Geometric and kinematic features of the dike complex at Mt. Somma, Vesuvio (Italy)

Dikes provide important information on the structure, state of stress and activity of a volcano. Mt. Somma borders part of the Vesuvio cone (Italy), displaying ∼ 100 dikes emplaced between ∼ 18 and 30 ka. Field, AMS (anisotropy of magnetic susceptibility) and thin section analyses are used to charac...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Earth and planetary science letters 2006-05, Vol.245 (1), p.389-407
Hauptverfasser: Porreca, M., Acocella, V., Massimi, E., Mattei, M., Funiciello, R., De Benedetti, A.A.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 407
container_issue 1
container_start_page 389
container_title Earth and planetary science letters
container_volume 245
creator Porreca, M.
Acocella, V.
Massimi, E.
Mattei, M.
Funiciello, R.
De Benedetti, A.A.
description Dikes provide important information on the structure, state of stress and activity of a volcano. Mt. Somma borders part of the Vesuvio cone (Italy), displaying ∼ 100 dikes emplaced between ∼ 18 and 30 ka. Field, AMS (anisotropy of magnetic susceptibility) and thin section analyses are used to characterize their geometry and kinematics (direction and sense of flow). The dikes mostly have a NNW–SSE to NE–SW strike. Approximately 57% are radial to the older Somma edifice, ∼ 27% are oblique and ∼ 16% tangential. Among the latter two groups, ∼ 32% are outward dipping and ∼ 11% inward dipping. The dike thickness varies between 0.2 and 3 m, with a mean value of 1.17 m. The kinematics of 19 dikes is determined through a combination of field (8 dikes), AMS (16 dikes) and thin section analyses (15 dikes). Thirteen dikes have a vertical upward flow, whereas six have an oblique-subhorizontal flow, suggesting a lateral propagation from the summit or eccentric vents of the former Somma edifice. These propagation paths differ from those deducible from the recent activity, as all the seven major fissure eruptions between 1631 and 1944 were related to the lateral propagation of radial dikes. We propose that these different behaviours in dike propagation may be mainly related to the opening conditions of the summit conduit. The laterally propagating dikes in 1631–1944 formed with an open conduit. Conversely, the vertically propagating dikes may have formed, between 18 and 30 ka, with a closed conduit.
doi_str_mv 10.1016/j.epsl.2006.02.027
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_28922821</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>S0012821X06001671</els_id><sourcerecordid>1082182216</sourcerecordid><originalsourceid>FETCH-LOGICAL-a418t-26dabc4baa04aa59bff2bdc7debce8e43d125d64e66b1bda5a54b912fbe0ac463</originalsourceid><addsrcrecordid>eNqNkVtLAzEQhYMoWC9_wKc8iYK7Junudhd8kaK1oAje6FuYJLOYutvUJBX7702pzyIMDAPfOcPMIeSEs5wzXl3Oc1yGLheMVTkTqUY7ZMCHdZkxPpztkgFjXGS14LN9chDCnCWwrJoBeZqg6zF6qyksDP2wC-whpqlFiCuPgbqWxnekxn4g1a5fdvhNIdKHmNNn1_dwQd8wrL6so2fTCN36_IjstdAFPP7th-T19uZlfJfdP06m4-v7DApex0xUBpQuFAArAMpGta1QRo8MKo01FkPDRWmqAqtKcWWghLJQDRetQga6qIaH5HTru_Tuc4Uhyt4GjV0HC3SrIEXdCJFO_gfIeM3KJoFnf4KcJbtaCL5ZLrao9i4Ej61cetuDXydIbiKRc7mJRG4ikUykGiXR1VaE6S1fFr0M2uJCo7EedZTG2b_kP75IlU8</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1082182216</pqid></control><display><type>article</type><title>Geometric and kinematic features of the dike complex at Mt. Somma, Vesuvio (Italy)</title><source>ScienceDirect Journals (5 years ago - present)</source><creator>Porreca, M. ; Acocella, V. ; Massimi, E. ; Mattei, M. ; Funiciello, R. ; De Benedetti, A.A.</creator><creatorcontrib>Porreca, M. ; Acocella, V. ; Massimi, E. ; Mattei, M. ; Funiciello, R. ; De Benedetti, A.A.</creatorcontrib><description>Dikes provide important information on the structure, state of stress and activity of a volcano. Mt. Somma borders part of the Vesuvio cone (Italy), displaying ∼ 100 dikes emplaced between ∼ 18 and 30 ka. Field, AMS (anisotropy of magnetic susceptibility) and thin section analyses are used to characterize their geometry and kinematics (direction and sense of flow). The dikes mostly have a NNW–SSE to NE–SW strike. Approximately 57% are radial to the older Somma edifice, ∼ 27% are oblique and ∼ 16% tangential. Among the latter two groups, ∼ 32% are outward dipping and ∼ 11% inward dipping. The dike thickness varies between 0.2 and 3 m, with a mean value of 1.17 m. The kinematics of 19 dikes is determined through a combination of field (8 dikes), AMS (16 dikes) and thin section analyses (15 dikes). Thirteen dikes have a vertical upward flow, whereas six have an oblique-subhorizontal flow, suggesting a lateral propagation from the summit or eccentric vents of the former Somma edifice. These propagation paths differ from those deducible from the recent activity, as all the seven major fissure eruptions between 1631 and 1944 were related to the lateral propagation of radial dikes. We propose that these different behaviours in dike propagation may be mainly related to the opening conditions of the summit conduit. The laterally propagating dikes in 1631–1944 formed with an open conduit. Conversely, the vertically propagating dikes may have formed, between 18 and 30 ka, with a closed conduit.</description><identifier>ISSN: 0012-821X</identifier><identifier>EISSN: 1385-013X</identifier><identifier>DOI: 10.1016/j.epsl.2006.02.027</identifier><language>eng</language><publisher>Elsevier B.V</publisher><subject>AMS ; Borders ; Conduits ; Dikes ; Dipping ; Kinematics ; Magnetic permeability ; Propagation ; Strikes ; Vesuvio ; volcanoes</subject><ispartof>Earth and planetary science letters, 2006-05, Vol.245 (1), p.389-407</ispartof><rights>2006 Elsevier B.V.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a418t-26dabc4baa04aa59bff2bdc7debce8e43d125d64e66b1bda5a54b912fbe0ac463</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/j.epsl.2006.02.027$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,780,784,3550,27924,27925,45995</link.rule.ids></links><search><creatorcontrib>Porreca, M.</creatorcontrib><creatorcontrib>Acocella, V.</creatorcontrib><creatorcontrib>Massimi, E.</creatorcontrib><creatorcontrib>Mattei, M.</creatorcontrib><creatorcontrib>Funiciello, R.</creatorcontrib><creatorcontrib>De Benedetti, A.A.</creatorcontrib><title>Geometric and kinematic features of the dike complex at Mt. Somma, Vesuvio (Italy)</title><title>Earth and planetary science letters</title><description>Dikes provide important information on the structure, state of stress and activity of a volcano. Mt. Somma borders part of the Vesuvio cone (Italy), displaying ∼ 100 dikes emplaced between ∼ 18 and 30 ka. Field, AMS (anisotropy of magnetic susceptibility) and thin section analyses are used to characterize their geometry and kinematics (direction and sense of flow). The dikes mostly have a NNW–SSE to NE–SW strike. Approximately 57% are radial to the older Somma edifice, ∼ 27% are oblique and ∼ 16% tangential. Among the latter two groups, ∼ 32% are outward dipping and ∼ 11% inward dipping. The dike thickness varies between 0.2 and 3 m, with a mean value of 1.17 m. The kinematics of 19 dikes is determined through a combination of field (8 dikes), AMS (16 dikes) and thin section analyses (15 dikes). Thirteen dikes have a vertical upward flow, whereas six have an oblique-subhorizontal flow, suggesting a lateral propagation from the summit or eccentric vents of the former Somma edifice. These propagation paths differ from those deducible from the recent activity, as all the seven major fissure eruptions between 1631 and 1944 were related to the lateral propagation of radial dikes. We propose that these different behaviours in dike propagation may be mainly related to the opening conditions of the summit conduit. The laterally propagating dikes in 1631–1944 formed with an open conduit. Conversely, the vertically propagating dikes may have formed, between 18 and 30 ka, with a closed conduit.</description><subject>AMS</subject><subject>Borders</subject><subject>Conduits</subject><subject>Dikes</subject><subject>Dipping</subject><subject>Kinematics</subject><subject>Magnetic permeability</subject><subject>Propagation</subject><subject>Strikes</subject><subject>Vesuvio</subject><subject>volcanoes</subject><issn>0012-821X</issn><issn>1385-013X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNqNkVtLAzEQhYMoWC9_wKc8iYK7Junudhd8kaK1oAje6FuYJLOYutvUJBX7702pzyIMDAPfOcPMIeSEs5wzXl3Oc1yGLheMVTkTqUY7ZMCHdZkxPpztkgFjXGS14LN9chDCnCWwrJoBeZqg6zF6qyksDP2wC-whpqlFiCuPgbqWxnekxn4g1a5fdvhNIdKHmNNn1_dwQd8wrL6so2fTCN36_IjstdAFPP7th-T19uZlfJfdP06m4-v7DApex0xUBpQuFAArAMpGta1QRo8MKo01FkPDRWmqAqtKcWWghLJQDRetQga6qIaH5HTru_Tuc4Uhyt4GjV0HC3SrIEXdCJFO_gfIeM3KJoFnf4KcJbtaCL5ZLrao9i4Ej61cetuDXydIbiKRc7mJRG4ikUykGiXR1VaE6S1fFr0M2uJCo7EedZTG2b_kP75IlU8</recordid><startdate>20060515</startdate><enddate>20060515</enddate><creator>Porreca, M.</creator><creator>Acocella, V.</creator><creator>Massimi, E.</creator><creator>Mattei, M.</creator><creator>Funiciello, R.