Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/5997
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dc.contributor.authorallApplegarth, L. J.; Lancaster Environment Centre, Lancaster University, Bailrigg, Lancasteren
dc.contributor.authorallPinkerton, H.; Lancaster Environment Centre, Lancaster University, Bailrigg, Lancasteren
dc.contributor.authorallJames, M. R.; Lancaster Environment Centre, Lancaster University, Bailrigg, Lancasteren
dc.contributor.authorallCalvari, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.date.accessioned2010-05-14T06:42:33Zen
dc.date.available2010-05-14T06:42:33Zen
dc.date.issued2010-05-10en
dc.identifier.urihttp://hdl.handle.net/2122/5997en
dc.description.abstractBasaltic 'a'ā lava flows often demonstrate compound morphology, consisting of many juxtaposed and superposed flow units. Following observations made during the 2001 eruption of Mt. Etna, Sicily, we examine the processes that can result from the superposition of flow units, when the underlying units are sufficiently young to have immature crusts and deformable cores. During this eruption, we observed that the emplacement of new surface flow units may reactivate older, underlying units by squeezing the still-hot flow core away from the site of loading. Here, we illustrate three different styles of reactivation that depend on the time elapsed between the emplacement of the two flow units, hence the rheological contrast between them. For relatively long time intervals (2 to 15 days), and consequently significant rheological contrasts, superposition can pressurise the underlying flow unit, leading to crustal rupture and the subsequent extrusion of a small volume of high yield strength lava. Following shorter intervals (1 to 2 days), the increased pressure caused by superposition can result in renewed, slow advance of the underlying immature flow unit front. On timescales of < 1 day, where there is little rheological contrast between the two units, the thin intervening crust can be disrupted during superposition, allowing mixing of the flow cores, large-scale reactivation of both units, and widespread channel drainage. This mechanism may explain the presence of drained channels in flows that are known to have been cooling-limited, contrary to the usual interpretation of drainage as an indicator of volume-limited behaviour. Because the remobilisation of previously stagnant lava can occur swiftly and unexpectedly, it may pose a significant hazard during the emplacement of compound flows. Constant monitoring of flow development to identify areas where superposition is occurring is therefore recommended, as this may allow potentially hazardous rapid drainage events to be forecast. Reactivation processes should also be borne in mind when reconstructing the emplacement of old lava flow fields, as failure to recognise their effects may result in the misinterpretation of features such as drained channels.en
dc.description.sponsorshipThe work was funded by NERC studentship NER/S/A2005/13681 and grant NE/F018010/1.en
dc.language.isoEnglishen
dc.publisher.nameElsevieren
dc.relation.ispartofJournal of Volcanology and Geothermal Researchen
dc.relation.ispartofseries4/194 (2010)en
dc.subjectEtnaen
dc.subjectflow uniten
dc.subjectcompound flowen
dc.subjectsuperpositionen
dc.titleLava flow superposition: The reactivation of flow units in compound ’a’a flowsen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.08. Volcanic risken
dc.identifier.doi10.1016/j.jvolgeores.2010.05.001en
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dc.description.obiettivoSpecifico1.5. TTC - Sorveglianza dell'attività eruttiva dei vulcanien
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorApplegarth, L. J.en
dc.contributor.authorPinkerton, H.en
dc.contributor.authorJames, M. R.en
dc.contributor.authorCalvari, S.en
dc.contributor.departmentLancaster Environment Centre, Lancaster University, Bailrigg, Lancasteren
dc.contributor.departmentLancaster Environment Centre, Lancaster University, Bailrigg, Lancasteren
dc.contributor.departmentLancaster Environment Centre, Lancaster University, Bailrigg, Lancasteren
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptLancaster Environment Centre, Lancaster University, Bailrigg, Lancaste-
crisitem.author.deptEnvironmental Science Department, Institute of Environmental and Natural Sciences, Lancaster University, Lancaster LA1 4YQ, UK-
crisitem.author.deptEnvironmental Science Department, Institute of Environmental and Natural Sciences, Lancaster University, Lancaster, United Kingdom-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.orcid0000-0001-8189-5499-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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