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. Author manuscript; available in PMC: 2020 Jan 24.
Published in final edited form as: Geostand Geoanal Res. 2016 Feb 5;40(3):433–445. doi: 10.1111/j.1751-908x.2016.00376.x

Forty-Nine Major and Trace Element Concentrations Measured in Soil Reference Materials NIST SRM 2586, 2587, 2709a, 2710a and 2711a Using ICP-MS and Wavelength Dispersive-XRF

Harris L Byers 1,*, Lindsay J McHenry 1, Timothy J Grundl 1
PMCID: PMC6980794  NIHMSID: NIHMS757100  PMID: 31983910

Abstract

Excellent agreement was noted in the concentration of major and trace elements in five NIST soil reference materials (NIST SRM 2586, 2587, 2709a, 2710a and 2711a) between measurement results from wavelength dispersive-XRF and ICP-MS from two independent laboratories, and NIST certificate of analysis and literature data. We describe the variability in concentrations of up to forty-nine elements (plus loss on ignition) and provide values for up to twenty-one elements previously uncharacterised by NIST in these soil RMs. The additional characterisation provided in this investigation can be utilised to reduce the measurement bias of custom calibration routines and improve the quality of control checks developed using these NIST RMs.

Keywords: National Institute for Science and Technology, inductively coupled plasma-mass spectrometry, wavelength dispersive X-ray fluorescence, WD-XRF, calibration materials, soil, urban agriculture


Numerous geoscience/urban geochemistry investigations have utilised commercially available NIST SRM soil certified reference materials for calibration or quality control purposes (e.g., Kenna et al. 2011, Murry et al. 2011, Sutton et al. 2012, Weindorf et al. 2012, Fernández et al. 2014, McComb et al. 2014). NIST defines and provides certified, reference and information values for element concentrations presented in certificates of analysis. NIST certified values represent concentrations measured with the smallest measurement uncertainty and where sources of bias have been accounted for (May et al. 2000). Concentrations provided by NIST with larger measurement uncertainty are defined as reference values, whereas reported concentrations where uncertainty has not been evaluated are referred to as information values (May et al. 2000). Reference values or information values for the soil materials NIST SRM 2709, 2710 and 2711, either reported directly or as part of quality control exercises, have been provided previously by numerous investigators using XRF and/or ICP-MS (e.g., Wilson et al. 1994, Cloquet et al. 2005, Makinen et al. 2005, Murry et al. 2011, Weindorf et al. 2012, Gueguen et al. 2013). However, these three soil RMs are no longer commercially available and have been replaced by NIST SRM 2709a, 2710a and 2711a. Along with NIST SRM 2586 and 2587, these five reference materials present a continuum of heavy metal concentrations and are considered representative of soils likely to be encountered in urban agriculture/urban geochemistry studies. However, characterisation of these five soil RMs remains incomplete because very few reference values are available in the literature (Moon et al. 2009, Paul et al. 2009, Hoang et al. 2010, Goix et al. 2011, Milliard et al. 2011, Alvarez-Toral et al. 2013, Claverie et al. 2013, Eriksson et al. 2013, Fernández et al. 2014). The purpose of this study is to further characterise the variability in element concentrations (strictly, the mass-fractions) in the five NIST SRM soil materials and provide reference values for previously uncharacterised elements. This will contribute to reducing the measurement bias of custom calibration routines and improving the quality of control checks developed using these NIST reference materials.

Materials

The commutability of reference materials to anticipated samples is critical in decreasing measurement uncertainty. This study was focussed on soils with heavy metal (primarily Pb) concentrations similar in magnitude to previous urban geochemistry and urban agriculture studies (Finster et al. 2004, Clark et al. 2006, 2008, Huang et al. 2012, Defoe et al. 2014, Hu et al. 2014, McBride et al. 2014, Sharma et al. 2015). Therefore, five commercially available NIST soil reference materials encompassing a continuum in heavy metal concentrations, organic carbon and mineralogy likely to be found in urban soils were selected for characterisation. These originated from (1) a fallow agricultural field in the San Joaquin Valley of California (NIST SRM 2709a); (2) the floodway of Silver Bow Creek in Montana near a Brownfield property (NIST SRM 2710a); (3) an agricultural field located near a former smelting plant in Helena, MT (NIST SRM 2011a); (4) an urban agricultural garden contaminated with lead-based paint (NIST SRM 2587); and (5) urban soils contaminated with lead based paint (NIST SRM 2586).

