The Transcrustal Magma Reservoir Beneath Soufrière Hills Volcano, Montserrat: Insights From 3‐D Geodetic Inversions
We invert intraeruptive ground displacements recorded between 2003 and 2005 on Montserrat to shed light on the magmatic plumbing system of Soufrière Hills Volcano. Incorporating 3‐dimensional crustal mechanical and topographic data in a finite‐element model, we show that the recorded displacements a...
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Veröffentlicht in: | Geophysical research letters 2020-10, Vol.47 (20), p.n/a |
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description | We invert intraeruptive ground displacements recorded between 2003 and 2005 on Montserrat to shed light on the magmatic plumbing system of Soufrière Hills Volcano. Incorporating 3‐dimensional crustal mechanical and topographic data in a finite‐element model, we show that the recorded displacements are best explained by a southeastward dipping (plunge angle of 9.3°) vertically extended triaxial ellipsoidal pressure source with semiaxes lengths of 1.9 and 2.0 km horizontally, and 5.0 km vertically. The source is centered at 9.35 km depth below main sea level and embedded in independently imaged anomalously weak crustal rocks. The source orientation appears to be controlled by the local stress field at the intersection of two major WNW‐ESE and NW‐SE striking tectonic lineaments. We derive an average volumetric strain rate of 8.4 × 10−12 s−1 by transcrustal pressurization which may have contributed to flank instability and mass wasting events in the southern and eastern sectors of the island.
Key Points
First 3‐D numerical inversion of surface displacements for Soufrière Hills Volcano highlights strong volcano‐tectonic interactions
Surface strains are controlled by topography and crustal mechanical heterogeneity
Transcrustal magmatic system is imaged by SE‐ward dipping triaxial ellipsoid |
doi_str_mv | 10.1029/2020GL089239 |
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Key Points
First 3‐D numerical inversion of surface displacements for Soufrière Hills Volcano highlights strong volcano‐tectonic interactions
Surface strains are controlled by topography and crustal mechanical heterogeneity
Transcrustal magmatic system is imaged by SE‐ward dipping triaxial ellipsoid</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1029/2020GL089239</identifier><language>eng</language><publisher>Washington: John Wiley & Sons, Inc</publisher><subject>Hills ; Inversions ; Lava ; Magma ; Mass wasting ; Pressurization ; Sea level ; Strain rate ; Stress distribution ; Tectonics ; Volcanoes ; Volumetric strain</subject><ispartof>Geophysical research letters, 2020-10, Vol.47 (20), p.n/a</ispartof><rights>2020. The Authors.</rights><rights>2020. This article is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a3672-4af75127a2eb7d2992d0b8c6f7159fcc65a188333223f9a6fc408b7191b31cd83</citedby><cites>FETCH-LOGICAL-a3672-4af75127a2eb7d2992d0b8c6f7159fcc65a188333223f9a6fc408b7191b31cd83</cites><orcidid>0000-0001-9280-4011 ; 0000-0002-5391-3415</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F2020GL089239$$EPDF$$P50$$Gwiley$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2020GL089239$$EHTML$$P50$$Gwiley$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,1416,1432,11512,27922,27923,45572,45573,46407,46466,46831,46890</link.rule.ids></links><search><creatorcontrib>Gottsmann, J.</creatorcontrib><creatorcontrib>Flynn, M.</creatorcontrib><creatorcontrib>Hickey, J.</creatorcontrib><title>The Transcrustal Magma Reservoir Beneath Soufrière Hills Volcano, Montserrat: Insights From 3‐D Geodetic Inversions</title><title>Geophysical research letters</title><description>We invert intraeruptive ground displacements recorded between 2003 and 2005 on Montserrat to shed light on the magmatic plumbing system of Soufrière Hills Volcano. Incorporating 3‐dimensional crustal mechanical and topographic data in a finite‐element model, we show that the recorded displacements are best explained by a southeastward dipping (plunge angle of 9.3°) vertically extended triaxial ellipsoidal pressure source with semiaxes lengths of 1.9 and 2.0 km horizontally, and 5.0 km vertically. The source is centered at 9.35 km depth below main sea level and embedded in independently imaged anomalously weak crustal rocks. The source orientation appears to be controlled by the local stress field at the intersection of two major WNW‐ESE and NW‐SE striking tectonic lineaments. We derive an average volumetric strain rate of 8.4 × 10−12 s−1 by transcrustal pressurization which may have contributed to flank instability and mass wasting events in the southern and eastern sectors of the island.
