<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "journalpub-oasis3.dtd">
<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" dtd-version="3.0">
  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">AMT</journal-id>
<journal-title-group>
<journal-title>Atmospheric Measurement Techniques</journal-title>
<abbrev-journal-title abbrev-type="publisher">AMT</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Meas. Tech.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1867-8548</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/amt-9-5607-2016</article-id><title-group><article-title>Stratospheric Air Sub-sampler (SAS) and its application to analysis
of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) from small air samples collected with an AirCore</article-title>
      </title-group><?xmltex \runningtitle{Stratospheric Air Sub-sampler (SAS)}?><?xmltex \runningauthor{D. J. Mrozek et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Mrozek</surname><given-names>Dorota Janina</given-names></name>
          <email>dorota.mrozek@gmail.com</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>van der Veen</surname><given-names>Carina</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Hofmann</surname><given-names>Magdalena E. G.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Chen</surname><given-names>Huilin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1573-6673</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Kivi</surname><given-names>Rigel</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-8828-2759</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Heikkinen</surname><given-names>Pauli</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Röckmann</surname><given-names>Thomas</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6688-8968</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Institute for Marine and Atmospheric research Utrecht (IMAU), Utrecht University, Princetonplein 5,<?xmltex \hack{\break}?> 3584CC Utrecht, the Netherlands</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Centre for Isotope Research (CIO), Energy and Sustainability Research Institute Groningen,<?xmltex \hack{\break}?> University of Groningen, the Netherlands</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Cooperative Institute for Research in Environmental Sciences (CIRES), University of Colorado, Boulder, Colorado, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Finnish Meteorological Institute (FMI), Arctic Research, Sodankyä, Finland</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Dorota Janina Mrozek (dorota.mrozek@gmail.com)</corresp></author-notes><pub-date><day>25</day><month>November</month><year>2016</year></pub-date>
      
      <volume>9</volume>
      <issue>11</issue>
      <fpage>5607</fpage><lpage>5620</lpage>
      <history>
        <date date-type="received"><day>9</day><month>April</month><year>2016</year></date>
           <date date-type="rev-request"><day>15</day><month>July</month><year>2016</year></date>
           <date date-type="rev-recd"><day>8</day><month>October</month><year>2016</year></date>
           <date date-type="accepted"><day>18</day><month>October</month><year>2016</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016.html">This article is available from https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016.html</self-uri>
<self-uri xlink:href="https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016.pdf">The full text article is available as a PDF file from https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016.pdf</self-uri>


      <abstract>
    <p>We present the set-up and a scientific application of the Stratospheric Air
Sub-sampler (SAS), a device to collect and to store the vertical profile of
air collected with an AirCore <xref ref-type="bibr" rid="bib1.bibx16" id="paren.1"/> in numerous sub-samples for
later analysis in the laboratory. The SAS described here is a 20 m long 1/4 inch stainless steel tubing that is separated by eleven valves to divide the
tubing into 10 identical segments, but it can be easily adapted to collect
smaller or larger samples. In the collection phase the SAS is directly
connected to the outlet of an optical analyzer that measures the mole
fractions of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and CO from an AirCore sampler. The stratospheric
part (or if desired any part of the AirCore air) is then directed through the
SAS. When the SAS is filled with the selected air, the valves are closed and
the vertical profile is maintained in the different segments of the SAS. The
segments can later be analysed to retrieve vertical profiles of other trace
gas signatures that require slower instrumentation. As an application, we
describe the coupling of the SAS to an analytical system to determine the
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O excess of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, which is a tracer for photochemical processing of
stratospheric air. For this purpose the analytical system described by
<xref ref-type="bibr" rid="bib1.bibx23" id="normal.2"/> was adapted for analysis of air directly from the SAS. The
performance of the coupled system is demonstrated for a set of air samples
from an AirCore flight in November 2014 near Sodankylä, Finland. The
standard error for a 25 mL air sample at stratospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mole fraction
is 0.56 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> (1<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and 0.03 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>
(1<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) for both <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C. Measured
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) values show a clear correlation with N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O in
agreement with already published data.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

      <?xmltex \hack{\vspace{-3mm}}?>
<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>Monitoring and studying the distribution of greenhouse gases throughout the
atmospheric column is an important constituent of understanding contemporary
climate change. Carbon dioxide (CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) is the most important molecule of the
atmospheric carbon cycle and the increase of its abundance in the atmosphere
is the primary factor of recent radiative forcing <xref ref-type="bibr" rid="bib1.bibx13" id="paren.3"/>. In the
stratosphere the <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O excess of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (expressed as
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>)) is a valuable long-lived tracer for stratospheric
chemistry and atmospheric circulation patterns. Measurement of the mole
fraction and oxygen isotopic composition of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> provides information on
both transport times and photochemical lifetimes of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
<xref ref-type="bibr" rid="bib1.bibx7 bib1.bibx28" id="paren.4"/>. Over the past decades several sampling
campaigns have been carried out to observe and to understand the oxygen
isotope enrichments of stratospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
<xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx1 bib1.bibx19 bib1.bibx7 bib1.bibx18 bib1.bibx28" id="paren.5"/>.
Unfortunately, measurement campaigns with rockets, balloons and aircraft
platforms are expensive and therefore it is in general difficult to obtain
stratospheric samples.</p>
      <p>The simple and lightweight sampling system AirCore <xref ref-type="bibr" rid="bib1.bibx16" id="paren.6"/> provides
new opportunities to sampling the high altitude atmosphere at relatively low
cost. The AirCore device consists of a long (usually 100 m of longer) piece
of coiled stainless steel tubing that is lifted to the stratosphere on a
balloon with one end open and the other end closed. During ascent, the
AirCore empties because of the decrease in pressure; during descent,
ambient air successively fills the AirCore coil again as pressure increases.
The atmospheric profile information in the coil is preserved because of
limited gas diffusion inside the long tube. This means that the altitude
profiles of various trace gases  such as CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and CO can be
determined by processing the content of the AirCore through a fast analytical
system quickly after recovery of the sampler.</p>
      <p>Previously, the air from an AirCore was vented after analysis with a real
time gas analyzer and not used for other, more sophisticated and slower,
analyses. We developed a Stratospheric Air Sub-sampler (SAS) that collects
(the stratospheric fraction of) air from an AirCore directly after online
analysis and stores it in different segments of the SAS so that the profile
is preserved. The SAS can be easily transported and processed, for example
for the isotopic composition of trace gases or for halocarbon analysis. The
limitation of the method is that the analytical system must be capable of
analysing very small air samples, since the total stratospheric fraction of
the AirCore profile is only of the order of 250 mL at ambient temperature and
pressure, which is split into multiple segments in the SAS.</p>
      <p>For the work presented here we apply the SAS concept to measurement of the
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O excess of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the stratospheric sub-samples. The analytical
system described in <xref ref-type="bibr" rid="bib1.bibx23" id="text.7"/> was modified to allow air from the SAS
to be flushed directly by the reference air into a new sample introduction
unit at ambient pressures. The change of the oxidation reagent from CeO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
powder to CuO wires reduced peak broadening and allowed detection of the
equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> peak without focusing on liquid nitrogen trap. The
improved system is fully automated; only the change of the individual SAS
segments is made manually. The successful coupling of the SAS and the
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O analysis system was demonstrated by CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> stable isotope
measurements on stratospheric air obtained from an AirCore flight near
Sodankylä, Finland, in November 2014.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p>A schematic diagram showing the overall procedure described in this
work, from AirCore sampling on the site to IRMS analysis in laboratory.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016-f01.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p>Schematic diagram of the analytical system for trace gas analyses
with a Picarro instrument and for transferring the air from the AirCore coil
into the Stratospheric Air Sub-Sampler (SAS). The three-way valves in the SAS
are in “open to the right” position when the AirCore air is transferred
into the SAS and closed after sub-sampling. The crossed circles are
conventional valves. The open circles at the inlet of the fill-gas and the
calibration-gas cylinder represent cylinder valves and pressure regulators.
The black circle represents the shut-off valve at the end of the AirCore
coil. The drying tube is filled with magnesium perchlorate (Mg(ClO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>)<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>)
from Sigma-Aldrich.</p></caption>
        <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016-f02.png"/>

