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Formation of Highly Oxygenated Organic Molecules from $\alpha$-Pinene Ozonolysis: Chemical Characteristics, Mechanism, and Kinetic Model Development

Terpenes are emitted by vegetation, and their oxidation in the atmosphere is an important source of secondary organic aerosol (SOA). A part of this oxidation can proceed through an autoxidation process, yielding highly oxygenated organic molecules (HOMs) with low saturation vapor pressure. They can...

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Autores principales: Molteni, Ugo, Simon, Mario, Heinritzi, Martin, Hoyle, Christopher R, Bernhammer, Anne-Kathrin, Bianchi, Federico, Breitenlechner, Martin, Brilke, Sophia, Dias, António, Duplissy, Jonathan, Frege, Carla, Gordon, Hamish, Heyn, Claudia, Jokinen, Tuija, Kürten, Andreas, Lehtipalo, Katrianne, Makhmutov, Vladimir, Petäjä, Tuukka, Pieber, Simone M, Praplan, Arnaud P, Schobesberger, Siegfried, Steiner, Gerhard, Stozhkov, Yuri, Tomé, António, Tröstl, Jasmin, Wagner, Andrea C, Wagner, Robert, Williamson, Christina, Yan, Chao, Baltensperger, Urs, Curtius, Joachim, Donahue, Neil M, Hansel, Armin, Kirkby, Jasper, Kulmala, Markku, Worsnop, Douglas R, Dommen, Josef
Lenguaje:eng
Publicado: 2019
Materias:
Acceso en línea:https://dx.doi.org/10.1021/acsearthspacechem.9b00035
http://cds.cern.ch/record/2805293
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author Molteni, Ugo
Simon, Mario
Heinritzi, Martin
Hoyle, Christopher R
Bernhammer, Anne-Kathrin
Bianchi, Federico
Breitenlechner, Martin
Brilke, Sophia
Dias, António
Duplissy, Jonathan
Frege, Carla
Gordon, Hamish
Heyn, Claudia
Jokinen, Tuija
Kürten, Andreas
Lehtipalo, Katrianne
Makhmutov, Vladimir
Petäjä, Tuukka
Pieber, Simone M
Praplan, Arnaud P
Schobesberger, Siegfried
Steiner, Gerhard
Stozhkov, Yuri
Tomé, António
Tröstl, Jasmin
Wagner, Andrea C
Wagner, Robert
Williamson, Christina
Yan, Chao
Baltensperger, Urs
Curtius, Joachim
Donahue, Neil M
Hansel, Armin
Kirkby, Jasper
Kulmala, Markku
Worsnop, Douglas R
Dommen, Josef
author_facet Molteni, Ugo
Simon, Mario
Heinritzi, Martin
Hoyle, Christopher R
Bernhammer, Anne-Kathrin
Bianchi, Federico
Breitenlechner, Martin
Brilke, Sophia
Dias, António
Duplissy, Jonathan
Frege, Carla
Gordon, Hamish
Heyn, Claudia
Jokinen, Tuija
Kürten, Andreas
Lehtipalo, Katrianne
Makhmutov, Vladimir
Petäjä, Tuukka
Pieber, Simone M
Praplan, Arnaud P
Schobesberger, Siegfried
Steiner, Gerhard
Stozhkov, Yuri
Tomé, António
Tröstl, Jasmin
Wagner, Andrea C
Wagner, Robert
Williamson, Christina
Yan, Chao
Baltensperger, Urs
Curtius, Joachim
Donahue, Neil M
Hansel, Armin
Kirkby, Jasper
Kulmala, Markku
Worsnop, Douglas R
Dommen, Josef
author_sort Molteni, Ugo
collection CERN
description Terpenes are emitted by vegetation, and their oxidation in the atmosphere is an important source of secondary organic aerosol (SOA). A part of this oxidation can proceed through an autoxidation process, yielding highly oxygenated organic molecules (HOMs) with low saturation vapor pressure. They can therefore contribute, even in the absence of sulfuric acid, to new particle formation (NPF). The understanding of the autoxidation mechanism and its kinetics is still far from complete. Here, we present a mechanistic and kinetic analysis of mass spectrometry data from α-pinene (AP) ozonolysis experiments performed during the CLOUD 8 campaign at CERN. We grouped HOMs in classes according to their identified chemical composition and investigated the relative changes of these groups and their components as a function of the reagent concentration. We determined reaction rate constants for the different HOM peroxy radical reaction pathways. The accretion reaction between HOM peroxy radicals was found to be extremely fast. We developed a pseudo-mechanism for HOM formation and added it to the AP oxidation scheme of the Master Chemical Mechanism (MCM). With this extended model, the observed concentrations and trends in HOM formation were successfully simulated.
