Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9718
Authors: Andronico, D.* 
Scollo, S.* 
Lo Castro, M. D.* 
Cristaldi, A.* 
Lodato, L.* 
Taddeucci, J.* 
Title: Eruption dynamics and tephra dispersal from the 24 November 2006 paroxysm at South-East Crater, Mt Etna, Italy
Journal: Journal of volcanology and geothermal research 
Series/Report no.: /274 (2014)
Publisher: Elsevier Science Limited
Issue Date: 2014
DOI: 10.1016/j.jvolgeores.2014.01.009
Keywords: tephra deposit
Etna eruption
Subject Classification04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring 
Abstract: Between 30 August and 15 December 2006,Mt Etna, Italy, underwent both effusive and explosive activity which took place fromthe South-East Crater, one of its summit craters. Several paroxysmal episodes followed in succession, separated by a fewdays of minor activity and characterised by dissimilar explosive style and intensity. Here, we report one of the most studied and powerful episodes, which started early in the morning on 24 November 2006 and lasted about 13 h. Excellent weather conditions enabled reconstructing in detail the onset and evolution of the eruptive phenomena both by live-camera recordings and direct observations. The explosive activity consisted of powerful Strombolian activity alternating with short periods of lava fountains. A weak volcanic plume rose up to ~2 km above the volcanic vent, followed by tephra fallout which covered the SE and S flanks of Etna. Campaigns allowed collecting about 40 tephra samples and mapping the fallout deposit. The clockwise shifting of the volcanic plume during the eruption caused the different timing of the fallout on the ground, thus widening the dispersal area. Voronoi's method was used to evaluate: i) the total grain-size distribution, indicating that the fallout deposit peaked at 1 ϕ, and, for the first time at Etna, ii) the total componentry distribution, finding thatmost of the particles were lithics, with a low proportion of juvenile vs. lithics (34:65). The total erupted mass was estimated ~1.9 × 108 kg, corresponding to a mass eruption rate of ~5 × 103 kg s−1. Physical parameters and textural features of the erupted products suggest that the 24 November 2006 explosive event may be classified as small-sized in the recent history of Etna, and that the eruptive dynamicwasmainly governed by magma/gas decoupling, which produced relatively fine-grained fallout deposits containing unusual elongated sideromelane ash particles.
Appears in Collections:Article published / in press

Files in This Item:
File Description SizeFormat Existing users please Login
Andronico_et_al_2014.pdf4.85 MBAdobe PDF
Show full item record

WEB OF SCIENCETM
Citations 20

27
checked on Feb 10, 2021

Page view(s) 50

278
checked on Apr 20, 2024

Download(s)

26
checked on Apr 20, 2024

Google ScholarTM

Check

Altmetric