Experimental procedure

Upon receipt of the NIST materials, each jar was shaken gently by hand for 30 s and aliquots of ca. 5 g were transferred from each jar to separate glass vials, which were then sealed with polyethylene caps. An aliquot of each NIST SRM soil sample was anonymised and submitted under chain of custody to the Wisconsin State Laboratory of Hygiene, Madison, Wisconsin (WSLH; a Wisconsin Department of Natural Resources certified laboratory) for ICP-MS analysis. Concurrently, two aliquots were used to prepare pressed pellets and fused beads for analysis by WD-XRF at the University of Wisconsin-Milwaukee Department of Geosciences XRF laboratory using two separate custom WD-XRF calibration routines. A fourth aliquot was used to determine the mass lost on ignition (LOI).

ICP-MS

NIST SRM soil samples were digested at the WSLH using a standard microwave digestion programme that involved adding 8.0 ml of 16 mol l−1 HNO3 plus 2.0 ml of 12 mol l−1 HCl plus 2.5 ml of HF to 30-mg test portions of each RM. Digestions were measured in triplicate using a Thermo-Finnigan Element 2 magnetic-sector ICP-MS.

WD-XRF (fused bead preparation)

Fused beads of each NIST soil RM were prepared using the protocol described in McHenry (2009) in which 1.000 g of soil was added to 1 g of oxidiser (ammonium nitrate) and 10.000 g of Claisse (Québec, Canada) 50:50 lithium metaborate: lithium tetraborate flux containing 0.5% LiBr as a non-wetting agent. The material was fused at 1050 °C in a Claisse M4 programmable fusion system. Fused beads were measured three times with a Bruker AXS, Inc. Pioneer S4 WDXRF instrument using a custom measurement and calibration procedure based on eleven USGS sedimentary and igneous geological reference materials made in the same manner as samples prepared for this study, as described by McHenry (2009). The USGS geological reference materials used in this calibration routine are AGV-1, BCR-2, BHVO-2, BIR-1, DNC-1, DTS-2b, G-2, GSP-2, RGM-1, SGR-1 and STM-1. The custom routine was refined in the Pioneer S4 software by correcting for peak overlaps, and adjusted for the use of the bromide non-wetting agent. Absorption and enhancement due to matrix effects were corrected in the Pioneer S4 software using fundamental parameters, and calibration materials with concentrations less than the limit of detection were removed from the calibration routine.

The intensities of eighteen major and trace elements in the reference materials were measured under vacuum using Kα1 lines except for Ba and Ce, which were measured using their Lα1 X-ray lines and concentrations determined through the custom fused bead calibration. To measure Na, K, Ca and Fe, the routine was optimised to count fluoresced X-rays for 10 s or until the statistical precision on counting values (determined as 3s based on a Poisson's law) was less than 0.3%. For Al and Si, fluoresced X-rays were counted for fixed times of 10 s and 4 s, respectively. To measure the concentrations of Mg and P, the routine counted fluoresced X-rays for 30 s or until the statistical precision (3s) was less than 0.3% and 1%, respectively. The remaining elements were measured for 10 s or until the statistical precision (3s) was less than 5%. Depending on the element, the routine used a pentaerythrite (PET), lithium fluoride (LIF200) or multi-layer (OVO-55) analyser crystal, and either a flow or scintillation counter. Specific routine details for each element, including generator voltage, tube current, collimator, analyser crystal, detector and peak overlap corrections are provided in online supporting material Table S1.

WD-XRF (pressed pellet preparation)

Pressed pellets of each NIST SRM soil were prepared by adding 10.0 g of material with four GeoQuant (Krupp Polysius Polab ®) wax binder pills (1.25 g total) and combining in a tungsten carbide shatterbox for 30 s. Each prepared sample was placed in an Al sample cup and pressed at 25 t for 60 s in a 40 mm diameter pellet die hydraulic press as described in McHenry et al. (2011). Pressed pellets were measured three times using a Bruker AXS, Inc. Pioneer S4 WD-XRF for major and trace elements utilising a custom measurement and calibration routine developed utilising nine USGS sedimentary and igneous rock reference materials (AGV-2, BCR-2, BHVO-2, DNC-1, DTS-2b, GSP-2, QLO-1, SGR-1 and W-2A) made in the same manner as samples prepared for this study as described in McHenry et al. (2011). The custom calibration routine was refined in the Pioneer S4 software by correcting for peak overlaps, Rh Rayleigh and Compton peaks, and contamination of W and Co from the shatterbox. Data points with concentrations less than the limit of detection were removed from the calibration routine.