      </fig>

      <p>We use the common delta notation to quantify isotopic composition,
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mtext>i</mml:mtext></mml:msup><mml:mi mathvariant="italic">δ</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mtext>i</mml:mtext></mml:msup><mml:msub><mml:mi>R</mml:mi><mml:mtext>SA</mml:mtext></mml:msub><mml:msup><mml:mo>/</mml:mo><mml:mtext>i</mml:mtext></mml:msup><mml:msub><mml:mi>R</mml:mi><mml:mtext>ST</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mtext>i</mml:mtext></mml:msup><mml:mi>R</mml:mi></mml:mrow></mml:math></inline-formula> represents the
heavy-to-light isotope ratio <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup><mml:mi>R</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>16</mml:mn></mml:msup></mml:math></inline-formula>O) or <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn>18</mml:mn></mml:msup><mml:mi>R</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>18</mml:mn></mml:msup></mml:math></inline-formula>O <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>16</mml:mn></mml:msup></mml:math></inline-formula>O) of a sample (index SA) or international standard (index
ST). The <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula> values are expressed in <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>. The international reference
material for oxygen isotopes is Vienna Standard Mean Ocean Water (VSMOW) with
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup><mml:msub><mml:mi>R</mml:mi><mml:mtext>VSMOW</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 382.7<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn>2.1</mml:mn></mml:mrow><mml:mrow><mml:mo>+</mml:mo><mml:mn>1.7</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx14" id="paren.8"/>
and <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn>18</mml:mn></mml:msup><mml:msub><mml:mi>R</mml:mi><mml:mtext>VSMOW</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2005.2 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.45 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
<xref ref-type="bibr" rid="bib1.bibx5" id="paren.9"/>. For quantifying the <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O excess of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> we use
the exponential definition
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> [1 <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O] <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> [1 <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mi mathvariant="italic">λ</mml:mi></mml:msup><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> with <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> of 0.528, but note that also
other definitions are in use <xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx14" id="paren.10"/>.</p><?xmltex \hack{\vspace{-3mm}}?>
</sec>
<sec id="Ch1.S2">
  <title>Method</title>
      <p>The stratospheric air samples are collected in a two-step procedure. First,
air samples from the surface up to the ceiling altitude of a stratospheric
balloon flight (typically 30 km) are obtained with an AirCore system.
Second, the stratospheric part of the collected air samples is recovered into
an SAS after online analysis of trace gas
concentrations. The details of the first step <xref ref-type="bibr" rid="bib1.bibx9" id="paren.11"/> are here briefly
described in Sect. <xref ref-type="sec" rid="Ch1.S2.SS1"/>. Section <xref ref-type="sec" rid="Ch1.S2.SS2"/> and <xref ref-type="sec" rid="Ch1.S2.SS3"/> provide the information relevant to the stratospheric air
samples: the sub-sampling method and the description of the analytical system
used for CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> isotope measurement. We include a schematic illustration for
describing all the instruments and procedure in Fig. <xref ref-type="fig" rid="Ch1.F1"/>.</p>
<sec id="Ch1.S2.SS1">
  <title>Stratospheric air sampling with AirCore</title>
      <p>The AirCore device is made of stainless steel tubing coated with
SilcoNert<sup>®</sup>1000 and has a total length of 100 m (40 m at 1/4 inch and 60 m at 1/8 inch, with a  wall thickness of 0.01 inch). The payload
that includes the AirCore and a radiosonde (Vaisala, type RS92-SGPL) weighs
about 3.6 kg. Before each flight the AirCore is filled with a standard dry
fill-gas with known CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and CO mole fractions (CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 386.10 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.09 ppm;
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1880 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2 ppb; CO <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 7972 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5 ppb) and closed with a
shut-off valve at the inlet (Swagelok, part number SS-1GS4). A stratospheric
balloon (Totex, type Tx3000) is used to launch the payload high into the
stratosphere near Sodankylä, Finland. Just before launching the AirCore,
the shut-off valve is opened, so that during the ascent the fill-gas leaves
the AirCore coil due to the drop in pressure. After reaching an altitude of
approximately 30 km, the balloon bursts, and the descent of the payload on a
parachute begins. Ambient air flows into the AirCore and the air from higher
altitudes is continuously compressed and pushed towards the closed end of the
AirCore by air from lower altitudes. The shut-off valve is closed
automatically about 10 s after the landing, and the AirCore is quickly
recovered and transported to the Finnish Meteorological Institute (FMI)
laboratory for analysis.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Sub-sampling into SAS</title>
      <p>The vertical profiles of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and CO mole
fractions are measured within 2–3 h after landing of the AirCore at FMI
using a gas analyzer (Picarro, model G2401), as presented in Fig. <xref ref-type="fig" rid="Ch1.F2"/>. The originally closed end of the AirCore coil is
connected to the analyzer, while the end with the shut-off valve is connected
to the fill-gas cylinder. By opening both ends of the AirCore, the air in the
AirCore is flushed into the analyzer by the fill-gas. The flow rate is
controlled at the outlet of Picarro instrument and set to 38.2 mL min<inline-formula><mml:math 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>.
Calibration air can be analysed before and after measurement of the AirCore
air. After the trace gas analysis, the top (i.e. stratospheric) part of the
air collected with the AirCore (less than 20 % of the total collected air)
is transferred into an SAS that is sent to
Utrecht University for CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> isotope analysis.</p>
      <p>The timing of the sub-sampling process is based on the flow rate of the air
through the analyzer and the pump. The timing of the sub-sampling procedure
has to be precisely established to ensure that the desired fraction of gas is
collected with the SAS. To establish the timing for the sub-sampling
procedure, we injected a spike of highly CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>-enriched gas into the inlet
of the Picarro analyzer and then connected the outlet of the pump to the
inlet of the Picarro analyzer. Thus a closed loop without the SAS was
established, and the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> spike was measured multiple times as it
circulated through the analyzer and the pump. This experiment allowed us to
determine the timing of air travelling from the inlet of the analyzer to the
inlet of the SAS. The flow rate was measured with a flow meter, and the
timing for the sub-sampling procedure was established. Also, the membrane
pump (Picarro Inc.) that is used for the sub-sampling was carefully tested
for leaks to avoid contamination of stratospheric air with ambient laboratory
air during the sub-sampling process. The outlet of the pump was connected to
the gas analyzer (Picarro Inc., model G2401-m) to form a closed loop, which
was filled with air with high mole fractions of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CO and CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>. The flow
rate was set to 35 mL min<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> and the air enclosed in this closed system
was circulated nine times while measuring the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CO, CH<inline-formula><mml:math 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 display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O mole
fractions. The CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mole fractions stayed between 940.4 and 941.0 ppm and
a small initial fluctuation quenched after nine cycles. The rate of change of
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mole fraction based on these measurements with a very high CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mole
fraction difference between the sample and ambient air was 0.1 ppm of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
per minute. The effect of such a small contamination on the isotopic
composition of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is therefore negligible (<inline-formula><mml:math display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.001 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> given the
maximum <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) of 5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>; see below). We note,
however, that CO gets contaminated in the sub-sampling process at a rate of
17 ppb min<inline-formula><mml:math 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 CO (from a starting value of 500 ppb), so CO
measurements would be compromised.</p>
      <p>The SAS used for the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> isotope measurements in Utrecht is made of 10 2 m long pieces of 1/4 inch diameter stainless steel tubing, which are
connected by 11 Swagelok valves (part number SS-3CXS4) to form the 20 m long
SAS. The tubes are bent to form identical rings to facilitate easy handling
and transport. In the following, we refer to the rings as “SAS segments”
and the valves as “three-way valves”. The three-way valves are open and
connect the segments when the stratospheric part of the AirCore air fills the
SAS and are kept closed when the sub-sampling process is finished. Each SAS
segment contains about 25 mL of the AirCore air. Segment 1 corresponds to the
highest altitude of the AirCore flight, and segment 10 contains air from the
lower-stratosphere.</p>
      <p>The idea of the SAS that is described here in
detail has already been successfully implemented to enable the radiocarbon
analysis of stratospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> at the Centre for Isotope Research in
Groningen, the Netherlands <xref ref-type="bibr" rid="bib1.bibx25" id="paren.12"/>.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <?xmltex \opttitle{Continuous flow system to measure the isotopic composition of CO${}_{2}$}?><title>Continuous flow system to measure the isotopic composition of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></title>
      <p>The analytical system to measure the isotopic composition (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C,
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O) of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in each SAS segment is based
on the principle presented in <xref ref-type="bibr" rid="bib1.bibx23" id="text.13"/>. The isotopic composition is
measured after gas chromatographic separation of the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from other air
constituents. The <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O content cannot be determined directly from the
measurement at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 45, because of the isobaric interferences of <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>C
and <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O. Therefore, the <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O content is obtained from isotope
measurements on CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> before (PreCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and after oxygen isotope exchange
(PostCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) with a large reservoir of oxygen. Instead of using cerium (IV)
oxide (CeO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) as exchange material <xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx23" id="paren.14"/>, we use in
our new system copper oxide (CuO) <xref ref-type="bibr" rid="bib1.bibx17" id="paren.15"/>. A single measurement
requires two independent injections of 1 mL of air: one for direct
measurement (PreCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and one for measurement after oxygen isotope exchange
(PostCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>), plus 0.7 mL for flushing the injection lines (all at 1 bar
pressure). To reduce the measurement uncertainty statistically we perform
multiple measurements on one air sample.</p>
      <p>In addition to the requirement of overpressure in the injection unit, another
disadvantage of the method presented in <xref ref-type="bibr" rid="bib1.bibx23" id="text.16"/> was the severe peak
broadening that was introduced by the strong flow resistance of the CeO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
powder in the oxygen exchange unit, which required re-focusing of the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
after equilibration. In the new system the powdered CeO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the oxygen
exchange unit was replaced with CuO wires. As a result the peak broadening
was dramatically reduced by a factor of 7.5 (from 450 to 60 s) and the
equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> could be analysed without re-focusing. In addition, we
developed a custom-made sample injection unit for samples provided by the
SAS, where both sample and reference gas are
injected via the SAS.</p>
      <p>The improved continuous flow isotope ratio mass spectrometry analytical system (CF-IRMS) analytical system consists of: a sample injection unit
to attach the SAS segments, a gas chromatographic column to separate the
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from a 1 mL air aliquot, an oxygen isotope exchange unit for CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
equilibration with CuO and open split interface and an IRMS for isotope
