Please use this identifier to cite or link to this item:
|Authors: ||Cappello, A.*|
Del Negro, C.*
|Title: ||MAGFLOW: a physics-based model for the dynamics of lava-flow emplacement|
|Issue Date: ||30-Jul-2015|
|Keywords: ||lava flow hazard|
|Abstract: ||The MAGFLOW model for lava-flow simulations is based on the cellular automaton (CA) approach, and uses a physical model for the thermal and rheological evolution of the flowing lava. We discuss the potential of MAGFLOW to improve our understanding of the dynamics of lava-flow emplacement and our ability to assess lava-flow hazards. Sensitivity analysis of the input parameters controlling the evolution function of the automaton demonstrates that water content and solidus temperatures are the parameters to which MAGFLOW is most sensitive.
Additional tests also indicate that temporal changes in effusion rate strongly influence the accuracy of the predictive modelling of lava-flow paths. The parallel implementation of MAGFLOW on graphic processing units (GPUs) can achieve speed-ups of two orders of magnitude relative to the corresponding serial implementation, providing a lava-flow simulation spanning several
days of eruption in just a few minutes. We describe and demonstrate the operation of MAGFLOW using two case studies from Mt Etna: one is a reconstruction of the detailed chronology of the lava-flow emplacement during the 2006 flank eruption; and the other is the production of the lava-flow hazard map of the persistent eruptive activity at the summit craters.|
|Appears in Collections:||Book chapters|
05.02.03. Volcanic eruptions
Files in This Item:
|2015 Geological Society, London, Special Publications-2015-Cappello-SP426.16.pdf||4.14 MB||Adobe PDF||only authorized users
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.