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  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">AMT</journal-id>
<journal-title-group>
<journal-title>Atmospheric Measurement Techniques</journal-title>
<abbrev-journal-title abbrev-type="publisher">AMT</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Meas. Tech.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1867-8548</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/amt-9-3879-2016</article-id><title-group><article-title>Intercomparison of two cavity ring-down spectroscopy analyzers for
atmospheric <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurement</article-title>
      </title-group><?xmltex \runningtitle{Intercomparison of two cavity ring-down spectroscopy analyzers}?><?xmltex \runningauthor{J.~Pang et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Pang</surname><given-names>Jiaping</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Wen</surname><given-names>Xuefa</given-names></name>
          <email>wenxf@igsnrr.ac.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Sun</surname><given-names>Xiaomin</given-names></name>
          <email>sunxm@igsnrr.ac.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Huang</surname><given-names>Kuan</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Key Laboratory of Ecosystem Network Observation and Modeling,
Institute of Geographic Sciences <?xmltex \hack{\newline}?> and Natural Resources Research, Chinese
Academy of Sciences, Beijing 100101, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>University of Chinese Academy of Sciences, Beijing 100049, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Picarro, Inc., Santa Clara, California 95054, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Xuefa Wen (wenxf@igsnrr.ac.cn) and Xiaomin Sun (sunxm@igsnrr.ac.cn)</corresp></author-notes><pub-date><day>22</day><month>August</month><year>2016</year></pub-date>
      
      <volume>9</volume>
      <issue>8</issue>
      <fpage>3879</fpage><lpage>3891</lpage>
      <history>
        <date date-type="received"><day>22</day><month>March</month><year>2016</year></date>
           <date date-type="rev-request"><day>25</day><month>April</month><year>2016</year></date>
           <date date-type="rev-recd"><day>28</day><month>July</month><year>2016</year></date>
           <date date-type="accepted"><day>31</day><month>July</month><year>2016</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016.html">This article is available from https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016.html</self-uri>
<self-uri xlink:href="https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016.pdf">The full text article is available as a PDF file from https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016.pdf</self-uri>


      <abstract>
    <p>Isotope ratio infrared spectroscopy (IRIS) permits continuous in situ
measurement of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> isotopic composition under ambient conditions.
Previous studies have mainly focused on single IRIS instrument performance;
few studies have considered the comparability among different IRIS
instruments. In this study, we carried out laboratory and ambient
measurements using two Picarro CO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C analyzers (G1101-i and
G2201-i (newer version)) and evaluated their performance and comparability.
The best precision was 0.08–0.15 ‰ for
G1101-i and 0.01–0.04 ‰ for G2201-i. The dependence of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
on CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration was 0.46 ‰ per 100 ppm and
0.09 ‰ per 100 ppm, the instrument drift ranged from
0.92–1.09 ‰ and 0.19–0.37 ‰, and the sensitivity of
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C to the water vapor mixing ratio was
1.01 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O  and 0.09 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O for
G1101-i and G2201-i, respectively. The accuracy after correction by the
two-point mixing ratio gain and offset calibration method ranged from
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.04–0.09 ‰ for G1101-i and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.13–0.03 ‰ for
G2201-i. The sensitivity of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C to the water vapor mixing ratio
improved from 1.01 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O before the upgrade of
G1101-i (G1101-i-original) to 0.15 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O after the
upgrade of G1101-i (G1101-i-upgraded). Atmospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measured by
G1101-i and G2201-i captured the rapid changes in atmospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
signals on hourly to diurnal cycle scales, with a difference of
0.07 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.24 ‰ between G1101-i-original and G2201-i and
0.05 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.30 ‰ between G1101-i-upgraded and G2201-i. A
significant linear correlation was observed between the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
difference of G1101-i-original and G2201-i and the water vapor concentration,
but there was no significant correlation between the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
difference of G1101-i-upgraded and G2201-i and the water vapor concentration.
The difference in the Keeling intercept values decreased from 1.24 ‰
between G1101-i-original and G2201-i to 0.36 ‰ between
G1101-i-upgraded and G2201-i, which indicates the importance of consistency
among different IRIS instruments.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>The development of stable isotope analyzers and measurement techniques has made
stable isotope analysis a powerful tool for gaining insight into the
underlying mechanisms of carbon and water cycling in atmospheric, ecological,
and hydrological studies (Yakir and Sternberg, 2000; Bowling et al., 2003;
Griffis, 2013). Isotope ratio infrared spectroscopy (IRIS) permits in situ
and continuous isotope measurements under ambient conditions and overcomes
the shortcoming of traditional isotope ratio mass spectrometers (IRMS), which
involve relatively labor-intensive sample collection and preparation (Bowling
et al., 2005; Schaeffer et al., 2008; Wingate et al., 2010; Griffith et al.,
2012; Werner et al., 2012; Griffis, 2013). To date, various IRIS techniques
are commercially available for measuring stable carbon isotopes, including
lead-salt tunable diode laser absorption spectrometry (TDLAS, Campbell
Scientific Inc.), wavelength-scanned cavity ring-down spectroscopy (WS-CRDS,
Picarro Inc.), off-axis cavity output spectroscopy (OA-ICOS, Los Gatos
Research), quantum cascade laser absorption spectrometry (QCLAS, Aerodyne
Research), and difference frequency generation laser spectroscopy (DFG,
Thermo Scientific; Griffis, 2013; Wen et al., 2012, 2013). All the
data monitored by IRIS analyzers should capture the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C variations of
atmospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with high precision under ambient conditions and should
be traceable to the standard Vienna Pee Dee Belemnite (VPDB) scale (Bowling
et al., 2005; Schaeffer et al., 2008; Griffis, 2013). To assess the data
comparability of different experiments, it is important to conduct an
intercomparison of different IRIS instruments to ensure their
compatibility (Flowers et al., 2012; Griffith et al., 2012; Wen et al.,
2013).</p>
      <p>Previous studies have shown that temperature dependence, concentration
dependence, and spectroscopic interference are among the major sources of
errors for IRIS measurements (Griffith et al., 2012; Guillon et al., 2012;
Vogel et al., 2013; Wen et al., 2013). Instrument long-term drift is another
source of errors affecting IRIS performance (Rella et al., 2013; Vogel et al.,
2013). Most previous studies focus on the methodology of a single IRIS
instrument (Bowling et al., 2003; Wahl et al., 2006; Tuzson et al., 2008;
Griffith et al., 2012; Guillon et al., 2012; Vogel et al., 2013). It is
important to obtain precise and accurate measurements that are traceable to
the international VPDB standard by improving measurement precision and by
constructing a proper calibration strategy. Previous laboratory and field
experiments showed precision of IRIS instruments ranging from
0.02  to 0.25 ‰ for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C (Bowling et al., 2003; Wahl et al., 2006; Schaeffer et al., 2008; Tuzson et
al., 2008; Griffith et al., 2012; Guillon et al., 2012; Sturm et al., 2012;
Vogel et al., 2013; Wen et al., 2013). Because of the nonlinear response of
the concentration dependence of IRIS instruments, it is recommended that
more than two standard gases with different CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations be used
for the <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> calibration to eliminate the
nonlinear response of the instruments (Bowling et al., 2005; Schaeffer et
al., 2008; Tuzson et al., 2008). The accuracy of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C is 0.01 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.03 ‰ for the three-point linear calibration and
0.00 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.01 ‰ for the four-point linear calibration (Bowling et al., 2005). Setting the proper calibration frequency according
to the stability of the instrument can eliminate the drift and the
environmental sensitivity of the instruments (Griffis, 2013; Wen et al.,
2013).</p>
      <p>System bias among different IRIS instrument measurements would result in
poor measurement comparability (Flowers et al., 2012; Hammer et al., 2013;
Griffis, 2013; Wen et al., 2013). Bowling et al. (2003) found a consistent
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C offset of 1.77 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.35 ‰ between
the TDLAS and flask-IRMS measurement (<inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 82) that was caused by pressure
broadening. Schaeffer et al. (2008) compared the TDLAS and portable flask
package sampling-IRMS measurement and observed a difference of 0.01 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.45 ‰ (<inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 277) for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C. Tuzson et al. (2008) found a difference between QCLAS and flask-IRMS measurement of
0.28–2 ‰ that was probably caused by
nonlinearity of the QCL instrument at elevated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations and
laser intensity variation. Note that an ideal IRIS instrument should be free
of nonlinear absorption or concentration dependence effects, meaning that
its measurements should not change with the changing CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations
at a constant isotopic composition. Mohn et al. (2008) observed a mean
difference of 0.4 ‰ (<inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 81) between Fourier transform infrared spectroscopy (FTIR) and flask-IRMS
measurements. Considering the time resolution difference between IRIS and
IRMS sampling technology, a clear difference was observed when rapid changes
in the atmospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration occurred (Schaeffer et al., 2008).
Mohn et al. (2008) used the Keeling plot method to eliminate the difference
in the sampling time resolution between IRMS and FTIR. The difference of
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">R</mml:mi></mml:msub></mml:math></inline-formula> obtained by this method was insignificant (<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>28.1 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.4  and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>27.9 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.5 ‰).
Very few studies have compared IRIS instruments (Griffis, 2013; Wen et
al., 2013); only Wen et al. (2013) compared two commercially available IRIS
instruments, Los Gatos DLT-100 and Picarro G1101-i, which had excellent
agreement over a 7-day atmospheric measurement period, with a difference of
only <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.02 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.18 ‰ after proper calibration.
However, there was still a slight correlation of the difference between the
two analyzers with concentration. This slight concentration dependence
resulted in a much larger difference (2.44 ‰) for the
Keeling intercept by propagating through the Keeling analysis.</p>
      <p>The objective of this study is to evaluate the performance and comparability
of two Picarro CO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C analyzers based on CRDS
technology (G1101-i and G2201-i). We aim to (1) determine the optimal
precision of both analyzers by Allan deviation; (2) test the dependence of
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C on CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration, drift, and accuracy using a
gradient switching experiment; (3) identify the sensitivity of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C to the water vapor mixing ratio using a dew point generator; and
(4) examine the compatibility of G1101-i and G2201-i using atmospheric
CO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measurements. The laboratory and atmospheric measurements data are available
at <uri>https://www.researchgate.net/publication/301644542_Inter-comparison_of_two_cavity_ring-down_spectroscopy_analyzers_for_atmospheric_13CO2_12CO2_measurement</uri>.</p>
</sec>
<sec id="Ch1.S2">
  <title>Materials and methods</title>
<sec id="Ch1.S2.SS1">
  <title>Analyzers, sampling, and calibration systems</title>
      <p>In this study, the inlets of two CO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C analyzers of
Picarro Inc., Sunnyvale, CA, G1101-i (manufactured in 2010) and G2201-i (manufactured in 2014), were connected in parallel and then connected with
three three-way solenoid valves, which constitutes the sampling and
calibration system with one ambient air inlet and three calibration gas
inlets (Fig. 1). The switch sequence of valves was controlled by the valve
sequencer software on the G2201-i analyzer. The built-in pressure and
temperature monitoring systems of G1101-i and G2201-i maintained the cavity
temperature of both systems at 45 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and the cavity pressures at
140  and 148 Torr, respectively. The observed stability of temperature
over 24 h was 45.0 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.0024  and 45.0 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.0005 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and the
observed stability of pressure was 140.0429 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.0580  and 147.9990 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.0165 Torr for G1101-i and G2201-i,
respectively. No relationship between temperature and pressure variation and
the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C difference of either instrument was found. A diaphragm
pump was used to pump the sample air and calibration gas continuously to the
cavity (volume of 35 mL) at a flow rate of 0.03 L min<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> at standard
temperature and pressure (STP); measurement frequencies were approximately
0.3 and 1 Hz for G1101-i and G2201-i, respectively. Note that the turnover
time of sample air in the analyzer is not fast enough for 0.3  and 1 Hz
data to be meaningful. In this study, the data reported were block-averaged
to average time intervals after deleting the data collected during
transitional periods in response to valve switching between the two sample
intakes. The physical laser arrays and the software of the G1101-i analyzer
were upgraded in March 2012 and August 2014 to correct the cross-interference caused by CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and water vapor, respectively. In the
following laboratory and atmospheric measurements, the water vapor
sensitivity test and atmospheric measurements were done before the upgrade
of G1101-i (G1101-i-original) and after the upgrade of G1101-i (G1101-i-upgraded) in August 2014.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Schematic setup of the laboratory and ambient measurements of two
Picarro CO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C analyzers.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016-f01.png"/>

