"><inline-formula><mml:math id="M21" 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> TVCDs from satellite measurements provide independent information on the spatial distribution and strength of tropospheric <inline-formula><mml:math id="M22" 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> levels on a global scale since the mid-1990s, allowing for the identification of <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> sources and quantification of <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 <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx22 bib1.bibx23 bib1.bibx21 bib1.bibx24" id="paren.5"><named-content content-type="pre">e.g.,</named-content><named-content content-type="post">and references therein</named-content></xref>.</p>
      <p id="d1e476">In October 2017, the TROPOspheric Monitoring Instrument <xref ref-type="bibr" rid="bib1.bibx30" id="paren.6"><named-content content-type="pre">TROPOMI;</named-content></xref> was launched as a single payload of ESA's Sentinel-5 Precursor satellite mission. TROPOMI provides <inline-formula><mml:math id="M25" 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> TVCDs on unprecedented high spatial resolution (7.2 <inline-formula><mml:math id="M26" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.6 km<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> until 5 August 2019, 5.6 <inline-formula><mml:math id="M28" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.6 km<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> thereafter) and with a high signal-to-noise ratio <xref ref-type="bibr" rid="bib1.bibx28" id="paren.7"/>.
Single TROPOMI overpasses clearly reveal <inline-formula><mml:math id="M30" 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> plumes downwind from strong <inline-formula><mml:math id="M31" 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 like megacities <xref ref-type="bibr" rid="bib1.bibx20" id="paren.8"/> or large power plants  <xref ref-type="bibr" rid="bib1.bibx3" id="paren.9"/>.
In temporal mean <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> TVCDs, however, the high spatial resolution is partly lost due to
the averaging over plumes with different directions (related to the variability of atmospheric winds).</p>
      <p id="d1e572"><xref ref-type="bibr" rid="bib1.bibx3" id="text.10"/> thus proposed to average <inline-formula><mml:math id="M33" 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>  <italic>fluxes</italic> <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">F</mml:mi><mml:mo>=</mml:mo><mml:mi>V</mml:mi><mml:mi mathvariant="bold-italic">u</mml:mi></mml:mrow></mml:math></inline-formula>, i.e., TVCDs multiplied with horizontal wind components.
Upscaling <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> to <inline-formula><mml:math id="M36" 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 applying the continuity equation for steady state, this
directly allows for the quantification of <inline-formula><mml:math id="M37" 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 divergence, i.e., the spatial derivative of the mean <inline-formula><mml:math id="M38" 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> flux:
          <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M39" display="block"><mml:mrow><mml:mi>D</mml:mi><mml:mo>:=</mml:mo><mml:mi mathvariant="normal">∇</mml:mi><mml:mo>⋅</mml:mo><mml:mi mathvariant="bold-italic">F</mml:mi><mml:mo>=</mml:mo><mml:mi>E</mml:mi><mml:mo>-</mml:mo><mml:mi>S</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        with <inline-formula><mml:math id="M40" display="inline"><mml:mi mathvariant="bold-italic">F</mml:mi></mml:math></inline-formula> being the mean <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> flux, <inline-formula><mml:math id="M42" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> the <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 <inline-formula><mml:math id="M44" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> representing <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> sinks, i.e., the chemical loss of <inline-formula><mml:math id="M46" 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>.</p>
      <p id="d1e742">In <xref ref-type="bibr" rid="bib1.bibx3" id="text.11"/>, maps of <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">∇</mml:mi><mml:mo>⋅</mml:mo><mml:mi mathvariant="bold-italic">F</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mi>E</mml:mi><mml:mo>=</mml:mo><mml:mi>D</mml:mi><mml:mo>+</mml:mo><mml:mi>S</mml:mi></mml:mrow></mml:math></inline-formula> have been derived and
<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> emissions have been localized and quantified exemplarily for Riyadh, South Africa, and Germany. The sink term <inline-formula><mml:math id="M50" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> was estimated assuming a constant lifetime of <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> h, as derived from the downwind decay of <inline-formula><mml:math id="M52" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> for Riyadh <xref ref-type="bibr" rid="bib1.bibx2" id="paren.12"/>.
For spatially extended sources, like megacities such as Riyadh, <inline-formula><mml:math id="M53" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> contributes significantly to the derived emissions. For point sources, however, such as the large power plants around Riyadh, emissions are dominated (<inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">90</mml:mn></mml:mrow></mml:math></inline-formula> %) by the divergence term <inline-formula><mml:math id="M55" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> directly: point sources show up as distinct peaks in the divergence map, which are much sharper than the corresponding peaks in mean TVCD maps, as the <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> flux increases abruptly at the <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> sources, resulting in large values of flux derivatives.</p>
      <p id="d1e872">Here we extend this study to the global scale, with a particular focus on point sources.
Note that due to TROPOMI's spatial resolution of about 5 km, point sources could be individual facilities but also the merged emissions from industrial areas.
Point sources are identified and quantified based on peaks above local background in divergence maps <inline-formula><mml:math id="M58" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> directly rather than emission maps <inline-formula><mml:math id="M59" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula>, which allows for clearer identification of point source peaks, as well as for the classification of ambiguous cases by artifacts in <inline-formula><mml:math id="M60" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula>.</p>
      <p id="d1e896">As the calculation of <inline-formula><mml:math id="M61" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> from the derivative of mean fluxes requires gridding of TROPOMI data on high spatial resolution, the data processing on a global scale is demanding for I/O operations and working memory.
Thus, the analysis is only performed around stationary <inline-formula><mml:math id="M62" 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, which are defined based on the magnitude as well as the temporal variability of TROPOMI TVCDs.</p>
      <p id="d1e917">From the derived divergence maps, a catalog of <inline-formula><mml:math id="M63" 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> point sources is extracted by a fully automated algorithm.</p>
      <p id="d1e931">The paper is organized as follows:
in Sect. <xref ref-type="sec" rid="Ch1.S2"/>, the input datasets used in this study are specified.
The detailed data processing is explained in Sect. <xref ref-type="sec" rid="Ch1.S3"/>.
Section <xref ref-type="sec" rid="Ch1.S4"/> presents the <inline-formula><mml:math id="M64" 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> point source catalog.
In Sect. <xref ref-type="sec" rid="Ch1.S5"/>, the limitations and the potential of the catalog are discussed, followed by an outlook and conclusions.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Input data</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><?xmltex \opttitle{Tropospheric {$\protect\chem{NO_{2}}$} column densities}?><title>Tropospheric <inline-formula><mml:math id="M65" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> column densities</title>
      <p id="d1e980">The <inline-formula><mml:math id="M66" 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> point source catalog is based on <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> TVCDs
from TROPOMI for the years 2018–2019,
using the offline product (with successively increasing algorithm version from 0.11.0 on 1 January 2018 to 1.3.0 on 31 December 2019), as provided by KNMI/ESA via <uri>http://copernicus.eu</uri> (last access: 21 June 2021).
Details of the TROPOMI tropospheric <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> product are given in <xref ref-type="bibr" rid="bib1.bibx29" id="text.13"/> and <xref ref-type="bibr" rid="bib1.bibx28" id="text.14"/>.</p>
      <p id="d1e1026">TROPOMI is flying on a sun-synchronous orbit with a local overpass time of about 13:30. The pixel size at nadir was 7.2 km <inline-formula><mml:math id="M69" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.6 km initially and even improved to 5.6 km <inline-formula><mml:math id="M70" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.6 km from 6 August 2019 on <xref ref-type="bibr" rid="bib1.bibx28" id="paren.15"/>. TROPOMI provides daily global coverage, resulting in quite good statistics already for annual means.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Meteorological data</title>
      <p id="d1e1054">Horizontal wind fields <inline-formula><mml:math id="M71" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M72" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> as well as air pressure <inline-formula><mml:math id="M73" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> and air temperature <inline-formula><mml:math id="M74" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> are taken from reanalysis data from the European Centre for Medium-Range Weather Forecasts (ECMWF).
Wind fields are required for the calculation of fluxes. Pressure and temperature are needed for scaling <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> up to <inline-formula><mml:math id="M76" 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>, which involves (a) the reaction rate constant of <inline-formula><mml:math id="M77" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> as function of <inline-formula><mml:math id="M78" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> and (b) the conversion of climatological <inline-formula><mml:math id="M79" 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> mixing ratios to concentrations depending on <inline-formula><mml:math id="M80" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M81" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> (see Sect <xref ref-type="sec" rid="Ch1.S3.SS4"/>).</p>
      <p id="d1e1158">Until August 2019, ERA-Interim data are used with a truncation at T255, corresponding to <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution. Since September 2019, ERA-5 data are used with a truncation at T639, corresponding to <inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M85" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution <xref ref-type="bibr" rid="bib1.bibx13" id="paren.16"/>.
For both datasets, a preprocessed dataset was created<?pagebreak page2997?> where the 6-hourly model output (00:00, 06:00, 12:00, and 18:00 UTC) was interpolated to a regular horizontal grid with a resolution of 1<inline-formula><mml:math id="M86" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.
For future processing, sampling will be based on finer temporal and spatial grids.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Ozone climatology</title>
      <p id="d1e1217">Ozone mixing ratios, used for the scaling of <inline-formula><mml:math id="M87" 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 <inline-formula><mml:math id="M88" 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>,
were taken from the Earth System Chemistry integrated Modelling
(ESCiMo) project <xref ref-type="bibr" rid="bib1.bibx16" id="paren.17"/>, using the RC1SD-base-10a simulation for the years 2000–2010. The monthly mean climatology was calculated from the model fields sampled online along the overpass time of OMI aboard Aura (which is close to the TROPOMI overpass time) using the MESSy SORBIT submodel <xref ref-type="bibr" rid="bib1.bibx15" id="paren.18"/>.
As the divergence is sensitive for the added <inline-formula><mml:math id="M89" 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> at the source, the relevant <inline-formula><mml:math id="M90" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio is that close to ground. We thus took <inline-formula><mml:math id="M91" 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> concentrations from the lowest model layer.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Power plant database</title>
      <p id="d1e1297">The World Resources Institute provides an open-access Global Power Plant Database (GPPD) <xref ref-type="bibr" rid="bib1.bibx6" id="paren.19"/>.
We use this database (v1.2) in order to automatically identify <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> point sources corresponding to power plants.</p>
      <p id="d1e1314">The GPPD lists almost 30 000 power plants of all kinds, including solar, nuclear, and hydro power.
For our purpose, we created a subset of those power plants using coal, gas, or oil as primary fuel. In addition, power plants with capacities below 100 MW are skipped. The resulting subset of GPPD comprises 4654 power plants of which 2013, 2265, and 376 use coal, gas, and oil as primary fuel, respectively.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Data processing</title>
      <p id="d1e1326">In this section we describe the data processing step by step.
Table <xref ref-type="table" rid="Ch1.T1"/> summarizes the main steps and also lists similarities and differences to the procedure described in <xref ref-type="bibr" rid="bib1.bibx3" id="text.20"/>.</p>

<?xmltex \floatpos{p}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e1337">Processing settings in this study as compared to <xref ref-type="bibr" rid="bib1.bibx3" id="text.21"/>. </p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Section</oasis:entry>
         <oasis:entry colname="col2">Procedure</oasis:entry>
         <oasis:entry colname="col3">This study</oasis:entry>
         <oasis:entry colname="col4">
                  <xref ref-type="bibr" rid="bib1.bibx3" id="text.22"/>
                </oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1"><xref ref-type="sec" rid="Ch1.S3.SS1"/></oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M93" 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> selection</oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"><?xmltex \hack{\hspace*{2mm}}?>Quality/clouds</oasis:entry>
         <oasis:entry colname="col3">qa <inline-formula><mml:math id="M94" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.75, CF <inline-formula><mml:math id="M95" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.3</oasis:entry>
         <oasis:entry colname="col4">qa <inline-formula><mml:math id="M96" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.75, CF <inline-formula><mml:math id="M97" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"><?xmltex \hack{\hspace*{2mm}}?>Time period</oasis:entry>
         <oasis:entry colname="col3">2018–2019</oasis:entry>
         <oasis:entry colname="col4">Dec 2017–Oct 2018</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"><?xmltex \hack{\hspace*{2mm}}?>Seasons</oasis:entry>
         <oasis:entry colname="col3">SZA <inline-formula><mml:math id="M98" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 65<inline-formula><mml:math id="M99" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">April to October (Germany)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"><?xmltex \hack{\hspace*{2mm}}?>Regions</oasis:entry>
         <oasis:entry colname="col3">stationary sources within 61<inline-formula><mml:math id="M100" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S to 61<inline-formula><mml:math id="M101" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N</oasis:entry>
         <oasis:entry colname="col4">Riyadh, South Africa, Germany</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><xref ref-type="sec" rid="Ch1.S3.SS2"/></oasis:entry>
         <oasis:entry colname="col2">Grid</oasis:entry>
         <oasis:entry colname="col3">0.025<inline-formula><mml:math id="M102" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">0.027<inline-formula><mml:math id="M103" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><xref ref-type="sec" rid="Ch1.S3.SS3"/></oasis:entry>
         <oasis:entry colname="col2">Interpolated wind fields</oasis:entry>
         <oasis:entry colname="col3">300 m above ground</oasis:entry>
         <oasis:entry colname="col4">fixed vertical level at about 450 m</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><xref ref-type="sec" rid="Ch1.S3.SS4"/></oasis:entry>
         <oasis:entry colname="col2">[<inline-formula><mml:math id="M104" 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>] <inline-formula><mml:math id="M105" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> [<inline-formula><mml:math id="M106" 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>]</oasis:entry>
         <oasis:entry colname="col3">photo-stationary state</oasis:entry>
         <oasis:entry colname="col4">1.32 <inline-formula><mml:math id="M107" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 20 %</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><xref ref-type="sec" rid="Ch1.S3.SS5"/></oasis:entry>
         <oasis:entry colname="col2">Selection of fluxes</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mi>w</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> m s<inline-formula><mml:math id="M109" 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></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:mi>w</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> m s<inline-formula><mml:math id="M111" 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></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><xref ref-type="sec" rid="Ch1.S3.SS6"/></oasis:entry>
         <oasis:entry colname="col2">Background correction</oasis:entry>
         <oasis:entry colname="col3">none</oasis:entry>
         <oasis:entry colname="col4">5th percentile</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><xref ref-type="sec" rid="Ch1.S3.SS6"/></oasis:entry>
         <oasis:entry colname="col2">Lifetime correction</oasis:entry>
         <oasis:entry colname="col3">none</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> h</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"><xref ref-type="sec" rid="Ch1.S3.SS7"/></oasis:entry>
         <oasis:entry colname="col2">AMF correction</oasis:entry>
         <oasis:entry colname="col3">none</oasis:entry>
         <oasis:entry colname="col4">up to factor 2 for Germany</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><xref ref-type="sec" rid="Ch1.S3.SS8"/></oasis:entry>
         <oasis:entry colname="col2">Peak fit</oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"><?xmltex \hack{\hspace*{2mm}}?>Iteration</oasis:entry>
         <oasis:entry colname="col3">automated</oasis:entry>
         <oasis:entry colname="col4">semi-automated</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"><?xmltex \hack{\hspace*{2mm}}?>Pre-classification</oasis:entry>
         <oasis:entry colname="col3">multi-step</oasis:entry>
         <oasis:entry colname="col4">none</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"><?xmltex \hack{\hspace*{2mm}}?>Fit function</oasis:entry>
         <oasis:entry colname="col3">linear background <inline-formula><mml:math id="M113" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 2-D Gaussian</oasis:entry>
         <oasis:entry colname="col4">linear background <inline-formula><mml:math id="M114" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 2-D Gaussian <inline-formula><mml:math id="M115" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> rotation</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"><?xmltex \hack{\hspace*{2mm}}?>Peak removal</oasis:entry>
         <oasis:entry colname="col3">fitted peak <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> set to NaN</oasis:entry>
         <oasis:entry colname="col4">fitted peak subtracted</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

