Author
Listed:
- Mingyi Wang
(Carnegie Mellon University
Carnegie Mellon University)
- Weimeng Kong
(California Institute of Technology)
- Ruby Marten
(Paul Scherrer Institute)
- Xu-Cheng He
(University of Helsinki)
- Dexian Chen
(Carnegie Mellon University
Carnegie Mellon University)
- Joschka Pfeifer
(CERN, the European Organization for Nuclear Research)
- Arto Heitto
(University of Eastern Finland)
- Jenni Kontkanen
(University of Helsinki)
- Lubna Dada
(University of Helsinki)
- Andreas Kürten
(Goethe University Frankfurt)
- Taina Yli-Juuti
(University of Eastern Finland)
- Hanna E. Manninen
(CERN, the European Organization for Nuclear Research)
- Stavros Amanatidis
(California Institute of Technology)
- António Amorim
(CENTRA and Faculdade de Ciências da Universidade de Lisboa)
- Rima Baalbaki
(University of Helsinki)
- Andrea Baccarini
(Paul Scherrer Institute)
- David M. Bell
(Paul Scherrer Institute)
- Barbara Bertozzi
(Karlsruhe Institute of Technology)
- Steffen Bräkling
(Tofwerk)
- Sophia Brilke
(University of Vienna)
- Lucía Caudillo Murillo
(Goethe University Frankfurt)
- Randall Chiu
(University of Colorado at Boulder)
- Biwu Chu
(University of Helsinki)
- Louis-Philippe Menezes
(CERN, the European Organization for Nuclear Research)
- Jonathan Duplissy
(University of Helsinki
University of Helsinki)
- Henning Finkenzeller
(University of Colorado at Boulder)
- Loic Gonzalez Carracedo
(University of Vienna)
- Manuel Granzin
(Goethe University Frankfurt)
- Roberto Guida
(CERN, the European Organization for Nuclear Research)
- Armin Hansel
(University of Innsbruck
Ionicon Analytik)
- Victoria Hofbauer
(Carnegie Mellon University
Carnegie Mellon University)
- Jordan Krechmer
(Aerodyne Research)
- Katrianne Lehtipalo
(University of Helsinki
Finnish Meteorological Institute)
- Houssni Lamkaddam
(Paul Scherrer Institute)
- Markus Lampimäki
(University of Helsinki)
- Chuan Ping Lee
(Paul Scherrer Institute)
- Vladimir Makhmutov
(P.N. Lebedev Physical Institute of the Russian Academy of Sciences)
- Guillaume Marie
(Goethe University Frankfurt)
- Serge Mathot
(CERN, the European Organization for Nuclear Research)
- Roy L. Mauldin
(Carnegie Mellon University
Carnegie Mellon University
University of Colorado at Boulder)
- Bernhard Mentler
(University of Innsbruck)
- Tatjana Müller
(Goethe University Frankfurt)
- Antti Onnela
(CERN, the European Organization for Nuclear Research)
- Eva Partoll
(University of Innsbruck)
- Tuukka Petäjä
(University of Helsinki)
- Maxim Philippov
(P.N. Lebedev Physical Institute of the Russian Academy of Sciences)
- Veronika Pospisilova
(Paul Scherrer Institute)
- Ananth Ranjithkumar
(University of Leeds)
- Matti Rissanen
(University of Helsinki
Tampere University)
- Birte Rörup
(University of Helsinki)
- Wiebke Scholz
(University of Innsbruck
Ionicon Analytik)
- Jiali Shen
(University of Helsinki)
- Mario Simon
(Goethe University Frankfurt)
- Mikko Sipilä
(University of Helsinki)
- Gerhard Steiner
(University of Innsbruck
Grimm Aerosol Technik Ainring)
- Dominik Stolzenburg
(University of Helsinki
University of Vienna)
- Yee Jun Tham
(University of Helsinki)
- António Tomé
(Institute Infante Dom Luíz, University of Beira Interior)
- Andrea C. Wagner
(Goethe University Frankfurt
University of Colorado at Boulder)
- Dongyu S. Wang
(Paul Scherrer Institute)
- Yonghong Wang
(University of Helsinki)
- Stefan K. Weber
(CERN, the European Organization for Nuclear Research)
- Paul M. Winkler
(University of Vienna)
- Peter J. Wlasits
(University of Vienna)
- Yusheng Wu
(University of Helsinki)
- Mao Xiao
(Paul Scherrer Institute)
- Qing Ye
(Carnegie Mellon University
Carnegie Mellon University
Carnegie Mellon University)
- Marcel Zauner-Wieczorek
(Goethe University Frankfurt)
- Xueqin Zhou
(Paul Scherrer Institute)
- Rainer Volkamer
(University of Colorado at Boulder)
- Ilona Riipinen
(University of Stockholm)
- Josef Dommen
(Paul Scherrer Institute)
