2018
DOI: 10.1016/j.chemgeo.2018.04.008
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Rapid measurement of strontium in speleothems using core-scanning micro X-ray fluorescence

Abstract: Speleothem trace element ratios such as Mg/Ca and Sr/Ca are increasingly used in speleothem paleoclimatology as a supplement to stable oxygen and carbon isotope ratios as proxies for past variability in the hydrologic system. Using multiple proxies together allows for a better understanding of both the local and distal hydrologic changes recorded in speleothem chemistry, and therefore of changes in past rainfall. Despite the potential benefits, trace element analysis of speleothems has yet to become widespread… Show more

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Cited by 18 publications
(10 citation statements)
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“…Sr/Ca ratios can be rapidly obtained by non-destructive XRF scanning (Scroxton et al, 2018). For this study, Sr/Ca ratios were measured on an ITRAX XRF core scanner from Cox Analytical Systems (Gothenburg, Sweden) using a 3 kW molybdenum (Mo) X-ray tube.…”
Section: Trace Elementsmentioning
confidence: 99%
“…Sr/Ca ratios can be rapidly obtained by non-destructive XRF scanning (Scroxton et al, 2018). For this study, Sr/Ca ratios were measured on an ITRAX XRF core scanner from Cox Analytical Systems (Gothenburg, Sweden) using a 3 kW molybdenum (Mo) X-ray tube.…”
Section: Trace Elementsmentioning
confidence: 99%
“…flowstones and stalagmites) (Hill et al, 1997). Inorganic geochemical properties (isotopic and trace element data) (Affolter et al, 2019;Nagra et al, 2017;Scroxton et al, 2018;Williams et al, 1999) and physical properties (e.g. nano-crystal aggregation, open vs. compact columnar fabrics, defect-ridden fabrics) of natural calcium carbonate minerals have been routinely used to determine environmental parameters atof their time of formation (Frisia et al, 2000;Nielsen et al, 2014).…”
Section: Introductionmentioning
confidence: 99%
“…Although the stalagmites are mainly made of calcium carbonate, seven elements can be detected by CXRF method for stalagmite C9, including Si, K, Fe, Cu, Ni, Sc and Sr. This is because, except for K (~3.31 keV), the characteristic peaks of Si (~1.74 keV), Sc (~4.09 keV), Fe (~6.4 keV), Cu (~8.04 keV), Ni (~7.47 keV) and Sr (~14.2 keV) are far away from the interference of Ca (~3.7 keV) and diffraction peaks (Richter et al, 2006;Scroxton et al, 2018). The spectral peaks produced by Ca and the pseudo-peaks produced by the diffraction of carbonate crystalline matrix do not interfere with identifying characteristic peaks of these elements.…”
Section: Accepted Articlementioning
confidence: 99%