Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published January 4, 2018 | Published
Journal Article Open

Influence of temperature on the molecular composition of ions and charged clusters during pure biogenic nucleation

Abstract

It was recently shown by the CERN CLOUD experiment that biogenic highly oxygenated molecules (HOMs) form particles under atmospheric conditions in the absence of sulfuric acid, where ions enhance the nucleation rate by 1–2 orders of magnitude. The biogenic HOMs were produced from ozonolysis of α-pinene at 5 °C. Here we extend this study to compare the molecular composition of positive and negative HOM clusters measured with atmospheric pressure interface time-of-flight mass spectrometers (APi-TOFs), at three different temperatures (25, 5 and −25 °C). Most negative HOM clusters include a nitrate (NO_3−) ion, and the spectra are similar to those seen in the nighttime boreal forest. On the other hand, most positive HOM clusters include an ammonium (NH_4+) ion, and the spectra are characterized by mass bands that differ in their molecular weight by ∼ 20 C atoms, corresponding to HOM dimers. At lower temperatures the average oxygen to carbon (O : C) ratio of the HOM clusters decreases for both polarities, reflecting an overall reduction of HOM formation with decreasing temperature. This indicates a decrease in the rate of autoxidation with temperature due to a rather high activation energy as has previously been determined by quantum chemical calculations. Furthermore, at the lowest temperature (−25 °C), the presence of C30 clusters shows that HOM monomers start to contribute to the nucleation of positive clusters. These experimental findings are supported by quantum chemical calculations of the binding energies of representative neutral and charged clusters.

Additional Information

© 2018 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: 05 May 2017 – Discussion started: 29 May 2017. Revised: 31 Oct 2017 – Accepted: 10 Nov 2017 – Published: 04 Jan 2018. Data availability: Data related to this article are available online at https://doi.org/10.5281/zenodo.1133985. We would like to thank CERN for supporting CLOUD with important technical and financial resources, and for providing a particle beam from the CERN Proton Synchrotron. We also thank P. Carrie, L.-P. De Menezes, J. Dumollard, K. Ivanova, F. Josa, I. Krasin, R. Kristic, A. Laassiri, O. S. Maksumov, B. Marichy, H. Martinati, S. V. Mizin, R. Sitals, A. Wasem and M. Wilhelmsson for their important contributions to the experiment. This research has received funding from the EC Seventh Framework Programme (Marie Curie Initial Training Network CLOUD-ITN no. 215072, MC-ITN CLOUD-TRAIN no. 316662, the ERC-Starting grant MOCAPAF no. 57360, the ERC-Consolidator grant NANODYNAMITE no. 616075 and ERC-Advanced grant ATMNUCLE no. 227463), European Union's Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement no. 656994, the PEGASOS project funded by the European Commission under the Framework Programme 7 (FP7-ENV-2010-265148), the German Federal Ministry of Education and Research (project nos. 01LK0902A and 01LK1222A), the Swiss National Science Foundation (project nos. 200020_152907, 206021_144947 and 20FI20_159851), the Academy of Finland (Center of Excellence project no. 1118615), the Academy of Finland (135054, 133872, 251427, 139656, 139995, 137749, 141217, 141451, 299574), the Finnish Funding Agency for Technology and Innovation, the Väisälä Foundation, the Nessling Foundation, the University of Innsbruck research grant for young scientists (Cluster Calibration Unit), the Portuguese Foundation for Science and Technology (project no. CERN/FP/116387/2010), the Swedish Research Council, Vetenskapsrådet (grant 2011-5120), the Presidium of the Russian Academy of Sciences and Russian Foundation for Basic Research (grants 08-02-91006-CERN and 12-02-91522-CERN), the US National Science Foundation (grants AGS1447056, and AGS1439551), and the Davidow Foundation. We thank the tofTools team for providing tools for mass spectrometry analysis. The authors declare that they have no conflict of interest.

Attached Files

Published - acp-18-65-2018.pdf

Files

acp-18-65-2018.pdf
Files (2.5 MB)
Name Size Download all
md5:3376d0cccefde2c1590a57169fc5fb1f
2.5 MB Preview Download

Additional details

Created:
August 19, 2023
Modified:
October 20, 2023