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dc.contributor.authorKoenig, A.M.
dc.contributor.authorMagand, O.
dc.contributor.authorRose, C.
dc.contributor.authorDi Muro, A.
dc.contributor.authorMiyazaki, Y.
dc.contributor.authorColomb, A.
dc.contributor.authorRissanen, M.
dc.contributor.authorLee, C.F.
dc.contributor.authorKoenig, T.K.
dc.contributor.authorVolkamer, R.
dc.contributor.authorBrioude, J.
dc.contributor.authorVerreyken, B.
dc.contributor.authorRoberts, T.
dc.contributor.authorEdwards, B.A.
dc.contributor.authorSellegri, K.
dc.contributor.authorArellano, S.
dc.contributor.authorKowalski, P.
dc.contributor.authorAiuppa, A.
dc.contributor.authorSonke, J.E.
dc.contributor.authorDommergue, A.
dc.date2023
dc.date.accessioned2023-10-16T08:48:37Z
dc.date.available2023-10-16T08:48:37Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/11158
dc.descriptionTerrestrial volcanism is known to emit mercury (Hg) into the atmosphere. However, despite many years of investigation, its net impact on the atmospheric Hg budget remains insufficiently constrained, in part because the transformations of Hg in volcanic plumes as they age and mix with background air are poorly understood. Here we report the observation of complete gaseous elemental mercury (GEM) depletion events in dilute and moderately aged (∼3–7 hours) volcanic plumes from Piton de la Fournaise on Réunion Island. While it has been suggested that co-emitted bromine could, once photochemically activated, deplete GEM in a volcanic plume, we measured low bromine concentrations in both the gas- and particle-phase and observed complete GEM depletion even before sunrise, ruling out a leading role of bromine chemistry here. Instead, we hypothesize that the GEM depletions were mainly caused by gas–particle interactions with sulfate-rich volcanic particles (mostly of submicron size), abundantly present in the dilute plume. We consider heterogeneous GEM oxidation and GEM uptake by particles as plausible manifestations of such a process and derive empirical rate constants. By extrapolation, we estimate that volcanic aerosols may scavenge 210 Mg y−1 (67–480 Mg y−1) of Hg from the atmosphere globally, acting effectively as atmospheric mercury sink. While this estimate is subject to large uncertainties, it highlights that Hg transformations in aging volcanic plumes must be better understood to determine the net impact of volcanism on the atmospheric Hg budget and Hg deposition pathways.
dc.languageeng
dc.titleObserved in-plume gaseous elemental mercury depletion suggests significant mercury scavenging by volcanic aerosols
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.source.titleEnvironmental Science: Atmospheres
dc.source.volume3
dc.source.issue10
dc.source.page1418-1438
Orfeo.peerreviewedYes
dc.identifier.doi10.1039/D3EA00063J
dc.identifier.url


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