Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/11698
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dc.date.accessioned2018-04-16T09:31:37Zen
dc.date.available2018-04-16T09:31:37Zen
dc.date.issued2017-08en
dc.identifier.urihttp://hdl.handle.net/2122/11698en
dc.description.abstractA simple formula relates lava discharge rate to the heat radiated per unit time from the surface of active lava flows (the “thermal proxy”). Although widely used, the physical basis of this proxy is still debated. In the present contribution, lava flows are approached as open, dissipative systems that, under favorable conditions, can attain a non-equilibrium stationary state. In this systems framework, the onset, growth and demise of lava flow units can be explained as a self-organization phenomenon characterized by a given temporal frequency defined by the average life span of active lava flow units. Here, I review empirical, physical, and experimental models designed to understand and link the flow of mass and energy through a lava flow system, as well as measurements and observations that support a “real world” view. I set up two systems: active lava flow system (or ALFS) for flowing, fluid lava and a lava deposit system for solidified, cooling lava. The review highlights surprising similarities between lava flows and electric currents, which typically work under stationary conditions. An electric current propagates almost instantaneously through an existing circuit, following the Kirchhoff law (a least dissipation principle). Flowing lavas, in contrast, build up a slow-motion “lava-circuit” over days, weeks or months by following a gravity-driven path down the steepest slopes. Attainment of a steady-state condition is hampered (and the classic thermal proxy does not hold) if the supply stops before completion of the “lava-circuit”. Although gravity determines initial flow path and extension, the least dissipation principle means that subsequent evolution of mature portions of the active lava flow system is controlled by increasingly insulated conditions.en
dc.language.isoEnglishen
dc.relation.ispartofBulletin of Volcanologyen
dc.relation.ispartofseries/79 (2017)en
dc.subjectlava flowsen
dc.subjectthermal proxyen
dc.subjectheat balanceen
dc.subjectlava flow morphologyen
dc.subjectlava flow emplacementen
dc.titleA review of mass and energy flow through a lava flow system: Insights provided from a non-equilibrium perspectiveen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber64en
dc.identifier.doi10.1007/s00445-017-1145-5en
dc.description.obiettivoSpecifico5V. Dinamica dei processi eruttivi e post-eruttivien
dc.description.journalTypeJCR Journalen
dc.contributor.authorTarquini, Simoneen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Pisa, Pisa, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Pisa, Pisa, Italia-
crisitem.author.orcid0000-0002-8064-621X-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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