2019
DOI: 10.1016/j.nimb.2019.02.009
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SIRIUS Performance: 10Be, 26Al and 36Cl measurements at ANSTO

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Cited by 38 publications
(18 citation statements)
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“…Following crushing and sieving, magnetic minerals were separated using a Franz magnetic separator and the non-magnetic fraction washed in Aqua-Regia at 100°C for at least 24 hours. Samples were analysed using the 10MV ANTARES and 6MV SIRIUS facilities at ANSTO (Fink and Smith, 2007;Wilcken et al, 2017Wilcken et al, , 2019. The above sample preparation steps were carried out at the University of Wollongong.…”
Section: Cosmogenic 10 Be and 26 Al Analysismentioning
confidence: 99%
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“…Following crushing and sieving, magnetic minerals were separated using a Franz magnetic separator and the non-magnetic fraction washed in Aqua-Regia at 100°C for at least 24 hours. Samples were analysed using the 10MV ANTARES and 6MV SIRIUS facilities at ANSTO (Fink and Smith, 2007;Wilcken et al, 2017Wilcken et al, , 2019. The above sample preparation steps were carried out at the University of Wollongong.…”
Section: Cosmogenic 10 Be and 26 Al Analysismentioning
confidence: 99%
“…Quartz dissolution and extraction of the Be and Al fractions was done at ANSTO following procedures described in Child et al (2000), using~300 μg of 9 Be from a low-level beryl carrier solution added prior to complete HF dissolution. Samples were analysed using the 10MV ANTARES and 6MV SIRIUS facilities at ANSTO (Fink and Smith, 2007;Wilcken et al, 2017Wilcken et al, , 2019. The native Al concentration of the samples ranged from 112 to 299 ppm (median = 158 ppm) and was determined via ICP-OES with a precision of 3-4% (Fujioka et al, 2015b).…”
Section: Cosmogenic 10 Be and 26 Al Analysismentioning
confidence: 99%
“…Meteoric cosmogenic 10 Be is produced in the atmosphere via nuclear reactions of cosmicray particles with nuclei such as nitrogen and oxygen. 10 Be readily attaches to aerosols and dust and, with a short residence time of ∼ 1 year, is deposited on the Earth surface mainly via precipitation (Willenbring and von Blanckenburg, 2010). In open depositional environments (i.e.…”
Section: Beryllium-10mentioning
confidence: 99%
“…Beryllium was separated from other cations by passage through anion and cation exchange columns, converted to Be(OH) 2 , oxidised to BeO at 800 • C, and finally mixed with Nb powder. AMS 10 Be / 9 Be measurements of these 59 samples were performed at the Centre for Accelerator Science, ANSTO (Australia), on the 6 MV SIRIUS accelerator (Wilcken et al, 2019). The measured 10 Be / 9 Be values were normalised to either the 2007-KN5-2 (nominal ratio of 8.558 × 10 −12 ) or the 2007-KN5-3 (6.320 × 10 −12 ) standard (Nishiizumi et al, 2007).…”
Section: Beryllium-10mentioning
confidence: 99%
“…Given the long half-life of 10 Be and the increasingly low analytical backgrounds that can be realized (Wilcken et al 2019), it is now possible to analyse samples covering a wide range of temporal settings, including historic times (Schaefer et al 2009). The rate at which cosmogenic nuclides are produced is extremely low -a couple of atoms per gram of rock per year (Borchers et al 2016) -and the rapid attenuation of cosmic radiation with depth (Fig.…”
Section: In-situ Cosmogenic Nuclide Analysis For Catchment Erosionmentioning
confidence: 99%