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Molecular understanding of new-particle formation from alpha-pinene between −50 °C and 25 °C

Authors :
Mario Simon
Lubna Dada
Martin Heinritzi
Wiebke Scholz
Dominik Stolzenburg
Lukas Fischer
Andrea C. Wagner
Andreas Kürten
Birte Rörup
Xu-Cheng He
João Almeida
Rima Baalbaki
Andrea Baccarini
Paulus S. Bauer
Lisa Beck
Anton Bergen
Federico Bianchi
Steffen Bräkling
Sophia Brilke
Lucia Caudillo
Dexian Chen
Biwu Chu
António Dias
Danielle C. Draper
Jonathan Duplissy
Imad El Haddad
Henning Finkenzeller
Carla Frege
Loic Gonzalez-Carracedo
Hamish Gordon
Manuel Granzin
Jani Hakala
Victoria Hofbauer
Christopher R. Hoyle
Changhyuk Kim
Weimeng Kong
Houssni Lamkaddam
Chuan P. Lee
Katrianne Lehtipalo
Markus Leiminger
Huajun Mai
Hanna E. Manninen
Guillaume Marie
Ruby Marten
Bernhard Mentler
Ugo Molteni
Leonid Nichman
Wei Nie
Andrea Ojdanic
Antti Onnela
Eva Partoll
Tuukka Petäjä
Joschka Pfeifer
Maxim Philippov
Lauriane L. J. Quéléver
Ananth Ranjithkumar
Matti Rissanen
Simon Schallhart
Siegfried Schobesberger
Simone Schuchmann
Jiali Shen
Mikko Sipilä
Gerhard Steiner
Yuri Stozhkov
Christian Tauber
Yee J. Tham
António R. Tomé
Miguel Vazquez-Pufleau
Alexander Vogel
Robert Wagner
Mingyi Wang
Dongyu S. Wang
Yonghong Wang
Stefan K. Weber
Yusheng Wu
Mao Xiao
Chao Yan
Penglin Ye
Qing Ye
Marcel Zauner-Wieczorek
Xueqin Zhou
Urs Baltensperger
Josef Dommen
Rick C. Flagan
Armin Hansel
Markku Kulmala
Rainer Volkamer
Paul M. Winkler
Douglas R. Worsnop
Neil M. Donahue
Jasper Kirkby
Joachim Curtius
Publication Year :
2020
Publisher :
Copernicus GmbH, 2020.

Abstract

Highly-oxygenated organic molecules (HOMs) contribute substantially to the formation and growth of atmospheric aerosol particles, which affect air quality, human health and Earth's climate. HOMs are formed by rapid, gas-phase autoxidation of volatile organic compounds (VOCs) such as α-pinene, the most abundant monoterpene in the atmosphere. Due to their abundance and low volatility, HOMs can play an important role for new-particle formation (NPF) and the early growth of atmospheric aerosols, even without any further assistance of other low-volatility compounds such as sulfuric acid. Both the autoxidation reaction forming HOMs and their new-particle formation rates are expected to be strongly dependent on temperature. However, experimental data on both effects are limited. Dedicated experiments were performed at the CLOUD (Cosmics Leaving OUtdoor Droplets) chamber at CERN to address this question. In this study, we show that a decrease in temperature (from +25 to −50 °C) results in a reduced HOM yield and reduced oxidation state of the products, whereas the new-particle formation rates (J1.7 nm) increase substantially. Measurements with two different chemical ionization mass spectrometers (using nitrate and protonated water as reagent ion, respectively) provide the molecular composition of the gaseous oxidation products and a 2-dimensional volatility basis set model (2D-VBS) provides their volatility distribution. The HOM yield decreases with temperature from 6.2 % at 25 °C to 0.7 % at −50 °C. However, there is a strong reduction of the saturation vapor pressure of each oxidation state as the temperature is reduced. Overall, the reduction in volatility with temperature leads to an increase in the nucleation rates by up to three orders of magnitude at −50 °C compared with 25 °C. In addition, the enhancement of the nucleation rates by ions decreases with decreasing temperature, since the neutral molecular clusters have increased stability against evaporation. The resulting data quantify how the interplay between the temperature-dependent oxidation pathways and the associated vapor pressures affect biogenic new-particle formation at the molecular level. Our measurements therefore improve our understanding of pure biogenic new-particle formation for a wide range of tropospheric temperatures and precursor concentrations.

Details

Database :
OpenAIRE
Accession number :
edsair.doi...........8acf413ea7e446402d8d76d7f59e2207
Full Text :
https://doi.org/10.5194/acp-2019-1058