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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-17-10753-2017</article-id><title-group><article-title>Estimation of the fossil fuel component in atmospheric CO<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula><?xmltex \hack{\newline}?> based on
radiocarbon measurements at the Beromünster<?xmltex \hack{\newline}?> tall tower, Switzerland</article-title>
      </title-group><?xmltex \runningtitle{Estimation of the fossil fuel component in atmospheric CO${}_{{2}}$}?><?xmltex \runningauthor{T. A. Berhanu et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Berhanu</surname><given-names>Tesfaye A.</given-names></name>
          <email>berhanu@climate.unibe.ch</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Szidat</surname><given-names>Sönke</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1824-6207</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Brunner</surname><given-names>Dominik</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4007-6902</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Satar</surname><given-names>Ece</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Schanda</surname><given-names>Rüdiger</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Nyfeler</surname><given-names>Peter</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Battaglia</surname><given-names>Michael</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Steinbacher</surname><given-names>Martin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7195-8115</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Hammer</surname><given-names>Samuel</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Leuenberger</surname><given-names>Markus</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4299-6793</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Climate and Environmental Physics, Physics Institute and Oeschger Centre for Climate Change Research,<?xmltex \hack{\newline}?> University of Bern, Bern, Switzerland</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Chemistry and Biochemistry and Oeschger Center for Climate Change Research,<?xmltex \hack{\newline}?> University of Bern, Bern, Switzerland</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Empa, Laboratory for Air Pollution/Environmental Technology, Dübendorf, Switzerland</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Institut für Umweltphysik, Universität Heidelberg, Heidelberg, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Tesfaye A. Berhanu (berhanu@climate.unibe.ch)</corresp></author-notes><pub-date><day>13</day><month>September</month><year>2017</year></pub-date>
      
      <volume>17</volume>
      <issue>17</issue>
      <fpage>10753</fpage><lpage>10766</lpage>
      <history>
        <date date-type="received"><day>25</day><month>February</month><year>2017</year></date>
           <date date-type="rev-request"><day>20</day><month>March</month><year>2017</year></date>
           <date date-type="rev-recd"><day>7</day><month>August</month><year>2017</year></date>
           <date date-type="accepted"><day>17</day><month>August</month><year>2017</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://acp.copernicus.org/articles/17/10753/2017/acp-17-10753-2017.html">This article is available from https://acp.copernicus.org/articles/17/10753/2017/acp-17-10753-2017.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/17/10753/2017/acp-17-10753-2017.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/17/10753/2017/acp-17-10753-2017.pdf</self-uri>


      <abstract>
    <p>Fossil fuel CO<inline-formula><mml:math id="M2" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (CO<inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the major contributor
of anthropogenic CO<inline-formula><mml:math id="M4" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the atmosphere, and accurate quantification is
essential to better understand the carbon cycle. Since October 2012, we have
been continuously measuring the mixing ratios of CO, CO<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CH<inline-formula><mml:math id="M6" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, and
H<inline-formula><mml:math id="M7" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O at five different heights at the Beromünster tall tower,
Switzerland. Air samples for radiocarbon (<inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> analysis
have also been collected from the highest sampling inlet (212.5 m) of the
tower on a biweekly basis. A correction was applied for <inline-formula><mml:math id="M10" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
emissions from nearby nuclear power plants (NPPs), which have been simulated
with the Lagrangian transport model FLEXPART-COSMO. The <inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math id="M13" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
emissions from NPPs offset the depletion in <inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C by fossil fuel
emissions, resulting in an underestimation of the fossil fuel component in atmospheric
CO<inline-formula><mml:math id="M15" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> by about 16 %. An average observed ratio (<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> of 13.4 <inline-formula><mml:math id="M17" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.3 mmol mol<inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
was calculated from the enhancements in CO mixing ratios
relative to the clean-air reference site Jungfraujoch (<inline-formula><mml:math id="M19" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO) and the
radiocarbon-based fossil fuel CO<inline-formula><mml:math id="M20" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mole fractions. The wintertime
<inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> estimate of 12.5 <inline-formula><mml:math id="M22" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.3 is about 30 % higher than the
wintertime ratio between in situ measured CO and CO<inline-formula><mml:math id="M23" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> enhancements at
Beromünster over the Jungfraujoch background (8.7 mmol mol<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) corrected for
non-fossil contributions due to strong biospheric contribution despite the
strong correlation between <inline-formula><mml:math id="M25" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO and <inline-formula><mml:math id="M26" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M27" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in winter. By
combining the ratio derived using the radiocarbon measurements and the
in situ measured CO mixing ratios, a high-resolution time series of
CO<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> was calculated exhibiting a clear seasonality driven by seasonal
variability in emissions and vertical mixing. By subtracting the fossil fuel
component and the large-scale background, we have determined the regional
biospheric CO<inline-formula><mml:math id="M29" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> component that is characterized by seasonal variations
ranging between <inline-formula><mml:math id="M30" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>15 and <inline-formula><mml:math id="M31" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>30 ppm. A pronounced diurnal variation was observed
during summer modulated by biospheric exchange and vertical mixing, while no
consistent pattern was found during winter.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>Fossil fuel CO<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (CO<inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the fundamental contributor to the
increase in atmospheric CO<inline-formula><mml:math id="M34" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>; hence its precise quantification is
crucial to better understand the global carbon budget. One of the major
uncertainties in the projections of climate change is the uncertainty in the
future carbon budget due to feedbacks between terrestrial ecosystems and
climate (Heimann and Reichstein, 2008). Information on the response of
the biosphere to climate variations can be obtained from atmospheric
CO<inline-formula><mml:math id="M35" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observations, but isolating the biospheric signal in the measured
CO<inline-formula><mml:math id="M36" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios requires an accurate quantification of the fossil
fuel component. Several methods have therefore been proposed for quantifying
CO<inline-formula><mml:math id="M37" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>, which are based on observations or models. A widely employed
approach is to determine CO<inline-formula><mml:math id="M38" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> with an atmospheric transport model that
incorporates CO<inline-formula><mml:math id="M39" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> emissions from a bottom-up emission inventory.</p>
      <p>Emission inventories are based on statistics of the energy use by different
sectors and the quantification of CO<inline-formula><mml:math id="M40" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> emissions by accounting for the
carbon content of each fuel and its corresponding oxidation ratios
(Friedlingstein et al., 2010; Le Quéré et al., 2016). When
compared to other greenhouse gases, national emission inventories for
CO<inline-formula><mml:math id="M41" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> are quite accurate, but the computation of these inventories is
laborious, and the quality depends on the energy statistics and reporting
methods that vary greatly between countries (Marland, 2008; Marland et
al., 2009). A recent study evaluating different energy statistics and cement
production data estimated an uncertainty of about 5 % for the global
fossil fuel emissions of the past decade (2006–2015) (Le Quéré
et al., 2016). At country level the uncertainties are usually below 5 %
in developed countries but often exceed 10 % in developing countries
(Ballantyne et al., 2015).</p>
      <p>Additional uncertainties arise from the spatial and temporal disaggregation
of national annual total emissions to the grid of the atmospheric transport
model. At sub-country scales (less than 150 km), the uncertainty from
bottom-up estimates can reach up to 50 % (Ciais et al., 2010).
Finally, errors in the transport model and the inability to correctly
represent point observations in the model may contribute substantially to
the uncertainty of model-simulated CO<inline-formula><mml:math id="M42" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> mixing ratios (Tolk et al.,
2008; Peylin et al., 2011).</p>
      <p>Radiocarbon measurements can be used to directly quantify CO<inline-formula><mml:math id="M43" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>
in atmospheric CO<inline-formula><mml:math id="M44" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observations. Radiocarbon is produced in the upper
atmosphere during the reaction of neutrons with nitrogen induced by cosmic
rays (Currie, 2004). In addition, nuclear bomb tests in the 1960s led to
large radiocarbon input into the atmosphere, which thereafter decreased due
to gradual uptake by the oceans and the terrestrial biosphere (Manning et
al., 1990; Levin et al., 2010). Nowadays, the decline in atmospheric
<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math id="M46" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is mainly driven by input from <inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C-free fossil fuel
CO<inline-formula><mml:math id="M48" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (Levin et al., 2010). This decline is well detectable at background
sites such as Jungfraujoch, Switzerland, and Schauinsland, Germany (Levin et
al., 2013). While all reservoirs exchanging carbon with the atmosphere are
relatively rich in <inline-formula><mml:math id="M49" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C, fossil fuels (millions of years old) are devoid
of <inline-formula><mml:math id="M50" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C due to its radioactive decay with a half-life of 5370 years.
Hence, any fossil fuel CO<inline-formula><mml:math id="M51" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emitted to the atmosphere will dilute the
background <inline-formula><mml:math id="M52" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C signal, the so-called Suess effect, which can then be
used to unravel recently added fossil fuel CO<inline-formula><mml:math id="M53" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to the atmosphere
(Zondervan and Meijer, 1996; Levin et al., 2003; Gamnitzer et al., 2006;
Turnbull et al., 2006, 2009, 2011a, 2014, 2015; Levin and Karstens, 2007;
Lopez et al., 2013). However, this depletion can also partially be offset by
CO<inline-formula><mml:math id="M54" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> release from the biosphere which has enriched
<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C <inline-formula><mml:math id="M56" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M57" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">12</mml:mn></mml:msup></mml:math></inline-formula>C ratios due to nuclear bomb tests in the 1960s.
<inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C produced by these tests was absorbed by the land biosphere and is
now gradually being released back to the atmosphere (Naegler and Levin,
2009). Another contribution could be direct <inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C emissions from nuclear
industries (Levin et al., 2010). This technique also enables separation
between biospheric and fossil fuel CO<inline-formula><mml:math id="M60" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> components in atmospheric
CO<inline-formula><mml:math id="M61" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observations, and it thus better constrains the biospheric CO<inline-formula><mml:math id="M62" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
fluxes when coupled with inversion models (Basu et al., 2016). The
uncertainty in CO<inline-formula><mml:math id="M63" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> estimated by the radiocarbon method is
mainly determined by the precision in the <inline-formula><mml:math id="M64" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C measurement, the choice of
background, and the uncertainty in the contribution from other sources of
<inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C such as nuclear power plants (NPPs) (Turnbull et al., 2009).</p>
      <p>Despite its importance as a fossil fuel tracer, measurements of <inline-formula><mml:math id="M66" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C are
still sparse. The measurements are expensive and laborious, which so far has
prevented frequent sampling and has motivated researchers to combine <inline-formula><mml:math id="M67" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C
measurements with additional tracers such as CO to enhance spatial and
temporal coverage (Gamnitzer et al., 2006; Turnbull et al., 2006, 2011a,
2014, 2015; Levin and Karstens, 2007; Vogel et al., 2010; Lopez et al.,
2013). The CO method relies on using high frequency CO measurements and
regular calibration of the temporally changing <inline-formula><mml:math id="M68" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO : <inline-formula><mml:math id="M69" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M70" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> ratios based on weekly or biweekly <inline-formula><mml:math id="M71" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C measurements.
Despite its advantage of providing a proxy for continuous CO<inline-formula><mml:math id="M72" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>
data, the method introduces additional uncertainties due to diurnal and
seasonal variability in the CO sink, and the presence of multiple non-fossil
CO sources such as oxidation of hydrocarbons or wood and biofuel combustion
(Gamnitzer et al., 2006). Spatial variations in the <inline-formula><mml:math id="M73" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO : <inline-formula><mml:math id="M74" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M75" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratio across Europe due to different source compositions and
environmental regulations, which affect the measured ratios due to changes in
air mass origin (Oney et al., 2017), are the main reason for the temporally
changing <inline-formula><mml:math id="M76" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO : <inline-formula><mml:math id="M77" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M78" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> ratio for a given
measurement site. Additionally, variability in the CO <inline-formula><mml:math id="M79" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> CO<inline-formula><mml:math id="M80" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emission
ratios of the sources can contribute to its spatial and temporal variability
(Vogel et al., 2010; Turnbull et al., 2015).</p>
      <p>In Switzerland, CO<inline-formula><mml:math id="M81" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> contributes about 82 % of the total greenhouse
gas emissions according to the Swiss national emission inventory for 2013,
and fossil fuel combustion from the energy sector contributes more than 80 % of the total CO<inline-formula><mml:math id="M82" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emission (FOEN, 2015b). In order to validate
such bottom-up estimates, independent techniques based on atmospheric
measurements are desirable. In addition, as mentioned above, the biospheric
CO<inline-formula><mml:math id="M83" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> signals can only be estimated with a good knowledge of CO<inline-formula><mml:math id="M84" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>.
In this study, we present and discuss <inline-formula><mml:math id="M85" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math id="M86" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements conducted
biweekly between 2013 and 2015 at the Beromünster tall tower in
Switzerland. From these samples in combination with background CO, CO<inline-formula><mml:math id="M87" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>,
and <inline-formula><mml:math id="M88" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math id="M89" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements at the high-altitude remote location
Jungfraujoch, Switzerland, <inline-formula><mml:math id="M90" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula> / <inline-formula><mml:math id="M91" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M92" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> ratios
(<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> are derived. These ratios are then combined with the in situ
measured <inline-formula><mml:math id="M94" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO mixing ratios to estimate a high-resolution time series
of atmospheric CO<inline-formula><mml:math id="M95" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> mixing ratios and, by difference, of the
biospheric CO<inline-formula><mml:math id="M96" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> component. The influence of <inline-formula><mml:math id="M97" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C emissions from
nearby NPPs and correction strategies are also discussed.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p>The geographical map of Beromünster and Jungfraujoch measurement
sites (blue) as well as the five NPPs in Switzerland (red).</p></caption>
        <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10753/2017/acp-17-10753-2017-f01.png"/>

