Journal of Environmental Quality 30:1118-1125 (2001)
© 2001 American Society of Agronomy, Crop Science Society of America, and Soil Science Society of America
TECHNICAL REPORT
Atmospheric Pollutants and Trace Gases
Aerosol Chemical and Optical Properties during the Mt. Zirkel Visibility Study
John G. Watson*,a,
Judith C. Chowa,
Douglas H. Lowenthala,
Catherine F. Cahillb,
Donald L. Blumenthalc,
L.Willard Richardsc and
Helena González Jorged
a Desert Research Institute, 2215 Raggio Parkway, Reno, NV 89512
b University of Alaska, 303 IARC, Fairbanks, AK 99775
c Sonoma Technology, Inc., 1360 Redwood Way, Suite C, Petaluma, CA 94954
d Univ. of La Laguna, Tenerife, Canary Islands, Spain
* Corresponding author (johnw{at}dri.edu)
Received for publication March 31, 2000.
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ABSTRACT
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Aerosol chemical and optical properties were measured near the Mt. Zirkel Wilderness Area in northwestern Colorado. Six-hour PM2.5 (particles with aerodynamic diameters less than 2.5 µm) mass concentrations and PM2.5 dry particle light scattering at 550 nm averaged 4.6 µg m-3 and 8.6 Mm-1, respectively. Sulfates, organic carbon, and geological material were the principle components of particle mass and light scattering. Hygroscopic growth was consistent with that expected for ammonium sulfate aerosols. Size distributions derived from three-wavelength (i.e., 450, 550, and 700 nm) nephelometer data were similar to those measured in other remote areas of the western USA. Quasi-dry chemical light scattering efficiencies derived using Mie theory were 3.6 m2 g-1 for organic carbon, 2.5 m2 g-1 for sulfates (ammonium sulfate and ammonium bisulfate), 2.6 m2 g-1 for ammonium nitrate, and 1.76 m2 g-1 for geological material. These values are lower than but consistent with previously reported results. Realistic efficiencies could not be derived using the multiple linear regression (MLR) approach.
Abbreviations: AAE, average absolute error EC, elemental carbon ELSIE, Elastic Light Scattering Interactive Efficiencies model GCVTC, Grand Canyon Visibility Transport Commission GMD, geometric mean diameter GSTD, geometric standard deviation MLR, multiple linear regression Mm-1, inverse megameter (1/106 m) MZVS, Mt. Zirkel Visibility Study OC, organic carbon PM2.5, particles with aerodynamic diameters less than 2.5 µm RH, relative humidity
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INTRODUCTION
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THE major cause of excessive haze in urban and nonurban areas is light scattering and absorption by suspended particles (Sloane and White, 1986; Malm et al., 1994; Watson and Chow, 1994). To require additional pollution controls on an existing industrial source or a group of sources outside 156 U.S. National Parks and Wilderness Areas, USEPA regulations require a perceptible increment in visibility impairment to be "reasonably attributable" to those sources (USEPA, 1980, 1999a,b). The Mt. Zirkel Wilderness Area (MZWA) in the Routt National Forest of northwestern Colorado (Fig. 1) is subject to these regulations. Potential contributors to haze-causing particles in the MZWA include the Craig and Hayden coal-fired power stations and the Steamboat Springs, Hayden, and Craig population centers located in the Yampa Valley west of the Wilderness. Other contributors include more distant emitters in northwestern Colorado, southern Wyoming, and western Utah. The Mt. Zirkel Visibility Study (MZVS) (Watson et al., 1996) was conducted in 1995 to determine: (i) the extent of visibility impairment, if any, within the MZWA; (ii) whether the cause of or contribution to any visibility impairment within the MZWA may be reasonably attributed to emissions from any source or group of sources; and (iii) the relative contribution of emissions from each source or group of sources to visibility impairment.
This paper estimates the fraction of extinction contributed by different chemical components of PM2.5. The measurements and theory to do this require certain assumptions that cannot be fully verified. The sensitivity of chemical light extinction estimates to assumptions about particle size and organic particle sampling artifacts are evaluated. These tests place reasonable bounds on the uncertainties in light extinction apportionment.
