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<!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" xml:lang="en" dtd-version="3.0" article-type="research-article"><?xmltex \makeatother\@nolinetrue\makeatletter?>
  <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-15-7337-2022</article-id><title-group><article-title>Improving continuous-flow analysis of triple oxygen isotopes in ice cores: insights from replicate measurements</article-title><alt-title>Improving continuous-flow analysis of triple oxygen isotopes in ice cores</alt-title>
      </title-group><?xmltex \runningtitle{Improving continuous-flow analysis of triple oxygen isotopes in ice cores}?><?xmltex \runningauthor{L. Davidge et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes">
          <name><surname>Davidge</surname><given-names>Lindsey</given-names></name>
          <email>ldavidge@uw.edu</email>
        <ext-link>https://orcid.org/0000-0002-1283-7508</ext-link></contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Steig</surname><given-names>Eric J.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8191-5549</ext-link></contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Schauer</surname><given-names>Andrew J.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5941-5396</ext-link></contrib>
        <aff id="aff1"><institution>Department of Earth and Space Sciences, University of Washington,
Seattle, WA 98195, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Lindsey Davidge (ldavidge@uw.edu)</corresp></author-notes><pub-date><day>22</day><month>December</month><year>2022</year></pub-date>
      
      <volume>15</volume>
      <issue>24</issue>
      <fpage>7337</fpage><lpage>7351</lpage>
      <history>
        <date date-type="received"><day>17</day><month>March</month><year>2022</year></date>
           <date date-type="rev-request"><day>25</day><month>April</month><year>2022</year></date>
           <date date-type="rev-recd"><day>2</day><month>November</month><year>2022</year></date>
           <date date-type="accepted"><day>9</day><month>November</month><year>2022</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2022 Lindsey Davidge et al.</copyright-statement>
        <copyright-year>2022</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://amt.copernicus.org/articles/15/7337/2022/amt-15-7337-2022.html">This article is available from https://amt.copernicus.org/articles/15/7337/2022/amt-15-7337-2022.html</self-uri><self-uri xlink:href="https://amt.copernicus.org/articles/15/7337/2022/amt-15-7337-2022.pdf">The full text article is available as a PDF file from https://amt.copernicus.org/articles/15/7337/2022/amt-15-7337-2022.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e96">Stable water isotope measurements from polar ice cores
provide high-resolution information about past hydrologic conditions and are therefore important for understanding earth's climate system. Routine
high-resolution measurements of <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, <inline-formula><mml:math id="M2" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>D, and deuterium
excess are made by continuous-flow analysis (CFA) methods that include laser spectrometers. Cavity ring-down laser spectroscopy (CRDS) allows for
simultaneous measurements of all stable water isotopes, including <inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:math></inline-formula>O excess (<inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O); however, the limitations
of CFA methodologies for <inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O are not well understood. Here, we
describe a measurement methodology for all stable water isotopes that uses a CFA system coupled with a CRDS instrument. We make repeated measurements of an ice-core section using this method to explore the reproducibility of CFA–CRDS measurements for <inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O. Our data demonstrate that the CFA–CRDS method can make high-precision measurements of <inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O (<inline-formula><mml:math id="M9" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 5 per meg at averaging times <inline-formula><mml:math id="M10" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 3000 s). We show that the
variations within our CFA ice-core measurements are well matched in
magnitude and timing by the variations within the discrete CRDS
measurements; we find that calibration offsets generate most of the
variability among the replicate datasets. When these offsets are accounted
for, the precision of CFA–CRDS ice-core data for <inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O is as
good as the precision of <inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O for continuous reference water
measurements. We demonstrate that this method can detect seasonal
variability in <inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in Greenland ice, and our work suggests
that the measurement resolution of CFA–CRDS is largely defined by the melt
and measurement rate. We suggest that CFA–CRDS has the potential to increase measurement resolution of <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in ice
cores, but also highlight the importance of developing calibration
strategies with attention to <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e272">Records of water isotopologues from ice cores are fundamental to the study
of past climate processes (Dansgaard, 1964). Oxygen (<inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O) and
hydrogen (<inline-formula><mml:math id="M18" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>D) isotope ratios have been measured routinely in ice-core samples and in other natural waters due to their well-understood,
first-order equilibrium fractionation relationship to atmospheric
temperature (Jouzel et al., 1997). Additionally, deuterium excess (<inline-formula><mml:math id="M19" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula>) is
commonly used as an indicator of kinetic fractionation processes within the
hydrologic cycle (Merlivat and Jouzel, 1979; Jouzel and Merlivat, 1984). Deuterium excess is
conventionally defined as
          <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M20" display="block"><mml:mrow><mml:mi>d</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="italic">δ</mml:mi><mml:mrow class="chem"><mml:mi mathvariant="normal">D</mml:mi></mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">8</mml:mn><mml:mo>×</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mrow></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
        Barkan and Luz (2005) showed that measuring <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O at a sufficiently high precision allows for the determination of
<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:math></inline-formula>O excess (<inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O), a quantity that, like <inline-formula><mml:math id="M25" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula>, also reflects
nonequilibrium fractionation processes such as sea-surface humidity (Uemura
et al., 2010; Barkan and Luz, 2007) and supersaturation effects during snow formation (Schoenemann et al., 2014; Schoenemann and Steig, 2016). <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O is defined by Luz and Barkan (2010) as the
deviation in <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O from the global meteoric water line:
          <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M28" display="block"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>=</mml:mo><mml:mi>ln⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfenced><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.528</mml:mn><mml:mi>ln⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math id="M29" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula> (“delta”) values are expressed as a unitless fractional
deviation from Vienna Standard Mean Ocean Water (VSMOW; see, e.g.,
Schoenemann et al., 2013, for a complete discussion of nomenclature).</p>
      <p id="d1e467">Measurements of <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, <inline-formula><mml:math id="M31" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>D, and <inline-formula><mml:math id="M32" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> by laser spectroscopy
have been demonstrated by many laboratories (e.g., Kerstel et al., 1999;
Iannone et al., 2010; Steen-Larsen et al., 2014; Schauer et al., 2016; Jones et al.,
2017a); for water isotope measurements of ice cores, it is increasingly
common to couple a laser spectrometer with a continuous-flow analysis (CFA)
system. CFA processing reduces sample handling and can produce very high
depth resolution (originally described by Gkinis et al., 2010, 2011). Highly
resolved water isotope measurements are advantageous for a variety of
studies, such as those that use the water isotope diffusion length to infer
information about firn processes or to reconstruct temperature histories
(e.g., Gkinis et al., 2014; Kahle et al., 2018, 2021; Jones et al., 2017b).
It is desirable to obtain measurements of <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O at a resolution comparable to that for <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, <inline-formula><mml:math id="M36" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>D, and <inline-formula><mml:math id="M37" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula>. Corresponding measurements of both <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M39" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> – which
have differing sensitivities to kinetic fractionation processes – could
help to disentangle the various processes that influence water isotope
values during evaporation, atmospheric transportation, and snow formation
(Angert et al., 2004; Uemura et al., 2010). However, measurements of <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O require much higher precision than the other water isotope ratios
and have therefore generally been obtained by isotope-ratio mass
spectrometry (IRMS) (Luz and Barkan, 2010; Landais et al., 2008, 2012a, b;
Schoenemann et al., 2013, 2014). Because the IRMS method is relatively
expensive and time-consuming, <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O measurements from ice cores
are limited in spatial and temporal resolution (e.g., Schoenemann et al., 2014; Aron et al., 2021). CFA for <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O has
the potential to address this limitation.</p>
      <p id="d1e595">Laser spectroscopy enables simultaneous measurements of <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O,
<inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, and <inline-formula><mml:math id="M45" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>D (and therefore <inline-formula><mml:math id="M46" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O).