      </fig>

</sec>
<sec id="Ch1.S2">
  <title>Methods</title>
<sec id="Ch1.S2.SS1">
  <?xmltex \opttitle{Site description and continuous measurement of CO and CO${}_{{2}}$}?><title>Site description and continuous measurement of CO and CO<inline-formula><mml:math id="M98" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></title>
      <p>A detailed description of the Beromünster tall tower measurement system
as well as a characterization of the site with respect to local
meteorological conditions, seasonal and diurnal variations of greenhouse
gases, and regional representativeness can be obtained from previous
publications (Oney et al., 2015; Berhanu et al., 2016; Satar et al.,
2016). In brief, the tower is located near the southern border of the Swiss
Plateau, the comparatively flat part of Switzerland between the Alps in the
south and the Jura Mountains in the northwest (47<inline-formula><mml:math id="M99" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>11<inline-formula><mml:math id="M100" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>23<inline-formula><mml:math id="M101" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> N, 8<inline-formula><mml:math id="M102" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>10<inline-formula><mml:math id="M103" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>32<inline-formula><mml:math id="M104" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> E, 797 m a.s.l.), which is characterized by intense
agriculture and rather high population density (Fig. 1). The tower is 217.5 m tall with access to five sampling heights
(12.5, 44.6, 71.5, 131.6, 212.5 m) for measuring CO, CO<inline-formula><mml:math id="M105" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CH<inline-formula><mml:math id="M106" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, and H<inline-formula><mml:math id="M107" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O using cavity
ring-down spectroscopy (CRDS) (Picarro Inc., G-2401). By sequentially
switching from the highest to the lowest level, mixing ratios of these trace
gases were recorded continuously for 3 min per height, but only the
last 60 s was retained for data analysis. The calibration procedure
for ambient air includes measurements of reference gases with high and low
mixing ratios traceable to international standards (WMO-X2007 for CO<inline-formula><mml:math id="M108" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
and WMO-X2004 for CO and CH<inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, as well as target gas and more frequent
working gas determinations to ensure the quality of the measurement system.
From 2 years of data a long-term reproducibility of 2.79 ppb, 0.05 ppm,
and 0.29 ppb for CO, CO<inline-formula><mml:math id="M110" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and CH<inline-formula><mml:math id="M111" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, respectively, was determined for
this system (Berhanu et al., 2016).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <?xmltex \opttitle{Sampling and CO${}_{{2}}$ extraction for isotope analysis}?><title>Sampling and CO<inline-formula><mml:math id="M112" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> extraction for isotope analysis</title>
      <p>Air samples for <inline-formula><mml:math id="M113" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math id="M114" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> analysis were collected from the highest
inlet usually between 09:00 to 13:00 UTC. At the beginning we collected one
sample per month, which was eventually changed to sampling every second week
from November 2013 onwards. During each sampling event, three samples were
collected over a 15 min interval in 100 L PE-AL-PE bags (TESSERAUX,
Germany) from the flush pump exhaust line of the 212.5 m sampling inlet,
which has a flow rate of about 9 L min<inline-formula><mml:math id="M115" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> at ambient conditions. The
sampling interval was chosen to ensure radiocarbon sample collection in
parallel with the continuous CO and CO<inline-formula><mml:math id="M116" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements by the CRDS
analyzer at the highest level. Each bag was filled at ambient air pressure
for 6 to 8 min, and a total air volume of 50 to 70 L (at STP) was
collected.</p>
      <p>CO<inline-formula><mml:math id="M117" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> extraction was conducted cryogenically in the laboratory at the
University of Bern usually the day after the sample collection. During the
extraction step, the air sample was first pumped through a stainless-steel
water trap (<inline-formula><mml:math id="M118" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>75 <inline-formula><mml:math id="M119" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C), which was filled with glass beads (Raschig
rings, 5 mm, Germany). A flow controller (Analyt-MTC, Aalborg, USA) with
a flow totalizer tool was attached to this trap to maintain a constant flow of
air (1.2 L min<inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> towards the second trap (trap 2), a spiral-shaped
stainless-steel tube (<inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> in.) filled with glass beads (<inline-formula><mml:math id="M122" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 2 mm)
and immersed in liquid nitrogen to freeze out CO<inline-formula><mml:math id="M123" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. When the flow
ceased, trap 2 was isolated from the line and evacuated to remove gases
which are non-condensable at this temperature. Then, trap 2 was warmed to
room temperature and eventually immersed in slush at <inline-formula><mml:math id="M124" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>75 <inline-formula><mml:math id="M125" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C to
freeze out any remaining water. Finally, the extracted CO<inline-formula><mml:math id="M126" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was expanded
and collected in a 50 mL glass flask immersed in liquid nitrogen.</p>
      <p>Sample extraction efficiency was calculated by comparing the amount of the
cryogenically extracted CO<inline-formula><mml:math id="M127" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with the CO<inline-formula><mml:math id="M128" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measured in situ by the
CRDS analyzer during the time of sampling. The amount of CO<inline-formula><mml:math id="M129" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> extracted
is determined first by transferring the extracted CO<inline-formula><mml:math id="M130" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> cryogenically to
a vacuum line of predetermined volume. Then, based on the pressure reading
of the expanded gas, and the total volume of air collected determined by the
mass flow controller with a totalizer function attached to trap 1, CO<inline-formula><mml:math id="M131" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
mixing ratios were calculated.</p>
      <p>At the end of 2014 we noticed that there was a leakage from the sampling
line exhaust pumps, which resulted in unrealistically high CO<inline-formula><mml:math id="M132" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing
ratios (usually more than 500 ppm). Therefore, we replaced all the exhaust
pumps. To further ensure that the leakage problem during sampling is solved,
we regularly check for leaks before sampling by closing the needle valves
leading to the pumps and monitoring in case there is any flow with the flow
meter attached after the pump. Since the replacement we have not observed
any indication of leakage. Seven samples which were suspected to be
contaminated due to this issue were consequently excluded. The sample
extraction efficiency since then has usually been better than 99 %. We
also conducted a blank test to check the presence of any leaks or contamination
during sample processing but did not observe any of these issues. Five more
samples were excluded in 2014 due to a strong mismatch among triplicates in
the measured CO<inline-formula><mml:math id="M133" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> after the sample extraction which indicated
contamination.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <?xmltex \opttitle{Measurement of $\delta^{{13}}$C, $\delta^{{18}}$O, and $\Delta^{{14}}$C}?><title>Measurement of <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C, <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, and <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C</title>
      <p>Prior to radiocarbon measurement, the extracted CO<inline-formula><mml:math id="M137" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was analyzed for
the stable isotopes <inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C and <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O using
an isotope ratio mass spectrometer (IRMS, Finnigan MAT 250) at the Climate and
Environmental Physics Division of the University of Bern, which has an accuracy
and precision of better than 0.1 ‰ for both <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C and <inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O (Leuenberger et al.,
2003). <inline-formula><mml:math id="M142" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C analysis of the extracted CO<inline-formula><mml:math id="M143" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was performed with an
accelerator mass spectrometer (AMS), MICADAS (MIni CArbon DAting System), at
the Laboratory for the Analysis of Radiocarbon (LARA) at the Department of
Chemistry and Biochemistry of the University of Bern
(Szidat et al., 2014). The Automated Graphitization
Equipment (AGE) was used to prepare solid target gas (Nemec et al.,
2010) from the extracted CO<inline-formula><mml:math id="M144" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> stored in 50 mL glass flasks. A
measurement series consisted of up to 15 air samples converted to 30 solid
graphite targets (duplicates), together with four and three targets from
CO<inline-formula><mml:math id="M145" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> produced by combustion of the NIST standard oxalic acid II (SRM
4990C) and fossil CO<inline-formula><mml:math id="M146" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (Carbagas, Gümligen), respectively, which
were used for the blank subtraction, standard normalization, and correction
for isotopic fractionations. For the fractionation correction, <inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values of the AMS were used, which show a long-term standard
