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  • 1
    In: Atmospheric Chemistry and Physics, Copernicus GmbH, Vol. 21, No. 9 ( 2021-05-05), p. 6857-6873
    Abstract: Abstract. We present novel measurements of the carbon isotope composition of CFC-11 (CCl3F), CFC-12 (CCl2F2), and CFC-113 (CF2ClCFCl2), three atmospheric trace gases that are important for both stratospheric ozone depletion and global warming. These measurements were carried out on air samples collected in the stratosphere – the main sink region for these gases – and on air extracted from deep polar firn snow. We quantify, for the first time, the apparent isotopic fractionation, ϵapp(13C), for these gases as they are destroyed in the high- and mid-latitude stratosphere: ϵapp(CFC-12, high-latitude) =(-20.2±4.4) ‰, and ϵapp(CFC-113, high-latitude) =(-9.4±4.4) ‰, ϵapp(CFC-12, mid-latitude) =(-30.3±10.7) ‰, and ϵapp(CFC-113, mid-latitude) =(-34.4±9.8) ‰. Our CFC-11 measurements were not sufficient to calculate ϵapp(CFC-11), so we instead used previously reported photolytic fractionation for CFC-11 and CFC-12 to scale our ϵapp(CFC-12), resulting in ϵapp(CFC-11, high-latitude) =(-7.8±1.7) ‰ and ϵapp(CFC-11, mid-latitude) =(-11.7±4.2) ‰. Measurements of firn air were used to construct histories of the tropospheric isotopic composition, δT(13C), for CFC-11 (1950s to 2009), CFC-12 (1950s to 2009), and CFC-113 (1970s to 2009), with δT(13C) increasing for each gas. We used ϵapp(high-latitude), which was derived from more data, and a constant isotopic composition of emissions, δE(13C), to model δT(13C, CFC-11), δT(13C, CFC-12), and δT(13C, CFC-113). For CFC-11 and CFC-12, modelled δT(13C) was consistent with measured δT(13C) for the entire period covered by the measurements, suggesting that no dramatic change in δE(13C, CFC-11) or δE(13C, CFC-12) has occurred since the 1950s. For CFC-113, our modelled δT(13C, CFC-113) did not agree with our measurements earlier than 1980. This discrepancy may be indicative of a change in δE(13C, CFC-113). However, this conclusion is based largely on a single sample and only just significant outside the 95 % confidence interval. Therefore more work is needed to independently verify this temporal trend in the global tropospheric 13C isotopic composition of CFC-113. Our modelling predicts increasing δT(13C, CFC-11), δT(13C, CFC-12), and δT(13C, CFC-113) into the future. We investigated the effect of recently reported new CFC-11 emissions on background δT(13C, CFC-11) by fixing model emissions after 2012 and comparing δT(13C, CFC-11) in this scenario to the model base case. The difference in δT(13C, CFC-11) between these scenarios was 1.4 ‰ in 2050. This difference is smaller than our model uncertainty envelope and would therefore require improved modelling and measurement precision as well as better quantified isotopic source compositions to detect.
    Type of Medium: Online Resource
    ISSN: 1680-7324
    Language: English
    Publisher: Copernicus GmbH
    Publication Date: 2021
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  • 2
    In: Atmospheric Chemistry and Physics, Copernicus GmbH, Vol. 17, No. 7 ( 2017-04-05), p. 4539-4564
    Abstract: Abstract. N2O is currently the third most important anthropogenic greenhouse gas in terms of radiative forcing and its atmospheric mole fraction is rising steadily. To quantify the growth rate and its causes over the past decades, we performed a multi-site reconstruction of the atmospheric N2O mole fraction and isotopic composition using new and previously published firn air data collected from Greenland and Antarctica in combination with a firn diffusion and densification model. The multi-site reconstruction showed that while the global mean N2O mole fraction increased from (290 ± 1) nmol mol−1 in 1940 to (322 ± 1) nmol mol−1 in 2008, the isotopic composition of atmospheric N2O decreased by (−2.2 ± 0.2) ‰ for δ15Nav, (−1.0 ± 0.3) ‰ for δ18O, (−1.3 ± 0.6) ‰ for δ15Nα, and (−2.8 ± 0.6) ‰ for δ15Nβ over the same period. The detailed temporal evolution of the mole fraction and isotopic composition derived from the firn air model was then used in a two-box atmospheric model (comprising a stratospheric box and a tropospheric box) to infer changes in the isotopic source signature over time. The precise value of the source strength depends on the choice of the N2O lifetime, which we choose to fix at 123 years. The average isotopic composition over the investigated period is δ15Nav =  (−7.6 ± 0.8) ‰ (vs. air-N2), δ18O  =  (32.2 ± 0.2) ‰ (vs. Vienna Standard Mean Ocean Water – VSMOW) for δ18O, δ15Nα =  (−3.0 ± 1.9) ‰ and δ15Nβ =  (−11.7 ± 2.3) ‰. δ15Nav, and δ15Nβ show some temporal variability, while for the other signatures the error bars of the reconstruction are too large to retrieve reliable temporal changes. Possible processes that may explain trends in 15N are discussed. The 15N site preference ( = δ15Nα − δ15Nβ) provides evidence of a shift in emissions from denitrification to nitrification, although the uncertainty envelopes are large.
