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  5. The effect of Etna volcanic ash clouds on the Maltese Islands
 
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The effect of Etna volcanic ash clouds on the Maltese Islands

Author(s)
Azzopardi, F.  
Physics Department, University of Malta, Msida MSD 2080, Malta  
Raymond, E.  
Physics Department, University of Malta, Msida MSD 2080, Malta  
Prestifilippo, M.  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia  
Scollo, S.  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia  
Coltelli, M.  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia  
Language
English
Obiettivo Specifico
3V. Dinamiche e scenari eruttivi
Status
Published
JCR Journal
JCR Journal
Journal
Journal of volcanology and geothermal research  
Issue/vol(year)
/260 (2013)
ISSN
0377-0273
Electronic ISSN
1872-6097
Publisher
Elsevier Science Limited
Pages (printed)
13-26
Date Issued
2013
DOI
10.1016/j.jvolgeores.2013.04.019
URI
https://www.earth-prints.org/handle/2122/9721
Subjects
04. Solid Earth::04.08. Volcanology::04.08.08. Volcanic risk  
Subjects

volcanic ash forecast...

Maltese Islands

Abstract
In this paper, we have studied in depth the effect of Etna volcanic ash clouds on the Maltese Islands. Research was carried out to gather information about Etna's eruptions that impacted the Maltese Islands, starting with historical eruptions dating back to the 14th century continuing to present day. A statistical approach was utilized
to provide tephra deposit load and ash concentration using PUFF — a model which simulates the transport, dispersion and sedimentation of volcanic ash. Three different eruptive scenarios that characterize Etna's recent activity were considered; the first scenario representing the 2001 eruption (Sc1), the second scenario
representing the July 1998 eruption (Sc2) whilst the third scenario represents the recent activity in 2011– 2012 (Sc3). We found that the time taken for the volcanic ash cloud to reach the Maltese Islands, when the wind direction is toward the south-west ranges from 4 to 6 h. The probability that an Etna volcanic cloud reaches Malta during an eruption is about 15% per annum. The now calibrated model may be now used to
produce deposit load and cumulative columnar load (i.e. summation from maximum height of volcanic cloud to ground) of volcanic ash in atmosphere for the Maltese area and help the aviation authorities and Malta airport to make decisions during Etna eruptions. This will be of direct use to local communities and aviation.
Type
article
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Azzopardi_et_al_2013.pdf

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