Real-time probabilistic assessment of volcanic hazard for tephra dispersal and fallout at Mt. Etna: the 2021 lava fountain episodes

被引:0
作者
Federica Pardini
Mattia de’ Michieli Vitturi
Daniele Andronico
Tomaso Esposti Ongaro
Antonino Cristaldi
Augusto Neri
机构
[1] Istituto Nazionale di Geofisica e Vulcanologia - Sezione di Pisa,Department of Geology
[2] University at Buffalo,undefined
[3] Istituto Nazionale di Geofisica e Vulcanologia-Osservatorio Etneo,undefined
[4] Sezione di Catania,undefined
来源
Bulletin of Volcanology | / 85卷
关键词
Mt. Etna; Paroxysmal episodes; Volcanic hazard assessment; VONA; Numerical modelling; HYSPLIT; PLUME-MoM-TSM;
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摘要
Starting from February 2021, Mt. Etna (Italy) experienced a period of intense explosive activity with 17 lava fountain episodes between 16 February and 1 April 2021. During the eruptive cycle, the Istituto Nazionale di Geofisica e Vulcanologia-Osservatorio Etneo (INGV-OE) issued 62 alert notifications known as VONAs (Volcano Observatory Notice for Aviation) to inform the aeronautical authorities about the volcanic activity. We present an automated VONA-based workflow aimed at real-time assessment of the volcanic hazard due to tephra fallout at Mt. Etna. When a VONA reporting tephra emission is issued by INGV-OE, numerical simulations accounting for atmospheric and eruptive uncertainties are automatically initialized to produce probabilistic hazard maps of tephra fallout and atmospheric dispersal. We applied the workflow to three lava fountains that occurred during the 2021 eruptive cycle. To test the modelling results, we compared the simulated ground load with field data, and the extent and position of the simulated volcanic cloud with the observed or estimated volcanic cloud from the Toulouse Volcanic Ash Advisory Center. Overall, we found a good match between simulated and observed quantities (tephra loads and volcanic cloud position), especially when accurate information on eruptive conditions (column height and duration) are supplied by the VONAs. Finally, through a statistical analysis, we found that column height and wind field are fundamental in determining tephra ground accumulation. For this reason, these parameters should be constrained by observational data as accurately as possible when performing numerical simulations, especially in the line of developing operational workflows.
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[1]  
Andronico D(2021)The 1986–2021 paroxysmal episodes at the summit craters of Mt. Etna: insights into volcano dynamics and hazard Earth-Sci Rev 220 103686-14
[2]  
Cannata A(2021)Uncovering the eruptive patterns of the 2019 double paroxysm eruption crisis of Stromboli volcano Nat Commun 12 1-96
[3]  
Di Grazia G(2021)The independent volcanic eruption source parameter archive (IVESPA, version 1.0): a new observational database to support explosive eruptive column model validation and development J Volcanol Geotherm Res 417 107295-456
[4]  
Ferrari F(2010)Quantitative assessment of volcanic ash hazards for health and infrastructure at Mt. Etna (Italy) by numerical simulation J Volcanol Geotherm Res 192 85-8
[5]  
Andronico D(2005)Total grain-size distribution and volume of tephra-fall deposits Bull Volcanol 67 441-69
[6]  
Del Bello E(2021)The radius of the umbrella cloud helps characterize large explosive volcanic eruptions Commun Earth Environ 2 1-25
[7]  
D’Oriano C(2018)Proximal monitoring of the 2011–2015 Etna lava fountains using MSG-SEVIRI data Geosciences 8 140-1172
[8]  
Landi P(2017)Monitoring the December 2015 summit eruptions of Mt. Etna (Italy): implications on eruptive dynamics J Volcanol Geotherm Res 341 53-4341
[9]  
Pardini F(2016)Results of the eruptive column model inter-comparison study J Volcanol Geotherm Res 326 2-1019
[10]  
Scarlato P(2009)Polynomial chaos expansion for sensitivity analysis Reliab Eng Syst Saf 94 1161-201