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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-19-3963-2019</article-id><title-group><article-title>Emissions of methane in Europe inferred by<?xmltex \hack{\break}?> total column measurements</article-title><alt-title>TCCON-derived European methane</alt-title>
      </title-group><?xmltex \runningtitle{TCCON-derived European methane}?><?xmltex \runningauthor{D. Wunch et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Wunch</surname><given-names>Debra</given-names></name>
          <email>dwunch@atmosp.physics.utoronto.ca</email>
        <ext-link>https://orcid.org/0000-0002-4924-0377</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Jones</surname><given-names>Dylan B. A.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Toon</surname><given-names>Geoffrey C.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff4">
          <name><surname>Deutscher</surname><given-names>Nicholas M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2906-2577</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Hase</surname><given-names>Frank</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Notholt</surname><given-names>Justus</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Sussmann</surname><given-names>Ralf</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Warneke</surname><given-names>Thorsten</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Kuenen</surname><given-names>Jeroen</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Denier van der Gon</surname><given-names>Hugo</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9552-3688</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Fisher</surname><given-names>Jenny A.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2921-1691</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8">
          <name><surname>Maasakkers</surname><given-names>Joannes D.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Department of Physics, University of Toronto, Toronto, Ontario, Canada</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Centre for Atmospheric Chemistry, University of Wollongong, Wollongong, New South Wales, Australia</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Institute of Environmental Physics, University of Bremen, Germany</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Karlsruhe Institute of Technology, IMK-ASF, Karlsruhe, Germany</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Karlsruhe Institute of Technology, IMK-IFU, Garmisch-Partenkirchen, Germany</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>TNO Dept Climate, Air and Sustainability, Utrecht, the Netherlands</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>School of Engineering and Applied Sciences, Harvard University, Cambridge, Massachusetts, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Debra Wunch (dwunch@atmosp.physics.utoronto.ca)</corresp></author-notes><pub-date><day>28</day><month>March</month><year>2019</year></pub-date>
      
      <volume>19</volume>
      <issue>6</issue>
      <fpage>3963</fpage><lpage>3980</lpage>
      <history>
        <date date-type="received"><day>12</day><month>March</month><year>2018</year></date>
           <date date-type="rev-request"><day>7</day><month>May</month><year>2018</year></date>
           <date date-type="rev-recd"><day>15</day><month>March</month><year>2019</year></date>
           <date date-type="accepted"><day>17</day><month>March</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 Debra Wunch et al.</copyright-statement>
        <copyright-year>2019</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019.html">This article is available from https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e231">Using five long-running ground-based atmospheric observatories in
Europe, we demonstrate the utility of long-term, stationary, ground-based
measurements of atmospheric total columns for verifying annual methane
emission inventories. Our results indicate that the methane emissions for the
region in Europe between Orléans, Bremen, Białystok, and
Garmisch-Partenkirchen are overestimated by the state-of-the-art inventories
of the Emissions Database for Global Atmospheric Research (EDGAR) v4.2 FT2010
and the high-resolution emissions database developed by the Netherlands Organisation for Applied Scientific Research (TNO) as part of the Monitoring
Atmospheric Composition and Climate project (TNO-MACC_III), possibly due to the
disaggregation of emissions onto a spatial grid. Uncertainties in the carbon
monoxide inventories used to compute the methane emissions contribute to the
discrepancy between our inferred emissions and those from the
inventories.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e243">Recent global policy agreements have led to renewed efforts to reduce
greenhouse gas emissions to cap global temperature rise (e.g., Conference of
the Parties 21, <xref ref-type="bibr" rid="bib1.bibx56" id="altparen.1"><named-content content-type="pre">COP 21;</named-content></xref>; <xref ref-type="bibr" rid="bib1.bibx14" id="altparen.2"/>).
This, in turn, has motivated countries to seek methods of reducing their
greenhouse gas emissions. In Europe, methane emissions account for a
significant fraction (about 11 % by mass of <inline-formula><mml:math id="M1" 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> equivalent) of the
total greenhouse gas emissions <xref ref-type="bibr" rid="bib1.bibx57" id="paren.3"/>. The lifetime of
atmospheric methane is significantly shorter than for carbon dioxide, its
100-year global warming potential is significantly larger, and it is at near
steady state in the atmosphere; therefore, significant reductions in methane
emissions are an effective short-term strategy for reducing greenhouse gas
emissions <xref ref-type="bibr" rid="bib1.bibx10" id="paren.4"/>. Emission reduction strategies that include
both methane emission reductions and carbon dioxide reductions are thought to
be among the most effective at slowing the increase in global temperatures
<xref ref-type="bibr" rid="bib1.bibx48" id="paren.5"/>. Thus, it is important to know exactly how
much methane is being emitted and the geographic and temporal source of the
emissions. This requires an approach that combines state-of-the-art emissions
inventories that contain information about the specific point and area
sources of the known emissions and timely and long-term measurements of
greenhouse gases in the atmosphere to verify that the emissions reduction
targets are met.</p>
      <p id="d1e275">Because atmospheric methane is well-mixed and has a lifetime of about 12 years <xref ref-type="bibr" rid="bib1.bibx52" id="paren.6"/>, it is<?pagebreak page3964?> transported far from its emission source,
making source attribution efforts challenging from atmospheric measurements
alone. Atmospheric measurements are often assimilated into “flux inversion”
models to locate the sources of the emissions <xref ref-type="bibr" rid="bib1.bibx24" id="paren.7"><named-content content-type="pre">e.g.,</named-content></xref>
but rely on model wind fields to drive transport, and they also tend to have spatial
resolutions that do not resolve subregional scales. Methane measurement
schemes that constrain emissions on local and regional scales are thus
important to help identify the sources of the emissions and to verify
inventory analyses. Regional- or national-scale emissions are important to
public policy as those emissions are reported annually to the United Nations
Framework Convention on Climate Change (UNFCCC).</p>
      <p id="d1e286">The atmospheric measurement techniques that are used to estimate methane
emissions include measurements made in situ, either on the ground, from tall
towers, or from aircraft. Remote sensing techniques are also used, either
from space or from the ground. The spatial scale of the sensitivity to
emissions differs with the measurement technique: surface in situ measurements
provide information about local emissions on urban scales <xref ref-type="bibr" rid="bib1.bibx37 bib1.bibx23" id="paren.8"><named-content content-type="pre">e.g.,</named-content></xref>, and aircraft in situ measurements can provide
information about regional- and synoptic-scale fluxes <xref ref-type="bibr" rid="bib1.bibx26 bib1.bibx30 bib1.bibx31 bib1.bibx63 bib1.bibx3 bib1.bibx18 bib1.bibx29" id="paren.9"><named-content content-type="pre">e.g.,</named-content></xref>.
Satellite remote sensing techniques provide information useful for extracting
emission information on larger scales (regional to global) <xref ref-type="bibr" rid="bib1.bibx49 bib1.bibx47 bib1.bibx1 bib1.bibx55" id="paren.10"><named-content content-type="pre">e.g.,</named-content></xref> and for large point or
urban sources <xref ref-type="bibr" rid="bib1.bibx32 bib1.bibx33 bib1.bibx40" id="paren.11"><named-content content-type="pre">e.g.,</named-content></xref>. Several studies
have shown the importance of simultaneous measurements of co-emitted species
<xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx50 bib1.bibx43 bib1.bibx49 bib1.bibx22 bib1.bibx68 bib1.bibx27" id="paren.12"><named-content content-type="pre">e.g., <inline-formula><mml:math id="M2" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M3" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M4" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M5" 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>,</named-content></xref>
or co-located measurements <xref ref-type="bibr" rid="bib1.bibx64 bib1.bibx68" id="paren.13"><named-content content-type="pre">e.g.,</named-content></xref>, showing the
added analytical power of the combination of atmospheric tracer information.
Ground-based remote sensing instruments have been used to estimate methane
emissions on urban <xref ref-type="bibr" rid="bib1.bibx64 bib1.bibx21 bib1.bibx68" id="paren.14"><named-content content-type="pre">e.g.,</named-content></xref> and
sub-urban <xref ref-type="bibr" rid="bib1.bibx6 bib1.bibx59" id="paren.15"><named-content content-type="pre">e.g.,</named-content></xref> scales. In <xref ref-type="bibr" rid="bib1.bibx21" id="text.16"/>,
<xref ref-type="bibr" rid="bib1.bibx59" id="text.17"/>, and <xref ref-type="bibr" rid="bib1.bibx6" id="text.18"/>, the authors have placed mobile
ground-based remote sensing instruments around a particular emitter of
interest (e.g., a city, dairy, or neighborhood) and have designed short-term
campaigns to measure the difference between upwind and downwind atmospheric
methane abundances. From these differences the authors have computed
emission fluxes. However, there is a network of nonmobile ground-based
remote sensing instruments that have been collecting long-term measurements
of atmospheric greenhouse gas abundances. These instruments were not placed
intentionally around an emitter of interest, but collectively they ought to
contain information about nearby emissions. To date, there have been no
studies that have attempted to extract regional methane emission information
from these existing ground-based remote sensing observatories.</p>
      <p id="d1e385">In this paper, we will describe our methods for computing the emissions of
methane using five stationary ground-based remote sensing instruments located
in Europe in Sect. <xref ref-type="sec" rid="Ch1.S2"/>. Our results and comparisons to the
state-of-the-art inventories are shown in Sect. <xref ref-type="sec" rid="Ch1.S3"/>, and we summarize
our results in Sect. <xref ref-type="sec" rid="Ch1.S4"/>.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
      <p id="d1e402">Our study area is the region between five long-running atmospheric
observatories situated in Europe. Three of the stations are in Germany:
Bremen <xref ref-type="bibr" rid="bib1.bibx41" id="paren.19"/>, Karlsruhe <xref ref-type="bibr" rid="bib1.bibx20" id="paren.20"/>,
and Garmisch-Partenkirchen <xref ref-type="bibr" rid="bib1.bibx53" id="paren.21"/>. The other two are in Poland
<xref ref-type="bibr" rid="bib1.bibx9" id="paren.22"><named-content content-type="pre">Białystok,</named-content></xref> and France
<xref ref-type="bibr" rid="bib1.bibx60" id="paren.23"><named-content content-type="pre">Orléans,</named-content></xref>. Each station measures the
vertical column-averaged dry-air mole fraction of carbon dioxide
(<inline-formula><mml:math id="M6" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>), carbon monoxide (<inline-formula><mml:math id="M7" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), methane
(<inline-formula><mml:math id="M8" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>), and other trace gas species. The locations are shown in
Fig. <xref ref-type="fig" rid="Ch1.F1"/>, overlaid on a nighttime light image from the
National Aeronautics and Space Administration (NASA) to provide a sense of
the population density of the area. These observatories are part of the Total
Carbon Column Observing Network <xref ref-type="bibr" rid="bib1.bibx66" id="paren.24"><named-content content-type="pre">TCCON,</named-content></xref> and have
been tied to the World Meteorological Organization trace-gas scale through
comparisons with vertically integrated, calibrated in situ profiles over the
observatories <xref ref-type="bibr" rid="bib1.bibx65 bib1.bibx67 bib1.bibx38 bib1.bibx19" id="paren.25"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><label>Figure 1</label><caption><p id="d1e478">The locations of the TCCON observatories overlaid on a NASA
nighttime
light image. From west to east, the stations are Orléans (or, pink),
Karlsruhe (ka, green), Bremen (br, blue-green), Garmisch-Partenkirchen (gm,
orange), and Białystok (bi, purple).</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f01.jpg"/>