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METHODS
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Figure 1 shows the MZVS study domain, which included multiple sites within and outside of the Yampa Valley. The Buffalo Pass site (elevation 3224 m above mean sea level) was intended to represent visibility and aerosol concentrations in the wilderness, especially at high elevations and at its southern extreme, which is closest to Yampa Valley emissions sources. Ambient measurements were acquired from 1 Dec. 1994 through 30 Nov. 1995. Daytime 6-h average (06001200 and 12001800 mountain standard time [MST]) aerosol and light scattering measurements from summer (3 Aug. 19952 Sept. 1995) and fall (15 Sept. 199515 Oct. 1995) are included in these analyses because visibility was poorer than during winter and spring.
Hourly particle light scattering (bsp) measurements were acquired with two different types of nephelometers. A TSI (Minneapolis, MN) 3563 nephelometer (Bodhaine et al., 1991; Anderson et al., 1996; Anderson and Ogren, 1998) preceded by a PM2.5 size-selective inlet measured bsp at three wavelengths: 450 nm (blue, bspb), 550 nm (green, bspg), and 700 nm (red, bspr). This instrument was located in a heated shelter, exposing the sampled particles to an average relative humidity (RH) of 31 ± 11%, thereby approximating dry particle scattering. Because the particles were heated, some of the volatile components (e.g., ammonium nitrate, organic carbon) may have been lost, resulting in an underestimation of bsp by the TSI nephelometer. An open-air Optec (Fort Collins, CO) NGN-2 nephelometer (Molenar, 1997) measured total particle scattering at a wavelength of 550 nm at near-ambient humidity with no size-selective inlet. Hourly ambient relative humidity was also recorded.
Morning and afternoon PM2.5 samples were collected with medium-volume sequential filter samplers (SFS) (Chow et al., 1996). The sample was preceded by a PM2.5 size-selective inlet followed by sodium carbonatecoated, anodized aluminum tubes to remove gaseous nitric acid from the sample stream. Aluminum denuders of this type have been shown to remove >95% of the nitric acid in the air stream, even in highly polluted environments (Fitz and Hering, 1996; John et al., 1988). Two filter packs sampled concurrently at flow rates of 55 L min-1 each. One filter pack contained a Teflon-membrane filter (Gelman [Ann Arbor, MI] #R2PJ047) for gravimetric and elemental analysis followed downstream by a quartz-fiber filter (Pallflex #2500 QAT-UP; Pall Gelman Laboratory, Ann Arbor, MI) to collect volatile organics (Turpin et al., 1994). A parallel filter pack contained a quartz-fiber filter for analysis of inorganic ions, organic carbon (OC), and elemental carbon (EC), followed downstream by a sodium chloride (NaCl)impregnated cellulose-fiber filter for analysis of nitrate volatilized from the front quartz-fiber filter during sampling and any ambient gaseous nitric acid not trapped by the denuder.
The Teflon membrane filters were analyzed for mass by gravimetry on a Cahn 31 electronic balance (Thermo Cahn, Madison, WI) after equilibration at RH < 20% and for elements by X-ray fluorescence (XRF) (Watson et al., 1999) on a Kevex Model 700/8000 energy dispersive x-ray fluorescence analyzer (Kevex X-Ray, Scotts Valley, CA). The front quartz-fiber filter was analyzed for water-soluble chloride, nitrate, and sulfate with a Dionex (Sunnyvale, CA) 2020i ion chromatograph on an AS-4 column (Chow and Watson, 1999); for water-soluble potassium by flame atomic absorption spectrophotometry (Chow et al., 2002) on a Varian (Palo Alto, CA) SpectrAA-880; and for water-soluble ammonium by automated colorimetry on a Technicon (Tarrytown, NY) TRAACS autoanalyzer using the indophenol method. The backup NaCl-impregnated filter was analyzed for nitrate by ion chromatography. The front and backup quartz-fiber filters were analyzed for undifferentiated OC and EC using the IMPROVE thermaloptical reflectance method (Chow et al., 1993, 2001). Although chemical-specific size distributions measured with MOUDI impactors (e.g., Sloane et al., 1991) were considered in the MZVS study design, the low concentrations, limited access, and unpredictable visibility events made these measurements impractical. Particle light extinction was estimated with Mie theory using the ELSIE (Elastic Light Scattering Interactive Efficiencies) model (Sloane, 1986; Lowenthal et al., 1995).