measurement (Fig. <xref ref-type="fig" rid="Ch1.F3"/>). Similar to the method described by
Mrozek et al. (2015), three 6-port, 2-position Valco valves (VICI, C6UWM)
direct the gas flows through the analytical system. The four main components
are described in the following subsections.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p>Schematic diagram of the CF-IRMS analytical system for complete
isotope analysis (including <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O) of stratospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. The
system is divided into four units: <bold>(a)</bold> sample injection,
<bold>(b)</bold> gas chromatographic column (GC) to separate CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from air and
N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O, <bold>(c)</bold> optional oxygen isotope exchange unit and
<bold>(d)</bold> isotope detection unit including open split interface and
isotope ratio mass spectrometer (IRMS). MFC is mass flow controller, V1–V3
are Valco valves, RefCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is Utrecht working reference CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, the crossed
circles are conventional valves and the blue T's are the three-way valves.
The SAS three-way valves are normally closed but here they are shown in the
sample admission position.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016-f03.png"/>

        </fig>

<sec id="Ch1.S2.SS3.SSS1">
  <title>Sample injection</title>
      <p>The 10 individual segments of the SAS are measured
separately (see Sect. <xref ref-type="sec" rid="Ch1.S2.SS4.SSS1"/>). After connecting a segment, the volume
between the mass flow controller (MFC) and the segment is evacuated with a low
vacuum (LV) pump and filled with reference air. All connections in the injection
sub-unit are made of 1/8 inch o.d. stainless steel tubing. When the valves
of a connected SAS segment are opened, as demonstrated in Fig. <xref ref-type="fig" rid="Ch1.F3"/>, the reference air flushes the stratospheric air sample from
the SAS into the analytical system. The flow rate of the MFC
is set to 1 mL min<inline-formula><mml:math 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> during sample gas injection. We use the reference
air itself as the carrier for the sample air.<?xmltex \hack{\newpage}?></p>
      <p>A single <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) measurement requires two independent
injections of the sample gas. The first injection is used for direct isotope
measurement of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (PreCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>), the second injection is for measuring the
isotopically equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>(PostCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>). We inject the gas (reference
air or sample air) into the GC column via a 1 mL sample loop in V1. The
sample loop is always filled to ambient pressure because it is open to the
outside air via the vent. We use extended flushing during sample loop loading
(the 1 mL sample loop is flushed with the sample gas at a flow rate of 1 mL min<inline-formula><mml:math 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 80 s) to avoid interference from outside air that may diffuse
through the vent tubing into the sample loop.</p>
      <p>It takes less than 1 h to measure an individual SAS segment, however, in the
present set-up reference air is measured for several hours between the
different segments (see Sect. <xref ref-type="sec" rid="Ch1.S2.SS4.SSS2"/>). Usually two SAS segments are
measured in one day. The CF-IRMS system operates fully automated and the only
manual step required is the connection of the segments.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS2">
  <?xmltex \opttitle{CO${}_{2}$ separation from air}?><title>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> separation from air</title>
      <p>This sub-unit consist of a gas chromatography (GC) capillary column (ParaPLOT
Q 25 m <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.53 mm, Varian). As a carrier we use helium at a flow rate
of 4 mL min<inline-formula><mml:math 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>, supplied to the GC through one of the ports in valve V1.
The GC is kept inside a heated stainless steel box at 40 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C to
ensure uniform conditions for gas separation. On the GC column the different
air constituents are separated. The air peak (mainly O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) elutes
at 120 s after sample injection, CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> at 160 s and N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O at 190 s. The air
peak leaves the analytical system through the vent in valve V3. Both CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
and N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O are directed either to IRMS or to the isotope exchange sub-unit.
Nitrous oxide in our system does not interfere with CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during the isotope
ratio measurement because it is fully separated from CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and gets
destroyed in the CuO oven. This is discussed in detail in Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/>.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS3">
  <title>Oxygen isotope exchange with CuO</title>
      <p>This sub-unit consists of Valco valve 2 (V2) and an optional oxygen
equilibration oven, the same as <xref ref-type="bibr" rid="bib1.bibx23" id="normal.17"/>. The Valco valve V2 directs
the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> aliquot either directly to the IRMS or first into the
equilibration oven before entering IRMS. The oven is an assembly of a quartz
glass reaction tube (1.4 mm i.d., 3.0 mm o.d., 300 mm length), a tube
furnace and a temperature controller. Inside the tube there are oxygenated
Cu wires and a Ni catalyst. We refer to this assembly as CuO oven. At a
temperature of 900 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, the wires act as a fast and highly
efficient oxygen equilibration medium. This is similar to
<xref ref-type="bibr" rid="bib1.bibx17" id="text.18"/>, who for the same purpose used twisted wires of CuO and
Pt catalyst, and different from <xref ref-type="bibr" rid="bib1.bibx2" id="normal.19"/> and <xref ref-type="bibr" rid="bib1.bibx23" id="text.20"/>, who
used CeO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> powder. The important advantage of oxygenated Cu <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Ni wires over
CeO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> powder in our system is the much smaller flow resistance. Therefore,
the new exchange unit induces a much smaller peak broadening, and the
equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> does not require focusing anymore. As a result, the
single analysis time shortened by 250 s in comparison to the method described
in <xref ref-type="bibr" rid="bib1.bibx23" id="normal.21"/> (650 s instead of 900 s) and no liquid nitrogen is
required.</p>
      <p>Before first use, and then on a weekly basis, the CuO oven is conditioned
with O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (Ultra High Purity (UHP), Air Products) at a flow rate of 20 mL min<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> and a temperature of 600 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, following the procedure of
<xref ref-type="bibr" rid="bib1.bibx17" id="normal.22"/>. Under these conditions, the copper metal forms a coating
of copper (II) oxide on the surface of the Cu wires according to
              <disp-formula id="R1" content-type="numbered reaction"><mml:math display="block"><mml:mrow><mml:mtext>Cu</mml:mtext><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:msub><mml:mtext>O</mml:mtext><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>→</mml:mo><mml:mtext>CuO</mml:mtext><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p>After oxygenation, the IRMS needs at least 50 measurements for the signal to
stabilize. During routine measurements we monitor the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>)
RefAir vs. VSMOW signal before and after equilibration to make sure that the
equilibration reaction is quantitative.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS4">
  <title>IRMS interface and mass spectrometric analysis</title>
      <p>This sub-unit of the analytical system (Fig. <xref ref-type="fig" rid="Ch1.F3"/>d) consists of a Valco valve 3 (V3), a
Nafion<sup>™</sup> dryer, a custom-made open split system
<xref ref-type="bibr" rid="bib1.bibx26" id="paren.23"/> and an IRMS (Thermo Fisher Scientific Delta V Advantage).
The loop in valve V3 is used to insert an additional volume of
approximatively 1 mL volume (1/4 inch o.d. tube connected with Swagelok
fittings) into the flow path, which smooths and ensures a compact shape of
the PostCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> peak in the IRMS. The Nafion dryer removes traces of water
before the gas stream enters the IRMS via the open split system, which is
also used to inject the pure CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> working gas. The IRMS measures ion
current ratios <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>45</mml:mn><mml:mo>/</mml:mo><mml:mn>44</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>46</mml:mn><mml:mo>/</mml:mo><mml:mn>44</mml:mn></mml:mrow></mml:math></inline-formula> that originate from CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> isotopologues with
masses 44, 45 and 46.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS5">
  <?xmltex \opttitle{Reference air and reference CO${}_{2}$}?><title>Reference air and reference CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></title>
      <p>Our reference air cylinder (referred to as RefAir in the
following) was filled with tropospheric air collected at an altitude of 20 m from the sixth floor of the Buys Ballot building on the Utrecht University
campus in July 2014. The isotopic composition of the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the reference
air cylinder was calibrated against air cylinders provided by an
intercomparison program of the World Meteorological Organization (WMO) and
assigned the following isotope values: <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mtext>RefAir/VPDB</mml:mtext></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>8.09 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mtext>RefAir/VSMOW</mml:mtext></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 41.05 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.20 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>.
Following a mass dependent fractionation relation of tropospheric
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx14" id="paren.24"/>, we assign <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mtext>RefAir/VSMOW</mml:mtext></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 21.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>,
so that <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mtext>RefAir</mml:mtext></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.0 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>. The isotopic
composition of the reference air is measured continuously in between the
samples to monitor the stability and to correct for long-term trends of the
CF-IRMS system.</p>
      <p>The <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula> values for the working reference CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> that is injected via the
open split system are <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mtext>RefCO2/VPDB</mml:mtext></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>36.16 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.01 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>
and <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mtext>RefCO2/VSMOW</mml:mtext></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 4.69 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.01 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>.</p>
</sec>
</sec>
<sec id="Ch1.S2.SS4">
  <title>Measurement procedure</title>
<sec id="Ch1.S2.SS4.SSS1">
  <title>Connecting the sub-sampler to the continuous flow isotope analysis  system</title>
      <p>We start the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> isotope analysis always from the SAS segment with the
highest segment number, here segment number 10. The common port of valve no.
11 (the end of segment 10) is connected to the injection line, which leads to
V1, and the free port of valve no. 10 (the beginning of segment 10) to the
MFC delivering reference air (see Fig. <xref ref-type="fig" rid="Ch1.F3"/>). Note that the
beginning of the segment 10 is also the end of segment 9.</p>
      <p>The injection lines are open to the laboratory air when the SAS segments are
being exchanged. To avoid mixing of the precious sample air with laboratory
air we evacuate the volume between the MFC and the SAS segment with the LV pump and flush this volume with reference air (LV pump exchanged
to vent). It is important to depressurize the volume behind the MFC before
opening the SAS segment. Overpressure in the injection lines must be avoided
so that the small air sample is not pushed out of the inlet system.</p>
      <p>After connecting an SAS segment as described above, the three-way valve no. 10
is opened, so that reference air starts slowly flowing through segment 10.
Next, the three-way valve no. 11 is opened, so that air is flushed to the
sample loop of the injection system (see Fig. <xref ref-type="fig" rid="Ch1.F3"/>). The sample
admission procedure is described in detail in the next section.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p>Example of a typical IRMS chromatogram of a single
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) analysis with the CF-IRMS system described here. The
eight square peaks are the working reference CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (RefCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) peaks
injected directly via the open split interface. The non-equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
(PreCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) peak and the equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (PostCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) peak are the two
sample gas peaks.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016-f04.png"/>

