Can Particle Size Magnifiers detect HOMs with carbon numbers between C10 and C30?
- 1Institute of Ion Physics and Applied Physics, University of Innsbruck, Innsbruck, Austria
- 2IONICON Analytik GmbH, 6020 Innsbruck, Austria
- 3Institute for Atmospheric and Earth System Research / Physics , Faculty of Science, University of Helsinki, Finland
- 4GRIMM Aerosol Technik Ainring GmbH & Co. KG, 83404 Ainring
The Particle Size Magnifier (PSM, Airmodus) [1] is able to size sub 3 nm particles in mobility diameter. A PSM‘s sensitivity and cutoff size (50% detection efficiency) is usually calibrated only with particles out of metal oxides, e.g. tungsten oxide [2], or with different salt particles [1]. The PSM used in this experiment has a cutoff size for ammonium sulfate particles of 1.3 nm in mobility diameter. Ternary nucleation in the atmospheric boundary layer, however, involves organic molecules. It is therefore questionable, if the inorganic calibration curves of the PSM can be applied to these particles.
In this study we aim to understand the PSM‘s response to purely biogenic particles as well as to highly oxidized molecules (HOMs) with carbon backbones of different sizes (C10-, C15-, C20- and C30-HOMs). We used a flow reactor with a short reaction time of about 9s that allows for undisturbed radical – radical reactions due to negligible wall contacts to quantitatively generate HOMs by ozonolysis of different precursors. Reactants were ozone and either alpha-Pinene (C10H16) or beta-Caryophyllene (C15H24) with and without an OH-scavenger.
A recent study [3] demonstrated, that the ozonolysis of alpha-Pinene produces covalently bound C20-HOMs from self- and cross-reactions of two C10-peroxy radicals. The C30-HOMs are formed equivalently from C15-radicals of beta-Caryophyllene oxidation. This mechanism shows, why the C20- and C30-HOMs increase quadratically, in contrast to the C10- and C15-HOMs, that increase linearly with respective reacted precursor concentrations. Making use of this principle, we are able to show, that already C20-HOMs are detected by the PSM, but with a much smaller detection efficiency than the C30-HOMs, that have an ion mobility diameter of approximately 1.6 nm. Our size-dependent calibration gave a steep sensitivity increase around the particle size of about 1.8 nm mobility diameter for organic particles, showing, that organics are far more difficult to detect than ammonium sulfate particles.
[1] J. Vanhanen, J. Mikkilä, K. Lehtipalo, M. Sipilä, H. E. Manninen, E. Siivola, T. Petäjä & M. Kulmala (2011) Particle Size Magnifier for Nano-CN Detection, Aerosol Science and Technology, 45:4, 533-542, DOI: 10.1080702786826.2010.547889
[2] J. Kangasluoma, M. Attoui, H. Junninen, K. Lehtipalo, A. Samodurov, F. Korhonen, N. Sarnela, A. Schmidt-Ott, D. Worsnop, M. Kulmala, T. Petäjä (2015) Sizing of neutral sub 3nm tungsten oxide clusters using Airmodus Particle Size Magnifier, Journal of Aerosol Science, 87, 53-62, DOI: https://doi.org/10.1016/j.jaerosci.2015.05.007
[3] T. Berndt, B. Mentler, W. Scholz, L. Fischer, H. Herrmann, M. Kulmala, A. Hansel (2018) Accretion Product Formation from Ozonolysis and OH Radical Reaction of α-Pinene: Mechanistic Insight and the Influence of Isoprene and Ethylene, Environ. Sci. Technol. 2018, 52, 19, 11069-11077, DOI: https://doi.org/10.1021/acs.est.8b02210
How to cite: Scholz, W., Rörup, B., Leiminger, M., Steiner, G., Lehtipalo, K., Kangasluoma, J., and Hansel, A.: Can Particle Size Magnifiers detect HOMs with carbon numbers between C10 and C30?, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-9468, https://doi.org/10.5194/egusphere-egu2020-9468, 2020