Survival of newly formed particles in haze conditions
- Creators
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Marten, Ruby
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Xiao, Mao
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Rörup, Birte
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Wang, Mingyi
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Kong, Weimeng
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He, Xu-Cheng
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Stolzenburg, Dominik
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Pfeifer, Joschka
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Marie, Guillaume
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Wang, Dongyu S.
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Scholz, Wiebke
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Baccarini, Andrea
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Lee, Chuan Ping
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Amorim, Antonio
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Baalbaki, Rima
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Bell, David M.
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Bertozzi, Barbara
- Caudillo, Lucía
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Chu, Biwu
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Dada, Lubna
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Duplissy, Jonathan
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Finkenzeller, Henning
- Gonzalez Carracedo, Loïc
- Granzin, Manuel
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Hansel, Armin
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Heinritzi, Martin
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Hofbauer, Victoria
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Kemppainen, Deniz
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Kürten, Andreas
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Lampimäki, Markus
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Lehtipalo, Katrianne
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Makhmutov, Vladimir
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Manninen, Hanna E.
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Mentler, Bernhard
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Petäjä, Tuukka
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Philippov, Maxim
- Shen, Jiali
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Simon, Mario
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Stozhkov, Yuri
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Tomé, António
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Wagner, Andrea C.
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Wang, Yonghong
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Weber, Stefan K.
- Wu, Yusheng
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Zauner-Wieczorek, Marcel
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Curtius, Joachim
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Kulmala, Markku
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Möhler, Ottmar
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Volkamer, Rainer
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Winkler, Paul M.
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Worsnop, Douglas R.
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Dommen, Josef
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Flagan, Richard C.
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Kirkby, Jasper
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Donahue, Neil M.
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Lamkaddam, Houssni
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Baltensperger, Urs
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El Haddad, Imad
Abstract
Intense new particle formation events are regularly observed under highly polluted conditions, despite the high loss rates of nucleated clusters. Higher than expected cluster survival probability implies either ineffective scavenging by pre-existing particles or missing growth mechanisms. Here we present experiments performed in the CLOUD chamber at CERN showing particle formation from a mixture of anthropogenic vapours, under condensation sinks typical of haze conditions, up to 0.1 s⁻¹. We find that new particle formation rates substantially decrease at higher concentrations of pre-existing particles, demonstrating experimentally for the first time that molecular clusters are efficiently scavenged by larger sized particles. Additionally, we demonstrate that in the presence of supersaturated gas-phase nitric acid (HNO₃) and ammonia (NH₃), freshly nucleated particles can grow extremely rapidly, maintaining a high particle number concentration, even in the presence of a high condensation sink. Such high growth rates may explain the high survival probability of freshly formed particles under haze conditions. We identify under what typical urban conditions HNO₃ and NH₃ can be expected to contribute to particle survival during haze.