          </fig>

      <p>As the sample air is flushed into the system by the reference air, we simply
continue measuring the reference air that is then flowing through the SAS
segment. A disadvantage is that the last injections of the sample air are
actually a mixture of sample and reference air (see below). The measurements
of reference air after the sample measurement are later used for referencing.
After the reference air measurements are completed, we close the three-way
valves and disconnect segment 10. As the common port of valve no. 10 has to
be connected to the injection line when measuring segment 9, segment 10 has
to be physically disconnected from the SAS. Segment 9 is then treated the
same as segment 10 before. We continue measuring and exchanging SAS segments
one by one.</p>
</sec>
<sec id="Ch1.S2.SS4.SSS2">
  <title>Isotope analysis procedure</title>
      <p>Each Valco valve has two possible positions: LOAD and INJECT. The initial
Valco valve configuration is shown in Fig. <xref ref-type="fig" rid="Ch1.F3"/>: V1 and V3 are in
position LOAD and V2 is in position INJECT. After an SAS segment has been
connected and the connecting lines flushed as described above, sample
admission starts. The MFC is set to a flow rate of 1 mL min<inline-formula><mml:math 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> 15 s
before opening the SAS valve in order to provide a small and reproducible
overpressure at the entrance of the SAS segment. We then open the three-way
valve towards the SAS segment to admit the reference air from the MFC, and 1 s later the three-way valve before V1. Now, the flow of reference air pushes
the AirCore air towards the sample loop in V1. It takes 10 s for the AirCore
air to travel from the SAS segment to the sample loop and another 80 s to
fill it. At 80 s, the flow rate at the MFC is stopped to save sample and the
air is allowed to further expand into and fill the injection loop. At 90 s
the loop is fully filled and Valco valve V1 is switched for 40 s to position
INJECT to transfer the first aliquot of the sample air into the analytical
system. The 1 mL aliquot of air from the SAS segment is transferred to the GC
column in a He carrier gas (4 mL min<inline-formula><mml:math 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>). In the GC column, the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is
separated from other atmospheric gases. All compounds are directed via Valco
valve V2 (INJECT) and Valco valve V3 (LOAD) directly towards the isotope
detection unit. The CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is injected into the ion source of the IRMS
(PreCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>), all other gases are discarded via the open split.</p>
      <p>As soon as the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> peak (PreCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) appears on the chromatogram, the
second aliquot of the AirCore air is introduced into the system. Similar to
the first injection, the sample loop is flushed with the AirCore air for 80 s
(MFC is set to a flow rate of 1 mL min<inline-formula><mml:math 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> between 290 and 370 s). At 380
s valve V1 is switched for 40 s from LOAD to INJECT, and the second aliquot
of the AirCore air is injected into the GC column. Non-CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> gases leave the
analytical system through the open split capillary between 500 and 520 s (V2
in position INJECT and V3 in position LOAD). At 545 s, V2 switches to
position LOAD, and the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is directed to the isotope exchange unit. After
the isotope exchange reaction, the equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (PostCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) is
flushed further to V3. An additional 1 mL stainless steel volume in front of
Valco valve V3 has been added to smoothen the peak shape of the equilibrated
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (PostCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>), leading to improved precision. The equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
is detected on the chromatogram between 560 and 640 s.</p>
      <p>Figure <xref ref-type="fig" rid="Ch1.F4"/> presents an example of an IRMS chromatogram. A
single measurement including two injections takes 650 s. The CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> peak from
the first injection (PreCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) is detected between 250 and 280 s, and the
equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> peak from the second injection (PostCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) between 560
and 640 s. The eight working reference CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> peaks (RefCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) are injected
to the IRMS directly via the open split interface: four before detection of
the PreCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (0–200 s) and four before detection of the PreCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (300–500 s). The two sample peaks (PreCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and PostCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) have a different shape
because the second one has passed the exchange unit and the additional
volume.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p>Raw-<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>45</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> data (<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> vs RefCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) from a
complete measurement sequence of an SASsegment. SA is the air sample stored
in the SAS segment. RefAir before SA refers to the reference air
passing through an empty SAS segment and defines IRMS stability before the
new SA is connected. After exchanging the SAS segments we obtain five “pure”
sample air measurements. Subsequent to the SA measurement, the reference air
first mixes into the sample air; it takes about 10 measurements until pure
reference air is processed. RefAir after SA refers to the reference
air passing through the SAS segment after the SA has been completely flushed
out. For the sample air presented here the “before equilibration' points
overlap with the “after equilibration” points and cannot be distinguished.</p></caption>
            <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016-f05.png"/>

          </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>Statistical improvement of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O analytical
error by combining multiple (<inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>) measurements of the same gas into
packages and taking the standard error of these packages.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="6">
     <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="center"/>
     <oasis:colspec colnum="5" colname="col5" align="center"/>
     <oasis:colspec colnum="6" colname="col6" align="center"/>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Test group</oasis:entry>  
         <oasis:entry colname="col2">Number of packages</oasis:entry>  
         <oasis:entry colname="col3">Number of measurements</oasis:entry>  
         <oasis:entry colname="col4">Random error</oasis:entry>  
         <oasis:entry colname="col5">SE theoretical:</oasis:entry>  
         <oasis:entry colname="col6">SE experimental:</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">name</oasis:entry>  
         <oasis:entry colname="col2">in the group</oasis:entry>  
         <oasis:entry colname="col3">in the package: (<inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col4">factor: 1/<inline-formula><mml:math display="inline"><mml:msqrt><mml:mrow><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msqrt></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5">SD/<inline-formula><mml:math display="inline"><mml:msqrt><mml:mrow><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msqrt></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col6">SD over <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O mean/<inline-formula><mml:math display="inline"><mml:msqrt><mml:mrow><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msqrt></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">A</oasis:entry>  
         <oasis:entry colname="col2">1</oasis:entry>  
         <oasis:entry colname="col3">270</oasis:entry>  
         <oasis:entry colname="col4">0.061</oasis:entry>  
         <oasis:entry colname="col5">0.074</oasis:entry>  
         <oasis:entry colname="col6"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">B</oasis:entry>  
         <oasis:entry colname="col2">2</oasis:entry>  
         <oasis:entry colname="col3">135</oasis:entry>  
         <oasis:entry colname="col4">0.086</oasis:entry>  
         <oasis:entry colname="col5">0.105</oasis:entry>  
         <oasis:entry colname="col6">0.205</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">C</oasis:entry>  
         <oasis:entry colname="col2">3</oasis:entry>  
         <oasis:entry colname="col3">90</oasis:entry>  
         <oasis:entry colname="col4">0.105</oasis:entry>  
         <oasis:entry colname="col5">0.129</oasis:entry>  
         <oasis:entry colname="col6">0.256</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">D</oasis:entry>  
         <oasis:entry colname="col2">5</oasis:entry>  
         <oasis:entry colname="col3">54</oasis:entry>  
         <oasis:entry colname="col4">0.136</oasis:entry>  
         <oasis:entry colname="col5">0.166</oasis:entry>  
         <oasis:entry colname="col6">0.170</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">E</oasis:entry>  
         <oasis:entry colname="col2">6</oasis:entry>  
         <oasis:entry colname="col3">45</oasis:entry>  
         <oasis:entry colname="col4">0.149</oasis:entry>  
         <oasis:entry colname="col5">0.182</oasis:entry>  
         <oasis:entry colname="col6">0.245</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">F</oasis:entry>  
         <oasis:entry colname="col2">9</oasis:entry>  
         <oasis:entry colname="col3">30</oasis:entry>  
         <oasis:entry colname="col4">0.183</oasis:entry>  
         <oasis:entry colname="col5">0.223</oasis:entry>  
         <oasis:entry colname="col6">0.251</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">G</oasis:entry>  
         <oasis:entry colname="col2">10</oasis:entry>  
         <oasis:entry colname="col3">27</oasis:entry>  
         <oasis:entry colname="col4">0.192</oasis:entry>  
         <oasis:entry colname="col5">0.235</oasis:entry>  
         <oasis:entry colname="col6">0.302</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">H</oasis:entry>  
         <oasis:entry colname="col2">15</oasis:entry>  
         <oasis:entry colname="col3">18</oasis:entry>  
         <oasis:entry colname="col4">0.236</oasis:entry>  
         <oasis:entry colname="col5">0.288</oasis:entry>  
         <oasis:entry colname="col6">0.316</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">I</oasis:entry>  
         <oasis:entry colname="col2">18</oasis:entry>  
         <oasis:entry colname="col3">15</oasis:entry>  
         <oasis:entry colname="col4">0.258</oasis:entry>  
         <oasis:entry colname="col5">0.315</oasis:entry>  
         <oasis:entry colname="col6">0.345</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">J</oasis:entry>  
         <oasis:entry colname="col2">27</oasis:entry>  
         <oasis:entry colname="col3">10</oasis:entry>  
         <oasis:entry colname="col4">0.316</oasis:entry>  
         <oasis:entry colname="col5">0.386</oasis:entry>  
         <oasis:entry colname="col6">0.405</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">K</oasis:entry>  
         <oasis:entry colname="col2">30</oasis:entry>  
         <oasis:entry colname="col3">9</oasis:entry>  
         <oasis:entry colname="col4">0.333</oasis:entry>  
         <oasis:entry colname="col5">0.407</oasis:entry>  
         <oasis:entry colname="col6">0.472</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">L</oasis:entry>  
         <oasis:entry colname="col2">45</oasis:entry>  
         <oasis:entry colname="col3">6</oasis:entry>  
         <oasis:entry colname="col4">0.408</oasis:entry>  
         <oasis:entry colname="col5">0.498</oasis:entry>  
         <oasis:entry colname="col6">0.531</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">M</oasis:entry>  
         <oasis:entry colname="col2">54</oasis:entry>  
         <oasis:entry colname="col3">5</oasis:entry>  
         <oasis:entry colname="col4">0.447</oasis:entry>  
         <oasis:entry colname="col5">0.546</oasis:entry>  
         <oasis:entry colname="col6"><bold>0.570</bold></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">N</oasis:entry>  
         <oasis:entry colname="col2">270</oasis:entry>  
         <oasis:entry colname="col3">1</oasis:entry>  
         <oasis:entry colname="col4">1.000</oasis:entry>  
         <oasis:entry colname="col5">1.220</oasis:entry>  
         <oasis:entry colname="col6"><bold>1.220</bold></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p>The bold values describe the uncertainty  for a single measurement
and the error expected for the five repeated measurements on one air sample stored in the SAS.<?xmltex \hack{\\}?>SD: standard deviation.</p></table-wrap-foot></table-wrap>