uncertainty of <inline-formula><mml:math id="M148" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1.2 ‰ (Szidat et
al., 2014). The AMS <inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values agree well on average with the
corresponding IRMS results, revealing a statistically insignificant
difference of <inline-formula><mml:math id="M150" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.2 <inline-formula><mml:math id="M151" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.2 ‰ with slightly more
depleted AMS results.</p>
      <p>Data reduction was performed using the BATS program (Wacker et
al., 2010). The uncertainty of an individual <inline-formula><mml:math id="M152" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C measurement typically
amounts to <inline-formula><mml:math id="M153" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 2.1 ‰, including
contributions from counting statistics (<inline-formula><mml:math id="M154" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1.1 ‰), corrections of normalization (i.e., blank subtraction,
standard normalization, and correction for isotopic fractionations)
(<inline-formula><mml:math id="M155" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1.1 ‰), and an unaccounted-for long-term
variability of sampling and <inline-formula><mml:math id="M156" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C analysis according to Szidat et al. (2014) (1.5 ‰). These contributions are comparable to
previous observations (Graven et al., 2007).</p>
      <p>During calculation of weighted averages of the duplicates, the uncertainty
of the mean is determined with the contributions of the counting statistics
and the normalization, whereas the uncertainty of the unaccounted-for long-term
variability is considered fully afterwards, as this contribution cannot be
reduced by averaging of two measurements performed on the same day. This
uncertainty of the weighted average typically amounts to <inline-formula><mml:math id="M157" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1.9 ‰; it is compared with the standard deviation of the
duplicates, and the larger of these values is used as the final uncertainty
of the duplicates. The mean of the three individual samples from the same
day, which is used below in Sect. 2.4.1 as <inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M159" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">meas</mml:mi></mml:msub></mml:math></inline-formula>, is
then determined and associated with the average uncertainty of the three
duplicates, as the variability of the three samples is comparable to this
average uncertainty for all cases.</p>
      <p>As the <inline-formula><mml:math id="M160" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C <inline-formula><mml:math id="M161" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M162" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">12</mml:mn></mml:msup></mml:math></inline-formula>C from Beromünster was measured at the LARA
laboratory in Bern, whereas the corresponding background samples from
Jungfraujoch were analyzed at the low-level counting (LLC) facility of the
Institute of Environmental Physics, Heidelberg University, the data sets
needed to be adjusted to each other. A recent interlaboratory compatibility
test between the LARA lab (code no. 2) and Heidelberg (LLC) estimated a
small bias (Hammer et al., 2016). The measurement bias
(i.e., the mean difference of the measured <inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C minus the consensus
value of the participating laboratories for all investigated CO<inline-formula><mml:math id="M164" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
samples) is <inline-formula><mml:math id="M165" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>1.8 <inline-formula><mml:math id="M166" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.1 and <inline-formula><mml:math id="M167" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.3 <inline-formula><mml:math id="M168" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.5 ‰ for Bern and Heidelberg, respectively, from which the
bias between both labs of 2.1 <inline-formula><mml:math id="M169" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.5 ‰ is
determined with a larger measured <inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C for Bern. Consequently,
2.1 <inline-formula><mml:math id="M171" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.5 ‰ was subtracted from the <inline-formula><mml:math id="M172" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C
measurements of the Beromünster samples.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <?xmltex \opttitle{Determination of the fossil fuel CO${}_{{2}}$ component}?><title>Determination of the fossil fuel CO<inline-formula><mml:math id="M173" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> component</title>
<sec id="Ch1.S2.SS4.SSS1">
  <?xmltex \opttitle{The $\Delta^{{14}}$C technique}?><title>The <inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C technique</title>
      <p>For the determination of the CO<inline-formula><mml:math id="M175" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> component we followed
approaches similar to those in in previous studies (Zondervan and Meijer, 1996; Levin et
al., 2003; Levin and Karstens, 2007; Turnbull et al., 2009). The measured
CO<inline-formula><mml:math id="M176" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is assumed to be composed of three major components: the free
troposphere background (CO<inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bg</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, the regional biospheric component
(CO<inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> comprising photosynthesis and respiration components, and the
fossil fuel component (CO<inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>:

                  <disp-formula id="Ch1.E1" content-type="numbered"><mml:math id="M180" display="block"><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">meas</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bg</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></disp-formula>

            Each of these components has a specific <inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C value (i.e., the
deviation in per mill of the <inline-formula><mml:math id="M182" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C <inline-formula><mml:math id="M183" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M184" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">12</mml:mn></mml:msup></mml:math></inline-formula>C ratio from its primary
standard, and corrected for fractionation and decay using <inline-formula><mml:math id="M185" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula>C
measurements) described as <inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M187" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">meas</mml:mi></mml:msub></mml:math></inline-formula>, <inline-formula><mml:math id="M188" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M189" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">bg</mml:mi></mml:msub></mml:math></inline-formula>, <inline-formula><mml:math id="M190" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M191" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">bio</mml:mi></mml:msub></mml:math></inline-formula>, and
<inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M193" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">ff</mml:mi></mml:msub></mml:math></inline-formula>. In analogy to Eq. (1), a mass balance
approximation equation can also be formulated for <inline-formula><mml:math id="M194" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C as

                  <disp-formula specific-use="align" content-type="numbered"><mml:math id="M195" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">meas</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">meas</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1000</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">‰</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bg</mml:mi></mml:mrow></mml:msub><mml:mo mathsize="1.5em">(</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mspace linebreak="nobreak" width="1em"/><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1000</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">‰</mml:mi><mml:mo mathsize="1.5em">)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">bio</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1000</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">‰</mml:mi></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mspace width="1em" linebreak="nobreak"/><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">ff</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1000</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">‰</mml:mi></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

              Note that non-fossil-fuel components such as biofuels are incorporated into
the biospheric component in Eq. (1). The fossil fuel term in Eq. (2) is zero
as fossil fuels are devoid of radiocarbon (<inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M197" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">ff</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> ‰). By replacing the biospheric CO<inline-formula><mml:math id="M198" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> component
in Eq. (1) by a formulation derived from Eq. (2), the fossil fuel CO<inline-formula><mml:math id="M199" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
component is derived as

                  <disp-formula specific-use="align" content-type="numbered"><mml:math id="M200" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><?xmltex \hack{\hbox\bgroup\fontsize{8.0}{8.0}\selectfont$\displaystyle}?><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><?xmltex \hack{$\egroup}?></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{8.0}{8.0}\selectfont$\displaystyle}?><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bg</mml:mi></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">bio</mml:mi></mml:msub></mml:mfenced><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">meas</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">meas</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">bio</mml:mi></mml:msub></mml:mfenced></mml:mrow><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">bio</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1000</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">‰</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><?xmltex \hack{$\egroup}?><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

