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: http://hdl.handle.net/2122/7266

Authors: Neri, M.*
Acocella, V.*
Behncke, B.*
Giammanco, S.*
Mazzarini, F.*
Rust, D.
Title: Structural analysis of the eruptive fissures at Mount Etna (Italy)
Other Titles: The eruptive fissures of Mt. Etna
Title of journal: Annals of Geophysics
Series/Report no.: 5/54 (2011)
Publisher: Istituto Nazionale di Geofisica e Vulcanologia
Issue Date: Dec-2011
DOI: 10.4401/ag-5332
URL: http://www.annalsofgeophysics.eu/index.php/annals/article/viewFile/5332/5465
Keywords: dike
magmas
tectonics
structural geology
Abstract: Mount Etna produces frequent eruptions from its summit craters and from fissures on its flanks. The flank fissures trend approximately radially to the summit, and are mainly concentrated in three rift zones that are located on the NE, S and W flanks. Many flank eruptions result from lateral magma transfer from the central conduit into fractures intersecting the flanks, although some eruptions are fed through newly formed conduits that are not directly linked to the central conduit. We analyzed the structural features of eruptions from 1900 to the present, one of the most active periods in the documented eruptive history of Etna, which comprised 35 summit and 33 flank events. Except for a small eruption on the W flank in 1974, all of the flank eruptions in this interval occurred on or near the NE and S rifts. Eruptions in the NE sector were generally shorter, but their fissure systems developed more rapidly and were longer than those in the S sector. In contrast, summit eruptions had longer mean durations, but generally lower effusion rates (excluding paroxysmal events characterized by very high effusion rates that lasted only a few hours). This database was examined considering the main parameters (frequency and strike) of the eruptive fissures that were active over the last ~2 ka. The distribution in time and space of summit and flank eruptions appears to be closely linked to the dynamics of the unstable E to S flank sector of Etna, which is undergoing periodic displacements induced by subvolcanic magma accumulation and gravitational pull. In this framework, magma accumulation below Etna exerts pressure against the unbuttressed E and S flanks, which have moved away from the rest of the volcano. This has caused an extension to the detachment zones, and has facilitated magma transfer from the central conduit into the flanks.
Appears in Collections:04.01.99. General or miscellaneous
04.04.99. General or miscellaneous
04.04.09. Structural geology
04.07.99. General or miscellaneous
04.07.05. Stress
04.07.07. Tectonics
04.08.99. General or miscellaneous
04.08.03. Magmas
04.08.06. Volcano monitoring
04.08.08. Volcanic risk
05.08.99. General or miscellaneous
Papers Published / Papers in press

Files in This Item:

File Description SizeFormatVisibility
2011 Neri et al AG 2011.pdfArticle971.54 kBAdobe 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
Del.icio.us

Citeulike

Connotea

Facebook

Stumble it!

reddit


 

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