      <p>For each SAS segment we run a sequence of 35 individual measurements (of two
injections each). The results show that 5 of these measurements represent
pure sample gas (SA), 10 of them contain sample-reference air mixtures, and
20 are pure reference air (RefAir) measurements (see Fig. <xref ref-type="fig" rid="Ch1.F5"/>).
Theoretically, we should be able to analyse nine SA aliquots from each SAS
segment (25/2.7 mL), but as described above the reference air is used as
carrier gas and mixes with the sample air. Since we know the isotopic
composition of the reference air, the method can potentially be improved by
extracting SA information also from the “mixed” SA/RefAir peaks, which may
decrease measurement uncertainty statistically (see Table <xref ref-type="table" rid="Ch1.T1"/>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p>IRMS chromatogram demonstrating the separation of N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O from CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
on the GC column and the absence of an N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O peak after the hot CuO <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Ni
isotope exchange unit. The artificially prepared mixture of N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O and CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
was injected to the analytical system following the procedure described in
Sect. <xref ref-type="sec" rid="Ch1.S2.SS4.SSS2"/>. In order to observe the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O peak the fifth working
RefCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> peak was omitted in the chromatogram and the measurement time was
extended to 750 s.</p></caption>
            <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016-f06.png"/>

          </fig>

</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Performance of the continuous flow isotope analysis system</title>
<sec id="Ch1.S3.SS1">
  <?xmltex \opttitle{Separation and destruction of N${}_{2}$O}?><title>Separation and destruction of N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O</title>
      <p>Nitrous oxide (N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O) interferes with the mass spectrometric analysis of
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> because the isotopologues of both CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O fall on the mass
44, 45 and 46 collectors and cannot be separated with conventional IRMS
instruments <xref ref-type="bibr" rid="bib1.bibx22" id="paren.25"/>. These mass interferences can lead to significant
analytical biases for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>), <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) values and, as result, decrease <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of
stratospheric air by as much as  3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx28" id="paren.26"/>. Note that
N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O and CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> can also not be separated cryogenically <xref ref-type="bibr" rid="bib1.bibx21" id="paren.27"/>.</p>
      <p>To measure CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> isotopes in an air sample without interference from N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O
we completely separate N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O from CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> before the isotope ratio analysis
on the GC column <xref ref-type="bibr" rid="bib1.bibx11" id="paren.28"/>. In addition, for the measurement of
PostCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O is quantitatively destroyed in the hot isotope exchange
unit <xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx4 bib1.bibx23" id="paren.29"/>.</p>
      <p>To demonstrate successful GC separation and N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O decomposition inside the
CuO oven at 900 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C we connected a dilution of 400 ppm N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O
in synthetic air to the injection sub-unit of our analytical system. The
N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O enriched gas was placed at the position of a flask, as shown in Fig. <xref ref-type="fig" rid="Ch1.F3"/>. The flask was opened and the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O enriched gas filled the
injection lines and the 4 mL inner volume of MFC. Next, we changed the
position of the three-way valve in front of the MFC so that the reference air
was flowing towards the MFC. As a consequence, the reference air mixed with
the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O-rich gas and both N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O and CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were observed on the
chromatogram. We monitored the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O peak before and after the isotope
exchange reaction: for the non-heated aliquot, the GC column separated
completely the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O from the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>; for the heated aliquot, the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O was
destroyed completely in the CuO oven (see Fig. <xref ref-type="fig" rid="Ch1.F6"/>). For the experiment
shown in Fig. <xref ref-type="fig" rid="Ch1.F6"/>, the chromatogram was extended to 750 s instead of
the normal length of 650 s because N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O elutes after CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. Additionally,
the fifth working RefCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> peak was omitted in order to observe the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O
peak. The test shows that N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O can be effectively removed on CuO <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Ni wires
at 900 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and confirms the results of <xref ref-type="bibr" rid="bib1.bibx17" id="normal.30"/>.
This removal method can potentially be applied to other trace gas measurement
techniques.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><caption><p>Efficiency of oxygen isotope equilibration in the CuO oven. The
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) values of RefAir and a mixture of RefCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in
synthetic air are shown before and after isotope equilibration. The last
point of the RefAir measurement sequence after exchange is missing because
the peak of the last run was accidentally not registered.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016-f07.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <?xmltex \opttitle{CuO--CO${}_{2}$ equilibration efficiency}?><title>CuO–CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> equilibration efficiency</title>
      <p>To quantify the efficiency of oxygen isotope equilibration in the CuO oven we
analysed two samples containing CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with very different isotopic
composition. The first one was our RefAir and the second one was a synthetic
mixture of RefCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> diluted to 400 ppm CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in synthetic air. The samples
were injected via a stainless tube that is similar to a segment of the SAS,
but longer (4 m length 1/4 inch o.d.). First, the reference air was injected
multiple times through this tube. Next, we filled the injection tube with the
RefCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> dilution and continued the measurements. Figure <xref ref-type="fig" rid="Ch1.F7"/>
presents the results. The isotopic difference between the two CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> samples
was about 36 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> before isotope exchange. After the isotopic exchange
reaction both gases were equilibrated to <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> (19.03 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.18) <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>. From the difference in the oxygen isotopic composition between
RefAir and RefCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> dilution before and after oxygen isotope exchange, the
oxygen exchange efficiency in CuO oven was calculated to be <inline-formula><mml:math display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 99.5 %. We
conclude that the oxygen exchange reaction with CuO/Ni wires at 900 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C is complete.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <title>Error analysis</title>
      <p>In order to investigate the long-term stability of our CF-IRMS system and the
measurement uncertainty, 540 aliquots of reference air were injected
continuously to the CF-IRMS system for 50 h, comprising 270 individual
measurements of the complete isotopic composition of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. The standard
deviation of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) over all 270 measurements was 1.22 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>. This is the error that we assign to a single measurement with the
new analytical system. In our previously published method <xref ref-type="bibr" rid="bib1.bibx23" id="paren.31"/>,
the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) standard deviation in such a long-term stability
test was 1.68 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>. The improvement compared to the system described in
<xref ref-type="bibr" rid="bib1.bibx23" id="normal.32"/> is  due to the replacement of the isotope
exchange medium from powdered CeO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to CuO wires and through
abandonment of a liquid nitrogen trap for re-focusing of the isotopically
equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. For <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>)
the standard deviation over all 270 measurements was 0.06 and 0.07 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>, respectively, vs. 0.16 and 0.09 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> in
<xref ref-type="bibr" rid="bib1.bibx23" id="normal.33"/>.</p>
      <p>To investigate how the measurement error is reduced statistically with
multiple measurements on an air sample, we divided the 270 measurements from
the stability test into different packages of <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> numbers of
measurements (two packages of 135 measurements each, three packages of
90 measurements each, etc.). The experimental standard error (SE) for each
set of packages was then compared to the theoretically expected error.
Calculations for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) are shown in Table <xref ref-type="table" rid="Ch1.T1"/>;
the results for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>), <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) are displayed in Fig. <xref ref-type="fig" rid="Ch1.F8"/>. Since the SE is
defined as <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>/</mml:mo><mml:msup><mml:mi>n</mml:mi><mml:mn>0.5</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> the expected slope on this double
logarithmic plot is <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.50. The error reduction follows the theoretically
expected relation quite well. When the two groups with only two and three members
each are neglected, the linear fit to the data has a slope of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.46 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.02 for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.42 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.03
for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.45 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.03 for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C. Within the error, this is close to the theoretical
slope of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.50.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><caption><p>Correlation of ln(SE) vs. ln(<inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>) for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>)
(based on data from Table <xref ref-type="table" rid="Ch1.T1"/>), <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>). SE is the standard error of the mean, and <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> is
the number of measurements in a package. The experimental SE of
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C are shown as circles,
triangles and black diamonds respectively. The dashed/dotted lines are the
theoretically expected slopes for the linear correlation between ln(SE) and
ln(<inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>). For a packages of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>≤</mml:mo></mml:mrow></mml:math></inline-formula> 54, the experimentally derived
slopes are <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.46 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.02 for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.42 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.03 for
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.45 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.03 for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C. The values are close
to the theoretical slope of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.50 (dotted/dashed lines). Based on this
experiment we expect an uncertainty of <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>0.57 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> for
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of an AirCore air sample stored in an individual SAS segment.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016-f08.png"/>

