Effect of relative humidity on the molecular composition of secondary organic aerosols from α-pinene ozonolysis
Secondary organic aerosols (SOAs) originating from the oxidation of biogenic volatile organic compounds such as monoterpenes by atmospheric oxidants ( e.g. OH, ozone, and NO 3 ), constitute a widespread source of organic aerosols in the atmosphere. Among monoterpenes, α-pinene has the highest emissi...
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Published in | Environmental science: atmospheres Vol. 4; no. 5; pp. 519 - 53 |
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Main Authors | , , , , , |
Format | Journal Article |
Language | English |
Published |
16.05.2024
|
Online Access | Get full text |
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Summary: | Secondary organic aerosols (SOAs) originating from the oxidation of biogenic volatile organic compounds such as monoterpenes by atmospheric oxidants (
e.g.
OH, ozone, and NO
3
), constitute a widespread source of organic aerosols in the atmosphere. Among monoterpenes, α-pinene has the highest emission rates and its ozonolysis is often used as a canonical SOA system. However, the molecular composition of SOAs obtained from monoterpene ozonolysis as a function of relative humidity (RH) remains unclear. Herein, we investigated the real-time molecular composition of SOAs obtained from the ozonolysis of α-pinene using extractive electrospray ionization coupled with long time-of-flight mass spectrometry (EESI-LTOF-MS). We investigated the dependence of the molecular composition on RH in the presence and absence of seed aerosols. We characterized a large number of organic compounds, including less oxygenated and highly oxygenated organic molecules (HOMs). In the presence of a ammonium sulfate (AS) seed aerosol, the fractions of both monomers and dimers in the SOAs from α-pinene ozonolysis remained largely unchanged as RH increased from 3% to 84%, which can be attributed to a similar extent of increase in the absolute abundance of both dimers and monomers with increasing RH. The increase of the absolute abundance of monomers is likely due to the enhanced partitioning of less oxygenated semi-volatile monomer products (such as C
10
H
16
O
x
≤6
) at higher RH. The increase in the absolute abundance of dimers may be attributed to acid-catalyzed reactions, which is corroborated by a marked change in the distribution pattern of dimers. The average O/C of the most abundant product families in the SOAs, such as C
10
H
16
O
x
, decreased with increasing RH due to the decreasing fractions of more oxygenated products (C
10
H
16
O
x
>6
). However, the elemental composition (O/C and H/C) of the total SOA remained stable with increasing RH. In contrast, in the absence of the seed aerosol, an increase in the monomer fraction and a decrease in the dimer fraction were observed with increasing RH. These changes were attributed to a combination of different extents of condensation enhancement of monomer and dimer vapors by increasing RH and different vapor wall losses of monomers and dimers. Our results provide new insights into the RH-dependent molecular chemical composition of α-pinene SOAs. We also highlight the necessity to characterize the composition of SOAs at the molecular level.
Secondary organic aerosols (SOAs) originating from the oxidation of biogenic volatile organic compounds such as monoterpenes by atmospheric oxidants (
e.g.
OH, ozone, and NO
3
), constitute a widespread source of organic aerosols in the atmosphere. |
---|---|
Bibliography: | v,w C τ 16 and dimers (C 28 Electronic supplementary information (ESI) available: Details of the experimental conditions; the molecular formula of the SOA products; the absolute abundance of monomer (C H 19 17-20 https://doi.org/10.1039/d3ea00149k O and C in the absence of seed aerosol. See DOI average molecule weight, O/C, and H/C; the estimated vapor-particle at 91% RH and 28% RH in the absence of AS seed aerosol; the absolute abundance of C x and vapor-wall equilibration timescale 9 v,p and total products; the fraction of C 10 the absolute abundance of C monomers with different O/C ratios; average oxygen number of monomer families under different RH; the abundance ratio of C |
ISSN: | 2634-3606 2634-3606 |
DOI: | 10.1039/d3ea00149k |