        </fig>

      <p>The sample air stream passed through a filter (pore size 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m, Swagelok
model B-4F-05, Connecticut Valves and Fittings, Norwalk Connecticut) to the
analyzers without being dried. In this study, only the water vapor dilution
effect was corrected, without considering the water vapor pressure
broadening effect and the spectral interference effect (Wen et al., 2013).
Data from the transitional periods, i.e., the first 180 s of each sample
measurement cycle after valve switching, were discarded. The transitional
periods in response to valve switching between two air sample intakes were
about 120 s.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Laboratory measurement</title>
      <p>Three reference gases (Ref1, Ref2, and Ref3) were produced by Beijing AP
BAIF Gases Industry Co., Ltd, with CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios of 368.1, 451.7,
and 550.1 ppm. The <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values were measured using an isotope
ratio mass spectrometer (Thermo Finnigan MAT 253) at the Key Laboratory of
Ecosystem Network Observation and Modeling, Institute of Geographic Sciences
and Natural Resources Research, Chinese Academy of Sciences. Because the
three reference gases originated from the same gas source, the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.38 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.06 ‰ for all three
reference gases.</p>
<sec id="Ch1.S2.SS2.SSS1">
  <title>Allan variance test</title>
      <p>Allan variance (Allan, 1987; Werle et al., 1993) is commonly used to express
measurement precision and stability as a function of average time. Here
Ref1, Ref2, and Ref3 were connected to the sampling and calibration systems
and were each measured for 24 h to conduct the Allan variance analysis for
G1101-i-original and G2201-i.</p>
</sec>
<sec id="Ch1.S2.SS2.SSS2">
  <title>Gradient switching test</title>
      <p>Ref1, Ref2, and Ref3 were connected to the sampling and calibration system
and switched sequentially every 40 min for a total of 48 h. Two of the
three reference gases were treated as calibration gases and the third was treated
as the target gas. The two-point mixing ratio gain and offset calibration
strategy (Bowling et al., 2003; Wen et al., 2013) was used for each 120 min
measurement cycle. The measured data and calibrated data were used to
evaluate the dependence of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C on CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration, and
long-term drift as well as the accuracy of both the G1101-i-original and
G2201-i analyzers.</p>
</sec>
<sec id="Ch1.S2.SS2.SSS3">
  <title>Water vapor sensitivity test</title>
      <p>The water vapor sensitivity of both analyzers was tested by connecting the
reference gas (Ref1) to a dew point generator (model LI-610, Li-Cor, Inc.,
Lincoln, NE, USA). The reference gas (Ref1) bubbled through the reservoir of
the dew point generator to produce different humidity levels by setting
different dew point temperatures. The dissolution of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the
reservoir (25–30 mL) of the dew point generator moved quickly into a dynamic
equilibrium state because of the carbonate chemistry in solution at
different dew point temperatures, which did not change the true <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C signal because of lasting bubbled processes. The first test was
conducted in June 2014 for both G1101-i-original and G2201-i analyzers; the
dew point temperatures were 5.0, 10.0, 15.0, 20.0, and 25.0 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C,
and the corresponding water vapor ranged from 0.87 to 3.15 %. The
second test was conducted in December 2014 for the G1101-i-upgraded and
G2201-i analyzers; the dew point temperatures were 1.0, 5.0, 10.0, 15.0, and
20.0 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and the corresponding water vapor ranged from 0.65
to 2.32 %. Reference gas at each humidity level was measured for 20 min a
total of three times.</p><?xmltex \hack{\newpage}?>
</sec>
</sec>
<sec id="Ch1.S2.SS3">
  <title>Atmospheric measurement</title>
      <p>The air sample inlet was located outside the Key Laboratory of Ecosystem
Network Observation and Modeling, 10 m above the ground (Wen et al., 2008,
2010, 2012, 2013). The first atmospheric measurement dataset was collected,
for both the G1101-i-original and G2201-i analyzers, from 15 June 2015 to
23 June 2015 (DOY 164–174), and the second dataset was
collected, for both G1101-i-upgraded and G2201-i analyzers, from 14 December to 22 December 2014 (DOY 348–356). The first
atmospheric measurement sampled Ref1 and Ref3 for 10 min each, followed by
alternate measurements of ambient air (50 min) and Ref2 (10 min) for 5 h.
The total duration of the sampling and calibration cycle was 320 min. The
second atmospheric measurement sampled Ref1, Ref2, and Ref3 for 10 min each,
followed by ambient air measurement for 300 min, i.e., a total duration of
330 min for each sampling and calibration cycle. The atmospheric sample and
Ref2 were calibrated by Ref1 and Ref3 for each measurement cycle, and the
calibrated atmospheric sample data were used to obtain hourly mean values.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <title>Calibration procedures</title>
      <p>The two-point mixing ratio gain and offset calibration method (Bowling et
al., 2003) was used to calibrate the <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
mixing ratio measured by G1101-i and G2201-i. Additional details about the
calibration method can be found in Wen et al. (2013). Following this method,
the calibrated mixing ratios of <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>x</mml:mi><mml:mn>12</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>x</mml:mi><mml:mn>13</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> are calculated as
            <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mi mathvariant="normal">a</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">t</mml:mi></mml:mrow><mml:mn>12</mml:mn></mml:msubsup><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">t</mml:mi></mml:mrow><mml:mn>12</mml:mn></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">t</mml:mi></mml:mrow><mml:mn>12</mml:mn></mml:msubsup></mml:mrow><mml:mrow><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">m</mml:mi></mml:mrow><mml:mn>12</mml:mn></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">m</mml:mi></mml:mrow><mml:mn>12</mml:mn></mml:msubsup></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced close=")" open="("><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mi mathvariant="normal">a</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">m</mml:mi></mml:mrow><mml:mn>12</mml:mn></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">m</mml:mi></mml:mrow><mml:mn>12</mml:mn></mml:msubsup></mml:mfenced><mml:mo>+</mml:mo><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">t</mml:mi></mml:mrow><mml:mn>12</mml:mn></mml:msubsup></mml:mrow></mml:math></disp-formula>

            <disp-formula id="Ch1.E2" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mi mathvariant="normal">a</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">t</mml:mi></mml:mrow><mml:mn>13</mml:mn></mml:msubsup><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">t</mml:mi></mml:mrow><mml:mn>13</mml:mn></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">t</mml:mi></mml:mrow><mml:mn>13</mml:mn></mml:msubsup></mml:mrow><mml:mrow><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">m</mml:mi></mml:mrow><mml:mn>13</mml:mn></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">m</mml:mi></mml:mrow><mml:mn>13</mml:mn></mml:msubsup></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced open="(" close=")"><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mi mathvariant="normal">a</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">m</mml:mi></mml:mrow><mml:mn>13</mml:mn></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">m</mml:mi></mml:mrow><mml:mn>13</mml:mn></mml:msubsup></mml:mfenced><mml:mo>+</mml:mo><mml:msubsup><mml:mi>x</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">t</mml:mi></mml:mrow><mml:mn>13</mml:mn></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where m and t represent the measured and true mixing ratios, and the
subscripts 1, 3, and a represent Ref1, Ref3, and ambient air, respectively.</p>
      <p>The isotopic composition of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the ambient air is expressed in the
delta notation:
            <disp-formula id="Ch1.E3" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup><mml:mi>C</mml:mi><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">sample</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">VPDB</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo><mml:mo>×</mml:mo><mml:mn>1000</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">sample</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>C <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>C ratio of the sample, and
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">VPDB</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>C <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>C ratio of the reference standard (i.e.,
the VPDB).</p><?xmltex \hack{\newpage}?><?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p>Allan deviation of the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C at endpoint for
the <bold>(a)</bold> G1101-i before upgradation (G1101-i-original) and <bold>(b)</bold> G2201-i analyzers with
three different CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations with same <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C standard
gases.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016-f02.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results</title>
<sec id="Ch1.S3.SS1">
  <title>Precision</title>
      <p>Figure 2 shows the Allan variance (Allan, 1987) as a function of the average
time of the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measurements for Ref1, Ref2, and Ref3 measured
by G1101-i-original and G2201-i. If the Allan variance is dominated by the
random white (Gaussian) noise, the Allan variance should decrease linearly
with average time, and the precision should increase with the average time.
However, for longer average times, the precision worsens because of
instrumental drift. In addition, the precision should increase with
increasing CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations because of high signal-to-noise ratio.
The <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C precision improved with the average time and achieved
optimum values of 0.08, 0.15, and 0.10 ‰ for
G1101-i-original at 7600, 1900, and 1900 s for Ref1, Ref2 and Ref3,
respectively and 0.03, 0.04, and 0.01 ‰ for G2201-i at
7600, 3800, and 7600 s for the three reference gases, respectively. The
5 min precision was 0.24–0.34 ‰ and
0.08–0.12 ‰ for G1101-i-original and G2201-i,
respectively (Table 1).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>Measurement precision (Allan deviation for 1 min, 5 min and
optimum averaging times) from three reference gases (Ref1, Ref2 and Ref3) with
0.3 and 1 Hz sampling rate for the Picarro G1101-i before
upgradation (G1101-i-original) and G2201-i analyzers.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="8">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right" colsep="1"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry namest="col1" nameend="col2"/>  
         <oasis:entry rowsep="1" namest="col3" nameend="col8" align="center">Averaging time </oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Species</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry rowsep="1" namest="col3" nameend="col5" align="center">G2201-i </oasis:entry>  
         <oasis:entry rowsep="1" namest="col6" nameend="col8" align="center">G1101-i-original </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3">1 min</oasis:entry>  
         <oasis:entry colname="col4">5 min</oasis:entry>  
         <oasis:entry colname="col5">Optimum</oasis:entry>  
         <oasis:entry colname="col6">1 min</oasis:entry>  
         <oasis:entry colname="col7">5 min</oasis:entry>  
         <oasis:entry colname="col8">Optimum</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1"><inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col2">Ref1</oasis:entry>  
         <oasis:entry colname="col3">0.03</oasis:entry>  
         <oasis:entry colname="col4">0.02</oasis:entry>  
         <oasis:entry colname="col5">0.01</oasis:entry>  
         <oasis:entry colname="col6">0.07</oasis:entry>  
         <oasis:entry colname="col7">0.03</oasis:entry>  
         <oasis:entry colname="col8">0.01</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Ref2</oasis:entry>  
         <oasis:entry colname="col3">0.04</oasis:entry>  
         <oasis:entry colname="col4">0.02</oasis:entry>  
         <oasis:entry colname="col5">0.01</oasis:entry>  
         <oasis:entry colname="col6">0.07</oasis:entry>  
         <oasis:entry colname="col7">0.04</oasis:entry>  
         <oasis:entry colname="col8">0.02</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Ref3</oasis:entry>  
         <oasis:entry colname="col3">0.04</oasis:entry>  
         <oasis:entry colname="col4">0.02</oasis:entry>  
         <oasis:entry colname="col5">0.01</oasis:entry>  
         <oasis:entry colname="col6">0.08</oasis:entry>  
         <oasis:entry colname="col7">0.04</oasis:entry>  
         <oasis:entry colname="col8">0.01</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Mean</oasis:entry>  
         <oasis:entry colname="col3">0.04</oasis:entry>  
         <oasis:entry colname="col4">0.02</oasis:entry>  
         <oasis:entry colname="col5">0.01</oasis:entry>  
         <oasis:entry colname="col6">0.07</oasis:entry>  
         <oasis:entry colname="col7">0.04</oasis:entry>  
         <oasis:entry colname="col8">0.02</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"><inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col2">Ref1</oasis:entry>  
         <oasis:entry colname="col3">0.0009</oasis:entry>  
         <oasis:entry colname="col4">0.0005</oasis:entry>  
         <oasis:entry colname="col5">0.0001</oasis:entry>  
         <oasis:entry colname="col6">0.0025</oasis:entry>  
         <oasis:entry colname="col7">0.0014</oasis:entry>  
         <oasis:entry colname="col8">0.0006</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Ref2</oasis:entry>  
         <oasis:entry colname="col3">0.0009</oasis:entry>  
         <oasis:entry colname="col4">0.0004</oasis:entry>  
         <oasis:entry colname="col5">0.0003</oasis:entry>  
         <oasis:entry colname="col6">0.0025</oasis:entry>  
         <oasis:entry colname="col7">0.0013</oasis:entry>  
         <oasis:entry colname="col8">0.0008</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Ref3</oasis:entry>  
         <oasis:entry colname="col3">0.0009</oasis:entry>  
         <oasis:entry colname="col4">0.0004</oasis:entry>  
         <oasis:entry colname="col5">0.0001</oasis:entry>  
         <oasis:entry colname="col6">0.0032</oasis:entry>  
         <oasis:entry colname="col7">0.0016</oasis:entry>  
         <oasis:entry colname="col8">0.0007</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Mean</oasis:entry>  
         <oasis:entry colname="col3">0.0009</oasis:entry>  
         <oasis:entry colname="col4">0.0004</oasis:entry>  
         <oasis:entry colname="col5">0.0002</oasis:entry>  
         <oasis:entry colname="col6">0.0027</oasis:entry>  
         <oasis:entry colname="col7">0.0014</oasis:entry>  
         <oasis:entry colname="col8">0.0007</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"><inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C</oasis:entry>  
         <oasis:entry colname="col2">Ref1</oasis:entry>  
         <oasis:entry colname="col3">0.22</oasis:entry>  
         <oasis:entry colname="col4">0.12</oasis:entry>  
         <oasis:entry colname="col5">0.03</oasis:entry>  
         <oasis:entry colname="col6">0.63</oasis:entry>  
         <oasis:entry colname="col7">0.34</oasis:entry>  
         <oasis:entry colname="col8">0.08</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Ref2</oasis:entry>  
         <oasis:entry colname="col3">0.17</oasis:entry>  
         <oasis:entry colname="col4">0.09</oasis:entry>  
         <oasis:entry colname="col5">0.04</oasis:entry>  
         <oasis:entry colname="col6">0.51</oasis:entry>  
         <oasis:entry colname="col7">0.26</oasis:entry>  
         <oasis:entry colname="col8">0.15</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Ref3</oasis:entry>  
         <oasis:entry colname="col3">0.16</oasis:entry>  
         <oasis:entry colname="col4">0.08</oasis:entry>  
         <oasis:entry colname="col5">0.01</oasis:entry>  
         <oasis:entry colname="col6">0.44</oasis:entry>  
         <oasis:entry colname="col7">0.24</oasis:entry>  
         <oasis:entry colname="col8">0.10</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Mean</oasis:entry>  
         <oasis:entry colname="col3">0.18</oasis:entry>  
         <oasis:entry colname="col4">0.09</oasis:entry>  
         <oasis:entry colname="col5">0.03</oasis:entry>  
         <oasis:entry colname="col6">0.53</oasis:entry>  
         <oasis:entry colname="col7">0.28</oasis:entry>  
         <oasis:entry colname="col8">0.13</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p>The precisions of G1101-i-original and G2201-i <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values were
comparable with other reported performances of IRIS instruments. The
precision of TDLAS instruments ranged from 0.03 to 4 ‰ (Bowling et al., 2003, 2005; Griffis et al., 2004; Pataki et al., 2006).
Picarro EnviroSense 2050 had a precision of 0.08 ‰ at
130 min (Friedrichs et al., 2010). The Picarro G1101-i had a precision of
0.2 ‰ at 5 min (Vogel et al., 2013), and the best
precision of 0.08 ‰ at 2000 s (Wen et al., 2013). For Los
Gatos DLT-100, the optimal precision of 0.04 ‰ was
obtained at 1000 s (Wen et al., 2013). The QCLAS typically has a precision
of 0.18 ‰ at 350 ppm CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (McManus et al., 2005), and
the optimal precision of 0.16 ‰ was obtained at 500 s (Tuzson et al., 2008). Nicolet Avatar 370 (Thermo Electron, USA) based on
FTIR technology obtained the optimal precision of 0.15 ‰
at 16 min (Mohn et al., 2007), and an improved version had a precision of
0.02 ‰ at 10 min (Griffith et al., 2012).</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Concentration dependence</title>
      <p>Figure 3 shows the dependence of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C on CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration
for G1101-i-original and G2201-i. The dependence of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C on
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration is the nonlinearity of the analyzer response to
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration variance (Griffith et al., 2012; Guillon et al.,
2012; Wen et al., 2013). The <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values of Ref1, Ref2, and
Ref3 measured by G1101-i-original were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>23.46 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.26, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22.99 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.28, and
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22.62 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.27 ‰, with an average value of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>23.02 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.27 ‰. The <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values measured by
G2201-i were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.65 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.07, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.51 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.08, and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.49 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.05 ‰,
with an average value of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.55 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.07 ‰ (Fig. 3).
In the range of 368.1–550.1 ppm, <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values
measured by G1101-i-original and G2201-i showed an increase with an increase
of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration at 0.46 ‰ per 100 ppm and
0.09 ‰ per 100 ppm, respectively, and the peak-to-peak
amplitudes were 1.75  and 0.47 ‰,
respectively.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Dependency of the measured <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C of G1101-i before
upgradation (G1101-i-original) and G2201-i analyzers on the measured
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration with three different CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations with same
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C reference gases.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016-f03.png"/>