        </fig>

      <p>We conclude that repeated measurements on one air sample (up to 54 repetition
that corresponds to 2.6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>mol CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) can reduce the uncertainty in
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) to 0.2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>. More than 54 repetitions on one air
sample improves the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) uncertainty only marginally. This
uncertainty is in the same range as previously reported techniques for large
samples, most of which did not allow the measurement of very small samples.
<xref ref-type="bibr" rid="bib1.bibx6" id="normal.34"/> reported an uncertainty of 0.1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> using
a BrF<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>-based technique, <xref ref-type="bibr" rid="bib1.bibx8" id="normal.35"/> obtained 0.2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>
with a two-step fluorination method, <xref ref-type="bibr" rid="bib1.bibx2" id="normal.36"/> reported 0.33 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> with a CeO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> exchange method and <xref ref-type="bibr" rid="bib1.bibx20" id="normal.37"/> improved this
method to an uncertainty of 0.12 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>. The <xref ref-type="bibr" rid="bib1.bibx17" id="normal.38"/> method is
the only technique that also targeted very small sample sizes (like our
system) and they reported an uncertainty of 0.35 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>. For five repeated
measurements on one stratospheric air sample stored in the SAS (an example of
a CF-IRMS measurement sequence is given in Fig. <xref ref-type="fig" rid="Ch1.F5"/>) we therefore
expect an uncertainty of 0.57 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and 0.03
<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> for both <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>). This
will be compared to the reproducibility of the actual SAS measurements in
Sect. <xref ref-type="sec" rid="Ch1.S4.SS2"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p>Stratospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mole fraction profile for an AirCore descent
near Sodankylä, Finland (67<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N), in November 2014, as a function of
altitude (km) and pressure (mbar). The numbers and the various line styles
indicate the sub-sampler segments into which the respective part of the air
from the AirCore coil was transferred after the trace gas analysis. The
general trend of the profile agrees with the already published data
<xref ref-type="bibr" rid="bib1.bibx12" id="paren.39"/>. The distribution of the air sample in the SAS segments
is proportional to the pressure change during the AirCore descent: here 16 mbar per SAS segment.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016-f09.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4">
  <title>AirCore flight on 5 November 2014 </title>
      <p>The AirCore payload was launched about 100 km upwind from Sodankylä, using
a meteorological balloon (67.35<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 26.93<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E). The AirCore
was released from the balloon at 34.5 km altitude (at 4.2 hPa) and the coil
filled with air during the balloon descent. Time of launch was 10:04 UTC,
while the payload landed at 12:40 UTC; thus the total flight duration was 2 h and 36 min. During the balloon ascent the payload travelled
south-east towards Sodankylä due to winds in the stratosphere and
troposphere. The payload landed with a parachute 53.8 km east from the
analysis laboratory (67.24<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 27.84<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E). After landing the
AirCore was transported to FMI. The analysis of trace gases started 2 h
and 15 min after the landing of the payload. In the laboratory the mole
fractions of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and CO were measured and the stratospheric air
was transferred into the SAS. The SAS was sent to the laboratory in Utrecht
for CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> isotope analysis.</p>
<sec id="Ch1.S4.SS1">
  <title>Assigning the trace gas data to the SAS segments</title>
      <p>We assigned the trace gas mixing ratios measured with the Picarro instrument
to the individual SAS segments based on the flow rate of the carrier gas and
the time required to fill the SAS. As the SAS has 10 segments, the air in
each segment represents 38.6 s of trace gas measurements with the Picarro
instrument. The second piece of information that is necessary for correct
assignment is the starting time for the sub-sampling. This starting time was
established by taking into account the transfer time of air from the outlet of
the Picarro analyser to the inlet of the SAS and the time required to flush
out the initial portion of fill-gas from the AirCore. To ensure that no
fill-gas was transferred into the SAS, the top fraction of the stratospheric
air (which immediately follows the fill-gas) also had to be discarded. This
way we lost the stratospheric air from above 25 km. The timing of
sub-sampling has in the meantime been improved to discard less stratospheric
air in future samplings.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p>Comparison of the linear negative correlation between
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O from measurements of the AirCore/SAS
samples (red rhombuses) presented here with literature data from
<xref ref-type="bibr" rid="bib1.bibx18" id="normal.40"/> (blue crosses) and <xref ref-type="bibr" rid="bib1.bibx28" id="normal.41"/> (black triangles).
For the AirCore dataset, N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O mole fractions were deduced from CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> mole
fractions as described in the text. The horizontal error bars are a
combination of the range of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> mole fractions that is combined within a
single SAS segment and the error of the CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>–N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O transfer function.
The vertical error bars represent <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) uncertainty of
0.56 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> (1<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/5607/2016/amt-9-5607-2016-f10.png"/>

        </fig>

      <p>Figure <xref ref-type="fig" rid="Ch1.F9"/> shows which part of the stratospheric AirCore air is stored
in which segment of the SAS, both as function of altitude and pressure. Note
that the SAS segments are equally spaced in pressure change (here 16 mbar/segment) during the descent rather than altitude. For example, the SAS
segment 1 contains air from 24.5 to 21.4 km, while the SAS segment 2 contains
air from 21.4 to 19.2 km. An analysis of the trace gas profiles from the
AirCore flight will be published separately.<?xmltex \hack{\newpage}?></p>
</sec>
<sec id="Ch1.S4.SS2">
  <?xmltex \opttitle{$\Delta^{{17}}$O(CO${}_{2}$) analysis of the AirCore air stored in the SAS}?><title><inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) analysis of the AirCore air stored in the SAS</title>
      <p>The stratospheric part of the AirCore air from 5 November 2014 flight was
measured in Utrecht between 25 November and 1 December 2014. The results
showed that segments 10 and 8 were contaminated with CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from outside air.
The precise origin of this contamination could not be determined, but it
could have happened when connecting SAS segments to the injection sub-unit of
the CF-IRMS system. Due to an accidental instability in the helium carrier
gas flow, the air sample from the SAS segment 6 was lost.</p>
      <p>As shown in Fig. <xref ref-type="fig" rid="Ch1.F5"/>, we were able to perform five repeated CF-IRMS
measurements on the other seven stratospheric air samples stored in SAS. The
average (1<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) standard deviation of the raw molecular mass ratios
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mn>45</mml:mn><mml:mo>/</mml:mo><mml:mn>44</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>46</mml:mn><mml:mo>/</mml:mo><mml:mn>44</mml:mn></mml:mrow></mml:math></inline-formula>) of an air sample was 0.04 and 0.02 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> for
non-equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and 0.07 and 0.11 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> for equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
respectively. The main contribution to the measurement error of
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O is the uncertainty in the isotope ratio <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>45</mml:mn><mml:mo>/</mml:mo><mml:mn>44</mml:mn></mml:mrow></mml:math></inline-formula>
<xref ref-type="bibr" rid="bib1.bibx8" id="paren.42"/>. Based on the reproducibility of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 45 of
equilibrated and non-equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ( <inline-formula><mml:math display="inline"><mml:mrow><mml:msqrt><mml:mrow><mml:mo>(</mml:mo><mml:mn>0.04</mml:mn><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:mn>0.07</mml:mn><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:msqrt><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> 15),
the uncertainty in <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O for a single measurement was 1.25 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>
and for a package of five measurements it was 0.56 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> (1.25 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">‰</mml:mi><mml:mo>/</mml:mo><mml:msqrt><mml:mn mathvariant="normal">5</mml:mn></mml:msqrt></mml:mrow></mml:math></inline-formula>). The error of 0.56 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> determined for the real
AirCore air measurements agrees very well with the uncertainty of 0.57 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>
expected from the long-term stability test (see Sect. <xref ref-type="sec" rid="Ch1.S3.SS3"/>). The standard deviations for all seven successfully
measured SAS segments were 0.08 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C and 0.05 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>
for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O. This results in the standard error of 0.03 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> for
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C and 0.02 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O for a
package of five repeated analyses from an SAS segment. This is again very similar
to the expected error from the long-term stability test as presented in Fig. <xref ref-type="fig" rid="Ch1.F8"/>.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <?xmltex \opttitle{$\Delta^{{17}}$O(CO${}_{2}$)--N${}_{2}$O correlation}?><title><inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>)–N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O correlation</title>
      <p>The mole fraction of N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O is a good tracer for the photochemical processing
of long-lived trace gases in the stratosphere <xref ref-type="bibr" rid="bib1.bibx24 bib1.bibx15" id="paren.43"/>.
Nitrous oxide was not measured in the AirCore air, but CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> was measured
and we use the relationship between stratospheric CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O mole
fractions at high latitudes to translate the CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> mole fractions to N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O
mole fractions. For this purpose we used CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>–N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O data from two
cryosampler flights in the Arctic in 2009 and 2011 <xref ref-type="bibr" rid="bib1.bibx10" id="paren.44"/>. The
fit function for the CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>–N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O dataset was provided to us by Andreas
Engel, Goethe University Frankfurt, Germany. The stratospheric pseudo-N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O
profile derived this way was then averaged according to the 10 individual
SAS segments. A detailed discussion on obtaining N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O mole fractions from
the measured CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> will be provided together with the scientific
interpretation of the data in Mrozek et al. (in prep.).</p>
      <p>In Fig. <xref ref-type="fig" rid="Ch1.F10"/> we show the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O mole fractions deduced from the CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>
profile vs. the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) data of the AirCore air samples
analysed from the SAS. The linear negative correlation between N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O and
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) is well known from previous studies and was discussed
before <xref ref-type="bibr" rid="bib1.bibx7 bib1.bibx18 bib1.bibx28" id="paren.45"/>. Here, we use this
correlation as an additional, independent check on the system calibration.
The AirCore air samples agree with the already published data, suggesting
that our measurements are well calibrated. The scatter of our data is similar
to the variability of the data presented by Kawagucci et al. (2008). The data
presented by Wiegel et al. (2013) show smaller variability, but our
measurements were obtained from samples of 25 mL of air at ambient pressure
only; this is up to 80 times smaller sample size than used in the
measurements of Wiegel et al. (2013). The variability of our data around the
linear fit is within the analytical uncertainty of 0.56 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula>
(1<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) per SAS segment. The uncertainty of the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O mole fraction in
Fig. <xref ref-type="fig" rid="Ch1.F10"/> reflects the standard deviation of the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O profile stored
in an individual SAS segment. It is up to 20 ppb (1<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) for the high-altitude AirCore air samples where N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O showed a strong trend and 2 ppb (1<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) for lower altitude samples where N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O is more constant. The
complete CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, CO and CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mole fraction dataset and in-depth analysis on
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> isotope measurements from the 5 November 2014 AirCore flight over
Sodankylä, Finland, will be published separately.</p>
      <p>We conclude that air sampling with an AirCore, followed by sub-sampling of
stratospheric air in 10 segments of the SAS and analysis with the analytical
system described here provides a relatively cost-effective technique for
obtaining vertical profiles of the complete isotopic composition of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in
the stratosphere.</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p>This article describes the concept of the SAS, a device constructed to recover and store the stratospheric part of
air obtained with an AirCore sampler. The SAS described here is an assembly
of 20 m, 1/4 inch o.d., stainless steel tubing divided into 10 segments.
Each SAS segment contains 25 mL of air sample at <inline-formula><mml:math display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 980 mbar. During
the procedure of sub-sampling air into the SAS, the air from an AirCore is
measured for CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and CO mole fractions with a Picarro analyzer.
This leads to some mixing of air and partial loss of the vertical
information, but once stored in the SAS the stratospheric profile of the
AirCore air after online analysis is preserved and the individual sub-samples
can be supplied to relatively slow analytical instrumentation. The SAS is
easy to construct and simple to use, also in the field.</p>
      <p>To illustrate the scientific possibilities, the SAS was coupled to a
continuous flow analytical system for measurement of the <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O excess of
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. The air from the SAS was supplied via a new sample introduction
system to allow isotope analysis on very small samples. The sample injection
occurs at ambient pressure and we use the reference air as the carrier gas.
The determination of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is performed by measuring
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> before and after complete oxygen isotope exchange with a large oxygen
reservoir provided by CuO <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Ni. The standard error for a 25 mL air sample at
stratospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mole fraction is 0.56 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> (1<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) for
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">‰</mml:mi></mml:math></inline-formula> (1<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) for both <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C. The analytical system operates free of liquid nitrogen  because
the isotopically equilibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> does not require a focusing step, unlike
the <xref ref-type="bibr" rid="bib1.bibx23" id="normal.46"/> method.</p>
      <p>The concept of SAS and its coupling to the analytical system for measurement
of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O was validated through measurements on stratospheric air
samples obtained during an AirCore flight over Sodankylä, Finland, in
November 2014. <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O shows the expected negative linear
correlation with N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O, which provides an independent check on the system
calibration. In the future, we plan routine measurements of stratospheric
profiles of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O together with the mole fractions of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>,
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and CO from AirCore flights on a regular basis, which could expedite
the use of the isotope signatures for studying stratospheric circulation
patterns and reaction mechanisms. The concept of the SAS will further broaden
the scientific questions that can be addressed by AirCore soundings (e.g.
<xref ref-type="bibr" rid="bib1.bibx25" id="altparen.47"/>).</p>
</sec>
<sec id="Ch1.S6">
  <title>Data availability</title>
      <p>The datasets are available from <uri>https://www.projects.science.uu.nl/atmosphereclimate/Data.php</uri> (APCG, 2016).</p>
</sec>