Steig et al. (2014) developed a cavity ring-down laser spectrometer (CRDS)
for <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O analysis, sold commercially as the Picarro L2140-<inline-formula><mml:math id="M49" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>;
other instruments with different spectroscopic methods have also been
developed for <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O analysis (e.g., Berman et al., 2013; Tian et
al., 2016). Schauer et al. (2016) demonstrated that the L2140-<inline-formula><mml:math id="M51" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> CRDS
configured with an autosampler can routinely measure <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O from
discrete water samples with precision and accuracy comparable to IRMS
methods. Steig et al. (2021) obtained continuous measurements of all water isotope quantities (<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, <inline-formula><mml:math id="M55" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>D, <inline-formula><mml:math id="M56" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula>, and
<inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O) on an ice core from the South Pole by using the L2140-<inline-formula><mml:math id="M58" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>
CRDS coupled with the CFA system developed by Jones et al. (2017a). However,
despite the potential shown by these studies, the adoption of CFA–CRDS for
<inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O faces two primary challenges. First, the integration time
required for high-precision <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O measurements by CRDS –
approximately 1000 s to achieve precision of 10 per meg (Steig et al., 2014)
– is much greater than the integration time required to achieve meaningful
precision for <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, <inline-formula><mml:math id="M62" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>D, or <inline-formula><mml:math id="M63" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula>. Second, the CFA system –
i.e., the melting and vaporization process used to introduce an ice-core
sample into the CRDS – may further degrade the measurement quality by
processes that are not yet well understood. For example, Steig et al. (2021)
identified occasional large (<inline-formula><mml:math id="M64" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 20 per meg) offsets in CFA–CRDS
<inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in their measurements of the South Pole ice core; the
cause of these offsets was unclear. It is our goal to characterize the
reproducibility of replicate ice-core measurements of <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O by
CFA–CRDS.</p>
      <p id="d1e826">Here, we describe a CFA–CRDS measurement methodology that was designed for
high-resolution measurements of <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O. We take advantage of
archived ice-core samples from Summit, Greenland, to make repeated CFA–CRDS
measurements of <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O. These samples (collected by Hastings et
al., 2009) provide an opportunity to explore the potential and limitations
of <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O measurements by CFA–CRDS more fully. We use replicate
measurements made by CFA–CRDS and discrete CRDS methods to assess the
reproducibility of CFA–CRDS <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O data and to identify sources
of measurement error.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>CFA–CRDS design and configuration</title>
      <p id="d1e881">We use a CFA processing line in combination with a CRDS laser spectrometer
(L2140-<inline-formula><mml:math id="M71" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>, Picarro Inc., as in Steig et al., 2014) to measure <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of ice-core samples. The function of the CFA line is to generate a
continuous supply of constant-humidity sample vapor to the CRDS analyzer; to
achieve this, we have built a custom vaporizer unit that is described below.
A constant stream of vaporized sample is important because errors in
isotope-ratio measurements can arise from inconsistent vapor pressure at the
CRDS inlet (Gkinis et al., 2011; Schauer et al., 2016). Finally, we aim to
reduce diffusion and mixing within the CFA system to avoid smoothing the
resulting measurements.</p>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Custom vaporizer design</title>
      <p id="d1e909">Continuous and complete vaporization is critical to reducing errors in all
CRDS stable water isotope measurements, and it is especially important for
attaining the per-meg precision necessary to detect meaningful variations in
<inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O. Previous studies have achieved continuous vaporization by
heating sample water in the presence of dry air, either within an insulated
stainless-steel tee (e.g., Gkinis et al., 2010, 2011) or within a concentric
glass nebulizer with a vaporizing tube (e.g., Emanuelsson et al., 2015;
Jones et al., 2017a). Gkinis et al. (2010, 2011) designed a flash vaporization process to instantaneously vaporize a continuous stream of
sample water; the flash vaporization process involves a continuous stream of
water that is combined with a continuous stream of dry air inside a 0.50 mm
internal diameter stainless-steel tee that is maintained at near-ambient
pressure. Steig et al. (2021) measured <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O by CFA–CRDS with
the CFA configuration of Jones et al. (2017a): a continuous stream of water
sample at 1030 kPa (150 psi) is aerosolized within a concentric glass
nebulizer; the aerosolized sample droplets then evaporate completely within
a 1.8 cm internal diameter, 20 cm long glass vaporizing tube that is heated
to 200 <inline-formula><mml:math id="M75" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. In this configuration, the CRDS analyzer draws vaporized
sample from the vaporizing tube, and excess sample vapor is vented to the
laboratory air (Jones et al., 2017a; Steig et al., 2021). Two critical
differences between the Gkinis et al. (2010, 2011) and Jones et al. (2017a)
methods are the volume of the vaporization chamber and the volume of vapor
that is generated. The smaller volume of the flash vaporizer should limit
signal smoothing between the vaporizer and the analyzer. However, the flash
vaporization method described by Gkinis et al. (2010, 2011) generates vapor at
approximately the rate that is required by the analyzer, whereas the
nebulizer method of Jones et al. (2017a) produces an excess of vapor that is
vented prior to reaching the analyzer. Producing excess vapor is another way
to limit the signal smoothing upstream of the vapor vent because it
increases the velocity of sample through the system.</p>
      <p id="d1e943">For this study, we built a custom vaporizer unit that benefits from both the
small volume of the flash vaporizer and also from the production of excess
sample vapor; we also adopted additional monitoring techniques to ensure
that there are stable flow conditions within the system during analysis. We
use a 0.50 mm stainless-steel tee like Gkinis et al. (2010, 2011) but instead operate our vaporizer at a high mixing pressure (typically
200 kPa) ​​​​​​​to produce excess vapor. A small system volume
combined with a high volumetric flow rate leads to a short retention time
within the vaporizer that limits mixing of adjacent ice-core layers. An
additional benefit of the small vaporizer volume is that flow
inconsistencies (i.e., changes in sample flow rate caused by flow
obstructions or bubble interruptions) that may occur within the vaporizer
can be observed by the 1 Hz CRDS measurement values; patterns in water vapor
concentration or instantaneous isotope readings provide information about
vaporization conditions that is important for identifying and avoiding water isotope fractionation. We use CRDS observations of water concentration and
uncalibrated water isotope values as well as electronic pressure sensors to
infer vaporization conditions that may affect <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O. This
information is used to tune the CFA–CRDS system prior to analysis, with the
goal of reducing possible isotope fractionation that may cause errors in
<inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O; this process is described more fully in Sect. 3.1.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>CFA–CRDS system configuration</title>
      <p id="d1e976">The CFA process from the ice-core melter to the vaporizer and vapor analyzer
is described below and illustrated in Fig. 1. Glacial ice is melted on a
30 mm <inline-formula><mml:math id="M78" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 30 mm aluminum melt head that is fitted with four
resistance heater cartridges and held at constant temperature by a PID
controller (Bigler et al., 2011). Sample melt is drawn away from the melt
head and through an automated selector valve (VICI, p/n C25Z-3186EMH) by a
dedicated peristaltic pump, PUMP-1 (MasterFLex L/S 7535-04). The automated
valve is configured to select a rotating sequence of calibration standards
when ice cores are not being measured. Sample melt is carried by 0.5 mm
internal diameter PFA conveyance tubing between all system components prior
to the vaporizer; PFA tubing was chosen because its transparency is
advantageous for identifying bubbles and investigating flow instability
issues. From PUMP-1, water flows through a Darwin Microfluidics
gas-permeable membrane bubble trap (44 <inline-formula><mml:math id="M79" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>L internal volume, p/n LVF-3526) where bubbles are removed and vented into the laboratory air. Excess
water pressure is relieved at a vent. Sample water is drawn away from the
vent by PUMP-2 (same model as PUMP-1), whose flow rate is set to match the
demand of the downstream vaporizer. The vent accommodates the difference
between PUMP-1, which controls the melt rate, and PUMP-2, which controls the
vaporization rate. Water flows through 2 and 1 <inline-formula><mml:math id="M80" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m in-line
filters in series to restrict the flow of particulates into the vaporizer.
