Modelling the macroscopic behavior of Strombolian explosions at Erebus volcano

Abstract We analyze seismic signals associated with the Strombolian explosion quakes at Erebus volcano (Antarctica), examining the high-frequency (>0.5Hz) portion of the spectrum. We consider recordings relative to two time periods during the years 2005 and 2006. Cross-correlation analysis allows...

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Published in:Physics of the Earth and Planetary Interiors
Language:English
Published: Elsevier 2011
Subjects:
Online Access:http://hdl.handle.net/2262/53007
https://doi.org/10.1016/j.pepi.2009.05.003
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spelling fttrinitycoll:oai:tara.tcd.ie:2262/53007 2023-05-15T13:46:17+02:00 Modelling the macroscopic behavior of Strombolian explosions at Erebus volcano 2011-03-04T02:48:54Z http://hdl.handle.net/2262/53007 https://doi.org/10.1016/j.pepi.2009.05.003 en eng Elsevier 00319201 (ISSN) S0031-9201(09)00123-X (PII) S0031-9201(09)00123-X (publisherID) http://hdl.handle.net/2262/53007 Physics of the Earth and Planetary Interiors 176 3-4 174 doi:10.1016/j.pepi.2009.05.003 2009 18 months Strombolian explosions Erebus volcano Diffusion 2011 fttrinitycoll https://doi.org/10.1016/j.pepi.2009.05.003 2020-02-16T13:51:40Z Abstract We analyze seismic signals associated with the Strombolian explosion quakes at Erebus volcano (Antarctica), examining the high-frequency (>0.5Hz) portion of the spectrum. We consider recordings relative to two time periods during the years 2005 and 2006. Cross-correlation analysis allows us to distinguish three classes of events. Spectral properties and polarization analysis provide evidence of a very complex volcanic structure. We conduct analyses to elucidate the macroscopic dynamic system associated with the explosions. The distribution of the times between successive explosion-quakes is exponential, implying a Poissonian process as observed at Stromboli volcano but on a different time scale. The sequence of the occurrence of the explosions can be described by classical intermittency. A coalescence Chandrasekar-Landau mean-field model reproduces gas bubble sizes comparable with those observed at the lava lake surface. Finally, the classical equation for the ascent of gas bubbles is generalized by adding a diffusive process. This model provides ascent velocities depending on the bubble radius: for gas bubbles greater than a few centimeters, variation in ascent velocity due to diffusion becomes negligible and the ascent velocity appears to be governed primarily by buoyancy. correspondance: Corresponding author at: Dipartimento di Matematica e Informatica, Universita di Salerno, Via Ponte Don Melillo, Fisciano (SA) 84084 Italia Tel.: +39 089965288; fax: +39 089965275. (Falanga, M.) rosfal@sa.infn.it (Falanga, M.) Dipartimento di Matematica e Informatica--> , Universita di Salerno--> , Via Ponte Don Melillo--> , 84084 Fisciano (SA)--> , Italia--> - (De Lauro, E.) Dipartimento di Matematica e Informatica--> , Universita di Salerno--> , Via Ponte Don Melillo--> , 84084 Fisciano (SA)--> , Italia--> - (De Martino, S.) INFN--> , Gruppo collegato di Salerno--> , Via S. Allende--> , 84081 Baronissi (SA)--> , Italia--> - (De Martino, S.) Dipartimento di Fisica--> , Universita di Salerno--> , Via S. Allende--> , 84081 Baronissi (SA)--> , Italia--> - (Falanga, M.) INFN--> , Gruppo collegato di Salerno--> , Via S. Allende--> , 84081 Baronissi (SA)--> , Italia--> - (Falanga, M.) Dipartimento di Matematica e Informatica--> , Universita di Salerno--> , Via Ponte Don Melillo--> , 84084 Fisciano (SA)--> , Italia--> - ITALY (Falanga, M.) Dipartimento di Matematica e Informatica--> , Universita di Salerno--> , Via Ponte Don Melillo--> , 84084 Fisciano (SA)--> , Italia--> - (Palo, M.) ITALY Received: 2008-10-30 Revised: 2009-04-03 Accepted: 2009-05-01 Other/Unknown Material Antarc* Antarctica The University of Dublin, Trinity College: TARA (Trinity's Access to Research Archive) Lava Lake ENVELOPE(-128.996,-128.996,55.046,55.046) Physics of the Earth and Planetary Interiors 176 3-4 174 186
institution Open Polar
collection The University of Dublin, Trinity College: TARA (Trinity's Access to Research Archive)
