treasure valley road dust study: final report - ResearchGate
treasure valley road dust study: final report - ResearchGate
treasure valley road dust study: final report - ResearchGate
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
?? Sieving each sample to obtain a suspendable fraction (< 38 µm geometric diameter),<br />
injecting this fraction into an enclosed chamber, and sampling onto Teflon-membrane<br />
and quartz-fiber filters through PM 10 and PM 2.5 impactor inlets (Chow et al., 1994a).<br />
In the laboratory, the soil samples were air-dried in a low-relative-humidity (approximately<br />
20% to 30%) environment and sieved through a Tyler 400-mesh screen (< 38 ?m geometric<br />
diameter) prior to resuspension in the laboratory chamber following the procedures described by<br />
Chow et al. (1994a).<br />
Filter samples were drawn through PM 10 and PM 2.5 inlets. Most of the mass of geological<br />
material is in the coarse particle portion of PM 10 (Houck et al., 1989a), and similar compositions<br />
were found for the PM 2.5 and PM 10 geological profiles (Chow and Watson, 1994b).<br />
Two additional samples were collected during the winter sampling period on board the<br />
TRAKER vehicle. Particles suspended from the <strong>road</strong> surface behind a moving tire were sampled<br />
through a tube into a plenum. A portion of the sample stream was drawn through a filter pack<br />
preceded by impactors with aerodynamic size cuts of either 10 ?m or 2.5 ?m. These filters were<br />
analyzed directly for mass and chemical speciation.<br />
All source profile samples were weighed and chemically characterized at the Desert<br />
Research Institutes Environmental Analysis Facility in Reno, Nevada. Samples were analyzed<br />
using Ion Chromatography (IC) for major ions, Automated Colorimetry (AC) for ammonium, X-<br />
Ray Fluorescence (XRF) for elements, and Thermal Optical Reflectance (TOR) for organic and<br />
elemental carbon. Table 7-1 lists all the chemical species analyzed and their corresponding<br />
mnemonics.<br />
Coarse particle Al, Si, P, Cl, K, and Ca values determined by XRF were originally<br />
adjusted for large particle self-absorption using the theoretical formulation developed by Dzubay<br />
(1975). This adjustment is a function of particle size distribution and composition. Since the<br />
actual particle size distribution and composition is unknown, the uncertainty of these adjustments<br />
is up to ± 25%, and is reflected in the <strong>report</strong>ed uncertainty. Particle size effects for Na and Mg<br />
are so large and variable that we cannot make accurate corrections for these two elements. Their<br />
raw, uncorrected concentrations are included in the data files, but they should not be considered<br />
quantitative for fine or coarse samples.<br />
A standard quality assurance test for speciated aerosol samples is to compare the<br />
reconstructed mass to the measured mass. Reconstructed mass should be less than or equal to the<br />
measured gravimetric mass within the limits of analytical uncertainties. Typical ratios of<br />
reconstructed mass to measured mass for PM10 range from 75% to 95%. Reconstructed mass is<br />
calculated from major species mass concentrations using the following equations to account for<br />
the unmeasured components of the aerosol (i.e., oxygen associated with mineral oxides and<br />
hydrogen associated with organic carbon compounds):<br />
[Soil] = 2.2*[Al] + 2.49*[Si] + 1.63*[Ca] + 2.42*[Fe] + 1.94*[Ti]<br />
[Organic Carbonacious Material (OCM)] = 1.4*[OC]<br />
7-2