PUMP-2 is also preceded and followed by electronic pressure sensors PI-1
(Elveflow PS3-Small) and PI-2 (Elveflow PS4-Small) to monitor injection
pressure conditions and pump and filter performance. Typically, the
pressurized dry air entering the vaporizer adds back pressure on the liquid
sample injection line, which damps the cyclic pressure fluctuations of the
peristaltic pump and stabilizes flow into the vaporizer. The
system also includes a flow valve (FV-1) that can be used to adjust the
back pressure on PUMP-2 before making a measurement.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e1004">Process flow diagram of the CFA system. Thick dashed lines
indicate transitions between temperature-controlled process spaces. Note
that F-1 and F-2 are filters, PI-1 and PI-2 are pressure sensors, and FV-1
is a flow valve.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://amt.copernicus.org/articles/15/7337/2022/amt-15-7337-2022-f01.png"/>

        </fig>

      <p id="d1e1013">At the vaporizer, filtered sample water is mixed and heated with dry air to
produce a constant-humidity stream of vaporized sample. Immediately before
entering the vaporizer, the liquid sample line is reduced to a 100 <inline-formula><mml:math id="M81" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m fused silica capillary tube. The 100 <inline-formula><mml:math id="M82" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m capillary provides sufficient
flow restriction that is important for efficient vaporization while also
performing well for periods of several days without clogging. The custom
vaporizer includes a 0.50 mm internal diameter tee heated to 170 <inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
using a PID-controlled resistance heater cartridge, similar to Gkinis et al. (2010, 2011). The vaporizer combines pressurized dry air with liquid sample,
and it is set within an aluminum enclosure that is lined with 3.175 cm of
calcium silicate insulation. After the sample is vaporized, the vapor is
drawn into the optical cavity where it is measured, and excess vapor is
vented into the laboratory. Vapor is carried from the vaporizer to the
optical cavity within insulated tubing to prevent condensation.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Design choices to mitigate memory effects</title>
      <p id="d1e1049">Design choices for the CFA system are intended to reduce
and characterize the memory between measurements. Because our automated
selector valve is positioned immediately after the ice-core melt head,
reference waters pass through all components of the sample handling system
except the melt head and its tubing; by design, the mixing length expected
between measured ice-core layers with differing isotopic compositions can be
approximated by the mixing length represented by transitions in reference
waters if all other system conditions are identical. Mixing length within
the system is reduced by increasing the flow velocity and therefore limiting
the sample retention time in two ways: overall sample handling system volume
and tubing diameters are minimized where possible, and excess sample volume
is drawn through the entire system during ice-core analysis. Approximately 6 times more water is handled by PUMP-1 than
is sent by PUMP-2 into the vaporizer; excess liquid volume is vented before
PUMP-2. Similarly, approximately 30 times more vapor is generated than
is analyzed; excess vapor is driven by the differential between PUMP-2 and
the L2140-<inline-formula><mml:math id="M84" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> inlet pump, and it is vented to laboratory air immediately before
vapor enters the optical cavity. In this way, the liquid and vapor tubing is
flushed with many times more sample volume than is required for analysis.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>CFA–CRDS operations and measurements</title>
      <p id="d1e1068">We designed an operational sequence for reference water and ice-core
measurements during a period when lab work was intermittent due to the
COVID-19 pandemic. The CFA system was configured to automatically measure an
alternating sequence of three in-house reference waters over a period of
approximately 7 weeks; reference waters included Seattle tap water
(SW2), West Antarctic Ice Sheet Divide snow (CW), and South Pole snow
(SPS2), as shown in Table 1 and indicated in Fig. 2. Measuring reference
waters continuously allows us to explore the long-term changes in system
calibration while also informing maintenance requirements over long
timescales. When available, an operator prepared and measured an ice-core
section between reference water measurements. The need for frequent
calibration of CRDS data for <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O has been well documented
(e.g., Schauer et al., 2016), and continuous reference water measurements
ensured that there were calibration data available adjacent in time to each
intermittent ice-core analysis.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e1085">Isotopic values of reference waters. SW2 is Seattle deionized tap
water, CW is melt water from the WDC06A core (i.e., West Antarctic Ice Sheet
precipitation), and SPS2 is South Pole snow. These three waters were
normalized to the VSMOW-SLAP scale using other in-house reference waters
that were analyzed against VSMOW, SLAP, and GISP. The calibrated <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O values are calculated from the combination of <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O
and <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and are therefore reported to four significant digits
(see Schoenemann et al., 2013, for additional details).</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="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right" colsep="1"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Reference water</oasis:entry>
         <oasis:entry rowsep="1" colname="col2"><inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O</oasis:entry>
         <oasis:entry rowsep="1" colname="col3"><inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O</oasis:entry>
         <oasis:entry rowsep="1" colname="col4"><inline-formula><mml:math id="M91" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>D</oasis:entry>
         <oasis:entry rowsep="1" colname="col5"><inline-formula><mml:math id="M92" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col6"><inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">(origin location)</oasis:entry>
         <oasis:entry namest="col2" nameend="col5" align="center" colsep="1">‰ vs. VSMOW </oasis:entry>
         <oasis:entry colname="col6">per meg vs.</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">VSMOW</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">SW2 (Seattle)</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M94" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5.7107</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M95" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10.85</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M96" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>77.96</oasis:entry>
         <oasis:entry colname="col5">8.84</oasis:entry>
         <oasis:entry colname="col6">33</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CW (West Antarctica)</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M97" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>17.8807</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M98" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>33.64</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M99" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>265.95</oasis:entry>
         <oasis:entry colname="col5">3.17</oasis:entry>
         <oasis:entry colname="col6">25</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SPS2 (South Pole)</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M100" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>25.1210</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M101" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>47.07</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M102" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>365.20</oasis:entry>
         <oasis:entry colname="col5">11.36</oasis:entry>
         <oasis:entry colname="col6">15</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1359">Uncalibrated 1 Hz measurements of <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O for the alternating sequence of reference waters during a full analysis day <bold>(c)</bold>. The 200 s preceding and 800 s following four reference water transitions are shown in the other
panels; two transitions (shown in orange and green) from SPS2 to CW are
stacked in panel <bold>(a)</bold> and two transitions from CW to SW2 are stacked in panel <bold>(b)</bold>.</p></caption>
        <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://amt.copernicus.org/articles/15/7337/2022/amt-15-7337-2022-f02.png"/>

      </fig>

      <p id="d1e1389">We operated the CFA–CRDS system to measure nine repeated sections of an ice
core and a repeated sequence of internal reference waters that we used to
calibrate the ice-core measurements. We also measured a replicate ice-core section by
discrete CRDS for comparison. Repeated reference water measurements are used
to develop a calibration for the ice-core data. We compare our calibrated
CFA–CRDS <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O data with the discrete measurements to evaluate
this method.</p>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Operational considerations to maintain efficient vaporization</title>
      <p id="d1e1410">Because the vaporizer is sensitive to small fluctuations in sample flow
rate, a careful balance of system pressures is required to control sample
flow (Gkinis et al., 2010, 2011); specifically, the pressure of the sample
at the vaporizer inlet must be slightly greater than the pressure of the dry
air within the vaporizer. Maintaining a balance between the air pressure and
sample pressure within the vaporizer requires knowledge of both pressure
conditions. We monitor pressures at PI-1 and PI-2 so that it is possible to
diagnose the source of system pressure changes when they occur; we also fix
the pressure of the dry air line with the back pressure regulator (typically
200 kPa). Vacuum conditions at PI-1 indicate particulate loading across the
filter screen at F-1; the filter screen will clog over time, and if the
filter screen is not replaced, suction from the inlet of PUMP-1 can draw a
vacuum at PI-1. Vacuum conditions at PI-1 can impact the downstream
peristaltic pump (PUMP-2) performance, ultimately causing inconsistent flow
into the vaporizer and analyzer. Under optimal analysis conditions, the
pressure is near ambient at PI-1. A decrease in pressure at PI-2 indicates
upstream vacuum conditions or worn peristaltic pump tubing at PUMP-2. An
increase in pressure at PI-2 indicates clogging downstream, which can occur
as particulate loading within F-2 or as mineral precipitation within the
capillary or vaporizer. The pressure at PI-2 generally varied between 200 and 400 kPa, depending on the injection air pressure and the precipitate
levels within the vaporizer or capillary tubing. High-pressure vaporizer
conditions allow sample to flow despite the inevitable accumulation of
precipitate within the vaporizer, which enables the system to operate in
balance for days or even weeks. However, over time, precipitate accumulation
within the vaporizer can restrict the flow of air, water, or both; this
typically requires re-balancing of system flow conditions, but it can
occasionally require removing and cleaning the vaporizer fittings with soap,
water, and physical agitation.</p>
      <p id="d1e1413">During operation of the CFA–CRDS, intermittent reductions in water vapor
concentration can occur within the vaporizer, which can produce
perturbations in the isotope data. Gkinis et al. (2010, 2011) described
sample flow inconsistencies at their CFA flash vaporizer that caused extreme
outliers in isotope data, though the cause of the fluctuations was unclear.
