| Literature DB >> 30167349 |
C Roulston1, C Paton-Walsh1, T E L Smith2,3, É-A Guérette1, S Evers4,5, C M Yule6,7, G Rein8, G R Van der Werf9.
Abstract
Southeast Asia experiences frequent fires in fuel-rich tropical peatlands, leading to extreme episodes of regional haze with high concentrations of fine particulate matter (PM2.5) impacting human health. In a study published recently, the first field measurements of PM2.5 emission factors for tropical peat fires showed larger emissions than from other fuel types. Here we report even higher PM2.5 emission factors, measured at newly ignited peat fires in Malaysia, suggesting that current estimates of fine particulate emissions from peat fires may be underestimated by a factor of 3 or more. In addition, we use both field and laboratory measurements of burning peat to provide the first mechanistic explanation for the high variability in PM2.5 emission factors, demonstrating that buildup of a surface ash layer causes the emissions of PM2.5 to decrease as the peat fire progresses. This finding implies that peat fires are more hazardous (in terms of aerosol emissions) when first ignited than when still burning many days later. Varying emission factors for PM2.5 also have implications for our ability to correctly model the climate and air quality impacts downwind of the peat fires. For modelers able to implement a time-varying emission factor, we recommend an emission factor for PM2.5 from newly ignited tropical peat fires of 58 g of PM2.5 per kilogram of dry fuel consumed (g/kg), reducing exponentially at a rate of 9%/day. If the age of the fire is unknown or only a single value may be used, we recommend an average value of 24 g/kg.Entities:
Keywords: PM2.5; emissions; fire; peat
Year: 2018 PMID: 30167349 PMCID: PMC6108036 DOI: 10.1029/2017JD027827
Source DB: PubMed Journal: J Geophys Res Atmos ISSN: 2169-897X Impact factor: 4.261
Figure 1(a) Site 1, 12 July 2016; (b) Site 2 (okra), 13 July 2016; (c) Site 3, 14 July 2016; (d) Site 4, 20 July 2016; (e) Site 4, 27 July 2016; and (f) Site 4, 3 August 2016.
Figure 2Correlation plots of PM2.5 plotted against CO observed at the six peat fires sampled.
Dates, Age of Burn, Modified Combustion Efficiency (MCE), Fuel Moisture Content, Bulk Density, Minutes of Data Recorded, Mean and Standard Deviation of the Concentration of CO and PM2.5 Measured, Emission Ratios (with 1σ uncertainty), and Emission Factors (with 1σ uncertainty) for PM2.5 at Each of the Fires Sampled
| Sampling date and location | Age of burn (days) | MCE | Fuel moisture content | Bulk density | Minutes of data | Mean and stdev of CO mg/m3 | Mean and stdev of PM2.5 mg/m3 | Emission ratio PM2.5/CO | Emission factor PM2.5 g/kg |
|---|---|---|---|---|---|---|---|---|---|
| 12 July 2016 Site 1 | >10 | 0.84 | 54% | 0.583 g/cm3 | 60 | 31 ± 9 | 3.0 ± 1.0 | 0.10 ± 0.02 | 19 ± 5 |
| 13 July 2016 Site 2 | 0 | 0.81 | 62% | 0.438 g/cm3 | 48 | 61 ± 13 | 18 ± 5 | 0.30 ± 0.06 | 58 ± 15 |
| 14 July 2016 Site 3 | 12 | 0.85 | 53% | 0.605 g/cm3 | 60 | 25 ± 8 | 2.6 ± 1.2 | 0.10 ± 0.02 | 20 ± 5 |
| 20 July 2016 Site 4 | 6 | 0.84 | 54% | 0.625 g/cm3 | 100 | 22 ± 6 | 4.3 ± 1.4 | 0.20 ± 0.04 | 38 ± 10 |
| 27 July 2016 Site 4 | 13 | 0.85 | 54% | 0.625 g/cm3 | 60 | 16 ± 7 | 1.9 ± 0.9 | 0.12 ± 0.02 | 23 ± 6 |
| 3 August 2016 Site 4 | 20 | 0.8 | 54% | 0.625 g/cm3 | 14 | 46 ± 5 | 2.0 ± 1.1 | 0.04 ± 0.03 | 8 ± 6 |
Figure 3PM2.5 to CO emission ratios (upper panel) and MCE (lower panel) as a function of age of burn in days. A linear fit to the data is given in red and an exponential fit in blue: both fits yield an R 2 value of 0.97. The error bars indicate the estimated uncertainties in the age of the burn (±12 hr): in MCE (±3%) and the 1σ uncertainties in the emission ratio (see Table 1).
Figure 4Time series of 15‐min averages of emission ratios PM2.5 to CO (black dots and left‐hand axis) and MCE (grey dots and right‐hand axis). The emission ratio is high after ignition, dropping steadily as the fire burns downward. Note that Burn 2 was ignited in three sections (and the other burns in a single section) and shows considerably more variability in the emission ratio. During all three burns, the emission ratio increases immediately when the ash layer is removed (red dotted vertical line) and then decreases steadily. The time series also show occasional short‐lived increases in the emission ratio above a very low baseline level, which we interpret as a collapse in the ash pile, causing a disturbance to the surface. MCE does not vary significantly as the fire progresses in any of the experimental burns. In Burn 3 the addition of the artificial ash layer is shown by the grey dotted vertical line.