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RESULTS AND DISCUSSION
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Aerosol Composition
Average morning (0600 to 1200 MST) and afternoon (1200 to 1800 MST) PM2.5 mass and chemical concentrations at the Buffalo Pass site are summarized in Table 1. During the summer and fall of 1995, average 6-h daytime mass was 4.6 ± 2.2 µg m-3 with a range of 0.95 to 9.0 µg m-3, excluding one apparent outlier (20 µg m-3, on 24 Aug. 1995, 0600 to 1200 MST). The PM2.5 nonvolatilized, volatilized, and total particulate nitrate and ammonium are presented, but volatilized ammonium and nitrate were a small fraction (
1%) of PM2.5 measured on the Teflon filter. While nitrate was a minor PM2.5 component, more than one-third of the total particulate nitrate had volatilized during sampling. In addition to carbonaceous and inorganic secondary aerosol, a geological material component was calculated by converting the major crustal species to their oxides (Zhang et al., 1994). The relative abundances of nonvolatilized ammonium, nitrate, and sulfate indicate that sulfate was fully neutralized as ammonium sulfate in most cases. The average molar ratio of ammonium to sulfate was 1.9.
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Table 1. Average morning (06001200 MST) and afternoon (12001800 MST) PM2.5 mass and chemical concentrations (µg m-3) and light scattering (Mm-1) at the Buffalo Pass site.
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Table 1 shows that the front-filter organic carbon, sulfate, geological material, and ammonium accounted for 24, 18, 15, and 6% of PM2.5, respectively. The average backup quartz-fiber filter OC concentration was nearly as large as that of the front quartz-fiber filter. Turpin et al. (1994) suggested that the backup OC represents adsorption of ambient volatile OC and should be subtracted from the front quartz-fiber filter OC. On the other hand, Eatough et al. (1993)(1995) demonstrated that quartz-fiber backup filters adsorb the products of organic particles volatilized from the front filter and recommended adding the backup-filter OC to the front-filter OC. Adjustment for artifact OC presents a major challenge in nonurban environments because OC concentrations are usually low (in the range of 0.5 to 1 µg m-3 for both front and backup quartz-fiber filters). Chow et al. (1996) reported that subtracting backup OC resulted in negative OC concentrations for 33% of samples from regional sampling sites in central California during the summer of 1990. At the Buffalo Pass site, more than 84% of the OC concentrations are zero or negative within their measurement uncertainties when the backup OC is subtracted. Since light scattering is caused by particles in the atmosphere prior to their collection on a filter, it is not affected by positive or negative carbon sampling artifacts. Light scattering is estimated below by adding, subtracting, and ignoring the carbon concentration on the backup filter.
Measured and reconstructed mass (sum of sulfate, nonvolatized nitrate and ammonium, 1.4 x OC [to account for unmeasured hydrogen and oxygen], EC, and geological material) are compared in Fig. 2. The OC component is the front-filter OC, front-filter minus backup-filter OC (assuming positive organic artifact), and front-filter plus backup-filter OC (assuming negative organic artifact) in Fig. 2a,b,c, respectively. The average ratios of reconstructed to measured mass based on front-filter OC (no correction), OC corrected for positive artifact, and OC corrected for negative artifact are 0.88, 0.59, and 1.26, respectively.

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Fig. 2. Measured PM2.5 (particles with aerodynamic diameters less than 2.5 µm) mass versus reconstructed mass with (a) front-filter organic carbon, (b) front-filter minus backup-filter organic carbon, (c) front-filter plus backup-filter organic carbon.
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Without independent information on the "true" or unbiased particulate OC concentration, the front-filter and backup-filter OC data imply that the average ambient OC concentration could range from 0.38 (assuming a positive artifact) to 2.97 µg m-3 (assuming a negative artifact). However, the gross under- and overestimations of mass that result from applying these corrections suggest that neither correction is warranted. This question is being further explored using organic denuders (XAD or charcoal-impregnated filters) and backup absorbents (Eatough et al., 1999).
Particle Light Scattering
The average particle light scattering measured by the TSI instrument at 550 nm (8.53 Mm-1) was comparable with Rayleigh scattering by atmospheric gases (8.42 Mm-1 at 3224 m). Linear regression of bspg vs. PM2.5 mass with effective-variance weighting (Watson et al., 1984) and intercept forced to zero yields a slope of 1.91 ± 0.12 m2 g-1 (r2 = 0.85) as the dry mass scattering efficiency at 550 nm. The average ratio of dry particle light scattering to PM2.5 (2.3 ± 1.0 m2 g-1) was comparable in magnitude with the linear regression slope.