The intensities of twenty-two elements in the NIST SRM materials were measured under vacuum using Kα1 lines, except for Ba and Ce, which were measured using Lα1 X-ray wavelengths and concentrations determined through the custom pressed pellet calibration. The routine was optimised to count fluoresced X-rays for 10 s or until the statistical precision (3s) was less than 5%. Depending on the element, the routine used a PET, LIF200 or OVO-55 crystal and either a flow or scintillation counter. Specific routine details for each element, including generator voltage, tube current, collimator, crystal, detector and peak overlap corrections are provided in Table S2 (online supporting information).

Water content and loss on ignition

Test portions, weighing 4 g, of each NIST SRM soil material were dried for 2 hours in an oven at 105 °C to estimate the adsorbed water content of each soil. Each oven-dried NIST SRM soil sample was divided into three 1-g aliquots and, following McHenry (2009), each aliquot was combusted in a muffle furnace at 1050 °C for 15 min and the mean LOI calculated for each RM to estimate the mass of material lost during fused bead preparation.

Quality control of WD-XRF measurements

As noted by Thomsen et al. (2003), the limit of detection (LOD) is considered the smallest concentration of an element that produces a response that can be distinguished from the background. The limit of quantitation (LOQ) is considered the smallest concentration that can be measured with minimal bias and error. The LOD for each WD-XRF measurement was calculated by the Pioneer S4 software and the LOQ of each WD-XRF measurement was estimated by multiplying the LOD by 3.3 as suggested by Thomsen et al. (2003). WD-XRF measurements less than the LOD are omitted from Tables 610. WD-XRF measurements greater than the LOD but less than the LOQ are denoted on Tables 610 with a “J” data qualifier and are considered information values; likewise the 1s and RSD for these measurements are provided for information purposes only and measurements less than the LOQ are omitted from further evaluation in this data assessment study. In addition, the statistical precision on the intensity measurement for each WD-XRF measurement was calculated by the Pioneer S4 software based on Poisson's law, and if the statistical precision was greater than 12%, WD-XRF measurement results were omitted from Tables 110.

Table 6.

Element concentrations in NIST SRM 2586 determined using three measurement methods

WD-XRF (FB) WD-XRF (PP) ICP-MS NIST

(μg g−1) 1s RSD (μg g−1) 1s RSD (μg g−1) 1s RSD (μg g−1) ±

Li 24.61 1.87 8 25
B 50.93 0.00 0
P 960.1 0.0 0 1352.9 0.0 0 870.53 67.15 8 1001 77
Sc 26.49 0.74 3 24
Ti 6273.1 34.6 1 6872.5 115.5 2 6492.62 335.33 5 6050 660
V 169.6 1.1 1 205.3 18.8 9 154.76 3.80 2 160
Cr 356.0 9.8 3 301.73 11.79 4 301 45
Mn 1000.0 0.0 0 1033.3 57.7 6 971.20 6.33 1 1000 18
Co 28 J 3.0 11 33.63 0.71 2 35
Ni 75.4 4.0 5 80.7 1.2 1 84.39 2.27 3 75
Cu 92.0 7.8 8 82.77 2.98 4 81
Zn 346.3 5.8 2 363.7 5.9 2 302.51 46.16 15 352 16
Ga 20.7 0.6 3 14
As 8.60 0.61 7 8.7 1.5
Rb 61.0 1.7 3 49.01 3.76 8
Sr 98.5 2.9 3 92.0 1.7 2 84.1 8
Y 27.0 1.0 4 23.46 1.11 5 21
Zr 277.9 4.6 2 287.7 1.5 1
Nb 12.74 0.33 3 6
Mo 1.11 0.25 23
Ag 0.55 0.09 17
Cd 2.48 0.23 9 2.71 0.54
Sn 13.29 0.05 0
Sb 3.07 0.11 3
Cs 1.93 0.16 9
Ba 374.4 34.8 9 491.3 16.5 3 411.72 15.61 4 413 18
La 23.52 0.40 2 29.7 4.8
Ce 66.3 29.2 44 51.17 2.08 4 58 8
Pr 6.17 0.18 3 7.3
Nd 24.00 0.84 4 26.4 2.9
Sm 5.01 0.27 5 6.1
Eu 1.23 0.03 3 1.5
Dy 4.36 0.21 5 5.4
Ho 0.88 0.02 3 1.1
Yb 2.44 0.09 4 2.64 0.51
Lu 0.35 0.01 3
Ta 0.85 0.00 0
W 1.24 0.28 22
Tl 0.35 0.01 2
Pb 419.48 14.41 3 432 17
Th 5.80 0.05 1 7
U 1.90 0.02 1

Element concentrations qualified with a “J” are greater than the limit of detection, but less than the limit of quantitation. Shaded rows represent elements not characterised by NIST.