      </fig>

      <p id="d1e487">Following a similar method to <xref ref-type="bibr" rid="bib1.bibx64 bib1.bibx68" id="text.26"/>, we estimate
emissions of methane from the data recorded from the TCCON observatories,
coupled with gridded inventories of carbon monoxide within the region. We
compute changes (or “anomalies”) in <inline-formula><mml:math id="M9" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M10" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> that
we will refer to as <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M12" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and we then
compute the slopes relating <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M14" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.
From the computed slopes (<inline-formula><mml:math id="M15" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>), we can infer emissions of methane
(E<inline-formula><mml:math id="M16" display="inline"><mml:msub><mml:mi/><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula>) if emissions of carbon monoxide (E<inline-formula><mml:math id="M17" display="inline"><mml:msub><mml:mi/><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>, in mass per
unit time) are known, using the following relationship:
          <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M18" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="normal">E</mml:mi><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:msub><mml:mi mathvariant="normal">E</mml:mi><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math id="M19" display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula> is the ratio of the molecular masses of <inline-formula><mml:math id="M20" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M21" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d1e701">In <xref ref-type="bibr" rid="bib1.bibx64 bib1.bibx68" id="text.27"/>, measurements from a single
atmospheric observatory were used to infer emissions because the unique
dynamics of the region advected the polluted air mass into and out of the
study area diurnally. In this paper, we rely on several stations to provide
measurements of the boundary of the study region to measure <inline-formula><mml:math id="M22" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M23" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emitted between the stations. This analysis relies on a few
assumptions about the nature of the emissions. First, that the lifetimes of
the gases of interest are longer than the transport<?pagebreak page3965?> time within the region.
This is the case both for methane, which has an atmospheric lifetime of 12 years, and for carbon monoxide, which has an atmospheric lifetime of a few
weeks. Second, we assume that typical emissions are consistent over time
periods longer than a few days so that they are advected together. The nature
of the emissions in this region (mostly residential and industrial energy
needs) supports this assumption. Third, we assume that the spatial
distribution of the emissions is similar for <inline-formula><mml:math id="M24" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M25" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>, as
confirmed by the inventory maps (Fig. <xref ref-type="fig" rid="App1.Ch1.F3"/>). This method
does not require carbon monoxide and methane to be co-emitted (as they
generally do not have the same emissions sources).</p>
      <p id="d1e748">To compute anomalies and slopes, we first filter the data to minimize the
impact of data sparsity and air mass differences between stations (Appendix
<xref ref-type="sec" rid="App1.Ch1.S1"/>). Then, for each station, the daily median value is
subtracted from each measurement. This reduces the impact of the station
altitude and any background seasonal cycle from aliasing into the results.
Subsequently, we compute the differences in the <inline-formula><mml:math id="M26" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M27" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> abundances measured at the same solar zenith and solar azimuth
angles on the same day at two TCCON stations. By computing anomalies at the
same solar zenith angles, we minimize any impact that air-mass-dependent
biases could have on the calculated anomalies. This analysis is repeated for
all combinations of pairs of stations within the study area. The vertical
sensitivity of the TCCON measurements is explicitly taken into account by
dividing the anomalies by the surface layer column averaging kernel value, as
we assume that the anomalies are due to emissions near the surface. The
slopes computed for each year and each pair of stations are shown in
Fig. <xref ref-type="fig" rid="Ch1.F2"/>.</p>
      <p id="d1e781">The farthest distance between the European TCCON stations included in this
study is between Orléans and Białystok (1580 <inline-formula><mml:math id="M28" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>).
Climatological annual mean surface wind speeds from the National Centers for
Environmental Prediction (NCEP) and National Center for Atmospheric Research
(NCAR) reanalysis <xref ref-type="bibr" rid="bib1.bibx28" id="paren.28"/> within the study area are about
6 <inline-formula><mml:math id="M29" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="App1.Ch1.F1"/>). The air from
Orléans will quickly mix vertically from the surface where the winds
aloft are more rapid than at the surface (see Appendix <xref ref-type="sec" rid="App1.Ch1.S2"/>).
Thus, air from Orléans would normally reach Białystok in a few days.
To determine whether these anomalies are consistent throughout the transport
time through the study area, we compute anomalies between sites lagged by up
to 14 days. The slopes of the anomalies do not change significantly or
systematically with the lag time (Appendix <xref ref-type="sec" rid="App1.Ch1.S2"/>; Fig. <xref ref-type="fig" rid="App1.Ch1.F2"/>), presumably because the atmospheric composition within
the study area is relatively well-mixed or because the emissions are
relatively consistent from day to day within the study area.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><label>Figure 2</label><caption><p id="d1e823">The bars show the methane to carbon monoxide anomaly slopes for each
site pair. The method of computing these anomaly slopes is detailed in Sect. <xref ref-type="sec" rid="Ch1.S2"/> of the main text. The black targets indicate the median
value of the slope for that year, when all site pairs are considered
simultaneously, and the 25th and 75th quartiles of the median
value are indicated by the vertical black bars. Outliers are indicated by
open black circles.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f02.png"/>