Additional Information
© 2022 The Author(s). Published by the Royal Society of Chemistry. This article is licensed under a Creative Commons Attribution-NonCommercial 3.0 Unported Licence. Received 23rd January 2022. Accepted 24th March 2022. We thank the European Organization for Nuclear Research (CERN) for supporting CLOUD with technical and financial resources and for providing a particle beam from the CERN Proton Synchrotron. This research has received funding from the European Community (EC) Seventh Framework Programme and the European Union (EU) H2020 programme (Marie Skłodowska Curie ITN CLOUD-TRAIN grant number 316662 and CLOUD-MOTION grant number 764991); European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement no. 895875 ("NPF-PANDA"); the Swiss National Science Foundation (no. 200021_169090, 200020_172602, 20FI20_172622); the US National Science Foundation (NSF; grant numbers AGS1602086, AGS1801329 and AGS-1801280); NASA graduate fellowship (NASA-NNX16AP36H); Project CLOUD-16 (project number 01LK1601C) funded by the German Bundesministerium für Bildung und Forschung (BMBF); ERC Advanced 'ATM-GP' grant no. 227463; The Portuguese Foundation for Science and Technology (project no. CERN/FIS-COM/0028/2019); ERC Consolidator grant NANODYNAMITE, 616075; the Austrian Science Fund (FWF; project no. P27295-N20); the Presidium of the Russian Academy of Sciences, the Program "Physics of Fundamental Interactions" 2017–2020; Ministry of Science and High education of the Russian Federation; VM acknowledges the Grant No. PCF IRN BR10965191. Author contributions. Conceptualization: R. M., M. X., M. W., J. Dommen, J. K., N. M. D., H. L., U. B. and I. E. H. Resources, prepared the CLOUD facility or measuring instruments: R. M., B. R., M. W., W. K., X.-C. H., D. S., J. P., G. M., D. S. W., W. S., A. B., C. P. L., R. B., L. C., B. C., J. C., L. D., J. Duplissy, H. F., L. G. C., M. G., A. H., M. H., V. H., D. K., A. K., M. K., K. L., V. M., H. E. M., B. M., O. M., T. P., M. P., J. S., M. S., Y. S., A. T., R. V., A. W., Y. Wang, S. K. W., P. M. W., Y. Wu, M. Z.-W., R. C. F., J. K., H. L., and I. E. H. Investigation: R. M., M. X., B. R., M. W., W. K., X.-C. H., D. S., J. P., G. M., D. S. W., W. S., A. B., C. P. L., A. A., R. B., D. B., B. B., L. C., L. D., J. Duplissy, H. F., L. G. C., M. G., M. H., V. H., D. K., M. L., V. M., B. M., J. S., M. S., A. T., A. W., S. K. W., Y. Wu, M. Z.-W., J. K., H. L., and I. E. H. Formal analysis: R. M., B. R., M. W., W. K., X. H., D. S., J. P., G. M., D. S. W., W. S., C. P. L., L. C., L. D., M. S., S. K. W., P. M. W., R. C. F., N. M. D., H. L., and I. E. H. Scientific discussion: R. M., M. X., B. R., M. W., W. K., X.-C. H., D. S., W. S., C. P. L., D. B., J. C., L. D., H. F., K. L., J. Dommen, R. C. F., J. K., N. M. D., H. L., U. B., and I. E. H. Writing: R. M., B. R., M. W., W. K., X.-C. H., D. S., J. P., D. S. W., J. Dommen, J. K., N. M. D., H. L., U. B., and I. E. H. There are no conflicts to declare.Attached Files
Published - d2ea00007e.pdf
Supplemental Material - d2ea00007e1.pdf
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Additional details
- PMCID
- PMC9119030
- Eprint ID
- 115140
- Resolver ID
- CaltechAUTHORS:20220614-221991000
- CERN
- Marie Curie Fellowship
- 316662
- Marie Curie Fellowship
- 764991
- Marie Curie Fellowship
- 895875
- Swiss National Science Foundation (SNSF)
- 200021_169090
- Swiss National Science Foundation (SNSF)
- 200020_172602
- Swiss National Science Foundation (SNSF)
- 20FI20_172622
- NSF
- AGS-1602086
- NSF
- AGS-1801329
- NSF
- AGS-1801280
- NASA Graduate Fellowship
- NNX16AP36H
- Bundesministerium für Bildung und Forschung (BMBF)
- 01LK1601C
- European Research Council (ERC)
- 227463
- Fundação para a Ciência e a Tecnologia (FCT)
- CERN/FIS-COM/0028/2019
- European Research Council (ERC)
- 616075
- FWF Der Wissenschaftsfonds
- P27295-N20
- Russian Academy of Sciences
- 2017-2020
- Ministry of Science and Higher Education of the Russian Federation
- Ministry of Education and Science (Kazakhstan)
- PCF IRN BR10965191
- Created
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2022-06-15Created from EPrint's datestamp field
- Updated
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2022-06-15Created from EPrint's last_modified field