EGU24-7707, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-7707
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Formation and temperature dependence of Highly Oxygenated Organic Molecules from ∆3-carene ozonolysis

Yuanyuan Luo1, Ditte Thomsen2, Emil Mark Iversen2, Pontus Roldin3,4, Jane Tygesen Skønager2, Linjie Li5, Michael Priestley5, Henrik B. Pedersen6, Mattias Hallquist5, Merete Bilde2, Marianne Glasius2, and Mikael Ehn1
Yuanyuan Luo et al.
  • 1University of Helsinki, Institute for Atmospheric and Earth System Research/Physics, Helsinki, Finland
  • 2Department of Chemistry, Aarhus University, Aarhus C, Denmark
  • 3Department of Physics, Lund University, Lund, Sweden
  • 4IVL, Swedish Environmental Research Institute, Malmö, Sweden
  • 5Department of Chemistry and Molecular Biology, University of Gothenburg, Gothenburg, Sweden
  • 6Department of Physics and Astronomy, Aarhus University, Aarhus C, Denmark

Monoterpenes, comprising 15% of global biogenic volatile organic compound emissions, play a pivotal role in atmospheric chemistry. ∆3-carene, the second most prevalent monoterpene, has been identified as a significant source of secondary organic aerosol (SOA) upon oxidation, potentially surpassing α-pinene under similar conditions. Despite its importance, research has predominantly focused on α-pinene , leaving gaps in our understanding of ∆3-carene's oxidation pathways, particularly its capacity to form highly oxygenated organic molecules (HOM).

To address this knowledge gap, we conducted an investigation into HOM formation during the ozonolysis of ∆3-carene using atmospheric simulation chambers. Employing a chemical ionization atmospheric pressure interface time-of-flight mass spectrometer with nitrate as the reagent ion (NO3-CIMS), we measured HOM resulting from ∆3-carene ozonolysis. Additionally, we explored the impact of temperature and relative humidity on HOM composition and distribution across various conditions (0, 10, and 20 ºC, and humidity levels below 15% and around 80%).

Our analysis revealed diverse HOM monomers and dimers from ∆3-carene ozonolysis. Predominant HOM monomers included C10H14,16O9 and C9H12,14O9, while the largest dimers comprised C19H30O6,10,11 and C20H32O7,9,11. Significantly, HOM monomers with 9 or more oxygen atoms and all dimers irreversibly condensed onto particles, while those with 6-8 oxygen atoms behaved as semi-volatile organic species, maintaining notable gas-phase concentrations. Intriguingly, ∆3-carene ozonolysis produced higher HOM concentrations than α-pinene, suggesting distinct formation pathways for these two monoterpenes. Furthermore, we observed a substantial decrease in HOM concentrations at lower temperatures, consistent with previous studies on α-pinene ozonolysis. Despite similar main HOM species at temperatures of 20, 10, and 0 ℃, the ratio of HOM dimers to monomers increased from 0.78 to 1.51 as temperatures decreased. This temperature-dependent variation underscores the complexity of ∆3-carene's atmospheric processing, revealing nuanced behaviors of HOM under different environmental conditions.

In conclusion, this study provides valuable insights into the HOM formation pathways of ∆3-carene, shedding light on its unique atmospheric chemistry. The observed differences in HOM concentrations and temperature-dependent behaviors highlight the need for a more comprehensive understanding of various monoterpenes, moving beyond the well-studied α-pinene. These findings contribute to the broader knowledge of biogenic volatile organic compounds and their impact on atmospheric processes.

How to cite: Luo, Y., Thomsen, D., Iversen, E. M., Roldin, P., Skønager, J. T., Li, L., Priestley, M., Pedersen, H. B., Hallquist, M., Bilde, M., Glasius, M., and Ehn, M.: Formation and temperature dependence of Highly Oxygenated Organic Molecules from ∆3-carene ozonolysis, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-7707, https://doi.org/10.5194/egusphere-egu24-7707, 2024.