Table 10.

Element concentrations in NIST SRM 2711a determined using three measurement methods

WD-XRF (FB) WD-XRF (PP) ICP-MS NIST

(μg g−1) 1s RSD (μg g−1) 1s RSD (μg g−1) 1s RSD (μg g−1) ±

Li 29.05 1.47 5
B 55.22 9.41 17 50
P 872.8 0.0 0 1352.9 0.0 0 796.05 112.82 14 842 11
Sc 10.60 1.47 14 8.5 0.1
Ti 3196.5 34.6 1 3476.2 0.0 0 3287.54 195.65 6 3170 80
V 85.0 3.5 4 109.0 1.7 2 66.85 15.67 23 80.7 5.7
Cr 84.0 5.6 7 48.24 1.68 3 52.3 2.9
Mn 666.7 57.7 9 719.0 10.8 2 670.44 39.41 6 675 18
Co 10.27 1.38 13 9.89 0.18
Ni 18 J 5.7 31 27 J 1.5 6 19.50 1.60 8 21.7 0.7
Cu 151.7 4.0 3 144.31 20.14 14 140 2
Zn 401.7 5.8 1 418.3 7.6 2 372.74 96.70 26 414 11
Ga 24.7 0.6 2
As 90.96 8.63 9 107 5
Rb 136.0 3.0 2 121.29 12.95 11 120 3
Sr 232.4 2.0 1 256.0 1.7 1 242 10
Y 29.9 0.9 3 33.0 0.0 0
Zr 318.1 2.5 1 310.3 0.6 0
Nb 20.07 1.79 9
Mo 1.74 0.15 8
Ag 6.17 0.94 15 6
Cd 50.64 10.39 21 54.1 0.5
Sn 4.72 0.27 6
Sb 23.04 3.52 15 23.8 1.4
Cs 6.67 0.68 10 6.7 0.2
Ba 697.7 24.6 4 850.0 21.5 3 760.16 77.74 10 730 15
La 30.53 3.17 10 38 1
Ce 146.33 5.13 4 63.33 5.79 9 70
Pr 7.30 0.65 9
Nd 27.99 2.39 9 29 2
Sm 5.51 0.31 6 5.93 0.28
Eu 1.17 0.16 14 1.1 0.2
Dy 4.74 0.39 8 5
Ho 0.96 0.06 7
Yb 2.95 0.27 9 3
Lu 0.43 0.03 7 0.5
Ta 1.48 0.19 13 1
W 3.07 0.04 1
Tl 2.85 0.45 16 3
Pb 1402.88 225.33 16 1400 10
Th 10.72 1.35 13 15 1
U 2.77 0.35 13 3.01 0.12

Element concentrations qualified with a “J” are greater than the limit of detection, but less than the limit of quantitation. Shaded rows represent elements not characterised by NIST.

Table 1.

Element concentrations in NIST SRM 2586 determined using three measurement methods

WD-XRF (FB) WD-XRF (PP) ICP-MS NIST

g/100 g 1s (μg g−1) RSD g/100 g 1s (μg g−1) RSD g/100 g 1s (μg g−1) RSD g/100 g ±

Na 0.50 113 2 0.52 63 1 0.468 730
Mg 1.69 0 0 2.48 265 1 1.67 51 0.3 1.707 840
Al 6.70 106 0.2 7.00 2570 2 6.83 2673 4 6.652 760
Si 28.94 546 0.2 28.72 6050 1 29.150 2100
K 0.99 48 0.4 1.01 115 1 1.03 1323 13 0.976 180
Ca 2.16 0 0 2.79 58 0.1 2.38 2695 11 2.218 540
Fe 5.16 162 0.3 5.96 58 0.1 5.20 918 2 5.161 890

Due to contamination during sample preparation in the shatterbox, W and Co values cannot be reported for pressed pellet WD-XRF measurements. The flux used to make the fused beads contained 1% LiBr as a non-wetting agent, and due to a large peak overlap between Br and Rb, we are not able to report concentrations of Rb in fused bead WD-XRF pellets.

During the manufacturing process, NIST sieved each soil material through a 200-mesh screen; therefore the maximum particle size should be no more than 75 μm. As WD-XRF X-ray penetration depths for the Mg, Al, Si, P, K, Ca and Ti Kα1 lines are less than 75 μm, it is possible that the concentrations of these elements measured in this study using WD-XRF of pressed pellets are biased to elements concentrated in particles on the surface of the pellet and thus may not be representative of the bulk. Values for these measurands are reported in Tables 110 for information purposes only. The penetration depth for Na is only 4.1 μm; therefore these results for WD-XRF measurements of pressed pellets are not reported.