        </fig>

      <p>The concentration dependence of the measured <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values is the
main error source affecting IRIS measurements. Guillon et al. (2012) found
that the DLT-100 based on ICOS technology had a nonlinear concentration
dependence in the range 300–2000 ppm. After correcting the
concentration dependence by a fifth-order polynomial calibration curve, the
accuracy improved from 2.7 to 1.3 ‰ for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C. The Picarro G1101-i analyzer, based on CRDS technology, showed no
significant concentration dependence of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C with a standard
deviation of  <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.2 ‰ in the range
303–437 ppm (Vogel et al., 2013). Griffith et al. (2012) used
a series of different CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios at constant <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C,
and found that a residual curvature against the reciprocal of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was
caused by a small nonlinear response of the analyzer.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><caption><p>The stability and accuracy of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values of the three reference gases (Ref1, Ref2, and Ref3) with same <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measured
by G1101-i before upgradation (G1101-i-original) and G2201-i analyzers.</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" colsep="1"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:thead>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry rowsep="1" namest="col2" nameend="col3" align="center" colsep="1">G1101-i-original </oasis:entry>

         <oasis:entry rowsep="1" namest="col4" nameend="col5" align="center">G2201-i </oasis:entry>

         <oasis:entry rowsep="1" colname="col6" morerows="1">IRMS</oasis:entry>

       </oasis:row>
       <oasis:row rowsep="1">

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2">Measured</oasis:entry>

         <oasis:entry colname="col3">Corrected</oasis:entry>

         <oasis:entry colname="col4">Measured</oasis:entry>

         <oasis:entry colname="col5">Corrected</oasis:entry>

       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>

         <oasis:entry colname="col1">Ref1</oasis:entry>

         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>23.46 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.26</oasis:entry>

         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.29 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.34</oasis:entry>

         <oasis:entry colname="col4"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.65 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.07</oasis:entry>

         <oasis:entry colname="col5"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.51 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.21</oasis:entry>

         <oasis:entry colname="col6"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.38 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.06</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">Ref2</oasis:entry>

         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22.99 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.28</oasis:entry>

         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.42 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.20</oasis:entry>

         <oasis:entry colname="col4"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.51 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.08</oasis:entry>

         <oasis:entry colname="col5"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.35 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.08</oasis:entry>

         <oasis:entry colname="col6"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.38 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.06</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">Ref3</oasis:entry>

         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22.62 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.27</oasis:entry>

         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.32 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.21</oasis:entry>

         <oasis:entry colname="col4"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.49 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.05</oasis:entry>

         <oasis:entry colname="col5"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.48 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.14</oasis:entry>

         <oasis:entry colname="col6"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.38 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.06</oasis:entry>

       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S3.SS3">
  <title>Stability and accuracy</title>
      <p>Based on the same data measured in Sect. 3.2, the temporal drift and
accuracy of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values of Ref1, Ref2, and Ref3 measured by
G1101-i-original and G2201-i are shown in Fig. 4. The two-point mixing
ratio gain and offset calibration method (Bowling et al., 2003) was used to
calibrate the measured <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C value for each 120 min measurement
cycle. The instrument temporal drift was calculated as the maximum
variability during the measurement period, which mainly resulted from the
sensitivity to the changing environmental conditions (e.g., temperature
dependence). During the 48 h measuring period, the standard deviations of
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values of Ref1, Ref2, and Ref3 measured by
G1101-i-original were 0.26, 0.28, and 0.27 ‰,
respectively, with temporal drifts (peak-to-peak magnitude) of 0.92, 1.09,
and 0.93 ‰. The standard deviations of the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values of Ref1, Ref2, and Ref3 measured by G2201-i were 0.07,
0.08, and 0.05 ‰, with temporal drifts of 0.23, 0.37,
and 0.19 ‰. The differences between the CRDS and IRMS
measurements were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.08 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.26, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.61 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.28, and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.24 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.27 ‰ for G1101-i-original and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.27 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.07, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.13 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.08,
and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.11 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.05 ‰ for G2201-i. After
calibration, the differences reduced to 0.09 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.34, 0.04 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.20, and 0.06 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.21 ‰ for G1101-i and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.13 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.21, 0.03 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.08,
and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.10 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.14 ‰
for G2201-i (Table 2). Much improved accuracy was obtained when the
calibration was interpolated for Ref2 with Ref1 and Ref3 rather than
extrapolated for Ref1 with Ref2 and Ref3 or Ref3 with Ref1 and Ref1.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p>Time variations of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C of the three different CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations with same <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C reference gases (Ref1, Ref2 and
Ref3) of G1101-i before upgradation (G1101-i-original) <bold>(a, c, e)</bold> and
G2201-i <bold>(b, d, f)</bold> analyzers. Panels <bold>(a)</bold> and <bold>(b)</bold> show data from Ref1, panels <bold>(c)</bold> and <bold>(d)</bold> show data
from Ref2, and panels <bold>(e)</bold> and <bold>(f)</bold> show data from Ref3.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016-f04.png"/>

        </fig>

      <p>As for the drift of IRIS instruments, Vogel et al. (2013) monitored two gas
cylinders sequentially with 10 min and 20 min for each cylinder lasting 3 days; the drift of G1101-i was around 0.3 ‰ day<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>.
Hammer et al. (2013) measured a target gas continuously for 6 days; the
FTIR instrument showed a drift of 0.02 ‰ day<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> for
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C after sensitivity correction. Tuzson et al. (2008)
measured identical air samples for 1 min every 15 min for 7 h; the standard
deviation of the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measured by QCLAS was
0.14 ‰ (<inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 28). Schaeffer et al. (2008) monitored two
quality control tanks in the field over 2.44 years, and the standard
deviations of the difference between actual and measured values were
0.31 and 0.33 ‰ (<inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2318 and
<inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2254). Wehr et al. (2008)  monitored a CSIRO standard gas over a period
of 30 min, and the standard deviations for integration times of 20 and 120 s
were 0.71 and 0.64 ‰, respectively. In this study, over
a period of 48 h, the standard deviations of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measured by
G1101-i-original and G2201-i were 0.26–0.28 and
0.05–0.08 ‰, respectively, and the drift
values were 0.92–1.09 and 0.19–0.37 ‰, respectively.</p>
      <p>Regarding the accuracy of IRIS instruments, Guillon et al. (2012) found that
in the range 300–2000 ppm, the accuracy of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
measured by DLT-100 was 2.7 ‰ for raw measurements and
improved to 1.3 ‰ after correction. Over the entire
2.44-year period, two quality control gases measured by TDLAS in the field
showed agreement between actual and measured values of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.17 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.33 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.14 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.4 ‰ for
tank 1 and tank 2 (Schaeffer et al., 2008). Over a period of 30 min, the
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values measured by optical feedback cavity enhanced
absorption spectroscopy (OF-CEAS) showed a systematic error of
0.9 ‰ between the measured and IRMS values (Wehr et al.,
2008). Using the optimized PLS algorithm, the accuracy of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
measured by FTIR was 0.4 ‰ with CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations
in the range 364–530 ppm (Mohn et al., 2007). Over a 1-year
period, Vogel et al. (2013) found that although a single measurement was
imprecise, the G1101-i <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C analyzer provided a mean accuracy
of 0.002 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.025 ‰ after proper calibration. In
this study, the accuracies of G1101-i-original and G2201-i <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
analyzers were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.06 to <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.22 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.25 to <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.09 ‰ before calibration and improved to
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.02–0.11 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.11–0.05 ‰
after calibration for each 120 min measurement cycle over a measurement
course of 48 h.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <?xmltex \opttitle{Sensitivity of $\delta^{{13}}$C to water vapor concentration}?><title>Sensitivity of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C to water vapor concentration</title>
      <p>The sensitivities of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C to water vapor concentration of
G1101-i-original and G2201-i before the upgrade of G1101-i and
G1101-i-upgraded and G2201-i after the upgrade of G1101-i are shown in Fig. 5. For the first test, the dew point temperature of the reference gas
ranged from 5 to 25 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. The mean <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values
measured by G1101-i-original and G2201-i were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.64 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.72 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.60 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.19 ‰, the
sensitivity of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C to the water vapor mixing ratio was
0.86 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O and 0.20 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O, and the peak-to-peak amplitudes of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C under
different water vapor mixing ratios were 1.96 and
0.45 ‰, respectively. For the second test, the mean
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values measured by G1101-i-upgraded and G2201-i were
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22.34 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.09 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22.27 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.18 ‰, the sensitivity of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C to the
water vapor mixing ratio was 0.13 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O and
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.19 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O, and the peak-to-peak amplitudes
of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C under different water vapor mixing ratios were
0.22 and 0.32 ‰, respectively. Note
that with the dew point in the range of 5–20 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C,
the mean <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values measured were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.84 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.66 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.68 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.07 ‰ by
G1101-i-original and G2201-i, respectively, and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22.34 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.10 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22.34 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.08 ‰ by
G1101-i-upgraded and G2201-i, respectively. The sensitivity of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C to the water vapor mixing ratio was 1.01 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O and 0.09 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O, and the
peak-to-peak amplitudes were 1.47 and 0.14 ‰ by G1101-i-original and G2201-i, respectively. The
sensitivity of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C to the water vapor mixing ratio was
0.15 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O and 0.13 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O, and the peak-to-peak amplitudes were
0.22 and 0.19 ‰ for G1101-i-upgraded
and G2201-i, respectively.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p>Sensitivity of the measured <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C by G1101-i and
G2201-i on water vapor mixing ratio. Panel <bold>(a)</bold> shows sensitivity measured before G1101-i
was upgraded (G1101-i-original and G2201-i) and <bold>(b)</bold> sensitivity measured after G1101-i was upgraded (G1101-i-upgraded and G2201-i).</p></caption>
          <?xmltex \igopts{width=213.395669pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016-f05.png"/>

