Crystals reveal magma convection and melt transport in dyke-fed eruptions
The processes and ranges of intensive variables that control magma transport and dyke propagation through the crust are poorly understood. Here we show that textural and compositional data of olivine crystals (Mg/Fe, Ni and P) from the tephra of the first months of Paricutin volcano monogenetic erup...
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description | The processes and ranges of intensive variables that control magma transport and dyke propagation through the crust are poorly understood. Here we show that textural and compositional data of olivine crystals (Mg/Fe, Ni and P) from the tephra of the first months of Paricutin volcano monogenetic eruption (Mexico, 1943–1952) record fast growth and large temperature and oxygen fugacity gradients. We interpret that these gradients are due to convective magma transport in a propagating dyke to the Earth’s surface in less than a few days. The shortest time we have obtained is 0.1 day, and more than 50% of the calculated timescales are |
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−1
. The olivine zoning patterns change with the eruptive stratigraphy, and record a transition towards a more steady magma flow before the transition from explosive to effusive dynamics. Our results can inform numerical and experimental analogue models of dyke propagation, and thus facilitate a better understanding of the seismicity and other precursors of dyke-fed eruptions.</description><identifier>ISSN: 2045-2322</identifier><identifier>EISSN: 2045-2322</identifier><identifier>DOI: 10.1038/s41598-020-68421-4</identifier><identifier>PMID: 32669582</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>704/2151/209 ; 704/2151/431 ; 704/2151/598 ; Convection ; Crystals ; Earth Sciences ; Eruptions ; Humanities and Social Sciences ; Lava ; Magma ; multidisciplinary ; Science ; Science (multidisciplinary) ; Sciences of the Universe ; Stratigraphy ; Volcanic eruptions ; Volcanoes ; Volcanology</subject><ispartof>Scientific reports, 2020-07, Vol.10 (1), p.11632-11632, Article 11632</ispartof><rights>The Author(s) 2020</rights><rights>The Author(s) 2020. This work 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><rights>Attribution</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a547t-d307b79ae27c30fc6670ba65675ea680dffc20a0994fa4d729871c90ba6779d53</citedby><cites>FETCH-LOGICAL-a547t-d307b79ae27c30fc6670ba65675ea680dffc20a0994fa4d729871c90ba6779d53</cites><orcidid>0000-0002-1409-5325</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.ncbi.nlm.nih.gov/pmc/articles/PMC7363826/pdf/$$EPDF$$P50$$Gpubmedcentral$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.ncbi.nlm.nih.gov/pmc/articles/PMC7363826/$$EHTML$$P50$$Gpubmedcentral$$Hfree_for_read</linktohtml><link.rule.ids>230,314,725,778,782,862,883,27907,27908,41103,42172,51559,53774,53776</link.rule.ids><backlink>$$Uhttps://hal.science/hal-03899778$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Albert, Helena</creatorcontrib><creatorcontrib>Larrea, Patricia</creatorcontrib><creatorcontrib>Costa, Fidel</creatorcontrib><creatorcontrib>Widom, Elisabeth</creatorcontrib><creatorcontrib>Siebe, Claus</creatorcontrib><title>Crystals reveal magma convection and melt transport in dyke-fed eruptions</title><title>Scientific reports</title><addtitle>Sci Rep</addtitle><description>The processes and ranges of intensive variables that control magma transport and dyke propagation through the crust are poorly understood. Here we show that textural and compositional data of olivine crystals (Mg/Fe, Ni and P) from the tephra of the first months of Paricutin volcano monogenetic eruption (Mexico, 1943–1952) record fast growth and large temperature and oxygen fugacity gradients. We interpret that these gradients are due to convective magma transport in a propagating dyke to the Earth’s surface in less than a few days. The shortest time we have obtained is 0.1 day, and more than 50% of the calculated timescales are < 2 days for the earliest erupted tephra, which implies magma ascent rates of about 0.1 and 1 m s
−1
. The olivine zoning patterns change with the eruptive stratigraphy, and record a transition towards a more steady magma flow before the transition from explosive to effusive dynamics. Our results can inform numerical and experimental analogue models of dyke propagation, and thus facilitate a better understanding of the seismicity and other precursors of dyke-fed eruptions.</description><subject>704/2151/209</subject><subject>704/2151/431</subject><subject>704/2151/598</subject><subject>Convection</subject><subject>Crystals</subject><subject>Earth Sciences</subject><subject>Eruptions</subject><subject>Humanities and Social Sciences</subject><subject>Lava</subject><subject>Magma</subject><subject>multidisciplinary</subject><subject>Science</subject><subject>Science (multidisciplinary)</subject><subject>Sciences of the Universe</subject><subject>Stratigraphy</subject><subject>Volcanic eruptions</subject><subject>Volcanoes</subject><subject>Volcanology</subject><issn>2045-2322</issn><issn>2045-2322</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNp9kU9r3DAQxUVpyC5JvkBOgl7ag1NZf61LYVnaJrCQS3IWWnm8cWpLW8le2G8fOQ5tuofqMkLze0_DPISuS3JTElZ9TbwUuioIJYWsOC0L_gEtKeGioIzSj-_uC3SV0jPJR1DNS32OFoxKqUVFl-huHY9psF3CEQ5gO9zbXW-xC_4AbmiDx9bXuIduwEO0Pu1DHHDrcX38BUUDNYY47icuXaKzJvvA1Vu9QI8_vj-sb4vN_c-79WpTWMHVUNSMqK3SFqhyjDROSkW2VgqpBFhZkbppHCWWaM0by2tFdaVKpydGKV0LdoG-zb77cdtD7cDnwTqzj21v49EE25p_O759MrtwMIpJVlGZDb7MBk8nstvVxkxveb1aK1Udysx-fvssht8jpMH0bXLQddZDGJOhnHLOBeMT-ukEfQ5j9HkVE8W0JJyQTNGZcjGkFKH5M0FJzBSsmYM1OVjzGqzhWcRmUcqw30H8a_0f1Qs47KOl</recordid><startdate>20200715</startdate><enddate>20200715</enddate><creator>Albert, Helena</creator><creator>Larrea, Patricia</creator><creator>Costa, Fidel</creator><creator>Widom, Elisabeth</creator><creator>Siebe, Claus</creator><general>Nature Publishing Group UK</general><general>Nature Publishing Group</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7X7</scope><scope>7XB</scope><scope>88A</scope><scope>88E</scope><scope>88I</scope><scope>8FE</scope><scope>8FH</scope><scope>8FI</scope><scope>8FJ</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BBNVY</scope><scope>BENPR</scope><scope>BHPHI</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>FYUFA</scope><scope>GHDGH</scope><scope>GNUQQ</scope><scope>HCIFZ</scope><scope>K9.