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Compatibility of Atmospheric 14CO2 Measurements: Comparing the Heidelberg Low-Level Counting Facility to International Accelerator Mass Spectrometry (AMS) Laboratories

Published online by Cambridge University Press:  19 September 2016

Samuel Hammer*
Affiliation:
Institut für Umweltphysik, Heidelberg University, Germany
Ronny Friedrich
Affiliation:
Curt Engelhorn Center for Archaeometry gGmbH, Mannheim, Germany
Bernd Kromer
Affiliation:
Institut für Umweltphysik, Heidelberg University, Germany Curt Engelhorn Center for Archaeometry gGmbH, Mannheim, Germany
Alexander Cherkinsky
Affiliation:
Center for Applied Isotope Studies, University of Georgia, USA
Scott J Lehman
Affiliation:
INSTAAR, University of Colorado, Boulder, Colorado, USA
Harro A J Meijer
Affiliation:
Centre for Isotope Research (CIO), Energy and Sustainability Research Institute Groningen (ESRIG), University of Groningen, the Netherlands
Toshio Nakamura
Affiliation:
Center for Chronological Research, Nagoya University, Japan
Vesa Palonen
Affiliation:
Department of Physics, University of Helsinki, Finland
Ron W Reimer
Affiliation:
14CHRONO Centre for Climate, the Environment and Chronology,School of Geography, Archaeology and Palaeoecology, Queen’s University Belfast, UK
Andrew M Smith
Affiliation:
Australian Nuclear Science and Technology Organisation, Lucas Heights, NSW 2234, Australia
John R Southon
Affiliation:
Earth System Science Department, University of California, Irvine, California 92612, USA
Sönke Szidat
Affiliation:
Department of Chemistry and Biochemistry & Oeschger Centre for Climate Change Research, University of Bern, Switzerland
Jocelyn Turnbull
Affiliation:
National Isotope Centre, GNS Science New Zealand and CIRES, University of Colorado, USA
Masao Uchida
Affiliation:
National Institute for Environmental Studies, Tsukuba, Japan
*
*Corresponding author. Email: shammer@iup.uni-heidelberg.de.
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Abstract

Combining atmospheric Δ14CO2 data sets from different networks or laboratories requires secure knowledge on their compatibility. In the present study, we compare Δ14CO2 results from the Heidelberg low-level counting (LLC) laboratory to 12 international accelerator mass spectrometry (AMS) laboratories using distributed aliquots of five pure CO2 samples. The averaged result of the LLC laboratory has a measurement bias of –0.3±0.5‰ with respect to the consensus value of the AMS laboratories for the investigated atmospheric Δ14C range of 9.6 to 40.4‰. Thus, the LLC measurements on average are not significantly different from the AMS laboratories, and the most likely measurement bias is smaller than the World Meteorological Organization (WMO) interlaboratory compatibility goal for Δ14CO2 of 0.5‰. The number of intercomparison samples was, however, too small to determine whether the measurement biases of the individual AMS laboratories fulfilled the WMO goal.

Type
Advances in Physical Measurement Techniques
Copyright
© 2016 by the Arizona Board of Regents on behalf of the University of Arizona 