- Joachim Curtius
(Goethe University Frankfurt)
- Urs Baltensperger
(Paul Scherrer Institute)
- Markku Kulmala
(University of Helsinki
University of Helsinki
Nanjing University
Beijing University of Chemical Technology)
- Douglas R. Worsnop
(University of Helsinki
Aerodyne Research)
- Jasper Kirkby
(CERN, the European Organization for Nuclear Research
Goethe University Frankfurt)
- John H. Seinfeld
(California Institute of Technology)
- Imad El-Haddad
(Paul Scherrer Institute)
- Richard C. Flagan
(California Institute of Technology)
- Neil M. Donahue
(Carnegie Mellon University
Carnegie Mellon University
Carnegie Mellon University
Carnegie Mellon University)
Abstract
A list of authors and their affiliations appears at the end of the paper New-particle formation is a major contributor to urban smog1,2, but how it occurs in cities is often puzzling3. If the growth rates of urban particles are similar to those found in cleaner environments (1–10 nanometres per hour), then existing understanding suggests that new urban particles should be rapidly scavenged by the high concentration of pre-existing particles. Here we show, through experiments performed under atmospheric conditions in the CLOUD chamber at CERN, that below about +5 degrees Celsius, nitric acid and ammonia vapours can condense onto freshly nucleated particles as small as a few nanometres in diameter. Moreover, when it is cold enough (below −15 degrees Celsius), nitric acid and ammonia can nucleate directly through an acid–base stabilization mechanism to form ammonium nitrate particles. Given that these vapours are often one thousand times more abundant than sulfuric acid, the resulting particle growth rates can be extremely high, reaching well above 100 nanometres per hour. However, these high growth rates require the gas-particle ammonium nitrate system to be out of equilibrium in order to sustain gas-phase supersaturations. In view of the strong temperature dependence that we measure for the gas-phase supersaturations, we expect such transient conditions to occur in inhomogeneous urban settings, especially in wintertime, driven by vertical mixing and by strong local sources such as traffic. Even though rapid growth from nitric acid and ammonia condensation may last for only a few minutes, it is nonetheless fast enough to shepherd freshly nucleated particles through the smallest size range where they are most vulnerable to scavenging loss, thus greatly increasing their survival probability. We also expect nitric acid and ammonia nucleation and rapid growth to be important in the relatively clean and cold upper free troposphere, where ammonia can be convected from the continental boundary layer and nitric acid is abundant from electrical storms4,5.
Suggested Citation
Mingyi Wang & Weimeng Kong & Ruby Marten & Xu-Cheng He & Dexian Chen & Joschka Pfeifer & Arto Heitto & Jenni Kontkanen & Lubna Dada & Andreas Kürten & Taina Yli-Juuti & Hanna E. Manninen & Stavros Ama, 2020.
"Rapid growth of new atmospheric particles by nitric acid and ammonia condensation,"
Nature, Nature, vol. 581(7807), pages 184-189, May.
Handle:
RePEc:nat:nature:v:581:y:2020:i:7807:d:10.1038_s41586-020-2270-4
DOI: 10.1038/s41586-020-2270-4
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Citations
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Cited by:
- Yongchun Liu & Junlei Zhan & Feixue Zheng & Boying Song & Yusheng Zhang & Wei Ma & Chenjie Hua & Jiali Xie & Xiaolei Bao & Chao Yan & Federico Bianchi & Tuukka Petäjä & Aijun Ding & Yu Song & Hong He , 2022.
"Dust emission reduction enhanced gas-to-particle conversion of ammonia in the North China Plain,"
Nature Communications, Nature, vol. 13(1), pages 1-10, December.
- Ke Yin & Shixin Mai & Jun Zhao, 2022.
"Atmospheric Sulfuric Acid Dimer Formation in a Polluted Environment,"
IJERPH, MDPI, vol. 19(11), pages 1-15, June.
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