        </fig>

      <p>The dilution and pressure broadening effects are the two major factors
leading to the dependence of the measured <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C on water vapor
concentrations (Chen et al., 2010; Nara et al., 2012). Variations in sample
water vapor significantly affect the mixing ratio of <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> via the dilution effect. In addition, the variability of
water vapor also introduces the broadening effect along the spectroscopic
line, which includes the Lorentzian line broadening and Dicke line narrowing
effect. The CRDS instruments measured <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations by the peak height of the absorption peak whose baseline and
shape can be affected by the absorption peaks of water (Nara et al., 2012;
Rella et al., 2013). As for CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, the systematic errors caused by the
broadening effects would be 40 % of the dilution effects if they were not
corrected (Chen et al., 2010). The transferability of water correction
functions among multiple instruments also biases the measurement data among
different instruments. Rella et al. (2013) found that for analyzers CFADS15 and 30, the
transferability of both CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, after correction of the water
vapor mole fraction in the range no more than 2 %, meets the Global Atmosphere Watch (GAW) Programme quality. For three
instruments based on CRDS technology, however, the residual errors of
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> showed substantially large values with increasing water vapor
concentration (Nara et al., 2012). The incompatibility of these results
indicates the need for more precise experiments to evaluate the
transferability of water correction functions (Kwok et al., 2015). Moreover,
potential long-term drift of the water vapor correction coefficients of
individual instruments needs to be assessed (Nara et al., 2012; Rella et
al., 2013).</p><?xmltex \hack{\newpage}?><?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p>Time variations of <bold>(a)</bold> and <bold>(d)</bold> hourly atmospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C, <bold>(b)</bold> and <bold>(e)</bold> difference between the Picarro G1101-i and G2201-i
analyzers, and <bold>(c)</bold> and <bold>(f)</bold> histogram of the differences. The left
panels <bold>(a, b, c)</bold> show time variations measured before G1101-i was upgraded (G1101-i-original) (DOY 164–174) and the right panels <bold>(d, e, f)</bold> show those measured after G1101-i
was upgraded (G1101-i-upgraded) (DOY 348–356).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016-f06.png"/>

        </fig>

      <p>In this study, the standard deviations of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measured by
G2201-i (0.07 and 0.08 ‰) under a dew point in the range 5–20 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C are better than the
precision given by manufacturer (0.15 ‰), and the standard
deviation of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measured by G1101-i-upgraded (0.10 ‰) is also smaller than the specified precision.
These results indicate that the water corrections embedded in the
instruments' software work sufficiently within the dew point range of
5–20 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p>Time series of the 10 min averaged <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C of quality
control gas (Ref2) monitored by <bold>(a)</bold> G1101-i analyzer and <bold>(b)</bold> G2201-i
analyzer.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016-f07.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS5">
  <title>Atmospheric measurement</title>
      <p>The <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C of atmospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was measured continuously by
G1101-i-original and G2201-i analyzers and by G1101-i-upgraded and G2201-i
analyzers. The temporal variations of atmospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C, the
difference between G1101-i and G2201-i analyzers, and the distribution of
differences are shown in Fig. 6. The measured atmospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values were calibrated using Ref1 and Ref3, and Ref2 was used as a
quality control gas to assess the accuracy of atmospheric sample
measurements (Fig. 7).</p>
      <p>Atmospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measured by G1101-i and G2201-i showed good
agreement, and both instruments captured the rapid changes in atmospheric
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C on hourly to diurnal cycle scales. Before G1101-i was
upgraded (DOY 164–174), atmospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
measured by G1101-i-original and G2201-i ranged from
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13.24 to <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>7.47 and
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13.41 to <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>7.62 ‰, with average
values of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>9.49 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.22 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>9.42 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.17 ‰, respectively. The difference between <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measured by G1101-i-original and G2201-i analyzers ranged from
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.62 to 0.76 ‰, with an average
value of 0.07 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.24 ‰. The difference exhibits a
Gaussian distribution. A significant systematic bias of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
values was identified between these two analyzers (<inline-formula><mml:math display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test, <inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> &lt; 0.01).
After G1101-i was upgraded (DOY 348–356), atmospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
measured by G1101-i-upgraded and G2201-i ranged from
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>14.08 to <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>8.64 and
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13.89 to <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>9.06 ‰, with average
values of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10.61 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10.56 ‰,
respectively. The difference of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measured by
G1101-i-upgraded and G2201-i analyzers ranged from
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.57 to 0.85 ‰, with an average
value of 0.05 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.30 ‰. A significant systematic
bias of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values still existed between these two analyzers (<inline-formula><mml:math display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn>0.018</mml:mn></mml:mrow></mml:math></inline-formula>). In addition, field measured values of Ref2 during the
atmospheric measurement period (DOY 164–174 and DOY 348–356) were used to assess the stability and accuracy of both
analyzers (Fig. 7). During the first atmospheric measurement period, the
average <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values of Ref2 were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.32 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.51 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.91 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.12 ‰ for
G1101-i-original and G2201-i, respectively. After calibration, the average
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.30 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.40 and
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.56 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.17 ‰, respectively. The accuracy (the
difference between calibration and actual values) respectively ranged from
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.70 to 0.91 and
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.42 to 0.19 ‰, with average
values of 0.09 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.40 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.17 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.17 ‰. During the second atmospheric measurement
period, the average <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values of Ref2 were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>24.37 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.59 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.92 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.18 ‰ for
G1101-i-upgraded and G2201-i. After calibration, the average <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.56 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.23 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.57 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.09 ‰, respectively. The accuracy ranged from
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.60 to 0.30 and
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.42 to 0.02 ‰, with average
values of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.17 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.23 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.18 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.09 ‰, respectively. These results indicate that
G2201-i is more stable than G1101-i, which is consistent with the Allan
variation results.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F8" specific-use="star"><caption><p>Dependence of the atmospheric <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>13C difference between the
Picarro G1101-i and G2201-i analyzers on the CO2 and H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O
concentration. Panels <bold>(a)</bold> and <bold>(c)</bold> show dependence measured before G1101-i was upgraded (G1101-i-original) (DOY 164–174), and <bold>(b)</bold> and <bold>(d)</bold> show dependence measured after G1101-i was upgraded (G1101-i-upgraded) (DOY 348–356).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016-f08.png"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F9" specific-use="star"><caption><p>Keeling plot of the calibrated atmospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
against the reciprocal of the calibrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration for the
Picarro <bold>(a, b)</bold> G1101-i and <bold>(c, d)</bold> G2201-i analyzers. Panels
<bold>(a)</bold> and <bold>(c)</bold> show plots measured before G1101-i was upgraded (G1101-i-original) (DOY 164–174),
and <bold>(b)</bold> and <bold>(d)</bold>  show plots measured after G1101-i was upgraded (G1101-i-upgraded) (DOY 348–356). Both daytime and nighttime data were used.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3879/2016/amt-9-3879-2016-f09.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4">
  <title>Discussion</title>
<sec id="Ch1.S4.SS1">
  <title>Calibration scheme of IRIS instruments</title>
      <p>In general, all of the IRIS instruments aim to maintain high enough
precision and accuracy such that the data are traceable to international
scales. However, sensitivity to changing environmental conditions (e.g.,
temperature dependence) and dependence of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C on the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentration affect the performance of IRIS measurements (Wada et al.,
2011; Guillon et al., 2012; Wen et al., 2013). Reliable and accurate
measurements similar to that of IRMS can be obtained with proper calibration (Bowling et al., 2005; Guillon et al., 2012; Hammer et al., 2013; Vogel et
al., 2013; Wen et al., 2013). In theory, both issues of delta scale
stretching and the concentration dependence should be corrected by
generating multiple delta values over a range of mixing ratios under ambient
conditions. In practice, ignoring the effect of the delta scale stretching,
the two-point mixing ratio gain and offset calibration method was
successfully applied to calibrate the mixing ratios of <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> separately (Bowling et al., 2003; Wen et al., 2013). For the
instrument performance diagnoses, it was suggested that another reference
gas be measured to monitor the long-term precision and accuracy.
Three-point or higher calibration schemes with CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration
signals spanning a range of ambient concentrations were suggested to
ensure the linearity of the analyzer and diagnose the instrument
performance. With proper calibration frequency, the instrument drifts would
be eliminated. Calibration frequency and sampling interval are
instrument-specific characteristics. Note that considering the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C dependence on H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O, researchers should consider drying moist
sample air when H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O is above 2.4 % as is factory-recommended, even
though the water correction works sufficiently well (Fig. 5).</p>
</sec>
<sec id="Ch1.S4.SS2">
  <title>Error propagation through the Keeling analysis</title>
      <p>Figure 8 shows the dependence of the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C difference between
G1101-i-original and G2201-i and between G1101-i-upgraded and G2201-i on
water vapor concentration and CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratio. Before and after
G1101-i was upgraded, there was no significant correlation between the
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C difference and CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratio (Fig. 8a and 8b).
Before G1101-i was upgraded, a significant linear correlation was observed
between the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C difference and water vapor concentration (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn>0 01</mml:mn></mml:mrow></mml:math></inline-formula>, Fig. 8c); after the upgrade of G1101-i, there was no
significant correlation between the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C difference and water
vapor concentration (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn> 0.05</mml:mn></mml:mrow></mml:math></inline-formula>, Fig. 8d). This relationship was
mainly due to the upgrade of G1101-i, which excluded <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
measurement errors that originated from variations in water vapor
concentration and improved the accuracy of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measurement.
This result is consistent with the results of the sensitivity of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C to water vapor concentration test. In addition, note that the
second measurement was conducted in winter when the atmospheric water vapor
concentration was relatively low and the water vapor interference was
small.</p>
      <p>The isotopic composition of source CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">S</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> was used
to gain insight into the potential local CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> sources and underlying
mechanisms at different temporal and spatial scales. In this study,
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:math></inline-formula> was calculated using the calibration dataset of
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C and 1/CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> by the Keeling plot intercept method (Keeling,
1958; Fig. 9). The total CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was calculated using the <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
and <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from the Picarro data. During the first atmospheric
measurement period, the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:math></inline-formula> values were
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>24.80 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.39 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>23.98 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.30 ‰, with a mean
difference of 0.82 ‰, respectively, for G1101-i-original with a
range of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations from 390.92 to 630.92 ppm and G2201-i with
a range of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations from 391.76 to 631.29 ppm. Note that the
uncertainties are the standard error of the intercept from the fitting
algorithm. If we assumed that the atmospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C is a linear
function of <inline-formula><mml:math display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo></mml:mrow></mml:math></inline-formula> CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with a small concentration-dependent error
<inline-formula><mml:math display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> (Eq. 18; Wen et al., 2013), then error propagation through the
concentration dependence would be a function of <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> with respect
to the intercept of the Keeling plot. When <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">ε</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.05 ‰,
this error would propagate through the Keeling plot and cause a difference of
0.99 ‰. This result is close to the actual difference of
0.82 ‰ between G1101-i-original and G2201-i. When we used only the
nighttime data (22:00–04:00)
for the Keeling analysis, the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:math></inline-formula> values were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>28.35 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.34 and
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>27.11 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.02 ‰ for G1101-i-original and G2201-i,
respectively, with a mean difference of 1.24 ‰. The
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:math></inline-formula> value deduced from nighttime data was a mixed
value of various local CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> sources, including the combustion of natural
gas, gasoline, and coal as well as the respiration of plants and soil (Pang
et al., 2016a).</p>
      <p>During the second atmospheric measurement period, the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:math></inline-formula> values were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>25.90 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.28 and
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>25.97 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.12 ‰, with a mean difference of
0.07 ‰, for G1101-i-upgraded with a range of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations from 398.51 to 552.66 ppm and G2201-i with a range of
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration from 399.92 to 555.90 ppm, respectively. When we used
only the nighttime data (22:00–04:00) for the Keeling
analysis, the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:math></inline-formula> values were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>26.05 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.16 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>25.69 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.41 ‰,
with a mean difference of 0.36 ‰ for G1101-i-upgraded and
G2201-I, respectively. The systematic bias of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:math></inline-formula>
decreased from 1.24 ‰ between G1101-i-original and
G2201-i to 0.36 ‰ between G1101-i-upgraded and G2201-i.
The results confirm that we should pay attention to the measurement
difference resulting from the uncorrected dependencies on CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> or
H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O concentrations among different IRIS instruments and that this
difference will result in error propagation through Keeling plot analysis (Wen et al., 2013).</p>
      <p>The potential problems caused by incompatibility include the integrity of
an internal calibration scale and modifications to analytical procedures in
decade-long records (Levin et al., 2012). In this study, the Keeling plot
intercepts of G1101-i and G2201-i measurements should be identical because
of the common air samples. Differences in the Keeling plot intercepts of 1.24 or 0.36 ‰ were caused by a systematic error
between G1101-i (before and after upgrade) and G2201-i. Note that the uncertainty of
the Keeling plot intercept was related to its underlying assumption, CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
range, and uncertainty in the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and isotopic measurements. Generally
speaking, the standard error of the Keeling plot intercept should be less
than 1 ‰ (Pataki et al., 2003; Zobitz et al., 2006).</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusion</title>
      <p>In this study, the performance and comparability of Picarro G1101-i and
G2201-i CO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C analyzers was evaluated. The main
conclusions are as follows.
<list list-type="order"><list-item><p>The Allan variation test indicates that the best precision was
0.08–0.15  and 0.01–0.04 ‰, measured respectively by G1101-i-original and
G2201-i with a CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> range from 368.1 to 550.1 ppm; the 5 min
precision was 0.24–0.34 and 0.08–0.12 ‰, respectively. With proper calibration, high
enough precision (<inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>0.1 ‰) for <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C
research, similar to that of IRMS, should be obtainable by all of the IRIS
instruments. It is difficult, however, to achieve <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>0.01 ‰ precision, as recommended by the Global Atmosphere
Watch Programme of the World Meteorological Organization (WMO-GAW; WMO,
2011).</p></list-item><list-item><p>For the gradient switching test lasting 48 h among Ref1, Ref2, and Ref3,
the dependence of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C on the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration was
0.46 ‰ per 100 ppm for G1101-i-original and
0.09 ‰ per 100 ppm for G2201-i in the range of
368.1–550.1 ppm, and the drift of the instruments ranged from
0.92 to 1.09 and 0.19 to 0.37 ‰,
respectively. After calibration by the two-point mixing ratio gain and
offset calibration method, the average <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C values of Ref1,
Ref2, and Ref3 were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.34 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.07 ‰ by
G1101-i-original and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.45 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.09 ‰ by G2201-i,
similar to the actual values measured by IRMS (<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>20.38 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.06 ‰).</p></list-item><list-item><p>With dew point temperatures in the range of 5–20 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, the sensitivity of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C to the water vapor
mixing ratio was 1.01 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O and
0.09 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O by G1101-i-original and G2201-i
during the first test (before the upgrade of G1101-i) and
0.15 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O and 0.13 ‰ <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> % H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O by G1101-i-upgraded and G2201-i during the second test (after the
upgrade of G1101-i). The standard deviations of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measured
by G1101-i-upgraded and G2201-i were <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.10 and <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.08 ‰.
These results indicate that the water corrections embedded in the
instruments' software work sufficiently within the dew point range of
5–20 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.</p></list-item><list-item><p>Atmospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measured by G1101-i and G2201-i captured
the rapid changes in atmospheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C on hourly to diurnal
cycle scales. Before G1101-i was upgraded (DOY 164–174), the difference of
hourly <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C averages measured by G1101-i-original and G2201-i
analyzers ranged from <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.62 to
0.76 ‰, with an average value of 0.07 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.24 ‰. After G1101-i was upgraded (DOY 348–356), the
difference in hourly <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C averages measured by G1101-i-upgraded
and G2201-i analyzers ranged from <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.57 to
0.85 ‰, with an average value of 0.05 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.30 ‰. This difference exhibits a Gaussian
distribution. Before the upgrade of G1101-i, a significant linear
correlation was observed between the <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C difference and water
vapor concentration (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn> 0.01</mml:mn></mml:mrow></mml:math></inline-formula>), but there is no significant
correlation (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn> 0.05</mml:mn></mml:mrow></mml:math></inline-formula>) after the upgrade of G1101-i. This is
mainly due to the improvement of the interference of water vapor in the
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C measurement by the upgraded algorithm of the G1101-i
software. The difference of Keeling intercept values between G1101-i and
G2201-i decreased from 1.24 to
0.36 ‰, which indicates the importance of consistency
among different IRIS instruments.</p></list-item></list></p>
</sec>
<sec id="Ch1.S6">
  <title>Data availability</title>
      <p>The dataset for G1101-i and G2201-i analyzers' tests are available for
ordering free of charge at
<uri>https://www.researchgate.net/publication/301644542_Inter-comparison_of_two_cavity_ring-down_spectroscopy_analyzers_for_atmospheric_13CO2_12CO2_measurement</uri>
(Pang et al., 2016b).</p>
</sec>