<sec id="Ch1.S3.SS1">
  <label>3.1</label><?xmltex \opttitle{{$\protect\chem{NO_{2}}$} selection}?><title><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> selection</title>
      <p id="d1e1863">For this study, we select TROPOMI tropospheric <inline-formula><mml:math id="M118" 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 densities <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><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:msub></mml:mrow></mml:math></inline-formula>
for the years 2018–2019 with values of the data quality indicator (“qa value”) above 0.75, as recommended in <xref ref-type="bibr" rid="bib1.bibx29" id="text.23"/>, and effective cloud fractions (CF) below 0.3. These selection criteria are the same as in <xref ref-type="bibr" rid="bib1.bibx3" id="text.24"/>.</p>
      <p id="d1e1898">In addition, we skip measurements with solar zenith angle (SZA) above 65<inline-formula><mml:math id="M120" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> for the calculation of fluxes. This strict criterion removes observations for sun being low and implicitly results in a gradual removal of wintertime measurements for midlatitudes, while in <xref ref-type="bibr" rid="bib1.bibx3" id="text.25"/>, winter months have been skipped explicitly for Germany.
Wintertime measurements are skipped in order to avoid unfavorable viewing conditions, snow-covered scenes, and stronger interference with aged plumes due to longer lifetimes.
Moreover, the SZA restriction allows us to simply parameterize the <inline-formula><mml:math id="M121" 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> photolysis as a function of the SZA (see Sect. <xref ref-type="sec" rid="Ch1.S3.SS4"/>).</p>
      <p id="d1e1926">Since large parts of the globe are free from stationary <inline-formula><mml:math id="M122" 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> point sources, in particular oceans, deserts, and forests, the processing focuses on potentially stationary sources. For this purpose, a selection mask is defined (Fig. <xref ref-type="fig" rid="Ch1.F1"/>), which is based on magnitude as well as the temporal variability of TROPOMI <inline-formula><mml:math id="M123" 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> TVCDs. The construction of the selection mask is explained in detail in the Supplement.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e1956"><bold>(a)</bold> Mean tropospheric <inline-formula><mml:math id="M124" 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 density for 2019.
<bold>(b)</bold> Mask <inline-formula><mml:math id="M125" display="inline"><mml:mi mathvariant="bold">M</mml:mi></mml:math></inline-formula> for the selection of pixels investigated in this study.
The construction of <inline-formula><mml:math id="M126" display="inline"><mml:mi mathvariant="bold">M</mml:mi></mml:math></inline-formula> is described in the Supplement. Boxes indicate the regions as defined in Table <xref ref-type="table" rid="Ch1.T2"/>.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://essd.copernicus.org/articles/13/2995/2021/essd-13-2995-2021-f01.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Grid</title>
      <p id="d1e2006">In order to have maximum sensitivity for point sources, the TROPOMI observations have to be oversampled, requiring a fine grid resolution of less than 3 km.
For each TROPOMI orbit, <inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><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:msub></mml:mrow></mml:math></inline-formula> is thus gridded to a regular longitude/latitude grid with 0.025<inline-formula><mml:math id="M128" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution for 61<inline-formula><mml:math id="M129" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S to 61<inline-formula><mml:math id="M130" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N.
Note that there are a few small <inline-formula><mml:math id="M131" 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 north of 61<inline-formula><mml:math id="M132" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, but due to the strict SZA threshold of 65<inline-formula><mml:math id="M133" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, the flux statistics would be poor for higher latitudes.</p>
      <p id="d1e2081">Gridding is done per orbit based on linear 2-D interpolation of TROPOMI pixel centers using the griddata function from the Python module SciPy <xref ref-type="bibr" rid="bib1.bibx32" id="paren.26"/>.
This approach allows for fast gridding.
In addition, there are no discontinuities at the TROPOMI pixel borders, which would lead to extremely high (positive and negative) values of the derivative.</p>
      <p id="d1e2087">All missing values (qa <inline-formula><mml:math id="M134" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.75) as well as the outermost pixels on each side of the TROPOMI swath (i.e., the pixels with the highest viewing zenith angles) are set to not a number (NaN). This is necessary in order to restrict the area of interpolated TVCDs to the actual area covered by measurements.</p>
      <p id="d1e2097">Hereafter we denote the longitude and latitude dimensions as <inline-formula><mml:math id="M135" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M136" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>, respectively, in vector indices as well as in the text.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Meteorological data</title>
      <p id="d1e2122">The meteorological datasets <inline-formula><mml:math id="M137" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M138" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M139" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M140" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> are extracted from ECMWF input data by linear interpolation in three steps:
<list list-type="order"><list-item>
      <p id="d1e2155"><italic>In vertical dimension to an altitude of 300 m above ground for each ECMWF input dataset with 6-hourly resolution.</italic> As emissions from point sources are the focus of this study, we consider wind fields representative for the transport of freshly released <inline-formula><mml:math id="M141" 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 stacks. The choice of altitude of wind fields is further discussed in Sect. <xref ref-type="sec" rid="Ch1.S5.SS2.SSS3"/>.
Only pixels with the mask <bold>M</bold> <inline-formula><mml:math id="M142" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 1 are extracted.</p></list-item><list-item>
      <?pagebreak page2999?><p id="d1e2184"><italic>In time dimension to the orbit time stamp of each TROPOMI orbit, as given in the orbit filename.</italic>
The actual TROPOMI overpass lags the orbit time stamp by about 33 and 67 min at 60<inline-formula><mml:math id="M143" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S and 60<inline-formula><mml:math id="M144" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N at solstice <inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula> min for summer/winter. Thus the orbit time stamp reflects the wind conditions for recent plume histories.</p></list-item><list-item>
      <p id="d1e2218"><italic>In horizontal dimensions (latitude, longitude) to the 0.025<inline-formula><mml:math id="M146" display="inline"><mml:msup><mml:mi/><mml:mo mathvariant="normal">∘</mml:mo></mml:msup></mml:math></inline-formula> grid.</italic></p></list-item></list></p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><?xmltex \opttitle{Upscaling of {$\protect\chem{NO_{2}}$} to {$\protect\chem{NO_{\mathit{x}}}$} }?><title>Upscaling of <inline-formula><mml:math id="M147" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M148" 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> </title>
      <p id="d1e2262">In this study we scale the measured <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> TVCD to a <inline-formula><mml:math id="M150" 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> TVCD for each TROPOMI pixel.
The conversion factor <inline-formula><mml:math id="M151" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> is calculated according to the photostationary steady state:
            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M152" display="block"><mml:mrow><mml:mi>L</mml:mi><mml:mo>:=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>[</mml:mo><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><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:mo>]</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><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><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:mo>]</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi>J</mml:mi><mml:mrow><mml:mi>k</mml:mi><mml:mo>[</mml:mo><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:mo>]</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p id="d1e2380">The impact of volatile organic compounds (VOCs) is neglected here as the focus is put on <inline-formula><mml:math id="M153" 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> point sources and thus generally high <inline-formula><mml:math id="M154" 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.</p>
      <p id="d1e2405">The photolysis frequency of <inline-formula><mml:math id="M155" 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="M156" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula> is parameterized as a function of the SZA <inline-formula><mml:math id="M157" display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula> by
            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M158" display="block"><mml:mrow><mml:mi>J</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.0167</mml:mn><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi>exp⁡</mml:mi><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.575</mml:mn><mml:mo>/</mml:mo><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:mrow></mml:math></disp-formula>
          as proposed by <xref ref-type="bibr" rid="bib1.bibx8" id="text.27"/>.
This parameterization is “accurate to about 10 % for mostly sunny conditions” for SZA <inline-formula><mml:math id="M159" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 65<inline-formula><mml:math id="M160" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx8" id="paren.28"/>.</p>
      <p id="d1e2497">The reaction rate constant <inline-formula><mml:math id="M161" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> for the reaction of NO with <inline-formula><mml:math id="M162" 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> is parameterized as a function of temperature (in kelvin) by
            <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M163" display="block"><mml:mrow><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.07</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:msup><mml:mo>×</mml:mo><mml:mi>exp⁡</mml:mi><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1400</mml:mn><mml:mo>/</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          following the recommendations from <xref ref-type="bibr" rid="bib1.bibx1" id="text.29"/> and <xref ref-type="bibr" rid="bib1.bibx14" id="text.30"/>.</p>
      <p id="d1e2565">Near-surface ozone mixing ratios are taken from a climatology based on the ESCiMo model simulation (Sect. <xref ref-type="sec" rid="Ch1.S2.SS3"/>) and converted into concentrations based on <inline-formula><mml:math id="M164" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M165" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> from ECMWF.</p>
      <p id="d1e2584">The derived values for <inline-formula><mml:math id="M166" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> represent conditions for near-surface pollution.
For background <inline-formula><mml:math id="M167" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the upper troposphere, the partitioning would be shifted towards NO.
However, any additive background is automatically removed by the calculation of the divergence.
Thus, the partitioning derived for near-surface concentrations is appropriate also for correcting the added column caused by a point source.</p>
      <p id="d1e2605">Figure <xref ref-type="fig" rid="Ch1.F2"/> displays the ratio of temporal means of <inline-formula><mml:math id="M168" 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 <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> TVCDs.
Global mean is 1.35 with a SD of 0.08.
Values for Riyadh, South Africa, and Germany are 1.22, 1.36, and 1.41, respectively, in agreement with the value of 1.32 <inline-formula><mml:math id="M170" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.26 applied in <xref ref-type="bibr" rid="bib1.bibx3" id="text.31"/>, which was based on the number given in <xref ref-type="bibr" rid="bib1.bibx27" id="text.32"/> for polluted conditions around noontime.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e2648">Effective <inline-formula><mml:math id="M171" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio, i.e., mean tropospheric <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> (as derived by assuming photostationary state according to Eq. <xref ref-type="disp-formula" rid="Ch1.E2"/> for each TROPOMI pixel) divided by the mean <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> column density for 2018–2019. Note that only cloud-free observations with SZA <inline-formula><mml:math id="M174" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 65<inline-formula><mml:math id="M175" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> are considered; thus wintertime measurements at mid- to high latitudes are skipped, and the expected latitudinal dependency of the <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:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio is suppressed. The spatial variability is a consequence of the dependency of the photostationary state on actinic flux, ozone concentration, and temperature (Eq. <xref ref-type="disp-formula" rid="Ch1.E2"/>).
</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://essd.copernicus.org/articles/13/2995/2021/essd-13-2995-2021-f02.png"/>

        </fig>

      <p id="d1e2737">Note that the actual [<inline-formula><mml:math id="M177" 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>] <inline-formula><mml:math id="M178" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> [<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>] ratio close to a point source might be different in the case of high NO concentrations causing <inline-formula><mml:math id="M180" 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> titration. In this case, however, the divergence method would detect the emitted <inline-formula><mml:math id="M181" 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> downwind from the source as soon as the NO is converted to <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> after mixing with ambient air. This results in a spatial smearing of the peak in the divergence map, leading to broader peaks, but the same integral (and thus emissions) for the peak fitting algorithm (Sect. <xref ref-type="sec" rid="Ch1.S3.SS8.SSS2"/>). For the final budget of <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> emissions, which are determined from the integrated peaks, the final photostationary state is thus still adequate.</p>
</sec>
<sec id="Ch1.S3.SS5">
  <label>3.5</label><title>Gridded fluxes and divergence</title>
      <p id="d1e2824">From gridded <inline-formula><mml:math id="M184" 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> columns and gridded wind fields, the gridded <inline-formula><mml:math id="M185" 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> flux in both the <inline-formula><mml:math id="M186" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M187" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> direction is derived for each TROPOMI orbit.
Mean fluxes are calculated for the period 2018–2019, where calm wind conditions (<inline-formula><mml:math id="M188" display="inline"><mml:mrow><mml:mi>w</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> m s<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>) are skipped. For grid pixels with less than 25 measurements, fluxes are set to missing values due to poor statistics.
Note that we do not explicitly skip winter months for midlatitudes, as in <xref ref-type="bibr" rid="bib1.bibx3" id="text.33"/> for Germany, but they are removed implicitly by the strict SZA threshold of 65<inline-formula><mml:math id="M190" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.</p>
      <p id="d1e2900">From the mean zonal and meridional flux maps, the divergence map <inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">∇</mml:mi><mml:mo>⋅</mml:mo><mml:mi mathvariant="bold-italic">F</mml:mi></mml:mrow></mml:math></inline-formula> is calculated, which is the basis for the identification and  quantification of point sources below.</p>
</sec>
<sec id="Ch1.S3.SS6">
  <label>3.6</label><title>Lifetime and background corrections</title>
      <p id="d1e2927">In <xref ref-type="bibr" rid="bib1.bibx3" id="text.34"/>, emission maps were derived by adding the sink term <inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:mi>S</mml:mi><mml:mo>=</mml:mo><mml:mi>V</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:math></inline-formula> to the divergence map. For this, a constant lifetime of <inline-formula><mml:math id="M193" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> h was applied, as derived from OMI data for Riyadh <xref ref-type="bibr" rid="bib1.bibx2" id="paren.35"/>. In addition, <inline-formula><mml:math id="M194" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> was corrected by subtracting the regional background, as the lifetime estimate was derived for freshly released, near-surface pollution, while upper-tropospheric background <inline-formula><mml:math id="M195" 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> generally has a longer lifetime.</p>
      <p id="d1e2983">As discussed in <xref ref-type="bibr" rid="bib1.bibx3" id="text.36"/>, the inclusion of the sink term has significant impact on area sources; it contributes about 50 % of integrated emissions for the Riyadh urban area.
For point sources, however, the emission signal is by far dominated by the divergence term, for instance accounting for 87 % of the emissions from power plant “PP9” in <xref ref-type="bibr" rid="bib1.bibx3" id="text.37"/>.</p>
      <p id="d1e2992">Within this study, we do not correct for the sink term <inline-formula><mml:math id="M196" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> for the following reasons:
<list list-type="bullet"><list-item>
      <p id="d1e3004">The <inline-formula><mml:math id="M197" 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 expected to be different for the diverse conditions in the considered regions, covering a large variability of temperature, humidity, actinic flux, VOC levels, and <inline-formula><mml:math id="M198" 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> levels. Note that the expected strong dependency of mean lifetime on latitude is again suppressed here due to the selection of SZA <inline-formula><mml:math id="M199" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 65<inline-formula><mml:math id="M200" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.</p></list-item><list-item>
      <?pagebreak page3000?><p id="d1e3046"><inline-formula><mml:math id="M201" 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> lifetimes simulated from global models cannot resolve the nonlinearities caused by point sources. In addition, emission inventories used as input to model runs generally have a time lag; thus emissions are outdated for quickly developing countries. Consequently, modeling the <inline-formula><mml:math id="M202" 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 for the investigated point sources is challenging and uncertain.</p></list-item><list-item>
      <p id="d1e3071">Identifying point sources in the divergence map <inline-formula><mml:math id="M203" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> directly is more immediate than in <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:mi>E</mml:mi><mml:mo>=</mml:mo><mml:mi>D</mml:mi><mml:mo>+</mml:mo><mml:mi>S</mml:mi></mml:mrow></mml:math></inline-formula>, as point sources reveal sharper peaks in <inline-formula><mml:math id="M205" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> than in <inline-formula><mml:math id="M206" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx3" id="paren.38"><named-content content-type="pre">Fig. 2 in</named-content></xref>. In addition, the identification of ambiguous candidates as, e.g., caused by inaccurate wind fields is clearer based on <inline-formula><mml:math id="M207" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> directly (Sect. <xref ref-type="sec" rid="Ch1.S3.SS8.SSS1"/>).</p></list-item></list></p>
      <p id="d1e3126">The resulting low bias of point source emissions caused by the missing lifetime correction is discussed in Sect. <xref ref-type="sec" rid="Ch1.S5.SS2.SSS2"/>.</p>
      <p id="d1e3132">Since no lifetime correction with <inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:mi>S</mml:mi><mml:mo>=</mml:mo><mml:mi>V</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:math></inline-formula> is performed, also the background correction for <inline-formula><mml:math id="M209" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>, which was performed in <xref ref-type="bibr" rid="bib1.bibx3" id="text.39"/> in order to exclude upper-tropospheric <inline-formula><mml:math id="M210" 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> with longer lifetime and different <inline-formula><mml:math id="M211" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula>, is omitted in the current study.
Note that the local background of <inline-formula><mml:math id="M212" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>, as well as any potential offset due to, e.g., stratospheric correction, would affect the lifetime correction but have no impact on <inline-formula><mml:math id="M213" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula>, as any additive term is lost by the calculation of the derivative.</p>
</sec>
<sec id="Ch1.S3.SS7">
  <label>3.7</label><title>AMF correction</title>
      <p id="d1e3202">Tropospheric column densities of <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> are derived from the total slant column by subtracting the stratospheric column and applying the so-called air mass factor (AMF). The AMF can be derived as the sum of height-dependent ”box AMFs”, representing the vertical measurement sensitivity, weighted by the relative profile <xref ref-type="bibr" rid="bib1.bibx33" id="paren.40"/>.
In the operational TROPOMI <inline-formula><mml:math id="M215" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> product, averaging kernels (AKs) are provided that are proportional to box AMFs and allow us to correct the AMF for a different vertical profile <xref ref-type="bibr" rid="bib1.bibx9" id="paren.41"/>.</p>
      <p id="d1e3233">Validation studies report on a general low bias 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> TVCD from TROPOMI of a factor of 2 and more for polluted sites <xref ref-type="bibr" rid="bib1.bibx31 bib1.bibx17" id="paren.42"><named-content content-type="pre">e.g., </named-content></xref>, caused by a high biased AMF. Part of this bias seems to be related to the a priori profiles which do not resolve the pollution profiles close to sources. In addition, there are indications that the cloud heights used for the TVCD retrieval are biased low <xref ref-type="bibr" rid="bib1.bibx7" id="paren.43"/> and the albedo maps used are biased high <xref ref-type="bibr" rid="bib1.bibx12" id="paren.44"/>, resulting in biased AKs.</p>
      <p id="d1e3258">In <xref ref-type="bibr" rid="bib1.bibx3" id="text.45"/>, an AMF correction was performed for South Africa and Germany by applying the provided AK to a near-surface profile.
In this study, we do not apply such an AMF correction,
as the effects of biased input albedo and cloud height cannot be corrected a posteriori based on the provided AKs but require a reprocessing of the TROPOMI <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> product.</p>
      <p id="d1e3275">Consequently, the low bias of TROPOMI TVCDs is directly transferred into the <inline-formula><mml:math id="M218" 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 listed in the catalog, as discussed in detail in Sect. <xref ref-type="sec" rid="Ch1.S5.SS2"/>.
The low bias is expected to be improved with an updated <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> product, which will then be used for deriving an updated version of the point source catalog.</p>
</sec>
<sec id="Ch1.S3.SS8">
  <label>3.8</label><title>Iterative peak fitting</title>
      <p id="d1e3311">We apply a fully automated iterative peak fitting algorithm in order to detect <inline-formula><mml:math id="M220" 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> point sources.
The goal is to identify clear point source peaks in the divergence map, where a robust quantification of emissions is possible, while ambiguous cases are skipped.
Thus, the resulting catalog of point sources is incomplete; a detailed discussion on various reasons for missing point sources is given in Sect. <xref ref-type="sec" rid="Ch1.S5.SS1"/>.
But the remaining point sources listed in the catalog correspond to actual <inline-formula><mml:math id="M221" 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 with high confidence.</p>
      <p id="d1e3338">In each iteration, the following procedure is executed:
<list list-type="order"><list-item>
      <?pagebreak page3001?><p id="d1e3343">The grid pixel with highest value of the divergence is considered the point source <italic>candidate</italic>.</p></list-item><list-item>
      <p id="d1e3350">Each candidate is classified into different categories and skipped if ambiguous (Sect. <xref ref-type="sec" rid="Ch1.S3.SS8.SSS1"/>).</p></list-item><list-item>
      <p id="d1e3356">For a promising candidate, a 2-D Gaussian is fitted to the divergence peak, and successful fits are included in the catalog (Sect. <xref ref-type="sec" rid="Ch1.S3.SS8.SSS2"/>).</p></list-item><list-item>
      <p id="d1e3362">The candidate is removed from the divergence map before searching for the next highest <inline-formula><mml:math id="M222" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> value (Sect. <xref ref-type="sec" rid="Ch1.S3.SS8.SSS3"/>).</p></list-item></list>
The iteration stops as soon as the maximum value of the divergence is less than 0.2 <inline-formula><mml:math id="M223" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M224" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M225" 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>, which is <inline-formula><mml:math id="M226" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> % of the initial maximum value of the first iteration. Below this threshold, almost no further point sources could be detected which meet the quality criteria listed below. For future versions, the availability of several years of TROPOMI data is expected to decrease the noise in divergence maps and will probably allow us to decrease this threshold and investigate additional small <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> point sources.</p>
<sec id="Ch1.S3.SS8.SSS1">
  <label>3.8.1</label><title>Pre-classification of candidates</title>
      <p id="d1e3436">Point source candidates are iteratively defined as the location of maximum divergence in the global map. Before fitting a Gaussian peak, and quantifying emissions, however, artifacts and ambiguous cases have to be excluded.</p>
      <p id="d1e3439">For this, a pre-classification is done based on the divergence map 30 km around the candidate. As soon as the candidate is classified as one of the following categories, the pre-classification stops.
In Fig. <xref ref-type="fig" rid="Ch1.F3"/>, examples for each category are shown.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e3446">Clippings of the mean divergence (2019–2020) showing examples for the different categories of point source candidates checked during pre-classification. White indicates missing data. The location of power plants from GPPD as well as cities is indicated by green markers.
<bold>(a)</bold> “Gap” candidate near Jebel Ali/Dubai. <bold>(b)</bold> “Negative” candidate near Tehran. <bold>(c)</bold> “Area source”  around Baghdad. <bold>(d)</bold> “Area source” candidate covering several power plants (with Vindhyachal and Anpara being the largest) in India.
</p></caption>
            <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/13/2995/2021/essd-13-2995-2021-f03.png"/>