      </fig>

      <?pagebreak page3966?><p id="d1e834">Previous papers have used carbon dioxide instead of carbon monoxide to infer
methane emissions. We choose to compute emissions using measurements of
<inline-formula><mml:math id="M30" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> instead of <inline-formula><mml:math id="M31" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> in this work because the natural
<inline-formula><mml:math id="M32" 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> fluxes in the region are large compared with the anthropogenic
emissions, and they have a strong diurnal and seasonal cycle. The distance
between the stations is large enough that local (sub-daily) uptake of
<inline-formula><mml:math id="M33" 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> differs from station to station, significantly obscuring the
relationships between methane and carbon dioxide, and thus the anomaly
slopes, especially in the summer months. While the emissions inventory of
anthropogenic <inline-formula><mml:math id="M34" 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> may be more accurate than the <inline-formula><mml:math id="M35" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> inventory
in the region, the presence of these large natural fluxes of <inline-formula><mml:math id="M36" 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>
precludes its use in the anomaly slope calculation. The accuracy of our
method, therefore, is limited by the accuracy of the carbon monoxide emission
inventory. Fires could provide a large flux of <inline-formula><mml:math id="M37" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> without a large
<inline-formula><mml:math id="M38" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> flux, and this should also be taken into consideration in these
types of analyses. In our study area fluxes from fires are small.</p>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Inventories</title>
      <p id="d1e943">To obtain an estimate of carbon monoxide emissions (<inline-formula><mml:math id="M39" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">E</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) within the
study area, we use gridded inventories and sum the emissions within the
study area to compare with our emissions inferred from the TCCON measurements
(see Appendix <xref ref-type="sec" rid="App1.Ch1.S3"/> and Fig. <xref ref-type="fig" rid="App1.Ch1.F3"/>
for details). The two inventories employed here are the Emissions Database for
Global Atmospheric Research (EDGAR) and the Netherlands Organisation for Applied Scientific Research (TNO)
high-resolution emissions database developed as part of the Monitoring Atmospheric
Composition and Climate project (TNO-MACC_III). The EDGAR version
v4.3.1_v2 of January 2016 annual gridded inventory is available at
<inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.1</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:mn mathvariant="normal">0.1</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> spatial resolution and reports global emissions
from the year 2000 to 2010 <xref ref-type="bibr" rid="bib1.bibx42 bib1.bibx11" id="paren.29"/>. The
TNO-MACC_III inventory is a Europe-specific air quality emissions inventory,
available on a <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.125</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:mn mathvariant="normal">0.0625</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> grid, and reports emissions
for 2000–2011 <xref ref-type="bibr" rid="bib1.bibx34" id="paren.30"/>. Both EDGAR and
TNO-MACC_III provide spatially and temporally coincident methane inventories
which we use to compare with our inferred emissions. We use the EDGAR version
v4.2 FT2010 and the TNO-MACC_III methane inventories.</p>
      <p id="d1e1008">Using country-level emissions reported through 2015 from the European
Environment Agency <xref ref-type="bibr" rid="bib1.bibx12" id="paren.31"/>, we extrapolate the EDGAR and
TNO-MACC_III
gridded inventory CO emissions for the study area through 2015. This
facilitates more direct comparisons with the TCCON measurements, which begin
with sufficient data for our study in 2009. We extrapolate the emissions by
scaling the total emissions from the countries that are intersected by the
area of interest (Germany, Poland, Belgium, France, Luxembourg, and the Czech
Republic) to the last reported year of emissions from the inventory. We then
assume that the same scaling factor applies for each subsequent year. The
details of the extrapolation method are in Appendix <xref ref-type="sec" rid="App1.Ch1.S4"/>
and Figs. <xref ref-type="fig" rid="App1.Ch1.F4"/> and <xref ref-type="fig" rid="App1.Ch1.F5"/>.</p>
      <p id="d1e1020">The time series of the reported emissions from 2000 to 2015 are shown in
Fig. <xref ref-type="fig" rid="Ch1.F3"/>. The inventories and scaled<?pagebreak page3967?> country-level
reported emissions for this region suggest that emissions of <inline-formula><mml:math id="M42" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M43" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> have decreased by about 40 % and 20 %, respectively, between 2000
and 2015. The TNO-MACC_III carbon monoxide emissions are on average 15 %
higher than the EDGAR v.4.3.1 emissions in the study area. The total
TNO-MACC_III and EDGAR methane emissions agree to within 2 % in the study
area.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><label>Figure 3</label><caption><p id="d1e1047">This figure shows the summed EDGAR (green) and TNO-MACC_III
(orange) emissions within the study area for <inline-formula><mml:math id="M44" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> (squares) and
<inline-formula><mml:math id="M45" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (triangles). The study area is defined in Fig. <xref ref-type="fig" rid="Ch1.F1"/>. All emissions are shown
in units of <inline-formula><mml:math id="M46" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Tg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">yr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. Extrapolation begins after 2010 for EDGAR and 2011 for
TNO-MACC_III.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f03.png"/>