              Equation (3) can be further simplified by assuming that <inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M202" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">bio</mml:mi></mml:msub></mml:math></inline-formula> is equal to <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M204" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">bg</mml:mi></mml:msub></mml:math></inline-formula> (Levin et al.,
2003) as
              <disp-formula id="Ch1.E4" content-type="numbered"><mml:math id="M205" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">meas</mml:mi></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">meas</mml:mi></mml:msub></mml:mfenced></mml:mrow><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1000</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">‰</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
            Hence, the fossil fuel CO<inline-formula><mml:math id="M206" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> component can be determined using the
CO<inline-formula><mml:math id="M207" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">meas</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M209" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">meas</mml:mi></mml:msub></mml:math></inline-formula> values measured at the site as
well as <inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M211" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">bg</mml:mi></mml:msub></mml:math></inline-formula> obtained from the Jungfraujoch mountain
background site in the Swiss Alps.</p>
      <p>However, the CO<inline-formula><mml:math id="M212" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> determined using Eq. (4) incorporates a small bias
due to the non-negligible disequilibrium contribution of heterotrophic
respiration as well as due to contributions from NPPs. To correct for the
bias from these other contributions, an additional term (CO<inline-formula><mml:math id="M213" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">other</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and
<inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">other</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> can be included in Eq. (4) as suggested by
Turnbull et al. (2009):

                  <disp-formula specific-use="align" content-type="numbered"><mml:math id="M216" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">meas</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">meas</mml:mi></mml:msub></mml:mfenced></mml:mrow><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1000</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">‰</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E5"><mml:mtd/><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">other</mml:mi></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">other</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub></mml:mfenced></mml:mrow><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1000</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">‰</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

              where CO<inline-formula><mml:math id="M217" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">other</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M219" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">other</mml:mi></mml:msub></mml:math></inline-formula> represent the additional
CO<inline-formula><mml:math id="M220" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and radiocarbon contributions from other sources such as NPPS and
biospheric fluxes, respectively.</p>
      <p>The contributions from heterotrophic respiration will lead to an
underestimation of CO<inline-formula><mml:math id="M221" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> on average by 0.2 ppm in winter and 0.5 ppm in
summer, estimated for the Northern Hemisphere using a mean
terrestrial carbon residence time of 10 years (Turnbull et al., 2006).</p>
      <p>To account for the bias from heterotrophic respiration, a harmonic function
varying seasonally between these values was added to the derived
CO<inline-formula><mml:math id="M222" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> values. However, variation of respiration fluxes on shorter
timescales cannot be accounted for by this simple correction. The correction
strategy for the contribution from NPPs is described in Sect. 2.4.2 below.</p>
</sec>
<sec id="Ch1.S2.SS4.SSS2">
  <?xmltex \opttitle{Simulation of ${}^{{14}}$CO${}_{{2}}$ from nuclear power plants}?><title>Simulation of <inline-formula><mml:math id="M223" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math id="M224" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from nuclear power plants</title>
      <p>Radiocarbon is produced by nuclear reactions in NPPs and primarily emitted in
the form of <inline-formula><mml:math id="M225" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math id="M226" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (Yim and Caron, 2006), except for pressurized
water reactors (PWRs), which release <inline-formula><mml:math id="M227" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C mainly in the form of
<inline-formula><mml:math id="M228" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>CH<inline-formula><mml:math id="M229" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>. Previous studies have shown that such emissions can lead to
large-scale gradients in atmospheric <inline-formula><mml:math id="M230" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C activity and offset the
depletion from fossil fuel emissions (Graven and Gruber, 2011). In
Heidelberg, Germany, an offset of 25 and 10 % of the fossil fuel signal was
observed during summer and winter, respectively, due to emissions from a
nearby plant (Levin et al., 2003). Similarly, Vogel et
al. (2013) determined the influence of NPPs for a measurement site in Canada and
estimated that about 56 % of the total CO<inline-formula><mml:math id="M231" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> component was
masked by the contribution from NPPs, though this large number was obtained
for a site in close vicinity of the CANadian Deutrium Uranium-type reactor
(CANDU), known for producing particularly high <inline-formula><mml:math id="M232" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C emissions. In
Switzerland, there are five NPPs, and the closest plant is located about
30 km to the northwest of Beromünster (Fig. 1). Furthermore, air masses
arriving at Beromünster are frequently advected from France, which is the
largest producer of nuclear power in Europe.</p>
      <p>To estimate the influence of Swiss and other European NPPs on <inline-formula><mml:math id="M233" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C at Beromünster, we used FLEXPART-COSMO backward Lagrangian
particle dispersion simulations (Henne et al., 2016). FLEXPART-COSMO was
driven by hourly operational analyses of the non-hydrostatic numerical
weather prediction model COSMO provided by the Swiss weather service
MeteoSwiss at approximately 7 <inline-formula><mml:math id="M234" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 7 km<inline-formula><mml:math id="M235" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> resolution for a domain covering
large parts of western Europe from the southern tip of Spain to the northern
tip of Denmark and from the west coast of Ireland to eastern Poland. For
each 3 h measurement interval during the 3-year period, a source
sensitivity map (footprint) was calculated by tracing the paths of 50 000 particles released from Beromünster at 212 m above ground over 4 days
backward in time. The source sensitivities were then multiplied with the
<inline-formula><mml:math id="M236" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math id="M237" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emissions of all NPPs within the model domain. Thereby, the
emission of a given NPP was distributed over the area of the model grid cell
containing the NPP. Source sensitivities were calculated for three different
vertical layers (0–50, 50–200, 200–500 m). Since the height of
ventilation chimneys of the Swiss NPPs is between 99 and 120 m, only the
sensitivity of the middle layer was selected here as it corresponds best to
the effective release height.</p>
      <p>The release of <inline-formula><mml:math id="M238" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C both in inorganic (CO<inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and organic form
(CH<inline-formula><mml:math id="M240" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is routinely measured at all Swiss NPPs. Annual totals of <inline-formula><mml:math id="M241" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C
emissions are published in the annual reports of the Swiss Federal Nuclear
Safety Inspectorate ENSI
(<uri>https://www.ensi.ch/de/dokumente/document-category/strahlenschutzberichte/</uri>).
The corresponding data have been kindly provided by the Swiss Federal Nuclear
Safety Inspectorate ENSI and the Berner Kraftwerke (BKW), operating the NPP
Mühleberg at temporal resolutions ranging from annual (Benznau 1 &amp; 2)
to monthly (Leibstadt, Gösgen) and biweekly (Mühleberg), and we
assumed constant emissions over the corresponding periods. For Beznau 1, the
emissions of 2015 were distributed over the first 3 months of the year due to
the shutdown of the plant in March 2015. The largest sources of
<inline-formula><mml:math id="M242" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math id="M243" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in Switzerland are the two boiling water
reactors Mühleberg and Leibstadt (Loosli and Oeschger, 1989).
Beznau 1 and 2 and Gösgen are PWRs emitting about 1 order of magnitude
less <inline-formula><mml:math id="M244" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math id="M245" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. For NPPs outside Switzerland, the emissions were
estimated from energy production data reported to the International Atomic
Energy Agency (IAEA) and NPP type-specific emission factors following Graven
and Gruber (2011). The difference <inline-formula><mml:math id="M246" display="inline"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M247" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">nucBRM</mml:mi></mml:msub></mml:math></inline-formula> in
<inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C between the nuclear emission signals at Beromünster
(<inline-formula><mml:math id="M249" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M250" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">nucBRM</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and at Jungfraujcoh (<inline-formula><mml:math id="M251" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">nucJFJ</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> was then computed following Eq. (4) in Levin et
al. (2010) and assuming that the mole fraction (<inline-formula><mml:math id="M253" display="inline"><mml:mrow><mml:msup><mml:mi>n</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M254" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C due to
NPPs at Jungfraujoch is negligible compared to Beromünster. We then
obtain
              <disp-formula id="Ch1.E6" content-type="numbered"><mml:math id="M255" display="block"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi mathvariant="normal">nuc</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>f</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mi>n</mml:mi><mml:mi mathvariant="normal">npp</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msubsup></mml:mrow><mml:mrow><mml:msubsup><mml:mi>n</mml:mi><mml:mi mathvariant="normal">meas</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:msubsup></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1000</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            with the dimensionless factor <inline-formula><mml:math id="M256" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">8.19</mml:mn><mml:mo>×</mml:mo><mml:msub><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">14</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M257" display="inline"><mml:mrow><mml:msubsup><mml:mi>n</mml:mi><mml:mi mathvariant="normal">npp</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M258" display="inline"><mml:mrow><mml:mo>/</mml:mo><mml:msubsup><mml:mi>n</mml:mi><mml:mi mathvariant="normal">meas</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:msubsup></mml:mrow></mml:math></inline-formula> being the number
of <inline-formula><mml:math id="M259" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C atoms due to NPPs simulated with FLEXPART-COSMO relative to the
total number of C atoms (<inline-formula><mml:math id="M260" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">12</mml:mn></mml:msup></mml:math></inline-formula>C <inline-formula><mml:math id="M261" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M262" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula>C <inline-formula><mml:math id="M263" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M264" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C) (which is
equal to the total number of CO<inline-formula><mml:math id="M265" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> molecules) measured at Beromünster.</p>
</sec>
<sec id="Ch1.S2.SS4.SSS3">
  <?xmltex \opttitle{Calculation of $R_{\mathrm{CO}}$, $\Delta$CO\,$/$\,$\Delta$CO${}_{{2}}$, and high-resolution CO${}_{\mathrm{2ff}}$}?><title>Calculation of <inline-formula><mml:math id="M266" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M267" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO <inline-formula><mml:math id="M268" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M269" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M270" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and high-resolution CO<inline-formula><mml:math id="M271" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula></title>
      <p>A <inline-formula><mml:math id="M272" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO / <inline-formula><mml:math id="M273" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M274" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> ratio (<inline-formula><mml:math id="M275" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> was calculated as the
slope of the geometric mean regression (model II), with <inline-formula><mml:math id="M276" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO being
the CO enhancement over a background measured at Jungfraujoch, and the
CO<inline-formula><mml:math id="M277" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> values as determined above. The CO measurements at Jungfraujoch
were conducted using a CRDS analyzer (Picarro Inc., G-2401) with a
measurement precision of <inline-formula><mml:math id="M278" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>2.5 ppb for 1 min aggregates (Zellweger et al., 2012).</p>
      <p>As CO is usually co-emitted with CO<inline-formula><mml:math id="M279" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during incomplete combustion of
fossil and other fuels, we have also computed a tracer ratio designated as
<inline-formula><mml:math id="M280" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO <inline-formula><mml:math id="M281" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M282" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M283" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from the enhancements in the in situ measured
CO and CO<inline-formula><mml:math id="M284" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios over the Jungfraujoch background
(Oney et al., 2017). CO<inline-formula><mml:math id="M285" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bg</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and CO<inline-formula><mml:math id="M286" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">bg</mml:mi></mml:msub></mml:math></inline-formula> values were
obtained by applying the robust extraction of baseline signal (REBS)
statistical method (Ruckstuhl et al., 2012) to the continuous CO<inline-formula><mml:math id="M287" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
and CO measurements at the high-altitude site Jungfraujoch (Schibig et
al., 2016) with a bandwidth of 60 days. Note that, while <inline-formula><mml:math id="M288" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> strictly
refers to the ratio of <inline-formula><mml:math id="M289" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO to fossil fuel CO<inline-formula><mml:math id="M290" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emissions, the
<inline-formula><mml:math id="M291" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO <inline-formula><mml:math id="M292" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M293" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M294" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratio can be influenced by biospheric
contribution as well as CO<inline-formula><mml:math id="M295" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emissions from non-fossil sources such as
biofuels and biomass burning.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p>CO<inline-formula><mml:math id="M296" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios (hourly averages) at Beromünster (black)
from the sample inlet at 212.5 m and from background measurements at
Jungfraujoch (blue) filtered using the REBS function for periods when
<inline-formula><mml:math id="M297" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C sampling was conducted <bold>(a)</bold>, <inline-formula><mml:math id="M298" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C determined from
the biweekly point samplings at the site before (green) and after (red)
correction for the intercomparison offset (see Sect. 2.3) and the <inline-formula><mml:math id="M299" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C
contribution from NPPs (see Eq. 5) and from 14-day integrated samplings at
Jungfraujoch (blue) <bold>(b)</bold>, CO<inline-formula><mml:math id="M300" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> determined during this
period applying Eq. (4) with a mean CO<inline-formula><mml:math id="M301" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> value of 4.3 ppm
(dashed line) <bold>(c)</bold>, the biospheric CO<inline-formula><mml:math id="M302" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> determined by simple
subtraction of CO<inline-formula><mml:math id="M303" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bg</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and CO<inline-formula><mml:math id="M304" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> from the
CO<inline-formula><mml:math id="M305" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">meas</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> <bold>(d)</bold>, and the temperature record during this
period at the 212.5 m height level <bold>(e)</bold>. Error bars in
panels <bold>(b)</bold> and <bold>(c)</bold> indicate the mean uncertainty in
<inline-formula><mml:math id="M306" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measurement (<inline-formula><mml:math id="M307" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>2.0 ‰) and calculated
CO<inline-formula><mml:math id="M308" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math id="M309" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1.2 ppm), averaged for the triplicate samples, while
error bars in panel <bold>(d)</bold> are obtained from error propagation of the
components in panels <bold>(a)</bold>, <bold>(b)</bold>, and <bold>(c)</bold>. CO<inline-formula><mml:math id="M310" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
mixing ratios in the top panel are only shown from times matching the
radiocarbon sampling at Beromünster tower.</p></caption>
            <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10753/2017/acp-17-10753-2017-f02.png"/>