Figure 3 shows how the ratio of hourly ambient total particle scattering (Optec bsp) to "quasi"-dry PM2.5 particle scattering (TSI bspg) changes with increasing RH. Periods influenced by cloud were excluded from Fig. 3. Also plotted in Fig. 3 is the hygroscopic growth curve for ammonium sulfate reported by Tang and Munkelwitz (1994). While the curve and data points are offset, growth inferred from the ratio of ambient to dry particle scattering is consistent with that expected for pure ammonium sulfate. Based on differences in spectral response and integration angle, Molenar (1997) estimated the Optec response to be about 3% greater than that of the TSI for 1-µm-diameter particles. For RH < 50% (i.e., dry conditions), the average ratio of total (Optec) to PM2.5 (TSI) particle scattering was 0.87 ± 0.27. On average, coarse particle scattering was not detected within the uncertainties of the light scattering measurements.

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Fig. 3. Hourly average ratio of Optec (ambient) total particle scattering to TSI (quasi-dry) PM2.5 (particles with aerodynamic diameters less than 2.5 µm) particle scattering (bsp) at 550 nm as a function of relative humidity (RH) (N = 1125).
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Derived Size Distributions
King et al. (1978), Heintzenberg (1975)(1980), Heintzenberg et al. (1981), and González Jorge and Ogren (1996) derived aerosol size distributions from measurements of optical depth and light scattering at different wavelengths. The particle light scattering coefficient (bsp) is defined as:
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where Qsp(m,
,D) is the optical scattering efficiency at wavelength
, m is the particle refractive index, D is the particle diameter, and n(D) is the number size distribution function (Seinfeld and Pandis, 1998). For multiple wavelengths, Eq. [1] becomes a series of simultaneous equations that can in principle be solved or inverted to obtain the size distribution.
Size distributions were derived for 62 aerosol sample periods from the corresponding time-integrated TSI nephelometer measurements at 450, 550, and 700 nm using the method of King et al. (1978). The kernel function for the inversion contains the optical cross section (optical efficiency times geometric cross section) and the Jungian power function [(D/2)-(
+1)] (King et al., 1978; González Jorge and Ogren, 1996). The exponents
are calculated from the empirical relation of Angstrom:
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where
is the wavelength and å = (
- 2). Since the shape of the size distribution is partially constrained in the inversion with the power law, it is possible to retrieve the size distribution in a larger number of discrete bins than the number of wavelengths. In this case, particle number and volume in 15 discrete bins were retrieved, as in González Jorge and Ogren (1996). The diameter interval was selected (Heintzenberg et al., 1981) based on the variations of the ratios of optical efficiencies at 450, 550, and 700 nm with respect to particle size. According to this criterion, there is independent information about the size distributions for diameters between 0.18 and 4 µm. Although the upper limit was further constrained by the size cutoff of the TSI nephelometer (2.5 µm), coarse particle concentrations were expected to be low, owing to vegetation and substantial precipitation at the measurement site.
It was assumed that all of the chemical components were internally mixed with a sample-specific refractive index, calculated as the volume-weighted average of the refractive indices of the components. The refractive index was assumed to be constant with particle size and wavelength. Sulfate was assumed to be fully neutralized as ammonium sulfate or partially neutralized as ammonium bisulfate, depending on the measured abundances of ammonium, nitrate, and sulfate. Water mass associated with sulfate and nitrate at the TSI RH was estimated using water activity data of Tang and Munkelwitz (1994) and Chan et al. (1992). Organic carbon was assumed to be nonhygroscopic (Malm et al., 1996). Assuming that the aerosol was completely dry would have changed the real and imaginary parts of the refractive index by less than 1 and 5%, respectively.
The resulting size distributions yield volume-weighted geometric mean diameters (GMD) averaging 0.29 ± 0.08 µm and ranging from 0.20 to 0.56 µm. Geometric standard deviations (GSTD) averaged 1.82 ± 0.36 and ranged from 1.23 to 2.6. For comparison, Pitchford and Green (1997) and Turpin et al. (1997) reported typical sulfur and sulfate GMD of about 0.3 µm at Meadview, AZ, during the summer of 1992 under low-humidity conditions. Although the inversion technique fits the measured scattering to within a few percent, the results are not unique. For example, Dellago and Horvath (1993) showed that two lognormal distributions with different GMDs, GSTDs, and particle volumes can produce the same spectral extinction. The uncertainties associated with this approach are discussed in detail by Heintzenberg et al. (1981) and González Jorge and Ogren (1996). This is a fundamental limitation of using a three-wavelength nephelometer to infer size distributions. The method does, however, substantially constrain the possible size distributions from all possibilities.