        </fig>

      <p id="d1e1094">An earlier version of the EDGAR carbon monoxide inventory was evaluated by
<xref ref-type="bibr" rid="bib1.bibx51" id="text.32"/> and
<xref ref-type="bibr" rid="bib1.bibx17" id="text.33"/>, who assimilated satellite
measurements of <inline-formula><mml:math id="M47" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> using the EDGAR v3.3FT2000 <inline-formula><mml:math id="M48" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions
inventory as the a priori. <xref ref-type="bibr" rid="bib1.bibx51" id="text.34"/> found that,
over Europe, the a posteriori emissions increase by less than 15 % when
assimilating carbon monoxide from the Measurements of Pollution in the
Troposphere (MOPITT) satellite instrument <xref ref-type="bibr" rid="bib1.bibx13" id="paren.35"/>.
<xref ref-type="bibr" rid="bib1.bibx17" id="text.36"/> assimilated Infrared Atmospheric
Sounding Interferometer (IASI) <inline-formula><mml:math id="M49" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>
<xref ref-type="bibr" rid="bib1.bibx7" id="paren.37"/> and MOPITT <inline-formula><mml:math id="M50" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and found that
the a posteriori emissions increase by 16 % and 45 %, respectively.</p>
      <p id="d1e1148">The more recent EDGAR v4.3.1 <inline-formula><mml:math id="M51" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions in our study are 24 % lower
than the EDGAR v3.3FT2000 <inline-formula><mml:math id="M52" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions for the year 2000, so it may be
that the EDGAR v4.3.1 <inline-formula><mml:math id="M53" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions are significantly underestimated.
However, assimilations of <inline-formula><mml:math id="M54" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> are known to be very sensitive to the
chemistry described in the model: most notably the <inline-formula><mml:math id="M55" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:math></inline-formula> chemistry
<xref ref-type="bibr" rid="bib1.bibx44 bib1.bibx69" id="paren.38"/>. Therefore, it is
difficult to determine how much of the discrepancy between versions of the
model is from the inventory or the model chemistry.</p>
      <p id="d1e1195">The EDGAR methane inventory has been evaluated in several previous studies.
It has been shown to overestimate regional <inline-formula><mml:math id="M56" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions
<xref ref-type="bibr" rid="bib1.bibx64 bib1.bibx62" id="paren.39"><named-content content-type="pre">e.g.,</named-content></xref> but to underestimate oil and gas
emissions <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx5" id="paren.40"><named-content content-type="pre">e.g.,</named-content></xref>.
However, recent methane isotope analysis by <xref ref-type="bibr" rid="bib1.bibx45" id="text.41"/> has
suggested that the EDGAR inventory overestimates fossil-fuel-related
emissions. The study area of interest here has little oil and gas production,
except for some test sites in Poland <xref ref-type="bibr" rid="bib1.bibx58" id="paren.42"/>, no
commercial shale gas industry, and few pipelines.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Model experiment</title>
      <p id="d1e1233">To test whether the anomaly method described in Sect. <xref ref-type="sec" rid="Ch1.S2"/> can
accurately infer methane emissions, we conducted a modeling experiment using
version v12.1.0 of the GEOS-Chem model (<uri>http://www.geos-chem.org</uri>, last access: 4 January 2019) to simulate
methane and carbon monoxide for the year 2010. The model is driven by the
Modern-Era Retrospective analysis for Research and Applications, version 2
(MERRA-2) meteorology from the NASA Global Modeling and Assimilation Office.
The native resolution of the meteorological fields is <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.25</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:mn mathvariant="normal">0.3125</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, with 72 vertical levels from the surface to
0.01 <inline-formula><mml:math id="M58" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">hPa</mml:mi></mml:mrow></mml:math></inline-formula>, which we degraded to <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:mn mathvariant="normal">2.5</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and 47 vertical levels. We use the linear <inline-formula><mml:math id="M60" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>-only and <inline-formula><mml:math id="M61" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-only
simulations of GEOS-Chem, with prescribed monthly mean <inline-formula><mml:math id="M62" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:math></inline-formula> fields. In
the <inline-formula><mml:math id="M63" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>-only simulation, global anthropogenic emissions are from EDGAR
v4.3.1, which are overwritten regionally with the following emissions: the
Cooperative Programme for Monitoring and Evaluation of the Long-range
Transmission of Air Pollutants in Europe (EMEP), the U.S. Environmental
Protection Agency National Emission Inventory for 2011 (NEI2011), the MIX
inventory for Asia, the Visibility Observational (BRAVO) Study Emissions
Inventory for Mexico, and the criteria air contaminants (CAC) inventory for
Canada. The sources of <inline-formula><mml:math id="M64" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> from the oxidation of <inline-formula><mml:math id="M65" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and
volatile organic compounds (VOCs) are prescribed following
<xref ref-type="bibr" rid="bib1.bibx16" id="text.43"/>. For the <inline-formula><mml:math id="M66" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-only simulation, the emissions are as
described in <xref ref-type="bibr" rid="bib1.bibx36" id="text.44"/>. Global anthropogenic
emissions are from EDGAR v4.3.2, but the US emissions were replaced with
those from <xref ref-type="bibr" rid="bib1.bibx35" id="text.45"/>, and emissions from
wetlands are from WetCHARTs version 1.0 <xref ref-type="bibr" rid="bib1.bibx4" id="paren.46"/>. For both <inline-formula><mml:math id="M67" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math id="M68" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> simulations, emissions from biomass burning are from the
Quick Fire Emissions Dataset (QFED) <xref ref-type="bibr" rid="bib1.bibx8" id="paren.47"/>. The biomass
burning in the study area produces less than 2 % of the total anthropogenic
emissions of <inline-formula><mml:math id="M69" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><label>Figure 4</label><caption><p id="d1e1401">This figure compares seasonally averaged modeled total <inline-formula><mml:math id="M70" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
with the <inline-formula><mml:math id="M71" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contribution from emissions in Europe. Each season has
two maps: the left map shows the total <inline-formula><mml:math id="M72" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and the right map shows
the contribution from European emissions (<inline-formula><mml:math id="M73" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:mi mathvariant="normal">CO</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Eur</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>). The spatial
pattern of the gradients in modeled <inline-formula><mml:math id="M74" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> between the TCCON stations
is reflected in the European contribution.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f04.png"/>

