Submarine pyroclastic deposits formed during the 20th May 2006 dome collapse of the Soufrière Hills Volcano, Montserrat

The 20th May 2006 lava dome collapse of the Soufrière Hills Volcano, Montserrat, had a total non-dense rock equivalent (non-DRE) collapse volume of approximately 115 × 10 6  m 3 . The majority of this volume was deposited into the ocean. The collapse was rapid, 85% of the mobilized volume being remo...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Bulletin of volcanology 2012-03, Vol.74 (2), p.391-405
Hauptverfasser: Trofimovs, J., Foster, C., Sparks, R. S. J., Loughlin, S., Le Friant, A., Deplus, C., Porritt, L., Christopher, T., Luckett, R., Talling, P. J., Palmer, M. R., Le Bas, T.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 405
container_issue 2
container_start_page 391
container_title Bulletin of volcanology
container_volume 74
creator Trofimovs, J.
Foster, C.
Sparks, R. S. J.
Loughlin, S.
Le Friant, A.
Deplus, C.
Porritt, L.
Christopher, T.
Luckett, R.
Talling, P. J.
Palmer, M. R.
Le Bas, T.
description The 20th May 2006 lava dome collapse of the Soufrière Hills Volcano, Montserrat, had a total non-dense rock equivalent (non-DRE) collapse volume of approximately 115 × 10 6  m 3 . The majority of this volume was deposited into the ocean. The collapse was rapid, 85% of the mobilized volume being removed in just 35 min, giving peak pyroclastic flow flux of 66 × 10 3  m 3  s −1 . Channel and levee facies on the submarine flanks of the volcano and formation of a thick, steep-sided ridge, suggest that the largest and most dense blocks were transported proximally as a high concentration granular flow. Of the submerged volume, 30% was deposited from the base of this granular flow, forming a linear, high-relief ridge that extends 7 km from shore. The remaining 70% of the submerged volume comprises the finer grain sizes, which were transported at least 40 km by turbidity currents on gradients of
doi_str_mv 10.1007/s00445-011-0533-5
format Article
fullrecord <record><control><sourceid>proquest_hal_p</sourceid><recordid>TN_cdi_hal_primary_oai_HAL_insu_03583366v1</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2590747491</sourcerecordid><originalsourceid>FETCH-LOGICAL-a4595-5fa67fe79ed8c99f5713ec41696772ffaab9ab073eb168434c6238b2c8448ee33</originalsourceid><addsrcrecordid>eNp1kd2KFDEQhYMoOI4-gHdBEEFsrfynL5dFHWEWL1a9Del04mTp6bRJtzhv5Hv4YmbsZQXBqyqorw7ncBB6SuA1AVBvCgDnogFCGhCMNeIe2hDOaAOatPfRBqjQjW4BHqJHpdwA1KNUG_TjeumONsfR4-mUkxtsmaPDvZ9SiXPBIeWj73G_VOQrng8eU5gP-Mqe6gIS9-nosUvDYKficQp_kOu0hBx__cwe7-IwFPwlDc6O6RW-SuNcfM52foweBDsU_-R2btHnd28_Xe6a_cf3Hy4v9o3lohWNCFaq4FXre-3aNghFmHecyFYqRUOwtmttB4r5jkjNGXeSMt1RpznX3jO2RS9X3YMdzJRjDXsyyUazu9ibOJbFABOaMSm_kwq_WOEpp2-LL7M5xuJ8TTf6tBTTUqm1UMAr-ewf8iYteaxJKkSZZKp62iKyQi6nUrIPdwYImHNtZq3N1NrMuTYj6s_zW2FbnB1CtqOL5e6RCqG0ElA5unJlOlfj818D_xf_DaX-pqo</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>922363707</pqid></control><display><type>article</type><title>Submarine pyroclastic deposits formed during the 20th May 2006 dome collapse of the Soufrière Hills Volcano, Montserrat</title><source>SpringerLink Journals - AutoHoldings</source><creator>Trofimovs, J. ; Foster, C. ; Sparks, R. S. J. ; Loughlin, S. ; Le Friant, A. ; Deplus, C. ; Porritt, L. ; Christopher, T. ; Luckett, R. ; Talling, P. J. ; Palmer, M. R. ; Le Bas, T.</creator><creatorcontrib>Trofimovs, J. ; Foster, C. ; Sparks, R. S. J. ; Loughlin, S. ; Le Friant, A. ; Deplus, C. ; Porritt, L. ; Christopher, T. ; Luckett, R. ; Talling, P. J. ; Palmer, M. R. ; Le Bas, T.