To validate these results, particle volumes were estimated from the measured chemical concentrations and their densities. The average absolute error (AAE), the average of the absolute differences between the measured and model-derived particle volume divided by the measured particle volume for each sample, expressed as a percent, was 35 ± 25%. The derived size distributions are self-consistent in one important respectbecause geological material is overwhelmingly associated with particles larger than 2.5 µm (e.g., Chow et al., 1996), Buffalo Pass samples with large geological material fractions should have larger derived GMDs. This is indeed the case, as shown in Fig. 4, where the correlation between derived GMD and the ratio of geological material to the reconstructed mass is 0.62.

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Fig. 4. Relationship between the derived geometric mean diameter (GMD) and the ratio of geological dust concentration to reconstructed mass.
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The derived size distributions were used in conjunction with the actual measured chemical concentrations to estimate scattering for the 62 sample periods using the ELSIE model. As described above, an internal mixture with constant composition as a function of size and nonhygroscopic organic carbon was assumed. The AAE between measured and estimated scattering at 550 nm was 58%. For comparison, the AAE for measured PM2.5 bsp and scattering estimated using Mie theory based on size-resolved chemical measurements was 15% at Meadview, AZ (Lowenthal et al., 2000). However, for 58, 43, 27, and 12 sample periods where model-derived and measured sample volumes agreed to within 75, 50, 25, and 10%, the AAE between measured and estimated scattering was 46, 28, 14, and 7%, respectively. The ability to reproduce measured scattering also improved at higher bspg. For example, measured and estimated scattering agreed with an AAE of 18% for 16 samples with bspg > 10 Mm-1 where model-derived and measured sample volumes agreed with an AAE of 50%.
Relationship between Chemical Composition and Light Scattering
Light scattering has been assigned to aerosol chemical components using scattering efficiencies derived from (i) multiple linear regression (MLR) (White and Roberts, 1977); (ii) Mie theory (Sloane, 1986; Zhang et al., 1994; Lowenthal et al., 1995); and (iii) "consensus" or literature values (e.g., Malm et al., 1996).
Results of MLR of bspg on sulfate (as ammonium sulfate), nitrate (as ammonium nitrate), organic carbon (as 1.4 x front-filter OC), and geological dust are presented in Table 2. To minimize the effects of hygroscopic growth, only samples (N = 52) with RH < 40% were considered. The resulting efficiencies differ from those of past studies. The sulfate and nitrate efficiencies are high (>5 m2 g-1) compared with those presented by Lowenthal et al. (2000) for Meadview, AZ. Indeed, scattering efficiencies of pure ammonium sulfate particles distributed log-normally with GMD of 0.2 and 0.4 µm and GSTD of 1.5 are 1.61 and 4.2 m2 g-1, respectively, at a wavelength of 550 nm. The OC efficiency of 1.07 m2 g-1 is also lower than expected and the geological dust efficiency is negative.
White (1986) and Lowenthal et al. (1995) discussed the potential effects of correlation (collinearity) between chemical species concentrations on MLR results. In this case, the apparently high coefficient for sulfate and the low coefficients for dust and organic carbon may have resulted from variance inflation caused by collinearity. Correlation coefficients were statistically significant between sulfate and organic carbon (0.41), sulfate and dust (0.29), and organic carbon and dust (0.61). This explanation is also supported by the similarity between the species mass-weighted average of the coefficients in Table 2 (2.2 m2 g-1) and the PM2.5 scattering efficiencies (1.91 to 2.3 m2 g-1) described above. Multiple linear regression results based on OC concentrations corrected for both positive and negative sampling artifacts (Table 2, second and third columns) were statistically indistinguishable from those based on the uncorrected front-filter OC.
The results obtained here do not imply that MLR does not work. Data quality obviously plays a role in the MLR results. Aerosol concentrations and light scattering levels were very low at this remote site. By contrast, Lowenthal et al. (1995) reported reasonable MLR results for Meadview in the Grand Canyon and Phoenix, AZ. Malm et al. (2000) reported excellent results based on MLR for Great Smokey Mountains National Park, where average PM2.5 concentrations were six times higher than those found at Buffalo Pass.