          </fig>

      <p id="d1e3468"><list list-type="order">
              <list-item>

      <p id="d1e3473"><italic>Gap category.</italic>
If more than 25 % of grid pixels are missing within 8 km around the candidate, it is classified as “gap”.
Gaps were found primarily at sandy coastlines and are caused by persistent cloud coverage above threshold, which is probably an artifact of the coarse resolution of the albedo map used for the cloud retrieval.
In the later stage of the iteration, gaps also occur in the vicinity of strong point sources which have been already removed from the divergence map.
Figure <xref ref-type="fig" rid="Ch1.F3"/>a displays an example for a candidate of the gap category around Dubai, where the global maximum of divergence was found, but missing data do not allow for further quantifications.</p>
              </list-item>
              <list-item>

      <p id="d1e3483"><italic>Negative category.</italic>
If the minimum divergence within 30 km is negative with an absolute value larger than 50 % of the maximum value, the candidate is “negative”.</p>

      <p id="d1e3488">Negative values of the divergence generally indicate <inline-formula><mml:math id="M228" 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> sinks. Thus values of <inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> have to be expected downwind from sources. But absolute values should be far lower than the positive values at the place of emissions, as the <inline-formula><mml:math id="M230" 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> removal is taking place over large distances (at a wind speed of 5 m s<inline-formula><mml:math id="M231" 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>, a lifetime of 4 h corresponds to an <inline-formula><mml:math id="M232" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding distance of 72 km).</p>

      <p id="d1e3544">High absolute values of negative divergence thus cannot be explained by chemical loss of <inline-formula><mml:math id="M233" 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> (except for very short lifetimes) but indicate an inappropriate simplification of the complex 3-D wind fields by a 2-D wind vector on rather coarse spatial resolution.
Also changes of <inline-formula><mml:math id="M234" 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 or wind patterns on temporal scales of some hours
(whereas Eq. <xref ref-type="disp-formula" rid="Ch1.E1"/> assumes steady state, i.e., neglects the temporal derivative of <inline-formula><mml:math id="M235" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>)
can cause high negative values of <inline-formula><mml:math id="M236" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula>.</p>

      <p id="d1e3585">Figure <xref ref-type="fig" rid="Ch1.F3"/>b displays an example of high negative divergence around Tehran.
Obviously, the divergence method fails here, even though TVCDs show a hotspot of very high <inline-formula><mml:math id="M237" 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> around Tehran that can even be spotted in the global map (Fig. <xref ref-type="fig" rid="Ch1.F1"/>a).
The reason for the noisy divergence is the location of Tehran next to the Alborz mountains, where actual wind patterns are not described appropriately by the low-resolution wind fields.</p>
              </list-item>
              <list-item>

      <p id="d1e3606"><italic>Area source category.</italic>
If the candidate is neither classified as “gap” nor as “negative”,
sections of zonal and meridional means are calculated in order to allow for a quick check of the spatial extent
of the divergence peak.
For both sections, the full width at half maximum (FWHM) <inline-formula><mml:math id="M238" display="inline"><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mtext>first guess</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> is determined by checking for the first occurrence of a value below half of the maximum in both directions.
For point sources, a FWHM of about 12 km has been reported in <xref ref-type="bibr" rid="bib1.bibx3" id="text.46"/>.
Values of <inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mtext>first guess</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> above 17 km in both <inline-formula><mml:math id="M240" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M241" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> thus indicate a <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> source, which cannot be categorized as single point source, but an area source, which could be a large city or an extended industrial area with several point sources nearby.
Figure <xref ref-type="fig" rid="Ch1.F3"/>c and d display two examples for candidates classified as “area source”. Figure <xref ref-type="fig" rid="Ch1.F3"/>c shows the city of Baghdad.
In Fig. <xref ref-type="fig" rid="Ch1.F3"/>d, an “area source” consisting of several point sources close to each other is shown, primarily the coal-fired power plants Vindhyachal (5 MW) and Anpara (2 MW) in India.</p>
              </list-item>
            </list></p>
</sec>
<sec id="Ch1.S3.SS8.SSS2">
  <label>3.8.2</label><title>Gaussian fit</title>
      <?pagebreak page3002?><p id="d1e3678">If a candidate passes all pre-classification checks, a 2-D Gaussian on top of a linear background is fitted to the peak in the divergence map:
              <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M243" display="block"><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{9.2}{9.2}\selectfont$\displaystyle}?><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi>A</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">π</mml:mi><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mi>exp⁡</mml:mi><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>-</mml:mo><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>x</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mi>exp⁡</mml:mi><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>-</mml:mo><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>y</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>y</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mi>x</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mi>y</mml:mi><mml:mo>+</mml:mo><mml:mi>b</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable><?xmltex \hack{$\egroup}?></mml:mrow></mml:math></disp-formula>
            with the fit parameters <inline-formula><mml:math id="M244" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> being the peak integral;
<inline-formula><mml:math id="M245" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M246" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> being the width of the Gaussian;
<inline-formula><mml:math id="M247" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:math></inline-formula> being the shift of the peak maximum (relative to the first guess candidate location corresponding to the highest <inline-formula><mml:math id="M249" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> value); and
<inline-formula><mml:math id="M250" display="inline"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M251" display="inline"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M252" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> describing a linear background.</p>
      <p id="d1e3908">In contrast to <xref ref-type="bibr" rid="bib1.bibx3" id="text.47"/>, no rotation of the peak is allowed in order to make the fit fast and stable and in order to be able to interpret the widths
<inline-formula><mml:math id="M253" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> as actual distance in latitudinal and longitudinal dimensions.</p>
      <p id="d1e3930">The parameters are determined by a least-squares fit of <inline-formula><mml:math id="M254" display="inline"><mml:mi>G</mml:mi></mml:math></inline-formula> to the divergence map within 22 km around the candidate.
As starting values, <inline-formula><mml:math id="M255" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> are set to <inline-formula><mml:math id="M256" display="inline"><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mtext>first guess</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>/2.355 for both <inline-formula><mml:math id="M257" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M258" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>.
But since the fit yields a more robust measure of the peak width than the simple
FWHM estimate determined during pre-classification, the candidate is again classified as “area source”, if <inline-formula><mml:math id="M259" display="inline"><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mtext>fit</mml:mtext></mml:msub><mml:mo>:=</mml:mo><mml:mn mathvariant="normal">2.355</mml:mn><mml:mo>×</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> exceeds 17 km for <inline-formula><mml:math id="M260" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> or <inline-formula><mml:math id="M261" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>.</p>
      <p id="d1e4023">Otherwise, the candidate is considered to be a point source, where
the fitted parameter <inline-formula><mml:math id="M262" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> of the Gaussian peak represents the corresponding point source emissions.
However, in order to only keep robust emission estimates in the point source catalog, cases with emissions below 0.03 kg s<inline-formula><mml:math id="M263" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (which has been derived in <xref ref-type="bibr" rid="bib1.bibx3" id="altparen.48"/> as the detection limit for optimal conditions) or a relative fit error above 30 % are categorized as “uncertain”.</p>
</sec>
<sec id="Ch1.S3.SS8.SSS3">
  <label>3.8.3</label><title>Candidate removal</title>
      <p id="d1e4057">The candidate has to be removed from the global map before the next iteration step.
Removal is implemented by setting the divergence values around the maximum to NaN.
Note that in <xref ref-type="bibr" rid="bib1.bibx3" id="text.49"/> the fitted peaks were subtracted instead. However, this would introduce a highly structured residue in the divergence map, which would create several new artificial candidates for the fully automated peak search algorithm. Removing candidates by setting <inline-formula><mml:math id="M264" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> to NaN avoids such artificial point sources and prevents any later interferences from fit residues from neighboring sources.</p>
      <p id="d1e4070">Depending on the classification, the following procedure is applied:
<?xmltex \hack{\newpage}?>
<list list-type="bullet"><list-item>
      <p id="d1e4077">For point sources, an ellipse with 2<inline-formula><mml:math id="M265" display="inline"><mml:mrow><mml:mo>×</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> as a semi-major/minor axis is removed, with <inline-formula><mml:math id="M266" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> from the Gaussian fit.</p></list-item><list-item>
      <p id="d1e4115">For categories “gaps” and “uncertain”, all pixels within 22 km around the maximum are removed.</p></list-item><list-item>
      <p id="d1e4119">For category “negative”, a larger area (30 km around the maximum) is removed, as negative artifacts generally occur not at but next to the sources.</p></list-item><list-item>
      <p id="d1e4123">For area sources, also an area of 30 km around the maximum is removed, if classified based on <inline-formula><mml:math id="M267" display="inline"><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mtext>first guess</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>.
If the area source was classified based on <inline-formula><mml:math id="M268" display="inline"><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mtext>fit</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, an ellipse with 2<inline-formula><mml:math id="M269" display="inline"><mml:mrow><mml:mo>×</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is removed as for point sources.</p></list-item></list></p>
</sec>
</sec>
<sec id="Ch1.S3.SS9">
  <label>3.9</label><title>Identification of point sources associated with power plants</title>
      <p id="d1e4175">We perform an automated match of the point source catalog with the combustion power plants listed in GPPD.
For each point source, we search for GPPD entries within 5 km radius.
In the point source catalog, we add
<list list-type="bullet"><list-item>
      <p id="d1e4180">the integrated capacity of all power plants within 5 km,</p></list-item><list-item>
      <p id="d1e4184">a complete list of the names of all power plants within 5 km, and</p></list-item><list-item>
      <p id="d1e4188">the primary fuel of the power plant with highest capacity within 5 km.</p></list-item></list></p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Results</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Candidate classification</title>
      <p id="d1e4207">The iterative peak fitting algorithm yields 7250 candidates, of which 451 are classified as point sources.
For 242 of these point sources, a match with GPPD power plants was found.
Table <xref ref-type="table" rid="Ch1.T3"/> lists the classification statistics for the regions defined in Table <xref ref-type="table" rid="Ch1.T2"/>.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e4217">Definition of regions used for the regional statistics shown in Table <xref ref-type="table" rid="Ch1.T3"/> and for regional figures shown in the Supplement.
</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Label</oasis:entry>
         <oasis:entry colname="col2">Region<inline-formula><mml:math id="M271" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">Longitude [<inline-formula><mml:math id="M272" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E]</oasis:entry>
         <oasis:entry colname="col4">Latitude [<inline-formula><mml:math id="M273" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N]</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">NAm</oasis:entry>
         <oasis:entry colname="col2">North America</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M274" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">124</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M275" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">69</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">10 to 58</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SAm</oasis:entry>
         <oasis:entry colname="col2">South America</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M276" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">79</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M277" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">38</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M278" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M279" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Eur</oasis:entry>
         <oasis:entry colname="col2">Europe</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M280" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:math></inline-formula> to 25</oasis:entry>
         <oasis:entry colname="col4">36 to 61</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">WAf</oasis:entry>
         <oasis:entry colname="col2">West Africa</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M281" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">19</mml:mn></mml:mrow></mml:math></inline-formula> to 25</oasis:entry>
         <oasis:entry colname="col4">4 to 36</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SAf</oasis:entry>
         <oasis:entry colname="col2">South Africa</oasis:entry>
         <oasis:entry colname="col3">11 to 50</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M282" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">35</mml:mn></mml:mrow></mml:math></inline-formula> to 0</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">WRu</oasis:entry>
         <oasis:entry colname="col2">Western Russia/eastern Europe</oasis:entry>
         <oasis:entry colname="col3">25 to 75</oasis:entry>
         <oasis:entry colname="col4">45 to 61</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SbM</oasis:entry>
         <oasis:entry colname="col2">Siberia/Mongolia</oasis:entry>
         <oasis:entry colname="col3">75 to 123</oasis:entry>
         <oasis:entry colname="col4">45 to 61</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MdE</oasis:entry>
         <oasis:entry colname="col2">Middle East</oasis:entry>
         <oasis:entry colname="col3">25 to 63</oasis:entry>
         <oasis:entry colname="col4">7 to 45</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Ind</oasis:entry>
         <oasis:entry colname="col2">Indian subcontinent/western China</oasis:entry>
         <oasis:entry colname="col3">63 to 93</oasis:entry>
         <oasis:entry colname="col4">7 to 45</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Chn</oasis:entry>
         <oasis:entry colname="col2">East China/Southeast Asia</oasis:entry>
         <oasis:entry colname="col3">93 to 123</oasis:entry>
         <oasis:entry colname="col4">7 to 45</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">EAs</oasis:entry>
         <oasis:entry colname="col2">East Asia</oasis:entry>
         <oasis:entry colname="col3">123 to 145</oasis:entry>
         <oasis:entry colname="col4">30 to 58</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IdM</oasis:entry>
         <oasis:entry colname="col2">Indonesia/Malaysia</oasis:entry>
         <oasis:entry colname="col3">100 to 115</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M283" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">9</mml:mn></mml:mrow></mml:math></inline-formula> to 6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Aus</oasis:entry>
         <oasis:entry colname="col2">Australia</oasis:entry>
         <oasis:entry colname="col3">113 to 155</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M284" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M285" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NwZ</oasis:entry>
         <oasis:entry colname="col2">New Zealand</oasis:entry>
         <oasis:entry colname="col3">168 to 177</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">45</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M287" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">35</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e4222"><inline-formula><mml:math id="M270" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula> Note that the regions are defined such that all considered pixels are covered by a limited number of figures with similar area as far as feasible.
Region names are mostly based on continents. For Asia, regions are labeled after the countries dominating the detected point sources, gaining tangibility while condoning some inaccuracies in actual country borders.</p></table-wrap-foot></table-wrap>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3" specific-use="star"><?xmltex \currentcnt{3}?><label>Table 3</label><caption><p id="d1e4635">Number of candidates and their respective classification found for the regions defined in Table <xref ref-type="table" rid="Ch1.T2"/>.
The number of point sources in brackets refers to the point sources associated with power plants.
</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="8">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Label</oasis:entry>
         <oasis:entry colname="col2">Region</oasis:entry>
         <oasis:entry colname="col3">Candidates</oasis:entry>
         <oasis:entry colname="col4">Point source</oasis:entry>
         <oasis:entry colname="col5">Gap</oasis:entry>
         <oasis:entry colname="col6">Negative</oasis:entry>
         <oasis:entry colname="col7">Area</oasis:entry>
         <oasis:entry colname="col8">Uncertain</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">(power plant)</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
         <oasis:entry colname="col8"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">NAm</oasis:entry>
         <oasis:entry colname="col2">North America</oasis:entry>
         <oasis:entry colname="col3">880</oasis:entry>
         <oasis:entry colname="col4">47 (32)</oasis:entry>
         <oasis:entry colname="col5">171</oasis:entry>
         <oasis:entry colname="col6">601</oasis:entry>
         <oasis:entry colname="col7">41</oasis:entry>
         <oasis:entry colname="col8">20</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SAm</oasis:entry>
         <oasis:entry colname="col2">South America</oasis:entry>
         <oasis:entry colname="col3">172</oasis:entry>
         <oasis:entry colname="col4">8 (2)</oasis:entry>
         <oasis:entry colname="col5">32</oasis:entry>
         <oasis:entry colname="col6">117</oasis:entry>
         <oasis:entry colname="col7">11</oasis:entry>
         <oasis:entry colname="col8">4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Eur</oasis:entry>
         <oasis:entry colname="col2">Europe</oasis:entry>
         <oasis:entry colname="col3">1558</oasis:entry>
         <oasis:entry colname="col4">24 (11)</oasis:entry>
         <oasis:entry colname="col5">499</oasis:entry>
         <oasis:entry colname="col6">1013</oasis:entry>
         <oasis:entry colname="col7">20</oasis:entry>
         <oasis:entry colname="col8">2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">WAf</oasis:entry>
         <oasis:entry colname="col2">West Africa</oasis:entry>
         <oasis:entry colname="col3">116</oasis:entry>
         <oasis:entry colname="col4">19 (6)</oasis:entry>
         <oasis:entry colname="col5">30</oasis:entry>
         <oasis:entry colname="col6">54</oasis:entry>
         <oasis:entry colname="col7">10</oasis:entry>
         <oasis:entry colname="col8">3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SAf</oasis:entry>
         <oasis:entry colname="col2">South Africa</oasis:entry>
         <oasis:entry colname="col3">171</oasis:entry>
         <oasis:entry colname="col4">16 (9)</oasis:entry>
         <oasis:entry colname="col5">43</oasis:entry>
         <oasis:entry colname="col6">97</oasis:entry>
         <oasis:entry colname="col7">9</oasis:entry>
         <oasis:entry colname="col8">6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">WRu</oasis:entry>
         <oasis:entry colname="col2">Western Russia/eastern Europe</oasis:entry>
         <oasis:entry colname="col3">469</oasis:entry>
         <oasis:entry colname="col4">41 (23)</oasis:entry>
         <oasis:entry colname="col5">84</oasis:entry>
         <oasis:entry colname="col6">319</oasis:entry>
         <oasis:entry colname="col7">19</oasis:entry>
         <oasis:entry colname="col8">6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SbM</oasis:entry>
         <oasis:entry colname="col2">Siberia/Mongolia</oasis:entry>
         <oasis:entry colname="col3">186</oasis:entry>
         <oasis:entry colname="col4">9 (6)</oasis:entry>
         <oasis:entry colname="col5">45</oasis:entry>
         <oasis:entry colname="col6">123</oasis:entry>
         <oasis:entry colname="col7">5</oasis:entry>
         <oasis:entry colname="col8">4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MdE</oasis:entry>
         <oasis:entry colname="col2">Middle East</oasis:entry>
         <oasis:entry colname="col3">721</oasis:entry>
         <oasis:entry colname="col4">107 (40)</oasis:entry>
         <oasis:entry colname="col5">245</oasis:entry>
         <oasis:entry colname="col6">305</oasis:entry>
         <oasis:entry colname="col7">43</oasis:entry>
         <oasis:entry colname="col8">21</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Ind</oasis:entry>
         <oasis:entry colname="col2">India/Pakistan/western China</oasis:entry>
         <oasis:entry colname="col3">493</oasis:entry>
         <oasis:entry colname="col4">114 (76)</oasis:entry>
         <oasis:entry colname="col5">129</oasis:entry>
         <oasis:entry colname="col6">198</oasis:entry>
         <oasis:entry colname="col7">36</oasis:entry>
         <oasis:entry colname="col8">16</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Chn</oasis:entry>
         <oasis:entry colname="col2">East China/Southeast Asia</oasis:entry>
         <oasis:entry colname="col3">1766</oasis:entry>
         <oasis:entry colname="col4">34 (16)</oasis:entry>
         <oasis:entry colname="col5">678</oasis:entry>
         <oasis:entry colname="col6">1013</oasis:entry>
         <oasis:entry colname="col7">36</oasis:entry>
         <oasis:entry colname="col8">5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">EAs</oasis:entry>
         <oasis:entry colname="col2">East Asia</oasis:entry>
         <oasis:entry colname="col3">561</oasis:entry>
         <oasis:entry colname="col4">19 (10)</oasis:entry>
         <oasis:entry colname="col5">139</oasis:entry>
         <oasis:entry colname="col6">378</oasis:entry>
         <oasis:entry colname="col7">20</oasis:entry>
         <oasis:entry colname="col8">5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IdM</oasis:entry>
         <oasis:entry colname="col2">Indonesia/Malaysia</oasis:entry>
         <oasis:entry colname="col3">65</oasis:entry>
         <oasis:entry colname="col4">5 (4)</oasis:entry>
         <oasis:entry colname="col5">25</oasis:entry>
         <oasis:entry colname="col6">34</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
         <oasis:entry colname="col8">0</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Aus</oasis:entry>
         <oasis:entry colname="col2">Australia</oasis:entry>
         <oasis:entry colname="col3">66</oasis:entry>
         <oasis:entry colname="col4">7 (7)</oasis:entry>
         <oasis:entry colname="col5">16</oasis:entry>
         <oasis:entry colname="col6">34</oasis:entry>
         <oasis:entry colname="col7">7</oasis:entry>
         <oasis:entry colname="col8">2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NwZ</oasis:entry>
         <oasis:entry colname="col2">New Zealand</oasis:entry>
         <oasis:entry colname="col3">11</oasis:entry>
         <oasis:entry colname="col4">0 (0)</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">10</oasis:entry>
         <oasis:entry colname="col7">0</oasis:entry>
         <oasis:entry colname="col8">0</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Glb</oasis:entry>
         <oasis:entry colname="col2">Global</oasis:entry>
         <oasis:entry colname="col3">7250</oasis:entry>
         <oasis:entry colname="col4">451 (242)</oasis:entry>
         <oasis:entry colname="col5">2139</oasis:entry>
         <oasis:entry colname="col6">4308</oasis:entry>
         <oasis:entry colname="col7">258</oasis:entry>
         <oasis:entry colname="col8">94</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?pagebreak page3003?><p id="d1e5140">Figure <xref ref-type="fig" rid="Ch1.F4"/> displays regional maps of color-coded <inline-formula><mml:math id="M288" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> for selected regions. The respective maps for all regions listed in table <xref ref-type="table" rid="Ch1.T2"/> are provided in the Supplement in PDF format, allowing for loss-free zooming.</p>

