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Air Quality Criteria for Lead Volume II of II - (NEPIS)(EPA) - US ...

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material to describe the chemical or kinetic factors controlling a metal’s release, transport,<br />

and/or exposure.<br />

X-Ray absorption Spectroscopy (XAS). X-ray absorption spectroscopy (XAS) is a<br />

powerful technique using the tunable, monochromatic (white light) X-rays produced by a<br />

synchrotron (2-4 GeV) to record oscillations in atomic absorption within a few 100 GeV <strong>of</strong> an<br />

element’s absorption edge. Spectra provide in<strong>for</strong>mation on both chemical state and atomic<br />

structure. Measurements are theoretically available <strong>for</strong> all elements and are not surface-sensitive<br />

nor sample-sensitive (i.e., gases, liquids, solids, and amorphous materials are testable).<br />

High-energy spectra within 30 eV <strong>of</strong> the edge, termed XANES (X-ray absorption near<br />

edge structure spectroscopy (Fendorf et al., 1994; Maginn, 1998), are particularly suited <strong>for</strong><br />

determination and quantification (10 to 100 ppm) <strong>of</strong> metal in a particular oxidation state<br />

(Szulczewski et al., 1997; Shaffer et al., 2001; Dupont et al., 2002). The lower-energy spectra<br />

persist some 100 eV above the edge. These oscillations are termed EXAFS (extended X-ray<br />

absorption fine structure) and are more commonly used <strong>for</strong> speciation analyses (Welter et al.,<br />

1999; Manceau et al., 1996, 2000a; Isaure et al., 2002).<br />

The main limitations to XAS techniques are (1) the lack <strong>of</strong> spatial resolution; (2) XAS<br />

techniques provide only a weighted average signal <strong>of</strong> structural configurations, providing<br />

in<strong>for</strong>mation on the predominant <strong>for</strong>m <strong>of</strong> the metal, while minor species, which may be more<br />

bioavailable, can be overlooked; (3) access to synchrotrons is limited and the beam time required<br />

to conduct a site investigation would be prohibitive; (4) a large spectral library must be<br />

developed; (5) generally, poor fits to solution models are achieved when the compound list is<br />

large; and (6) high atomic number elements have masking problems based on compound density.<br />

X-Ray Diffraction (XRD). In X-ray diffraction, a monochromatic Fe, Mo, Cr, Co, W, or<br />

Cu X-ray beam rotates about a finely powdered sample and is reflected <strong>of</strong>f the interplanar<br />

spacings <strong>of</strong> all crystalline compounds in the sample, fulfilling Bragg’s law (nλ = 2dsinθ). The<br />

identification <strong>of</strong> a species from this pattern is based upon the position <strong>of</strong> the lines (in terms <strong>of</strong><br />

θ or 2θ) and their intensities as recorded by an X-ray detector. The diffraction angle (2θ) is<br />

determined by the spacing between a particular set <strong>of</strong> atomic planes. Identification <strong>of</strong> the species<br />

is empirical, and current available databases contain more than 53,000 compounds.<br />

If a sample contains multiple compounds, interpretation becomes more difficult and<br />

computer-matching programs are essential. In some instances, by measuring the intensity <strong>of</strong> the<br />

AX7-13

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