</scope><scope>LK8</scope><scope>M0S</scope><scope>M1P</scope><scope>M2P</scope><scope>M7P</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope><scope>7X8</scope><scope>1XC</scope><scope>VOOES</scope><scope>5PM</scope><orcidid>https://orcid.org/0000-0002-1409-5325</orcidid></search><sort><creationdate>20200715</creationdate><title>Crystals reveal magma convection and melt transport in dyke-fed eruptions</title><author>Albert, Helena ; Larrea, Patricia ; Costa, Fidel ; Widom, Elisabeth ; Siebe, Claus</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a547t-d307b79ae27c30fc6670ba65675ea680dffc20a0994fa4d729871c90ba6779d53</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>704/2151/209</topic><topic>704/2151/431</topic><topic>704/2151/598</topic><topic>Convection</topic><topic>Crystals</topic><topic>Earth Sciences</topic><topic>Eruptions</topic><topic>Humanities and Social Sciences</topic><topic>Lava</topic><topic>Magma</topic><topic>multidisciplinary</topic><topic>Science</topic><topic>Science (multidisciplinary)</topic><topic>Sciences of the Universe</topic><topic>Stratigraphy</topic><topic>Volcanic eruptions</topic><topic>Volcanoes</topic><topic>Volcanology</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Albert, Helena</creatorcontrib><creatorcontrib>Larrea, Patricia</creatorcontrib><creatorcontrib>Costa, Fidel</creatorcontrib><creatorcontrib>Widom, Elisabeth</creatorcontrib><creatorcontrib>Siebe, Claus</creatorcontrib><collection>Springer Nature OA Free Journals</collection><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Health & Medical Collection</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Biology Database (Alumni Edition)</collection><collection>Medical Database (Alumni Edition)</collection><collection>Science Database (Alumni Edition)</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Natural Science Collection</collection><collection>Hospital Premium Collection</collection><collection>Hospital Premium Collection (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>Biological Science Collection</collection><collection>ProQuest Central</collection><collection>Natural Science Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>Health Research Premium Collection</collection><collection>Health Research Premium Collection (Alumni)</collection><collection>ProQuest Central Student</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Health & Medical Complete (Alumni)</collection><collection>ProQuest Biological Science Collection</collection><collection>Health & Medical Collection (Alumni Edition)</collection><collection>Medical Database</collection><collection>Science Database</collection><collection>Biological Science Database</collection><collection>Publicly Available Content 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>MEDLINE - Academic</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><collection>PubMed Central (Full Participant titles)</collection><jtitle>Scientific reports</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Albert, Helena</au><au>Larrea, Patricia</au><au>Costa, Fidel</au><au>Widom, Elisabeth</au><au>Siebe, Claus</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Crystals reveal magma convection and melt transport in dyke-fed eruptions</atitle><jtitle>Scientific reports</jtitle><stitle>Sci Rep</stitle><date>2020-07-15</date><risdate>2020</risdate><volume>10</volume><issue>1</issue><spage>11632</spage><epage>11632</epage><pages>11632-11632</pages><artnum>11632</artnum><issn>2045-2322</issn><eissn>2045-2322</eissn><abstract>The processes and ranges of intensive variables that control magma transport and dyke propagation through the crust are poorly understood. Here we show that textural and compositional data of olivine crystals (Mg/Fe, Ni and P) from the tephra of the first months of Paricutin volcano monogenetic eruption (Mexico, 1943–1952) record fast growth and large temperature and oxygen fugacity gradients. We interpret that these gradients are due to convective magma transport in a propagating dyke to the Earth’s surface in less than a few days. The shortest time we have obtained is 0.1 day, and more than 50% of the calculated timescales are < 2 days for the earliest erupted tephra, which implies magma ascent rates of about 0.1 and 1 m s
−1
. The olivine zoning patterns change with the eruptive stratigraphy, and record a transition towards a more steady magma flow before the transition from explosive to effusive dynamics. Our results can inform numerical and experimental analogue models of dyke propagation, and thus facilitate a better understanding of the seismicity and other precursors of dyke-fed eruptions.</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><pmid>32669582</pmid><doi>10.1038/s41598-020-68421-4</doi><tpages>1</tpages><orcidid>https://orcid.org/0000-0002-1409-5325</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | 704/2151/209 704/2151/431 704/2151/598 Convection Crystals Earth Sciences Eruptions Humanities and Social Sciences Lava Magma multidisciplinary Science Science (multidisciplinary) Sciences of the Universe Stratigraphy Volcanic eruptions Volcanoes Volcanology |
title | Crystals reveal magma convection and melt transport in dyke-fed eruptions |
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