Scattering efficiencies for the chemical components (ammonium sulfate or ammonium bisulfate, ammonium nitrate, organic carbon, and geological dust) were estimated using the ELSIE model, as described by Lowenthal et al. (1995). Hygroscopic growth was estimated for the relative humidity in the TSI nephelometer, as described above. The average scattering efficiency and reconstructed scattering coefficient (the average of the product of the individual sample scattering efficiency and the corresponding chemical concentration) associated with each component are presented in Table 3. Backup-filter OC was neither subtracted nor added to the front-filter OC concentration. These values are compared with the corresponding scattering efficiencies adopted by the Grand Canyon Visibility Transport Commission (GCVTC) to evaluate visibility impairment in Class I areas along the Colorado Plateau (Ryan and Kendall, 1996). In this case, the effects of hygroscopic growth for RH
30% are accounted for using the growth function:
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Table 3. Scattering efficiencies and reconstructed scattering derived from Mie theory (Elastic Light Scattering Interactive Efficiencies Model, ELSIE) and literature consensus (Grand Canyon Visibility Transport Commission, GCVTC).
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Scattering estimated from the GCVTC efficiencies is independent of the actual ambient particle size distribution. Measured and reconstructed scattering estimated with ELSIE and the GCVTC protocol are compared for individual samples in Fig. 5. Comparisons of measured bsp with ELSIE and GCVTC estimates yielded AAEs of 58 and 72%, respectively. Note that the average of the efficiencies derived from Mie theory is lower than the GCVTC efficiencies. Nonetheless, this comparison shows that even with such divergent approaches for estimating light scattering, similar results were obtained.

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Fig. 5. Comparison of measured dry PM2.5 (particles with aerodynamic diameters less than 2.5 µm) particle scattering (bspg) based on uncorrected front-filter organic carbon (OC) with (a) particle scattering reconstructed from the Elastic Light Scattering Interactive Efficiencies (ELSIE) model and (b) particle scattering (bsp) based on Grand Canyon Visibility Transport Commission (GCVTC) scattering efficiencies (outlier excluded from regression).
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Table 3 also contains reconstructed ELSIE and GCVTC scattering based on OC with the backup-filter concentration subtracted and added. When the backup-filter OC is added, reconstructed scattering significantly overestimates measured scattering. When it is subtracted, reconstructed scattering underestimates measured scattering. The degree of underestimation is constrained by the fact that the OC concentration cannot be negative. These results are similar to those obtained for reconstructed PM2.5 mass. As noted, the measured bsp may be lower than actual, owing to particle volatilization caused by heating in the TSI nephelometer.
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CONCLUSIONS
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Six-hour average PM2.5 mass concentrations and dry particle scattering during the MZVS at Buffalo Pass, CO were low, averaging 4.6 µg m-3 and 8.6 Mm-1, respectively. Sulfates, organic carbon uncorrected for potential sampling artifacts, and geological material were the major components of PM2.5 mass. Hygroscopic growth inferred from the ratio of total (Optec nephelometer) to PM2.5 (TSI nephelometer) particle light scattering as a function of relative humidity was consistent with that expected for ammonium sulfate. Particle size distributions inverted from three-wavelength nephelometer data had an average volume geometric mean diameter (GMD) of 0.29 ± 0.08 µm and an average geometric standard deviation (GSTD) of 1.82 ± 0.36. The derived size distributions reproduced the measured volume and particle light scattering to within 50 and 28%, respectively, in 43 out of 62 sample cases. In addition, the derived GMDs and the corresponding mass fractions of geological material, which are expected to be associated with relatively larger particles than sulfate, nitrate, or carbon, were reasonably correlated (r = 0.62). Average "quasi"-dry scattering efficiencies based on the derived size distributions were 3.6 m2 g-1 for organics (estimated as 1.4 x OC), 2.5 m2 g-1 for sulfates (ammonium sulfate and ammonium bisulfate), 2.6 m2 g-1 for ammonium nitrate, and 1.76 m2 g-1 for geological material. The multiple linear regression (MLR) approach was not able to resolve scattering efficiencies for individual chemical components. This might be caused by the low aerosol concentrations and scattering levels at this remote site and to correlations among the chemical species concentrations.
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