id cern-2805293
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2019
record_format invenio
spelling cern-28052932022-10-28T12:45:40Zdoi:10.1021/acsearthspacechem.9b00035http://cds.cern.ch/record/2805293engMolteni, UgoSimon, MarioHeinritzi, MartinHoyle, Christopher RBernhammer, Anne-KathrinBianchi, FedericoBreitenlechner, MartinBrilke, SophiaDias, AntónioDuplissy, JonathanFrege, CarlaGordon, HamishHeyn, ClaudiaJokinen, TuijaKürten, AndreasLehtipalo, KatrianneMakhmutov, VladimirPetäjä, TuukkaPieber, Simone MPraplan, Arnaud PSchobesberger, SiegfriedSteiner, GerhardStozhkov, YuriTomé, AntónioTröstl, JasminWagner, Andrea CWagner, RobertWilliamson, ChristinaYan, ChaoBaltensperger, UrsCurtius, JoachimDonahue, Neil MHansel, ArminKirkby, JasperKulmala, MarkkuWorsnop, Douglas RDommen, JosefFormation of Highly Oxygenated Organic Molecules from $\alpha$-Pinene Ozonolysis: Chemical Characteristics, Mechanism, and Kinetic Model DevelopmentAstrophysics and AstronomyTerpenes are emitted by vegetation, and their oxidation in the atmosphere is an important source of secondary organic aerosol (SOA). A part of this oxidation can proceed through an autoxidation process, yielding highly oxygenated organic molecules (HOMs) with low saturation vapor pressure. They can therefore contribute, even in the absence of sulfuric acid, to new particle formation (NPF). The understanding of the autoxidation mechanism and its kinetics is still far from complete. Here, we present a mechanistic and kinetic analysis of mass spectrometry data from α-pinene (AP) ozonolysis experiments performed during the CLOUD 8 campaign at CERN. We grouped HOMs in classes according to their identified chemical composition and investigated the relative changes of these groups and their components as a function of the reagent concentration. We determined reaction rate constants for the different HOM peroxy radical reaction pathways. The accretion reaction between HOM peroxy radicals was found to be extremely fast. We developed a pseudo-mechanism for HOM formation and added it to the AP oxidation scheme of the Master Chemical Mechanism (MCM). With this extended model, the observed concentrations and trends in HOM formation were successfully simulated.oai:cds.cern.ch:28052932019
spellingShingle Astrophysics and Astronomy
Molteni, Ugo
Simon, Mario
Heinritzi, Martin
Hoyle, Christopher R
Bernhammer, Anne-Kathrin
Bianchi, Federico
Breitenlechner, Martin
Brilke, Sophia
Dias, António
Duplissy, Jonathan
Frege, Carla
Gordon, Hamish
Heyn, Claudia
Jokinen, Tuija
Kürten, Andreas
Lehtipalo, Katrianne
Makhmutov, Vladimir
Petäjä, Tuukka
Pieber, Simone M
Praplan, Arnaud P
Schobesberger, Siegfried
Steiner, Gerhard
Stozhkov, Yuri
Tomé, António
Tröstl, Jasmin
Wagner, Andrea C
Wagner, Robert
Williamson, Christina
Yan, Chao
Baltensperger, Urs
Curtius, Joachim
Donahue, Neil M
Hansel, Armin
Kirkby, Jasper
Kulmala, Markku
Worsnop, Douglas R
Dommen, Josef
Formation of Highly Oxygenated Organic Molecules from $\alpha$-Pinene Ozonolysis: Chemical Characteristics, Mechanism, and Kinetic Model Development
title Formation of Highly Oxygenated Organic Molecules from $\alpha$-Pinene Ozonolysis: Chemical Characteristics, Mechanism, and Kinetic Model Development
title_full Formation of Highly Oxygenated Organic Molecules from $\alpha$-Pinene Ozonolysis: Chemical Characteristics, Mechanism, and Kinetic Model Development
title_fullStr Formation of Highly Oxygenated Organic Molecules from $\alpha$-Pinene Ozonolysis: Chemical Characteristics, Mechanism, and Kinetic Model Development
title_full_unstemmed Formation of Highly Oxygenated Organic Molecules from $\alpha$-Pinene Ozonolysis: Chemical Characteristics, Mechanism, and Kinetic Model Development
title_short Formation of Highly Oxygenated Organic Molecules from $\alpha$-Pinene Ozonolysis: Chemical Characteristics, Mechanism, and Kinetic Model Development
title_sort formation of highly oxygenated organic molecules from $\alpha$-pinene ozonolysis: chemical characteristics, mechanism, and kinetic model development
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1021/acsearthspacechem.9b00035
http://cds.cern.ch/record/2805293
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