INTRODUCTION

The Heidelberg global atmospheric 14CO2 sampling network (Levin et al. Reference Levin, Naegler, Kromer, Diehl, Francey, Gomez-Pelaez, Steel, Wagenbach, Weller and Worthy2010) is unique in terms of its spatial and temporal coverage. The tropospheric measurements cover the bomb peak in the Northern Hemisphere and have thus, among other reasons, become of major importance after other laboratories largely discontinued their global observations (e.g. Nydal and Lövseth Reference Nydal and Lövseth1983). Current 14CO2 observations are not only used for global carbon cycle research (e.g. Levin and Kromer 2004; Naegler et al. Reference Naegler, Ciais, Rodgers and Levin2006; Turnbull et al. Reference Turnbull, Rayner, Miller, Naegler, Ciais and Cozic2009; Levin et al. Reference Levin, Naegler, Kromer, Diehl, Francey, Gomez-Pelaez, Steel, Wagenbach, Weller and Worthy2010, Reference Levin, Kromer and Hammer2013; Francey et al. Reference Francey, Trudinger, van der Schoot, Law, Krummel, Langenfelds, Steele, Allison, Stavert, Andres and Rodenbeck2013), but they are also applied in various other research disciplines. These range from firn core studies (e.g. Buizert et al. Reference Buizert, Martinerie, Petrenko, Severinghaus, Trudinger, Witrant, Rosen, Orsi, Rubino, Etheridge, Steele, Hogan, Laube, Sturges, Levchenko, Smith, Levin, Conway, Dlugokencky, Lang, Kawamura, Jenk, White, Sowers, Schwander and Blunier2012), aerosol source attribution (e.g. Gelencsér et al. Reference Gelencsér, May, Simpson, Sánchez-Ochoa, Kasper-Giebl, Puxbaum, Caseiro, Pio and Legrand2007), soil carbon turnover (e.g. Trumbore Reference Trumbore1993; Lindahl et al. Reference Lindahl, Ihrmark, Boberg, Trumbore, Högberg, Stenlid and Finlay2007), to neuroscience (e.g. Spalding et al. Reference Spalding, Bergmann, Alkass, Bernard, Salehpour, Huttner and Possnert2013) and forensics (e.g. Santos et al. Reference Santos, De La Torre, Boudin, Bonafini and Saverwyns2015), just to name a few of the many applications.

The sampling strategy in the Heidelberg 14CO2 network (i.e. weekly or biweekly integrated absorption of atmospheric CO2 in NaOH solution) is similar for all stations and has remained essentially unchanged since the inception of the network in 1959. A detailed description of the sampling procedures is available in Levin et al. (Reference Levin, Münnich and Weiss1980). All of the samples have been analyzed using gas proportional counting in the Heidelberg low-level laboratory. The counting facilities are described in depth by Kromer and Münnich (Reference Kromer and Münnich1992). These two constant features have been fundamental to achieving and maintaining highest intranetwork compatibility.

Over the last 2 decades, other global 14CO2 networks and single stations (Turnbull et al. Reference Turnbull, Lehman, Miller, Sparks, Southon and Tans2007; Graven et al. Reference Graven, Guilderson and Keeling2012) have become operational. All of these new data sets make use of accelerator mass spectrometry (AMS) analyses of whole air samples. Combining 14C data sets from different groups comprising different measurement techniques immediately raises the question of intertechnique and interlaboratory compatibility. This is especially crucial for atmospheric studies since the 14CO2 gradients in background air are very small (Levin et al. Reference Levin, Naegler, Kromer, Diehl, Francey, Gomez-Pelaez, Steel, Wagenbach, Weller and Worthy2010). The World Meteorological Organization–Global Atmosphere Watch (WMO-GAW) guidelines have therefore set a desired level of interlaboratory compatibility (ILC) of only 0.5‰ (WMO-GAW 2013). It should be noted that the compatibility goal refers to the averaged deviation between laboratories and not the uncertainty of individual samples.

Traditionally, 14C labs perform internal quality-control (QC) checks by measuring secondary standard reference materials, such as those provided by the IAEA (Rozanski et al. Reference Rozanski, Stichler, Gonfiantini, Scott, Beukens, Kromer and van der Plicht1992). However, only a few laboratories make those QC results publicly available. In addition to the laboratory internal QC, the 14C community has a long tradition of performing intercomparison exercises. The most recent intercomparison was carried out from 2004 to 2008, called VIRI (Scott et al. Reference Scott, Cook, Naysmith, Bryant and O’Donnell2007), with 70 participating labs. The 14C activities of the distributed materials ranged from 0 to 110 pMC. One aim of VIRI was to examine the effects of sample preparation for a range of materials to determine the amount of total variability that may be associated with pretreatment. For the samples with recent activity, an overall 1σ standard deviation of 25‰ was found (including all outliers). Comparing only the AMS laboratories resulted in much better compatibility of 5 to 6‰. This is due to the typical practice, when using AMS, of measurement and normalization to primary reference materials (typically OxI or OxII), in the same measurement sequence as the unknown samples. Counting techniques do not permit such within-run calibration and are instead dependent on careful periodic calibration (compare Kromer and Münnich Reference Kromer and Münnich1992), which is subsequently interpolated to the point in time when the measurement of the unknown sample took place.