      
      </body>
    <back><ack><title>Acknowledgements</title><p>This study was supported by the National Natural Science Foundation of China (41571130043, 31290221, and 31470500)
and the National Key Research and Development Program of China (2016YFC0500102).<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: T. F. Hanisco<?xmltex \hack{\newline}?>
Reviewed by: L. R. Welp and one anonymous referee</p></ack><ref-list>
    <title>References</title>

      <ref id="bib1.bib1"><label>1</label><mixed-citation>
Allan, D. W.: Should the classical variance be used as a basic measure in
standards metrology?, IEEE T. Instrum. Meas., 1001, 646–654, 1987.</mixed-citation></ref>
      <ref id="bib1.bib2"><label>2</label><mixed-citation>Bowling, D. R., Sargent, S. D., Tanner, B. D., and Ehleringer, J. R.:
Tunable diode laser absorption spectroscopy for stable isotope studies of
ecosystem-atmosphere CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> exchange, Agr. Forest Meteorol., 118, 1–19, <ext-link xlink:href="http://dx.doi.org/10.1016/s0168-1923(03)00074-1" ext-link-type="DOI">10.1016/s0168-1923(03)00074-1</ext-link>, 2003.</mixed-citation></ref>
      <ref id="bib1.bib3"><label>3</label><mixed-citation>Bowling, D. R., Burns, S. P., Conway, T. J., Monson, R. K., and White, J. W.
C.: Extensive observations of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> carbon isotope content in and above a
high-elevation subalpine forest, Global Biogeochem. Cy, 19, GB3023, <ext-link xlink:href="http://dx.doi.org/10.1029/2004gb002394" ext-link-type="DOI">10.1029/2004gb002394</ext-link>,
2005.</mixed-citation></ref>
      <ref id="bib1.bib4"><label>4</label><mixed-citation>Chen, H., Winderlich, J., Gerbig, C., Hoefer, A., Rella, C. W., Crosson, E.
R., Van Pelt, A. D., Steinbach, J., Kolle, O., Beck, V., Daube, B. C.,
Gottlieb, E. W., Chow, V. Y., Santoni, G. W., and Wofsy, S. C.: High-accuracy
continuous airborne measurements of greenhouse gases (CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>)
using the cavity ring-down spectroscopy (CRDS) technique, Atmos. Meas. Tech.,
3, 375–386, <ext-link xlink:href="http://dx.doi.org/10.5194/amt-3-375-2010" ext-link-type="DOI">10.5194/amt-3-375-2010</ext-link>, 2010.</mixed-citation></ref>
      <ref id="bib1.bib5"><label>5</label><mixed-citation>Flowers, B. A., Powers, H. H., Dubey, M. K., and McDowell, N. G.:
Inter-comparison of two high-accuracy fast-response spectroscopic sensors of
carbon dioxide: a case study, Atmos. Meas. Tech., 5, 991–997,
<ext-link xlink:href="http://dx.doi.org/10.5194/amt-5-991-2012" ext-link-type="DOI">10.5194/amt-5-991-2012</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bib6"><label>6</label><mixed-citation>Friedrichs, G., Bock, J., Temps, F., Fietzek, P., Kortzinger, A., and
Wallace, D. W. R.: Toward continuous monitoring of seawater
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>/<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> isotope ratio and pCO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>: Performance of
cavity ringdown spectroscopy and gas matrix effects, Limnol. Oceanogr.-Meth., 8, 539–551, <ext-link xlink:href="http://dx.doi.org/10.4319/lom.2010.8.539" ext-link-type="DOI">10.4319/lom.2010.8.539</ext-link>, 2010.</mixed-citation></ref>
      <ref id="bib1.bib7"><label>7</label><mixed-citation>Griffis, T. J.: Tracing the flow of carbon dioxide and water vapor between
the biosphere and atmosphere: A review of optical isotope techniques and
their application, Agr. Forest Meteorol., 174, 85–109, <ext-link xlink:href="http://dx.doi.org/10.1016/j.agrformet.2013.02.009" ext-link-type="DOI">10.1016/j.agrformet.2013.02.009</ext-link>, 2013.</mixed-citation></ref>
      <ref id="bib1.bib8"><label>8</label><mixed-citation>Griffis, T. J., Baker, J. M., Sargent, S. D., Tanner, B. D., and Zhang, J.:
Measuring field-scale isotopic CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> fluxes with tunable diode laser
absorption spectroscopy and micrometeorological techniques, Agr. Forest
Meteorol., 124, 15–29, <ext-link xlink:href="http://dx.doi.org/10.1016/j.agrformet.2004.01.009" ext-link-type="DOI">10.1016/j.agrformet.2004.01.009</ext-link>, 2004.</mixed-citation></ref>
      <ref id="bib1.bib9"><label>9</label><mixed-citation>Griffith, D. W. T., Deutscher, N. M., Caldow, C., Kettlewell, G., Riggenbach,
M., and Hammer, S.: A Fourier transform infrared trace gas and isotope
analyser for atmospheric applications, Atmos. Meas. Tech., 5, 2481–2498,
<ext-link xlink:href="http://dx.doi.org/10.5194/amt-5-2481-2012" ext-link-type="DOI">10.5194/amt-5-2481-2012</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bib10"><label>10</label><mixed-citation>Guillon, S., Pili, E., and Agrinier, P.: Using a laser-based CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> carbon
isotope analyser to investigate gas transfer in geological media, Applied
Physics B-Lasers and Optics, 107, 449–457, <ext-link xlink:href="http://dx.doi.org/10.1007/s00340-012-4942-8" ext-link-type="DOI">10.1007/s00340-012-4942-8</ext-link>,
2012.</mixed-citation></ref>
      <ref id="bib1.bib11"><label>11</label><mixed-citation>Hammer, S., Griffith, D. W. T., Konrad, G., Vardag, S., Caldow, C., and
Levin, I.: Assessment of a multi-species in situ FTIR for precise atmospheric
greenhouse gas observations, Atmos. Meas. Tech., 6, 1153–1170,
<ext-link xlink:href="http://dx.doi.org/10.5194/amt-6-1153-2013" ext-link-type="DOI">10.5194/amt-6-1153-2013</ext-link>, 2013.</mixed-citation></ref>
      <ref id="bib1.bib12"><label>12</label><mixed-citation>
Keeling, C. D.: The concentration and isotopic abundances of atmospheric
carbon dioxide in rural areas, Geochim. Cosmochim. Ac., 13, 322–334, 1958.</mixed-citation></ref>
      <ref id="bib1.bib13"><label>13</label><mixed-citation>Kwok, Y. C., Laurent, O., Guemri, A., Philippon, C., Wastine, B., Rella, C.
W., Vuillemin, C., Truong, F., Delmotte, M., Kazan, V., Darding, M.,
Lebègue, B., Kaiser, C., Xueref-Rémy, I., and Ramonet, M.:
Comprehensive laboratory and field testing of cavity ring-down spectroscopy
analyzers measuring H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O, CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and CO, Atmos. Meas. Tech.,
8, 3867–3892, <ext-link xlink:href="http://dx.doi.org/10.5194/amt-8-3867-2015" ext-link-type="DOI">10.5194/amt-8-3867-2015</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bib14"><label>14</label><mixed-citation>Levin, I., C. Veidt, B. Vaughn, G. Brailsford, T. Bromley, R. Heinz, D. Lowe,
J. Miller, C. Poß and J. White: No inter-hemispheric <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> trend observed, Nature, 486, E3–E4, 2012.</mixed-citation></ref>
      <ref id="bib1.bib15"><label>15</label><mixed-citation>McManus, J. B., Nelson, D. D., Shorter, J. H., Jimenez, R., Herndon, S.,
Saleska, S., and Zahniser, M.: A high precision pulsed quantum cascade laser
spectrometer for measurements of stable isotopes of carbon dioxide,
J. Mod. Optic., 52, 2309–2321,
<ext-link xlink:href="http://dx.doi.org/10.1080/09500340500303710" ext-link-type="DOI">10.1080/09500340500303710</ext-link>, 2005.</mixed-citation></ref>
      <ref id="bib1.bib16"><label>16</label><mixed-citation>Mohn, J., Werner, R. A., Buchmann, B., and Emmenegger, L.: High-precision
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> analysis by FTIR spectroscopy using a novel calibration
strategy, J. Mol. Struct., 834, 95–101, <ext-link xlink:href="http://dx.doi.org/10.1016/j.molstruc.2006.09.024" ext-link-type="DOI">10.1016/j.molstruc.2006.09.024</ext-link>,
2007.</mixed-citation></ref>
      <ref id="bib1.bib17"><label>17</label><mixed-citation>Mohn, J., Zeeman, M. J., Werner, R. A., Eugster, W., and Emmenegger, L.:
Continuous field measurements of<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn>13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and trace gases by FTIR
spectroscopy, Isotopes Environ. Health Stud., 44, 241–251,
<ext-link xlink:href="http://dx.doi.org/10.1080/10256010802309731" ext-link-type="DOI">10.1080/10256010802309731</ext-link>, 2008.</mixed-citation></ref>
      <ref id="bib1.bib18"><label>18</label><mixed-citation>Nara, H., Tanimoto, H., Tohjima, Y., Mukai, H., Nojiri, Y., Katsumata, K.,
and Rella, C. W.: Effect of air composition (N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, Ar, and
H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O) on CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> measurement by wavelength-scanned cavity
ring-down spectroscopy: calibration and measurement strategy, Atmos. Meas.
Tech., 5, 2689–2701, <ext-link xlink:href="http://dx.doi.org/10.5194/amt-5-2689-2012" ext-link-type="DOI">10.5194/amt-5-2689-2012</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bib19"><label>19</label><mixed-citation>Pang, J., Wen, X., and Sun, X.: Mixing ratio and carbon isotopic composition
investigation of atmospheric CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in Beijing, China, Sci. Total Environ.,
