Mercury emissions from volcanic sources in Central America

dc.contributor.authorKushner, David Skye
dc.contributor.examiningcommitteePapakyriakou, Tim (Environment and Geography)en_US
dc.contributor.examiningcommitteeOutridge, Peter (Environment and Geography)en_US
dc.contributor.examiningcommitteeHalden, Norman (Geological Sciences)en_US
dc.contributor.supervisorWang, Feiyue (Environment and Geography)en_US
dc.date.accessioned2019-03-18T16:16:37Z
dc.date.available2019-03-18T16:16:37Z
dc.date.issued2019-02-26en_US
dc.date.submitted2019-02-26T22:32:19Zen
dc.date.submitted2019-03-15T21:48:17Zen
dc.degree.disciplineEnvironment and Geographyen_US
dc.degree.levelMaster of Science (M.Sc.)en_US
dc.description.abstractVolcanoes are recognized contributors of mercury (Hg) emissions to the atmosphere; however, the amount of Hg released globally from these natural sources remains poorly constrained. To improve this understanding, a multi-year suite of atmospheric, water, and ash samples were collected from Poás and Turrialba volcanoes, Costa Rica. Atmospheric sampling at Poás was conducted over two stages of volcanic activity (passive degassing and active eruption) using continuous monitoring near the crater in addition to passive and active sampling techniques within the crater. Results corroborate earlier assessments that Poás is a low Hg emitting volcano compared to Turrialba, even during active phases. A novel model of crustal Hg incorporation is proposed to explain the large global variance in volcanic plume Hg concentrations in relationship to eruption frequency. Based on the model, a new global volcanic Hg flux is estimated to be 30 ± 39 t/a for 2006‒2015.en_US
dc.description.noteMay 2019en_US
dc.identifier.urihttp://hdl.handle.net/1993/33787
dc.language.isoengen_US
dc.subjectMercury
dc.subjectContaminants
dc.subjectCosta Rica
dc.subjectVolcanology
dc.titleMercury emissions from volcanic sources in Central Americaen_US
dc.typemaster thesisen_US

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