The atmospheric 14CO2 community identified a need for an additional intercomparison program, which is more tailored towards ambient atmospheric activities and sample handling procedures. So far, two dedicated atmospheric intercomparisons have been published. Graven et al. (Reference Graven, Xu, Guilderson, Keeling, Trumbore and Tyler2013) made use of co-located sampling of two different sampling programs at Point Barrow, Alaska, testing thereby the entire data genesis from sampling through sample preparation and analysis. Graven et al. (Reference Graven, Xu, Guilderson, Keeling, Trumbore and Tyler2013) report on 22 samples (analyzed and pretreated in two independent AMS laboratories) with an overall agreement of the two data sets of 0.2±0.7‰. This result is certainly remarkable and proves that the WMO-GAW interlaboratory compatibility goal is achievable. Since not all laboratories involved in atmospheric 14C measurement have access to co-located sampling, Miller et al. (Reference Miller, Lehman, Wolak, Turnbull, Dunn, Graven, Keeling, Meijer, Aerts-Bijma, Palstra, Smith, Allison, Southon, Xu, Nakazawa, Aoki, Nakamura, Guilderson, LaFranchi, Mukai, Terao, Uchida and Kondo2013) initiated a flask intercomparison program (ICP) for 14CO2. In this program, the flasks of the participating laboratories are filled with atmospheric air from high-pressure cylinders. Miller et al. (Reference Miller, Lehman, Wolak, Turnbull, Dunn, Graven, Keeling, Meijer, Aerts-Bijma, Palstra, Smith, Allison, Southon, Xu, Nakazawa, Aoki, Nakamura, Guilderson, LaFranchi, Mukai, Terao, Uchida and Kondo2013) have so far accomplished three intercomparison rounds with eight participating laboratories. Three of the labs showed compatibility within 1‰ and four of them within 2‰. The Heidelberg LLC laboratory cannot participate in such flask ICP exercises since samples for low-level counting require around 20 m3 of atmospheric air, greatly exceeding the available sample size of those ICPs. Therefore, we were encouraged by the WMO-GAW community to undertake a focused ICP program that would link the Heidelberg LLC to state-of-the-art AMS laboratories. The results of this ICP are reported in the present paper; they are important for three reasons:

  1. 1. Comparing two independent and fundamentally different measurement techniques, which determine the same physical quantity, i.e. 14C activity, is essential and reassuring in itself.

  2. 2. The Heidelberg global 14CO2 network, for the sake of continuity, will carry on applying the same sampling and analysis techniques for the coming years. Therefore, secure constraints on possible interlaboratory deviations, at least for the analytical part, is vital when combining data sets from different networks in global 14CO2 assimilation models.

  3. 3. The Heidelberg radiocarbon laboratory was recently transferred into the ICOS Central Radiocarbon Laboratory (CRL) (www.icos-ri.eu), and plans to use both analytical techniques, LLC and AMS, to provide coherent information on European 14CO2 activities.

FIRST PURE CO2 INTERCOMPARISON EXERCISE

The ICOS CRL initiated a pure CO2 ICP exercise where 12 international AMS laboratories agreed to participate (see Table 1). We used five pure CO2 samples, which were analyzed by low-level counting, split volumetrically into 1-mg C aliquots and stored in break seals. In total, 20 aliquots of each pure CO2 sample were prepared and distributed among the participating AMS labs in a blind test (1 aliquot of each sample per lab). Some labs (e.g. lab 12) indicated interest in participating in the ICP only after the first results have been presented at conferences.

Table 1 Participating laboratories in alphabetical order, which is not identical to the lab number used in this study.