We observe similar fluctuations, and the pressure sensor data provide
insight into their cause. We find that the most common causes of such
variations are microbubbles entering the vaporizer owing to particulate
loading, which can cause poor debubbler performance and can also cause
blockages to form within the small tubing fittings. Microbubbles that remain
suspended in the fluid stream after the debubbler cause volumetric flow rate
reductions at the vaporizer inlet. Blockages within fittings upstream of
PUMP-2 can cause extreme vacuum conditions before the pump (i.e., pressure
observations associated with blockages were as low as <inline-formula><mml:math id="M105" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>140 kPa before PUMP-2 instead of the typical ambient conditions); this can lead to the
contamination of system tubing with small bubbles that also cause temporary
flow reductions. To avoid these inconsistencies, we find that it is
important to periodically clean the debubbler unit and to maintain ambient
pressure at the PUMP-2 inlet by replacing clogged filter screens or tubing
fittings. Although data outliers could be systematically removed (as done in
Gkinis et al., 2011), occasional bubbles do not substantially impact the
isotopic mean value of our ice-core measurements and are retained here. We
do exclude some reference-water calibration data, where bubble interruptions
are most frequent due to limited operator oversight during the automated
reference water measurements. Calibration measurement criteria are discussed
in Sect. 3.4.</p>
      <p id="d1e1423">In addition to monitoring pressure evolution across the system, we can also
observe the quality of vapor at the CRDS analyzer via characteristic
patterns that arise in the CRDS data. Specific patterns in water vapor
concentration and <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O that emerge from unstable flow into the
vaporizer are shown in Fig. 3. We observe that pulsating flow conditions can
cause incomplete vaporization, identified by anticorrelated fluctuations in
water vapor concentration and <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O. When a pulse of water
overwhelms the vaporizer, the isotopic composition becomes lighter as
H<inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mn mathvariant="normal">16</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula>O preferentially evaporates into the vapor stream; as the
vaporizer dries out between pulses, the isotopic composition becomes
heavier, exhibiting an evaporation signal. Pulsating flow conditions are
caused by pressure fluctuations from the peristaltic pump (<inline-formula><mml:math id="M109" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 70 kPa) when insufficient back pressure is applied on PUMP-2. The resulting
patterns have a large amplitude (up to 10 000 ppm for water vapor and
several ‰ for <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O) and a frequency that
mirrors that of the peristaltic pump (e.g., Fig. 3a). The observed
fractionation that occurs during these vaporization conditions leads to
large calibration bias for <inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, causing errors of tens to
hundreds of per meg. If there is sufficient back pressure at PUMP-2, the
pressure readings at PI-2 are typically <inline-formula><mml:math id="M112" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 40 kPa. We attribute small
fluctuations in <inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O that are anticorrelated with water vapor
concentration to the incomplete vaporization of individual droplets (e.g.,
Fig. 3b). Because inconsistent flow into the vaporizer can cause isotope
fractionation and because it is important to measure calibration standards
under the same conditions as the ice-core samples, we tune the system to
maintain steady pressure readings at the vaporizer inlet prior to
calibration standard and ice-core analysis, as discussed in Sect. 3.2;
vapor concentration data that are typical of a well-maintained CFA system
are shown in Fig. 3d.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1511">Observations of vapor quality as real-time indicators of vaporizer
performance. Each panel shows corresponding observations of water vapor
concentration and <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of SW2, reported in parts per thousand
vapor (pptv) and ‰, respectively. Panels <bold>(a)</bold> and <bold>(b)</bold> show
observations indicative of imbalanced vaporizer conditions for large and
small pressure imbalances, respectively. Panels <bold>(c)</bold> and <bold>(d)</bold> show observations indicative of acceptable vaporizer performance. Though both include low-variability observations of <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O (<inline-formula><mml:math id="M116" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M117" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.3 ‰) and of water vapor concentration, <bold>(c)</bold> also includes microbubble interruptions at the vaporizer (e.g., at 5 and 440 s). Panel <bold>(d)</bold> indicates optimal vaporizer performance. Note that the vertical scaling of <bold>(a)</bold> is different from the other panels.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/15/7337/2022/amt-15-7337-2022-f03.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><?xmltex \opttitle{Measuring $\Delta^{{17}}$O by CFA--CRDS in ice-core samples}?><title>Measuring <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O by CFA–CRDS in ice-core samples</title>
      <p id="d1e1598">Approximately 12 to 24 h before making an ice-core
measurement, an operator maintained the CFA system to balance the flow rate
into the vaporizer. For example, when indicated by anomalously high or low
pressure sensor data, the filter screens, peristaltic pump tubing, or
capillary tubing were replaced. When indicated by CRDS data trends as in
Fig. 3, the vaporizer components were cleaned. Returning the CFA system to a
balanced state before making measurements of all reference waters increases
the likelihood of having usable, high-quality calibration data against which
to calibrate the ice-core samples. At other times when ice-core measurements
were not made, the system occasionally drifted out of balance and was not
actively maintained such that some of the reference water measurements are
of lower quality than those used to calibrate the ice-core measurements.
This is discussed in more detail in Sect. 3.4.</p>
      <p id="d1e1601">We cut an 87.5 cm ice-core sample from <inline-formula><mml:math id="M119" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 92 m depth beneath
the surface at Summit, Greenland, into nine 26 mm square slices to prepare
them for continuous analysis. After preparing these nine CFA sticks, a 10th
section of core was cut into 63 discrete depth intervals. Discrete ice
samples were melted in sealed polyethylene sample bottles in a refrigerator
at 4 <inline-formula><mml:math id="M120" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. We measured the 87.5 cm section of ice 10 times: the
nine replicate slices were measured by the CFA–CRDS configuration described
above, and the 10th measurement was made by a discrete injection of 63 melt
samples from the core using the commercially available vaporizer unit
(Picarro p/n A0211) and automated injections as in Schauer et al. (2016).
The depth resolution of the discretely measured ice is 1.39 cm.</p>
      <p id="d1e1620">For all CFA measurements, we made visual observations of the core height to
monitor the melt rate during analysis, then later assigned a high-resolution
depth equivalent for each analysis time that is based on the value of
<inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and the measured depth of discrete samples. Previous work
has monitored core depth with electronic distance meters (e.g., Bigler et
al., 2011; Jones et al., 2017a), and such measurements are critical for
depth registration for routine CFA measurement campaigns. Here, we forego
electronic depth registration and instead adjust initial depth estimates for
each core section by aligning the seasonal cycle of <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O for
all core samples. Assigning depths by aligning the <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O
variations should largely eliminate depth-registration errors, since the
strong seasonal <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O variations must be essentially identical
in each replicate sample, and the signal-to-noise ratio for <inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O is very high. Summit, Greenland, has a modern annual accumulation rate of
24 <inline-formula><mml:math id="M126" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5 cm (ice equivalent) per year (Meese et al., 1994; Dibb and
Fahnestock, 2004; Hawley et al., 2008, 2020), and we expect to see 2 to
3 years represented by the core sample that we measured in replicate
(Hastings et al., 2009). We compressed the timescale of each CFA time series to
maximize the cross-correlation of <inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O (0.93 <inline-formula><mml:math id="M128" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M129" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M130" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.99) between the CFA measurements and the discrete measurements.
We then assigned each CFA time a depth equivalent based on the
depth of the corresponding discrete <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O data. We note that the
amplitude of the seasonal variations in <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O is somewhat
compressed in the lower <inline-formula><mml:math id="M133" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 cm of this core sample, so the
depth designations for this interval are likely a greater source of error
than in the rest of the ice. Nevertheless, we are confident that our depth
registration is precise to within 1 cm or better, determined by assessing
the variance in depth assignments at inflection points.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Operational choices to mitigate memory effects</title>
      <p id="d1e1756">Mitigating memory effects is important for both ice-core and reference water
measurements; in addition to the design choices highlighted in Sect. 2.3,
there are several operational choices that were made to reduce the memory
between isotopically distinct waters. For example, increasing the pump rates
at PUMP-1 during ice-core analysis should drive shorter retention times
within the tubing upstream of the liquid vent, which should reduce system
mixing. In this way, the transition times for reference waters (shown in
Fig. 2) are a conservative estimate of mixing effects. The transition time
between measurements of reference waters generally varied between 180 and
360 s. We therefore assume a conservative mixing time of 360 s during
reference water transitions, and we ignore the 360 s that initiate and
conclude each reference water measurement. Before measuring each section of
ice (which is typically <inline-formula><mml:math id="M134" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 m long), we also condition the
system with at least 10 min of water with similar isotopic composition
to prevent mixing between isotopically disparate reference waters and ice-core samples at the beginning of the analysis. Finally, the replicate
CFA–CRDS measurements that are the focus of this study provide a practical
evaluation of the effects of memory on measurement fidelity in this
configuration.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><?xmltex \opttitle{Calibrating CFA--CRDS $\Delta^{{17}}$O data}?><title>Calibrating CFA–CRDS <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O data</title>
      <p id="d1e1787">To achieve an accurate calibration, similar treatment of reference waters
and sample melt during vaporization is critical. For this study, we measured
the calibration standards immediately before and after measuring an ice-core
section; this ensures the most comparable treatment of reference waters and
sample melt. Achieving similar treatment also requires that the system is
stable during the entire measurement period, including reference water
measurements and ice sample measurements. Because an individual ice-core
measurement takes a few hours at the melt rates that we employ, we limit our
reference water measurements to 3 h each to increase the likelihood
that the complete sequence of reference waters and ice-core samples is
measured under similar CFA and CRDS conditions.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e1793">Sequence of CFA–CRDS measurements, including calibration
information and calibration offset determined by Eq. (5) for 1.39 cm
resolved data. Note that the long reference water measurement of SW2 used to
generate Fig. 7 was made on 18 September 2020. Also note that none of the
reference water measurements on 8 September were acceptable to use for
