Abstract
Nucleation and growth of aerosol particles from atmospheric vapors constitutes a major source of global cloud condensation nuclei (CCN). The fraction of newly formed particles that reaches CCN sizes is highly sensitive to particle growth rates, especially for particle sizes <10 nm, where coagulation losses to larger aerosol particles are greatest. Recent results show that some oxidation products from biogenic volatile organic compounds are major contributors to particle formation and initial growth. However, whether oxidized organics contribute to particle growth over the broad span of tropospheric temperatures remains an open question, and quantitative mass balance for organic growth has yet to be demonstrated at any temperature. Here, in experiments performed under atmospheric conditions in the Cosmics Leaving Outdoor Droplets (CLOUD) chamber at the European Organization for Nuclear Research (CERN), we show that rapid growth of organic particles occurs over the range from −25 ◦C to 25 ◦C. The lower extent of autoxidation at reduced temperatures is compensated by the decreased volatility of all oxidized molecules. This is confirmed by particle-phase composition measurements, showing enhanced uptake of relatively less oxygenated products at cold temperatures. We can reproduce the measured growth rates using an aerosol growth model based entirely on the experimentally measured gas-phase spectra of oxidized organic molecules obtained from two complementary mass spectrometers. We show that the growth rates are sensitive to particle curvature, explaining widespread atmospheric observations that particle growth rates increase in the single-digit-nanometer size range. Our results demonstrate that organic vapors can contribute to particle growth over a wide range of tropospheric temperatures from molecular cluster sizes onward.
Originalsprog | Engelsk |
---|---|
Tidsskrift | Proceedings of the National Academy of Sciences of the United States of America |
Vol/bind | 115 |
Udgave nummer | 37 |
Sider (fra-til) | 9122-9127 |
Antal sider | 6 |
ISSN | 0027-8424 |
DOI | |
Status | Udgivet - 11 sep. 2018 |
Udgivet eksternt | Ja |
Bibliografisk note
Publisher Copyright:© 2018 National Academy of Sciences. All Rights Reserved.
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I: Proceedings of the National Academy of Sciences of the United States of America, Bind 115, Nr. 37, 11.09.2018, s. 9122-9127.
Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › peer review
}
TY - JOUR
T1 - Rapid growth of organic aerosol nanoparticles over a wide tropospheric temperature range
AU - Stolzenburg, Dominik
AU - Fischer, Lukas
AU - Vogel, Alexander L.
AU - Heinritzi, Martin
AU - Schervish, Meredith
AU - Simon, Mario
AU - Wagner, Andrea C.
AU - Dada, Lubna
AU - Ahonen, Lauri R.
AU - Amorim, Antonio
AU - Baccarini, Andrea
AU - Bauer, Paulus S.
AU - Baumgartner, Bernhard
AU - Bergen, Anton
AU - Bianchi, Federico
AU - Breitenlechner, Martin
AU - Brilke, Sophia
AU - Mazon, Stephany Buenrostro
AU - Chen, Dexian
AU - Dias, António
AU - Draper, Danielle C.
AU - Duplissy, Jonathan
AU - Haddad, Imad El
AU - Finkenzeller, Henning
AU - Frege, Carla
AU - Fuchs, Claudia
AU - Garmash, Olga
AU - Gordon, Hamish
AU - He, Xucheng
AU - Helm, Johanna
AU - Hofbauer, Victoria
AU - Hoyle, Christopher R.
AU - Kim, Changhyuk
AU - Kirkby, Jasper
AU - Kontkanen, Jenni
AU - Kürten, Andreas
AU - Lampilahti, Janne
AU - Lawler, Michael
AU - Lehtipalo, Katrianne
AU - Leiminger, Markus
AU - Mai, Huajun
AU - Mathot, Serge
AU - Mentler, Bernhard
AU - Molteni, Ugo
AU - Nie, Wei
AU - Nieminen, Tuomo
AU - Nowak, John B.
AU - Ojdanic, Andrea
AU - Onnela, Antti
AU - Passananti, Monica
AU - Petäjä, Tuukka
AU - Quéléver, Lauriane L.J.
AU - Rissanen, Matti P.
AU - Sarnela, Nina
AU - Schallhart, Simon
AU - Tauber, Christian
AU - Tomé, António
AU - Wagner, Robert
AU - Wang, Mingyi
AU - Weitz, Lena
AU - Wimmer, Daniela
AU - Xiao, Mao
AU - Yan, Chao
AU - Ye, Penglin
AU - Zha, Qiaozhi
AU - Baltensperger, Urs
AU - Curtius, Joachim
AU - Dommen, Josef
AU - Flagan, Richard C.
AU - Kulmala, Markku
AU - Smith, James N.
AU - Worsnop, Douglas R.
AU - Hansel, Armin
AU - Donahue, Neil M.
AU - Winkler, Paul M.