The five pure CO2 samples were selected to have recent atmospheric 14C activities and to span a considerable δ13C range as listed in Table 2. We chose one sample to be oxalic acid I (SRM 4990B) in order to provide one independent reference sample of known value. All labs reported Δ14C according to Equation 1, along with δ13C from the AMS and/or isotope ratio mass spectrometry (IRMS), together with the respective uncertainties:

(1) $$\Delta {}^{{14}}{\rm C({\permil}){\equals}}\left\{ {\left[ {\left( {{{R_{{sam}} } \over {R_{{ref}} }}} \right)\left( {{{1{\plus}{{{\minus}25} \over {1000}}} \over {1{\plus}{{\delta ^{{13}} {\rm C}_{{sam}} } \over {1000}}}}} \right)^{2} e^{{\lambda (1950{\minus}t)}} } \right]{\minus}1} \right\}\cdot 1000$$

where R denotes the ratio of 14C to C in the sample or the reference, t is the date of sample collection, and δ13C sam is the 13C/12C ratio of the sample with respect to VPDB scale. Note that this Δ14C definition is equivalent to the definition of Δ in Stuiver and Polach (Reference Stuiver and Polach1977).

Table 2 Summary of the ICP samples.

RESULTS

The main focus of this study is to determine the compatibility of the Heidelberg LLC with the international AMS laboratories performing atmospheric 14CO2 measurements. Moreover, we can investigate whether such an ICP exercise is also suitable to further evaluate the 0.5‰ WMO-GAW interlaboratory compatibility goal among the individual AMS labs. Some labs have reported issues with processing the pure CO2 aliquots. A common problem was the apparently large size of the break seals, requiring modification of vacuum-sealed crackers and/or splitting of samples. Table 3 summarizes the reported problems in the different laboratories.

Table 3 Remarks and problems with the ICP samples as reported by the laboratories.

We followed a two-stage data evaluation approach. First, the medians for all samples were calculated using data from all AMS laboratories. According to those median values, the reduced χ² red (see Table 4) was calculated for each laboratory according to Equation 2:

(2) $$\chi ^{2} _{{red}} {\equals}{{\chi ^{2} } \over {N{\minus}1}}{\equals}{1 \over {N{\minus}1}}.\mathop{\sum}\limits_{i{\equals}1}^n {{{(x_{i} {\minus}\bar{x}_{i} )^{2} } \over {\sigma ^{2} _{i} }}} $$

where x i and σ i denote the individual measurement and its reported 1σ uncertainty, $\bar{x}_{i} $ is the median of all laboratories for sample i, and N is the total number of analyzed aliquots per sample. Based on this preliminary evaluation, three laboratories (labs 3, 6, and 11) showed very large reduced χ² values (>6), indicating that the spread in their results is not compatible with the provided measurement uncertainties (likelihood <1%). Therefore, the results of those labs have been excluded in the calculation of the consensus values for the five samples.

Table 4 Measurement bias (i.e. mean difference of measured Δ14C minus consensus value for all five CO2 samples) and respective uncertainties given as standard error of the mean. In addition, the reduced χ² values are listed, based on the consensus value and the median (see text for explanation). Results from laboratories marked by an asterisk have not been included in the calculation of the consensus value.

In the second step, we calculated the consensus values (i.e. weighted means, compare Equation 3) for each of the five CO2 samples based on the results of the remaining AMS laboratories excluding lab 3, 6, and 11. The weight of each measurement was chosen as inverse of its squared uncertainty. The uncertainty of the consensus value was calculated according to Equation 4:

(3) $$\bar{x}{\equals}{{\mathop{\sum}\nolimits_{i{\equals}1}^n {\left( {x_{i} \sigma _{i} ^{{{\minus}2}} } \right)} } \over {\mathop{\sum}\nolimits_{i{\equals}1}^n {\sigma _{i} ^{{{\minus}2}} } }}$$
(4) $$\sigma _{{\bar{x}}}^{2} {\equals}{1 \over {\mathop{\sum}\nolimits_{i{\equals}1}^n {\sigma _{i}^{{{\minus}2}} } }}$$

The differences between the individual aliquot measurements and the respective consensus values were calculated for all labs, including the LLC laboratory. The uncertainty of the difference is the propagation of the uncertainty of the consensus value and the measurement error in quadrature. Figure 1 shows the deviations of all laboratories to the consensus value (of this study) for the OxI sample, which is 40.4±0.7‰ (normalized to δ13C=−25‰). The uncertainty of the consensus value is represented as the gray shaded area in Figure 1. Comparing our consensus value to the nominal value of OxI, which is 39.8‰ (normalized to δ13C=−25‰) (red dashed line in Figure 1), shows that it is accurate within its 1σ uncertainty.