        </fig>

      <?pagebreak page3968?><p id="d1e1470">We used identical <inline-formula><mml:math id="M75" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:math></inline-formula> fields (from version v7-02-03 of GEOS-Chem) for
the <inline-formula><mml:math id="M76" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M77" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> simulations, so that the chemical losses of
methane and carbon monoxide are consistent, and ran tagged <inline-formula><mml:math id="M78" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>
experiments so that we could identify the source of the emissions. The model
atmospheric carbon monoxide and methane profiles were integrated to compute
simulated <inline-formula><mml:math id="M79" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M80" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>. To illustrate the sensitivity of
the modeled fields to European emissions, we show the seasonal means of the modeled <inline-formula><mml:math id="M81" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
sampled at the five TCCON stations in Fig. <xref ref-type="fig" rid="Ch1.F4"/>. Also plotted is the column contribution
(<inline-formula><mml:math id="M82" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:mi mathvariant="normal">CO</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Eur</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) from <inline-formula><mml:math id="M83" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions only in Europe (defined as the
broader region between 0–45<inline-formula><mml:math id="M84" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E and 45–55<inline-formula><mml:math id="M85" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N). As can be seen, the spatial pattern of the differences in
modeled <inline-formula><mml:math id="M86" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> between the TCCON stations is reflected in
<inline-formula><mml:math id="M87" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:mi mathvariant="normal">CO</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Eur</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>. We calculated the anomalies in <inline-formula><mml:math id="M88" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M89" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:mi mathvariant="normal">CO</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Eur</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, using the same approach employed with the atmospheric
data, and found that the anomalies in <inline-formula><mml:math id="M90" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:mi mathvariant="normal">CO</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Eur</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, which represent the
direct influence of European emissions on atmospheric CO, account for about
35 % of the anomalies in <inline-formula><mml:math id="M91" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. This confirms that the <inline-formula><mml:math id="M92" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
anomalies between the TCCON stations are sensitive to European emissions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><label>Figure 5</label><caption><p id="d1e1687">This figure shows the results from the modeling experiment using
GEOS-Chem. Panel <bold>(a)</bold> shows the model <inline-formula><mml:math id="M93" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M94" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> slopes for each month and pair of stations (indicated by the
colors). The median slopes for each month are overlaid with grey squares. Panel <bold>(b)</bold> shows the model carbon monoxide emissions (excluding VOC
and methane oxidation) and the model methane emissions. The inferred methane
emissions from our tracer–tracer slope method are plotted in pink squares.
Panel <bold>(c)</bold> shows the annual methane emissions from the
tracer–tracer slope method and the
model.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f05.png"/>

        </fig>

      <p id="d1e1735">To estimate the modeled <inline-formula><mml:math id="M95" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions using the modeled <inline-formula><mml:math id="M96" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>,
the modeled <inline-formula><mml:math id="M97" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M98" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> were interpolated to the
locations of the TCCON stations and anomalies and slopes were computed. We
then applied Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>) to our anomaly slopes to compute
methane emissions from the known <inline-formula><mml:math id="M99" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions, accounting for only the
<inline-formula><mml:math id="M100" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions from anthropogenic, biomass burning, and biofuel sources.
We neglect sources of <inline-formula><mml:math id="M101" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions from the oxidation of <inline-formula><mml:math id="M102" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
and VOCs because the column enhancements for those emissions are relatively
spatially uniform across this region of Europe, and thus they should not contribute
significantly to the anomalies. The resulting annual <inline-formula><mml:math id="M103" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions
agree well with the model emissions: the inferred emissions from the anomaly
analysis are higher than the model emissions by less than 2 % (Fig. <xref ref-type="fig" rid="Ch1.F5"/>).</p>
      <p id="d1e1834">While the inferred annual emissions agree well with the modeled annual
emissions, the seasonal pattern of the emissions inferred from the anomaly
analysis differs from that of the model. The anomaly analysis overestimates
emissions in the winter and underestimates emissions in the summer. This may
be due to small spatial inhomogeneities in the column enhancements from VOC
(biogenic) emissions that influence the anomaly analysis most in summertime
when VOC emissions are largest. Including the VOC emissions in the total
carbon monoxide emissions leads us to infer annual methane emissions that are
overestimated by 15 %, increasing the inferred summertime emissions without
significantly changing the inferred wintertime emissions.</p>
      <p id="d1e1837">The seasonal analysis suggests that the 2 % agreement in the annual emission
estimate may reflect the compensating effects of discrepancies over the
seasonal cycle, and improving the seasonal estimate may require a better
treatment of the VOC contribution to atmospheric <inline-formula><mml:math id="M104" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>. Nevertheless, the
results here suggest that for this region of Europe, where VOC and methane
oxidation emissions lead to relatively spatially uniform column enhancements
and fire emissions are small, we can successfully use the anomaly method
described in Sect. <xref ref-type="sec" rid="Ch1.S2"/> to infer annual methane emissions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><label>Figure 6</label><caption><p id="d1e1852">The black line is the summed EDGAR (green) and TNO-MACC_III
(orange) methane emissions within the study area shown in Fig. <xref ref-type="fig" rid="Ch1.F1"/>. The grey lines indicate the projected emissions
based on scaling the country-level emissions reported by the UNFCCC
<xref ref-type="bibr" rid="bib1.bibx57" id="paren.48"/> to the area emissions in 2010 for EDGAR and 2011 for
TNO-MACC_III. The lower solid lines show the emissions inferred from the
TCCON anomaly analysis using CO emissions from the two models, and the dashed
lines indicate the 5th and 95th percentiles.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f06.png"/>