op_collection_id fttrinitycoll
language English
topic Strombolian explosions
Erebus volcano
Diffusion
spellingShingle Strombolian explosions
Erebus volcano
Diffusion
Modelling the macroscopic behavior of Strombolian explosions at Erebus volcano
topic_facet Strombolian explosions
Erebus volcano
Diffusion
description Abstract We analyze seismic signals associated with the Strombolian explosion quakes at Erebus volcano (Antarctica), examining the high-frequency (>0.5Hz) portion of the spectrum. We consider recordings relative to two time periods during the years 2005 and 2006. Cross-correlation analysis allows us to distinguish three classes of events. Spectral properties and polarization analysis provide evidence of a very complex volcanic structure. We conduct analyses to elucidate the macroscopic dynamic system associated with the explosions. The distribution of the times between successive explosion-quakes is exponential, implying a Poissonian process as observed at Stromboli volcano but on a different time scale. The sequence of the occurrence of the explosions can be described by classical intermittency. A coalescence Chandrasekar-Landau mean-field model reproduces gas bubble sizes comparable with those observed at the lava lake surface. Finally, the classical equation for the ascent of gas bubbles is generalized by adding a diffusive process. This model provides ascent velocities depending on the bubble radius: for gas bubbles greater than a few centimeters, variation in ascent velocity due to diffusion becomes negligible and the ascent velocity appears to be governed primarily by buoyancy. correspondance: Corresponding author at: Dipartimento di Matematica e Informatica, Universita di Salerno, Via Ponte Don Melillo, Fisciano (SA) 84084 Italia Tel.: +39 089965288; fax: +39 089965275. (Falanga, M.) rosfal@sa.infn.it (Falanga, M.) Dipartimento di Matematica e Informatica--> , Universita di Salerno--> , Via Ponte Don Melillo--> , 84084 Fisciano (SA)--> , Italia--> - (De Lauro, E.) Dipartimento di Matematica e Informatica--> , Universita di Salerno--> , Via Ponte Don Melillo--> , 84084 Fisciano (SA)--> , Italia--> - (De Martino, S.) INFN--> , Gruppo collegato di Salerno--> , Via S. Allende--> , 84081 Baronissi (SA)--> , Italia--> - (De Martino, S.) Dipartimento di Fisica--> , Universita di Salerno--> , Via S. Allende--> , 84081 Baronissi (SA)--> , Italia--> - (Falanga, M.) INFN--> , Gruppo collegato di Salerno--> , Via S. Allende--> , 84081 Baronissi (SA)--> , Italia--> - (Falanga, M.) Dipartimento di Matematica e Informatica--> , Universita di Salerno--> , Via Ponte Don Melillo--> , 84084 Fisciano (SA)--> , Italia--> - ITALY (Falanga, M.) Dipartimento di Matematica e Informatica--> , Universita di Salerno--> , Via Ponte Don Melillo--> , 84084 Fisciano (SA)--> , Italia--> - (Palo, M.) ITALY Received: 2008-10-30 Revised: 2009-04-03 Accepted: 2009-05-01
title Modelling the macroscopic behavior of Strombolian explosions at Erebus volcano
title_short Modelling the macroscopic behavior of Strombolian explosions at Erebus volcano
title_full Modelling the macroscopic behavior of Strombolian explosions at Erebus volcano
title_fullStr Modelling the macroscopic behavior of Strombolian explosions at Erebus volcano
title_full_unstemmed Modelling the macroscopic behavior of Strombolian explosions at Erebus volcano
title_sort modelling the macroscopic behavior of strombolian explosions at erebus volcano
publisher Elsevier
publishDate 2011
url http://hdl.handle.net/2262/53007
https://doi.org/10.1016/j.pepi.2009.05.003
long_lat ENVELOPE(-128.996,-128.996,55.046,55.046)
geographic Lava Lake
geographic_facet Lava Lake
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation 00319201 (ISSN)
S0031-9201(09)00123-X (PII)
S0031-9201(09)00123-X (publisherID)
http://hdl.handle.net/2262/53007
Physics of the Earth and Planetary Interiors
176
3-4
174
doi:10.1016/j.pepi.2009.05.003
op_rights 2009
18 months
op_doi https://doi.org/10.1016/j.pepi.2009.05.003
container_title Physics of the Earth and Planetary Interiors
container_volume 176
container_issue 3-4
container_start_page 174
op_container_end_page 186
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