Data reduction

Based on the triplicate measurements of each analyte by ICP-MS and WD-XRF, the mean concentration of each element, associated standard deviation (s), and the relative standard deviation (RSD; expressed as per cent) were calculated for each NIST SRM soil for each measurement technique. Major element concentrations are presented in Tables 15 and trace element concentrations are presented in Tables 610 along with corresponding NIST certified, information, and reference values and associated uncertainties reported by NIST.

Table 5.

Element concentrations in NIST SRM 2711a determined using three measurement methods

WD-XRF (FB) WD-XRF (PP) ICP-MS NIST

g/100 g 1s (μg g−1) RSD g/100 g 1s (μg g−1) RSD g/100 g 1s (μg g−1) RSD g/100 g ±

Na 1.24 113 1 1.30 1169 9 1.20 100
Mg 1.02 0 0 1.66 173 1 1.00 340 3 1.07 600
Al 6.73 397 1 6.75 2512 2 6.98 4559 7 6.72 600
Si 30.55 742 0.2 28.78 7410 1 31.40 7000
K 2.53 0 0 2.58 115 0.4 2.15 7479 35 2.53 1000
Ca 2.37 0 0 2.76 58 0.1 2.59 2725 11 2.42 600
Fe 2.89 40 0.1 3.20 321 1 2.72 578 2 2.82 400

To compare concentrations measured in this study to concentrations reported by NIST and to other values reported in the literature, the relative difference (RD; expressed as a per cent) was calculated following USEPA (2007, 2014) as:

RD={(C1C2)[(C1+C2)2]}×100 (1)

where C1 and C2 are element concentrations in sample 1 and sample 2, respectively. Relative difference is a dimensionless statistical measurement commonly used to evaluate the precision of two measurements of inorganic elements (USEPA 2007, 2014). A RD of 0 indicates that the two measurements are equal, while a larger or smaller RD indicates an increasing difference between the two measurements. A positive RD indicates that C1 > C2; conversely, a negative RD indicates C1 < C2.

For the purpose of this investigation, we assumed that the NIST values are the correct values; therefore, we used RD as a measurement of bias. As recommended in USEPA (2014), we define a RD of ± 20% as the control limit. We acknowledge that many trace elements are difficult to measure; therefore, for our evaluation, we define a RD of ± 40% as the threshold limit. Element concentrations with RD values outside the threshold limit are provided for information purposes only.

The RD for each element for each NIST SRM soil comparing the NIST concentrations (C1) with the WSLH ICP-MS concentrations (C2) is illustrated in Figure 1. The RD for each element for each RM comparing the NIST concentrations (C1) with the fused bead WD-XRF concentrations (C2) is illustrated in Figure 2. The RDs comparing concentrations measured in this study by WSLH using ICP-MS (C2) to concentrations reported in the literature (C1) by Moon et al. (2009) and Paul et al. (2009), Hoang et al. (2010), Goix et al. (2011), Milliard et al. (2011), Alvarez-Toral et al. (2013), Claverie et al. (2013), Eriksson et al. (2013), Fernandez et al. (2014) are shown in Figure 3.

Figure 1.

Figure 1

Relative difference between NIST data and ICP-MS measurements (from WSLH). Positive values indicate NIST values > WSLH measurements. Relative differences outside the presented intervals are provided as text on the figure.

Figure 2.

Figure 2

Relative difference between NIST data and fused bead WD-XRF measurements. Positive values indicate NIST values > fused bead WD-XRF measurements.

Figure 3.

Figure 3

Relative difference between ICP-MS (WSLH) and literature values. Positive values indicate WSLH measurements > literature values.

Results and discussion

Comparison of our measurements to NIST and literature values

Excellent agreement was noted in the major and trace elements between measurements made in this investigation and the NIST certified, reference and information values (Figures 1 and 2). Measurement results from ICP-MS (at WSLH) seem to be uniformly lower compared with NIST values for NIST SRM 2710a, but no other bias is apparent in the WSLH measurements. As illustrated in Figure 1, 85% of WSLH measurements were within the control limit of ± 20% RD compared with NIST values and 99% of measurements were within the threshold limit of ± 40% RD compared with NIST values. In comparing the WD-XRF measurements of fused beads from our laboratory to NIST values, 97% of WD-XRF measurements were within the control limit of ± 20% RD and 100% of measurements were within the threshold limit of ± 40% RD. Elements with RD values outside the threshold limit are present in trace concentrations and are challenging to measure with reasonable precision. Therefore, we have great confidence in the values for the major and minor elements reported in this study.