        </fig>

</sec>
</sec>
<?pagebreak page3969?><sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
      <p id="d1e1875">To compute methane emissions, we apply Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>) to our
anomaly slopes and the inventory-reported carbon monoxide emissions in the
study region (Fig. <xref ref-type="fig" rid="Ch1.F6"/>). If we choose the mean of the
reported <inline-formula><mml:math id="M105" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions from EDGAR v4.3.1 and TNO-MACC_III, the methane
emissions we compute within the study area based on the TCCON measurements
are <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.7</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M107" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Tg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">yr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> in 2009, with a non-monotonic decrease
to <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.2</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M109" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Tg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">yr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> in 2015. The uncertainties quoted here
are from the standard errors on the data slope fitting only; we have not
included uncertainties from the inventories. The magnitude of methane
emissions we compute from the TCCON data are, on average, about 2.3 times
lower than the methane emissions reported by EDGAR and about 2 times lower
than the methane emissions reported by TNO-MACC_III.</p>
      <p id="d1e1949">Our method of inferring methane emissions depends critically on the carbon
monoxide inventory. The carbon monoxide emissions for 2010 in the study area
from our GEOS-Chem model run, derived from EMEP emissions, were
6.4 <inline-formula><mml:math id="M110" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Tg</mml:mi></mml:mrow></mml:math></inline-formula>, about 35 % higher than the average of the EDGAR and
TNO-MACC_III emissions for that year. This magnitude underestimate has also
been suggested by <xref ref-type="bibr" rid="bib1.bibx51" id="text.49"/> and
<xref ref-type="bibr" rid="bib1.bibx17" id="text.50"/> using independent data. Using the
GEOS-Chem carbon monoxide<?pagebreak page3970?> emissions increases the methane emissions inferred
by the anomaly analysis to <inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.4</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M112" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Tg</mml:mi></mml:mrow></mml:math></inline-formula> in 2010. This value remains
lower than the EDGAR and TNO-MACC_III methane emissions estimates for 2010,
which are 3 <inline-formula><mml:math id="M113" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Tg</mml:mi></mml:mrow></mml:math></inline-formula>, but by only 20 %. Therefore, we find that the
inventories likely overestimate methane emissions, but the accuracy of our
results relies on the accuracy of the carbon monoxide inventory.</p>
      <p id="d1e1995">Although the EDGAR and TNO-MACC_III inventories agree to within 15 % in
carbon monoxide emissions and 2 % in methane emissions in the study region,
they spatially distribute these emissions differently. Maps of the spatial
differences between the TNO-MACC_III and EDGAR emissions are shown in Fig. <xref ref-type="fig" rid="Ch1.F7"/> for carbon monoxide and Fig. <xref ref-type="fig" rid="Ch1.F8"/> for methane. EDGAR estimates larger emissions of
carbon monoxide from the main cities in the study region and the surrounding
areas. This is clearly visible from the difference map (Fig. <xref ref-type="fig" rid="Ch1.F7"/>), where cities such as Hamburg, Berlin, Prague,
Wrocław, Warsaw, Munich, Paris, and Vienna appear in blue. However, the
overall carbon monoxide emissions from TNO-MACC_III in the study area are
higher than EDGAR, and this comes from regions between the main cities,
particularly in Poland and eastern France.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><label>Figure 7</label><caption><p id="d1e2007">This map shows the difference between the TNO-MACC_III carbon
monoxide emissions and the EDGAR emissions for the year 2010. The black
straight lines delineate the study area from the surrounding region. The
TCCON stations included in this study are marked with black “x”
symbols and labeled in black bold font. The countries intersected by or
contained within the study area are labeled in grey. Warm (red) colors
indicate that the TNO-MACC_III inventory is larger than the EDGAR inventory;
cool (blue) colors indicate that the EDGAR inventory is larger than
TNO-MACC_III.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f07.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><label>Figure 8</label><caption><p id="d1e2018">This map shows the difference between the TNO-MACC_III methane
emissions and the EDGAR emissions for the year 2010. The labeling and
coloring follows that in
Fig. <xref ref-type="fig" rid="Ch1.F7"/>.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f08.png"/>

      </fig>

      <p id="d1e2029">The differences between EDGAR and TNO-MACC_III methane emissions also show
that the EDGAR emissions estimates near large cities are significantly larger
(Fig. <xref ref-type="fig" rid="Ch1.F8"/>). In contrast to the carbon monoxide
spatial distribution, the TNO-MACC_III methane emissions are generally
smaller everywhere, except for discrete point sources.</p>
      <p id="d1e2034">Comparing country-level carbon monoxide emissions reported in 2010 with the
inventories shows reasonable agreement, which is expected since the
inventories use country-level reports as input. The sum of the carbon
monoxide emissions within the entire countries of Germany, Poland, France,
Luxembourg, Belgium, and the Czech Republic differ between EDGAR and
TNO-MACC_III by 18 %, with EDGAR estimates lower than those from
TNO-MACC_III. Emissions from Germany, most of which are included in the
study area, differ by only 6 % between EDGAR and TNO-MACC_III, again with
EDGAR estimates lower than TNO-MACC_III. The national carbon monoxide
emissions reported to the Convention on Long-range Transboundary Air
Pollution <xref ref-type="bibr" rid="bib1.bibx12" id="paren.51"><named-content content-type="pre">LRTAP Convention,
<uri>https://www.eea.europa.eu/ds_resolveuid/0156b7a0ca47485593e7754c52c24afd</uri>, last access: 15 November 2017,
</named-content></xref> agree to within a few percent of the TNO-MACC_III
country-level emissions (e.g., 5.5 % for Germany in 2010).</p>
      <p id="d1e2045">The differences between 2010 country-level emissions estimates are larger for
methane: EDGAR estimates are larger than TNO-MACC_III estimates by 36 % when
summing all countries intersected by the study area and 8 % when considering
only German emissions. The TNO-MACC_III country-level emissions estimates
agree to within a few percent of the UNFCCC
(<uri>http://di.unfccc.int/time_series</uri>, last access: 15 November 2017) country-level reported methane
emissions (e.g., 8 % for Germany in 2010).</p>
      <?pagebreak page3971?><p id="d1e2052">The differences between the EDGAR and TNO-MACC_III inventories suggest that
the spatial distribution of emissions is less certain than the larger-scale
emissions, since the total carbon monoxide and methane emissions between the
inventories agree to within 15 % and 2 %, respectively, in the study area, but
these estimates can disagree by a factor of 2 on city-level scales.</p>
      <p id="d1e2055">If we assume that the national-scale methane emissions are correctly reported
in EDGAR and TNO-MACC_III, our results indicate that the methane emissions
in the region are incorrectly spatially distributed in the inventories. It
could be that point or urban sources outside the study area but within the
countries intersected by the study area emit a larger proportion of the
country-level emissions than previously thought.</p>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusions</title>
      <p id="d1e2066">Using co-located measurements of methane and carbon monoxide from five
long-running ground-based atmospheric observing stations, we have shown that
in the area of Europe between Orléans, Bremen, Białystok, and
Garmisch-Partenkirchen, the inventories likely overestimate methane emissions and point to
a large uncertainty in the spatial distribution (i.e., the spatial
disaggregation) of country-level emissions. However, the magnitude of our
inferred methane emissions relies heavily on the EDGAR v4.3.1 and
TNO-MACC_III carbon monoxide inventories, and thus there is a need for
rigorous validation of the carbon monoxide inventories.</p>
      <p id="d1e2069">This study demonstrates the potential of clusters of long-term ground-based
stations monitoring total columns of atmospheric greenhouse and tracer
gases. It also shows the potential of having co-located measurements of
multiple pollutants to derive better estimates of emissions. These types of
observing systems can help policy makers verify that greenhouse gas emissions
are reducing at a rate necessary to meet regulatory obligations. The
atmospheric measurements are agnostic to the source (and country of origin)
of the methane, measuring only what is emitted into the atmosphere in a given
area. Thus, they can help validate and reveal inadequacies in the current
inventories, and, in particular, how country-wide emission reports are
disaggregated on a grid. To enhance these results, simultaneous measurements
of complementary atmospheric trace gases, such as ethane, acetylene, nitrous
oxide, nitrogen dioxide, ammonia, and isotopes, would help distinguish between
sources of methane. This would provide additional valuable information that
would likely improve inventory disaggregation.</p>
</sec>