      <?xmltex \floatpos{h}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e5156">Divergence <inline-formula><mml:math id="M289" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> (color coded) and point source classification (symbols) for <bold>(a)</bold> the Middle East, <bold>(b)</bold> India, <bold>(c)</bold> Europe, and <bold>(d)</bold> Ukraine/western Russia. Triangles display the point sources listed in the catalog, where matches to GPPD power plants are indicated in magenta.
Respective maps for all regions defined in Table <xref ref-type="table" rid="Ch1.T2"/> are provided in the Supplement (Figs. S2–S14).
Also for sake of clarity, non-point sources are only shown for candidates with <inline-formula><mml:math id="M290" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mtext>max</mml:mtext></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M291" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M292" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M293" 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 the integrated divergence within 30 km exceeding 0.1 kg s<inline-formula><mml:math id="M294" 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></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/13/2995/2021/essd-13-2995-2021-f04.png"/>

        </fig>

      <p id="d1e5246">The candidate classifications are indicated by symbols, where point sources with/without a power plant match are displayed as triangles in magenta/dark grey, respectively.
Non-point sources are shown in light grey. For sake of clarity, they are only displayed for high divergence values (<?xmltex \hack{\mbox\bgroup}?><inline-formula><mml:math id="M295" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mtext>max</mml:mtext></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M296" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M297" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M298" 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><?xmltex \hack{\egroup}?> or integrated <inline-formula><mml:math id="M299" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.1</mml:mn></mml:mrow></mml:math></inline-formula> kg s<inline-formula><mml:math id="M300" 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>), as they would otherwise dominate the figure for some regions like Europe, where 499 candidates are classified as “gap” and 1013 as “negative” (Table <xref ref-type="table" rid="Ch1.T3"/>).</p>
      <p id="d1e5324">The map of the Middle East (a) contains most of the non-point-source examples shown in Fig. <xref ref-type="fig" rid="Ch1.F3"/>. Several more gaps occur all along the Persian Gulf coastline, and further negative candidates are found in mountains as well as along the coastlines.</p>
      <p id="d1e5329">Several large cities like (a) Cairo and Jeddah, (b) Paris and Madrid, (c) Delhi and Mumbai, or (d) Moscow and Saint Petersburg are categorized as area source.
However, there are also some candidates categorized as area source which do not correspond to a megacity. In particular the candidate<?pagebreak page3004?> corresponding to the maximum divergence over India, which is caused by the coal-fired 5 GW Vindhyachal Super Thermal Power Station, was categorized as area source, as it interferes with the 4 GW Anpara power plant about 16 km northeast (Fig. <xref ref-type="fig" rid="Ch1.F3"/>d).
Such sources could still be investigated in detail based on the divergence map.
However, for interfering sources so close to each other, a quantification by a fully automated algorithm is challenging.</p>
      <p id="d1e5335">For Riyadh, the power plants PP9 and PP10 northeast and southeast of the city center are identified as point sources (compare <xref ref-type="bibr" rid="bib1.bibx3" id="altparen.50"/>). In contrast to <xref ref-type="bibr" rid="bib1.bibx3" id="text.51"/>, PP8 west of Riyadh is not identified as a point source as it could not be separated from Riyadh city, as a consequence of the strict pre-selection of candidates and the slightly larger fit interval, which were necessary in order to run the algorithm fully automated globally.</p>
      <p id="d1e5344">Several point sources are detected in the Middle East. There is a remarkable cluster of several point sources detected south of Baghdad. Note that there was even a point<?pagebreak page3005?> source detected within the Persian Gulf, which corresponds to the Zakum offshore oilfield.</p>
      <p id="d1e5347">The Indian subcontinent reveals the highest number of point sources of the investigated regions, contributing one-fourth of the global number.
This reflects the quickly growing industrial activities, while measures for emission reduction still need to catch up. In addition, the divergence method obviously works very well for India, as the noise in divergence is quite low. This might be related to the dry season providing very good observation conditions without gaps, thereby suppressing sampling effects (compare Sect. <xref ref-type="sec" rid="Ch1.S5.SS1.SSS1"/>).</p>
      <p id="d1e5352">In Europe, only very few point sources are detected, like the world's largest charcoal power plant Bełchatów in Poland; the German charcoal power plants  Jänschwalde, Boxberg, and Neurath/Niederaußem <xref ref-type="bibr" rid="bib1.bibx3" id="paren.52"><named-content content-type="pre">compare</named-content></xref>; or Europe's largest steel plant in Taranto, southern Italy.
Remarkably, almost no point sources are detected for England and the Benelux countries, where the mean TVCD has a local maximum (Fig. <xref ref-type="fig" rid="Ch1.F1"/>a).
Instead, there are several candidates classified as “gaps” and “negative”, which is related to the high noise observed in the divergence map. A similar situation is found for China, where TVCD is highest globally (Fig. <xref ref-type="fig" rid="Ch1.F1"/>a), but noise in <inline-formula><mml:math id="M301" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> is large (Fig. S11 in the Supplement) such that the number of negative candidates is high (1013), but only few (34) point sources could be clearly identified.
In Ukraine and western Russia, where mean TVCD levels are moderate, several point sources could be clearly identified. These striking regional differences in the performance of the automated point source detection will be discussed in detail in Sect. <xref ref-type="sec" rid="Ch1.S5.SS1"/>.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Catalog of point sources</title>
      <p id="d1e5381">We derive a global catalog of <inline-formula><mml:math id="M302" 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 451 peaks categorized as point sources by sorting them according to the fitted emissions.
A complete list of all detected point sources, including latitude/longitude and the estimated emissions, is provided in CSV format at  <uri>https://doi.org/10.26050/WDCC/Quant_NOx_TROPOMI</uri> <xref ref-type="bibr" rid="bib1.bibx4" id="paren.53"/> and also added as a data file to the Supplement.</p>
      <p id="d1e5401">Table <xref ref-type="table" rid="Ch1.T4"/> lists a selection of the identified point sources with some additional information on the respective <inline-formula><mml:math id="M303" 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> source. It contains the top 10 emitters of the catalog. In addition, every 100th rank is included in order to illustrate conditions for lower divergence levels.
Divergence maps for the same selection are shown in Fig. <xref ref-type="fig" rid="Ch1.F5"/>, where also external information on <inline-formula><mml:math id="M304" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> sources have been added. In the Supplement, respective divergence maps and tables of regional top emitters are shown for all considered regions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e5432">Divergence maps for the selected point sources listed in Table <xref ref-type="table" rid="Ch1.T4"/>. In addition to the location of the fitted Gaussian peak (grey), also some external information on GPPD power plants as well as industrial facilities and cities is added (green).
</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/13/2995/2021/essd-13-2995-2021-f05.png"/>

        </fig>

      <p id="d1e5444">Most of the point sources listed in Table <xref ref-type="table" rid="Ch1.T4"/> can actually be associated with single or groups of power plants.
Overall, a GPPD match was found for 242 point sources. The median distance between GPPD and point source locations was found to be 1.6 km, which is better than TROPOMI resolution.
For the selection in Table <xref ref-type="table" rid="Ch1.T4"/>, we did some additional inquiry and could identify the power plants Medupi (no. 3) and Presidente Vargas (no. 300), both missing in GPPD, as probable <inline-formula><mml:math id="M305" 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.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T4" specific-use="star"><?xmltex \currentcnt{4}?><label>Table 4</label><caption><p id="d1e5465">Extract of the point source catalog for the top 10 and every 100th rank.
Power plant capacity, fuel type, and facility names are added for matches to GPPD.
The last two columns are not part of the catalog but have been added manually for the presented selection in order to provide information on the likely <inline-formula><mml:math id="M306" 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> source where no (or insignificant) GPPD match has been found.
Divergence maps for the same selection are displayed in Fig. <xref ref-type="fig" rid="Ch1.F5"/>.
As discussed in detail in Sect. <xref ref-type="sec" rid="Ch1.S5.SS2.SSS6"/>, the given emissions are biased low.
Respective tables for regional top emitters are listed in the Supplement for all considered regions.
</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="9">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="center"/>
     <oasis:colspec colnum="7" colname="col7" align="left" colsep="1"/>
     <oasis:colspec colnum="8" colname="col8" align="left"/>
     <oasis:colspec colnum="9" colname="col9" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col7" align="center" colsep="1">From point source catalog </oasis:entry>
         <oasis:entry namest="col8" nameend="col9" align="center">Additional Information </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Rank</oasis:entry>
         <oasis:entry colname="col2">Lat</oasis:entry>
         <oasis:entry colname="col3">Long</oasis:entry>
         <oasis:entry colname="col4">Emissions</oasis:entry>
         <oasis:entry colname="col5">Capacity</oasis:entry>
         <oasis:entry colname="col6">Fuel<inline-formula><mml:math id="M310" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">Name(s)<inline-formula><mml:math id="M311" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">Country</oasis:entry>
         <oasis:entry colname="col9">Other sources</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">[<inline-formula><mml:math id="M312" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N]</oasis:entry>
         <oasis:entry colname="col3">[<inline-formula><mml:math id="M313" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E]</oasis:entry>
         <oasis:entry colname="col4">[kg s<inline-formula><mml:math id="M314" 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>]</oasis:entry>
         <oasis:entry colname="col5">[GW]</oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
         <oasis:entry colname="col8"/>
         <oasis:entry colname="col9"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">1</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M315" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">26.284</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">29.176</oasis:entry>
         <oasis:entry colname="col4">0.886</oasis:entry>
         <oasis:entry colname="col5">6.600</oasis:entry>
         <oasis:entry colname="col6">Coal</oasis:entry>
         <oasis:entry colname="col7">Matla; Kriel</oasis:entry>
         <oasis:entry colname="col8">South Africa</oasis:entry>
         <oasis:entry colname="col9"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M316" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">26.566</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">29.181</oasis:entry>
         <oasis:entry colname="col4">0.679</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
         <oasis:entry colname="col8">South Africa</oasis:entry>
         <oasis:entry colname="col9">Secunda CTL coal liquifier</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">3</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M317" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">23.686</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">27.594</oasis:entry>
         <oasis:entry colname="col4">0.669</oasis:entry>
         <oasis:entry colname="col5">3.990</oasis:entry>
         <oasis:entry colname="col6">Coal</oasis:entry>
         <oasis:entry colname="col7">Matimba</oasis:entry>
         <oasis:entry colname="col8">South Africa</oasis:entry>
         <oasis:entry colname="col9">Medupi power plant<inline-formula><mml:math id="M318" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">4</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M319" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">27.104</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">29.788</oasis:entry>
         <oasis:entry colname="col4">0.668</oasis:entry>
         <oasis:entry colname="col5">4.110</oasis:entry>
         <oasis:entry colname="col6">Coal</oasis:entry>
         <oasis:entry colname="col7">Majuba</oasis:entry>
         <oasis:entry colname="col8">South Africa</oasis:entry>
         <oasis:entry colname="col9"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">5</oasis:entry>
         <oasis:entry colname="col2">22.397</oasis:entry>
         <oasis:entry colname="col3">82.692</oasis:entry>
         <oasis:entry colname="col4">0.588</oasis:entry>
         <oasis:entry colname="col5">4.830</oasis:entry>
         <oasis:entry colname="col6">Coal</oasis:entry>
         <oasis:entry colname="col7">Korba</oasis:entry>
         <oasis:entry colname="col8">India</oasis:entry>
         <oasis:entry colname="col9"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">6</oasis:entry>
         <oasis:entry colname="col2">40.637</oasis:entry>
         <oasis:entry colname="col3">109.739</oasis:entry>
         <oasis:entry colname="col4">0.528</oasis:entry>
         <oasis:entry colname="col5">0.200</oasis:entry>
         <oasis:entry colname="col6">Coal</oasis:entry>
         <oasis:entry colname="col7">Baotou</oasis:entry>
         <oasis:entry colname="col8">China</oasis:entry>
         <oasis:entry colname="col9">Steel works</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">7</oasis:entry>
         <oasis:entry colname="col2">35.502</oasis:entry>
         <oasis:entry colname="col3">129.303</oasis:entry>
         <oasis:entry colname="col4">0.523</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
         <oasis:entry colname="col8">South Korea</oasis:entry>
         <oasis:entry colname="col9">Ulsan industrial area</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">8</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M320" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">26.777</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">29.379</oasis:entry>
         <oasis:entry colname="col4">0.474</oasis:entry>
         <oasis:entry colname="col5">3.654</oasis:entry>
         <oasis:entry colname="col6">Coal</oasis:entry>
         <oasis:entry colname="col7">Tutuka</oasis:entry>
         <oasis:entry colname="col8">South Africa</oasis:entry>
         <oasis:entry colname="col9"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">9</oasis:entry>
         <oasis:entry colname="col2">28.696</oasis:entry>
         <oasis:entry colname="col3">48.334</oasis:entry>
         <oasis:entry colname="col4">0.460</oasis:entry>
         <oasis:entry colname="col5">6.905</oasis:entry>
         <oasis:entry colname="col6">Gas</oasis:entry>
         <oasis:entry colname="col7">Az-Zour</oasis:entry>
         <oasis:entry colname="col8">Kuwait</oasis:entry>
         <oasis:entry colname="col9"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">10</oasis:entry>
         <oasis:entry colname="col2">34.930</oasis:entry>
         <oasis:entry colname="col3">127.723</oasis:entry>
         <oasis:entry colname="col4">0.460</oasis:entry>
         <oasis:entry colname="col5">1.330</oasis:entry>
         <oasis:entry colname="col6">Gas</oasis:entry>
         <oasis:entry colname="col7">Gwangyang</oasis:entry>
         <oasis:entry colname="col8">South Korea</oasis:entry>
         <oasis:entry colname="col9">Steel works</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">100</oasis:entry>
         <oasis:entry colname="col2">29.009</oasis:entry>
         <oasis:entry colname="col3">31.216</oasis:entry>
         <oasis:entry colname="col4">0.151</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
         <oasis:entry colname="col8">Egypt</oasis:entry>
         <oasis:entry colname="col9">Cement plant</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">200</oasis:entry>
         <oasis:entry colname="col2">44.669</oasis:entry>
         <oasis:entry colname="col3">89.089</oasis:entry>
         <oasis:entry colname="col4">0.093</oasis:entry>
         <oasis:entry colname="col5">7.000</oasis:entry>
         <oasis:entry colname="col6">Coal</oasis:entry>
         <oasis:entry colname="col7">Wucaiwan</oasis:entry>
         <oasis:entry colname="col8">China</oasis:entry>
         <oasis:entry colname="col9"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">300</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M321" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">22.537</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M322" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">44.121</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">0.062</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
         <oasis:entry colname="col8">Brazil</oasis:entry>
         <oasis:entry colname="col9">Presidente Vargas power plant<inline-formula><mml:math id="M323" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">400</oasis:entry>
         <oasis:entry colname="col2">29.099</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M324" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">110.988</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">0.040</oasis:entry>
         <oasis:entry colname="col5">0.250</oasis:entry>
         <oasis:entry colname="col6">Gas</oasis:entry>
         <oasis:entry colname="col7">Hermosillo</oasis:entry>
         <oasis:entry colname="col8">Mexico</oasis:entry>
         <oasis:entry colname="col9">City of Hermosillo</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e5483"><inline-formula><mml:math id="M307" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula> Primary fuel of the GPPD match with highest capacity within 5 km.<?xmltex \hack{\\}?><inline-formula><mml:math id="M308" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> GPPD names have been shortened.<?xmltex \hack{\\}?><inline-formula><mml:math id="M309" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> Missing in GPPD.</p></table-wrap-foot></table-wrap>