          </fig>

      <p>In order to construct the high-resolution CO<inline-formula><mml:math id="M311" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> time series, we
combined the in situ measured CO enhancements at the Beromünster tower
with the radiocarbon-derived ratios <inline-formula><mml:math id="M312" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and estimated
CO<inline-formula><mml:math id="M313" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow><mml:mi mathvariant="normal">CO</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> for the 3-year data set as
              <disp-formula id="Ch1.E7" content-type="numbered"><mml:math id="M314" display="block"><mml:mrow><mml:msubsup><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow><mml:mi mathvariant="normal">CO</mml:mi></mml:msubsup><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mi mathvariant="normal">bg</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            where CO<inline-formula><mml:math id="M315" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">obs</mml:mi></mml:msub></mml:math></inline-formula> is the hourly averaged CO measurements at the tower.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results and discussions</title>
<sec id="Ch1.S3.SS1">
  <?xmltex \opttitle{$\Delta^{{14}}$CO${}_{{2}}$ and CO${}_{\mathrm{2ff}}$}?><title><inline-formula><mml:math id="M316" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math id="M317" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and CO<inline-formula><mml:math id="M318" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula></title>
      <p>Figure 2a shows the in situ measured hourly mean CO<inline-formula><mml:math id="M319" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> dry-air mole
fractions at Beromünster (black) from the 212.5 m sample inlet matching
at hours when air samples were collected for radiocarbon analysis and the
corresponding background CO<inline-formula><mml:math id="M320" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> at Jungfraujoch (blue). During the
measurement period, we recorded CO<inline-formula><mml:math id="M321" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios between 389 and
417 ppm. Spikes of CO<inline-formula><mml:math id="M322" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were observed mainly during winter, associated
with weak vertical mixing and enhanced anthropogenic emissions, while lower
CO<inline-formula><mml:math id="M323" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios were recorded during summer due to strong vertical
mixing and photosynthetic uptake.</p>
      <p>Isotopic analysis of the air samples yielded <inline-formula><mml:math id="M324" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M325" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">meas</mml:mi></mml:msub></mml:math></inline-formula>
between <inline-formula><mml:math id="M326" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>12.3 and <inline-formula><mml:math id="M327" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>22.8 ‰, with no clear seasonal trend, after
correction for the model-simulated contribution from NPPs (Fig. 2b). Based on
the simulations described in Sect. 2.4.2, we have calculated a mean
enhancement in <inline-formula><mml:math id="M328" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C of <inline-formula><mml:math id="M329" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>1.6 ‰ and a maximum of
<inline-formula><mml:math id="M330" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>8.4 ‰ due to NPPs. This agrees qualitatively with the
coarse-resolution simulations of Graven and Gruber (2011), which suggest a mean
enhancement of <inline-formula><mml:math id="M331" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>1.4 to <inline-formula><mml:math id="M332" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2.8 ‰ over this region (Graven and
Gruber, 2011). While about 70 % of this contribution is due to Swiss
NPPs, the remaining contribution is of foreign origin. About 75 % of the
contribution from the Swiss NPPs is due to Mühleberg, which is located
west of Beromünster and hence frequently upstream of the site, due to the
prevailing westerly winds (Oney et al., 2015). Note that each data point
represents a mean value of the triplicate samples collected consecutively
with a standard error of 2 ‰ among triplicates. During this period,
the background <inline-formula><mml:math id="M333" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values measured at Jungfraujoch varied between
15 and 28 ‰. Regional depletions in <inline-formula><mml:math id="M334" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C due to
fossil fuel emissions, i.e., differences between Beromünster and the
clean-air reference site Jungfraujoch, were in the range of <inline-formula><mml:math id="M335" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.7 to
<inline-formula><mml:math id="M336" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>29.9 ‰ with a mean value of <inline-formula><mml:math id="M337" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>9.9 ‰.</p>
      <p>Figure 2c shows the corresponding CO<inline-formula><mml:math id="M338" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> determined after
correcting for radiocarbon emissions from NPPs. The typical uncertainty in
CO<inline-formula><mml:math id="M339" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> is 1.2 ppm calculated by quadratically combining a mean
<inline-formula><mml:math id="M340" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measurement uncertainty of 2.0 ‰ in both the sample
and the background values, 0.3 ‰ from biospheric correction,
0.5 ‰ from interlaboratory offset, and a mean uncertainty of
1.2 ‰ in the estimation of <inline-formula><mml:math id="M341" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C contribution from NPPs. A mean
fossil fuel CO<inline-formula><mml:math id="M342" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> contribution of 4.3 ppm was calculated from these
samples. Few cases, notably the sample from 27 March 2014, showed a higher
CO<inline-formula><mml:math id="M343" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and a strong depletion in <inline-formula><mml:math id="M344" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math id="M345" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">meas</mml:mi></mml:msub></mml:math></inline-formula>,
consistent with the high CO<inline-formula><mml:math id="M346" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratio shown in the top panel. This
could be due to a strong local fossil fuel contribution or a polluted air mass
transported from other regions of Europe coinciding with the grab samplings.
As this event occurred during a period with moderate temperatures (mean
temperature of 6.8 <inline-formula><mml:math id="M347" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C measured at the highest level of the
Beromünster tower between March and May), strong fossil fuel CO<inline-formula><mml:math id="M348" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
emissions due to heating are not expected. The FLEXPART-COSMO transport
simulations for this event suggest an air mass origin from southeastern
Europe (see Supplement). Periods with winds from the east, colloquially known
as Bise, are well known to be associated with very stable boundary layers and
correspondingly strong accumulation of air pollutants during the cold months
of the year between autumn and spring. Air masses reaching Beromünster
from eastern Europe have recently been reported to contain unusually high
levels of CO during late winter and early spring periods, coinciding with
this sampling period (Oney et al., 2017).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>Ratios (<inline-formula><mml:math id="M349" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> determined using radiocarbon measurements
after correcting for influence from NPPs and applying model II regression,
and ratios derived from continuous CO and CO<inline-formula><mml:math id="M350" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements by the CRDS
analyzer as enhancements (<inline-formula><mml:math id="M351" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO : <inline-formula><mml:math id="M352" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M353" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> using
Jungfraujoch background measurements. <inline-formula><mml:math id="M354" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values are given in
mmol mol<inline-formula><mml:math id="M355" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> with standard uncertainties of the slope and <inline-formula><mml:math id="M356" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> values
in brackets, and n represents the number of samples for the radiocarbon
method. Note that, according to the Swiss emission inventory report for
greenhouse gas emissions in 2013, the annual anthropogenic CO <inline-formula><mml:math id="M357" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> CO<inline-formula><mml:math id="M358" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
emission ratio for the national estimate is 7.8 mmol mol<inline-formula><mml:math id="M359" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"><inline-formula><mml:math id="M360" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M361" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO : <inline-formula><mml:math id="M362" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M363" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Number of</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math id="M364" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO : <inline-formula><mml:math id="M365" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M366" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">(radiocarbon)</oasis:entry>  
         <oasis:entry colname="col3">samples (<inline-formula><mml:math id="M367" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col4">(CRDS)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Winter (Dec–Feb)</oasis:entry>  
         <oasis:entry colname="col2">12.5 <inline-formula><mml:math id="M368" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.3 (0.6)</oasis:entry>  
         <oasis:entry colname="col3">8</oasis:entry>  
         <oasis:entry colname="col4">7.3 (0.9)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Summer (Jun–Aug)</oasis:entry>  
         <oasis:entry colname="col2">14.1 <inline-formula><mml:math id="M369" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 4.0 (0.3)</oasis:entry>  
         <oasis:entry colname="col3">14</oasis:entry>  
         <oasis:entry colname="col4">13.4 (0.02)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">All data</oasis:entry>  
         <oasis:entry colname="col2">13.4 <inline-formula><mml:math id="M370" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.3 (0.6)</oasis:entry>  
         <oasis:entry colname="col3">45</oasis:entry>  
         <oasis:entry colname="col4">8.3 (0.5)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p>By subtracting the background and fossil fuel CO<inline-formula><mml:math id="M371" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> contributions from
the measured mixing ratios, CO<inline-formula><mml:math id="M372" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> values were also determined, ranging
between <inline-formula><mml:math id="M373" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>11.2 and <inline-formula><mml:math id="M374" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>12.4 ppm (Fig. 2d). Even if there is no clear
seasonal trend, the lowest CO<inline-formula><mml:math id="M375" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> values were recorded during
summer, implying net photosynthetic CO<inline-formula><mml:math id="M376" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> uptake, while most of the values in
winter are positive or close to zero due to respiration. During summer 2015,
we observed strong variability in both CO<inline-formula><mml:math id="M377" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and CO<inline-formula><mml:math id="M378" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (Fig. 2a
and d). However, this period was one of the hottest and driest summers in
central Europe (Orth et al., 2016). In Switzerland, it was the
