Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10398
Authors: Tierz, P.* 
Sandri, L.* 
Costa, A.* 
Zaccarelli, L.* 
Di Vito, M. A.* 
Sulpizio, R.* 
Marzocchi, W.* 
Title: Suitability of energy cone for probabilistic volcanic hazard assessment: validation tests at Somma-Vesuvius and Campi Flegrei (Italy)
Journal: Bulletin of volcanology 
Series/Report no.: /78(2016)
Publisher: Springer Berlin Heidelberg
Issue Date: 2016
DOI: 10.1007/s00445-016-1073-9
Keywords: Pyroclastic density currents
Probabilistic hazard assessment
Energy cone
Somma-Vesuvius
Campi Flegrei
Subject Classification04. Solid Earth::04.08. Volcanology::04.08.99. General or miscellaneous 
Abstract: Pyroclastic density currents (PDCs) are gravitydriven hot mixtures of gas and volcanic particles which can propagate at high speed and cover distances up to several tens of kilometers around a given volcano. Therefore, they pose a severe hazard to the surroundings of explosive volcanoes able to produce such phenomena. Despite this threat, probabilistic volcanic hazard assessment (PVHA) of PDCs is still in an early stage of development. PVHA is rooted in the quantification of the large uncertainties (aleatory and epistemic) which characterize volcanic hazard analyses. This quantification typically requires a big dataset of hazard footprints obtained from numerical simulations of the physical process. For PDCs, numerical models range from very sophisticated (not useful for PVHA because of their very long runtimes) to very simple models (criticized because of their highly simplified physics). We present here a systematic and robust validation testing of a simple PDC model, the energy cone (EC), to unravel whether it can be applied to PVHA of PDCs. Using past PDC deposits at Somma-Vesuvius and Campi Flegrei (Italy), we assess the ability of EC to capture the values and variability in some relevant variables for hazard assessment, i.e., area of PDC invasion and maximum runout. In terms of area of invasion, the highest Jaccard coefficients range from 0.33 to 0.86 which indicates an equal or better performance compared to other volcanic mass-flow models. The p values for the observed maximum runouts vary from 0.003 to 0.44. Finally, the frequencies of PDC arrival computed from the EC are similar to those determined from the spatial distribution of past PDC deposits, with high PDC-arrival frequencies over an ∼8-km radius from the crater area at Somma-Vesuvius and around the Astroni crater at Campi Flegrei. The insights derived from our validation tests seem to indicate that the EC is a suitable candidate to compute PVHA of PDCs.
Appears in Collections:Article published / in press

Files in This Item:
File Description SizeFormat Existing users please Login
di_tierz_2016 bv energy cone 445-016-1073-9.pdf3.68 MBAdobe PDF
Show full item record

WEB OF SCIENCETM
Citations 50

23
checked on Feb 10, 2021

Page view(s)

377
checked on Apr 24, 2024

Download(s)

24
checked on Apr 24, 2024

Google ScholarTM

Check

Altmetric