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

      <p id="d1e2077">TCCON data are available from the TCCON archive, hosted by
the California Institute of Technology at <uri>https://tccondata.org</uri>.
Karlsruhe data were obtained
from <ext-link xlink:href="https://doi.org/10.14291/tccon.ggg2014.karlsruhe01.R1/1182416" ext-link-type="DOI">10.14291/tccon.ggg2014.karlsruhe01.R1/1182416</ext-link>
(<xref ref-type="bibr" rid="bib1.bibx20" id="altparen.52"/>). Bremen data were obtained from
<ext-link xlink:href="https://doi.org/10.14291/tccon.ggg2014.bremen01.R0/1149275" ext-link-type="DOI">10.14291/tccon.ggg2014.bremen01.R0/1149275</ext-link>
(<xref ref-type="bibr" rid="bib1.bibx41" id="altparen.53"/>). Garmisch data were obtained from
<ext-link xlink:href="https://doi.org/10.14291/tccon.ggg2014.garmisch01.R0/1149299" ext-link-type="DOI">10.14291/tccon.ggg2014.garmisch01.R0/1149299</ext-link>
(<xref ref-type="bibr" rid="bib1.bibx53" id="altparen.54"/>). Orléans data were obtained from
<ext-link xlink:href="https://doi.org/10.14291/tccon.ggg2014.orleans01.R0/1149276" ext-link-type="DOI">10.14291/tccon.ggg2014.orleans01.R0/1149276</ext-link>
(<xref ref-type="bibr" rid="bib1.bibx60" id="altparen.55"/>). Bialystok data were obtained from
<ext-link xlink:href="https://doi.org/10.14291/tccon.ggg2014.bialystok01.R1/1183984" ext-link-type="DOI">10.14291/tccon.ggg2014.bialystok01.R1/1183984</ext-link>
(<xref ref-type="bibr" rid="bib1.bibx9" id="altparen.56"/>). The Emissions Database for Global Atmospheric Research (EDGAR) inventory is
available from the European Commission Joint Research Centre (JRC) and the
Netherlands Environmental Assessment Agency (PBL),
<uri>http://edgar.jrc.ec.europa.eu</uri> (last access: 7 April 2017). The GEOS-Chem v12.1.0 model is available
from <ext-link xlink:href="https://doi.org/10.5281/zenodo.1553349" ext-link-type="DOI">10.5281/zenodo.1553349</ext-link> (<xref ref-type="bibr" rid="bib1.bibx54" id="altparen.57"/>).</p>
  </notes><?xmltex \hack{\clearpage}?><app-group>

<?pagebreak page3972?><app id="App1.Ch1.S1">
  <label>Appendix A</label><title>Filtering</title>
      <p id="d1e2135">The filtering method was designed to remove days of data for which the
atmospheric air mass was inconsistent between sites (e.g., a front was
passing through or there were significant stratospheric incursions into the
troposphere) and for years in which there were too few simultaneous
measurements at a pair of TCCON stations to compute robust
annually representative anomalies.</p>
      <p id="d1e2138">To address the consistency of the air mass between sites, we retained days on
which the retrievals of hydrogen fluoride (<inline-formula><mml:math id="M114" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">HF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) were between
50 <inline-formula><mml:math id="M115" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> and 100 <inline-formula><mml:math id="M116" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula>, and deviated by less
than 10 <inline-formula><mml:math id="M117" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> of the median <inline-formula><mml:math id="M118" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">HF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> value for all sites on that
day. <inline-formula><mml:math id="M119" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">HF</mml:mi></mml:mrow></mml:math></inline-formula> is a trace gas that exists only in the stratosphere, and thus
it serves as a tracer of tropopause height <xref ref-type="bibr" rid="bib1.bibx61 bib1.bibx46" id="paren.58"/>.
Since the concentration of <inline-formula><mml:math id="M120" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> decreases significantly above the
tropopause in the midlatitudes, its total column dry-air mole fraction
(<inline-formula><mml:math id="M121" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) is sensitive to the tropopause height. Filtering out days
on which <inline-formula><mml:math id="M122" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">X</mml:mi><mml:mi mathvariant="normal">HF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> varies significantly between sites also ensures that
the anomalies (and thus the slopes) are minimally impacted by stratospheric
variability. This filter removed less than <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:math></inline-formula> of the data.</p>
      <p id="d1e2247">To ensure that the anomalies are representative of the full year, we require
that each year has 400 coincident measurements across at least three seasons.</p>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.F1"><label>Figure A1</label><caption><p id="d1e2253">These box plots show the NCEP/NCAR reanalysis long-term climatological monthly mean wind speeds at
the surface (filled black boxes) and at 850 hPa (open red boxes) in the
study area (see Figs. <xref ref-type="fig" rid="Ch1.F1"/>, <xref ref-type="fig" rid="Ch1.F7"/>,
or <xref ref-type="fig" rid="Ch1.F8"/> for study area maps). The solid black and
dashed red horizontal lines indicate the annual mean wind speed at the
surface and 850 hPa (<inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> km), respectively. Wind speeds that are
aloft (on average 17 <inline-formula><mml:math id="M125" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) are significantly swifter than those
at the surface (on average 7.5 <inline-formula><mml:math id="M126" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>).</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f09.png"/>

      </fig>

<?xmltex \hack{\newpage}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.F2"><label>Figure A2</label><caption><p id="d1e2316">These are the anomaly slopes (<inline-formula><mml:math id="M127" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>)
in <inline-formula><mml:math id="M128" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppb</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">ppb</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> for each station pair, for the entire time series.
The anomalies are computed by subtracting data within the same solar zenith angle bin
between two TCCON stations. For more detail, see Sect. <xref ref-type="sec" rid="Ch1.S2"/> of the
main text. The <inline-formula><mml:math id="M129" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis indicates the number of days separating the
measurements. The legend identifiers are as follows: br – Bremen, gm – Garmisch-Partenkirchen, bi – Białystok, or – Orléans, ka –
Karlsruhe.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f10.png"/>

      </fig>

<?xmltex \hack{\clearpage}?><?xmltex \floatpos{t}?><fig id="App1.Ch1.F3" specific-use="star"><label>Figure A3</label><caption><p id="d1e2373">These maps show the inventory emissions for the year 2010 in the
study area (delineated by the solid straight lines) and the surrounding
region. The TCCON stations are marked with black “x” symbols and
labeled in black bold font. The countries intersected by, or contained
within, the study area are labeled in grey. The map in <bold>(a)</bold> shows
the EDGAR
v4.3.1 emissions inventory for carbon monoxide. The map in <bold>(b)</bold> shows the
EDGAR FT2010 emissions inventory for methane. The map in <bold>(c)</bold> shows the
TNO-MACC_III emissions inventory for carbon monoxide. The map in <bold>(d)</bold> shows the TNO-MACC_III emissions inventory for
methane.</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f11.jpg"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.F4" specific-use="star"><label>Figure A4</label><caption><p id="d1e2397">This four-panel plot shows the methodology for scaling the
country-level reported emissions of <inline-formula><mml:math id="M130" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> to extrapolate the gridded
inventory emissions to 2015. Panel <bold>(a)</bold> shows the <inline-formula><mml:math id="M131" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions
reported by the European Environment Agency (EEA) for the countries contained
within the study area (Germany, France, Czech Republic, Belgium, Luxembourg,
and Poland). The black stars with a joining line represent the summed total
from the five countries. The EDGAR (green) and TNO-MACC_III (orange)
inventories summed within the study area are plotted with squares joined by
solid lines. Panel <bold>(b)</bold> shows the ratio between the individual country
totals and the EDGAR area total, normalized to produce an emission ratio of 1
in 2010. The quantity with the least interannual variability in the ratio is
from the country total (black stars with line). Panel <bold>(c)</bold> shows the
ratio between the individual country totals and the TNO-MACC_III area total,
normalized to produce an emission ratio of 1 in 2011. The quantity with the
least interannual variability in the ratio is, again, from the country total.
Panel <bold>(d)</bold> shows the scaled country total, normalized to produce the
EDGAR <inline-formula><mml:math id="M132" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions for 2010 and the TNO-MACC_III <inline-formula><mml:math id="M133" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> emissions
for 2011. This permits us to compute a sensible emission for the study area
through to 2015.</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f12.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.F5" specific-use="star"><label>Figure A5</label><caption><p id="d1e2453">This four-panel plot shows the methodology for scaling the
country-level emissions of <inline-formula><mml:math id="M134" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> reported to the UNFCCC to extrapolate
the gridded inventory emissions to 2015. The panels and symbols follow the
same description as in Fig. <xref ref-type="fig" rid="App1.Ch1.F4"/>.</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/3963/2019/acp-19-3963-2019-f13.png"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>