calibration and that the large calibration offset for this measurement may
be attributed to instrument drift or a change in CFA conditions between 8
and 9 September. Notable flow instabilities led to vaporizer cleaning on 14 September and 8 October 2020, and no measurements were made between 27 September and 8 October 2020.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="7">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="center"/>
     <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:colspec colnum="7" colname="col7" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">JEMS2 (91.28–92.15 m)</oasis:entry>
         <oasis:entry colname="col2">SW2, CW, SPS2</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O offset</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">measurement date</oasis:entry>
         <oasis:entry colname="col2">measurement date</oasis:entry>
         <oasis:entry colname="col3">(unitless)</oasis:entry>
         <oasis:entry colname="col4">(unitless)</oasis:entry>
         <oasis:entry colname="col5">(‰)</oasis:entry>
         <oasis:entry colname="col6">(‰)</oasis:entry>
         <oasis:entry colname="col7">(per meg)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">1 September 2020</oasis:entry>
         <oasis:entry colname="col2">1 September 2020</oasis:entry>
         <oasis:entry colname="col3">1.0163</oasis:entry>
         <oasis:entry colname="col4">1.0068</oasis:entry>
         <oasis:entry colname="col5">4.5250</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M141" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.6133</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M142" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1 September 2020</oasis:entry>
         <oasis:entry colname="col2">2 September 2020</oasis:entry>
         <oasis:entry colname="col3">1.0094</oasis:entry>
         <oasis:entry colname="col4">0.9999</oasis:entry>
         <oasis:entry colname="col5">4.4551</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M143" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.6766</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M144" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>9</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2 September 2020</oasis:entry>
         <oasis:entry colname="col2">2 September 2020</oasis:entry>
         <oasis:entry colname="col3">1.0094</oasis:entry>
         <oasis:entry colname="col4">0.9999</oasis:entry>
         <oasis:entry colname="col5">4.4551</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M145" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.6766</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M146" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">4 September 2020</oasis:entry>
         <oasis:entry colname="col2">4 September 2020</oasis:entry>
         <oasis:entry colname="col3">1.0089</oasis:entry>
         <oasis:entry colname="col4">0.9996</oasis:entry>
         <oasis:entry colname="col5">4.4396</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M147" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.6892</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">8 September 2020</oasis:entry>
         <oasis:entry colname="col2">9 September 2020</oasis:entry>
         <oasis:entry colname="col3">1.0132</oasis:entry>
         <oasis:entry colname="col4">1.0040</oasis:entry>
         <oasis:entry colname="col5">4.5910</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M148" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.5211</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M149" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>25</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">15 September 2020</oasis:entry>
         <oasis:entry colname="col2">15 September 2020</oasis:entry>
         <oasis:entry colname="col3">1.0065</oasis:entry>
         <oasis:entry colname="col4">0.9971</oasis:entry>
         <oasis:entry colname="col5">4.2982</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M150" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.9084</oasis:entry>
         <oasis:entry colname="col7">8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">25 September2020</oasis:entry>
         <oasis:entry colname="col2">25 September 2020</oasis:entry>
         <oasis:entry colname="col3">1.0058</oasis:entry>
         <oasis:entry colname="col4">0.9966</oasis:entry>
         <oasis:entry colname="col5">4.4130</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M151" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.6878</oasis:entry>
         <oasis:entry colname="col7">19</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">9–10 October 2020</oasis:entry>
         <oasis:entry colname="col2">10 October 2020</oasis:entry>
         <oasis:entry colname="col3">0.9983</oasis:entry>
         <oasis:entry colname="col4">0.9908</oasis:entry>
         <oasis:entry colname="col5">4.2542</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M152" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.8581</oasis:entry>
         <oasis:entry colname="col7">9</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">10 October 2020</oasis:entry>
         <oasis:entry colname="col2">10 October 2020</oasis:entry>
         <oasis:entry colname="col3">1.0054</oasis:entry>
         <oasis:entry colname="col4">0.9967</oasis:entry>
         <oasis:entry colname="col5">4.4621</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M153" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.5888</oasis:entry>
         <oasis:entry colname="col7">5</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e2222">To calibrate our measurements, we create a two-point
linear calibration from the
nearest measurements of our internal reference waters, SW2 and SPS2; a third
reference water (CW) is used as an independent verification of the
calibration. The values of SW2, CW, and SPS2 have been measured
independently and are normalized to the VSMOW-SLAP scale as in Schoenemann
et al. (2013). An alternating sequence of the three
reference waters was measured between ice core analyses; the selector valve was
programmed to automatically switch between the reference water containers every 3 h.
Automated reference water measurements were typically unsupervised. Reference water measurements were
automated and typically unsupervised. Because measurement conditions evolve
over time due to particulate loading and mineral precipitation within the
CFA components and because there were periods of time during the analysis
window when no operator was available to monitor system conditions, there
were periods of time during which the water vapor concentration was outside
the ideal range, during which large bubbles or other flow inconsistencies
degraded the quality of reference water data, or during which the CFA system
was not operating; consequently, only about 50 % of the data within the
study period is included in this analysis, as described
below and in Table 2. We automatically reject calibration data and
measurements of CW that were generated from water vapor concentrations beyond
the targeted range (i.e., <inline-formula><mml:math id="M154" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 20 000 or <inline-formula><mml:math id="M155" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 50 000 ppm) or
data with insufficient vaporizer operations, indicated by <inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M157" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.5 ‰ across the measurement window.
Typical variability of water vapor concentration within a single 3 h
period is 0.5 % to 5 %. We identify transitions from one reference water
to the next in the data by the second derivative of <inline-formula><mml:math id="M158" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>D and assign
known standard values based on the uncalibrated measurement values of
<inline-formula><mml:math id="M159" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>D. We include measurements of SW2 and SPS2 that contain at least
6000 s of analysis time, and we trim 360 s of data from the beginning and end of each measurement interval to avoid memory effects. The mean and standard deviation of the analysis time for calibration standard data are 9350 <inline-formula><mml:math id="M160" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 660 s. To calibrate all ice-core and CW measurements made during this study, we use 47 continuous 3 h measurements of SW2 and 40
continuous 3 h measurements of SPS2. All analyses include measurements
for <inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, <inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, and <inline-formula><mml:math id="M163" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>D. Calculations of
<inline-formula><mml:math id="M164" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O were obtained from the calibrated <inline-formula><mml:math id="M166" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula> values as
given in Eqs. (1) and (2), respectively. Calibration for <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O
is more completely described below.</p>
      <p id="d1e2353">The calibration data used for all measurements are generated from adjacent
measurements of SW2 and SPS2 that meet the screening criteria above;
calibration data and the sequence of CFA–CRDS measurements are provided in
Table 2. For each calibration of CW or ice-core data, we employ the nearest
measurements of SW2 and SPS2 for the calibration. The calibration is
performed separately for <inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O: using a
least-squares approach, we fit a linear equation to the uncalibrated average
measurements so that the calibrated SW2 and SPS2 measurements match their
known values. The calibration equation therefore becomes
            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M170" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">δ</mml:mi><mml:mi mathvariant="normal">calibrated</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>m</mml:mi><mml:mo>×</mml:mo><mml:msub><mml:mi mathvariant="italic">δ</mml:mi><mml:mi mathvariant="normal">uncalibrated</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi>b</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M171" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula> represents either <inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O or <inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O. An account of <inline-formula><mml:math id="M174" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M175" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> for both <inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O is shown for all measurements in Table 2. Finally, <inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O is calculated from the calibrated values of <inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and
<inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O:
            <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M181" display="block"><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi>ln⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.528</mml:mn><mml:mi>ln⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
          The mean and standard deviation of all CW measurements of <inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O
during the analysis period are 25 <inline-formula><mml:math id="M183" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 12 per meg (<inline-formula><mml:math id="M184" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M185" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 53). The subset of CW measurements with the most consistent CFA operations – and therefore the lowest variability for <inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O (<inline-formula><mml:math id="M187" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M188" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.06 ‰) – had corresponding <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O values of
25 <inline-formula><mml:math id="M190" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 6 per meg (<inline-formula><mml:math id="M191" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M192" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 36). Low variability among reference water
measurements gives confidence in the use of this system for this study of
replicate ice-core measurements.</p>
</sec>
<sec id="Ch1.S3.SS5">
  <label>3.5</label><?xmltex \opttitle{Processing CFA--CRDS $\Delta^{{17}}$O data}?><title>Processing CFA–CRDS <inline-formula><mml:math id="M193" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O data</title>
      <p id="d1e2691">After assigning approximate depth values and calibrating the <inline-formula><mml:math id="M194" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 Hz data, we discretize the CFA–CRDS data by binning the calibrated data
into prescribed depth intervals and averaging across the entire interval.