Figure 1 Differences of the individual labs to the consensus value of sample 30874 (OxI). The gray shaded area indicates the uncertainty of the consensus value. The difference between the consensus value and the nominal value of the NIST oxalic acid I (SRM 4990B) is shown as red dashed line. Lab 6 reported insufficient graphitization for this sample 30874.

A similar evaluation for all five samples is shown in Figure 2, summarizing all results of the pure CO2 ICP samples. The averaged differences of all five samples from the consensus values is defined as measurement bias of the individual laboratory. The uncertainty of the measurement bias is calculated as the standard error of the mean difference. The LLC measurement bias is −0.3±0.5‰ and is thus not significant. The measurement biases for the individual laboratories along with their uncertainties and the reduced χ2 values based on the consensus value (calculated according to Equation 2, replacing the median with the consensus value) are also given in Table 4. Considering the uncertainty of the measurement bias of each AMS lab, which describes how well the measurement bias can be known from five samples, it is evident that the number of samples used in this exercise is too low to determine whether the 0.5‰ interlaboratory compatibility (ILC) goal is met by each AMS laboratory. Assuming a 2‰ measurement uncertainty, approximately 50 samples would be needed for reducing the error of the measurement bias to better than 0.3‰ (assuming Gaussian distributions). As highlighted by the results of lab 4, which had prepared duplicate sets of AMS targets, measured 1 month apart, the temporal variability within a laboratory needs also to be considered. Although our study has too little statistical significance to judge regarding the 0.5‰ ILC goal, we can still conclude that the measurement bias of three AMS labs is within 1‰ and for six labs within 2‰.

Figure 2 Summary of all ICP results. The difference for each sample to the consensus value based on 9 labs is shown. Labs 3, 6, and 11 have been excluded from calculation of the consensus value (compare also reduced χ2 vs. the median in Table 4 for those labs). The measurements in brackets from labs 5 and 6 are subject to sample handling problems (compare Table 3).

CONCLUSIONS

In this study, we prepared aliquots of five pure CO2 samples, which have been analyzed for 14C activity by low-level counting and by 12 labs by AMS. The averaged LLC result agrees well with the overall averaged AMS results to within –0.3±0.5‰. Thus, the most likely LLC measurement bias accomplishes the WMO-GAW interlaboratory compatibility goal. However, taking into account the uncertainty of the individual 14C analyses, and thus the resulting uncertainty of the measurement bias, the number of samples was too small to determine whether the LLC nor the individual AMS laboratories met the Δ14CO2 compatibility goal. We plan to address this shortcoming in a second pure CO2 ICP round in the near future, in which 10 aliquots for each of the five samples will be distributed to each laboratory. This should provide the statistics needed to address whether the 0.5‰ ILC goal is satisfied by the individual AMS labs. However, since a significant amount of work is associated to prepare this large quantity of aliquots, the number of participating labs will be reduced to those performing atmospheric background 14CO2 observations. Note that the ultimate aim of this exercise is to merge individual data sets from different labs, thus providing optimum benefit for global carbon cycle research.

ACKNOWLEDGMENTS

We are deeply indebted to Ingeborg Levin who initiated, pushed forward and greatly supported this study. This work would also not have been possible without the help of Sabine Kühr and Eva Gier, technicians at the ICOS CRL lab, who prepared the aliquots for the ICP exercise with utmost care. This work has been funded by the German Ministry of Education and Research (Project No. 01LK1225A).