</creatorcontrib><description>The 20th May 2006 lava dome collapse of the Soufrière Hills Volcano, Montserrat, had a total non-dense rock equivalent (non-DRE) collapse volume of approximately 115 × 10 6  m 3 . The majority of this volume was deposited into the ocean. The collapse was rapid, 85% of the mobilized volume being removed in just 35 min, giving peak pyroclastic flow flux of 66 × 10 3  m 3  s −1 . Channel and levee facies on the submarine flanks of the volcano and formation of a thick, steep-sided ridge, suggest that the largest and most dense blocks were transported proximally as a high concentration granular flow. Of the submerged volume, 30% was deposited from the base of this granular flow, forming a linear, high-relief ridge that extends 7 km from shore. The remaining 70% of the submerged volume comprises the finer grain sizes, which were transported at least 40 km by turbidity currents on gradients of &lt;2°. At several localities, the May 2006 distal turbidity currents ran up 200 m of topography and eroded up to 20 cm of underlying substrate. Multiple turbidites are preserved, representing current reflection from the graben margins and deflection around topography. The high energy of the May 2006 collapse resulted in longer submarine run out than the larger (210 × 10 6  m 3 ) Soufrière Hills dome collapse in July 2003.</description><identifier>ISSN: 0258-8900</identifier><identifier>EISSN: 1432-0819</identifier><identifier>DOI: 10.1007/s00445-011-0533-5</identifier><identifier>CODEN: BUVOEW</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer-Verlag</publisher><subject>Bathymetry ; Crystalline rocks ; Earth and Environmental Science ; Earth Sciences ; Earth, ocean, space ; Engineering and environment geology. Geothermics ; Exact sciences and technology ; Geology ; Geophysics ; Geophysics/Geodesy ; Hills ; Igneous and metamorphic rocks petrology, volcanic processes, magmas ; Lava ; Lava domes ; Mineralogy ; Natural hazards: prediction, damages, etc ; Research Article ; Sciences of the Universe ; Sedimentology ; Topography ; Turbidity ; Turbidity currents ; Volcanoes ; Volcanology</subject><ispartof>Bulletin of volcanology, 2012-03, Vol.74 (2), p.391-405</ispartof><rights>Springer-Verlag 2011</rights><rights>2015 INIST-CNRS</rights><rights>Springer-Verlag 2012</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a4595-5fa67fe79ed8c99f5713ec41696772ffaab9ab073eb168434c6238b2c8448ee33</citedby><cites>FETCH-LOGICAL-a4595-5fa67fe79ed8c99f5713ec41696772ffaab9ab073eb168434c6238b2c8448ee33</cites><orcidid>0000-0003-3689-3704 ; 0000-0001-8901-2515</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s00445-011-0533-5$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s00445-011-0533-5$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>230,314,776,780,881,27901,27902,41464,42533,51294</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=25578750$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://insu.hal.science/insu-03583366$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Trofimovs, J.</creatorcontrib><creatorcontrib>Foster, C.</creatorcontrib><creatorcontrib>Sparks, R. S. J.</creatorcontrib><creatorcontrib>Loughlin, S.</creatorcontrib><creatorcontrib>Le Friant, A.</creatorcontrib><creatorcontrib>Deplus, C.</creatorcontrib><creatorcontrib>Porritt, L.</creatorcontrib><creatorcontrib>Christopher, T.</creatorcontrib><creatorcontrib>Luckett, R.</creatorcontrib><creatorcontrib>Talling, P. J.</creatorcontrib><creatorcontrib>Palmer, M. R.