      <p id="d1e6155">Other point sources are the Secunda CTL coal liquifying facility (no. 2), steel work facilities (no. 6, no. 10), and a cement plant (no. 100).
Point source no. 7 is located in Ulsan, an industrial hotspot in South Korea. Here, however, we could not identify a single dominating <inline-formula><mml:math id="M325" 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> point source.
For the Hermosillo power plant, the peak fit is probably affected by Hermosillo city nearby (0.7 million inhabitants).</p>
      <p id="d1e6169">The four highest point source <inline-formula><mml:math id="M326" 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 all found for South African coal power plants, which have already been presented in <xref ref-type="bibr" rid="bib1.bibx3" id="text.54"/>. Note that the emissions in Table <xref ref-type="table" rid="Ch1.T4"/> are lower than those given in <xref ref-type="bibr" rid="bib1.bibx3" id="text.55"/> for various reasons, as discussed in detail in Sect. <xref ref-type="sec" rid="Ch1.S5.SS2.SSS6"/>, mainly due to the missing AMF and lifetime corrections in the current study.</p>
      <p id="d1e6193">The thresholds for artifacts in divergence have been defined rather strictly. Consequently, the remaining locations listed in the catalog actually indicate stationary <inline-formula><mml:math id="M327" 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.
In the spot tests investigated exemplarily, we found no indication for false signals in the catalog.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Comparison to power plant database</title>
      <p id="d1e6215">Figure <xref ref-type="fig" rid="Ch1.F6"/>a provides a scatter plot of power plant capacity and point source emissions.
Respective regional figures for all considered regions are provided in Fig. S15 in the Supplement.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e6222">Correlation between point source emissions and power plant capacity. <bold>(a)</bold> Scatter plot for all matches globally, with color coding primary fuel. <bold>(b)</bold> Scatter plot for coal-fired power plants in Australia, Europe, and South Africa.
</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://essd.copernicus.org/articles/13/2995/2021/essd-13-2995-2021-f06.png"/>

        </fig>

      <p id="d1e6237">Note that a perfect correlation between power plant capacity and <inline-formula><mml:math id="M328" 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 cannot be expected, as the emissions per capacity strongly depend on fuel type and technology and are particularly modified if emission control measures like selective catalytic reduction (SCR) are applied.
High emissions for power plants with low capacity probably indicate other dominating <inline-formula><mml:math id="M329" 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 nearby, like for Baotou (no. 6), where a 0.2 GW power plant was matching the point source location, but emissions are probably mainly caused by the metal smelting facilities.
Low emissions from high-capacity power plants probably indicate the installation of SCR or a recent reduction in capacity.</p>
      <p id="d1e6263">High correlations can be observed for some regions like South Africa and Australia. This is probably indicating that the GPPD entries are reliable for these regions, the level of power plant technology is regionally similar, and the divergence method works well here. Figure <xref ref-type="fig" rid="Ch1.F6"/>b displays the scatter plots for coal-fired power plants for Australia, Europe, and South Africa. The slopes indicate clear regional differences in the emissions-per-capacity ratio.</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Discussion</title>
      <?pagebreak page3007?><p id="d1e6278">In this section we discuss the limitations as well as the potential of the presented point source catalog, give an outline on possible applications, and an outlook on improvements of the catalog in a future update.</p>
<sec id="Ch1.S5.SS1">
  <label>5.1</label><title>Limitations</title>
      <p id="d1e6288">When interpreting the presented point source catalog, the following limitations have to be kept in mind.</p>
<sec id="Ch1.S5.SS1.SSS1">
  <label>5.1.1</label><title>Missing point sources</title>
      <p id="d1e6298">The catalog is incomplete, as point sources might be missing due to the following reasons:
<list list-type="order"><list-item>
      <p id="d1e6303"><italic>Considered pixels.</italic>
Only latitudes between 61<inline-formula><mml:math id="M330" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N/S are considered, as for higher latitudes, the strict SZA threshold of 65<inline-formula><mml:math id="M331" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> would result in poor statistics.
In addition, the criteria for defining the selection mask are quite strict in order to reduce the amount of data to be processed. There might thus be <inline-formula><mml:math id="M332" 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> point sources not included in the selection mask. However, based on maps of the mean TVCD, we see no indication for strong point sources outside the considered area defined by <bold>M</bold>
(compare Fig. <xref ref-type="fig" rid="Ch1.F1"/>a and b).</p></list-item><list-item>
      <p id="d1e6343"><italic>Gaps in input data.</italic>
The mean divergence map reveals persistent gaps at some coastlines, in particular around the Persian Gulf. These gaps are caused by the cloud algorithm, as cloud retrievals are challenging for the transition of dark ocean to bright sand.
The situation will improve for an updated cloud product which will be based on a ground albedo with higher spatial resolution.</p></list-item><list-item>
      <p id="d1e6349"><italic>Artifacts in divergence.</italic>
In cases of inaccurate wind fields, as over mountainous terrain, as well as for systematic violation of the steady-state assumption, like systematic diurnal cycles of wind direction, the divergence map reveals artifacts, i.e., patterns of high negative values for <inline-formula><mml:math id="M333" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> which cannot be explained by the loss term <inline-formula><mml:math id="M334" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>.
These cases are classified as “negative” and are thus missing in the catalog.</p></list-item><list-item>
      <p id="d1e6369"><italic>Noise in divergence.</italic>
The noise level of the divergence map reveals large regional differences, causing respective differences in the performance of the peak fit algorithm.
Noise levels are particularly high over regions with generally high TVCD levels, like eastern China or western Europe.
This is caused by sampling effects.
For high TVCD levels, also fluxes are generally high.
As the daily flux maps have gaps due to cloud masking,
the mean fluxes reveal “jumps”.
This effect is probably intensified by the gridding by interpolation, where a gap (<inline-formula><mml:math id="M335" display="inline"><mml:mo lspace="0mm">=</mml:mo></mml:math></inline-formula> missing value) in the input data results in gaps for a substantially larger area in the gridded data, as interpolation requires information from all surrounding pixels.
Note that due to day-to-day changes of wind directions, a far higher amount of data would be needed in order to get  smooth flux maps than to overcome the respective sampling issues in mean TVCDs.
As the spatial derivative amplifies these jumps,
the divergence is generally noisy over regions with high TVCD.
Consequently, only few point sources are identified for the highly polluted regions in western Europe or eastern China, while many candidates are classified as “negative” due to the high noise levels.</p></list-item><list-item>
      <p id="d1e6382"><italic>Interfering sources.</italic>
Point sources cause peaks in the divergence map which can be described by a Gaussian. Typical widths are <inline-formula><mml:math id="M336" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:msub><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km, in accordance to the spatial resolution of TROPOMI. Thus, point sources within a distance of less than about 20 km cannot be clearly separated by the automated algorithm. In cases of point sources close to each other, they are identified and quantified as one single point source (see next section), and their emissions are just added.
If the distance is about 15–20 km, however, the joined peak from both sources is still processed as a single candidate but classified as “area source” due to the large width of the peak.
For example, the Indian power plants Vindhyachal and Anpara located within 16 km (Fig. <xref ref-type="fig" rid="Ch1.F3"/>d) or PP8 at the western edge of Riyadh megacity <xref ref-type="bibr" rid="bib1.bibx3" id="paren.56"><named-content content-type="pre">compare Fig. 2 in</named-content></xref> are classified as “area source” and thus missing in the catalog.</p></list-item></list></p>
</sec>
<sec id="Ch1.S5.SS1.SSS2">
  <label>5.1.2</label><title>Multiple sources</title>
      <p id="d1e6422">Due to the spatial resolution of TROPOMI, sources within about 10 km cannot be separated by the automatic peak-finding algorithm,
and power plant stack emissions would automatically be merged with emissions from on-site activities such as heavy-duty diesel around the power plant.
Several entries in the catalog contain multiple sources, like no. 1 (power plants Matla and Kriel within 5 km) or no. 3 (power plants Matimba and Medupi within 7 km).
Similarly, the emissions from large industrial complexes, like the Ulsan industrial area, cannot be further specified.
Thus the term “point source” means with respect to the TROPOMI<?pagebreak page3008?> spatial resolution. This is however still better resolved than many bottom-up inventories and typical horizontal resolutions of regional chemical transport models (CTMs).
Thus, for emission inventories, also multiple and extended sources could appropriately be treated as point source emissions if used for models with a spatial resolution coarser than that of TROPOMI.</p>
</sec>
</sec>
<sec id="Ch1.S5.SS2">
  <label>5.2</label><title>Uncertainties and accuracy</title>
      <p id="d1e6434">The main goal of v1.0 of the point source catalog is the identification rather than the quantification of <inline-formula><mml:math id="M337" 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> point sources. Still we discuss and try to quantify the various sources for uncertainties of the derived point source emissions.</p>
<sec id="Ch1.S5.SS2.SSS1">
  <label>5.2.1</label><title>Gridding</title>
      <p id="d1e6455">Gridding is done by 2-D linear interpolation, which avoids abrupt jumps at the satellite pixel edges. Such jumps would cause large response in the divergence, i.e., the spatial derivative.</p>
      <p id="d1e6458">For narrow plumes, however, linear interpolation carries the risk of introducing a low bias. We have investigated this exemplarily for the power plant plume of PP9 northeast of Riyadh on 17 December 2017 <xref ref-type="bibr" rid="bib1.bibx3" id="paren.57"><named-content content-type="post">Fig. 1a therein</named-content></xref>. The average plume TVCD from interpolation yields almost the same value as for conventional gridding (1 % lower). For the peak maximum, however, which is more relevant for the divergence than the mean, interpolation is 6 % lower.
Thus, there is a low bias caused by linear interpolation, which is small compared to the other effects discussed below.</p>
</sec>
<sec id="Ch1.S5.SS2.SSS2">
  <label>5.2.2</label><title>Lifetime</title>
      <p id="d1e6474">The quantification of <inline-formula><mml:math id="M338" 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 is based on the peak in <inline-formula><mml:math id="M339" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula>, ignoring the chemical loss of <inline-formula><mml:math id="M340" 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> during downwind transport.
We estimate the impact of neglecting the lifetime correction by comparing the catalog emissions to the respective emissions based on <inline-formula><mml:math id="M341" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> (assuming a lifetime of 4 h). On average, the latter were higher than those based on <inline-formula><mml:math id="M342" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> by about 25 %, which is quite small compared to other effects, in particular the AMF (see below).</p>
      <p id="d1e6520">In cases of much shorter lifetimes, like 1.5 h, as reported by <xref ref-type="bibr" rid="bib1.bibx11" id="text.58"/> for the Colstrip power plant in the USA (Fig. 1 therein), the emission estimates after lifetime correction would be higher by a factor of 1.73 on average.</p>
</sec>
<sec id="Ch1.S5.SS2.SSS3">
  <label>5.2.3</label><title>Wind fields</title>
      <p id="d1e6534">As discussed in <xref ref-type="bibr" rid="bib1.bibx3" id="text.59"/>, different effects on wind field uncertainties have to be considered:
<list list-type="bullet"><list-item>
      <p id="d1e6542">Errors of the wind direction (both random and systematic) result in a underestimation of the flux and thus the estimated emissions, as any mismatch in wind direction leads to a low bias of the wind speed component projected to the actual wind direction.
The underestimation is thus proportional to the cosine of the wind direction. For wind direction errors of 25<inline-formula><mml:math id="M343" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, it is about 10 %.</p>
      <p id="d1e6554">Larger systematic errors in wind direction would cause visible artifacts in the divergence map and would thus be captured and removed by the check for negative divergence during candidate classification. In cases of larger random effects, the artifacts of individual days would at least partly cancel in the mean flux. But the wind speed component in the actual wind direction would be significantly underestimated, as well as the resulting divergence.</p></list-item><list-item>
      <p id="d1e6558">The calculated fluxes, and thus the divergence map, are proportional to wind speed.
The choice of the altitude of input wind fields thus affects the resulting emissions, as wind speeds are generally higher for higher altitudes. In <xref ref-type="bibr" rid="bib1.bibx3" id="text.60"/>, the effect for taking wind fields from 250 or 730 m rather than from 450 m on emissions was quantified as about 10 %.</p>
      <p id="d1e6564">In this study, the focus was set to the clear identification of point sources. Thus, winds from a lower altitude (300 m) compared to <xref ref-type="bibr" rid="bib1.bibx3" id="text.61"/> (450 m) were chosen in order to have optimal wind direction data close to the <inline-formula><mml:math id="M344" 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 source. As discussed below, this choice removes the artifacts of divergence around the Matimba/Medupi power plants seen in <xref ref-type="bibr" rid="bib1.bibx3" id="text.62"/>.</p></list-item></list></p>
</sec>
<sec id="Ch1.S5.SS2.SSS4">
  <label>5.2.4</label><title>Peak fit</title>
      <p id="d1e6593">The fitted emissions depend on the settings for fit radius and the forward model function.
The fit window of 22 km around the source was chosen as compromise in order to cover the peak caused by a point source as far as possible while avoiding interference with neighboring sources.
Variations of the fit settings within reasonable limits cause an uncertainty of about 20 % in the fitted emissions <xref ref-type="bibr" rid="bib1.bibx3" id="paren.63"/>.</p>
</sec>
<sec id="Ch1.S5.SS2.SSS5">
  <label>5.2.5</label><title>AMF</title>