Footnotes

Selected Papers from the 2015 Radiocarbon Conference, Dakar, Senegal, 16–20 November 2015

References

REFERENCES

Buizert, C, Martinerie, P, Petrenko, VV, Severinghaus, JP, Trudinger, CM, Witrant, E, Rosen, JL, Orsi, AJ, Rubino, M, Etheridge, DM, Steele, LP, Hogan, C, Laube, JC, Sturges, WT, Levchenko, VA, Smith, AM, Levin, I, Conway, TJ, Dlugokencky, EJ, Lang, PM, Kawamura, K, Jenk, TM, White, JWC, Sowers, T, Schwander, J, Blunier, T. 2012. Gas transport in firn: multiple-tracer characterisation and model intercomparison for NEEM, Northern Greenland. Atmospheric Chemistry and Physics 12:42594277.Google Scholar
Francey, RJ, Trudinger, CM, van der Schoot, M, Law, RM, Krummel, PB, Langenfelds, RL, Steele, LP, Allison, C, Stavert, A, Andres, R, Rodenbeck, C. 2013. Atmospheric verification of anthropogenic CO2 emission trends. Nature Climate Change 3(5):520524.Google Scholar
Gelencsér, A, May, B, Simpson, D, Sánchez-Ochoa, A, Kasper-Giebl, A, Puxbaum, H, Caseiro, A, Pio, C, Legrand, M. 2007. Source apportionment of PM2.5 organic aerosol over Europe: primary/secondary, natural/anthropogenic, and fossil/biogenic origin. Journal of Geophysical Research 112:D23S04.Google Scholar
Graven, HD, Guilderson, TP, Keeling, RF. 2012. Observations of radiocarbon in CO2 at seven global sampling sites in the Scripps flask network: analysis of spatial gradients and seasonal cycles. Journal of Geophysical Research 117:D02303.Google Scholar
Graven, H, Xu, X, Guilderson, TP, Keeling, RF, Trumbore, SE, Tyler, S. 2013. Comparison of independent delta 14CO2 records at Point Barrow, Alaska. Radiocarbon 55(2–3):15411545.Google Scholar
Kromer, B, Münnich, KO. 1992. CO2 gas proportional counting in radiocarbon dating—review and perspective. In: Taylor RE, Long A, Kra S, editors. Radiocarbon after Four Decades. New York: Springer. p 184197.Google Scholar
Levin, I, Naegler, T, Kromer, B, Diehl, M, Francey, RJ, Gomez-Pelaez, AJ, Steel, LP, Wagenbach, D, Weller, R, Worthy, DE. 2010. Observations and modelling of the global distribution and long-term trend of atmospheric 14CO2 . Tellus B 62:2646.Google Scholar
Levin, I, Kromer, B. 2004. The tropospheric 14CO2 level in mid-latitudes of the Northern Hemisphere (1959–2003). Radiocarbon 46(3):12611272.CrossRefGoogle Scholar
Levin, I, Münnich, KO, Weiss, W. 1980. The effect of anthropogenic CO2 and 14C sources on the distribution of 14CO2 in the atmosphere. Radiocarbon 22(2):379391.Google Scholar
Levin, I, Kromer, B, Hammer, S. 2013. Atmospheric Δ14CO2 trend in Western European background air from 2000 to 2012. Tellus B 65:20092.Google Scholar
Lindahl, BD, Ihrmark, K, Boberg, J, Trumbore, SE, Högberg, P, Stenlid, J, Finlay, RD. 2007. Spatial separation of litter decomposition and mycorrhizal nitrogen uptake in a boreal forest. New Phytologist 173(3):611620.CrossRefGoogle Scholar
Miller, J, Lehman, S, Wolak, C, Turnbull, J, Dunn, G, Graven, H, Keeling, R, Meijer, H, Aerts-Bijma, A, Palstra, S, Smith, A, Allison, C, Southon, J, Xu, X, Nakazawa, T, Aoki, S, Nakamura, T, Guilderson, T, LaFranchi, B, Mukai, H, Terao, Y, Uchida, M, Kondo, M. 2013. Initial results of an intercomparison of AMS-based atmospheric 14CO2 measurements. Radiocarbon 55(2–3):14751483.Google Scholar
Naegler, T, Ciais, P, Rodgers, KB, Levin, I. 2006. Excess radiocarbon constraints on air-sea gas exchange and the uptake of CO2 by the oceans. Geophysical Research Letters 33:L11802.Google Scholar