</creatorcontrib><creatorcontrib>Le Bas, T.</creatorcontrib><title>Submarine pyroclastic deposits formed during the 20th May 2006 dome collapse of the Soufrière Hills Volcano, Montserrat</title><title>Bulletin of volcanology</title><addtitle>Bull Volcanol</addtitle><description>The 20th May 2006 lava dome collapse of the Soufrière Hills Volcano, Montserrat, had a total non-dense rock equivalent (non-DRE) collapse volume of approximately 115 × 10 6  m 3 . The majority of this volume was deposited into the ocean. The collapse was rapid, 85% of the mobilized volume being removed in just 35 min, giving peak pyroclastic flow flux of 66 × 10 3  m 3  s −1 . Channel and levee facies on the submarine flanks of the volcano and formation of a thick, steep-sided ridge, suggest that the largest and most dense blocks were transported proximally as a high concentration granular flow. Of the submerged volume, 30% was deposited from the base of this granular flow, forming a linear, high-relief ridge that extends 7 km from shore. The remaining 70% of the submerged volume comprises the finer grain sizes, which were transported at least 40 km by turbidity currents on gradients of &lt;2°. At several localities, the May 2006 distal turbidity currents ran up 200 m of topography and eroded up to 20 cm of underlying substrate. Multiple turbidites are preserved, representing current reflection from the graben margins and deflection around topography. The high energy of the May 2006 collapse resulted in longer submarine run out than the larger (210 × 10 6  m 3 ) Soufrière Hills dome collapse in July 2003.</description><subject>Bathymetry</subject><subject>Crystalline rocks</subject><subject>Earth and Environmental Science</subject><subject>Earth Sciences</subject><subject>Earth, ocean, space</subject><subject>Engineering and environment geology. Geothermics</subject><subject>Exact sciences and technology</subject><subject>Geology</subject><subject>Geophysics</subject><subject>Geophysics/Geodesy</subject><subject>Hills</subject><subject>Igneous and metamorphic rocks petrology, volcanic processes, magmas</subject><subject>Lava</subject><subject>Lava domes</subject><subject>Mineralogy</subject><subject>Natural hazards: prediction, damages, etc</subject><subject>Research Article</subject><subject>Sciences of the Universe</subject><subject>Sedimentology</subject><subject>Topography</subject><subject>Turbidity</subject><subject>Turbidity currents</subject><subject>Volcanoes</subject><subject>Volcanology</subject><issn>0258-8900</issn><issn>1432-0819</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNp1kd2KFDEQhYMoOI4-gHdBEEFsrfynL5dFHWEWL1a9Del04mTp6bRJtzhv5Hv4YmbsZQXBqyqorw7ncBB6SuA1AVBvCgDnogFCGhCMNeIe2hDOaAOatPfRBqjQjW4BHqJHpdwA1KNUG_TjeumONsfR4-mUkxtsmaPDvZ9SiXPBIeWj73G_VOQrng8eU5gP-Mqe6gIS9-nosUvDYKficQp_kOu0hBx__cwe7-IwFPwlDc6O6RW-SuNcfM52foweBDsU_-R2btHnd28_Xe6a_cf3Hy4v9o3lohWNCFaq4FXre-3aNghFmHecyFYqRUOwtmttB4r5jkjNGXeSMt1RpznX3jO2RS9X3YMdzJRjDXsyyUazu9ibOJbFABOaMSm_kwq_WOEpp2-LL7M5xuJ8TTf6tBTTUqm1UMAr-ewf8iYteaxJKkSZZKp62iKyQi6nUrIPdwYImHNtZq3N1NrMuTYj6s_zW2FbnB1CtqOL5e6RCqG0ElA5unJlOlfj818D_xf_DaX-pqo</recordid><startdate>201203</startdate><enddate>201203</enddate><creator>Trofimovs, J.</creator><creator>Foster, C.</creator><creator>Sparks, R. S. J.</creator><creator>Loughlin, S.</creator><creator>Le Friant, A.</creator><creator>Deplus, C.</creator><creator>Porritt, L.</creator><creator>Christopher, T.</creator><creator>Luckett, R.</creator><creator>Talling, P. J.</creator><creator>Palmer, M. R.