Element concentrations measured in this study by ICP-MS by WSLH are in close agreement with concentrations reported in the literature (Figure 3). In comparing the WSLH ICP-MS measurements with literature values, 88% of WSLH measurements were within the control limit of ± 20% RD and 99% of measurements were within the threshold limit (± 40% RD). Therefore, we have great confidence in the values for the major and minor elements reported in this study.

For reference, the water contents in NIST SRM 2586, 2587, 2709a, 2710a and 2711a measured in this study were 1.6%, 1.1%, 2.7%, 1.8% and 2.1% m/m, respectively, and the mean LOI concentrations were 8.6%, 6.4%, 6.6%, 7.5% and 6.4% m/m, respectively. The respective standard deviations of the LOI measurements of NIST SRMs 2586, 2587, 2709a, 2710a and 2711a were 0.2%, 0.1%, 0.2%, 0.02% and 0.03% m/m.

Our future goal is to advance the use of portable ED-XRF in measuring concentrations of heavy metals in urban soil in situ. As demonstrated in recent work completed by Perroy et al. (2014) and Weindorf et al. (2012), portable ED-XRF is a promising tool for use in urban agriculture/geochemistry investigations. With the increased information provided in this investigation, the bias in custom calibration routines for portable ED-XRF spectrometers developed with the characterised NIST SRMs will be reduced.

Conclusions

Eighty-five per cent of ICP-MS measurements (made at the Wisconsin State Laboratory of Hygiene, Madison, Wisconsin) and 97% of WD-XRF measurements (made at the Department of Geosciences, University of Wisconsin-Milwaukee) generated in this data assessment exercise when compared with NIST certified, reference and information values fell within a control limit of ± 20% relative difference. This provides confidence in the values for the major and minor elements reported in this study. We have described the variability in concentrations of up to forty-nine elements (plus LOI) and have provided values for up to twenty-one elements previously uncharacterised by NIST in soil reference materials NIST SRM 2709a, 2710a, 2711a, 2586 and 2587. The additional characterisation provided in this investigation will contribute to reducing measurement uncertainty in custom calibration routines and improving the quality of control checks developed utilising these NIST SRMs.

Supplementary Material

Supp Table S1
Supp Table S2

Table 2.

Element concentrations in NIST SRM 2587 determined using three measurement methods

WD-XRF (FB) WD-XRF (PP) ICP-MS NIST

g/100 g 1s (μg g−1) RSD g/100 g 1s (μg g−1) RSD g/100 g 1s (μg g−1) RSD g/100 g ±

Na 1.16 0 0 1.20 69 1 1.13 330
Mg 0.69 0 0 1.33 100 0.4 0.67 374 6 0.67 250
Al 6.07 140 0.2 6.33 208 0.2 6.07 3184 5 5.86 1700
Si 33.06 221 0.1 32.86 1966 0.3 33.13 2600
K 1.62 0 0 1.68 58 0.3 1.60 1801 11 1.58 550
Ca 0.91 41 0.4 1.32 0 0 0.89 728 8 0.93 200
Fe 2.84 107 0.4 3.11 100 0.2 2.79 1096 4 2.81 250

Table 3.

Element concentrations in NIST SRM 2709a determined using three measurement methods

WD-XRF (FB) WD-XRF (PP) ICP-MS NIST

g/100 g 1s (μg g−1) RSD g/100 g 1s (μg g−1) RSD g/100 g 1s (μg g−1) RSD g/100 g ±

Na 1.26 74 1 1.29 1150 9 1.22 300
Mg 1.45 60 0.4 2.52 208 0.4 1.41 1008 7 1.46 200
Al 7.44 360 0.4 7.76 3177 2 7.45 6528 9 7.37 1600
Si 29.93 1374 0.4 27.87 6372 1 30.30 4000
K 2.11 48 0.2 2.00 100 0.4 2.08 1611 8 2.11 600
Ca 1.89 0 0 2.52 153 0.4 1.94 1233 6 1.91 900
Fe 3.38 214 1 4.09 586 1 3.34 1026 3 3.36 700

Table 4.