Nydal, R, Lövseth, K. 1983. Tracing bomb 14C in the atmosphere 1962–1980. Journal of Geophysical Research 88(C6):36213642.Google Scholar
Rozanski, K, Stichler, W, Gonfiantini, R, Scott, EM, Beukens, RP, Kromer, B, van der Plicht, J. 1992. The IAEA 14C Intercomparison Exercise 1990. Radiocarbon 34(3):506519.Google Scholar
Santos, GM, De La Torre, HAM, Boudin, M, Bonafini, M, Saverwyns, S. 2015. Improved radiocarbon analyses of modern human hair to determine the year-of-death by cross-flow nanofiltered amino acids: common contaminants, implications for isotopic analysis, and recommendations. Rapid Communications in Mass Spectrometry 29(19):17651773.Google Scholar
Scott, E, Cook, G, Naysmith, P, Bryant, C, O’Donnell, D. 2007. A report on Phase 1 of the 5th International Radiocarbon Intercomparison (VIRI). Radiocarbon 49(2):409426.Google Scholar
Spalding, KL, Bergmann, O, Alkass, K, Bernard, S, Salehpour, M, Huttner, HB, Possnert, G. 2013. Dynamics of hippocampal neurogenesis in adult humans. Cell 153(6):12191227.Google Scholar
Stuiver, M, Polach, H. 1977. Discussion: reporting of 14C data. Radiocarbon 19(3):355363.CrossRefGoogle Scholar
Trumbore, SE. 1993. Comparison of carbon dynamics in tropical and temperate soils using radiocarbon measurements. Global Biogeochemical Cycles 7(2):275290.Google Scholar
Turnbull, JC, Lehman, SJ, Miller, JB, Sparks, RJ, Southon, JR, Tans, PP. 2007. A new high precision 14CO2 time series for North American continental air. Journal of Geophysical Research 112:D11310.Google Scholar
Turnbull, J, Rayner, P, Miller, J, Naegler, T, Ciais, P, Cozic, A. 2009. On the use of 14CO2 as a tracer for fossil fuel CO2: quantifying uncertainties using an atmospheric transport model. Journal of Geophysical Research 114:D22302.Google Scholar
WMO-GAW (World Meteorological Organization–Global Atmosphere Watch). 2013. 17th WMO/IAEA Meeting of Experts on Carbon Dioxide, Other Greenhouse Gases, and Related Tracer Measurement Techniques. Volume 213, Global Atmosphere Watch. Beijing, China, 10–14 June 2013.Google Scholar
Figure 0

Table 1 Participating laboratories in alphabetical order, which is not identical to the lab number used in this study.

Figure 1

Table 2 Summary of the ICP samples.

Figure 2

Table 3 Remarks and problems with the ICP samples as reported by the laboratories.

Figure 3

Table 4 Measurement bias (i.e. mean difference of measured Δ14C minus consensus value for all five CO2 samples) and respective uncertainties given as standard error of the mean. In addition, the reduced χ² values are listed, based on the consensus value and the median (see text for explanation). Results from laboratories marked by an asterisk have not been included in the calculation of the consensus value.

Figure 4

Figure 1 Differences of the individual labs to the consensus value of sample 30874 (OxI). The gray shaded area indicates the uncertainty of the consensus value. The difference between the consensus value and the nominal value of the NIST oxalic acid I (SRM 4990B) is shown as red dashed line. Lab 6 reported insufficient graphitization for this sample 30874.

Figure 5

Figure 2 Summary of all ICP results. The difference for each sample to the consensus value based on 9 labs is shown. Labs 3, 6, and 11 have been excluded from calculation of the consensus value (compare also reduced χ2 vs. the median in Table 4 for those labs). The measurements in brackets from labs 5 and 6 are subject to sample handling problems (compare Table 3).