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dc.contributor.authorChristopher, TE
dc.contributor.authorBlundy, J
dc.contributor.authorCashman, K
dc.contributor.authorCole, P
dc.contributor.authorEdmonds, M
dc.contributor.authorSmith, PJ
dc.contributor.authorSparks, RSJ
dc.contributor.authorStinton, A
dc.date.accessioned2017-02-13T14:31:03Z
dc.date.available2017-02-13T14:31:03Z
dc.date.issued2015-09
dc.identifier.issn1525-2027
dc.identifier.issn1525-2027
dc.identifier.urihttp://hdl.handle.net/10026.1/8459
dc.description.abstract

<jats:title>Abstract</jats:title><jats:p>Activity since 1995 at Soufrière Hills Volcano (SHV), Montserrat has alternated between andesite lava extrusion and quiescence, which are well correlated with seismicity and ground deformation cycles. Large variations in SO<jats:sub>2</jats:sub> flux do not correlate with these alternations, but high and low HCl/SO<jats:sub>2</jats:sub> characterize lava dome extrusion and quiescent periods respectively. Since lava extrusion ceased (February 2010) steady SO<jats:sub>2</jats:sub> emissions have continued at an average rate of 374 tonnes/day (± 140 t/d), and incandescent fumaroles (temperatures up to 610<jats:sup>o</jats:sup>C) on the dome have not changed position or cooled. Occasional short bursts (over several hours) of higher (∼ 10x) SO<jats:sub>2</jats:sub> flux have been accompanied by swarms of volcano‐tectonic earthquakes. Strain data from these bursts indicate activation of the magma system to depths up to 10 km. SO<jats:sub>2</jats:sub> emissions since 1995 greatly exceed the amounts that could be derived from 1.1 km<jats:sup>3</jats:sup> of erupted andesite, and indicating extensive partitioning of sulfur into a vapour phase, as well as efficient decoupling and outgassing of sulfur‐rich gases from the magma. These observations are consistent with a vertically extensive, crustal magmatic mush beneath SHV. Three states of the magmatic system are postulated to control degassing. During dormant periods (10<jats:sup>3</jats:sup> to 10<jats:sup>4</jats:sup> years) magmatic vapour and melts separate as layers from the mush and decouple from each other. In periods of unrest (years) without eruption, melt and fluid layers become unstable, ascend and can amalgamate. Major destabilization of the mush system leads to eruption, characterized by magma mixing and release of volatiles with different ages, compositions and sources.</jats:p>

dc.format.extent2797-2811
dc.languageen
dc.language.isoen
dc.publisherAmerican Geophysical Union (AGU)
dc.subject37 Earth Sciences
dc.subject3703 Geochemistry
dc.subject3705 Geology
dc.subject3706 Geophysics
dc.titleCrustal‐scale degassing due to magma system destabilization and magma‐gas decoupling at <scp>S</scp>oufrière <scp>H</scp>ills <scp>V</scp>olcano, <scp>M</scp>ontserrat
dc.typejournal-article
dc.typeArticle
plymouth.author-urlhttps://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000365039400001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=11bb513d99f797142bcfeffcc58ea008
plymouth.issue9
plymouth.volume16
plymouth.publication-statusPublished
plymouth.journalGeochemistry, Geophysics, Geosystems
dc.identifier.doi10.1002/2015gc005791
plymouth.organisational-group/Plymouth
plymouth.organisational-group/Plymouth/Faculty of Science and Engineering
plymouth.organisational-group/Plymouth/Faculty of Science and Engineering/School of Geography, Earth and Environmental Sciences
plymouth.organisational-group/Plymouth/REF 2021 Researchers by UoA
plymouth.organisational-group/Plymouth/REF 2021 Researchers by UoA/UoA07 Earth Systems and Environmental Sciences
plymouth.organisational-group/Plymouth/Users by role
plymouth.organisational-group/Plymouth/Users by role/Academics
dc.identifier.eissn1525-2027
dc.rights.embargoperiodNot known
rioxxterms.versionofrecord10.1002/2015gc005791
rioxxterms.licenseref.urihttp://www.rioxx.net/licenses/all-rights-reserved
rioxxterms.typeJournal Article/Review


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