</creator><creator>De Benedetti, A.A.</creator><general>Elsevier B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7U5</scope></search><sort><creationdate>20060515</creationdate><title>Geometric and kinematic features of the dike complex at Mt. Somma, Vesuvio (Italy)</title><author>Porreca, M. ; Acocella, V. ; Massimi, E. ; Mattei, M. ; Funiciello, R. ; De Benedetti, A.A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a418t-26dabc4baa04aa59bff2bdc7debce8e43d125d64e66b1bda5a54b912fbe0ac463</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>AMS</topic><topic>Borders</topic><topic>Conduits</topic><topic>Dikes</topic><topic>Dipping</topic><topic>Kinematics</topic><topic>Magnetic permeability</topic><topic>Propagation</topic><topic>Strikes</topic><topic>Vesuvio</topic><topic>volcanoes</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Porreca, M.</creatorcontrib><creatorcontrib>Acocella, V.</creatorcontrib><creatorcontrib>Massimi, E.</creatorcontrib><creatorcontrib>Mattei, M.</creatorcontrib><creatorcontrib>Funiciello, R.</creatorcontrib><creatorcontrib>De Benedetti, A.A.</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Solid State and Superconductivity Abstracts</collection><jtitle>Earth and planetary science letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Porreca, M.</au><au>Acocella, V.</au><au>Massimi, E.</au><au>Mattei, M.</au><au>Funiciello, R.</au><au>De Benedetti, A.A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Geometric and kinematic features of the dike complex at Mt. Somma, Vesuvio (Italy)</atitle><jtitle>Earth and planetary science letters</jtitle><date>2006-05-15</date><risdate>2006</risdate><volume>245</volume><issue>1</issue><spage>389</spage><epage>407</epage><pages>389-407</pages><issn>0012-821X</issn><eissn>1385-013X</eissn><abstract>Dikes provide important information on the structure, state of stress and activity of a volcano. Mt. Somma borders part of the Vesuvio cone (Italy), displaying ∼ 100 dikes emplaced between ∼ 18 and 30 ka. Field, AMS (anisotropy of magnetic susceptibility) and thin section analyses are used to characterize their geometry and kinematics (direction and sense of flow). The dikes mostly have a NNW–SSE to NE–SW strike. Approximately 57% are radial to the older Somma edifice, ∼ 27% are oblique and ∼ 16% tangential. Among the latter two groups, ∼ 32% are outward dipping and ∼ 11% inward dipping. The dike thickness varies between 0.2 and 3 m, with a mean value of 1.17 m. The kinematics of 19 dikes is determined through a combination of field (8 dikes), AMS (16 dikes) and thin section analyses (15 dikes). Thirteen dikes have a vertical upward flow, whereas six have an oblique-subhorizontal flow, suggesting a lateral propagation from the summit or eccentric vents of the former Somma edifice. These propagation paths differ from those deducible from the recent activity, as all the seven major fissure eruptions between 1631 and 1944 were related to the lateral propagation of radial dikes. We propose that these different behaviours in dike propagation may be mainly related to the opening conditions of the summit conduit. The laterally propagating dikes in 1631–1944 formed with an open conduit. Conversely, the vertically propagating dikes may have formed, between 18 and 30 ka, with a closed conduit.</abstract><pub>Elsevier B.V</pub><doi>10.1016/j.epsl.2006.02.027</doi><tpages>19</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0012-821X
ispartof Earth and planetary science letters, 2006-05, Vol.245 (1), p.389-407
issn 0012-821X
1385-013X
language eng
recordid cdi_proquest_miscellaneous_28922821
source ScienceDirect Journals (5 years ago - present)
subjects AMS
Borders
Conduits
Dikes
Dipping
Kinematics
Magnetic permeability
Propagation
Strikes
Vesuvio
volcanoes
title Geometric and kinematic features of the dike complex at Mt. Somma, Vesuvio (Italy)
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-06T18%3A39%3A04IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Geometric%20and%20kinematic%20features%20of%20the%20dike%20complex%20at%20Mt.%20Somma,%20Vesuvio%20(Italy)&rft.jtitle=Earth%20and%20planetary%20science%20letters&rft.au=Porreca,%20M.&rft.date=2006-05-15&rft.volume=245&rft.issue=1&rft.spage=389&rft.epage=407&rft.pages=389-407&rft.issn=0012-821X&rft.eissn=1385-013X&rft_id=info:doi/10.1016/j.epsl.2006.02.027&rft_dat=%3Cproquest_cross%3E1082182216%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1082182216&rft_id=info:pmid/&rft_els_id=S0012821X06001671&rfr_iscdi=true