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  5. A review of mass and energy flow through a lava flow system: Insights provided from a non-equilibrium perspective
 
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A review of mass and energy flow through a lava flow system: Insights provided from a non-equilibrium perspective

Author(s)
Tarquini, Simone  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Pisa, Pisa, Italia  
Language
English
Obiettivo Specifico
5V. Dinamica dei processi eruttivi e post-eruttivi
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Journal
Bulletin of Volcanology  
Issue/vol(year)
/79 (2017)
Pages (printed)
64
Date Issued
August 2017
DOI
10.1007/s00445-017-1145-5
URI
https://www.earth-prints.org/handle/2122/11698
Subjects

lava flows

thermal proxy

heat balance

lava flow morphology

lava flow emplacement...

Abstract
A 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.
Type
article
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Tarquini_BV_2017_review.pdf

Size

2.5 MB

Format

Adobe PDF

Checksum (MD5)

36d33d61c434687a6b3da70821b69064

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