      
      </body>
    <back><ack><title>Acknowledgements</title><p>This work was funded by the Marie-Skłodowska Curie ITN INTRAMIF (Initial
Training Network in Mass Independent Fractionation) as a part of the European
Community's Seventh Framework Program (FP7/2007–2013), grant agreement
237890. Research at the FMI has been partly supported by the EU project
GAIA-CLIM and the Academy of Finland grant number 140408. We thank Andreas
Engel, Goethe University Frankfurt, Germany, for sharing with us the
stratospheric N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O–CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> correlation function. We also appreciate the efforts of the Associate Editor, Murray Hamilton, whose comments helped to shape this paper.
<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: M. Hamilton<?xmltex \hack{\newline}?>
Reviewed by: two anonymous referees</p></ack><ref-list>
    <title>References</title>

      <ref id="bib1.bibx1"><label>Alexander et al.(2001)Alexander, Vollmer, Jackson, Weiss, and
Thiemens</label><mixed-citation>Alexander, B., Vollmer, M. K., Jackson, T., Weiss, R. F., and Thiemens, M. H.:
Stratospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> isotopic anomalies and SF<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and CFC tracer
concentrations in the Arctic polar vortex, Geophys. Res. Lett., 28,
4103–4106, 2001.</mixed-citation></ref>
      <ref id="bib1.bib1"><label>1</label><mixed-citation>APCG: IMAU-APCG measurements data, available at:
<uri>https://www.projects.science.uu.nl/atmosphereclimate/Data.php</uri>,
last access: 17 November 2016.</mixed-citation></ref>
      <ref id="bib1.bibx2"><label>Assonov and Brenninkmeijer(2001)</label><mixed-citation>Assonov, S. S. and Brenninkmeijer, C. A. M.: A new method to determine the
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O isotopic abundance in CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> using oxygen isotope exchange with a
solid oxide, Rapid Commun. Mass Sp., 15, 2426–2437,
<ext-link xlink:href="http://dx.doi.org/10.1002/rcm.529" ext-link-type="DOI">10.1002/rcm.529</ext-link>, 2001.</mixed-citation></ref>
      <ref id="bib1.bibx3"><label>Assonov and Brenninkmeijer(2005)</label><mixed-citation>Assonov, S. S. and Brenninkmeijer, C. M.: Reporting small <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O
values: existing definitions and concepts, Rapid Commun. Mass Sp., 19, 627–636, <ext-link xlink:href="http://dx.doi.org/10.1002/rcm.1833" ext-link-type="DOI">10.1002/rcm.1833</ext-link>, 2005.</mixed-citation></ref>
      <ref id="bib1.bibx4"><label>Assonov and Brenninkmeijer(2006)</label><mixed-citation>Assonov, S. S. and Brenninkmeijer, C. A. M.: On the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O correction used for
mass spectrometric analysis of atmospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, Rapid Commun. Mass Sp., 20, 1809–1819, <ext-link xlink:href="http://dx.doi.org/10.1002/rcm.2516" ext-link-type="DOI">10.1002/rcm.2516</ext-link>, 2006.</mixed-citation></ref>
      <ref id="bib1.bibx5"><label>Baertschi(1976)</label><mixed-citation>Baertschi, P.: Absolute <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>18</mml:mn></mml:msup></mml:math></inline-formula>O content of standard mean ocean water, Earth
Planet. Sci. Lett., 31, 341–344, <ext-link xlink:href="http://dx.doi.org/10.1016/0012-821X(76)90115-1" ext-link-type="DOI">10.1016/0012-821X(76)90115-1</ext-link>, 1976.</mixed-citation></ref>
      <ref id="bib1.bibx6"><label>Bhattacharya and Thiemens(1989)</label><mixed-citation>
Bhattacharya, S. and Thiemens, M.: Oxygen Isotopic Fractionations in Symmetry
Dependent Chemical Reactions, in: Lunar and Planetary Science Conference, 20, p. 71, 1989.</mixed-citation></ref>
      <ref id="bib1.bibx7"><label>Boering et al.(2004)Boering, Jackson, Hoag, Cole, Perri, Thiemens,
and Atlas</label><mixed-citation>Boering, K. A., Jackson, T., Hoag, K. J., Cole, A. S., Perri, M. J., Thiemens,
M., and Atlas, E.: Observations of the anomalous oxygen isotopic composition
of carbon dioxide in the lower stratosphere and the flux of the anomaly to
the troposphere, Geophys. Res. Lett., 31, L03109, <ext-link xlink:href="http://dx.doi.org/10.1029/2003GL018451" ext-link-type="DOI">10.1029/2003GL018451</ext-link>, 2004.</mixed-citation></ref>
      <ref id="bib1.bibx8"><label>Brenninkmeijer and Röckmann(1998)</label><mixed-citation>Brenninkmeijer, C. A. M. and Röckmann, T.: A rapid method for the
preparation of O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> for mass spectrometric measurement of
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>16</mml:mn></mml:msup></mml:math></inline-formula>O ratios, Rapid Commun. Mass Sp., 12,
479–483, 1998.</mixed-citation></ref>
      <ref id="bib1.bibx9"><label>Chen et al.(2016)Chen, Kivi, Heikkinen, de Vreis, Hatakka,
Laurila, Sweeney, and Tans</label><mixed-citation>Chen, H., Kivi, R., Heikkinen, P.and Kers, B., de Vreis, M., Hatakka, J.,
Laurila, T., Sweeney, C., and Tans, P.: High-latitude balloon observations of
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>/CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>/CO using AirCore: evaluation of Sodankylä TCCON retrievals,
in prep., 2016.</mixed-citation></ref>
      <ref id="bib1.bibx10"><label>Engel et al.(2016)Engel, Bönisch, Schwarzenberger, Haase, Grunow,
Abalichin, and Sala</label><mixed-citation>Engel, A., Bönisch, H., Schwarzenberger, T., Haase, H.-P., Grunow, K.,
Abalichin, J., and Sala, S.: Long-term validation of ESA operational
retrieval (version 6.0) of MIPAS Envisat vertical profiles of methane,
nitrous oxide, CFC11, and CFC12 using balloon-borne observations and
trajectory matching, Atmos. Meas. Tech., 9, 1051–1062,
<ext-link xlink:href="http://dx.doi.org/10.5194/amt-9-1051-2016" ext-link-type="DOI">10.5194/amt-9-1051-2016</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bibx11"><label>Ferretti et al.(2000)Ferretti, Lowe, Martin, and
Brailsford</label><mixed-citation>Ferretti, D. F., Lowe, D. C., Martin, R. J., and Brailsford, G. W.: A new gas
chromatograph-isotope ratio mass spectrometry technique for high-precision,
N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O-free analysis of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C and <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in atmospheric
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from small air samples, J. Geophys. Res.-Atmos,
105, 6709–6718, <ext-link xlink:href="http://dx.doi.org/10.1029/1999JD901051" ext-link-type="DOI">10.1029/1999JD901051</ext-link>, 2000.</mixed-citation></ref>
      <ref id="bib1.bibx12"><label>Foucher et al.(2011)Foucher, Chédin, Armante, Boone, Crevoisier,
and Bernath</label><mixed-citation>Foucher, P. Y., Chédin, A., Armante, R., Boone, C., Crevoisier, C., and
Bernath, P.: Carbon dioxide atmospheric vertical profiles retrieved from
space observation using ACE-FTS solar occultation instrument, Atmos. Chem.
Phys., 11, 2455–2470, <ext-link xlink:href="http://dx.doi.org/10.5194/acp-11-2455-2011" ext-link-type="DOI">10.5194/acp-11-2455-2011</ext-link>, 2011.</mixed-citation></ref>
      <ref id="bib1.bibx13"><label>IPCC(2013)Ciais, Sabine, Bala, Bopp, Brovkin, Canadell,
Chhabra, DeFries, Galloway, Heimann, Jones, Le Quéré, Myneni, Piao,
and Thornton</label><mixed-citation>IPCC 2013: Ciais, P., Sabine, C., Bala, G., Bopp, L., Brovkin, V., Canadell, J., Chhabra,
A., DeFries, R., Galloway, J., Heimann, M., Jones, C., Le Quéré, C.,
Myneni, R., Piao, S., and Thornton, P.: Climate Change 2013: The Physical
Science Basis. Contribution of Working Group I to the Fifth Assessment Report
of the Intergovernmental Panel on Climate Change, edited by: Stocker, T. F., Qin,
D., Plattner, G.-K., Tignor, M., Allen, S. K., Boschung, J., Nauels, A., Xia, Y., Bex, V.
and Midgley, P. M., Tech. rep., <ext-link xlink:href="http://dx.doi.org/10.1017/CBO9781107415324.015" ext-link-type="DOI">10.1017/CBO9781107415324.015</ext-link>,
2013.</mixed-citation></ref>
      <ref id="bib1.bibx14"><label>Kaiser(2009)</label><mixed-citation>Kaiser, J.: Reformulated <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O correction of mass spectrometric stable
isotope measurements in carbon dioxide and a critical appraisal of historic
“absolute” carbon and oxygen isotope ratios, Geochim. Cosmochim.
Ac., 72, 1312–1334, <ext-link xlink:href="http://dx.doi.org/10.1016/j.gca.2007.12.011" ext-link-type="DOI">10.1016/j.gca.2007.12.011</ext-link>, 2009.</mixed-citation></ref>
      <ref id="bib1.bibx15"><label>Kaiser et al.(2006)Kaiser, Engel, Borchers, and
Röckmann</label><mixed-citation>Kaiser, J., Engel, A., Borchers, R., and Röckmann, T.: Probing stratospheric
transport and chemistry with new balloon and aircraft observations of the
meridional and vertical N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O isotope distribution, Atmos. Chem. Phys., 6,
3535–3556, <ext-link xlink:href="http://dx.doi.org/10.5194/acp-6-3535-2006" ext-link-type="DOI">10.5194/acp-6-3535-2006</ext-link>, 2006.</mixed-citation></ref>
      <ref id="bib1.bibx16"><label>Karion et al.(2010)Karion, Sweeney, Tans, and Newberger</label><mixed-citation>Karion, A., Sweeney, C., Tans, P., and Newberger, T.: AirCore: An innovative
atmospheric sampling system, J. Atmos. Ocean. Techn.,
27, 1839–1853, <ext-link xlink:href="http://dx.doi.org/10.1175/2010JTECHA1448.1" ext-link-type="DOI">10.1175/2010JTECHA1448.1</ext-link>, 2010.</mixed-citation></ref>
      <ref id="bib1.bibx17"><label>Kawagucci et al.(2005)Kawagucci, Tsunogai, Kudo, Nakagawa, Honda,
Aoki, Nakazawa, and Gamo</label><mixed-citation>Kawagucci, S., Tsunogai, U., Kudo, S., Nakagawa, F., Honda, H., Aoki, S.,
Nakazawa, T., and Gamo, T.: An analytical system for determining <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn>17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> using continuous flow-isotope ratio MS, Anal.
Chem., 77, 4509–4514, <ext-link xlink:href="http://dx.doi.org/10.1021/ac050266u" ext-link-type="DOI">10.1021/ac050266u</ext-link>, 2005.</mixed-citation></ref>
      <ref id="bib1.bibx18"><label>Kawagucci et al.(2008)Kawagucci, Tsunogai, Kudo, Nakagawa, Honda,
Aoki, Nakazawa, Tsutsumi, and Gamo</label><mixed-citation>Kawagucci, S., Tsunogai, U., Kudo, S., Nakagawa, F., Honda, H., Aoki, S.,
Nakazawa, T., Tsutsumi, M., and Gamo, T.: Long-term observation of
mass-independent oxygen isotope anomaly in stratospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, Atmos. Chem.
Phys., 8, 6189–6197, <ext-link xlink:href="http://dx.doi.org/10.5194/acp-8-6189-2008" ext-link-type="DOI">10.5194/acp-8-6189-2008</ext-link>, 2008.</mixed-citation></ref><?xmltex \hack{\newpage}?>
      <ref id="bib1.bibx19"><label>Lämmerzahl et al.(2002)Lämmerzahl, Röckmann, Brenninkmeijer,
Krankowsky, and Mauersberger</label><mixed-citation>
Lämmerzahl, P., Röckmann, T., Brenninkmeijer, C. M., Krankowsky, D., and
Mauersberger, K.: Oxygen isotope composition of stratospheric carbon
dioxide, Geophys. Res. Lett., 29, 2–5, 2002.</mixed-citation></ref>
      <ref id="bib1.bibx20"><label>Mahata et al.(2012)Mahata, Bhattacharya, Wang, and Liang</label><mixed-citation>Mahata, S., Bhattacharya, S. K., Wang, C.-H., and Liang, M.-C.: An improved
CeO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> method for high-precision measurements of <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>16</mml:mn></mml:msup></mml:math></inline-formula>O ratios
for atmospheric carbon dioxide., Rapid Commun. Mass Sp.,
26, 1909–1922, <ext-link xlink:href="http://dx.doi.org/10.1002/rcm.6296" ext-link-type="DOI">10.1002/rcm.6296</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bibx21"><label>Mook and Jongsma(1987)</label><mixed-citation>Mook, W. G. and Jongsma, J.: Measurement of the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O correction for <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>C
/<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>C ratios of atmospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> by removal of N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O, Tellus B, 39B,
96–99, <ext-link xlink:href="http://dx.doi.org/10.1111/j.1600-0889.1987.tb00274.x" ext-link-type="DOI">10.1111/j.1600-0889.1987.tb00274.x</ext-link>, 1987.</mixed-citation></ref>
      <ref id="bib1.bibx22"><label>Mook and van der Hoek(1983)</label><mixed-citation>Mook, W. G. and van der Hoek, S.: The N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O correction in the carbon and
oxygen isotopic analysis of atmospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, Chem. Geol., 41, 237–242, <ext-link xlink:href="http://dx.doi.org/10.1016/S0009-2541(83)80021-7" ext-link-type="DOI">10.1016/S0009-2541(83)80021-7</ext-link>, 1983.</mixed-citation></ref>
      <ref id="bib1.bibx23"><label>Mrozek et al.(2015)Mrozek, van der Veen, Kliphuis, Kaiser, Wiegel,
and Röckmann</label><mixed-citation>Mrozek, D. J., van der Veen, C., Kliphuis, M., Kaiser, J., Wiegel, A. A., and
Röckmann, T.: Continuous-flow IRMS technique for determining the <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>17</mml:mn></mml:msup></mml:math></inline-formula>O excess
of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> using complete oxygen isotope exchange with cerium oxide, Atmos. Meas.
Tech., 8, 811–822, <ext-link xlink:href="http://dx.doi.org/10.5194/amt-8-811-2015" ext-link-type="DOI">10.5194/amt-8-811-2015</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bibx24"><label>Park et al.(2004)Park, Atlas, and Boering</label><mixed-citation>Park, S., Atlas, E. L., and Boering, K. A.: Measurements of N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O
isotopologues in the stratosphere: Influence of transport on the apparent
enrichment factors and the isotopologue fluxes to the troposphere, J.
Geophys. Res.-Atmos., 109, D01305, <ext-link xlink:href="http://dx.doi.org/10.1029/2003JD003731" ext-link-type="DOI">10.1029/2003JD003731</ext-link>, 2004.</mixed-citation></ref>
      <ref id="bib1.bibx25"><label>Paul et al.(2016)Paul, Chen, Been, Kivi, and Meijer</label><mixed-citation>Paul, D., Chen, H., Been, H. A., Kivi, R., and Meijer, H. A. J.: Radiocarbon
analysis of stratospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> retrieved from AirCore sampling, Atmos. Meas.
Tech., 9, 4997–5006, <ext-link xlink:href="http://dx.doi.org/10.5194/amt-9-4997-2016" ext-link-type="DOI">10.5194/amt-9-4997-2016</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bibx26"><label>Röckmann et al.(2003)Röckmann, Kaiser, Brenninkmeijer, and
Brand</label><mixed-citation>Röckmann, T., Kaiser, J., Brenninkmeijer, C. A. M., and Brand, W. A.: Gas
chromatography/isotope-ratio mass spectrometry method for high-precision
position-dependent <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>15</mml:mn></mml:msup></mml:math></inline-formula>N and <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>18</mml:mn></mml:msup></mml:math></inline-formula>O measurements of atmospheric nitrous
oxide., Rapid Commun. Mass Sp., 17, 1897–908,
<ext-link xlink:href="http://dx.doi.org/10.1002/rcm.1132" ext-link-type="DOI">10.1002/rcm.1132</ext-link>, 2003.</mixed-citation></ref>
      <ref id="bib1.bibx27"><label>Thiemens et al.(1995)Thiemens, Jackson, Zipf, Erdman, and
Egmond</label><mixed-citation>
Thiemens, M., Jackson, T., Zipf, E. C., Erdman, P. W., and Egmond, V. C.:
Carbon dioxide and oxygen isotope anomalies in the mesosphere and
stratosphere, Science, 270, 969–972, 1995.</mixed-citation></ref>
      <ref id="bib1.bibx28"><label>Wiegel et al.(2013)Wiegel, Cole, Hoag, Atlas, Schauffler, and
Boering</label><mixed-citation>Wiegel, A. A., Cole, A. S., Hoag, K. J., Atlas, E. L., Schauffler, S. M., and
Boering, K. A.: Unexpected variations in the triple oxygen isotope
composition of stratospheric carbon dioxide, P. Natl.
Acad. Sci., 110, 17680–17685, <ext-link xlink:href="http://dx.doi.org/10.1073/pnas.1213082110" ext-link-type="DOI">10.1073/pnas.1213082110</ext-link>,
2013.</mixed-citation></ref>