</creator><creator>Le Bas, T.</creator><general>Springer-Verlag</general><general>Springer</general><general>Springer Nature B.V</general><general>Springer Verlag</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7TN</scope><scope>7XB</scope><scope>88I</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>F1W</scope><scope>GNUQQ</scope><scope>H96</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L.G</scope><scope>M2P</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0003-3689-3704</orcidid><orcidid>https://orcid.org/0000-0001-8901-2515</orcidid></search><sort><creationdate>201203</creationdate><title>Submarine pyroclastic deposits formed during the 20th May 2006 dome collapse of the Soufrière Hills Volcano, Montserrat</title><author>Trofimovs, J. ; Foster, C. ; Sparks, R. S. J. ; Loughlin, S. ; Le Friant, A. ; Deplus, C. ; Porritt, L. ; Christopher, T. ; Luckett, R. ; Talling, P. J. ; Palmer, M. R. ; Le Bas, T.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a4595-5fa67fe79ed8c99f5713ec41696772ffaab9ab073eb168434c6238b2c8448ee33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Bathymetry</topic><topic>Crystalline rocks</topic><topic>Earth and Environmental Science</topic><topic>Earth Sciences</topic><topic>Earth, ocean, space</topic><topic>Engineering and environment geology. Geothermics</topic><topic>Exact sciences and technology</topic><topic>Geology</topic><topic>Geophysics</topic><topic>Geophysics/Geodesy</topic><topic>Hills</topic><topic>Igneous and metamorphic rocks petrology, volcanic processes, magmas</topic><topic>Lava</topic><topic>Lava domes</topic><topic>Mineralogy</topic><topic>Natural hazards: prediction, damages, etc</topic><topic>Research Article</topic><topic>Sciences of the Universe</topic><topic>Sedimentology</topic><topic>Topography</topic><topic>Turbidity</topic><topic>Turbidity currents</topic><topic>Volcanoes</topic><topic>Volcanology</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Trofimovs, J.</creatorcontrib><creatorcontrib>Foster, C.</creatorcontrib><creatorcontrib>Sparks, R. S. J.</creatorcontrib><creatorcontrib>Loughlin, S.</creatorcontrib><creatorcontrib>Le Friant, A.</creatorcontrib><creatorcontrib>Deplus, C.</creatorcontrib><creatorcontrib>Porritt, L.</creatorcontrib><creatorcontrib>Christopher, T.</creatorcontrib><creatorcontrib>Luckett, R.</creatorcontrib><creatorcontrib>Talling, P. J.</creatorcontrib><creatorcontrib>Palmer, M. R.</creatorcontrib><creatorcontrib>Le Bas, T.</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Oceanic Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric &amp; Aquatic Science Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>ProQuest Central Student</collection><collection>Aquatic Science &amp; Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy &amp; Non-Living Resources</collection><collection>SciTech Premium Collection</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science &amp; Fisheries Abstracts (ASFA) Professional</collection><collection>Science Database</collection><collection>Earth, Atmospheric &amp; Aquatic Science Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Bulletin of volcanology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Trofimovs, J.</au><au>Foster, C.</au><au>Sparks, R. S. J.</au><au>Loughlin, S.</au><au>Le Friant, A.</au><au>Deplus, C.</au><au>Porritt, L.</au><au>Christopher, T.</au><au>Luckett, R.</au><au>Talling, P. J.</au><au>Palmer, M. R.</au><au>Le Bas, T.