Element concentrations in NIST SRM 2710a determined using three measurement methods

WD-XRF (FB) WD-XRF (PP) ICP-MS NIST

g/100 g 1s (μg g−1) RSD g/100 g 1s (μg g−1) RSD g/100 g 1s (μg g−1) RSD g/100 g ±

Na 0.99 43 0.4 0.85 872 10 0.89 190
Mg 0.75 35 0.4 0.87 0 0 0.62 500 8 0.73 380
Al 6.00 372 1 6.31 2747 2 5.43 4330 8 5.95 500
Si 30.31 1362 0.4 28.84 6523 1 31.10 4000
K 2.15 0 0 2.20 58 0.2 1.95 883 5 2.17 1300
Ca 0.93 41 0.4 1.48 58 0.3 0.84 734 9 0.96 450
Fe 4.29 331 1 4.72 473 1 3.83 3102 8 4.32 800

Table 7.

Element concentrations in NIST SRM 2587 determined using three measurement methods

WD-XRF (FB) WD-XRF (PP) ICP-MS NIST

(μg g−1) 1s RSD (μg g−1) 1s RSD (μg g−1) 1s RSD (μg g−1) ±

Li 34.19 2.83 8 32
B 66.84 3.32 5
P 931.0 25.2 3 1352.9 0.0 0 851.06 70.98 8 970 100
Sc 11.76 1.07 9 11
Ti 4235.4 34.6 1 4495.1 0.0 0 4153.97 185.30 4 3920 650
V 96.1 6.9 7 109.0 1.7 2 80.64 2.70 3 78
Cr 99.7 4.2 4 92.67 5.02 5 92 11
Mn 666.7 57.7 9 669.7 6.7 1 655.46 28.47 4 651 23
Co 11.78 0.32 3 14
Ni 43 J 2.4 6 37.0 2.6 7 32.28 1.95 6 36
Cu 170.7 2.5 1 160.68 3.52 2 160
Zn 324.7 6.4 2 341.0 1.7 1 309.74 34.87 11 335.8 7.6
Ga 24.0 1.0 4 13
As 13.71 1.38 10 13.7 2.3
Rb 82.7 2.5 3 72.30 4.97 7
Sr 125.6 4.5 4 131.7 2.9 2 126 19
Y 28.0 0.0 0 18.51 1.16 6 15
Zr 296.0 4.4 1 269.0 0.0 0
Nb 11.17 0.32 3 14
Mo 1.64 0.20 12
Cd 1.91 0.14 7 1.92 0.23
Sn 17.10 5.73 33
Sb 2.10 0.34 16
Cs 3.10 0.30 10
Ba 544.3 12.7 2 650.3 1.2 0 566.81 25.03 4 568 12
La 20.77 1.42 7 29
Ce 82.7 4.0 5 44.89 2.81 6 57
Pr 5.09 0.27 5
Nd 19.77 1.18 6 25
Sm 3.95 0.19 5
Eu 1.03 0.06 6
Dy 3.38 0.26 8
Ho 0.68 0.04 6
Yb 2.01 0.10 5 1.6
Lu 0.29 0.02 7
Tl 0.48 0.03 7
Pb 3165.52 195.50 6 3242 57
Th 5.69 0.29 5 7.5
U 2.08 0.17 8

Element concentrations qualified with a “J” are greater than the limit of detection, but less than the limit of quantitation. Shaded rows represent elements not characterised by NIST.

Table 8.

Element concentrations in NIST SRM 2709a determined using three measurement methods