  </ref-list><app-group content-type="float"><app><title/>

    </app></app-group></back>
    <!--<article-title-html>Stratospheric Air Sub-sampler (SAS) and its application to analysis of  Δ<sup>17</sup>O(CO<sub>2</sub>) from small air samples collected with an AirCore</article-title-html>
<abstract-html><p class="p">We present the set-up and a scientific application of the Stratospheric Air
Sub-sampler (SAS), a device to collect and to store the vertical profile of
air collected with an AirCore [Karion et al.(2010)] in numerous sub-samples for
later analysis in the laboratory. The SAS described here is a 20 m long 1/4 inch stainless steel tubing that is separated by eleven valves to divide the
tubing into 10 identical segments, but it can be easily adapted to collect
smaller or larger samples. In the collection phase the SAS is directly
connected to the outlet of an optical analyzer that measures the mole
fractions of CO<sub>2</sub>, CH<sub>4</sub> and CO from an AirCore sampler. The stratospheric
part (or if desired any part of the AirCore air) is then directed through the
SAS. When the SAS is filled with the selected air, the valves are closed and
the vertical profile is maintained in the different segments of the SAS. The
segments can later be analysed to retrieve vertical profiles of other trace
gas signatures that require slower instrumentation. As an application, we
describe the coupling of the SAS to an analytical system to determine the
<sup>17</sup>O excess of CO<sub>2</sub>, which is a tracer for photochemical processing of
stratospheric air. For this purpose the analytical system described by
[Mrozek et al.(2015)] was adapted for analysis of air directly from the SAS. The
performance of the coupled system is demonstrated for a set of air samples
from an AirCore flight in November 2014 near Sodankylä, Finland. The
standard error for a 25 mL air sample at stratospheric CO<sub>2</sub> mole fraction
is 0.56 ‰ (1<i>σ</i>) for <i>δ</i><sup>17</sup>O and 0.03 ‰
(1<i>σ</i>) for both <i>δ</i><sup>18</sup>O and <i>δ</i><sup>13</sup>C. Measured
Δ<sup>17</sup>O(CO<sub>2</sub>) values show a clear correlation with N<sub>2</sub>O in
agreement with already published data.</p></abstract-html>
<ref-html id="bib1.bib1"><label>Alexander et al.(2001)Alexander, Vollmer, Jackson, Weiss, and
Thiemens</label><mixed-citation>
Alexander, B., Vollmer, M. K., Jackson, T., Weiss, R. F., and Thiemens, M. H.:
Stratospheric CO<sub>2</sub> isotopic anomalies and SF<sub>6</sub> and CFC tracer
concentrations in the Arctic polar vortex, Geophys. Res. Lett., 28,
4103–4106, 2001.
</mixed-citation></ref-html>
<ref-html id="bib1.bib2"><label>1</label><mixed-citation>
APCG: IMAU-APCG measurements data, available at:
<a href="https://www.projects.science.uu.nl/atmosphereclimate/Data.php" target="_blank">https://www.projects.science.uu.nl/atmosphereclimate/Data.php</a>,
last access: 17 November 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib3"><label>Assonov and Brenninkmeijer(2001)</label><mixed-citation>
Assonov, S. S. and Brenninkmeijer, C. A. M.: A new method to determine the
<sup>17</sup>O isotopic abundance in CO<sub>2</sub> using oxygen isotope exchange with a
solid oxide, Rapid Commun. Mass Sp., 15, 2426–2437,
<a href="http://dx.doi.org/10.1002/rcm.529" target="_blank">doi:10.1002/rcm.529</a>, 2001.
</mixed-citation></ref-html>
<ref-html id="bib1.bib4"><label>Assonov and Brenninkmeijer(2005)</label><mixed-citation>
Assonov, S. S. and Brenninkmeijer, C. M.: Reporting small Δ<sup>17</sup>O
values: existing definitions and concepts, Rapid Commun. Mass Sp., 19, 627–636, <a href="http://dx.doi.org/10.1002/rcm.1833" target="_blank">doi:10.1002/rcm.1833</a>, 2005.
</mixed-citation></ref-html>
<ref-html id="bib1.bib5"><label>Assonov and Brenninkmeijer(2006)</label><mixed-citation>
Assonov, S. S. and Brenninkmeijer, C. A. M.: On the N<sub>2</sub>O correction used for
mass spectrometric analysis of atmospheric CO<sub>2</sub>, Rapid Commun. Mass Sp., 20, 1809–1819, <a href="http://dx.doi.org/10.1002/rcm.2516" target="_blank">doi:10.1002/rcm.2516</a>, 2006.
</mixed-citation></ref-html>
<ref-html id="bib1.bib6"><label>Baertschi(1976)</label><mixed-citation>
Baertschi, P.: Absolute <sup>18</sup>O content of standard mean ocean water, Earth
Planet. Sci. Lett., 31, 341–344, <a href="http://dx.doi.org/10.1016/0012-821X(76)90115-1" target="_blank">doi:10.1016/0012-821X(76)90115-1</a>, 1976.
</mixed-citation></ref-html>
<ref-html id="bib1.bib7"><label>Bhattacharya and Thiemens(1989)</label><mixed-citation>
Bhattacharya, S. and Thiemens, M.: Oxygen Isotopic Fractionations in Symmetry
Dependent Chemical Reactions, in: Lunar and Planetary Science Conference, 20, p. 71, 1989.
</mixed-citation></ref-html>
<ref-html id="bib1.bib8"><label>Boering et al.(2004)Boering, Jackson, Hoag, Cole, Perri, Thiemens,
and Atlas</label><mixed-citation>
Boering, K. A., Jackson, T., Hoag, K. J., Cole, A. S., Perri, M. J., Thiemens,
M., and Atlas, E.: Observations of the anomalous oxygen isotopic composition
of carbon dioxide in the lower stratosphere and the flux of the anomaly to
the troposphere, Geophys. Res. Lett., 31, L03109, <a href="http://dx.doi.org/10.1029/2003GL018451" target="_blank">doi:10.1029/2003GL018451</a>, 2004.
</mixed-citation></ref-html>
<ref-html id="bib1.bib9"><label>Brenninkmeijer and Röckmann(1998)</label><mixed-citation>
Brenninkmeijer, C. A. M. and Röckmann, T.: A rapid method for the
preparation of O<sub>2</sub> from CO<sub>2</sub> for mass spectrometric measurement of
<sup>17</sup>O ∕ <sup>16</sup>O ratios, Rapid Commun. Mass Sp., 12,
479–483, 1998.
</mixed-citation></ref-html>
<ref-html id="bib1.bib10"><label>Chen et al.(2016)Chen, Kivi, Heikkinen, de Vreis, Hatakka,
Laurila, Sweeney, and Tans</label><mixed-citation>
Chen, H., Kivi, R., Heikkinen, P.and Kers, B., de Vreis, M., Hatakka, J.,
Laurila, T., Sweeney, C., and Tans, P.: High-latitude balloon observations of
CO<sub>2</sub>/CH<sub>4</sub>/CO using AirCore: evaluation of Sodankylä TCCON retrievals,
in prep., 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib11"><label>Engel et al.(2016)Engel, Bönisch, Schwarzenberger, Haase, Grunow,
Abalichin, and Sala</label><mixed-citation>
Engel, A., Bönisch, H., Schwarzenberger, T., Haase, H.-P., Grunow, K.,
Abalichin, J., and Sala, S.: Long-term validation of ESA operational
retrieval (version 6.0) of MIPAS Envisat vertical profiles of methane,
nitrous oxide, CFC11, and CFC12 using balloon-borne observations and
trajectory matching, Atmos. Meas. Tech., 9, 1051–1062,
<a href="http://dx.doi.org/10.5194/amt-9-1051-2016" target="_blank">doi:10.5194/amt-9-1051-2016</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib12"><label>Ferretti et al.(2000)Ferretti, Lowe, Martin, and
Brailsford</label><mixed-citation>
Ferretti, D. F., Lowe, D. C., Martin, R. J., and Brailsford, G. W.: A new gas
chromatograph-isotope ratio mass spectrometry technique for high-precision,
N<sub>2</sub>O-free analysis of <i>δ</i><sup>13</sup>C and <i>δ</i><sup>18</sup>O in atmospheric
CO<sub>2</sub> from small air samples, J. Geophys. Res.-Atmos,
105, 6709–6718, <a href="http://dx.doi.org/10.1029/1999JD901051" target="_blank">doi:10.1029/1999JD901051</a>, 2000.
</mixed-citation></ref-html>
<ref-html id="bib1.bib13"><label>Foucher et al.(2011)Foucher, Chédin, Armante, Boone, Crevoisier,
and Bernath</label><mixed-citation>
Foucher, P. Y., Chédin, A., Armante, R., Boone, C., Crevoisier, C., and
Bernath, P.: Carbon dioxide atmospheric vertical profiles retrieved from
space observation using ACE-FTS solar occultation instrument, Atmos. Chem.
Phys., 11, 2455–2470, <a href="http://dx.doi.org/10.5194/acp-11-2455-2011" target="_blank">doi:10.5194/acp-11-2455-2011</a>, 2011.
</mixed-citation></ref-html>
<ref-html id="bib1.bib14"><label>IPCC(2013)Ciais, Sabine, Bala, Bopp, Brovkin, Canadell,
Chhabra, DeFries, Galloway, Heimann, Jones, Le Quéré, Myneni, Piao,
and Thornton</label><mixed-citation>
IPCC 2013: Ciais, P., Sabine, C., Bala, G., Bopp, L., Brovkin, V., Canadell, J., Chhabra,
A., DeFries, R., Galloway, J., Heimann, M., Jones, C., Le Quéré, C.,
Myneni, R., Piao, S., and Thornton, P.: Climate Change 2013: The Physical
Science Basis. Contribution of Working Group I to the Fifth Assessment Report
of the Intergovernmental Panel on Climate Change, edited by: Stocker, T. F., Qin,
D., Plattner, G.-K., Tignor, M., Allen, S. K., Boschung, J., Nauels, A., Xia, Y., Bex, V.
and Midgley, P. M., Tech. rep., <a href="http://dx.doi.org/10.1017/CBO9781107415324.015" target="_blank">doi:10.1017/CBO9781107415324.015</a>,
2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib15"><label>Kaiser(2009)</label><mixed-citation>
Kaiser, J.: Reformulated <sup>17</sup>O correction of mass spectrometric stable
isotope measurements in carbon dioxide and a critical appraisal of historic
“absolute” carbon and oxygen isotope ratios, Geochim. Cosmochim.
Ac., 72, 1312–1334, <a href="http://dx.doi.org/10.1016/j.gca.2007.12.011" target="_blank">doi:10.1016/j.gca.2007.12.011</a>, 2009.
</mixed-citation></ref-html>
<ref-html id="bib1.bib16"><label>Kaiser et al.(2006)Kaiser, Engel, Borchers, and
Röckmann</label><mixed-citation>
Kaiser, J., Engel, A., Borchers, R., and Röckmann, T.: Probing stratospheric
transport and chemistry with new balloon and aircraft observations of the
meridional and vertical N<sub>2</sub>O isotope distribution, Atmos. Chem. Phys., 6,
3535–3556, <a href="http://dx.doi.org/10.5194/acp-6-3535-2006" target="_blank">doi:10.5194/acp-6-3535-2006</a>, 2006.
</mixed-citation></ref-html>
<ref-html id="bib1.bib17"><label>Karion et al.(2010)Karion, Sweeney, Tans, and Newberger</label><mixed-citation>
Karion, A., Sweeney, C., Tans, P., and Newberger, T.: AirCore: An innovative
atmospheric sampling system, J. Atmos. Ocean. Techn.,
27, 1839–1853, <a href="http://dx.doi.org/10.1175/2010JTECHA1448.1" target="_blank">doi:10.1175/2010JTECHA1448.1</a>, 2010.
</mixed-citation></ref-html>
<ref-html id="bib1.bib18"><label>Kawagucci et al.(2005)Kawagucci, Tsunogai, Kudo, Nakagawa, Honda,
Aoki, Nakazawa, and Gamo</label><mixed-citation>
Kawagucci, S., Tsunogai, U., Kudo, S., Nakagawa, F., Honda, H., Aoki, S.,
Nakazawa, T., and Gamo, T.: An analytical system for determining Δ<sup>17</sup>O in CO<sub>2</sub> using continuous flow-isotope ratio MS, Anal.
Chem., 77, 4509–4514, <a href="http://dx.doi.org/10.1021/ac050266u" target="_blank">doi:10.1021/ac050266u</a>, 2005.
</mixed-citation></ref-html>
<ref-html id="bib1.bib19"><label>Kawagucci et al.(2008)Kawagucci, Tsunogai, Kudo, Nakagawa, Honda,
Aoki, Nakazawa, Tsutsumi, and Gamo</label><mixed-citation>
Kawagucci, S., Tsunogai, U., Kudo, S., Nakagawa, F., Honda, H., Aoki, S.,
Nakazawa, T., Tsutsumi, M., and Gamo, T.: Long-term observation of
mass-independent oxygen isotope anomaly in stratospheric CO<sub>2</sub>, Atmos. Chem.
Phys., 8, 6189–6197, <a href="http://dx.doi.org/10.5194/acp-8-6189-2008" target="_blank">doi:10.5194/acp-8-6189-2008</a>, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib20"><label>Lämmerzahl et al.(2002)Lämmerzahl, Röckmann, Brenninkmeijer,
Krankowsky, and Mauersberger</label><mixed-citation>
Lämmerzahl, P., Röckmann, T., Brenninkmeijer, C. M., Krankowsky, D., and
Mauersberger, K.: Oxygen isotope composition of stratospheric carbon
dioxide, Geophys. Res. Lett., 29, 2–5, 2002.
</mixed-citation></ref-html>
<ref-html id="bib1.bib21"><label>Mahata et al.(2012)Mahata, Bhattacharya, Wang, and Liang</label><mixed-citation>
Mahata, S., Bhattacharya, S. K., Wang, C.-H., and Liang, M.-C.: An improved
CeO<sub>2</sub> method for high-precision measurements of <sup>17</sup>O ∕ <sup>16</sup>O ratios
for atmospheric carbon dioxide., Rapid Commun. Mass Sp.,
26, 1909–1922, <a href="http://dx.doi.org/10.1002/rcm.6296" target="_blank">doi:10.1002/rcm.6296</a>, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib22"><label>Mook and Jongsma(1987)</label><mixed-citation>
Mook, W. G. and Jongsma, J.: Measurement of the N<sub>2</sub>O correction for <sup>13</sup>C
/<sup>12</sup>C ratios of atmospheric CO<sub>2</sub> by removal of N<sub>2</sub>O, Tellus B, 39B,
96–99, <a href="http://dx.doi.org/10.1111/j.1600-0889.1987.tb00274.x" target="_blank">doi:10.1111/j.1600-0889.1987.tb00274.x</a>, 1987.
</mixed-citation></ref-html>
<ref-html id="bib1.bib23"><label>Mook and van der Hoek(1983)</label><mixed-citation>
Mook, W. G. and van der Hoek, S.: The N<sub>2</sub>O correction in the carbon and
oxygen isotopic analysis of atmospheric CO<sub>2</sub>, Chem. Geol., 41, 237–242, <a href="http://dx.doi.org/10.1016/S0009-2541(83)80021-7" target="_blank">doi:10.1016/S0009-2541(83)80021-7</a>, 1983.
</mixed-citation></ref-html>
<ref-html id="bib1.bib24"><label>Mrozek et al.(2015)Mrozek, van der Veen, Kliphuis, Kaiser, Wiegel,
and Röckmann</label><mixed-citation>
Mrozek, D. J., van der Veen, C., Kliphuis, M., Kaiser, J., Wiegel, A. A., and
Röckmann, T.: Continuous-flow IRMS technique for determining the <sup>17</sup>O excess
of CO<sub>2</sub> using complete oxygen isotope exchange with cerium oxide, Atmos. Meas.
Tech., 8, 811–822, <a href="http://dx.doi.org/10.5194/amt-8-811-2015" target="_blank">doi:10.5194/amt-8-811-2015</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib25"><label>Park et al.(2004)Park, Atlas, and Boering</label><mixed-citation>
Park, S., Atlas, E. L., and Boering, K. A.: Measurements of N<sub>2</sub>O
isotopologues in the stratosphere: Influence of transport on the apparent
enrichment factors and the isotopologue fluxes to the troposphere, J.
Geophys. Res.-Atmos., 109, D01305, <a href="http://dx.doi.org/10.1029/2003JD003731" target="_blank">doi:10.1029/2003JD003731</a>, 2004.
</mixed-citation></ref-html>
<ref-html id="bib1.bib26"><label>Paul et al.(2016)Paul, Chen, Been, Kivi, and Meijer</label><mixed-citation>
Paul, D., Chen, H., Been, H. A., Kivi, R., and Meijer, H. A. J.: Radiocarbon
analysis of stratospheric CO<sub>2</sub> retrieved from AirCore sampling, Atmos. Meas.
Tech., 9, 4997–5006, <a href="http://dx.doi.org/10.5194/amt-9-4997-2016" target="_blank">doi:10.5194/amt-9-4997-2016</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib27"><label>Röckmann et al.(2003)Röckmann, Kaiser, Brenninkmeijer, and
Brand</label><mixed-citation>
Röckmann, T., Kaiser, J., Brenninkmeijer, C. A. M., and Brand, W. A.: Gas
chromatography/isotope-ratio mass spectrometry method for high-precision
position-dependent <sup>15</sup>N and <sup>18</sup>O measurements of atmospheric nitrous
oxide., Rapid Commun. Mass Sp., 17, 1897–908,
<a href="http://dx.doi.org/10.1002/rcm.1132" target="_blank">doi:10.1002/rcm.1132</a>, 2003.
</mixed-citation></ref-html>
<ref-html id="bib1.bib28"><label>Thiemens et al.(1995)Thiemens, Jackson, Zipf, Erdman, and
Egmond</label><mixed-citation>
Thiemens, M., Jackson, T., Zipf, E. C., Erdman, P. W., and Egmond, V. C.:
Carbon dioxide and oxygen isotope anomalies in the mesosphere and
stratosphere, Science, 270, 969–972, 1995.
</mixed-citation></ref-html>
<ref-html id="bib1.bib29"><label>Wiegel et al.(2013)Wiegel, Cole, Hoag, Atlas, Schauffler, and
Boering</label><mixed-citation>
Wiegel, A. A., Cole, A. S., Hoag, K. J., Atlas, E. L., Schauffler, S. M., and
Boering, K. A.: Unexpected variations in the triple oxygen isotope
composition of stratospheric carbon dioxide, P. Natl.
Acad. Sci., 110, 17680–17685, <a href="http://dx.doi.org/10.1073/pnas.1213082110" target="_blank">doi:10.1073/pnas.1213082110</a>,
2013.
</mixed-citation></ref-html>--></article>