This enables a direct comparison between the continuous CFA–CRDS time series
and the discrete CRDS measurements. Small differences in the instantaneous
melt rate cause some variability in the data-averaging duration for each
reported measurement; the typical instantaneous melt rate was
<inline-formula><mml:math id="M195" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.3 cm min<inline-formula><mml:math id="M196" 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>, but rates ranged from <inline-formula><mml:math id="M197" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.1 to <inline-formula><mml:math id="M198" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.4 cm min<inline-formula><mml:math id="M199" 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 analysis. We report our CFA–CRDS
measurements with 1.39 cm resolution to match the resolution of our discrete
CRDS measurements. We also explore the effects of depth resolutions that
range from 0.5 to <inline-formula><mml:math id="M200" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 40 cm, given that increasing the
averaging window of the <inline-formula><mml:math id="M201" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 Hz spectroscopic measurements
reduces instrumental noise (e.g., Werle et al., 1993; Gkinis et al., 2010,
2011; Steig et al., 2014, 2021; Schauer et al., 2016; Jones et al., 2017a).</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Results and analysis</title>
      <p id="d1e2770">Our isotope measurements capture a period of approximately 2 years of
precipitation, as expected for a Greenland ice core from the depth we
analyzed (discussed in Sect. 3.2). The seasonal cycle of <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O
is shown in Fig. 4. We estimate that our depth assignments are accurate to
<inline-formula><mml:math id="M203" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 7 mm throughout the core by determining the variability in depth
assignments at all inflection points; this allows us to compare CFA–CRDS
measurements of <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O at the <inline-formula><mml:math id="M205" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> cm scale,
an appreciably finer resolution than has previously been reported. Our
comparison quantifies the reproducibility of our measurements and identifies
sources of variability among these CFA–CRDS <inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O data.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e2822">Comparison of discrete CRDS ice-core measurements (black) with
calibrated CFA–CRDS data averaged over 1.39 cm intervals (blue).
Corresponding <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M208" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> data are shown for seasonal context.
Discrete CRDS measurements are shown with the root mean square error of
corresponding reference water measurements (grey shading), and CFA–CRDS
measurements are shown as the mean of nine measurements with the standard
error (blue shading). Note that <inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M210" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> are reported in
‰ and that <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O is measured in per meg;
each vertical axis uses different scaling.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/15/7337/2022/amt-15-7337-2022-f04.png"/>

      </fig>

<?xmltex \hack{\newpage}?>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><?xmltex \opttitle{Seasonal $\Delta^{{17}}$O variations in replicated CFA and discrete measurements}?><title>Seasonal <inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O variations in replicated CFA and discrete measurements</title>
      <p id="d1e2900">We compare our CFA–CRDS data for <inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O with discrete CRDS
measurements to evaluate the CFA–CRDS method. We present the mean value and
standard error of all replicate measurements in Fig. 4 with 1.39 cm
averaging (representing approximately 270 s of data per interval for each
individual CFA–CRDS replicate); Fig. 4 also shows the discrete CRDS
measurements with the root mean square error of the corresponding discrete
reference water measurements. The mean of all CFA–CRDS measurements
(representing more than 2000 s of data per interval) is well correlated with
the discrete measurements (<inline-formula><mml:math id="M214" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M215" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.52, where 0.28 <inline-formula><mml:math id="M216" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M217" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M218" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 0.69 with 95 % confidence), especially in the upper 50 cm of the core (<inline-formula><mml:math id="M219" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M220" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.74, where 0.54 <inline-formula><mml:math id="M221" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M222" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M223" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 0.88 with 95 % confidence). Both the CFA–CRDS
data and the discrete CRDS data show clear seasonal <inline-formula><mml:math id="M224" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O
variations at this measurement resolution that are matched in magnitude and
timing.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><?xmltex \opttitle{Error attribution for CFA--CRDS $\Delta^{{17}}$O measurements}?><title>Error attribution for CFA–CRDS <inline-formula><mml:math id="M225" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O measurements</title>
      <p id="d1e3017">Next, we characterize the variability observed among our nine CFA–CRDS
measurements. In addition to the depth alignment errors discussed above,
sources of variability introduced by the CFA–CRDS method may include
high-frequency instrumental noise, calibration errors, and smoothing or bias
generated by mixing within the CFA system. High-frequency, high-amplitude
noise (<inline-formula><mml:math id="M226" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 1 ‰) in the uncalibrated CRDS
data is inherent to the instrument and can cause large aberrations from the
true value of <inline-formula><mml:math id="M227" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, especially over short averaging times; long
averaging times (<inline-formula><mml:math id="M228" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 1000 s) are typically used when measuring
<inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O by CFA–CRDS to minimize instrumental noise. Calibration
errors in <inline-formula><mml:math id="M230" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O occur when measurement treatment differs between
calibration standards and samples or between calibration standards; this can
cause fractionation to occur in the uncalibrated <inline-formula><mml:math id="M231" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and
<inline-formula><mml:math id="M232" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O measurements, leading to biased calibration slope and
intercept information. Despite efforts to stabilize vaporizer system
conditions prior to ice-core sample analysis and to measure ice-core samples
with the same treatment, it is likely that some calibration errors persist
in our ice-core data because it is not possible to measure the standards and
the sample at the same time. Finally, CFA measurement error for <inline-formula><mml:math id="M233" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O may result from mixing isotopically distinct waters during CFA
processing or from other processing issues that affect the internal
variability (i.e., perceived seasonality) of the continuous ice-core
measurement.</p>
      <p id="d1e3101">Typical CRDS characterization studies have used repeated measurements of
reference waters to identify measurement error; for this study, we instead
use repeated measurements of an ice core to characterize the sources of the
measurement error. By measuring reference waters, it is possible to
approximate the precision of the uncalibrated measurements by determining
the effect of averaging time on the intrinsic noise of the measurement; it
is also possible to quantify the variance of the calibrated, averaged data.
Our best data for CW were measured at 25 <inline-formula><mml:math id="M234" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 6 per meg, but without
additional information, it is not straightforward to identify whether the
error associated with this measurement is caused by instrumental
limitations, calibration bias, or other CFA processing effects. Our
replicate CFA–CRDS measurements provide an opportunity to identify the
source of CFA–CRDS errors because we can separately analyze the variability
internal to each time series (e.g., due to the seasonal cycle of <inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O or due to CFA errors) and the variability between the mean values
for each ice-core replicate (e.g., due to calibration offsets); further, we
can compare this variability with instrument expectations at different
averaging times</p>
      <p id="d1e3122">To isolate the error imparted by the calibration strategy, we processed the
data in two ways: first, we calibrated the data as described in Sect. 3.4, and
second, we set the mean values of all calibrated CFA measurements equal to
the mean value of the discrete CFA measurements in order to consider only
the variability internal to each measurement. Steig et al. (2021)
demonstrated that making a linear adjustment to the calibration intercept
for <inline-formula><mml:math id="M236" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O could reduce the noise of their
CFA–CRDS measurements for <inline-formula><mml:math id="M238" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in the SPC14 core. They
exploited additional reference water information taken before or after the
CFA measurement to define an adjusted calibration intercept value. Here, we
can instead use the mean value of the CFA–CRDS measurements themselves,
further eliminating uncertainty around this correction by setting the mean
of each calibrated CFA–CRDS time series equal to the mean value of our
discrete ice-core measurements; in this way, we are able to eliminate
offsets in calibration and examine the variability within each continuous
measurement. We define the calibration-adjusted <inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O data as
below:
            <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M240" display="block"><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">adjusted</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>n</mml:mi></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>n</mml:mi></mml:munderover><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">discrete</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>n</mml:mi></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>n</mml:mi></mml:munderover><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
          where the value of <inline-formula><mml:math id="M241" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>, which represents the number of data points per meter,
varies as a function of the depth resolution.</p>
      <p id="d1e3317">The calibration offset error is therefore <inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">adjusted</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>. Equivalently, <inline-formula><mml:math id="M243" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">adjusted</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> can be expressed in terms of <inline-formula><mml:math id="M244" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O
and <inline-formula><mml:math id="M245" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O using calibration correction information that is
based on the differences between average <inline-formula><mml:math id="M246" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M247" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O values for the discrete and continuous datasets. That is,
            <disp-formula id="Ch1.E6" content-type="numbered"><label>6</label><mml:math id="M248" display="block"><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">adjusted</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mi>ln⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msub><mml:mo>×</mml:mo><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">uncalibrated</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>b</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>b</mml:mi><mml:mrow><mml:mn mathvariant="normal">17</mml:mn><mml:mi mathvariant="italic">_</mml:mi><mml:mi mathvariant="normal">corr</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.528</mml:mn><mml:mi>ln⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msub><mml:mo>×</mml:mo><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mi mathvariant="normal">uncalibrated</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>b</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>b</mml:mi><mml:mrow><mml:mn mathvariant="normal">18</mml:mn><mml:mi mathvariant="italic">_</mml:mi><mml:mi mathvariant="normal">corr</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
          where the correction values <inline-formula><mml:math id="M249" display="inline"><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mrow><mml:mn mathvariant="normal">17</mml:mn><mml:mi mathvariant="italic">_</mml:mi><mml:mi mathvariant="normal">corr</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M250" display="inline"><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mrow><mml:mn mathvariant="normal">18</mml:mn><mml:mi mathvariant="italic">_</mml:mi><mml:mi mathvariant="normal">corr</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> are defined by the difference in mean <inline-formula><mml:math id="M251" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>
for CFA and discrete measurements. This calibration adjustment method is
analogous to that used in Steig et al. (2021).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e3600">Average <inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O with standard error and all CFA–CRDS
measurements, shown for three different depth resolutions. Dots and
blue error envelopes indicate <inline-formula><mml:math id="M253" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, and X symbols and red error envelopes indicate <inline-formula><mml:math id="M254" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">adjusted</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>.
