Published July 18, 2011 | Version Published + Supplemental Material
Journal Article Open

Explicit modelling of SOA formation from α-pinene photooxidation: sensitivity to vapour pressure estimation

  • 1. ROR icon Laboratoire Interuniversitaire des Systèmes Atmosphériques
  • 2. ROR icon Aerodyne Research
  • 3. ROR icon California Institute of Technology
  • 4. ROR icon National Center for Atmospheric Research

Abstract

The sensitivity of the formation of secondary organic aerosol (SOA) to the estimated vapour pressures of the condensable oxidation products is explored. A highly detailed reaction scheme was generated for α-pinene photooxidation using the Generator for Explicit Chemistry and Kinetics of Organics in the Atmosphere (GECKO-A). Vapour pressures (P^(vap)) were estimated with three commonly used structure activity relationships. The values of P^(vap) were compared for the set of secondary species generated by GECKO-A to describe α-pinene oxidation. Discrepancies in the predicted vapour pressures were found to increase with the number of functional groups borne by the species. For semi-volatile organic compounds (i.e. organic species of interest for SOA formation), differences in the predicted Pvap range between a factor of 5 to 200 on average. The simulated SOA concentrations were compared to SOA observations in the Caltech chamber during three experiments performed under a range of NO_x conditions. While the model captures the qualitative features of SOA formation for the chamber experiments, SOA concentrations are systematically overestimated. For the conditions simulated, the modelled SOA speciation appears to be rather insensitive to the P^vap estimation method.

Additional Information

© 2011 the Author(s). This work is distributed under the Creative Commons Attribution 3.0 License. Published by Copernicus Publications on behalf of the European Geosciences Union. Received: 24 March 2011; Published in Atmos. Chem. Phys. Discuss.: 29 March 2011; Revised: 28 June 2011; Accepted: 8 July 2011; Published: 18 July 2011. NCAR is sponsored by the National Science Foundation. JLT was supported and SM was supported in part by a grant from the US Department of Energy, Office of Science, ER, DE-FG02-ER63993.

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Published - Valorso2011p15497Atmos_Chem_Phys.pdf

Supplemental Material - acp-11-6895-2011-supplement.pdf

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Additional details

Identifiers

Eprint ID
24882
DOI
10.5194/acp-11-6895-2011
Resolver ID
CaltechAUTHORS:20110816-103548738

Funding

NSF
Department of Energy (DOE)
DE-FG02-ER63993

Dates

Created
2011-08-16
Created from EPrint's datestamp field
Updated
2021-11-09
Created from EPrint's last_modified field