Key Points
First 3‐D numerical inversion of surface displacements for Soufrière Hills Volcano highlights strong volcano‐tectonic interactions
Surface strains are controlled by topography and crustal mechanical heterogeneity
Transcrustal magmatic system is imaged by SE‐ward dipping triaxial ellipsoid</description><subject>Hills</subject><subject>Inversions</subject><subject>Lava</subject><subject>Magma</subject><subject>Mass wasting</subject><subject>Pressurization</subject><subject>Sea level</subject><subject>Strain rate</subject><subject>Stress distribution</subject><subject>Tectonics</subject><subject>Volcanoes</subject><subject>Volumetric strain</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>24P</sourceid><sourceid>WIN</sourceid><recordid>eNp90E1OwzAQBWALgUQp7DiAJbYNjO38mR0UmlZKhVQK28hx7DZVGhc7KeqOI3AM7sFNOAlBZcGK1Yw0n95ID6FzApcEKL-iQCFJIeaU8QPUI9z3vRggOkQ9AN7tNAqP0YlzKwBgwEgPbedLhedW1E7a1jWiwlOxWAs8U07ZrSktvlW1Es0SP5pW2_Lzwyo8LqvK4WdTSVGbAZ6auum0Fc01ntSuXCwbh0fWrDH7enu_w4kyhWpK2R23yrrS1O4UHWlROXX2O_voaXQ_H4699CGZDG9ST7Awop4vdBQQGgmq8qignNMC8liGOiIB11KGgSBxzBijlGkuQi19iPOIcJIzIouY9dHFPndjzUurXJOtTGvr7mVG_cAnPAiAdGqwV9Ia56zS2caWa2F3GYHsp9nsb7Mdp3v-WlZq96_NklkaEhpQ9g0dtXsi</recordid><startdate>20201028</startdate><enddate>20201028</enddate><creator>Gottsmann, J.</creator><creator>Flynn, M.</creator><creator>Hickey, J.</creator><general>John Wiley & Sons, Inc</general><scope>24P</scope><scope>WIN</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7TN</scope><scope>8FD</scope><scope>F1W</scope><scope>FR3</scope><scope>H8D</scope><scope>H96</scope><scope>KL.</scope><scope>KR7</scope><scope>L.G</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0001-9280-4011</orcidid><orcidid>https://orcid.org/0000-0002-5391-3415</orcidid></search><sort><creationdate>20201028</creationdate><title>The Transcrustal Magma Reservoir Beneath Soufrière Hills Volcano, Montserrat: Insights From 3‐D Geodetic Inversions</title><author>Gottsmann, J. ; Flynn, M. ; Hickey, J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a3672-4af75127a2eb7d2992d0b8c6f7159fcc65a188333223f9a6fc408b7191b31cd83</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Hills</topic><topic>Inversions</topic><topic>Lava</topic><topic>Magma</topic><topic>Mass wasting</topic><topic>Pressurization</topic><topic>Sea level</topic><topic>Strain rate</topic><topic>Stress distribution</topic><topic>Tectonics</topic><topic>Volcanoes</topic><topic>Volumetric strain</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gottsmann, J.</creatorcontrib><creatorcontrib>Flynn, M.</creatorcontrib><creatorcontrib>Hickey, J.</creatorcontrib><collection>Wiley Online Library Open Access</collection><collection>Wiley Free Content</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Oceanic Abstracts</collection><collection>Technology Research Database</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Civil Engineering Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gottsmann, J.</au><au>Flynn, M.</au><au>Hickey, J.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Transcrustal Magma Reservoir Beneath Soufrière Hills Volcano, Montserrat: Insights From 3‐D Geodetic Inversions</atitle><jtitle>Geophysical research letters</jtitle><date>2020-10-28</date><risdate>2020</risdate><volume>47</volume><issue>20</issue><epage>n/a</epage><issn>0094-8276</issn><eissn>1944-8007</eissn><abstract>We invert intraeruptive ground displacements recorded between 2003 and 2005 on Montserrat to shed light on the magmatic plumbing system of Soufrière Hills Volcano. Incorporating 3‐dimensional crustal mechanical and topographic data in a finite‐element model, we show that the recorded displacements are best explained by a southeastward dipping (plunge angle of 9.3°) vertically extended triaxial ellipsoidal pressure source with semiaxes lengths of 1.9 and 2.0 km horizontally, and 5.0 km vertically. The source is centered at 9.35 km depth below main sea level and embedded in independently imaged anomalously weak crustal rocks. The source orientation appears to be controlled by the local stress field at the intersection of two major WNW‐ESE and NW‐SE striking tectonic lineaments. We derive an average volumetric strain rate of 8.4 × 10−12 s−1 by transcrustal pressurization which may have contributed to flank instability and mass wasting events in the southern and eastern sectors of the island.
Key Points
First 3‐D numerical inversion of surface displacements for Soufrière Hills Volcano highlights strong volcano‐tectonic interactions
Surface strains are controlled by topography and crustal mechanical heterogeneity
Transcrustal magmatic system is imaged by SE‐ward dipping triaxial ellipsoid</abstract><cop>Washington</cop><pub>John Wiley & Sons, Inc</pub><doi>10.1029/2020GL089239</doi><tpages>10</tpages><orcidid>https://orcid.org/0000-0001-9280-4011</orcidid><orcidid>https://orcid.org/0000-0002-5391-3415</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Hills Inversions Lava Magma Mass wasting Pressurization Sea level Strain rate Stress distribution Tectonics Volcanoes Volumetric strain |
title | The Transcrustal Magma Reservoir Beneath Soufrière Hills Volcano, Montserrat: Insights From 3‐D Geodetic Inversions |
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