All data are plotted at the upper depth of the depth interval that they
represent. Note that the upper panel is expanded such that all three
vertical scales are identical.</p></caption>
          <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://amt.copernicus.org/articles/15/7337/2022/amt-15-7337-2022-f05.png"/>

        </fig>

      <p id="d1e3662">Evaluating both <inline-formula><mml:math id="M255" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M256" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">adjusted</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> allows us to disentangle the calibration offset
error from other sources of measurement error. We discretized the CFA–CRDS
data to a series of depth-resolution schemes that ranged from 1.39 to
43.75 cm; the data are provided for three different depth resolutions in
Fig. 5. We calculated the standard error for all depth intervals across all
measurement resolutions.
The total error for the <inline-formula><mml:math id="M257" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and the error for the <inline-formula><mml:math id="M258" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">adjusted</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> are approximated by the blue and red lines in Fig. 6, respectively.
The region between the two solid lines is the fraction of the total error that can be attributed to the calibration offset. Figures 5 and 6 indicate that the calibration offset noise is essentially indistinguishable from the
instrumental noise at short averaging times, so the calibration offset
adjustment does little to improve the measurement for the best-resolved
data. The results show that the total error is <inline-formula><mml:math id="M259" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 10 per meg for all
data. The total error is <inline-formula><mml:math id="M260" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 5 per meg at averaging times longer
than <inline-formula><mml:math id="M261" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 3000 s, which corresponds to depth averages of
<inline-formula><mml:math id="M262" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 15 cm at the melt rates we used. Figure 6 also shows that
the error that arises from differences in internal variability (i.e., the
CFA error) for the CFA–CRDS data is <inline-formula><mml:math id="M263" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 2 per meg by <inline-formula><mml:math id="M264" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 3000 s and that the total error is dominated by calibration offset error
at long averaging times.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F6"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e3794">Standard error of all replicate CFA measurements as a function of
measurement integration depth. The blue line shows the mean of the standard
error of <inline-formula><mml:math id="M265" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> as calculated for each depth interval; the shaded blue area indicates the minimum and maximum values of the standard error across all depth intervals. The red line and shaded area show the relationship between the standard error in <inline-formula><mml:math id="M266" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">adjusted</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and the measurement resolution. The area beneath the total error line is highlighted to indicate error attribution.</p></caption>
          <?xmltex \igopts{width=213.395669pt}?><graphic xlink:href="https://amt.copernicus.org/articles/15/7337/2022/amt-15-7337-2022-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e3848">Comparison of Allan deviation of continuous reference water
measurements and standard deviation of nine duplicate CFA ice-core
measurements. In both panels <bold>(a)</bold> and <bold>(b)</bold>, the Allan deviation line (solid grey) for a long measurement of SW2 is overlain by the standard deviation of the CFA–CRDS ice-core measurements (crosses) and the mean of the standard deviations for each integration time (dashed line). The <inline-formula><mml:math id="M267" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M268" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">adjusted</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>
data are shown in blue and red similarly to Figs. 5 and 6. The standard
deviation on the left is calculated from calibrated replicate CFA–CRDS
measurements and shows the total variability between CFA–CRDS replications
along the depth of the core. The standard deviation information in the right
plot is calculated from calibration-adjusted datasets so that the effect of
the calibration offset error is removed; this analysis is still dependent
upon instrumental noise, CFA errors, depth registration errors, and natural
variability within the core.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/15/7337/2022/amt-15-7337-2022-f07.png"/>

        </fig>

      <p id="d1e3905">Finally, we directly compare the variability of our CFA–CRDS data with the
variability of reference waters measured by CFA–CRDS, which is determined by
an Allan variance analysis. An Allan variance analysis quantifies the
relationship between signal noise and integration time (Allan, 1966; Werle
et al., 1993); for CRDS data, this analysis of reference water measurements
is commonly used to approximate the measurement precision of the system for
any given measurement duration (Gkinis et al., 2010; Steig et al., 2014). We
determine the Allan deviation (square root of the Allan variance) from a
long continuous analysis (<inline-formula><mml:math id="M269" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 8.5 h) of the SW2 reference
water made during our analysis window (see Table 2); the result is shown in
Fig. 7. Differences between the Allan deviation and the standard deviation
of our measurements should confirm whether the magnitude and timing of the
variability are as precise as during reference water measurements, or if
there are other changes imparted by the CFA system or calibration that may
degrade CFA–CRDS data quality. We find the standard deviation <inline-formula><mml:math id="M270" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mi mathvariant="normal">_</mml:mi><mml:mi mathvariant="normal">CFA</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> among all nine <inline-formula><mml:math id="M271" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> datasets averaged over integration windows
that vary from 5 mm to 43.75 cm. This analysis compares the variability of
the final, calibrated measurements along the depth of the core sample with
the variability of the reference water measurement, and ultimately
quantifies the reproducibility of our CFA–CRDS measurements. We track the
analysis time associated with each averaging interval and overlay the
measured <inline-formula><mml:math id="M272" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mi mathvariant="normal">_</mml:mi><mml:mi mathvariant="normal">CFA</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> with the corresponding mean integration time for each depth interval on Fig. 7a.</p>
      <p id="d1e3988">Figure 7a shows generally good agreement between <inline-formula><mml:math id="M273" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mi mathvariant="normal">_</mml:mi><mml:mi mathvariant="normal">CFA</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M274" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">Allan</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> at integration times less than 400 s, but the <inline-formula><mml:math id="M275" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mi mathvariant="normal">_</mml:mi><mml:mi mathvariant="normal">CFA</mml:mi><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> data asymptotically
approach a limit of 10 per meg at longer averaging times instead of
following the stability trend expected by the Allan variance analysis. To
evaluate to what extent this mismatch between expected and observed <inline-formula><mml:math id="M276" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> can be attributed to errors arising from the calibration offset (as shown
in Fig. 6), we repeat this analysis for the <inline-formula><mml:math id="M277" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">adjusted</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">CFA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> data. Figure 7b shows excellent agreement between <inline-formula><mml:math id="M278" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">adusted</mml:mi><mml:mi mathvariant="normal">_</mml:mi><mml:mi mathvariant="normal">CFA</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M279" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">Allan</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>at all integration times; this demonstrates that the drift in
<inline-formula><mml:math id="M280" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">calibrated</mml:mi><mml:mi mathvariant="normal">_</mml:mi><mml:mi mathvariant="normal">CFA</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> shown in Fig. 7a can
be entirely attributed to calibration effects and not to the CFA process
directly. Figure 7 suggests that reducing the error of calibrated CFA–CRDS
measurements is not limited by the CFA process – nor by the
CRDS instrument – but rather by the quality of the calibration information,
which depends on the treatment and frequency of reference water
measurements.</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Discussion and conclusions</title>
<sec id="Ch1.S5.SS1">
  <label>5.1</label><?xmltex \opttitle{Comparison of CFA--CRDS $\Delta^{{17}}$O measurements with other $\Delta^{{17}}$O measurements from Greenland}?><title>Comparison of CFA–CRDS <inline-formula><mml:math id="M281" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O measurements with other <inline-formula><mml:math id="M282" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O measurements from Greenland</title>
      <p id="d1e4206">Our work complements previous studies that have examined the seasonal cycle
of <inline-formula><mml:math id="M283" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in the polar regions, and good agreement with earlier work
validates our measurements. Consistent with previous measurements from
Greenland, the <inline-formula><mml:math id="M284" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O signal in our data is anticorrelated with
<inline-formula><mml:math id="M285" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> and anticorrelated with the seasonal cycle in <inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O (Landais et
al., 2008). The measurements presented here were made from a core that
represents approximately 2 years of ice accumulation from the 1760s
(Hastings et al., 2009). The measured magnitude (peak to trough) of the
seasonal cycle in <inline-formula><mml:math id="M287" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O is <inline-formula><mml:math id="M288" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 45 per meg at 1.39 cm
resolution in our data (Fig. 4), which is in excellent agreement with the
magnitude of the seasonal cycle reported previously for Greenland.