      <p id="d1e6607">Validation studies report on <inline-formula><mml:math id="M345" 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> TVCDs from TROPOMI being biased low for polluted sites <xref ref-type="bibr" rid="bib1.bibx31" id="paren.64"/>. This is probably due to the a priori vertical profiles, the cloud height product being biased low <xref ref-type="bibr" rid="bib1.bibx7" id="paren.65"/>, and the surface albedo being biased high <xref ref-type="bibr" rid="bib1.bibx12" id="paren.66"/>, all resulting in high biased AMFs.</p>
      <p id="d1e6630">In <xref ref-type="bibr" rid="bib1.bibx3" id="text.67"/>, a correction of the low bias was applied by assuming the <inline-formula><mml:math id="M346" 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> profile close to point sources to be in the lowest layer.
Note that since the divergence is sensitive for the <italic>change</italic> of the <inline-formula><mml:math id="M347" 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> flux due to the point source emissions,
the required AMF correction has to be applied to the profile of the <italic>added</italic> rather than the total <inline-formula><mml:math id="M348" 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>.</p>
      <?pagebreak page3009?><p id="d1e6676">Still, we do not apply such a correction here, since there are indications that the cloud heights and surface albedo used for the <inline-formula><mml:math id="M349" 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 are systematically biased. Thus, also the provided AKs are biased, and a simple a posteriori correction of TVCDs is not possible.</p>
      <p id="d1e6690">For Germany, the AMF correction applied in <xref ref-type="bibr" rid="bib1.bibx3" id="text.68"/> was a factor of 2 due to profile shape.
In combination with a bias in the cloud height and ground albedo used for the TVCD retrieval, even higher factors have to be expected.
The actual number will depend on surface albedo, aerosols, and cloud statistics (within the selection of low effective cloud fractions) and is high over dark surfaces and frequent cloud contamination but low over bright surfaces and few clouds (like for Riyadh).
For partly clouded scenes, the AMF for the added <inline-formula><mml:math id="M350" 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 could be easily too high by an order of magnitude if the real cloud is above the plume, but the retrieved cloud is below. Consequently, the added <inline-formula><mml:math id="M351" 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 biased low by an order of magnitude.
This issue was improved in a recent update of the TROPOMI <inline-formula><mml:math id="M352" 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> L2 processor now using improved albedo and cloud products and thus more appropriate AKs. However, so far, no reprocessed <inline-formula><mml:math id="M353" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> time series is available.</p>
</sec>
<sec id="Ch1.S5.SS2.SSS6">
  <label>5.2.6</label><title>Low bias</title>
      <p id="d1e6748">As listed above, many effects contribute to the uncertainty of emission estimates from the divergence of mean <inline-formula><mml:math id="M354" 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> fluxes.
Several of these effects are systematic in nature, resulting in an overall low bias of the derived emissions.
In particular the effects of biased cloud height and inaccurate a priori profiles are expected to reveal large regional dependencies.
Consequently, the low bias is hard to quantify for the global catalog.
Thus we decided not to try to correct for the low bias of catalog emissions in this study
but present the low biased estimates as they are with a clear disclaimer that the given emission estimates are biased low.</p>
      <p id="d1e6762">Accordingly, the emission estimates for South Africa reported in <xref ref-type="bibr" rid="bib1.bibx3" id="text.69"/> were higher than the values listed in Table <xref ref-type="table" rid="Ch1.T4"/> by a factor of about 1.87 (for Matla/Kriel) up to 2.56 (for Medupi/Matimba). This discrepancy is a consequence of the missing AMF correction (factor 1.35 applied in <xref ref-type="bibr" rid="bib1.bibx3" id="altparen.70"/>),
the missing lifetime correction (factor 1.1),
the wind input data from lower altitudes (factor 1.1),
and differences in grid definition, fit function (no rotation), and fit settings (factor 1.2), which
together explain a factor of 1.9 as found for Matla/Kriel.</p>
      <p id="d1e6773">For Medupi/Matimba, the reason for the remaining discrepancy is the difference in input wind fields.
The winds from higher altitudes (450 m) used in <xref ref-type="bibr" rid="bib1.bibx3" id="text.71"/> cause a pattern of high negative <inline-formula><mml:math id="M355" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> southwest of the power plants, indicating a mismatch of wind direction <xref ref-type="bibr" rid="bib1.bibx3" id="paren.72"><named-content content-type="pre">see Fig. S2B in the Supplement of</named-content></xref>. Even in <inline-formula><mml:math id="M356" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula>, after applying lifetime correction, the negative values southwest remain in maps of <inline-formula><mml:math id="M357" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx3" id="paren.73"><named-content content-type="pre">Fig. 4A in</named-content></xref>.
Consequently, the fit function finds a low background with a linear increase from southwest to northeast,
and the emissions fitted on top of this low background are biased high.</p>
      <?pagebreak page3010?><p id="d1e6811"><?xmltex \hack{\newpage}?>In the current study, this artifact is not present (see point source no. 3 in Fig. <xref ref-type="fig" rid="Ch1.F5"/>), indicating that the wind direction from lower altitude (300 m) matches better to the actual <inline-formula><mml:math id="M358" 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> transport of Medupi/Matimba emissions.</p>
      <p id="d1e6829">In the Supplement, catalog emissions are exemplarily compared to emissions reported by EPA for the top 10 emitters of the USA. A total of 7 of these 10 emitters are listed in the catalog, with correct naming found from the merging of GPPD. The other 3 emitters were also found as candidates but were classified as “negative”.
EPA emissions were found to be higher than the emissions listed in the catalog by a factor of 3 (Navajo) up to 8 (Hunter). These power plants, however, are quite remote from large cities. Thus, in the absence of other significant <inline-formula><mml:math id="M359" 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, the modeled profiles used as a priori for the calculation of AMFs do not reflect the near-surface power plant plume due to the coarse model resolution.
In addition, the cloud altitude used for the calculation of averaging kernels is biased low <xref ref-type="bibr" rid="bib1.bibx7" id="paren.74"/>, causing high biased AMFs and low biased columns. The impact of this bias can easily reach 1 order of magnitude for cases where the retrieval assumes a cloud below the plume, while it is actually above.
For these reasons, we have to expect that the low bias of the partial column added by a point source close to the ground is considerably larger than that of the complete tropospheric column, where validation studies report typical low biases of a factor of 2 for polluted sites.
We will focus on this issue more quantitatively when preparing an update of the catalog, which we plan to process after reprocessing of the TROPOMI <inline-formula><mml:math id="M360" 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> product based on improved albedo and cloud products and thus more appropriate AKs.</p>
</sec>
</sec>
<sec id="Ch1.S5.SS3">
  <label>5.3</label><title>Potential</title>
      <p id="d1e6866">Though the catalog is incomplete and the derived emissions are biased low, it still has the potential to improve our knowledge on <inline-formula><mml:math id="M361" 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. Here we discuss the benefits of the divergence approach and the point source catalog and propose future applications.</p>
<sec id="Ch1.S5.SS3.SSS1">
  <label>5.3.1</label><?xmltex \opttitle{Localization of {$\protect\chem{NO_{\mathit{x}}}$} and {$\protect\chem{CO_{2}}$} sources}?><title>Localization of <inline-formula><mml:math id="M362" 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 <inline-formula><mml:math id="M363" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> sources</title>
      <p id="d1e6910">The Gaussian fit determines the location of the peak maximum.
For all catalog locations which were inspected manually (i.e., all point sources listed in Table <xref ref-type="table" rid="Ch1.T4"/> or labeled in Fig. <xref ref-type="fig" rid="Ch1.F4"/>), Google Maps quickly reveals a plausible origin of the emissions close to the fitted peak location.
For the examples shown in Fig. <xref ref-type="fig" rid="Ch1.F5"/> which are related to power plants, the fitted point source location agrees to the actual power plant locations within about 2–3 km.
Thus, the point source catalog accurately lists the location of <inline-formula><mml:math id="M364" 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> point sources. As these sources are all related to combustion, this also provides valuable information on the location of <inline-formula><mml:math id="M365" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> sources, which may also help to quantify <inline-formula><mml:math id="M366" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions from <inline-formula><mml:math id="M367" 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> measurements <xref ref-type="bibr" rid="bib1.bibx19" id="paren.75"/> and current and future satellite measurements of <inline-formula><mml:math id="M368" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
</sec>
<sec id="Ch1.S5.SS3.SSS2">
  <label>5.3.2</label><title>Spatial patterns</title>
      <p id="d1e6986">Within a regional focus, the catalog reflects the spatial distribution and relative importance of point sources.
Regionally, high correlation between <inline-formula><mml:math id="M369" 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 power plant capacity was observed (Fig. <xref ref-type="fig" rid="Ch1.F6"/>).
Thus, it might be possible to re-distribute emissions from bottom-up inventories regionally according to the location of point sources in the catalog.</p>
      <p id="d1e7002">In addition, striking discrepancies between bottom-up inventories and the catalog,
like strong point sources present in one but missing in the other, might be investigated in more detail and should result in improved emission inventories.</p>
</sec>
<sec id="Ch1.S5.SS3.SSS3">
  <label>5.3.3</label><title>Up to dateness</title>
      <p id="d1e7013">Bottom-up inventories based on fuel consumption statistics have to collect and process input data from national reports.
Thus, they have a time lag and are outdated when released for countries with high dynamics in industrial activities.
Based on the divergence of <inline-formula><mml:math id="M370" 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> fluxes, single power plants can be identified and quantified, e.g., on an annual basis. This would allow us to detect short-term trends and power plants being switched on or off even in the vicinity of polluted cities such as Riyadh.</p>
</sec>
</sec>
<sec id="Ch1.S5.SS4">
  <label>5.4</label><title>Outlook</title>
      <p id="d1e7037">This paper describes v1.0 of the <inline-formula><mml:math id="M371" 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> point source catalog.
We plan to update the catalog as soon as a reprocessed TROPOMI <inline-formula><mml:math id="M372" 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> product is available.
We expect that some of the persistent gaps along coastlines, e.g., around Dubai, can be closed in the future, as soon as the cloud information is based on high-resolution maps of the surface albedo, and thus <inline-formula><mml:math id="M373" 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> TVCD becomes available there. In addition, improved surface albedo, cloud height, and a priori profiles are expected to improve the TVCD and (at least partly) remove the low bias.</p>
      <p id="d1e7073">In addition, we plan to use meteorological data from ERA-5 on higher spatial and temporal resolution.
Currently, 6-hourly model output of ECMWF meteorological data was interpolated to a regular horizontal grid with a resolution of 1<inline-formula><mml:math id="M374" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. Case studies will be performed in order to find out which is the best compromise between spatiotemporal sampling and processing time.</p>
</sec>
</sec>
<sec id="Ch1.S6">
  <label>6</label><title>Data availability</title>
      <?pagebreak page3011?><p id="d1e7094">TROPOMI NO<inline-formula><mml:math id="M375" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> data are available via Copernicus Sentinel-5P (processed by ESA), 2018,
TROPOMI Level 2 Nitrogen Dioxide tropospheric column products, Version 01, European Space Agency, <uri>https://doi.org/10.5270/S5P-s4ljg54</uri> <xref ref-type="bibr" rid="bib1.bibx10" id="paren.76"/>.
The full <inline-formula><mml:math id="M376" 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> point source catalog v1.0 is available at <uri>https://doi.org/10.26050/WDCC/Quant_NOx_TROPOMI</uri> <xref ref-type="bibr" rid="bib1.bibx4" id="paren.77"/>.
The corresponding divergence maps are provided by the authors on request.</p>
</sec>
<sec id="Ch1.S7" sec-type="conclusions">
  <label>7</label><title>Conclusions</title>
      <p id="d1e7138">The high spatial resolution provided by TROPOMI allows for the detection and quantification of strong <inline-formula><mml:math id="M377" 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> point sources like large power plants, metal smelters, cement plants, or industrial areas.
We present v1.0 of a global catalog of <inline-formula><mml:math id="M378" 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> point sources derived from the divergence of the mean <inline-formula><mml:math id="M379" 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> flux 2018–2019 by a fully automated iterative algorithm, yielding 451 point sources.
A total of 242 of these point sources could be matched to combustion power plants from a global database,
with a median distance of 1.6 km.
The top four point source emissions are all located in South Africa and related to coal burning.
About one-fourth of all point sources were found over the Indian subcontinent, where the method works quite well due to low noise levels.</p>
      <p id="d1e7174">The catalog is incomplete and misses point sources due to gaps in the divergence map (caused by gaps in the cloud product), artifacts in the divergence map (caused by non-steady state and inaccurate wind fields),
noise in the divergence map (caused by sampling effects for regions with high background TVCD like western Europe or China), and interference of sources within about 10–20 km distance.</p>
      <p id="d1e7177">The listed emissions are biased low mainly due to a low bias of input TVCDs from TROPOMI. As this bias is expected to vary regionally and is hard to quantify, it is not corrected for v1.0 of the catalog.
Exemplary comparisons to emissions reported from in situ monitoring reveals a low bias which can be as high as a factor of 8 for some power plants, which is probably caused by inappropriate a priori profiles and a low bias in the cloud height.</p>
      <p id="d1e7180">Still, the catalog has high potential for checking and improving emission inventories, as it localizes <inline-formula><mml:math id="M380" 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 also <inline-formula><mml:math id="M381" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) sources, provides spatial patterns of the distribution of sources, and yields up-to-date emission data.</p>
</sec>

