Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10238
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dc.contributor.authorallSlatcher, N.; Lancaster Environment Centre, Lancaster University, Lancaster LA1 4YQ, UKen
dc.contributor.authorallJames, M.; Lancaster Environment Centre, Lancaster University, Lancaster LA1 4YQ, UKen
dc.contributor.authorallCalvari, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallGanci, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallBrowning, J.; Department of Earth Sciences, Royal Holloway, University of London, Egham TW20 0EX, UKen
dc.date.accessioned2016-02-23T13:29:13Zen
dc.date.available2016-02-23T13:29:13Zen
dc.date.issued2015-11-10en
dc.identifier.urihttp://hdl.handle.net/2122/10238en
dc.description.abstractDuring volcanic eruptions, measurements of the rate at which magma is erupted underpin hazard assessments. For eruptions dominated by the effusion of lava, estimates are often made using satellite data; here, in a case study at Mount Etna (Sicily), we make the first measurements based on terrestrial laser scanning (TLS), and we also include explosive products. During the study period (17–21 July 2012), regular Strombolian explosions were occurring within the Bocca Nuova crater, producing a ~50 m-high scoria cone and a small lava flow field. TLS surveys over multi-day intervals determined a mean cone growth rate (effusive and explosive products) of ~0.24 m3·s−1. Differences between 0.3-m resolution DEMs acquired at 10-minute intervals captured the evolution of a breakout lava flow lobe advancing at 0.01–0.03 m3·s−1. Partial occlusion within the crater prevented similar measurement of the main flow, but integrating TLS data with time-lapse imagery enabled lava viscosity (7.4 × 105 Pa·s) to be derived from surface velocities and, hence, a flux of 0.11 m3·s−1 to be calculated. Total dense rock equivalent magma discharge estimates are ~0.1–0.2 m3·s−1 over the measurement period and suggest that simultaneous estimates from satellite data are somewhat overestimated. Our results support the use of integrated TLS and time-lapse photography for ground-truthing space-based measurements and highlight the value of interactive image analysis when automated approaches, such as particle image velocimetry (PIV), fail.en
dc.language.isoEnglishen
dc.publisher.nameMolecular Diversity Preservation Internationalen
dc.relation.ispartofRemote Sensingen
dc.relation.ispartofseries/7(2015)en
dc.subjectlava flow; scoria cone; effusion rate; terrestrial laser scanning; time-lapse photography; Mt. Etnaen
dc.titleQuantifying Effusion Rates at Active Volcanoes through Integrated Time-Lapse Laser Scanning and Photographyen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber14967 - 14987en
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoringen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.07. Instruments and techniquesen
dc.subject.INGV05. General::05.02. Data dissemination::05.02.03. Volcanic eruptionsen
dc.identifier.doi10.3390/rs71114967en
dc.description.obiettivoSpecifico3V. Dinamiche e scenari eruttivien
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.relation.issn2072-4292en
dc.contributor.authorSlatcher, N.en
dc.contributor.authorJames, M.en
dc.contributor.authorCalvari, S.en
dc.contributor.authorGanci, G.en
dc.contributor.authorBrowning, J.en
dc.contributor.departmentLancaster Environment Centre, Lancaster University, Lancaster LA1 4YQ, UKen
dc.contributor.departmentLancaster Environment Centre, Lancaster University, Lancaster LA1 4YQ, UKen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentDepartment of Earth Sciences, Royal Holloway, University of London, Egham TW20 0EX, UKen
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, 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.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptDepartment of Earth Sciences, Royal Holloway, University of London, Egham TW20 0EX, UK-
crisitem.author.orcid0000-0001-8189-5499-
crisitem.author.orcid0000-0002-9914-1107-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent05. General-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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