539, 322–330, 2016a.</mixed-citation></ref>
      <ref id="bib1.bib20"><label>20</label><mixed-citation>Pang, J., Wen, X., Sun, X., and Huang, K.: Inter-comparison of two cavity
ring-down spectroscopy analyzers for atmospheric <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>/<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
measurement, available at:
<uri>https://www.researchgate.net/publication/301644542_Inter-comparison_of_two_cavity_ring-down_spectroscopy_analyzers_for_atmospheric_13CO2_12CO2_measurement</uri>,
2016b.</mixed-citation></ref>
      <ref id="bib1.bib21"><label>21</label><mixed-citation>Pataki, D. E., Bowling, D. R., Ehleringer, J. R., and Zobitz, J. M.: High
resolution atmospheric monitoring of urban carbon dioxide sources, Geophys.
Res. Lett., 33, L03813, <ext-link xlink:href="http://dx.doi.org/10.1029/2005gl024822" ext-link-type="DOI">10.1029/2005gl024822</ext-link>, 2006.</mixed-citation></ref>
      <ref id="bib1.bib22"><label>22</label><mixed-citation>Rella, C. W., Chen, H., Andrews, A. E., Filges, A., Gerbig, C., Hatakka, J.,
Karion, A., Miles, N. L., Richardson, S. J., Steinbacher, M., Sweeney, C.,
Wastine, B., and Zellweger, C.: High accuracy measurements of dry mole
fractions of carbon dioxide and methane in humid air, Atmos. Meas. Tech., 6,
837–860, <ext-link xlink:href="http://dx.doi.org/10.5194/amt-6-837-2013" ext-link-type="DOI">10.5194/amt-6-837-2013</ext-link>, 2013.</mixed-citation></ref>
      <ref id="bib1.bib23"><label>23</label><mixed-citation>Schaeffer, S. M., Miller, J. B., Vaughn, B. H., White, J. W. C., and Bowling,
D. R.: Long-term field performance of a tunable diode laser absorption
spectrometer for analysis of carbon isotopes of CO2 in forest air, Atmos.
Chem. Phys., 8, 5263–5277, <ext-link xlink:href="http://dx.doi.org/10.5194/acp-8-5263-2008" ext-link-type="DOI">10.5194/acp-8-5263-2008</ext-link>, 2008.</mixed-citation></ref>
      <ref id="bib1.bib24"><label>24</label><mixed-citation>Sturm, P., Eugster, W., and Knohl, A.: Eddy covariance measurements of
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> isotopologues with a quantum cascade laser absorption spectrometer,
Agr. Forest Meteorol., 152, 73–82, <ext-link xlink:href="http://dx.doi.org/10.1016/j.agrformet.2011.09.007" ext-link-type="DOI">10.1016/j.agrformet.2011.09.007</ext-link>,
2012.</mixed-citation></ref>
      <ref id="bib1.bib25"><label>25</label><mixed-citation>Tuzson, B., Zeeman, M. J., Zahniser, M. S., and Emmenegger, L.: Quantum
cascade laser based spectrometer for in situ stable carbon dioxide isotope
measurements, Infrared Phys. Techn., 51, 198–206,
<ext-link xlink:href="http://dx.doi.org/10.1016/j.infrared.2007.05.006" ext-link-type="DOI">10.1016/j.infrared.2007.05.006</ext-link>, 2008.</mixed-citation></ref>
      <ref id="bib1.bib26"><label>26</label><mixed-citation>Vogel, F. R., Huang, L., Ernst, D., Giroux, L., Racki, S., and Worthy, D. E.
J.: Evaluation of a cavity ring-down spectrometer for in situ observations of
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, Atmos. Meas. Tech., 6, 301–308, <ext-link xlink:href="http://dx.doi.org/10.5194/amt-6-301-2013" ext-link-type="DOI">10.5194/amt-6-301-2013</ext-link>,
2013.</mixed-citation></ref>
      <ref id="bib1.bib27"><label>27</label><mixed-citation>Wada, R., Pearce, J. K., Nakayama, T., Matsumi, Y., Hiyama, T., Inoue, G.,
and Shibata, T.: Observation of carbon and oxygen isotopic compositions of
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> at an urban site in Nagoya using Mid-IR laser absorption
spectroscopy, Atmos. Environ., 45, 1168–1174, 2011.
</mixed-citation></ref><?xmltex \hack{\newpage}?>
      <ref id="bib1.bib28"><label>28</label><mixed-citation>Wahl, E. H., Fidric, B., Rella, C. W., Koulikov, S., Kharlamov, B., Tan, S.,
Kachanov, A. A., Richman, B. A., Crosson, E. R., Paldus, B. A., Kalaskar, S.,
and Bowling, D. R.: Applications of cavity ring-down spectroscopy to high
precision isotope ratio measurement of <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>C <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>C in carbon
dioxide, Isotopes Environ. Health Stud., 42, 21–35,
<ext-link xlink:href="http://dx.doi.org/10.1080/10256010500502934" ext-link-type="DOI">10.1080/10256010500502934</ext-link>, 2006.</mixed-citation></ref>
      <ref id="bib1.bib29"><label>29</label><mixed-citation>Wehr, R., Kassi, S., Romanini, D., and Gianfrani, L.: Optical feedback cavity-enhanced
absorption spectroscopy for in situ measurements of the ratio <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>C: <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>C in CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, Appl. Phys. B-Lasers O., 92, 459–465, 2008.</mixed-citation></ref>
      <ref id="bib1.bib30"><label>30</label><mixed-citation>Wen, X. F., Sun, X. M., Zhang, S. C., Yu, G. R., Sargent, S. D., and Lee, X.:
Continuous measurement of water vapor D/H and <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>18</mml:mn></mml:msup></mml:math></inline-formula>O/<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>16</mml:mn></mml:msup></mml:math></inline-formula>O isotope
ratios in the atmosphere, J. Hydrol., 349, 489–500,
<ext-link xlink:href="http://dx.doi.org/10.1016/j.jhydrol.2007.11.021" ext-link-type="DOI">10.1016/j.jhydrol.2007.11.021</ext-link>, 2008.</mixed-citation></ref>
      <ref id="bib1.bib31"><label>31</label><mixed-citation>Wen, X. F., Zhang, S. C., Sun, X. M., Yu, G. R., and Lee, X.: Water vapor and
precipitation isotope ratios in Beijing, China, J. Geophys. Res.-Atoms., 115,
D01103,  <ext-link xlink:href="http://dx.doi.org/10.1029/2009jd012408" ext-link-type="DOI">10.1029/2009jd012408</ext-link>, 2010.</mixed-citation></ref>
      <ref id="bib1.bib32"><label>32</label><mixed-citation>
Wen, X. F., Lee, X., Sun, X. M., Wang, J. L., Tang, Y. K., Li, S. G., and
Yu, G. R.: Inter-comparison of four commercial analyzers for water vapor
isotope measurement, J. Atmos. Ocean. Tech., 29, 235–247, 2012.</mixed-citation></ref>
      <ref id="bib1.bib33"><label>33</label><mixed-citation>Wen, X.-F., Meng, Y., Zhang, X.-Y., Sun, X.-M., and Lee, X.: Evaluating
calibration strategies for isotope ratio infrared spectroscopy for
atmospheric <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>/<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>12</mml:mn></mml:msup></mml:math></inline-formula>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurement, Atmos. Meas. Tech.,
6, 1491–1501, <ext-link xlink:href="http://dx.doi.org/10.5194/amt-6-1491-2013" ext-link-type="DOI">10.5194/amt-6-1491-2013</ext-link>, 2013.</mixed-citation></ref>
      <ref id="bib1.bib34"><label>34</label><mixed-citation>Werle, P., Mucke, R., and Slemr, F.: The limits of signal averaging in
atmospheric trace-gas monitoring by tunable diode-laser
absorption-spectroscopy (TDLAS), Appl. Phys. B-Photo., 57, 131–139, <ext-link xlink:href="http://dx.doi.org/10.1007/bf00425997" ext-link-type="DOI">10.1007/bf00425997</ext-link>, 1993.</mixed-citation></ref>
      <ref id="bib1.bib35"><label>35</label><mixed-citation>Werner, C., Schnyder, H., Cuntz, M., Keitel, C., Zeeman, M. J., Dawson, T.
E., Badeck, F.-W., Brugnoli, E., Ghashghaie, J., Grams, T. E. E., Kayler, Z.
E., Lakatos, M., Lee, X., Máguas, C., Ogée, J., Rascher, K. G.,
Siegwolf, R. T. W., Unger, S., Welker, J., Wingate, L., and Gessler, A.:
Progress and challenges in using stable isotopes to trace plant carbon and
water relations across scales, Biogeosciences, 9, 3083–3111,
<ext-link xlink:href="http://dx.doi.org/10.5194/bg-9-3083-2012" ext-link-type="DOI">10.5194/bg-9-3083-2012</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bib36"><label>36</label><mixed-citation>Wingate, L., Ogee, J., Burlett, R., Bosc, A., Devaux, M., Grace, J., Loustau,
D., and Gessler, A.: Photosynthetic carbon isotope discrimination and its
relationship to the carbon isotope signals of stem, soil and ecosystem
respiration, New Phytol., 188, 576–589,
<ext-link xlink:href="http://dx.doi.org/10.1111/j.1469-8137.2010.03384.x" ext-link-type="DOI">10.1111/j.1469-8137.2010.03384.x</ext-link>, 2010.</mixed-citation></ref>
      <ref id="bib1.bib37"><label>37</label><mixed-citation>
WMO: Report no. 194. 15th WMO/IAEA Meeting of Experts on Carbon Dioxide,
Other Greenhouse Gases and Related Tracers Measurement Techniques,
GenevaWMO/TD-No. 1553, 2011.</mixed-citation></ref>
      <ref id="bib1.bib38"><label>38</label><mixed-citation>Yakir, D., and Sternberg, L. D. L.: The use of stable isotopes to study
ecosystem gas exchange, Oecologia, 123, 297–311, <ext-link xlink:href="http://dx.doi.org/10.1007/s004420051016" ext-link-type="DOI">10.1007/s004420051016</ext-link>,
2000.</mixed-citation></ref>
      <ref id="bib1.bib39"><label>39</label><mixed-citation>
Zobitz, J. M., Keener, J. P., Schnyder, H., and Bowling, D. R.: Sensitivity
analysis and quantification of uncertainty for isotopic mixing relationships
in carbon cycle research, Agr. Forest Meteorol., 136, 56–75, 2006.</mixed-citation></ref>