second-hottest summer since the beginning of measurements in 1864 with most
of the extreme dates in July (MeteoSuisse, 2015). Such climate
extremes can lead to enhanced respiration and reduced photosynthesis and, in
turn, higher CO<inline-formula><mml:math id="M379" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and CO<inline-formula><mml:math id="M380" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> in the atmosphere. Looking
specifically at the two data points in June and July 2015, the daily average
temperatures recorded at Beromünster were 24.6 and 26 <inline-formula><mml:math id="M381" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C at the highest inlet of 212.5 m (Fig. 2e). Based on
measurements at Beromünster and other cities of the CarboCount CH
network in 2013, Oney et al. (2017) reported that for a daily mean
temperature of greater than 20 <inline-formula><mml:math id="M382" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C the biosphere over the Swiss
plateau tends to become a net CO<inline-formula><mml:math id="M383" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> source. The observed positive spikes
in CO<inline-formula><mml:math id="M384" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (Fig. 2a) and CO<inline-formula><mml:math id="M385" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (Fig. 2d) likely resulted from such
extremes.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <?xmltex \opttitle{$R_{\mathrm{CO}}$ values from radiocarbon measurements}?><title><inline-formula><mml:math id="M386" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values from radiocarbon measurements</title>
      <p>From the simultaneous CO and radiocarbon measurements, we calculated an
<inline-formula><mml:math id="M387" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of 13.4 <inline-formula><mml:math id="M388" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.3 mmol CO/mol CO<inline-formula><mml:math id="M389" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with a
correlation coefficient (<inline-formula><mml:math id="M390" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> of 0.7 and a median value of
11.2 mmol CO/mol CO<inline-formula><mml:math id="M391" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (note that change in <inline-formula><mml:math id="M392" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is
insignificant when we use smoothed <inline-formula><mml:math id="M393" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C background from Jungfraujoch).
When we split the data seasonally, <inline-formula><mml:math id="M394" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values of 12.5 <inline-formula><mml:math id="M395" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.3
and 14.1 <inline-formula><mml:math id="M396" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 4.0 mmol CO/mol CO<inline-formula><mml:math id="M397" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were obtained during winter and
summer, respectively (Table 1). Even if the two values are not significantly
different considering the uncertainties, the very low correlation coefficient
during summer (<inline-formula><mml:math id="M398" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula>) implies a larger uncertainty in the derived
<inline-formula><mml:math id="M399" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Our wintertime estimate is well within the range of values
from previous studies (10–15 mmol mol<inline-formula><mml:math id="M400" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) observed at other sites in
Europe and North America (Gamnitzer et al., 2006; Vogel et al., 2010;
Turnbull et al., 2011a). To test the sensitivity of this ratio to the
selection of background site, we additionally calculated <inline-formula><mml:math id="M401" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
using background values estimated with the REBS method from the in situ CO
measurements at Beromünster instead of Jungfraujoch. The value obtained
in this way (12.7 <inline-formula><mml:math id="M402" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.2, <inline-formula><mml:math id="M403" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.6</mml:mn></mml:mrow></mml:math></inline-formula>) is not significantly different
from the value obtained using Jungfraujoch as the background site.
Considering the persistent decrease in CO emissions (Zellweger et al., 2009)
in response to the European emission legislation, our estimated
<inline-formula><mml:math id="M404" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is surprisingly high. A recent study investigating the
CO / CO<inline-formula><mml:math id="M405" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratio from road traffic in Islisberg tunnel, Switzerland,
also observed a significant decrease in this ratio compared to previous
estimates, pointing to a substantial reduction in CO emissions from road
traffic, with a CO <inline-formula><mml:math id="M406" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> CO<inline-formula><mml:math id="M407" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratio of 4.15 <inline-formula><mml:math id="M408" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.34 ppb ppm<inline-formula><mml:math id="M409" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
(Popa et al., 2014). This may indicate a significant contribution from
non-road traffic emissions, which account for more than 70 % of the total
CO<inline-formula><mml:math id="M410" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emissions leading to the high apparent <inline-formula><mml:math id="M411" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p>The <inline-formula><mml:math id="M412" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> value derived in this study is significantly higher than the
anthropogenic CO / CO<inline-formula><mml:math id="M413" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emission ratio of 7.8 mmol mol<inline-formula><mml:math id="M414" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> calculated from
Switzerland's greenhouse gas inventory report for 2013 (FOEN, 2015b, a).
However, this can be due to enhanced CO emissions transported from other
European cities towards Beromünster. Oney et al. (2017) observed
particularly large CO <inline-formula><mml:math id="M415" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> CO<inline-formula><mml:math id="M416" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratios at Beromünster during several
pollution events in late winter and early spring 2013 which were associated
with air mass transport from eastern Europe, where poorly controlled
combustion of biofuels and coal likely results in high ratios.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <?xmltex \opttitle{$\Delta$CO\,$/$\,$\Delta$CO${}_{{2}}$ from continuous measurements}?><title><inline-formula><mml:math id="M417" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO <inline-formula><mml:math id="M418" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M419" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M420" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from continuous measurements</title>
      <p>Figure 3 shows the seasonally resolved correlations of <inline-formula><mml:math id="M421" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO with
<inline-formula><mml:math id="M422" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M423" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> derived from in situ measured CO and CO<inline-formula><mml:math id="M424" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> enhancements
over the background observed at Jungfraujoch, for which we estimated a tracer
ratio of 8.3 <inline-formula><mml:math id="M425" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.1 mmol mol<inline-formula><mml:math id="M426" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math id="M427" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula>) for the entire
measurement period. Considering the seasonally resolved <inline-formula><mml:math id="M428" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO <inline-formula><mml:math id="M429" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M430" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M431" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratios, barely any correlation is observed in
summer, and weak correlations (<inline-formula><mml:math id="M432" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> &lt; 0.4) are observed during
spring and autumn. This can be due to the dominance of biogenic fluxes over
fossil fuel fluxes during these periods of the year. From measurements during
winter, when the two species are most strongly correlated, a <inline-formula><mml:math id="M433" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO <inline-formula><mml:math id="M434" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M435" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M436" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratio of 7.3 <inline-formula><mml:math id="M437" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.1 mmol mol<inline-formula><mml:math id="M438" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
(<inline-formula><mml:math id="M439" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.9</mml:mn></mml:mrow></mml:math></inline-formula>) is obtained. Recently, Oney et al. (2017) reported a higher
wintertime ratio of 8.3 mmol mol<inline-formula><mml:math id="M440" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> for the same combination of
measurements at Beromünster and Jungfraujoch but for a different time
period. If we consider only winter 2013 as in their data, we obtain
essentially the same value, while much lower ratios of 6.5 and
6.4 mmol mol<inline-formula><mml:math id="M441" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> were calculated for 2014 and 2015, respectively. The
higher ratios in winter 2013 are likely related to the unusually cold
conditions and extended periods of air mass transport from eastern Europe.
Note that, in contrast to <inline-formula><mml:math id="M442" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, these enhancement ratios also
include emissions from non-fossil sources such as biofuels and biomass
burning as well as the influence of biogenic fluxes. The Swiss national
inventory attributes about 15 % of total CO<inline-formula><mml:math id="M443" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emissions in 2014 to
non-fossil-fuel sources (FOEN, 2015b). If we correct for these sources
assuming a constant contribution throughout the year, the wintertime <inline-formula><mml:math id="M444" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO <inline-formula><mml:math id="M445" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M446" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M447" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratio for the 3-year data becomes
8.7 mmol mol<inline-formula><mml:math id="M448" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>The correlation between enhancements in CO and CO<inline-formula><mml:math id="M449" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> at
Beromünster over Jungfraujoch background for the different seasons. The
black dots and the black solid line correspond to the individual wintertime
<inline-formula><mml:math id="M450" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values and the linear fit to these points, respectively.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10753/2017/acp-17-10753-2017-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p>Time series of hourly mean CO mixing ratios measured at
Jungfraujoch <bold>(a)</bold> and Beromünster <bold>(b)</bold> sites, with the red
curve showing the estimated background values using the REBS method with
60-day window. Panel <bold>(c)</bold> shows the hourly mean CO<inline-formula><mml:math id="M451" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>
time series calculated using the emission ratios determined from radiocarbon
measurements, and the CO enhancements at Beromünster over the
Jungfraujoch background based on Eq. (7). The blue dots in panel <bold>(c)</bold>
shows the CO<inline-formula><mml:math id="M452" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> values determined using the radiocarbon
measurements.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10753/2017/acp-17-10753-2017-f04.png"/>