    Type of Medium: Online Resource
    ISSN: 1680-7324
    Language: English
    Publisher: Copernicus GmbH
    Publication Date: 2017
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  • 3
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2003
    In:  Geophysical Research Letters Vol. 30, No. 7 ( 2003-04)
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 30, No. 7 ( 2003-04)
    Type of Medium: Online Resource
    ISSN: 0094-8276
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2003
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  • 4
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2001
    In:  Journal of Geophysical Research: Atmospheres Vol. 106, No. D10 ( 2001-05-27), p. 10403-10410
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 106, No. D10 ( 2001-05-27), p. 10403-10410
    Abstract: Nitrous oxide (N 2 O) extracted from stratospheric whole air samples has been analyzed for its 15 N and 18 O isotopic composition, and strong enrichments in the heavy isotopes are observed concomitant with decreasing N 2 O mixing ratio. Notably, the 15 N enrichment is strongly different at the two nonequivalent positions in the molecule. Laboratory broadband photolysis experiments at wavelengths representative for the stratosphere confirm that photolysis is the prime cause for the observed fractionation in the stratosphere. However, the in situ stratospheric fractionation constants are significantly reduced compared to the laboratory data, reflecting the importance of dynamic processes. In addition, small but significant variations in the ratio of the two 15 N fractionation constants indicate the influence of additional chemical processes like the oxidation of N 2 O by O( 1 D ).
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2001
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  • 5
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2001
    In:  Geophysical Research Letters Vol. 28, No. 3 ( 2001-02), p. 503-506
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 28, No. 3 ( 2001-02), p. 503-506
    Abstract: Analysis of the complete oxygen isotopic composition ( 16 O, 17 O, 18 O) of tropospheric N 2 O from various northern hemispheric locations reveals a mass independent anomaly with a 17 O excess of Δ 17 O = 1.0±0.2‰ at δ 18 O = 20.7±0.3‰. So far, the origin of this intriguing isotope signature has remained elusive. New laboratory experiments demonstrate that the fractionation during UV photolysis of N 2 O, which causes 15 N and 18 O enrichments in the stratosphere, is strictly mass dependent (Δ 17 O = 0). To explain the isotope anomaly in atmospheric N 2 O, we propose a chemical mechanism for heavy oxygen transfer from O 3 to N 2 O. In a first step, the NO x ‐O 3 photochemical interaction leads to the formation of NO 2 with significant excess 17 O. In a second step, the heavy oxygen anomaly is transferred to N 2 O via the reaction , as part of the gas phase degradation of ammonia. This small but significant N 2 O source is of the right magnitude to explain the tropospheric observations.
    Type of Medium: Online Resource
    ISSN: 0094-8276 , 1944-8007
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2001
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  • 6
    Online Resource
    Online Resource
    Wiley ; 2008
    In:  Rapid Communications in Mass Spectrometry Vol. 22, No. 24 ( 2008-12-30), p. 3997-4008
    In: Rapid Communications in Mass Spectrometry, Wiley, Vol. 22, No. 24 ( 2008-12-30), p. 3997-4008
    Abstract: Gas isotope ratio mass spectrometers usually measure ion current ratios of molecules, not atoms. Often several isotopologues contribute to an ion current at a particular mass‐to‐charge ratio ( m / z ). Therefore, corrections have to be applied to derive the desired isotope ratios. These corrections are usually formulated in terms of isotope ratios ( R ), but this does not reflect the practice of measuring the ion current ratios of the sample relative to those of a reference material. Correspondingly, the relative ion current ratio differences (expressed as δ values) are first converted into isotopologue ratios, then into isotope ratios and finally back into elemental δ values. Here, we present a reformulation of this data reduction procedure entirely in terms of δ values and the ‘absolute’ isotope ratios of the reference material. This also shows that not the absolute isotope ratios of the reference material themselves, but only product and ratio combinations of them, are required for the data reduction. These combinations can be and, for carbon and oxygen have been, measured by conventional isotope ratio mass spectrometers. The frequently implied use of absolute isotope ratios measured by specially calibrated instruments is actually unnecessary. Following related work on CO 2 , we here derive data reduction equations for the species O 2 , CO, N 2 O and SO 2 . We also suggest experiments to measure the required absolute ratio combinations for N 2 O, SO 2 and O 2 . As a prelude, we summarise historic and recent measurements of absolute isotope ratios in international isotope reference materials. Copyright © 2008 John Wiley & Sons, Ltd.
    Type of Medium: Online Resource
    ISSN: 0951-4198 , 1097-0231
    URL: Issue
    Language: English
    Publisher: Wiley
    Publication Date: 2008
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  • 7
    In: Rapid Communications in Mass Spectrometry, Wiley, Vol. 17, No. 16 ( 2003-08-30), p. 1897-1908
    Type of Medium: Online Resource
    ISSN: 0951-4198
    Language: English
    Publisher: Wiley
    Publication Date: 2003
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  • 8
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2004
    In:  Journal of Geophysical Research: Atmospheres Vol. 109, No. D3 ( 2004-02-16), p. n/a-n/a
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 109, No. D3 ( 2004-02-16), p. n/a-n/a
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2004
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  • 9
    Online Resource
    Online Resource
    Royal Society of Chemistry (RSC) ; 2002
    In:  Phys. Chem. Chem. Phys. Vol. 4, No. 18 ( 2002), p. 4420-4430
    In: Phys. Chem. Chem. Phys., Royal Society of Chemistry (RSC), Vol. 4, No. 18 ( 2002), p. 4420-4430
    Type of Medium: Online Resource
    ISSN: 1463-9076 , 1463-9084
    Language: English
    Publisher: Royal Society of Chemistry (RSC)
    Publication Date: 2002
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  • 10
    Online Resource
    Online Resource
    American Chemical Society (ACS) ; 2007
    In:  Analytical Chemistry Vol. 79, No. 2 ( 2007-01-01), p. 599-607
    In: Analytical Chemistry, American Chemical Society (ACS), Vol. 79, No. 2 ( 2007-01-01), p. 599-607
    Type of Medium: Online Resource
    ISSN: 0003-2700 , 1520-6882
    Language: English
    Publisher: American Chemical Society (ACS)
    Publication Date: 2007
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