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    <!--<article-title-html>Intercomparison of two cavity ring-down spectroscopy analyzers for
atmospheric <sup>13</sup>CO<sub>2</sub>  ∕ <sup>12</sup>CO<sub>2</sub> measurement</article-title-html>
<abstract-html><p class="p">Isotope ratio infrared spectroscopy (IRIS) permits continuous in situ
measurement of CO<sub>2</sub> isotopic composition under ambient conditions.
Previous studies have mainly focused on single IRIS instrument performance;
few studies have considered the comparability among different IRIS
instruments. In this study, we carried out laboratory and ambient
measurements using two Picarro CO<sub>2</sub><i>δ</i><sup>13</sup>C analyzers (G1101-i and
G2201-i (newer version)) and evaluated their performance and comparability.
The best precision was 0.08–0.15 ‰ for
G1101-i and 0.01–0.04 ‰ for G2201-i. The dependence of <i>δ</i><sup>13</sup>C
on CO<sub>2</sub> concentration was 0.46 ‰ per 100 ppm and
0.09 ‰ per 100 ppm, the instrument drift ranged from
0.92–1.09 ‰ and 0.19–0.37 ‰, and the sensitivity of
<i>δ</i><sup>13</sup>C to the water vapor mixing ratio was
1.01 ‰ ∕ % H<sub>2</sub>O  and 0.09 ‰ ∕ % H<sub>2</sub>O for
G1101-i and G2201-i, respectively. The accuracy after correction by the
two-point mixing ratio gain and offset calibration method ranged from
−0.04–0.09 ‰ for G1101-i and −0.13–0.03 ‰ for
G2201-i. The sensitivity of <i>δ</i><sup>13</sup>C to the water vapor mixing ratio
improved from 1.01 ‰ ∕ % H<sub>2</sub>O before the upgrade of
G1101-i (G1101-i-original) to 0.15 ‰ ∕ % H<sub>2</sub>O after the
upgrade of G1101-i (G1101-i-upgraded). Atmospheric <i>δ</i><sup>13</sup>C measured by
G1101-i and G2201-i captured the rapid changes in atmospheric <i>δ</i><sup>13</sup>C
signals on hourly to diurnal cycle scales, with a difference of
0.07 ± 0.24 ‰ between G1101-i-original and G2201-i and
0.05 ± 0.30 ‰ between G1101-i-upgraded and G2201-i. A
significant linear correlation was observed between the <i>δ</i><sup>13</sup>C
difference of G1101-i-original and G2201-i and the water vapor concentration,
but there was no significant correlation between the <i>δ</i><sup>13</sup>C
difference of G1101-i-upgraded and G2201-i and the water vapor concentration.
The difference in the Keeling intercept values decreased from 1.24 ‰
between G1101-i-original and G2201-i to 0.36 ‰ between
G1101-i-upgraded and G2201-i, which indicates the importance of consistency
among different IRIS instruments.</p></abstract-html>
<ref-html id="bib1.bib1"><label>1</label><mixed-citation>
Allan, D. W.: Should the classical variance be used as a basic measure in
standards metrology?, IEEE T. Instrum. Meas., 1001, 646–654, 1987.
</mixed-citation></ref-html>
<ref-html id="bib1.bib2"><label>2</label><mixed-citation>
Bowling, D. R., Sargent, S. D., Tanner, B. D., and Ehleringer, J. R.:
Tunable diode laser absorption spectroscopy for stable isotope studies of
ecosystem-atmosphere CO<sub>2</sub> exchange, Agr. Forest Meteorol., 118, 1–19, <a href="http://dx.doi.org/10.1016/s0168-1923(03)00074-1" target="_blank">doi:10.1016/s0168-1923(03)00074-1</a>, 2003.
</mixed-citation></ref-html>
<ref-html id="bib1.bib3"><label>3</label><mixed-citation>
Bowling, D. R., Burns, S. P., Conway, T. J., Monson, R. K., and White, J. W.
C.: Extensive observations of CO<sub>2</sub> carbon isotope content in and above a
high-elevation subalpine forest, Global Biogeochem. Cy, 19, GB3023, <a href="http://dx.doi.org/10.1029/2004gb002394" target="_blank">doi:10.1029/2004gb002394</a>,
2005.
</mixed-citation></ref-html>
<ref-html id="bib1.bib4"><label>4</label><mixed-citation>
Chen, H., Winderlich, J., Gerbig, C., Hoefer, A., Rella, C. W., Crosson, E.
R., Van Pelt, A. D., Steinbach, J., Kolle, O., Beck, V., Daube, B. C.,
Gottlieb, E. W., Chow, V. Y., Santoni, G. W., and Wofsy, S. C.: High-accuracy
continuous airborne measurements of greenhouse gases (CO<sub>2</sub> and CH<sub>4</sub>)
using the cavity ring-down spectroscopy (CRDS) technique, Atmos. Meas. Tech.,
3, 375–386, <a href="http://dx.doi.org/10.5194/amt-3-375-2010" target="_blank">doi:10.5194/amt-3-375-2010</a>, 2010.
</mixed-citation></ref-html>
<ref-html id="bib1.bib5"><label>5</label><mixed-citation>
Flowers, B. A., Powers, H. H., Dubey, M. K., and McDowell, N. G.:
Inter-comparison of two high-accuracy fast-response spectroscopic sensors of
carbon dioxide: a case study, Atmos. Meas. Tech., 5, 991–997,
<a href="http://dx.doi.org/10.5194/amt-5-991-2012" target="_blank">doi:10.5194/amt-5-991-2012</a>, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib6"><label>6</label><mixed-citation>
Friedrichs, G., Bock, J., Temps, F., Fietzek, P., Kortzinger, A., and
Wallace, D. W. R.: Toward continuous monitoring of seawater
<sup>13</sup>CO<sub>2</sub>/<sup>12</sup>CO<sub>2</sub> isotope ratio and pCO<sub>2</sub>: Performance of
cavity ringdown spectroscopy and gas matrix effects, Limnol. Oceanogr.-Meth., 8, 539–551, <a href="http://dx.doi.org/10.4319/lom.2010.8.539" target="_blank">doi:10.4319/lom.2010.8.539</a>, 2010.
</mixed-citation></ref-html>
<ref-html id="bib1.bib7"><label>7</label><mixed-citation>
Griffis, T. J.: Tracing the flow of carbon dioxide and water vapor between
the biosphere and atmosphere: A review of optical isotope techniques and
their application, Agr. Forest Meteorol., 174, 85–109, <a href="http://dx.doi.org/10.1016/j.agrformet.2013.02.009" target="_blank">doi:10.1016/j.agrformet.2013.02.009</a>, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib8"><label>8</label><mixed-citation>
Griffis, T. J., Baker, J. M., Sargent, S. D., Tanner, B. D., and Zhang, J.:
Measuring field-scale isotopic CO<sub>2</sub> fluxes with tunable diode laser
absorption spectroscopy and micrometeorological techniques, Agr. Forest
Meteorol., 124, 15–29, <a href="http://dx.doi.org/10.1016/j.agrformet.2004.01.009" target="_blank">doi:10.1016/j.agrformet.2004.01.009</a>, 2004.
</mixed-citation></ref-html>
<ref-html id="bib1.bib9"><label>9</label><mixed-citation>
Griffith, D. W. T., Deutscher, N. M., Caldow, C., Kettlewell, G., Riggenbach,
M., and Hammer, S.: A Fourier transform infrared trace gas and isotope
analyser for atmospheric applications, Atmos. Meas. Tech., 5, 2481–2498,
<a href="http://dx.doi.org/10.5194/amt-5-2481-2012" target="_blank">doi:10.5194/amt-5-2481-2012</a>, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib10"><label>10</label><mixed-citation>
Guillon, S., Pili, E., and Agrinier, P.: Using a laser-based CO<sub>2</sub> carbon
isotope analyser to investigate gas transfer in geological media, Applied
Physics B-Lasers and Optics, 107, 449–457, <a href="http://dx.doi.org/10.1007/s00340-012-4942-8" target="_blank">doi:10.1007/s00340-012-4942-8</a>,
2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib11"><label>11</label><mixed-citation>
Hammer, S., Griffith, D. W. T., Konrad, G., Vardag, S., Caldow, C., and
Levin, I.: Assessment of a multi-species in situ FTIR for precise atmospheric
greenhouse gas observations, Atmos. Meas. Tech., 6, 1153–1170,
<a href="http://dx.doi.org/10.5194/amt-6-1153-2013" target="_blank">doi:10.5194/amt-6-1153-2013</a>, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib12"><label>12</label><mixed-citation>
Keeling, C. D.: The concentration and isotopic abundances of atmospheric
carbon dioxide in rural areas, Geochim. Cosmochim. Ac., 13, 322–334, 1958.
</mixed-citation></ref-html>
<ref-html id="bib1.bib13"><label>13</label><mixed-citation>
Kwok, Y. C., Laurent, O., Guemri, A., Philippon, C., Wastine, B., Rella, C.
W., Vuillemin, C., Truong, F., Delmotte, M., Kazan, V., Darding, M.,
Lebègue, B., Kaiser, C., Xueref-Rémy, I., and Ramonet, M.:
Comprehensive laboratory and field testing of cavity ring-down spectroscopy
analyzers measuring H<sub>2</sub>O, CO<sub>2</sub>, CH<sub>4</sub> and CO, Atmos. Meas. Tech.,
8, 3867–3892, <a href="http://dx.doi.org/10.5194/amt-8-3867-2015" target="_blank">doi:10.5194/amt-8-3867-2015</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib14"><label>14</label><mixed-citation>
Levin, I., C. Veidt, B. Vaughn, G. Brailsford, T. Bromley, R. Heinz, D. Lowe,
J. Miller, C. Poß and J. White: No inter-hemispheric <i>δ</i><sup>13</sup>CH<sub>4</sub> trend observed, Nature, 486, E3–E4, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib15"><label>15</label><mixed-citation>
McManus, J. B., Nelson, D. D., Shorter, J. H., Jimenez, R., Herndon, S.,
Saleska, S., and Zahniser, M.: A high precision pulsed quantum cascade laser
spectrometer for measurements of stable isotopes of carbon dioxide,
J. Mod. Optic., 52, 2309–2321,
<a href="http://dx.doi.org/10.1080/09500340500303710" target="_blank">doi:10.1080/09500340500303710</a>, 2005.
</mixed-citation></ref-html>
<ref-html id="bib1.bib16"><label>16</label><mixed-citation>
Mohn, J., Werner, R. A., Buchmann, B., and Emmenegger, L.: High-precision
<i>δ</i><sup>13</sup>CO<sub>2</sub> analysis by FTIR spectroscopy using a novel calibration
strategy, J. Mol. Struct., 834, 95–101, <a href="http://dx.doi.org/10.1016/j.molstruc.2006.09.024" target="_blank">doi:10.1016/j.molstruc.2006.09.024</a>,
2007.
</mixed-citation></ref-html>
<ref-html id="bib1.bib17"><label>17</label><mixed-citation>
Mohn, J., Zeeman, M. J., Werner, R. A., Eugster, W., and Emmenegger, L.:
Continuous field measurements of<i>δ</i><sup>13</sup>CO<sub>2</sub> and trace gases by FTIR
spectroscopy, Isotopes Environ. Health Stud., 44, 241–251,
<a href="http://dx.doi.org/10.1080/10256010802309731" target="_blank">doi:10.1080/10256010802309731</a>, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib18"><label>18</label><mixed-citation>
Nara, H., Tanimoto, H., Tohjima, Y., Mukai, H., Nojiri, Y., Katsumata, K.,
and Rella, C. W.: Effect of air composition (N<sub>2</sub>, O<sub>2</sub>, Ar, and
H<sub>2</sub>O) on CO<sub>2</sub> and CH<sub>4</sub> measurement by wavelength-scanned cavity
ring-down spectroscopy: calibration and measurement strategy, Atmos. Meas.
Tech., 5, 2689–2701, <a href="http://dx.doi.org/10.5194/amt-5-2689-2012" target="_blank">doi:10.5194/amt-5-2689-2012</a>, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib19"><label>19</label><mixed-citation>
Pang, J., Wen, X., and Sun, X.: Mixing ratio and carbon isotopic composition
investigation of atmospheric CO<sub>2</sub> in Beijing, China, Sci. Total Environ.,
539, 322–330, 2016a.
</mixed-citation></ref-html>
<ref-html id="bib1.bib20"><label>20</label><mixed-citation>
Pang, J., Wen, X., Sun, X., and Huang, K.: Inter-comparison of two cavity
ring-down spectroscopy analyzers for atmospheric <sup>13</sup>CO<sub>2</sub>/<sup>12</sup>CO<sub>2</sub>
measurement, available at:
<a href="https://www.researchgate.net/publication/301644542_Inter-comparison_of_two_cavity_ring-down_spectroscopy_analyzers_for_atmospheric_13CO2_12CO2_measurement" target="_blank">https://www.researchgate.net/publication/301644542_Inter-comparison_of_two_cavity_ring-down_spectroscopy_analyzers_for_atmospheric_13CO2_12CO2_measurement</a>,
2016b.
</mixed-citation></ref-html>
<ref-html id="bib1.bib21"><label>21</label><mixed-citation>
Pataki, D. E., Bowling, D. R., Ehleringer, J. R., and Zobitz, J. M.: High
resolution atmospheric monitoring of urban carbon dioxide sources, Geophys.
Res. Lett., 33, L03813, <a href="http://dx.doi.org/10.1029/2005gl024822" target="_blank">doi:10.1029/2005gl024822</a>, 2006.
</mixed-citation></ref-html>
<ref-html id="bib1.bib22"><label>22</label><mixed-citation>
Rella, C. W., Chen, H., Andrews, A. E., Filges, A., Gerbig, C., Hatakka, J.,
Karion, A., Miles, N. L., Richardson, S. J., Steinbacher, M., Sweeney, C.,
Wastine, B., and Zellweger, C.: High accuracy measurements of dry mole
fractions of carbon dioxide and methane in humid air, Atmos. Meas. Tech., 6,
837–860, <a href="http://dx.doi.org/10.5194/amt-6-837-2013" target="_blank">doi:10.5194/amt-6-837-2013</a>, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib23"><label>23</label><mixed-citation>
Schaeffer, S. M., Miller, J. B., Vaughn, B. H., White, J. W. C., and Bowling,
D. R.: Long-term field performance of a tunable diode laser absorption
spectrometer for analysis of carbon isotopes of CO2 in forest air, Atmos.
Chem. Phys., 8, 5263–5277, <a href="http://dx.doi.org/10.5194/acp-8-5263-2008" target="_blank">doi:10.5194/acp-8-5263-2008</a>, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib24"><label>24</label><mixed-citation>
Sturm, P., Eugster, W., and Knohl, A.: Eddy covariance measurements of
CO<sub>2</sub> isotopologues with a quantum cascade laser absorption spectrometer,
Agr. Forest Meteorol., 152, 73–82, <a href="http://dx.doi.org/10.1016/j.agrformet.2011.09.007" target="_blank">doi:10.1016/j.agrformet.2011.09.007</a>,
2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib25"><label>25</label><mixed-citation>
Tuzson, B., Zeeman, M. J., Zahniser, M. S., and Emmenegger, L.: Quantum
cascade laser based spectrometer for in situ stable carbon dioxide isotope
measurements, Infrared Phys. Techn., 51, 198–206,
<a href="http://dx.doi.org/10.1016/j.infrared.2007.05.006" target="_blank">doi:10.1016/j.infrared.2007.05.006</a>, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib26"><label>26</label><mixed-citation>
Vogel, F. R., Huang, L., Ernst, D., Giroux, L., Racki, S., and Worthy, D. E.
J.: Evaluation of a cavity ring-down spectrometer for in situ observations of
<sup>13</sup>CO<sub>2</sub>, Atmos. Meas. Tech., 6, 301–308, <a href="http://dx.doi.org/10.5194/amt-6-301-2013" target="_blank">doi:10.5194/amt-6-301-2013</a>,
2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib27"><label>27</label><mixed-citation>
Wada, R., Pearce, J. K., Nakayama, T., Matsumi, Y., Hiyama, T., Inoue, G.,
and Shibata, T.: Observation of carbon and oxygen isotopic compositions of
CO<sub>2</sub> at an urban site in Nagoya using Mid-IR laser absorption
spectroscopy, Atmos. Environ., 45, 1168–1174, 2011.