      
      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p id="d1e7205">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/essd-13-2995-2021-supplement" xlink:title="zip">https://doi.org/10.5194/essd-13-2995-2021-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e7216">SB performed the analysis and wrote the paper with input from all co-authors.
CB processed the TROPOMI L2 data.
SD processed ECMWF meteorological data.
HE performed the retrieval of operational TROPOMI L2 <inline-formula><mml:math id="M382" 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> TVCDs.
VK compiled the ozone climatology from ESCiMo model data.
AdL initiated the matching between catalog point sources and GPPD.
TW contributed to the data analysis and interpretation and supervised the study.</p>
  </notes><?xmltex \hack{\newpage}?><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e7234">The authors declare that they have no conflict of interest.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e7240">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e7246">We thank ESA and the TROPOMI L1/L2 teams for realizing TROPOMI and providing <inline-formula><mml:math id="M383" 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 data.
ERA-Interim and ERA-5 data used in this study are provided by the European Centre for Medium-Range Weather Forecasts (ECMWF).
Andrea Pozzer is acknowledged for providing the ESCiMo model data used for the ozone climatology.</p></ack><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e7263">This paper was edited by Nellie Elguindi and reviewed by two anonymous referees.</p>
  </notes><ref-list>
    <title>References</title>

      <ref id="bib1.bibx1"><?xmltex \def\ref@label{Atkinson et al.(2004)}?><label>Atkinson et al.(2004)</label><?label Atkinson?><mixed-citation>Atkinson, R., Baulch, D. L., Cox, R. A., Crowley, J. N., Hampson, R. F., Hynes, R. G., Jenkin, M. E., Rossi, M. J., and Troe, J.: Evaluated kinetic and photochemical data for atmospheric chemistry: Volume I – gas phase reactions of <inline-formula><mml:math id="M384" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mi mathvariant="normal">x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M385" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mi mathvariant="normal">x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M386" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi mathvariant="normal">x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M387" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mi mathvariant="normal">x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> species, Atmos. Chem. Phys., 4, 1461–1738, <ext-link xlink:href="https://doi.org/10.5194/acp-4-1461-2004" ext-link-type="DOI">10.5194/acp-4-1461-2004</ext-link>, 2004.</mixed-citation></ref>
      <ref id="bib1.bibx2"><?xmltex \def\ref@label{Beirle et al.(2011)}?><label>Beirle et al.(2011)</label><?label BE11?><mixed-citation>Beirle, S., Boersma, K. F., Platt, U., Lawrence, M. G., and Wagner, T.:
Megacity Emissions and Lifetimes of Nitrogen Oxides Probed from Space,
Science, 333, 1737–1739, <ext-link xlink:href="https://doi.org/10.1126/science.1207824" ext-link-type="DOI">10.1126/science.1207824</ext-link>, 2011.</mixed-citation></ref>
      <ref id="bib1.bibx3"><?xmltex \def\ref@label{Beirle et al.(2019)}?><label>Beirle et al.(2019)</label><?label BE19?><mixed-citation>Beirle, S., Borger, C., Dörner, S., Li, A., Hu, Z., Liu, F., Wang, Y., and Wagner, T.:
Pinpointing nitrogen oxide emissions from space,
Sci. Adv. 5, eaax9800, <ext-link xlink:href="https://doi.org/10.1126/sciadv.aax9800" ext-link-type="DOI">10.1126/sciadv.aax9800</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bibx4"><?xmltex \def\ref@label{Beirle et al.(2020)}?><label>Beirle et al.(2020)</label><?label BE20?><mixed-citation>Beirle, S., Borger, C., Dörner, S., Eskes, H., Kumar, V., de Laat, A., and Wagner, T.:
Quantification of NOx point sources from the TROPOspheric Monitoring Instrument (TROPOMI),
World Data Center for Climate (WDCC) at DKRZ [data set],
<ext-link xlink:href="https://doi.org/10.26050/WDCC/Quant_NOx_TROPOMI" ext-link-type="DOI">10.26050/WDCC/Quant_NOx_TROPOMI</ext-link>, 2020.</mixed-citation></ref>
      <ref id="bib1.bibx5"><?xmltex \def\ref@label{Bouarar et al.(2019)}?><label>Bouarar et al.(2019)</label><?label Bouarar?><mixed-citation>Bouarar, I., Brasseur, G., Petersen, K., Granier, C., Fan, Q., Wang, X., Wang, L., Ji, D., Liu, Z., Xie, Y., Gao, W., and Elguindi, N.:
Influence of anthropogenic emission inventories on simulations of air quality in China during winter and summer 2010,
Atmos. Environ., 198, 236–256, <ext-link xlink:href="https://doi.org/10.1016/j.atmosenv.2018.10.043" ext-link-type="DOI">10.1016/j.atmosenv.2018.10.043</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bibx6"><?xmltex \def\ref@label{Byers et al.(2019)}?><label>Byers et al.(2019)</label><?label Byers?><mixed-citation>Byers, L., Friedrich, J., Hennig, R., Kressig, A., Li, X., McCormick, C., and Malaguzzi Valeri, L.:
A Global Database of Power Plants,
World Resources Institute, Washington, DC,
available at: <uri>https://datasets.wri.org/dataset/globalpowerplantdatabase</uri> (last access: 21 June 2021), 2019.</mixed-citation></ref>
      <ref id="bib1.bibx7"><?xmltex \def\ref@label{Compernolle et al.(2021)}?><label>Compernolle et al.(2021)</label><?label Compernolle?><mixed-citation>Compernolle, S., Argyrouli, A., Lutz, R., Sneep, M., Lambert, J.-C., Fjæraa, A. M., Hubert, D., Keppens, A., Loyola, D., O'Connor, E., Romahn, F., Stammes, P., Verhoelst, T., and Wang, P.: Validation of the Sentinel-5 Precursor TROPOMI c<?pagebreak page3012?>loud data with Cloudnet, Aura OMI O2–O2, MODIS, and Suomi-NPP VIIRS, Atmos. Meas. Tech., 14, 2451–2476, <ext-link xlink:href="https://doi.org/10.5194/amt-14-2451-2021" ext-link-type="DOI">10.5194/amt-14-2451-2021</ext-link>, 2021.</mixed-citation></ref>
      <ref id="bib1.bibx8"><?xmltex \def\ref@label{Dickerson et al.(1982)}?><label>Dickerson et al.(1982)</label><?label Dickerson?><mixed-citation>Dickerson, R. R., Stedman, D. H., and Delany, A. C.:
Direct Measurements of ozone and Nitrogen Dioxide Photolysis Rates in the Troposphere,
J. Geophys. Res., 87, 4933–4946, <ext-link xlink:href="https://doi.org/10.1029/JC087iC07p04933" ext-link-type="DOI">10.1029/JC087iC07p04933</ext-link>, 1982.</mixed-citation></ref>
      <ref id="bib1.bibx9"><?xmltex \def\ref@label{Eskes et al.(2003)}?><label>Eskes et al.(2003)</label><?label AK?><mixed-citation>Eskes, H. J. and Boersma, K. F.: Averaging kernels for DOAS total-column satellite retrievals, Atmos. Chem. Phys., 3, 1285–1291, <ext-link xlink:href="https://doi.org/10.5194/acp-3-1285-2003" ext-link-type="DOI">10.5194/acp-3-1285-2003</ext-link>, 2003.</mixed-citation></ref>
      <ref id="bib1.bibx10"><?xmltex \def\ref@label{European Space Agency(2019)}?><label>European Space Agency(2019)</label><?label ESA18?><mixed-citation>European Space Agency (ESA): Copernicus Sentinel-5P data products, ESA [data set], <ext-link xlink:href="https://doi.org/10.5270/S5P-s4ljg54" ext-link-type="DOI">10.5270/S5P-s4ljg54</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bibx11"><?xmltex \def\ref@label{Goldberg et al.(2019)}?><label>Goldberg et al.(2019)</label><?label Goldberg?><mixed-citation>Goldberg, D. L., Lu, Z., Streets, D. G., de Foy, B., Griffin, D., McLinden, C. A., Lamsal, L. N., Krotkov, N. A., and Eskes, H.:
Enhanced Capabilities of TROPOMI <inline-formula><mml:math id="M388" 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>: Estimating <inline-formula><mml:math id="M389" 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> from North American Cities and Power Plants,
Environ. Sci. Technol., 53, 12594–12601, <ext-link xlink:href="https://doi.org/10.1021/acs.est.9b04488" ext-link-type="DOI">10.1021/acs.est.9b04488</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bibx12"><?xmltex \def\ref@label{Griffin et al.(2019)}?><label>Griffin et al.(2019)</label><?label Griffin?><mixed-citation>Griffin, D., Zhao, X., McLinden, C. A., Boersma, F., Bourassa, A., Dammers, E., Degenstein, D., Eskes, H., Fehr, L., Fioletov, V., Hayden, K., Kharol, S. K., Li, S.-M., Makar, P., Martin, R. V., Mihele, C., Mittermeier, R. L., Krotkov, N., Sneep, M., Lamsal, L. N., Linden, M. ter, Geffen, J. van, Veefkind, P., and Wolde, M.:
High-Resolution Mapping of Nitrogen Dioxide With TROPOMI: First Results and Validation Over the Canadian Oil Sands,
Geophys. Res. Lett., 46, 1049–1060, <ext-link xlink:href="https://doi.org/10.1029/2018GL081095" ext-link-type="DOI">10.1029/2018GL081095</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bibx13"><?xmltex \def\ref@label{Hoffmann et al.(2019)}?><label>Hoffmann et al.(2019)</label><?label ERA5?><mixed-citation>Hoffmann, L., Günther, G., Li, D., Stein, O., Wu, X., Griessbach, S., Heng, Y., Konopka, P., Müller, R., Vogel, B., and Wright, J. S.: From ERA-Interim to ERA5: the considerable impact of ECMWF's next-generation reanalysis on Lagrangian transport simulations, Atmos. Chem. Phys., 19, 3097–3124, <ext-link xlink:href="https://doi.org/10.5194/acp-19-3097-2019" ext-link-type="DOI">10.5194/acp-19-3097-2019</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bibx14"><?xmltex \def\ref@label{IUPAC(2013)}?><label>IUPAC(2013)</label><?label IUPAC?><mixed-citation>IUPAC: Task Group on Atmospheric Chemical Kinetic Data Evaluation, available at:
<uri>http://iupac.pole-ether.fr</uri> (last access: 21 June 2021),
Data Sheet NOx24, last evaluated: June 2013.</mixed-citation></ref>
      <ref id="bib1.bibx15"><?xmltex \def\ref@label{J\"{o}ckel et al.(2010)}?><label>Jöckel et al.(2010)</label><?label PJ10?><mixed-citation>Jöckel, P., Kerkweg, A., Pozzer, A., Sander, R., Tost, H., Riede, H., Baumgaertner, A., Gromov, S., and Kern, B.: Development cycle 2 of the Modular Earth Submodel System (MESSy2), Geosci. Model Dev., 3, 717–752, <ext-link xlink:href="https://doi.org/10.5194/gmd-3-717-2010" ext-link-type="DOI">10.5194/gmd-3-717-2010</ext-link>, 2010.</mixed-citation></ref>
      <ref id="bib1.bibx16"><?xmltex \def\ref@label{J\"{o}ckel et al.(2016)}?><label>Jöckel et al.(2016)</label><?label PJ16?><mixed-citation>Jöckel, P., Tost, H., Pozzer, A., Kunze, M., Kirner, O., Brenninkmeijer, C. A. M., Brinkop, S., Cai, D. S., Dyroff, C., Eckstein, J., Frank, F., Garny, H., Gottschaldt, K.-D., Graf, P., Grewe, V., Kerkweg, A., Kern, B., Matthes, S., Mertens, M., Meul, S., Neumaier, M., Nützel, M., Oberländer-Hayn, S., Ruhnke, R., Runde, T., Sander, R., Scharffe, D., and Zahn, A.: Earth System Chemistry integrated Modelling (ESCiMo) with the Modular Earth Submodel System (MESSy) version 2.51, Geosci. Model Dev., 9, 1153–1200, <ext-link xlink:href="https://doi.org/10.5194/gmd-9-1153-2016" ext-link-type="DOI">10.5194/gmd-9-1153-2016</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bibx17"><?xmltex \def\ref@label{Judd et al.(2020)}?><label>Judd et al.(2020)</label><?label Judd?><mixed-citation>Judd, L. M., Al-Saadi, J. A., Szykman, J. J., Valin, L. C., Janz, S. J., Kowalewski, M. G., Eskes, H. J., Veefkind, J. P., Cede, A., Mueller, M., Gebetsberger, M., Swap, R., Pierce, R. B., Nowlan, C. R., Abad, G. G., Nehrir, A., and Williams, D.: Evaluating Sentinel-5P TROPOMI tropospheric <inline-formula><mml:math id="M390" 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 densities with airborne and Pandora spectrometers near New York City and Long Island Sound, Atmos. Meas. Tech., 13, 6113–6140, <ext-link xlink:href="https://doi.org/10.5194/amt-13-6113-2020" ext-link-type="DOI">10.5194/amt-13-6113-2020</ext-link>, 2020.</mixed-citation></ref>
      <ref id="bib1.bibx18"><?xmltex \def\ref@label{Leue et al.(2001)}?><label>Leue et al.(2001)</label><?label Leue?><mixed-citation>Leue, C., Wenig, M., Wagner, T., Klimm, O., Platt, U., and Jähne, B.:
Quantitative analysis of <inline-formula><mml:math id="M391" 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
Global Ozone Monitoring Experiment satellite image sequences,
J. Geophys. Res., 106, 5493–5505, 2001.</mixed-citation></ref>
      <ref id="bib1.bibx19"><?xmltex \def\ref@label{Liu et al.(2020)}?><label>Liu et al.(2020)</label><?label Liu?><mixed-citation>Liu, F., Duncan, B. N., Krotkov, N. A., Lamsal, L. N., Beirle, S., Griffin, D., McLinden, C. A., Goldberg, D. L., and Lu, Z.: A methodology to constrain carbon dioxide emissions from coal-fired power plants using satellite observations of co-emitted nitrogen dioxide, Atmos. Chem. Phys., 20, 99–116, <ext-link xlink:href="https://doi.org/10.5194/acp-20-99-2020" ext-link-type="DOI">10.5194/acp-20-99-2020</ext-link>, 2020.</mixed-citation></ref>
      <ref id="bib1.bibx20"><?xmltex \def\ref@label{Lorente et al.(2019)}?><label>Lorente et al.(2019)</label><?label Lorente?><mixed-citation>Lorente, A., Boersma, K. F., Eskes, H. J., Veefkind, J. P., Geffen, J. H. G. M. van, Zeeuw, M. B. de, Gon, H. A. C. D. van der, Beirle, S., and Krol, M. C.:
Quantification of nitrogen oxides emissions from build-up of pollution over Paris with TROPOMI,
Sci. Rep., 9, 20033, <ext-link xlink:href="https://doi.org/10.1038/s41598-019-56428-5" ext-link-type="DOI">10.1038/s41598-019-56428-5</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bibx21"><?xmltex \def\ref@label{Martin(2008)}?><label>Martin(2008)</label><?label Martin08?><mixed-citation>Martin, R. V.: Satellite remote sensing of surface air quality,
Atmos. Environ., 42, 7823–7843,
<ext-link xlink:href="https://doi.org/10.1016/j.atmosenv.2008.07.018" ext-link-type="DOI">10.1016/j.atmosenv.2008.07.018</ext-link>, 2008.</mixed-citation></ref>
      <ref id="bib1.bibx22"><?xmltex \def\ref@label{Martin et al.(2003)}?><label>Martin et al.(2003)</label><?label Martin03?><mixed-citation>Martin, R. V., Jacob, D. J., Chance, K., Kurosu, T. P., Palmer, P. I., and Evans, M. J.: Global inventory of nitrogen oxide emissions constrained by space-based observations of <inline-formula><mml:math id="M392" 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,
J. Geophys. Res., 108, 4537, <ext-link xlink:href="https://doi.org/10.1029/2003JD003453" ext-link-type="DOI">10.1029/2003JD003453</ext-link>, 2003.</mixed-citation></ref>
      <ref id="bib1.bibx23"><?xmltex \def\ref@label{Mijling and van der A(2012)}?><label>Mijling and van der A(2012)</label><?label Mijling?><mixed-citation>Mijling,  B.  and  van  der  A,  R.  J.:
Using  daily  satellite  observations  to  estimate  emissions  of  short-lived  air  pollutants  on a  mesoscopic  scale,
J. Geophys. Res.-Atmos.,  117,  D17302,
<ext-link xlink:href="https://doi.org/10.1029/2012JD017817" ext-link-type="DOI">10.1029/2012JD017817</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bibx24"><?xmltex \def\ref@label{Monks and Beirle(2011)}?><label>Monks and Beirle(2011)</label><?label MonksBeirle?><mixed-citation>Monks, P. S. and Beirle, S.:
Applications of Satellite Observations of Tropospheric Composition,
in: The Remote Sensing of Tropospheric Composition from Space,
edited by: Burrows, J. P., Borrell, P., Platt, U., Guzzi, R., Platt, U., and Lanzerotti, L. J.,
Springer Berlin Heidelberg,
available at: <uri>https://link.springer.com/chapter/10.1007/978-3-642-14791-3_8</uri> (last access: 21 June 2021), pp. 365–449,
2011.</mixed-citation></ref>
      <ref id="bib1.bibx25"><?xmltex \def\ref@label{Platt and Stutz(2008)}?><label>Platt and Stutz(2008)</label><?label Platt08?><mixed-citation>
Platt, U. and Stutz, J.: Differential Optical Absorption Spectroscopy,
Springer-Verlag, Berlin, Heidelberg, 2008.</mixed-citation></ref>
      <ref id="bib1.bibx26"><?xmltex \def\ref@label{Richter and Wagner(2011)}?><label>Richter and Wagner(2011)</label><?label RichterWagner?><mixed-citation>Richter, A. and Wagner, T.:
The Use of UV, Visible and Near IR Solar Back Scattered Radiation to Determine Trace Gases,
in The Remote Sensing of Tropospheric Composition from Space,
edited by: Burrows, J. P., Borrell, P., Platt, U., Guzzi, R., Platt, U., and Lanzerotti, L. J.,
Springer Berlin Heidelberg,
available at: <uri>https://link.springer.com/chapter/10.1007/978-3-642-14791-3_2</uri> (last
access: 21 June 2021), pp. 67–121,
2011.</mixed-citation></ref>
      <ref id="bib1.bibx27"><?xmltex \def\ref@label{Seinfeld and Pandis(2006)}?><label>Seinfeld and Pandis(2006)</label><?label Seinfeld?><mixed-citation>
Seinfeld, J. H. and Pandis, S. N.: Atmospheric Chemistry and Physics: From Air Pollution to Climate Change, 2nd edn., John Wiley &amp; Sons, New York, 2006.</mixed-citation></ref>
      <ref id="bib1.bibx28"><?xmltex \def\ref@label{Geffen et al.(2020)}?><label>Geffen et al.(2020)</label><?label Geffen?><mixed-citation>van Geffen, J., Boersma, K. F., Eskes, H., Sneep, M., ter Linden, M., Zara, M., and Veefkind, J. P.: S5P TROPOMI <inline-formula><mml:math id="M393" 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> slant column retrieval: method, stability, uncertainties and comparisons with OMI, Atmos. Meas. Tech., 13, 1315–1335, <ext-link xlink:href="https://doi.org/10.5194/amt-13-1315-2020" ext-link-type="DOI">10.5194/amt-13-1315-2020</ext-link>, 2020.</mixed-citation></ref>
      <ref id="bib1.bibx29"><?xmltex \def\ref@label{Geffen et al.(2019)}?><label>Geffen et al.(2019)</label><?label ATBD?><mixed-citation>van Geffen, J. H. G. M., Eskes, H. J., Boersma, K. F., Maasakkers, J. D., and Veefkind, J. P.:
TROPOMI ATBD of the total and tropospheric <inline-formula><mml:math id="M394" 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 products,
S5P-KNMI-L2-0005-RP, Royal Netherlands Meteorological Institute, available at: <uri>https://sentinel.esa.int/documents/247904/2476257/Sentinel-5P-TROPOMI-ATBD-NO2-data-products</uri> (last access: 21 June 2021),
2019.
</mixed-citation></ref><?xmltex \hack{\newpage}?>
      <ref id="bib1.bibx30"><?xmltex \def\ref@label{Veefkind et al.(2012)}?><label>Veefkind et al.(2012)</label><?label TROPOMI?><mixed-citation>Veefkind, J. P., Aben, I., McMullan, K., Förster, H., de Vries, J., Otter, G., Claas, J., Eskes, H. J., de Haan, J. F., Kleipool, Q., van Weele, M., Hasekamp, O., Hoogeveen, R., Landgraf, J., Snel, R., Tol, P., Ingmann, P., Voors, R., Kruizinga, B., Vink, R., Visser, H., and Levelt, P. F.:
TROPOMI on the ESA Sentinel-5 Precursor: A GMES mission for global observations of the atmospheric composition for climate, air quality and ozone layer applications,
Remote Sens. Environ., 120, 70–83, <ext-link xlink:href="https://doi.org/10.1016/j.rse.2011.09.027" ext-link-type="DOI">10.1016/j.rse.2011.09.027</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bibx31"><?xmltex \def\ref@label{Verhoelst et al.(2021)}?><label>Verhoelst et al.(2021)</label><?label Verhoelst?><mixed-citation>Verhoelst, T., Compernolle, S., Pinardi, G., Lambert, J.-C., Eskes, H. J., Eichmann, K.-U., Fjæraa, A. M., Granville, J., Niemeijer, S., Cede, A., Tiefengraber, M., Hendrick, F., Pazmiño, A., Bais, A., Bazureau, A., Boersma, K. F., Bognar, K., Dehn, A., Donner, S., Elokhov, A., Gebetsberger, M., Goutail, F., Grutter de la Mora, M., Gruzdev, A., Gratsea, M., Hansen, G. H., Irie, H., Jepsen, N., Kanaya, Y., Karagkiozidis, D., Kivi, R., Kreher, K., Levelt, P. F., Liu, C., Müller, M., Navarro Comas, M., Piters, A. J. M., Pommereau, J.-P., Portafaix, T., Prados-Roman, C., Puentedura, O., Querel, R., Remmers, J., Richter, A., Rimmer, J., Rivera Cárdenas, C., Saavedra de Miguel, L., Sinyakov, V. P., Stremme, W., Strong, K., Van Roozendael, M., Veefkind, J. P., Wagner, T., Wittrock, F., Yela González, M., and Zehner, C.: Ground-based validation of the Copernicus Sentinel-5P TROPOMI NO<inline-formula><mml:math id="M395" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements with the NDACC ZSL-DOAS, MAX-DOAS and Pandonia global networks, Atmos. Meas. Tech., 14, 481–510, <ext-link xlink:href="https://doi.org/10.5194/amt-14-481-2021" ext-link-type="DOI">10.5194/amt-14-481-2021</ext-link>, 2021.</mixed-citation></ref>
      <ref id="bib1.bibx32"><?xmltex \def\ref@label{Virtanen et al.(2020)}?><label>Virtanen et al.(2020)</label><?label Virtanen?><mixed-citation>Virtanen, P., Gommers, R., Oliphant, T. E., Haberland, M., Reddy, T., Cournapeau, D., Burovski, E., Peterson, P., Weckesser, W., Bright, J., van der Walt, S. J., Brett, M., Wilson, J., Millman, K. J., Mayorov, N., Nelson, A. R. J., Jones, E., Kern, R., Larson, E., Carey, C. J., Polat, İ., Feng, Y., Moore, E. W., VanderPlas, J., Laxalde, D., Perktold, J., Cimrman, R., Henriksen, I., Quintero, E. A., Harris, C. R., Archibald, A. M., Ribeiro, A. H., Pedregosa, F., and van Mulbregt, P.:
SciPy 1.0: fundamental algorithms for scientific computing in Python,
Nat. Methods, 17, 261–272, <ext-link xlink:href="https://doi.org/10.1038/s41592-019-0686-2" ext-link-type="DOI">10.1038/s41592-019-0686-2</ext-link>, 2020.</mixed-citation></ref>
      <ref id="bib1.bibx33"><?xmltex \def\ref@label{Wagner et al.(2007)}?><label>Wagner et al.(2007)</label><?label Wagner?><mixed-citation>Wagner, T., Burrows, J. P., Deutschmann, T., Dix, B., von Friedeburg, C., Frieß, U., Hendrick, F., Heue, K.-P., Irie, H., Iwabuchi, H., Kanaya, Y., Keller, J., McLinden, C. A., Oetjen, H., Palazzi, E., Petritoli, A., Platt, U., Postylyakov, O., Pukite, J., Richter, A., van Roozendael, M., Rozanov, A., Rozanov, V., Sinreich, R., Sanghavi, S., and Wittrock, F.: Comparison of box-air-mass-factors and radiances for Multiple-Axis Differential Optical Absorption Spectroscopy (MAX-DOAS) geometries calculated from different UV/visible radiative transfer models, Atmos. Chem. Phys., 7, 1809–1833, <ext-link xlink:href="https://doi.org/10.5194/acp-7-1809-2007" ext-link-type="DOI">10.5194/acp-7-1809-2007</ext-link>, 2007.</mixed-citation></ref>

