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(BRAVO) Study: Final Report. - Desert Research Institute

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<strong>Final</strong> <strong>Report</strong> — September 2004<br />

which was a critical orifice. The rotation rate was 6 mm/day, which over four weeks<br />

produced eight Apiezon-greased Mylar strips each 168 mm long. The strips, representing the<br />

finest particles, 0.26 > D p > 0.09 µm, were analyzed on the University of California at Davis<br />

DELTA Group synchrotron x-ray fluorescence (S-XRF) microprobe (Bench et al., 2002).<br />

The extremely high x-ray flux and 100% polarization allowed highly sensitive measurements<br />

of all elements sodium and heavier, to a few pg/m 3 , although elements heavier than<br />

molybdenum and lighter than gold are often interfered with by more abundant light elements.<br />

The seven larger-particle DRUM strips were archived and have not been analyzed.<br />

The results for two of the most abundant very fine elements, silicon and sulfur, are<br />

shown in Figure 5-9 for August 1999. Generally, the average concentrations of these<br />

particles are very low, (Si = 0.14 ng/m 3 , S = 1.88 ng/m 3 ) with the very fine sulfur<br />

(presumably sulfate) a small fraction of PM 2.5 sulfate. However, on occasion, sharp increases<br />

in both very fine Si and S occur, always in correlation (r 2 = 0.95 for August, for example).<br />

Comparison with high resolution PM 2.5 sulfate data show that on one occasion, August 18,<br />

there were three hours in which almost all of the PM 2.5 sulfate was in the very fine size range.<br />

The silicon is not accompanied by other crustal elements (enrichment factor vs. aluminum is<br />

∼20) but is probably derived from the same processes as the “large glassy plerospheres” long<br />

associated with coal-fired power plants. (The postulated formation mechanism is SiO 2 →<br />

SiO in the reducing fuel rich region of combustion, then oxidation to SiO 2 in the flame,<br />

followed by rapid condensation to very fine glassy mist that can form very fine particles,<br />

some of which agglomerate into the large plerospheres.) The sulfur in the largest peaks is<br />

probably H 2 SO 4 , based on hydrated droplets seen even after vacuum, which argues against<br />

long-range transport.<br />

Silicon x 25<br />

Sulfur<br />

Nanograms/m3<br />

80<br />

70<br />

60<br />

50<br />

40<br />

30<br />

20<br />

10<br />

0<br />

1<br />

2<br />

3<br />

4<br />

5<br />

6<br />

7<br />

8<br />

9<br />

11 13 15 17 19 21 23 25<br />

10 12 14 16 18 20 22 24<br />

August, 1999<br />

Figure 5-9. Timeline of very fine (0.26 µm > D p > 0.09 µm) silicon (x 25) and sulfur concentrations<br />

at Big Bend National Park during August 1999.<br />

HYSPLIT4 isentropic backward trajectory analyses at 500, 1,000, and 2,000 m AGL<br />

for these events show that the largest of these events in early and late August occurred with<br />

5-14

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