N1 - Funding Information: We thank T. Kurten and N. Hyttinen for providing helpful COSMOtherm volatility estimates. We also thank K. Ivanova, P. Carrie, L.-P. De Menezes, J. Dumollard, 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 contributions to the experiment. We thank the European Organization for Nuclear Research (CERN) for supporting CLOUD with important technical and financial resources and for providing a particle beam from the CERN Proton Synchrotron. This research was supported by the European Commission Seventh Framework Programme (Marie Curie Initial Training Network \u201CCLOUD-TRAIN\u201D 316662); German Federal Ministry of Education and Research Grants 01LK1222 A and 01LK1601 A; Swiss National Science Foundation Projects 20FI20 159851, 200020 172602, and 20FI20 172622; Austrian Research Funding Association FFG Project 846050; Austrian Science Fund (FWF) Projects J3951-N36 and J-3900; European Research Council (ERC) Consolidator Grant NANO-DYNAMITE 616075; ERC-Advanced Grant DAMOCLES 692891; ERC Starting Grant COALA 638703; Horizon 2020 Marie Sklodowska-Curie Grant 656994 (\u201CNano-CAVa\u201D); ERC Advanced Grant 742206 ATM-GP; Academy of Finland Center of Excellence Programme Grant 307331; US Department of Energy Grant DE-SC0014469; and the Presidium of the Russian Academy of Sciences Program \u201CHigh Energy Physics and Neutrino Astrophysics\u201D 2015. Funding Information: ACKNOWLEDGMENTS. We thank T. Kurten and N. Hyttinen for providing helpful COSMOtherm volatility estimates. We also thank K. Ivanova, P. Carrie, L.-P. De Menezes, J. Dumollard, 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 contributions to the experiment. We thank the European Organization for Nuclear Research (CERN) for supporting CLOUD with important technical and financial resources and for providing a particle beam from the CERN Proton Synchrotron. This research was supported by the European Commission Seventh Framework Programme (Marie Curie Initial Training Network \u201CCLOUD-TRAIN\u201D 316662); German Federal Ministry of Education and Research Grants 01LK1222 A and 01LK1601 A; Swiss National Science Foundation Projects 20FI20 159851, 200020 172602, and 20FI20 172622; Austrian Research Funding Association FFG Project 846050; Austrian Science Fund (FWF) Projects J3951-N36 and J-3900; European Research Council (ERC) Consolidator Grant NANO-DYNAMITE 616075; ERC-Advanced Grant DAMOCLES 692891; ERC Starting Grant COALA 638703; Horizon 2020 Marie Sklodowska-Curie Grant 656994 (\u201CNano-CAVa\u201D); ERC Advanced Grant 742206 ATM-GP; Academy of Finland Center of Excellence Programme Grant 307331; US Department of Energy Grant DE-SC0014469; and the Presidium of the Russian Academy of Sciences Program \u201CHigh Energy Physics and Neutrino Astrophysics\u201D 2015. Publisher Copyright: © 2018 National Academy of Sciences. All Rights Reserved.
PY - 2018/9/11
Y1 - 2018/9/11
N2 - Nucleation and growth of aerosol particles from atmospheric vapors constitutes a major source of global cloud condensation nuclei (CCN). The fraction of newly formed particles that reaches CCN sizes is highly sensitive to particle growth rates, especially for particle sizes <10 nm, where coagulation losses to larger aerosol particles are greatest. Recent results show that some oxidation products from biogenic volatile organic compounds are major contributors to particle formation and initial growth. However, whether oxidized organics contribute to particle growth over the broad span of tropospheric temperatures remains an open question, and quantitative mass balance for organic growth has yet to be demonstrated at any temperature. Here, in experiments performed under atmospheric conditions in the Cosmics Leaving Outdoor Droplets (CLOUD) chamber at the European Organization for Nuclear Research (CERN), we show that rapid growth of organic particles occurs over the range from −25 ◦C to 25 ◦C. The lower extent of autoxidation at reduced temperatures is compensated by the decreased volatility of all oxidized molecules. This is confirmed by particle-phase composition measurements, showing enhanced uptake of relatively less oxygenated products at cold temperatures. We can reproduce the measured growth rates using an aerosol growth model based entirely on the experimentally measured gas-phase spectra of oxidized organic molecules obtained from two complementary mass spectrometers. We show that the growth rates are sensitive to particle curvature, explaining widespread atmospheric observations that particle growth rates increase in the single-digit-nanometer size range. Our results demonstrate that organic vapors can contribute to particle growth over a wide range of tropospheric temperatures from molecular cluster sizes onward.
AB - Nucleation and growth of aerosol particles from atmospheric vapors constitutes a major source of global cloud condensation nuclei (CCN). The fraction of newly formed particles that reaches CCN sizes is highly sensitive to particle growth rates, especially for particle sizes <10 nm, where coagulation losses to larger aerosol particles are greatest. Recent results show that some oxidation products from biogenic volatile organic compounds are major contributors to particle formation and initial growth. However, whether oxidized organics contribute to particle growth over the broad span of tropospheric temperatures remains an open question, and quantitative mass balance for organic growth has yet to be demonstrated at any temperature. Here, in experiments performed under atmospheric conditions in the Cosmics Leaving Outdoor Droplets (CLOUD) chamber at the European Organization for Nuclear Research (CERN), we show that rapid growth of organic particles occurs over the range from −25 ◦C to 25 ◦C. The lower extent of autoxidation at reduced temperatures is compensated by the decreased volatility of all oxidized molecules. This is confirmed by particle-phase composition measurements, showing enhanced uptake of relatively less oxygenated products at cold temperatures. We can reproduce the measured growth rates using an aerosol growth model based entirely on the experimentally measured gas-phase spectra of oxidized organic molecules obtained from two complementary mass spectrometers. We show that the growth rates are sensitive to particle curvature, explaining widespread atmospheric observations that particle growth rates increase in the single-digit-nanometer size range. Our results demonstrate that organic vapors can contribute to particle growth over a wide range of tropospheric temperatures from molecular cluster sizes onward.
KW - Aerosol formation
KW - Aerosols
KW - CLOUD experiment
KW - Nanoparticle growth
KW - Volatile organic compounds
U2 - 10.1073/pnas.1807604115
DO - 10.1073/pnas.1807604115
M3 - Journal article
C2 - 30154167
AN - SCOPUS:85053056558
SN - 0027-8424
VL - 115
SP - 9122
EP - 9127
JO - Proceedings of the National Academy of Sciences of the United States of America
JF - Proceedings of the National Academy of Sciences of the United States of America
IS - 37
ER -