2020
DOI: 10.1016/j.chemgeo.2020.119487
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Isobar-free neon isotope measurements of flux-fused potential reference minerals on a Helix-MC-Plus mass spectrometer

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Cited by 11 publications
(12 citation statements)
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References 28 publications
(45 reference statements)
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“…The calculated cosmogenic 21 Ne abundances from 22 aliquots of CREU-1 (Table 1) all agree within 2σ with their arithmetic mean (348 ±10 x 10 6 atoms/g; ±2σ); thus, we may calculate an error-weighted mean: 348 ± 2 x 10 atoms/g (±2σ), which is indistinguishable from the published value (348± 10 x 10 6 atoms/g; Vermeesch et al, 2015). We conclude that the reproducibility and accuracy of the current set up at the University of Cologne for determining cosmogenic 21 Ne in quartz is similar to or better than those reported for other laboratories worldwide (Vermeesch et al, 2015;Farley et al, 2020;Ma et al, 2015). Vermeesch et al, 2015).…”
Section: Performancecontrasting
confidence: 48%
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“…The calculated cosmogenic 21 Ne abundances from 22 aliquots of CREU-1 (Table 1) all agree within 2σ with their arithmetic mean (348 ±10 x 10 6 atoms/g; ±2σ); thus, we may calculate an error-weighted mean: 348 ± 2 x 10 atoms/g (±2σ), which is indistinguishable from the published value (348± 10 x 10 6 atoms/g; Vermeesch et al, 2015). We conclude that the reproducibility and accuracy of the current set up at the University of Cologne for determining cosmogenic 21 Ne in quartz is similar to or better than those reported for other laboratories worldwide (Vermeesch et al, 2015;Farley et al, 2020;Ma et al, 2015). Vermeesch et al, 2015).…”
Section: Performancecontrasting
confidence: 48%
“…Honda et al, 2015;Wielandt and Storey, 2019) and its ability to reliably measure 21 Ne at an off-centre peak position that is free of interference from 20 NeH + (Honda et al, 2015;Wielandt and Storey, 2019). The remaining interference of 12 C 16 O2 2+ at m/e=22 can be corrected via monitoring of the double/single-charged ratio of CO2 in-between samples (Honda et al, 2015) or the measurement of 13 C 16 O2 2+ at m/e= 22.5 during sample analysis (Wielandt and Storey, 2019 (Farley et al, 2020).…”
Section: Introductionmentioning
confidence: 99%
“…PC2: (L1: 22 Ne-CDD: 21 High precision Ne isotope analysis is complicated by isobaric interferences at all peaks. Although new instruments can either fully or partially resolve some of the common interferences [8,9], in many cases, a correction is required [6,7,10,14,15]. This requires the measurement of several other peaks, which has an implication on measurement time and data precision.…”
Section: Figurementioning
confidence: 99%
“…Cosmogenic Ne was proven to be an adept recorder of the timing and rates of surface processes on the Earth and Moon [1][2][3] and the time of meteorite release from parent bodies [4]. Precise determination of neon isotopes in rocks and minerals are conventionally made using static gas magnetic sector mass spectrometers [5][6][7][8]. The low production rate at the Earth's surface and the presence of isobaric interferences at all Ne isotopes means that precise determination of terrestrial cosmogenic Ne is routinely measured in only a handful of laboratories worldwide [5].…”
Section: Introductionmentioning
confidence: 99%
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