</mixed-citation></ref-html>
<ref-html id="bib1.bib28"><label>28</label><mixed-citation>
Wahl, E. H., Fidric, B., Rella, C. W., Koulikov, S., Kharlamov, B., Tan, S.,
Kachanov, A. A., Richman, B. A., Crosson, E. R., Paldus, B. A., Kalaskar, S.,
and Bowling, D. R.: Applications of cavity ring-down spectroscopy to high
precision isotope ratio measurement of <sup>13</sup>C ∕ <sup>12</sup>C in carbon
dioxide, Isotopes Environ. Health Stud., 42, 21–35,
<a href="http://dx.doi.org/10.1080/10256010500502934" target="_blank">doi:10.1080/10256010500502934</a>, 2006.
</mixed-citation></ref-html>
<ref-html id="bib1.bib29"><label>29</label><mixed-citation>
Wehr, R., Kassi, S., Romanini, D., and Gianfrani, L.: Optical feedback cavity-enhanced
absorption spectroscopy for in situ measurements of the ratio <sup>13</sup>C: <sup>12</sup>C in CO<sub>2</sub>, Appl. Phys. B-Lasers O., 92, 459–465, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib30"><label>30</label><mixed-citation>
Wen, X. F., Sun, X. M., Zhang, S. C., Yu, G. R., Sargent, S. D., and Lee, X.:
Continuous measurement of water vapor D/H and <sup>18</sup>O/<sup>16</sup>O isotope
ratios in the atmosphere, J. Hydrol., 349, 489–500,
<a href="http://dx.doi.org/10.1016/j.jhydrol.2007.11.021" target="_blank">doi:10.1016/j.jhydrol.2007.11.021</a>, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib31"><label>31</label><mixed-citation>
Wen, X. F., Zhang, S. C., Sun, X. M., Yu, G. R., and Lee, X.: Water vapor and
precipitation isotope ratios in Beijing, China, J. Geophys. Res.-Atoms., 115,
D01103,  <a href="http://dx.doi.org/10.1029/2009jd012408" target="_blank">doi:10.1029/2009jd012408</a>, 2010.
</mixed-citation></ref-html>
<ref-html id="bib1.bib32"><label>32</label><mixed-citation>
Wen, X. F., Lee, X., Sun, X. M., Wang, J. L., Tang, Y. K., Li, S. G., and
Yu, G. R.: Inter-comparison of four commercial analyzers for water vapor
isotope measurement, J. Atmos. Ocean. Tech., 29, 235–247, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib33"><label>33</label><mixed-citation>
Wen, X.-F., Meng, Y., Zhang, X.-Y., Sun, X.-M., and Lee, X.: Evaluating
calibration strategies for isotope ratio infrared spectroscopy for
atmospheric <sup>13</sup>CO<sub>2</sub>/<sup>12</sup>CO<sub>2</sub> measurement, Atmos. Meas. Tech.,
6, 1491–1501, <a href="http://dx.doi.org/10.5194/amt-6-1491-2013" target="_blank">doi:10.5194/amt-6-1491-2013</a>, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib34"><label>34</label><mixed-citation>
Werle, P., Mucke, R., and Slemr, F.: The limits of signal averaging in
atmospheric trace-gas monitoring by tunable diode-laser
absorption-spectroscopy (TDLAS), Appl. Phys. B-Photo., 57, 131–139, <a href="http://dx.doi.org/10.1007/bf00425997" target="_blank">doi:10.1007/bf00425997</a>, 1993.
</mixed-citation></ref-html>
<ref-html id="bib1.bib35"><label>35</label><mixed-citation>
Werner, C., Schnyder, H., Cuntz, M., Keitel, C., Zeeman, M. J., Dawson, T.
E., Badeck, F.-W., Brugnoli, E., Ghashghaie, J., Grams, T. E. E., Kayler, Z.
E., Lakatos, M., Lee, X., Máguas, C., Ogée, J., Rascher, K. G.,
Siegwolf, R. T. W., Unger, S., Welker, J., Wingate, L., and Gessler, A.:
Progress and challenges in using stable isotopes to trace plant carbon and
water relations across scales, Biogeosciences, 9, 3083–3111,
<a href="http://dx.doi.org/10.5194/bg-9-3083-2012" target="_blank">doi:10.5194/bg-9-3083-2012</a>, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib36"><label>36</label><mixed-citation>
Wingate, L., Ogee, J., Burlett, R., Bosc, A., Devaux, M., Grace, J., Loustau,
D., and Gessler, A.: Photosynthetic carbon isotope discrimination and its
relationship to the carbon isotope signals of stem, soil and ecosystem
respiration, New Phytol., 188, 576–589,
<a href="http://dx.doi.org/10.1111/j.1469-8137.2010.03384.x" target="_blank">doi:10.1111/j.1469-8137.2010.03384.x</a>, 2010.
</mixed-citation></ref-html>
<ref-html id="bib1.bib37"><label>37</label><mixed-citation>
WMO: Report no. 194. 15th WMO/IAEA Meeting of Experts on Carbon Dioxide,
Other Greenhouse Gases and Related Tracers Measurement Techniques,
GenevaWMO/TD-No. 1553, 2011.
</mixed-citation></ref-html>
<ref-html id="bib1.bib38"><label>38</label><mixed-citation>
Yakir, D., and Sternberg, L. D. L.: The use of stable isotopes to study
ecosystem gas exchange, Oecologia, 123, 297–311, <a href="http://dx.doi.org/10.1007/s004420051016" target="_blank">doi:10.1007/s004420051016</a>,
2000.
</mixed-citation></ref-html>
<ref-html id="bib1.bib39"><label>39</label><mixed-citation>
Zobitz, J. M., Keener, J. P., Schnyder, H., and Bowling, D. R.: Sensitivity
analysis and quantification of uncertainty for isotopic mixing relationships
in carbon cycle research, Agr. Forest Meteorol., 136, 56–75, 2006.
</mixed-citation></ref-html>--></article>