Specifically, Landais et al. (2012b) reported seasonal magnitudes of
<inline-formula><mml:math id="M289" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 25 per meg from a shallow firn core at NEEM (in northwestern
Greenland) that represented accumulation periods between 1962–1963 and
between 2003–2005; when we coarsen our measurement resolution to 3.6 cm –
which approximates the <inline-formula><mml:math id="M290" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> monthly (5 cm) measurement resolution
in the NEEM core (detailed in Steen-Larsen et al., 2011) – the magnitude of
the seasonal cycle in our data is <inline-formula><mml:math id="M291" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 per meg. Low errors
between replicate values and the good agreement with previous studies
strengthen confidence in the CFA–CRDS approach for high-resolution <inline-formula><mml:math id="M292" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O.</p>
      <p id="d1e4300">Our results reinforce the use of the CFA–CRDS method for high-precision,
high-resolution measurements of <inline-formula><mml:math id="M293" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in ice cores. CFA–CRDS
methods are valuable for detecting detail in <inline-formula><mml:math id="M294" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O variations in
deep ice layers, for measuring <inline-formula><mml:math id="M295" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in ice from sites with low
accumulation rates, or for measuring <inline-formula><mml:math id="M296" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in any glacial ice
where high depth resolution is desired.</p>
</sec>
<sec id="Ch1.S5.SS2">
  <label>5.2</label><?xmltex \opttitle{Addressing CFA--CRDS calibration errors in $\Delta^{{17}}$O}?><title>Addressing CFA–CRDS calibration errors in <inline-formula><mml:math id="M297" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O</title>
      <p id="d1e4367">Because the error of all <inline-formula><mml:math id="M298" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O measurements by CRDS depends on
the calibration, the importance of establishing a robust calibration
strategy for CFA–CRDS cannot be understated. We iteratively revised our
CFA–CRDS system and designed our calibration strategy as recommended below.</p>
      <p id="d1e4381">First, the CFA–CRDS configuration must be capable of stable operations that
span the total duration of the ice-core and reference water measurements.
System stability for a given CFA system should be characterized with an
Allan variance analysis. We have chosen to measure calibration standards
immediately before and after ice-core measurements to improve the likelihood
of measuring the calibration standard under the same system conditions as
the ice-core sample. Additionally, limiting system memory and reducing the
transition time between reference waters maximize the useful fraction of
reference water data, allowing measurements of longer duration or
measurements of more reference waters to be made within a period of
consistent CFA operations.</p>
      <p id="d1e4384">Next, quantifying the drift in calibration information over time can allow
an operator to determine the physical controls on fractionation within a
CFA–CRDS system. The change in calibration information can be used to inform
system maintenance schedules or operational sequences. For example, we have
observed that after operating our CFA–CRDS system for several weeks, the
fractionation responses for <inline-formula><mml:math id="M299" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M300" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O diverge,
degrading the quality of calibration data for <inline-formula><mml:math id="M301" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O. Cleaning
the vaporizer fittings appears to “reset” the calibration response,
suggesting that the fractionation that occurs over long timescales is a
result of physical effects within the vaporizer itself, likely owing to visible
precipitate formation.</p>
      <p id="d1e4421">Though our system is capable of high-precision measurements for <inline-formula><mml:math id="M302" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, our analysis suggests that calibration bias persists in our data, which is unsurprising when considering previously published work on similar methods. The largest offsets (shown in Table 2) were associated with poor CFA stability due to a dirty vaporizer chamber. Large errors in <inline-formula><mml:math id="M303" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O were occasionally observed during the analysis of the South Pole
ice core (SPC14); Steig et al. (2021) attributed these errors to calibration
differences and performed a correction by shifting the mean value of their
measurements based on the offset identified by a calibrated reference water
measurement, similarly to Eq. (6). Our work supports the attribution of
these errors to the calibration, and it also supports the calibration
adjustment method. We recommend the use of additional reference water
measurements to account for calibration offsets in <inline-formula><mml:math id="M304" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, and we
also recommend that CFA systems are designed to ensure complete vaporization
with flow conditions that are stable over long timescales. In our vaporizer,
we observe that precipitate coatings can change the geometry of the
vaporizer chamber and lead to incomplete vaporization over time, which
degrades the quality of the calibration over time. When there is clear
evidence of inconsistent vaporization (as in Fig. 3), we observe large
calibration errors in <inline-formula><mml:math id="M305" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O by this method (tens to hundreds of
per meg). Such issues likely also influence the vaporization process in
other CFA systems, though they will not be readily detected in measurements
of <inline-formula><mml:math id="M306" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O or <inline-formula><mml:math id="M307" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>D if the water vapor has homogenized before
reaching the analyzer.</p>
      <p id="d1e4487">Finally, though it is perhaps impractical to measure replicate ice-core
samples as we have done here, the average of our nine CFA–CRDS measurements
shows that, like dual-inlet IRMS operations, stacking the CFA–CRDS data
effectively averages over calibration inconsistencies. The results are
comparable to highly resolved discrete CRDS or IRMS measurements. While
CFA–CRDS measurements resolved to the centimeter scale still require long
measurement times to achieve precise <inline-formula><mml:math id="M308" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O data (<inline-formula><mml:math id="M309" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 1000 s for 10 per meg precision), stacking CFA–CRDS measurements is an
effective way to increase analysis time. Typically, achieving long
measurement times while maintaining high depth resolution necessitates a
reduction of melt rates. In practice, reduced melt rates may be incompatible
with other measurement goals (such as trace gases) during an ice-core
measurement campaign; reduced melt rates may also prevent the measurement of
both ice-core samples and calibration standards within a period of stable
system operations. We show that stacking multiple CFA–CRDS measurements
provides a viable alternative strategy; stacking replicate CFA–CRDS
measurements improves the accuracy of the measurement by averaging over the
calibration offset noise, and it improves the measurement precision or
measurement resolution by increasing the total analysis time for a given
depth interval.</p>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Summary</title>
      <p id="d1e4517">We measured <inline-formula><mml:math id="M310" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in nine replicate ice-core samples using a
continuous-flow analysis (CFA) system combined with a cavity-ring down laser
spectrometer (CRDS). We measured a 10th replicate sample by discrete CRDS
methods. We show that CFA–CRDS can reliably capture centimeter-scale variability of
<inline-formula><mml:math id="M311" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in ice-core samples; we identified seasonal fluctuations of
<inline-formula><mml:math id="M312" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 45 per meg in <inline-formula><mml:math id="M313" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O from an ice core
representing the preindustrial period in Greenland that agree with the
discrete CRDS data and also with previously published measurements of
seasonal <inline-formula><mml:math id="M314" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O variability in Greenland.</p>
      <p id="d1e4571">Our work shows that using CFA–CRDS methods can be valuable when
high-precision and highly resolved measurements are desired. Our results
show that mixing within the CFA system does not jeopardize CFA–CRDS
measurements of <inline-formula><mml:math id="M315" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, even at centimeter-scale resolution. The mean of
our stacked measurements exhibits neither a time lag nor any amplitude
smoothing in comparison to the discretely prepared CRDS measurements.
Rather, we show that the total error (<inline-formula><mml:math id="M316" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 5 per meg for analysis
times <inline-formula><mml:math id="M317" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 3000 s) is dominated by calibration bias. We note the
importance of developing robust calibration strategies for <inline-formula><mml:math id="M318" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O
when making measurements by CFA–CRDS, but we demonstrate that when
calibration is accounted for, CFA–CRDS for <inline-formula><mml:math id="M319" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O is highly
reproducible and can be tailored for high-resolution and high-precision
measurements.</p>
</sec>

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

      <p id="d1e4625">Data generated for this study are available from the corresponding author upon reasonable request.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e4631">EJS, AJS, and LD conceived of the study. LD developed the measurement method, made the measurements, and completed the analysis with the support of AJS and EJS. All authors contributed to the paper.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e4637">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e4643">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e4649">This work was partially funded by the Hercules Dome Ice Core project and the Center for Oldest Ice Exploration. We are grateful
to the two anonymous reviewers for their thoughtful improvements to this
paper. Finally, making continuous measurements during the COVID-19
pandemic would not have been possible without the support of University of
Washington undergraduate students Jacob Childers and Shana Edouard, who
assisted with system maintenance and measurements.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e4654">This research has been supported by the National Science Foundation (grant nos. 1841844 and 2019719).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e4660">This paper was edited by Christof Janssen and reviewed by two anonymous referees.</p>
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