WD-XRF (FB) WD-XRF (PP) ICP-MS NIST

(μg g−1) (1 s) RSD (μg g−1) (1 s) RSD (μg g−1) (1 s) RSD (μg g−1) ±

Li 51.88 0.74 1
B 73.42 2.14 3 74
P 712.8 25.2 4 1352.9 0.0 0 694.49 45.98 7 688 13
Sc 12.18 0.85 7 11.1 0.1
Ti 3336.3 34.6 1 3895.7 0.0 0 3344.09 102.09 3 3360 70
V 124.7 12.3 10 154.3 4.5 3 105.96 4.05 4 110 11
Cr 114.7 9.9 9 151.0 1.7 1 119.58 3.21 3 130 9
Mn 500 J 0.0 0 593.3 7.6 1 522.47 4.74 1 529 18
Co 12.79 0.28 2 12.8 0.2
Ni 87.4 7.9 9 87.3 2.1 2 82.71 6.55 8 85 2
Cu 54.7 2.5 5 34.34 2.42 7 33.9 0.5
Zn 107.2 4.2 4 108.0 1.7 2 86.74 7.83 9 103 4
Ga 22.7 0.6 3
As 11.92 3.04 25 10.5 0.3
Rb 111.3 0.6 1 96.16 2.31 2 99 3
Sr 240.5 2.3 1 270.3 2.5 1 239 6
Y 27.3 0.6 2 15.34 0.62 4
Zr 153.2 4.0 3 170.3 1.2 1 195 46
Nb 8.61 0.09 1
Mo 1.30 0.36 27
Ag 0.31 0.08 25
Cd 0.36 0.03 8 0.371 0.002
Sn 1.87 0.78 42
Sb 1.29 0.49 38 1.55 0.06
Cs 5.14 0.21 4 5 0.1
Ba 936.6 5.4 1 1100.0 0.0 0 972.86 16.19 2 979 28
La 19.89 1.10 6 21.7 0.4
Ce 194.0 4.4 2 40.89 1.75 4 42 1
Pr 4.68 0.13 3
Nd 17.88 0.35 2 17
Sm 3.50 0.13 4 4
Eu 1.02 0.06 6 0.83 0.02
Dy 2.77 0.10 4 3
Ho 0.57 0.01 2
Yb 1.67 0.04 2 2
Lu 0.24 0.01 5 0.3
Tl 0.52 0.05 10 0.58 0.01
Pb 17.26 0.77 4 17.3 0.1
Th 9.28 0.28 3 10.9 0.2
U 3.17 0.14 4 3.15 0.05

Element concentrations qualified with a “J” are greater than the limit of detection, but less than the limit of quantitation. Shaded rows represent elements not characterised by NIST.

Table 9.

Element concentrations in NIST SRM 2710a determined using three measurement methods

WD-XRF (FB) WD-XRF (PP) ICP-MS NIST

(μg g−1) 1s RSD (μg g−1) 1s RSD (μg g−1) 1s RSD (μg g−1) ±

Li 24.57 0.58 2
B 16.16 0.26 2 20
P 1047.4 0.0 0 1352.9 0.0 0 841.29 135.73 16 1050 40
Sc 10.03 0.80 8 9.9 0.1
Ti 3056.6 59.9 2 3416.3 0.0 0 2819.15 158.77 6 3110 70
V 97.4 14.8 15 112.3 2.5 2 72.69 3.84 5 82 9
Cr 19.98 1.00 5 23 6
Mn 2066.7 57.7 3 2200.0 0.0 0 1895.26 150.89 8 2140 60
Co 5.04 0.33 6 5.99 0.14
Ni 9 J 1.5 18 6.66 1.57 24 8 1
Cu 3100.0 0.0 0 3062.89 412.13 13 3420 50
Zn 3923.2 33.3 1 4100.0 0.0 0 3567.00 631.33 18 4180 150
Ga 38.7 1.5 4
As 1157.05 29.31 3 1540 100
Rb 122.0 1.0 1 102.22 9.55 9 117 3
Sr 240.4 2.1 1 257.3 1.5 1 255 7
Y 27.6 1.2 4 29.0 0.0 0 13.27 1.10 8
Zr 232.9 4.9 2 233.7 2.1 1 200
Nb 11.32 0.79 7
Mo 7.61 0.61 8
Ag 36.11 3.21 9 40
Cd 10.55 1.76 17 12.3 0.3
Sn 8.89 1.03 12
Sb 46.12 5.44 12 52.5 1.6
Cs 7.61 0.88 12 8.25 0.11
Ba 767.3 25.4 3 941.0 11.8 1 724.21 54.64 8 792 36
La 23.92 2.77 12 30.6 1.2
Ce 148.0 9.5 6 47.86 4.63 10 60
Pr 5.22 0.45 9
Nd 19.22 1.72 9 22 2
Sm 3.46 0.27 8 4 0.2
Eu 0.80 0.11 14 0.82 0.01
Dy 2.34 0.22 9 3
Ho 0.48 0.04 9
Yb 1.54 0.17 11 2
Lu 0.23 0.02 11 0.31 0.01
Tl 1.38 0.18 13 1.52 0.02
Pb 4976.80 615.47 12 5520 30
Th 14.16 1.75 12 18.1 0.3
U 8.03 0.88 11 9.11 0.3

Element concentrations qualified with a “J” are greater than the limit of detection, but less than the limit of quantitation. Shaded rows represent elements not characterised by NIST.

Acknowledgements

This work was supported by the Children's Health Environmental Core Centre at the University of Wisconsin Milwaukee, and funded through National Institute of Environmental Health Sciences Grant Number P30ES004184. The authors would also like to thank Razia Azen and Rebecca Klaper for providing significant comments and suggestions on this manuscript.

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