The complexity of aerosol production from bubble bursting
Research Article
December 30, 2022
Jiang et al. (1) address the fundamental question of the origin of submicron primary sea salt aerosols by proposing the mechanism of film flapping in bubble bursting. To support that, they report detailed experimental measurements of aerosols produced by controlled-size bubble swarms. First, instead of the equivalent bubble volume radius R, Jiang et al. use the bubble cap radius (approximately twice R, for most of the relevant size range) calculated according to Toba (2). However, comparing the average number of particles <nd> produced per bubble, Jiang et al. mix their data with other works that use the equivalent radius R (ref. 1, figure 3B). The correct comparison is shown here in Fig. 1 using the Laplace number La = ρσR/μ2 (ρ, σ, and μ are the liquid density, surface tension, and viscosity).
Fig. 1.

That comparison collapses much better prior data with Jiang et al.’s (1) (see ref. 1, SI Appendix), and emphasizes the success of Jiang et al.’s proposal in explaining the puzzle of Blanchard and Syzdek (3) in the region for La > 104 where the jetting mechanism is subdominant. Two observations are as follows:
(i)
For La < 104, Jiang et al. (1) correctly state that their 73-, 137-, and 199-micron bubbles would produce daughter bubbles whose jet droplets would yield particles of 24, 52, and 83 nm, respectively. However, in contrast with the general inconsistency claimed by Jiang et al. for jet droplets, these values agree with their experimental peaks at about 35, 50, and 80 nm (ref. 1, figure 2).
(ii)
Fig. 1 shows additional published data for bubble jetting. Since Jiang et al. (1) cannot experimentally discriminate the mechanism producing their aerosols, their measurements should reproduce the number of jet droplets that others report for La < 104 (4–6). However, Jiang et al.’s values for La < 104 are at least 30 times smaller. This major experimental inconsistency suggests a possible underperformance of their scanning mobility particle sizer and aerodynamic particle sizer equipment or the inadequate measurement of bubble sizes actually bursting at the water surface. In effect, complex mechanisms involving water supersaturation with air, bubble coalescence, and daughter formation at the water surface (6–8) cannot be ruled out. Hence, the bubble size distribution actually bursting at the surface (7, 8) for their La > 104 range may contain an indeterminate but significant fraction of bubbles in the actual range La < 104.
These considerations and the latest model of ref. 9 suggest that a sparse-sized submicrometer jet droplet population should be expected along the whole bubble size range reported by Jiang et al. (1), which is, indeed, consistent with their measurements. However, they exclusively attribute their measurements to film flapping. Furthermore, given that the molecular mean free path in air at atmospheric pressure is about 143 nm, extrapolating to bubbles with R < 0.2 mm (La < 104, with a film thickness less than 10 nm), the same flapping mechanism observed at larger scales might be difficult to justify.
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Acknowledgments
This research has been supported by the Spanish Agencia Estatal de Investigación (Grant PID2019-108278RB), and by the Junta de Andalucía (Grant P18-FR-3375).
References
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X. Jiang, L. Rotily, E. Villermaux, X. Wang, Submicron drops from flapping bursting bubbles. Proc. Natl. Acad. Sci. U.S.A. 119, e2112924119 (2022).
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A. Berny, S. Popinet, T. Séon, L. Deike, Statistics of jet drop production. Geophys. Res. Lett. 48, e2021GL092919 (2021).
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Copyright © 2022 the Author(s). Published by PNAS. This article is distributed under Creative Commons Attribution-NonCommercial-NoDerivatives License 4.0 (CC BY-NC-ND).
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Published online: July 27, 2022
Published in issue: August 23, 2022
Acknowledgments
This research has been supported by the Spanish Agencia Estatal de Investigación (Grant PID2019-108278RB), and by the Junta de Andalucía (Grant P18-FR-3375).
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The complexity of aerosol production from bubble bursting, Proc. Natl. Acad. Sci. U.S.A.
119 (34) e2208770119,
https://doi.org/10.1073/pnas.2208770119
(2022).
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