        </fig>

      <p>This ratio of 8.7 mmol mol<inline-formula><mml:math id="M453" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> is still about 30 % lower than the
<inline-formula><mml:math id="M454" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> estimate for the same period of 12.5 mmol mol<inline-formula><mml:math id="M455" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, shown
as a black line in Fig. 3. This suggests that despite the strong correlation
between <inline-formula><mml:math id="M456" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO and <inline-formula><mml:math id="M457" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M458" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in winter the regional CO<inline-formula><mml:math id="M459" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
enhancements are not only caused by anthropogenic emissions but include a
significant contribution from biospheric respiration. Miller et al. (2012)
showed that such strong correlations between CO<inline-formula><mml:math id="M460" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and CO during winter
may arise from respiratory fluxes co-located with fossil fuel fluxes trapped
under the wintertime shallow and stable boundary layer but with strongly
biased ratios when compared to <inline-formula><mml:math id="M461" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Turnbull et al. (2011b) also
observed a substantial contribution of biospheric CO<inline-formula><mml:math id="M462" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> fluxes even during
winter (20–30 % from non-fossil-fuel sources including photosynthesis
and respiration) from samples collected at two sites in East Asia. The
magnitude of these fluxes was roughly similar to the CO<inline-formula><mml:math id="M463" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> flux
when continental background was used (Turnbull et al., 2015). Hence, the
observed correlation between <inline-formula><mml:math id="M464" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO and <inline-formula><mml:math id="M465" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M466" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in this study
is not only due to spatially and temporally correlated sources but is caused
to a large extent by meteorological variability associated with more or less
accumulation of trace gases in the boundary layer irrespective of their
sources. This interpretation is also supported by the fact that a strong
correlation (<inline-formula><mml:math id="M467" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> &gt; 0.7) was also observed between CO and
CH<inline-formula><mml:math id="M468" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> during winter at the same tower site (Satar et al., 2016) despite
their sources being vastly distinct. In Switzerland about 80 % of
CH<inline-formula><mml:math id="M469" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> emissions are from agriculture (mainly from ruminants), while more
than 85 % of CO emissions are from the transport sector and residential
heating (FOEN, 2015a).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p>Time series (hourly resolution) of the biospheric CO<inline-formula><mml:math id="M470" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> derived
as a residual of the difference between the total CO<inline-formula><mml:math id="M471" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>,
CO<inline-formula><mml:math id="M472" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bg</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>, and CO<inline-formula><mml:math id="M473" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> for all data <bold>(a)</bold>, and only afternoon data from
12:00–15:00 UTC <bold>(b)</bold>. The green lines show negative
CO<inline-formula><mml:math id="M474" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>, implying uptake, while red ones represent positive
CO<inline-formula><mml:math id="M475" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>. The average uncertainty of CO<inline-formula><mml:math id="M476" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> amounts
<inline-formula><mml:math id="M477" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1.3 ppm calculated from error propagation.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10753/2017/acp-17-10753-2017-f05.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <?xmltex \opttitle{High-resolution time series of CO${}_{\mathrm{2ff}}$ and CO${}_{\mathrm{2bio}}$}?><title>High-resolution time series of CO<inline-formula><mml:math id="M478" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and CO<inline-formula><mml:math id="M479" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula></title>
      <p>Figure 4 shows the hourly mean CO mixing ratios at Jungfraujoch and
Beromünster between 2013 and 2015. CO mixing ratios as high as 480 ppb
were recorded at Beromünster, while generally lower CO values were
recorded at the more remote site Jungfraujoch. A pronounced seasonality in
CO can be observed at Beromünster with higher values in winter and lower
values during summer due to stronger vertical mixing and chemical depletion
of CO by OH (Satar et al., 2016). The hourly mean
CO<inline-formula><mml:math id="M480" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> time series calculated using these continuous CO measurements and
the seasonally resolved <inline-formula><mml:math id="M481" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values derived using the radiocarbon
measurements are displayed in Fig. 4c. A seasonal trend in the calculated
CO<inline-formula><mml:math id="M482" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> is observed with frequent spikes of CO<inline-formula><mml:math id="M483" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> during
winter, while summer values show less variability. We calculated a monthly mean
amplitude (peak to trough) of 6.3 ppm with a maximum in February and a
minimum in July. During the measurement period, we observed CO<inline-formula><mml:math id="M484" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>
mixing ratios ranging up to 27 ppm coinciding with cold periods and likely
from enhanced anthropogenic emissions due to heating. Instances of slightly
negative CO<inline-formula><mml:math id="M485" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> contributions, which occurred during less than 5 % of
the time, were associated with negative enhancements in CO (i.e., <inline-formula><mml:math id="M486" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO &lt; 0). This could be simply due to an overestimation of background
values by the REBS function during these periods.</p>
      <p>Figure 5a shows the hourly averaged residual CO<inline-formula><mml:math id="M487" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> values, which
exhibit not only a clear seasonal cycle but also a considerable scatter in all
seasons, ranging from <inline-formula><mml:math id="M488" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13 to <inline-formula><mml:math id="M489" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>30 ppm. During winter, most values were close to
zero or positive, implying a dominance of respiration fluxes. In summer,
conversely, pronounced negative and positive excursions were observed mostly
due to the diurnal cycle in net CO<inline-formula><mml:math id="M490" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> fluxes, which are dominated by
photosynthetic uptake during daytime and respiration at night. Another factor
contributing to such variations may be the application of a constant emission
ratio neglecting any diurnal variability (Vogel et al., 2010).</p>
      <p>It should also be noted that any non-fossil-fuel CO<inline-formula><mml:math id="M491" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> sources such as
emissions from biofuels would be incorporated into the CO<inline-formula><mml:math id="M492" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> term
since CO<inline-formula><mml:math id="M493" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> in Eq. (1) represents the fossil fuel sources only, adding
more variability to the data set. In order to reduce the influence of these
diurnal factors, we have looked into afternoon CO<inline-formula><mml:math id="M494" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> values (12:00–15:00 UTC), when the CO<inline-formula><mml:math id="M495" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios along the tower are uniform
(Satar et al., 2016) and <inline-formula><mml:math id="M496" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> variability is minimal.
Similar to the seasonal pattern in Fig. 5a, a clear seasonal cycle in
biospheric CO<inline-formula><mml:math id="M497" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> can be observed (Fig. 5b) in agreement with biospheric
exchange, but both positive and negative extremes are less frequently
observed (<inline-formula><mml:math id="M498" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>12 to <inline-formula><mml:math id="M499" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>22 ppm).</p>
      <p>The variation in CO<inline-formula><mml:math id="M500" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> during afternoon (12:00–15:00 UTC) was
recently estimated at this site at a range of <inline-formula><mml:math id="M501" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20 to <inline-formula><mml:math id="M502" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>20 ppm by
combining observations and model simulations for the year 2013
(Oney et al., 2017). Our estimates are more positive than those in their study,
due to the higher <inline-formula><mml:math id="M503" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> which results in lower
CO<inline-formula><mml:math id="M504" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and correspondingly higher CO<inline-formula><mml:math id="M505" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> values.</p>
      <p>Biospheric CO<inline-formula><mml:math id="M506" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> shows a seasonally dependent diurnal variation as shown
in Fig. 6. During winter (December–February), the biospheric CO<inline-formula><mml:math id="M507" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
component remains consistently positive (<inline-formula><mml:math id="M508" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 to <inline-formula><mml:math id="M509" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>5 ppm) throughout the
day, implying net respiration fluxes. In summer, a clear feature with
increasing CO<inline-formula><mml:math id="M510" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> values during the night peaking between 07:00
and 08:00 UTC (i.e., between 08:00 and 09:00 local time) can be observed.
This buildup during the night can be explained by CO<inline-formula><mml:math id="M511" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from respiration
fluxes accumulating in the stable and shallow nocturnal boundary layer. Then,
after sunrise, the early morning CO<inline-formula><mml:math id="M512" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> peak starts to gradually
decrease due to a combination of onset of photosynthesis and enhanced
vertical mixing due to the growth of the boundary layer. At Beromünster,
a decrease in CO<inline-formula><mml:math id="M513" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios from both processes is visible more or
less at the same time at the 212.5 m height level. As reported by Satar et
al. (2016), this decrease in early morning CO<inline-formula><mml:math id="M514" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations at the
212 m inlet lags behind the decrease at the lowest sampling level of 12.5 m
by approximately 1 h. Between 12:00 and 15:00 UTC, when the daytime
convective boundary layer is fully established, the biospheric CO<inline-formula><mml:math id="M515" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
continues to become more negative, implying net photosynthetic uptake, which
eventually stabilizes for 3–5 h until nighttime CO<inline-formula><mml:math id="M516" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>
accumulation starts.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p>Hourly variations of monthly averaged biospheric CO<inline-formula><mml:math id="M517" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during
summer (June–August) and winter (December–February). While winter values
dominated by respiration are constant throughout a day, summer values show a
significant diurnal variation induced by photosynthesis and vertical mixing.
The error bars are the standard deviations of the hourly averaged
CO<inline-formula><mml:math id="M518" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> values for each month.</p></caption>
          <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10753/2017/acp-17-10753-2017-f06.png"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <title>Conclusions</title>
      <p>From continuous measurements of CO and CO<inline-formula><mml:math id="M519" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and biweekly radiocarbon
samples at the Beromünster tall tower, we have estimated a <inline-formula><mml:math id="M520" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO / <inline-formula><mml:math id="M521" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>CO<inline-formula><mml:math id="M522" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> ratio (<inline-formula><mml:math id="M523" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> which was
subsequently used to construct a 2.3-year-long high-resolution
CO<inline-formula><mml:math id="M524" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> time series. We have corrected the ratio for an offset of
about 16 % caused by <inline-formula><mml:math id="M525" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C emissions from nearby NPPs. This bias was
calculated by comparing the simulated mean enhancement in <inline-formula><mml:math id="M526" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
(1.6 ‰) due to NPPs with the measured mean depletion in
<inline-formula><mml:math id="M527" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C due to fossil fuel CO<inline-formula><mml:math id="M528" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (9.9 ‰). The
radiocarbon-based <inline-formula><mml:math id="M529" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> derived in this study during winter is
about 30 % higher than the CO:CO<inline-formula><mml:math id="M530" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> enhancement ratios estimated from
continuous CO and CO<inline-formula><mml:math id="M531" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements during the same period, suggesting a
significant biospheric contribution to regional CO<inline-formula><mml:math id="M532" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> enhancements during
this period. This is in agreement with previous studies that observed
20–30 % biospheric contribution during winter (Turnbull et al., 2011b).</p>
      <p>The obtained CO<inline-formula><mml:math id="M533" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> time series shows a clear seasonality with frequent
spikes during winter associated with enhanced anthropogenic emissions and
weak vertical mixing, while summer values are mostly stable.</p>
      <p>By subtracting the estimated CO<inline-formula><mml:math id="M534" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and CO<inline-formula><mml:math id="M535" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bg</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> from CO<inline-formula><mml:math id="M536" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">meas</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>, we
have also calculated the biospheric CO<inline-formula><mml:math id="M537" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> component, which ranges between
<inline-formula><mml:math id="M538" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>15 and <inline-formula><mml:math id="M539" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>30 ppm. Considering only afternoon data (12:00–15:00 UTC),
when the convective boundary layer is fully established, CO<inline-formula><mml:math id="M540" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> showed
its minimum in summer coinciding with net photosynthetic uptake but still
with frequent positive excursions, especially during summer 2015, possibly
driven by the record hot and dry summer during this period. During winter,
CO<inline-formula><mml:math id="M541" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> becomes nearly zero or positive, implying respiration fluxes.</p>
      <p><?xmltex \hack{\newpage}?>A pronounced diurnal variation in CO<inline-formula><mml:math id="M542" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> was observed during
summer modulated by vertical mixing and biospheric exchange, while this
variation disappears during winter. However, the variation in
CO<inline-formula><mml:math id="M543" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">bio</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> may also be influenced by the uncertainty of the
CO<inline-formula><mml:math id="M544" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> estimate, especially due to applying a constant emission
ratio while calculating CO<inline-formula><mml:math id="M545" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>. Hence, it will be important in the
future to include seasonally and diurnally resolved <inline-formula><mml:math id="M546" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values
from high-frequency radiocarbon measurements to better estimate
CO<inline-formula><mml:math id="M547" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">ff</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>. Detailed analysis of the planetary boundary layer height
may also provide useful information to better clarify such variations, and it
will be the focus of future studies. Additionally, including independent
tracers such as atmospheric potential oxygen estimates
based on concurrent CO<inline-formula><mml:math id="M548" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M549" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements will be very useful to
validate fossil fuel emission estimates from the radiocarbon method. This
technique is also advantageous as the fossil fuel CO<inline-formula><mml:math id="M550" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> estimate is
unaltered by contribution from NPPs, and it accounts for the contribution
from biofuels.</p>
</sec>