  </ref-list></back>
    <!--<article-title-html>Catalog of NO<sub><i>x</i></sub> emissions from point sources as derived from the divergence of the NO<sub>2</sub> flux for TROPOMI</article-title-html>
<abstract-html><p>We present version 1.0 of a global catalog of NO<sub><i>x</i></sub> emissions from point sources, derived from TROPOspheric Monitoring Instrument (TROPOMI) measurements of tropospheric NO<sub>2</sub> for 2018–2019.
The identification of sources and quantification of emissions are based on the divergence (spatial derivative) of the mean horizontal flux, which is highly sensitive for point sources like power plant exhaust stacks.</p><p>The catalog lists 451 locations which could be clearly identified as NO<sub><i>x</i></sub> point sources by a fully automated algorithm, while ambiguous cases as well as area sources such as megacities are skipped.
A total of 242 of these point sources could be automatically matched to power plants.
Other NO<sub><i>x</i></sub> point sources listed in the catalog are metal smelters, cement plants, or industrial areas.
The four largest localized NO<sub><i>x</i></sub> emitters are all coal combustion plants in South Africa. About 1∕4 of all detected point sources are located in the Indian subcontinent and are mostly associated with power plants.</p><p>The catalog is incomplete, mainly due to persisting gaps in the TROPOMI NO<sub>2</sub> product at some coastlines, inaccurate or complex wind fields in coastal and mountainous regions, and high noise in the divergence maps for high background pollution.
The derived emissions are generally too low, lacking a factor of about 2 up to 8 for extreme cases.
This strong low bias results from combination of different effects, most of all a strong underestimation of near-surface NO<sub>2</sub> in TROPOMI NO<sub>2</sub> columns.</p><p>Still, the catalog has high potential for checking and improving emission inventories, as it provides accurate and independent up-to-date information on the location of sources of NO<sub><i>x</i></sub> and thus also CO<sub>2</sub>.</p><p>The catalog of NO<sub><i>x</i></sub> emissions from point sources is freely available at <a href="https://doi.org/10.26050/WDCC/Quant_NOx_TROPOMI" target="_blank"/> (Beirle et al., 2020).</p></abstract-html>
<ref-html id="bib1.bib1"><label>Atkinson et al.(2004)</label><mixed-citation>
Atkinson, R., Baulch, D. L., Cox, R. A., Crowley, J. N., Hampson, R. F., Hynes, R. G., Jenkin, M. E., Rossi, M. J., and Troe, J.: Evaluated kinetic and photochemical data for atmospheric chemistry: Volume I – gas phase reactions of O<sub>x</sub>, HO<sub>x</sub>, NO<sub>x</sub> and SO<sub>x</sub> species, Atmos. Chem. Phys., 4, 1461–1738, <a href="https://doi.org/10.5194/acp-4-1461-2004" target="_blank">https://doi.org/10.5194/acp-4-1461-2004</a>, 2004.
</mixed-citation></ref-html>
<ref-html id="bib1.bib2"><label>Beirle et al.(2011)</label><mixed-citation>
Beirle, S., Boersma, K. F., Platt, U., Lawrence, M. G., and Wagner, T.:
Megacity Emissions and Lifetimes of Nitrogen Oxides Probed from Space,
Science, 333, 1737–1739, <a href="https://doi.org/10.1126/science.1207824" target="_blank">https://doi.org/10.1126/science.1207824</a>, 2011.
</mixed-citation></ref-html>
<ref-html id="bib1.bib3"><label>Beirle et al.(2019)</label><mixed-citation>
Beirle, S., Borger, C., Dörner, S., Li, A., Hu, Z., Liu, F., Wang, Y., and Wagner, T.:
Pinpointing nitrogen oxide emissions from space,
Sci. Adv. 5, eaax9800, <a href="https://doi.org/10.1126/sciadv.aax9800" target="_blank">https://doi.org/10.1126/sciadv.aax9800</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib4"><label>Beirle et al.(2020)</label><mixed-citation>
Beirle, S., Borger, C., Dörner, S., Eskes, H., Kumar, V., de Laat, A., and Wagner, T.:
Quantification of NOx point sources from the TROPOspheric Monitoring Instrument (TROPOMI),
World Data Center for Climate (WDCC) at DKRZ [data set],
<a href="https://doi.org/10.26050/WDCC/Quant_NOx_TROPOMI" target="_blank">https://doi.org/10.26050/WDCC/Quant_NOx_TROPOMI</a>, 2020.
</mixed-citation></ref-html>
<ref-html id="bib1.bib5"><label>Bouarar et al.(2019)</label><mixed-citation>
Bouarar, I., Brasseur, G., Petersen, K., Granier, C., Fan, Q., Wang, X., Wang, L., Ji, D., Liu, Z., Xie, Y., Gao, W., and Elguindi, N.:
Influence of anthropogenic emission inventories on simulations of air quality in China during winter and summer 2010,
Atmos. Environ., 198, 236–256, <a href="https://doi.org/10.1016/j.atmosenv.2018.10.043" target="_blank">https://doi.org/10.1016/j.atmosenv.2018.10.043</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib6"><label>Byers et al.(2019)</label><mixed-citation>
Byers, L., Friedrich, J., Hennig, R., Kressig, A., Li, X., McCormick, C., and Malaguzzi Valeri, L.:
A Global Database of Power Plants,
World Resources Institute, Washington, DC,
available at: <a href="https://datasets.wri.org/dataset/globalpowerplantdatabase" target="_blank"/> (last access: 21 June 2021), 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib7"><label>Compernolle et al.(2021)</label><mixed-citation>
Compernolle, S., Argyrouli, A., Lutz, R., Sneep, M., Lambert, J.-C., Fjæraa, A. M., Hubert, D., Keppens, A., Loyola, D., O'Connor, E., Romahn, F., Stammes, P., Verhoelst, T., and Wang, P.: Validation of the Sentinel-5 Precursor TROPOMI cloud data with Cloudnet, Aura OMI O2–O2, MODIS, and Suomi-NPP VIIRS, Atmos. Meas. Tech., 14, 2451–2476, <a href="https://doi.org/10.5194/amt-14-2451-2021" target="_blank">https://doi.org/10.5194/amt-14-2451-2021</a>, 2021.
</mixed-citation></ref-html>
<ref-html id="bib1.bib8"><label>Dickerson et al.(1982)</label><mixed-citation>
Dickerson, R. R., Stedman, D. H., and Delany, A. C.:
Direct Measurements of ozone and Nitrogen Dioxide Photolysis Rates in the Troposphere,
J. Geophys. Res., 87, 4933–4946, <a href="https://doi.org/10.1029/JC087iC07p04933" target="_blank">https://doi.org/10.1029/JC087iC07p04933</a>, 1982.
</mixed-citation></ref-html>
<ref-html id="bib1.bib9"><label>Eskes et al.(2003)</label><mixed-citation>
Eskes, H. J. and Boersma, K. F.: Averaging kernels for DOAS total-column satellite retrievals, Atmos. Chem. Phys., 3, 1285–1291, <a href="https://doi.org/10.5194/acp-3-1285-2003" target="_blank">https://doi.org/10.5194/acp-3-1285-2003</a>, 2003.
</mixed-citation></ref-html>
<ref-html id="bib1.bib10"><label>European Space Agency(2019)</label><mixed-citation>
European Space Agency (ESA): Copernicus Sentinel-5P data products, ESA [data set], <a href="https://doi.org/10.5270/S5P-s4ljg54" target="_blank">https://doi.org/10.5270/S5P-s4ljg54</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib11"><label>Goldberg et al.(2019)</label><mixed-citation>
Goldberg, D. L., Lu, Z., Streets, D. G., de Foy, B., Griffin, D., McLinden, C. A., Lamsal, L. N., Krotkov, N. A., and Eskes, H.:
Enhanced Capabilities of TROPOMI NO<sub>2</sub>: Estimating NO<sub><i>x</i></sub> from North American Cities and Power Plants,
Environ. Sci. Technol., 53, 12594–12601, <a href="https://doi.org/10.1021/acs.est.9b04488" target="_blank">https://doi.org/10.1021/acs.est.9b04488</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib12"><label>Griffin et al.(2019)</label><mixed-citation>
Griffin, D., Zhao, X., McLinden, C. A., Boersma, F., Bourassa, A., Dammers, E., Degenstein, D., Eskes, H., Fehr, L., Fioletov, V., Hayden, K., Kharol, S. K., Li, S.-M., Makar, P., Martin, R. V., Mihele, C., Mittermeier, R. L., Krotkov, N., Sneep, M., Lamsal, L. N., Linden, M. ter, Geffen, J. van, Veefkind, P., and Wolde, M.:
High-Resolution Mapping of Nitrogen Dioxide With TROPOMI: First Results and Validation Over the Canadian Oil Sands,
Geophys. Res. Lett., 46, 1049–1060, <a href="https://doi.org/10.1029/2018GL081095" target="_blank">https://doi.org/10.1029/2018GL081095</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib13"><label>Hoffmann et al.(2019)</label><mixed-citation>
Hoffmann, L., Günther, G., Li, D., Stein, O., Wu, X., Griessbach, S., Heng, Y., Konopka, P., Müller, R., Vogel, B., and Wright, J. S.: From ERA-Interim to ERA5: the considerable impact of ECMWF's next-generation reanalysis on Lagrangian transport simulations, Atmos. Chem. Phys., 19, 3097–3124, <a href="https://doi.org/10.5194/acp-19-3097-2019" target="_blank">https://doi.org/10.5194/acp-19-3097-2019</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib14"><label>IUPAC(2013)</label><mixed-citation>
IUPAC: Task Group on Atmospheric Chemical Kinetic Data Evaluation, available at:
<a href="http://iupac.pole-ether.fr" target="_blank"/> (last access: 21 June 2021),
Data Sheet NOx24, last evaluated: June 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib15"><label>Jöckel et al.(2010)</label><mixed-citation>
Jöckel, P., Kerkweg, A., Pozzer, A., Sander, R., Tost, H., Riede, H., Baumgaertner, A., Gromov, S., and Kern, B.: Development cycle 2 of the Modular Earth Submodel System (MESSy2), Geosci. Model Dev., 3, 717–752, <a href="https://doi.org/10.5194/gmd-3-717-2010" target="_blank">https://doi.org/10.5194/gmd-3-717-2010</a>, 2010.
</mixed-citation></ref-html>
<ref-html id="bib1.bib16"><label>Jöckel et al.(2016)</label><mixed-citation>
Jöckel, P., Tost, H., Pozzer, A., Kunze, M., Kirner, O., Brenninkmeijer, C. A. M., Brinkop, S., Cai, D. S., Dyroff, C., Eckstein, J., Frank, F., Garny, H., Gottschaldt, K.-D., Graf, P., Grewe, V., Kerkweg, A., Kern, B., Matthes, S., Mertens, M., Meul, S., Neumaier, M., Nützel, M., Oberländer-Hayn, S., Ruhnke, R., Runde, T., Sander, R., Scharffe, D., and Zahn, A.: Earth System Chemistry integrated Modelling (ESCiMo) with the Modular Earth Submodel System (MESSy) version 2.51, Geosci. Model Dev., 9, 1153–1200, <a href="https://doi.org/10.5194/gmd-9-1153-2016" target="_blank">https://doi.org/10.5194/gmd-9-1153-2016</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib17"><label>Judd et al.(2020)</label><mixed-citation>
Judd, L. M., Al-Saadi, J. A., Szykman, J. J., Valin, L. C., Janz, S. J., Kowalewski, M. G., Eskes, H. J., Veefkind, J. P., Cede, A., Mueller, M., Gebetsberger, M., Swap, R., Pierce, R. B., Nowlan, C. R., Abad, G. G., Nehrir, A., and Williams, D.: Evaluating Sentinel-5P TROPOMI tropospheric NO<sub>2</sub> column densities with airborne and Pandora spectrometers near New York City and Long Island Sound, Atmos. Meas. Tech., 13, 6113–6140, <a href="https://doi.org/10.5194/amt-13-6113-2020" target="_blank">https://doi.org/10.5194/amt-13-6113-2020</a>, 2020.
</mixed-citation></ref-html>
<ref-html id="bib1.bib18"><label>Leue et al.(2001)</label><mixed-citation>
Leue, C., Wenig, M., Wagner, T., Klimm, O., Platt, U., and Jähne, B.:
Quantitative analysis of NO<sub><i>x</i></sub> emissions from
Global Ozone Monitoring Experiment satellite image sequences,
J. Geophys. Res., 106, 5493–5505, 2001.
</mixed-citation></ref-html>
<ref-html id="bib1.bib19"><label>Liu et al.(2020)</label><mixed-citation>
Liu, F., Duncan, B. N., Krotkov, N. A., Lamsal, L. N., Beirle, S., Griffin, D., McLinden, C. A., Goldberg, D. L., and Lu, Z.: A methodology to constrain carbon dioxide emissions from coal-fired power plants using satellite observations of co-emitted nitrogen dioxide, Atmos. Chem. Phys., 20, 99–116, <a href="https://doi.org/10.5194/acp-20-99-2020" target="_blank">https://doi.org/10.5194/acp-20-99-2020</a>, 2020.
</mixed-citation></ref-html>
<ref-html id="bib1.bib20"><label>Lorente et al.(2019)</label><mixed-citation>
Lorente, A., Boersma, K. F., Eskes, H. J., Veefkind, J. P., Geffen, J. H. G. M. van, Zeeuw, M. B. de, Gon, H. A. C. D. van der, Beirle, S., and Krol, M. C.:
Quantification of nitrogen oxides emissions from build-up of pollution over Paris with TROPOMI,
Sci. Rep., 9, 20033, <a href="https://doi.org/10.1038/s41598-019-56428-5" target="_blank">https://doi.org/10.1038/s41598-019-56428-5</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib21"><label>Martin(2008)</label><mixed-citation>
Martin, R. V.: Satellite remote sensing of surface air quality,
Atmos. Environ., 42, 7823–7843,
<a href="https://doi.org/10.1016/j.atmosenv.2008.07.018" target="_blank">https://doi.org/10.1016/j.atmosenv.2008.07.018</a>, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib22"><label>Martin et al.(2003)</label><mixed-citation>
Martin, R. V., Jacob, D. J., Chance, K., Kurosu, T. P., Palmer, P. I., and Evans, M. J.: Global inventory of nitrogen oxide emissions constrained by space-based observations of NO<sub>2</sub> columns,
J. Geophys. Res., 108, 4537, <a href="https://doi.org/10.1029/2003JD003453" target="_blank">https://doi.org/10.1029/2003JD003453</a>, 2003.
</mixed-citation></ref-html>
<ref-html id="bib1.bib23"><label>Mijling and van der A(2012)</label><mixed-citation>
Mijling,  B.  and  van  der  A,  R.  J.:
Using  daily  satellite  observations  to  estimate  emissions  of  short-lived  air  pollutants  on a  mesoscopic  scale,
J. Geophys. Res.-Atmos.,  117,  D17302,
<a href="https://doi.org/10.1029/2012JD017817" target="_blank">https://doi.org/10.1029/2012JD017817</a>, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib24"><label>Monks and Beirle(2011)</label><mixed-citation>
Monks, P. S. and Beirle, S.:
Applications of Satellite Observations of Tropospheric Composition,
in: The Remote Sensing of Tropospheric Composition from Space,
edited by: Burrows, J. P., Borrell, P., Platt, U., Guzzi, R., Platt, U., and Lanzerotti, L. J.,
Springer Berlin Heidelberg,
available at: <a href="https://link.springer.com/chapter/10.1007/978-3-642-14791-3_8" target="_blank"/> (last access: 21 June 2021), pp. 365–449,
2011.
</mixed-citation></ref-html>
<ref-html id="bib1.bib25"><label>Platt and Stutz(2008)</label><mixed-citation>
Platt, U. and Stutz, J.: Differential Optical Absorption Spectroscopy,
Springer-Verlag, Berlin, Heidelberg, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib26"><label>Richter and Wagner(2011)</label><mixed-citation>
Richter, A. and Wagner, T.:
The Use of UV, Visible and Near IR Solar Back Scattered Radiation to Determine Trace Gases,
in The Remote Sensing of Tropospheric Composition from Space,
edited by: Burrows, J. P., Borrell, P., Platt, U., Guzzi, R., Platt, U., and Lanzerotti, L. J.,
Springer Berlin Heidelberg,
available at: <a href="https://link.springer.com/chapter/10.1007/978-3-642-14791-3_2" target="_blank"/> (last
access: 21 June 2021), pp. 67–121,
2011.
</mixed-citation></ref-html>
<ref-html id="bib1.bib27"><label>Seinfeld and Pandis(2006)</label><mixed-citation>
Seinfeld, J. H. and Pandis, S. N.: Atmospheric Chemistry and Physics: From Air Pollution to Climate Change, 2nd edn., John Wiley &amp; Sons, New York, 2006.
</mixed-citation></ref-html>
<ref-html id="bib1.bib28"><label>Geffen et al.(2020)</label><mixed-citation>
van Geffen, J., Boersma, K. F., Eskes, H., Sneep, M., ter Linden, M., Zara, M., and Veefkind, J. P.: S5P TROPOMI NO<sub>2</sub> slant column retrieval: method, stability, uncertainties and comparisons with OMI, Atmos. Meas. Tech., 13, 1315–1335, <a href="https://doi.org/10.5194/amt-13-1315-2020" target="_blank">https://doi.org/10.5194/amt-13-1315-2020</a>, 2020.
</mixed-citation></ref-html>
<ref-html id="bib1.bib29"><label>Geffen et al.(2019)</label><mixed-citation>
van Geffen, J. H. G. M., Eskes, H. J., Boersma, K. F., Maasakkers, J. D., and Veefkind, J. P.:
TROPOMI ATBD of the total and tropospheric NO<sub>2</sub> data products,
S5P-KNMI-L2-0005-RP, Royal Netherlands Meteorological Institute, available at: <a href="https://sentinel.esa.int/documents/247904/2476257/Sentinel-5P-TROPOMI-ATBD-NO2-data-products" target="_blank"/> (last access: 21 June 2021),
2019.

</mixed-citation></ref-html>
<ref-html id="bib1.bib30"><label>Veefkind et al.(2012)</label><mixed-citation>
Veefkind, J. P., Aben, I., McMullan, K., Förster, H., de Vries, J., Otter, G., Claas, J., Eskes, H. J., de Haan, J. F., Kleipool, Q., van Weele, M., Hasekamp, O., Hoogeveen, R., Landgraf, J., Snel, R., Tol, P., Ingmann, P., Voors, R., Kruizinga, B., Vink, R., Visser, H., and Levelt, P. F.:
TROPOMI on the ESA Sentinel-5 Precursor: A GMES mission for global observations of the atmospheric composition for climate, air quality and ozone layer applications,
Remote Sens. Environ., 120, 70–83, <a href="https://doi.org/10.1016/j.rse.2011.09.027" target="_blank">https://doi.org/10.1016/j.rse.2011.09.027</a>, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib31"><label>Verhoelst et al.(2021)</label><mixed-citation>
Verhoelst, T., Compernolle, S., Pinardi, G., Lambert, J.-C., Eskes, H. J., Eichmann, K.-U., Fjæraa, A. M., Granville, J., Niemeijer, S., Cede, A., Tiefengraber, M., Hendrick, F., Pazmiño, A., Bais, A., Bazureau, A., Boersma, K. F., Bognar, K., Dehn, A., Donner, S., Elokhov, A., Gebetsberger, M., Goutail, F., Grutter de la Mora, M., Gruzdev, A., Gratsea, M., Hansen, G. H., Irie, H., Jepsen, N., Kanaya, Y., Karagkiozidis, D., Kivi, R., Kreher, K., Levelt, P. F., Liu, C., Müller, M., Navarro Comas, M., Piters, A. J. M., Pommereau, J.-P., Portafaix, T., Prados-Roman, C., Puentedura, O., Querel, R., Remmers, J., Richter, A., Rimmer, J., Rivera Cárdenas, C., Saavedra de Miguel, L., Sinyakov, V. P., Stremme, W., Strong, K., Van Roozendael, M., Veefkind, J. P., Wagner, T., Wittrock, F., Yela González, M., and Zehner, C.: Ground-based validation of the Copernicus Sentinel-5P TROPOMI NO<sub>2</sub> measurements with the NDACC ZSL-DOAS, MAX-DOAS and Pandonia global networks, Atmos. Meas. Tech., 14, 481–510, <a href="https://doi.org/10.5194/amt-14-481-2021" target="_blank">https://doi.org/10.5194/amt-14-481-2021</a>, 2021.
</mixed-citation></ref-html>
<ref-html id="bib1.bib32"><label>Virtanen et al.(2020)</label><mixed-citation>
Virtanen, P., Gommers, R., Oliphant, T. E., Haberland, M., Reddy, T., Cournapeau, D., Burovski, E., Peterson, P., Weckesser, W., Bright, J., van der Walt, S. J., Brett, M., Wilson, J., Millman, K. J., Mayorov, N., Nelson, A. R. J., Jones, E., Kern, R., Larson, E., Carey, C. J., Polat, İ., Feng, Y., Moore, E. W., VanderPlas, J., Laxalde, D., Perktold, J., Cimrman, R., Henriksen, I., Quintero, E. A., Harris, C. R., Archibald, A. M., Ribeiro, A. H., Pedregosa, F., and van Mulbregt, P.:
SciPy 1.0: fundamental algorithms for scientific computing in Python,
Nat. Methods, 17, 261–272, <a href="https://doi.org/10.1038/s41592-019-0686-2" target="_blank">https://doi.org/10.1038/s41592-019-0686-2</a>, 2020.
</mixed-citation></ref-html>
<ref-html id="bib1.bib33"><label>Wagner et al.(2007)</label><mixed-citation>
Wagner, T., Burrows, J. P., Deutschmann, T., Dix, B., von Friedeburg, C., Frieß, U., Hendrick, F., Heue, K.-P., Irie, H., Iwabuchi, H., Kanaya, Y., Keller, J., McLinden, C. A., Oetjen, H., Palazzi, E., Petritoli, A., Platt, U., Postylyakov, O., Pukite, J., Richter, A., van Roozendael, M., Rozanov, A., Rozanov, V., Sinreich, R., Sanghavi, S., and Wittrock, F.: Comparison of box-air-mass-factors and radiances for Multiple-Axis Differential Optical Absorption Spectroscopy (MAX-DOAS) geometries calculated from different UV/visible radiative transfer models, Atmos. Chem. Phys., 7, 1809–1833, <a href="https://doi.org/10.5194/acp-7-1809-2007" target="_blank">https://doi.org/10.5194/acp-7-1809-2007</a>, 2007.
</mixed-citation></ref-html>--></article>