<?pagebreak page3976?><app id="App1.Ch1.S2">
  <label>Appendix B</label><title>Transport time between stations</title>
      <p id="d1e2485">Figure <xref ref-type="fig" rid="App1.Ch1.F1"/> shows the annual change in monthly mean
climatological wind speeds from the NCEP/NCAR reanalysis <xref ref-type="bibr" rid="bib1.bibx28" id="paren.59"/>. These are interpolated to
surface pressure and 850 <inline-formula><mml:math id="M135" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">hPa</mml:mi></mml:mrow></mml:math></inline-formula> pressures (<inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1500</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M137" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>
geopotential height) from model (sigma) surfaces and cover from January 1948
through March 2017. Vertical mixing into the boundary layer occurs on the
timescale of a day or two <xref ref-type="bibr" rid="bib1.bibx25" id="paren.60"/>, and thus the relevant wind speed
is between the surface and 850 <inline-formula><mml:math id="M138" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">hPa</mml:mi></mml:mrow></mml:math></inline-formula>. The annual mean surface wind
speed is <inline-formula><mml:math id="M139" display="inline"><mml:mn mathvariant="normal">6</mml:mn></mml:math></inline-formula> <inline-formula><mml:math id="M140" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, which gives a mean transit time between
Orléans and Białystok of 11 days. The annual mean 850 hPa winds are
<inline-formula><mml:math id="M141" display="inline"><mml:mn mathvariant="normal">17</mml:mn></mml:math></inline-formula> <inline-formula><mml:math id="M142" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, which give a shorter mean transit time between
Orléans and Białystok of 4 days.</p>
      <p id="d1e2579">To test whether the transport time impacts the anomalies, we computed the
slopes for time lags between sites of 0–14 days. Figure <xref ref-type="fig" rid="App1.Ch1.F2"/> shows a small change in anomaly slope as a function of
the lag used to calculate the anomalies. This figure shows that the transport
time between TCCON stations is of negligible importance to the slopes and
lends weight to the decision to compute anomalies from data recorded at two
TCCON stations on the same day.</p>
</app>

<app id="App1.Ch1.S3">
  <label>Appendix C</label><title>Computing study area emissions from the inventories</title>
      <p id="d1e2592">The study area emissions for 2010 are shown in Fig. <xref ref-type="fig" rid="App1.Ch1.F3"/>. We define the study area as the area bounded by
the TCCON stations at (clockwise from the west) Orléans, Bremen,
Białystok, and Garmisch-Partenkirchen, which is marked by the black lines in the figure.
To compute the emissions from the study area, the grid points intersected by
and contained within the solid black lines are summed for each year. The
EDGAR v4.3.1_v2 emissions inventory for <inline-formula><mml:math id="M143" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and FT2010 inventory for
<inline-formula><mml:math id="M144" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> provide estimates for years 2000–2010. The TNO-MACC_III
inventory provides emissions estimates for both <inline-formula><mml:math id="M145" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M146" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> for
the years 2000–2011.</p>
</app>

<app id="App1.Ch1.S4">
  <label>Appendix D</label><title>Projecting inventory emissions beyond 2010</title>
      <p id="d1e2643">Using data from the European Environment Agency National Database
<xref ref-type="bibr" rid="bib1.bibx15" id="paren.61"/>, we extrapolate the inventory
<inline-formula><mml:math id="M147" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M148" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions for the study area through 2015. This is
done by summing the total emissions for the five countries that are
intersected by the study area (France, Belgium, Germany, Poland, Luxembourg,
Czech Republic), and normalizing the emissions to the last year of the
inventory (2010 for EDGAR, 2011 for TNO-MACC_III). Figures <xref ref-type="fig" rid="App1.Ch1.F4"/> and <xref ref-type="fig" rid="App1.Ch1.F5"/> show the
process for the EDGAR and TNO-MACC_III <inline-formula><mml:math id="M149" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M150" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions,
respectively.</p>
      <p id="d1e2692">Figure <xref ref-type="fig" rid="App1.Ch1.F4"/>a shows the reported
country-level emissions for the years 1990–2015, their sum (black stars),
and the sum of the inventory emissions for the years available (2000–2010
for EDGAR; 2000–2011 for TNO-MACC_III) in squares. Figure <xref ref-type="fig" rid="App1.Ch1.F4"/>b–c show the ratio of the country-level emissions to the area emissions,
normalized to <inline-formula><mml:math id="M151" display="inline"><mml:mn mathvariant="normal">1</mml:mn></mml:math></inline-formula> for the last year available in the inventory. These panels
show that the ratio of the summed country total emissions to the emissions
from the area of interest is less variable from year to year than the
emissions reported for individual countries. Thus, we choose to extrapolate
the area emissions using the country total emissions, scaled to the last year
of the inventory for the study area.</p>
      <p id="d1e2706">Figure <xref ref-type="fig" rid="App1.Ch1.F4"/>d shows the results of using a single scaling factor to
estimate the study area emissions from the country-level emissions for each
year. We use the summed study area emissions for the years available, and the
extrapolated emissions through 2015 for subsequent analysis (e.g.,
Figs. <xref ref-type="fig" rid="Ch1.F3"/> and <xref ref-type="fig" rid="Ch1.F6"/>).</p><?xmltex \hack{\clearpage}?>
</app>
  </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e2720">DW designed the study, performed the analysis, and wrote the paper. DBAJ ran
the GEOS-Chem model, supported by the <inline-formula><mml:math id="M152" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M153" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> work of JAF
and JDM. JK and HDvdG provided the TNO-MACC_III inventory. GCT helped refine
the data analysis methodology. NMD, FH, JN, RS, and TW provided TCCON data.
All coauthors read and provided feedback on the contents of the paper and
helped interpret the results.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2745">The authors declare no competing interests.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2751">The NASA Earth Observatory images were prepared by Joshua Stevens, using
Suomi National Polar-orbiting Partnership (NPP) Visible Infrared Imaging
Radiometer (VIIRS) data from Miguel Román, at
NASA's Goddard Space Flight Center. The
authors would like to thank two anonymous reviewers for thoughtful comments
and suggestions that significantly strengthened the paper.</p></ack><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2756">This paper was edited by William Lahoz and reviewed by two
anonymous referees.</p>
  </notes><ref-list>
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