Earth-prints repository, logo   DSpace

About DSpace Software
|earth-prints home page | roma library | bologna library | catania library | milano library | napoli library | palermo library
Please use this identifier to cite or link to this item:

Authors: Scollo, S.*
Folch, A.*
Costa, A.*
Title: A parametric and comparative study of different tephra fallout models
Title of journal: Journal of Volcanology and Geothermal Research
Series/Report no.: /176 (2008)
Publisher: Elsevier
Issue Date: 16-Apr-2008
DOI: 10.1016/j.jvolgeores.2008.04.002
Keywords: tephra dispersal models; input parameter; parametric and comparative study; Mount Etna; forecasting.
Abstract: We perform a parametric and comparative study on three different tephra dispersal models (FALL3D,HAZMAP, and TEPHRA) applied to two different scenarios expected for Etna volcano. These scenarios are similar to the recent 2002–03 and 1990 Etna eruptions and correspond, respectively, to a weak and to a strong plume eruption. For each model and scenario we perform a parametric study on several inputs in order to quantify how a variation on a given input parameter (i.e. an uncertainty on the model input) affects the results of the model. The study considers topographic effects, different description for the eruption column, column height influence, different fits for terminal velocities of particles, the effect of particle shape and, finally, the variation of the modal grain-size. Model differences are quantified by means of a normalized distance that indicates how close, in average, the results from two different simulations are.We also compare predictions from different models to determine under which circumstances the use of a more elaborated model is justified. Results from our parametric study show that output of the models can be strongly sensitive to the uncertainties and assumptions on input parameters, such as mainly mass eruption rate, column height, distribution of the mass along the column, bulk grain-size distribution. This highlights that, for optimal forecasts, is urgent to improve the description of these parameters and of some important physical processes like fragmentation and eruption column dynamics. Further, differences between models are often lower than those due to the uncertainties of input parameters, although they become more high in simulating weak plumes. Thus the choice of the model mainly depends on the kind of application such as the need to simulate the evolution of volcanic clouds in the atmosphere. Finally, the use of both a semi-analytical (HAZMAP) and a fully computational (FALL3D) model for inverting field data of the 2001 Etna eruption showed that the best-fit parameters are similar for both models, and are consistent with values obtained using independent techniques.
Appears in Collections:05.01.01. Data processing
Papers Published / Papers in press

Files in This Item:

File SizeFormatVisibility
Scollo_et_al_2008.pdf2.68 MBAdobe PDFView/Open

This item is licensed under a Creative Commons License
Creative Commons

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.

Share this record




Stumble it!



Valid XHTML 1.0! ICT Support, development & maintenance are provided by CINECA. Powered on DSpace Software. CINECA