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Dependence of SOA oxidation on organic aerosol mass concentration and OH exposure: experimental PAM chamber studies

Item

Title (Dublin Core)

Dependence of SOA oxidation on organic aerosol mass concentration and OH exposure: experimental PAM chamber studies

Description (Dublin Core)

The oxidation of secondary organic aerosol (SOA) is studied with mass spectra analysis of SOA formed in a Potential Aerosol Mass (PAM) chamber, a small flow-through photo-oxidation chamber with extremely high OH and ozone levels. The OH exposure from a few minutes in the PAM chamber is similar to that from days to weeks in the atmosphere. The mass spectra were measured with a Quadrupole Aerosol Mass Spectrometer (Q-AMS) for SOA formed from oxidation of α-pinene, <i>m</i>-xylene, <i>p</i>-xylene, and a mixture of the three. The organic mass fractions of <i>m/z</i> 44 (CO<sub>2</sub><sup>+</sup>) and <i>m/z</i> 43 (mainly C<sub>2</sub>H<sub>3</sub>O<sup>+</sup>), named <i>f</i><sub>44</sub> and <i>f</i><sub>43</sub> respectively, are used as indicators of the degree of organic aerosol (OA) oxidation that occurs as the OA mass concentration or the OH exposure are varied. The degree of oxidation is sensitive to both. For a fixed OH exposure, the degree of oxidation initially decreases rapidly and then more slowly as the OA mass concentration increases. For fixed initial precursor VOC amounts, the degree of oxidation increases linearly with OH exposure, with <i>f</i><sub>44</sub> increasing and <i>f</i><sub>43</sub> decreasing. In this study, the degree of SOA oxidation spans much of the range observed in the atmosphere. These results, while sensitive to the determination of <i>f</i><sub>44</sub> and <i>f</i><sub>43</sub>, provide evidence that some characteristics of atmospheric OA oxidation can be generated in a PAM chamber. For all measurements in this study, the sum of <i>f</i><sub>44</sub> and <i>f</i><sub>43</sub> is 0.25 ± 0.03, so that the slope of a linear regression is approximately &minus;1 on an <i>f</i><sub>44</sub> vs. <i>f</i><sub>43</sub> plot. This constancy of the sum suggests that these ions are complete proxies for organic mass in the OA studied.

Creator (Dublin Core)

Kang, E.
Toohey, D. W.
Brune, W. H.

Date (Dublin Core)

2018-01-15

Type (Dublin Core)

Text

Format (Dublin Core)

application/pdf

Identifier (Dublin Core)

10.5194/acp-11-1837-2011
https://acp.copernicus.org/articles/11/1837/2011/

Source (Dublin Core)

eISSN: 1680-7324

Language (Dublin Core)

eng
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