Abstract
Biomass burning (BB) is a major source of atmospheric pollutants. Field and laboratory studies indicate that secondary organic aerosol (SOA) formation from BB emissions is highly variable. We investigated sources of this variability using a novel dual-smog-chamber method that directly compares the SOA formation from the same BB emissions under two different atmospheric conditions. During each experiment, we filled two identical Teflon smog chambers simultaneously with BB emissions from the same fire. We then perturbed the smoke with UV lights, UV lights plus nitrous acid (HONO), or dark ozone in one or both chambers. These perturbations caused SOA formation in nearly every experiment with an average organic aerosol (OA) mass enhancement ratio of 1.78 ± 0.91 (mean ± 1σ). However, the effects of the perturbations were highly variable ranging with OA mass enhancement ratios ranging from 0.7 (30% loss of OA mass) to 4.4 across the set of perturbation experiments. There was no apparent relationship between OA enhancement and perturbation type, fuel type, and modified combustion efficiency. To better isolate the effects of different perturbations, we report dual-chamber enhancement (DUCE), which is the quantity of the effects of a perturbation relative to a reference condition. DUCE values were also highly variable, even for the same perturbation and fuel type. Gas measurements indicate substantial burn-to-burn variability in the magnitude and composition of SOA precursor emissions, even in repeated burns of the same fuel under nominally identical conditions. Therefore, the effects of different atmospheric perturbations on SOA formation from BB emissions appear to be less important than burn-to-burn variability.
| Original language | English |
|---|---|
| Pages (from-to) | 6043-6058 |
| Number of pages | 16 |
| Journal | Journal of Geophysical Research |
| Volume | 122 |
| Issue number | 11 |
| DOIs | |
| State | Published - 2017 |
Funding
Carnegie Mellon University was supported in part by the DOE ASR (ER65296) and NSF (AGS-1256042), with instrumentation provided by NSF MRI (CBET-0922643) and the Wallace Research Foundation. The FLAME-IV experiment was supported by NSF (AGS-0936321). The authors thank Chris Hennigan for his useful discussions as well as the Fire Science Laboratory Staff and other FLAME-IV team members. In accordance with AGU data policy, experimental data can be found in the supporting information.
| Funder number |
|---|
| ER65296 |
| CBET-0922643 |
| AGS-0936321 |
| AGS-1256042 |
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