Simulation of a Large Wildfire in a Coupled Fire-Atmosphere Model

The Aullene fire devastated more than 3000 ha of Mediterranean maquis and pine forest in July 2009. The simulation of combustion processes, as well as atmospheric dynamics represents a challenge for such scenarios because of the various involved scales, from the scale of the individual flames to the...

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Main Authors: Jean-Baptiste Filippi, Frédéric Bosseur, Céline Mari, Christine Lac
Format: Article
Language:English
Published: MDPI AG 2018-06-01
Series:Atmosphere
Subjects:
Online Access:http://www.mdpi.com/2073-4433/9/6/218
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author Jean-Baptiste Filippi
Frédéric Bosseur
Céline Mari
Christine Lac
author_facet Jean-Baptiste Filippi
Frédéric Bosseur
Céline Mari
Christine Lac
author_sort Jean-Baptiste Filippi
collection DOAJ
description The Aullene fire devastated more than 3000 ha of Mediterranean maquis and pine forest in July 2009. The simulation of combustion processes, as well as atmospheric dynamics represents a challenge for such scenarios because of the various involved scales, from the scale of the individual flames to the larger regional scale. A coupled approach between the Meso-NH (Meso-scale Non-Hydrostatic) atmospheric model running in LES (Large Eddy Simulation) mode and the ForeFire fire spread model is proposed for predicting fine- to large-scale effects of this extreme wildfire, showing that such simulation is possible in a reasonable time using current supercomputers. The coupling involves the surface wind to drive the fire, while heat from combustion and water vapor fluxes are injected into the atmosphere at each atmospheric time step. To be representative of the phenomenon, a sub-meter resolution was used for the simulation of the fire front, while atmospheric simulations were performed with nested grids from 2400-m to 50-m resolution. Simulations were run with or without feedback from the fire to the atmospheric model, or without coupling from the atmosphere to the fire. In the two-way mode, the burnt area was reproduced with a good degree of realism at the local scale, where an acceleration in the valley wind and over sloping terrain pushed the fire line to locations in accordance with fire passing point observations. At the regional scale, the simulated fire plume compares well with the satellite image. The study explores the strong fire-atmosphere interactions leading to intense convective updrafts extending above the boundary layer, significant downdrafts behind the fire line in the upper plume, and horizontal wind speeds feeding strong inflow into the base of the convective updrafts. The fire-induced dynamics is induced by strong near-surface sensible heat fluxes reaching maximum values of 240 kW m − 2 . The dynamical production of turbulent kinetic energy in the plume fire is larger in magnitude than the buoyancy contribution, partly due to the sheared initial environment, which promotes larger shear generation and to the shear induced by the updraft itself. The turbulence associated with the fire front is characterized by a quasi-isotropic behavior. The most active part of the Aullene fire lasted 10 h, while 9 h of computation time were required for the 24 million grid points on 900 computer cores.
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spelling doaj.art-3f14b8228916432cac8b5e5ecf4b33bd2022-12-21T23:32:16ZengMDPI AGAtmosphere2073-44332018-06-019621810.3390/atmos9060218atmos9060218Simulation of a Large Wildfire in a Coupled Fire-Atmosphere ModelJean-Baptiste Filippi0Frédéric Bosseur1Céline Mari2Christine Lac3SPE—Sciences Pour l’Environnement, Université de Corse, CNRS, Campus Grimaldi, 20250 Corte, FranceSPE—Sciences Pour l’Environnement, Université de Corse, CNRS, Campus Grimaldi, 20250 Corte, FranceLA—Laboratoire D’Aérologie, Université de Toulouse, CNRS, UPS, 14 Avenue Edouard Belin, 31400 Toulouse, FranceCNRM—Centre National de Recherches Météorologiques, Météo-France, CNRS, 42 Avenue Coriolis, 31057 Toulouse, FranceThe Aullene fire devastated more than 3000 ha of Mediterranean maquis and pine forest in July 2009. The simulation of combustion processes, as well as atmospheric dynamics represents a challenge for such scenarios because of the various involved scales, from the scale of the individual flames to the larger regional scale. A coupled approach between the Meso-NH (Meso-scale Non-Hydrostatic) atmospheric model running in LES (Large Eddy Simulation) mode and the ForeFire fire spread model is proposed for predicting fine- to large-scale effects of this extreme wildfire, showing that such simulation is possible in a reasonable time using current supercomputers. The coupling involves the surface wind to drive the fire, while heat from combustion and water vapor fluxes are injected into the atmosphere at each atmospheric time step. To be representative of the phenomenon, a sub-meter resolution was used for the simulation of the fire front, while atmospheric simulations were performed with nested grids from 2400-m to 50-m resolution. Simulations were run with or without feedback from the fire to the atmospheric model, or without coupling from the atmosphere to the fire. In the two-way mode, the burnt area was reproduced with a good degree of realism at the local scale, where an acceleration in the valley wind and over sloping terrain pushed the fire line to locations in accordance with fire passing point observations. At the regional scale, the simulated fire plume compares well with the satellite image. The study explores the strong fire-atmosphere interactions leading to intense convective updrafts extending above the boundary layer, significant downdrafts behind the fire line in the upper plume, and horizontal wind speeds feeding strong inflow into the base of the convective updrafts. The fire-induced dynamics is induced by strong near-surface sensible heat fluxes reaching maximum values of 240 kW m − 2 . The dynamical production of turbulent kinetic energy in the plume fire is larger in magnitude than the buoyancy contribution, partly due to the sheared initial environment, which promotes larger shear generation and to the shear induced by the updraft itself. The turbulence associated with the fire front is characterized by a quasi-isotropic behavior. The most active part of the Aullene fire lasted 10 h, while 9 h of computation time were required for the 24 million grid points on 900 computer cores.http://www.mdpi.com/2073-4433/9/6/218wildland firemesoscale atmospheric modelcoupling
spellingShingle Jean-Baptiste Filippi
Frédéric Bosseur
Céline Mari
Christine Lac
Simulation of a Large Wildfire in a Coupled Fire-Atmosphere Model
Atmosphere
wildland fire
mesoscale atmospheric model
coupling
title Simulation of a Large Wildfire in a Coupled Fire-Atmosphere Model
title_full Simulation of a Large Wildfire in a Coupled Fire-Atmosphere Model
title_fullStr Simulation of a Large Wildfire in a Coupled Fire-Atmosphere Model
title_full_unstemmed Simulation of a Large Wildfire in a Coupled Fire-Atmosphere Model
title_short Simulation of a Large Wildfire in a Coupled Fire-Atmosphere Model
title_sort simulation of a large wildfire in a coupled fire atmosphere model
topic wildland fire
mesoscale atmospheric model
coupling
url http://www.mdpi.com/2073-4433/9/6/218
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