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Submarine pyroclastic deposits formed during the 20th May 2006 dome collapse of the Soufrière Hills Volcano, Montserrat</atitle><jtitle>Bulletin of volcanology</jtitle><stitle>Bull Volcanol</stitle><date>2012-03</date><risdate>2012</risdate><volume>74</volume><issue>2</issue><spage>391</spage><epage>405</epage><pages>391-405</pages><issn>0258-8900</issn><eissn>1432-0819</eissn><coden>BUVOEW</coden><abstract>The 20th May 2006 lava dome collapse of the Soufrière Hills Volcano, Montserrat, had a total non-dense rock equivalent (non-DRE) collapse volume of approximately 115 × 10 6  m 3 . The majority of this volume was deposited into the ocean. The collapse was rapid, 85% of the mobilized volume being removed in just 35 min, giving peak pyroclastic flow flux of 66 × 10 3  m 3  s −1 . Channel and levee facies on the submarine flanks of the volcano and formation of a thick, steep-sided ridge, suggest that the largest and most dense blocks were transported proximally as a high concentration granular flow. Of the submerged volume, 30% was deposited from the base of this granular flow, forming a linear, high-relief ridge that extends 7 km from shore. The remaining 70% of the submerged volume comprises the finer grain sizes, which were transported at least 40 km by turbidity currents on gradients of &lt;2°. At several localities, the May 2006 distal turbidity currents ran up 200 m of topography and eroded up to 20 cm of underlying substrate. Multiple turbidites are preserved, representing current reflection from the graben margins and deflection around topography. The high energy of the May 2006 collapse resulted in longer submarine run out than the larger (210 × 10 6  m 3 ) Soufrière Hills dome collapse in July 2003.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer-Verlag</pub><doi>10.1007/s00445-011-0533-5</doi><tpages>15</tpages><orcidid>https://orcid.org/0000-0003-3689-3704</orcidid><orcidid>https://orcid.org/0000-0001-8901-2515</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0258-8900
ispartof Bulletin of volcanology, 2012-03, Vol.74 (2), p.391-405
issn 0258-8900
1432-0819
language eng
recordid cdi_hal_primary_oai_HAL_insu_03583366v1
source SpringerLink Journals - AutoHoldings
subjects Bathymetry
Crystalline rocks
Earth and Environmental Science
Earth Sciences
Earth, ocean, space
Engineering and environment geology. Geothermics
Exact sciences and technology
Geology
Geophysics
Geophysics/Geodesy
Hills
Igneous and metamorphic rocks petrology, volcanic processes, magmas
Lava
Lava domes
Mineralogy
Natural hazards: prediction, damages, etc
Research Article
Sciences of the Universe
Sedimentology
Topography
Turbidity
Turbidity currents
Volcanoes
Volcanology
title Submarine pyroclastic deposits formed during the 20th May 2006 dome collapse of the Soufrière Hills Volcano, Montserrat
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-03T14%3A54%3A46IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_hal_p&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Submarine%20pyroclastic%20deposits%20formed%20during%20the%2020th%20May%202006%20dome%20collapse%20of%20the%20Soufri%C3%A8re%20Hills%20Volcano,%20Montserrat&rft.jtitle=Bulletin%20of%20volcanology&rft.au=Trofimovs,%20J.&rft.date=2012-03&rft.volume=74&rft.issue=2&rft.spage=391&rft.epage=405&rft.pages=391-405&rft.issn=0258-8900&rft.eissn=1432-0819&rft.coden=BUVOEW&rft_id=info:doi/10.1007/s00445-011-0533-5&rft_dat=%3Cproquest_hal_p%3E2590747491%3C/proquest_hal_p%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=922363707&rft_id=info:pmid/&rfr_iscdi=true