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

      <p>CO<inline-formula><mml:math id="M551" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements are available through the Obspack
data set under the Cooperative Global Atmospheric Data Integration
Project (2017). Multi-laboratory compilation of atmospheric carbon dioxide
data for the period 1957–2016;
obspack_co2_1_GLOBALVIEWplus_v3.0_2017-08-11 [Data set]. NOAA Earth
System Research Laboratory, Global Monitoring Division.
<ext-link xlink:href="https://doi.org/10.15138/g3cw4q" ext-link-type="DOI">10.15138/g3cw4q</ext-link>. Carbon monoxide, radioncarbon, CO2ff and CO2bio data
can be requested from M. Leuenberger (leuenberger@climate.unibe.ch).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p><bold>The Supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-17-10753-2017-supplement" xlink:title="zip">https://doi.org/10.5194/acp-17-10753-2017-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
        </app-group><notes notes-type="competinginterests">

      <p>The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p>This project was funded by the Swiss National Science Foundation through the
Sinergia project CarboCount CH (CRSII2 136273). We are also grateful to
ICOS-Switzerland and the International Foundation High Alpine Research
Stations Jungfraujoch and Gornergrat. The LARA laboratory would like to
thank René Fischer for the production of large CO<inline-formula><mml:math id="M552" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> amounts by
combustion of the NIST standard oxalic acid II, and Dejan Husrefovic for the
evaluation of the sample transfer line. Finally, we would like to thank
Heather Graven and Nicolas Gruber for helpful input regarding radiocarbon
emissions from NPPs and the Swiss Federal Nuclear Safety Inspectorate (ENSI)
and the Berner Kraftwerke (BKW) for fruitful discussions and providing
radiocarbon emission data.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: Thomas Röckmann<?xmltex \hack{\newline}?>
Reviewed by: Jocelyn Turnbull and one anonymous referee</p></ack><ref-list>
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    <!--<article-title-html>Estimation of the fossil fuel component in atmospheric CO<sub>2</sub> based on radiocarbon measurements at the Beromünster tall tower, Switzerland</article-title-html>
<abstract-html><p class="p">Fossil fuel CO<sub>2</sub> (CO<sub>2ff</sub>) is the major contributor
of anthropogenic CO<sub>2</sub> in the atmosphere, and accurate quantification is
essential to better understand the carbon cycle. Since October 2012, we have
been continuously measuring the mixing ratios of CO, CO<sub>2</sub>, CH<sub>4</sub>, and
H<sub>2</sub>O at five different heights at the Beromünster tall tower,
Switzerland. Air samples for radiocarbon (Δ<sup>14</sup>CO<sub>2</sub>) analysis
have also been collected from the highest sampling inlet (212.5 m) of the
tower on a biweekly basis. A correction was applied for <sup>14</sup>CO<sub>2</sub>
emissions from nearby nuclear power plants (NPPs), which have been simulated
with the Lagrangian transport model FLEXPART-COSMO. The <sup>14</sup>CO<sub>2</sub>
emissions from NPPs offset the depletion in <sup>14</sup>C by fossil fuel
emissions, resulting in an underestimation of the fossil fuel component in atmospheric
CO<sub>2</sub> by about 16 %. An average observed ratio (<i>R</i><sub>CO</sub>) of 13.4 ± 1.3 mmol mol<sup>−1</sup>
was calculated from the enhancements in CO mixing ratios
relative to the clean-air reference site Jungfraujoch (ΔCO) and the
radiocarbon-based fossil fuel CO<sub>2</sub> mole fractions. The wintertime
<i>R</i><sub>CO</sub> estimate of 12.5 ± 3.3 is about 30 % higher than the
wintertime ratio between in situ measured CO and CO<sub>2</sub> enhancements at
Beromünster over the Jungfraujoch background (8.7 mmol mol<sup>−1</sup>) corrected for
non-fossil contributions due to strong biospheric contribution despite the
strong correlation between ΔCO and ΔCO<sub>2</sub> in winter. By
combining the ratio derived using the radiocarbon measurements and the
in situ measured CO mixing ratios, a high-resolution time series of
CO<sub>2ff</sub> was calculated exhibiting a clear seasonality driven by seasonal
variability in emissions and vertical mixing. By subtracting the fossil fuel
component and the large-scale background, we have determined the regional
biospheric CO<sub>2</sub> component that is characterized by seasonal variations
ranging between −15 and +30 ppm. A pronounced diurnal variation was observed
during summer modulated by biospheric exchange and vertical mixing, while no
consistent pattern was found during winter.</p></abstract-html>
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