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Secondary Organic Aerosols. Formation and Characterization. Overview. Background Formation Modeling Theoretical investigations Chamber experiments. Particulate Matter in the Atmosphere. PM affects visibility, climate, health. Inorganic fractions well characterized.
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Secondary Organic Aerosols Formation and Characterization
Overview • Background • Formation • Modeling • Theoretical investigations • Chamber experiments
Particulate Matter in the Atmosphere PM affects visibility, climate, health. Inorganic fractions well characterized. Organic fractions are poorly characterized, very complex.
Modeling Atmospheric Aerosol Formation • Model aerosol formation to understand its affects on air quality and climate change • Accurately represent organic fraction • Better characterization chemical composition of atmospheric organic aerosols • Better understanding of secondary organic aerosol (SOA) formation, including the role of MW-building reactions (i.e., "accretion reactions”)
Aerosols = liquid or solid particles suspended in a gas (e.g., the atmosphere) Physical state of compound largely dependent on pure-compound vapor pressure (p°L) How can a compound have low/lower volatility? Inherent: compounds emitted as PM Undergo oxidation: VOCs + NOx,O3, •OH → oxidation products Undergo MW-building reactions: oxidation products/ atmospheric compounds→ high-MW products Lowering volatility increases the tendency of a compound to condense, thereby forming PM Formation of Atmospheric Organic Aerosols
-COOH oxidation products -OH -C=O Formation of Atmospheric Organic Aerosols OA gas/particle (G/P) partitioning gas/particle (G/P)partitioning high molecular-weight (MW)/ low-volatility products accretion reactions Biogenic Anthropogenic oxidation Emissions Volatile Organic Compounds
Fundamental Thermodynamics of SOA Formation by Accretion Reaction Ag + Bg Cg Cliq
2A C1 2A C2 + H2O A + B C3 A + B C4 + H2O Mathematical Solution Process Multiple accretion reactions and products from parent compound A: Mass balance leads to: A and C denote concentrations (µg m-3) N number of accretion products from A
Accretion Reactions of Aldehydes and Ketones • Based on work of Jang and Kamens • Reaction of 4 n-aldehydes and ketones (C4, C6, C8, C10) • 5 Accretion products for each aldehyde/ketone (hydrate, dimer, trimer, hemiacetal, acetal, hydroxy carbonyl, unsaturated carbonyl) • Considered same reactions for pinonaldehyde, inputs representative of ambient conditions
Accretion Reactions of Dialdehydes, Methylglyoxal, Diketones
Accretion Reactions of Carboxylic and Dicarboxylic Acids: Ester and Amide Formation • Accretion reactions of 5 acids • Ester formation w/ MBO, amide formation w/DEA and NH3 • Inputs representative of ambient conditions
Results for Carboxylic and Dicarboxylic Acids MBO0 and DEA0= 1 µg m-3 NH3 ≈ 0.1 µg m-3 OPMna = 10 µg m-3 RH = 20%, T = 298 K • For malic, maleic, and pinic acids OPM formation is significant • For acetic acid, accretion products do not condense into OPM phase • Esters and at least 1 amide contribute to predicted level of additional OPM Predicted OPM as a Function of A0
Implications for Observed OPM Formation in Chamber Experiments • MW 256-695 g mol-1 dominant accretion reactions • MW 200-900 g mol-1, combination of monomers (Tolocka et al., 2004) • MW 250-450 g mol-1 dimers, MW 450-950 g mol-1 trimers and higher oligomers (Gao et al., 2004a,b) OPMna = 0, RH = 50%, T = 298 K
Summary of Dissertation Research • Accretion reactions appear to play a role in atmospheric SOA formation • Currently, the dominant accretion reactions/products are not known • Developed a “first-cut” approach to identifying favorable reactions and estimating their potential contribution to SOA • Lot’s of work to be done!
PTRMS Reaction Chamber Ozone Monitor Ozone Source SO2 Monitor 2 Cylinder Air CIMS Humidifier SMPS T, RH UFPC SO2 Scrubber HTDMA Filter Sampler TDCIMS Biomass Chamber Biogenic Aerosol Chamber
Filter Sample Analysis: GC x GC • Entire sample passed through two different columns • First column usually separates based on volatility, second usually separates based on polarity
GC x GC Spectrum alcohols polarity (← ret. time) aldehydes alkanes volatility (→ ret. time)
Future Plans • Look for accretion products in filter samples from chamber experiments and field experiments • Use PTR-MS to “track” gas phase species • Use GC x GC to analyze filter samples • Compare data with thermodynamic model predictions • Parameterize reactions to include in regional/global models