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Analysis of the Spatiotemporal Evolution of the Maurienne Swarm (French Alps) Based on Earthquake Clustering
Between August 2017 and March 2019, an intense seismic swarm was recorded in the Maurienne valley in the north of the Belledonne massif (Western French Alps). In order to study the spatiotemporal evolution of the Maurienne swarm, we created a high‐resolution catalog based on template matching, doubl...
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Published in: | Earth and space science (Hoboken, N.J.) N.J.), 2022-07, Vol.9 (7), p.n/a |
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creator | Minetto, Riccardo Helmstetter, Agnès Schwartz, Stéphane Langlais, Mickaël Nomade, Jérôme Guéguen, Philippe |
description | Between August 2017 and March 2019, an intense seismic swarm was recorded in the Maurienne valley in the north of the Belledonne massif (Western French Alps). In order to study the spatiotemporal evolution of the Maurienne swarm, we created a high‐resolution catalog based on template matching, double‐difference relocation, and moment magnitudes. The catalog includes 71,064 events with a maximum moment magnitude of 3.5 and a magnitude of completeness of 0.7. The seismic activity is interpreted as the reactivation of an N80 strike‐slip fault system called Fond de France. Moreover, earthquake relocation reveals the presence of a shallower fault system with the same strike, but opposite dip direction and smaller size. The presence of two distinct fault systems may explain the observed variation of the b‐value with depth. The seismicity migrated asymmetrically in all directions during the course of about 15 months. Shorter migrations lasting 2–3 days are also observed. The different migration patterns suggest that the swarm is driven by several mechanisms, possibly pore‐pressure diffusion, aseismic slip, and earthquake interactions.
Key Points
We use template matching, double‐difference relocations, and moment magnitudes to create a high‐resolution catalog of the Maurienne swarm
At least two conjugate fault systems with opposite dip directions were reactivated during the swarm
The complex migration of seismicity suggests that the swarm may be driven both by pore‐pressure diffusion and by earthquake interactions |
doi_str_mv | 10.1029/2021EA002097 |
format | article |
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Key Points
We use template matching, double‐difference relocations, and moment magnitudes to create a high‐resolution catalog of the Maurienne swarm
At least two conjugate fault systems with opposite dip directions were reactivated during the swarm
The complex migration of seismicity suggests that the swarm may be driven both by pore‐pressure diffusion and by earthquake interactions</description><identifier>ISSN: 2333-5084</identifier><identifier>EISSN: 2333-5084</identifier><identifier>DOI: 10.1029/2021EA002097</identifier><language>eng</language><publisher>Hoboken: John Wiley & Sons, Inc</publisher><subject>Earth Sciences ; Earthquakes ; Fault lines ; Geology ; Relocation ; Sciences of the Universe ; Seismic activity ; Tectonics</subject><ispartof>Earth and space science (Hoboken, N.J.), 2022-07, Vol.9 (7), p.n/a</ispartof><rights>2022 The Authors. Earth and Space Science published by Wiley Periodicals LLC on behalf of American Geophysical Union.</rights><rights>2022. 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>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-a5065-6750f1b4b9c02651b6ee1e1deb07243a9aeadd95550bb13a682d57754e099a1b3</citedby><cites>FETCH-LOGICAL-a5065-6750f1b4b9c02651b6ee1e1deb07243a9aeadd95550bb13a682d57754e099a1b3</cites><orcidid>0000-0003-3072-4635 ; 0000-0001-7942-7071 ; 0000-0002-6797-5190 ; 0000-0003-0597-8289 ; 0000-0003-2211-5960 ; 0000-0001-6362-0694</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/2695507441/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/2695507441?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>230,314,780,784,885,11562,25753,27924,27925,37012,44590,46052,46476,75126</link.rule.ids><backlink>$$Uhttps://hal.science/hal-03753320$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Minetto, Riccardo</creatorcontrib><creatorcontrib>Helmstetter, Agnès</creatorcontrib><creatorcontrib>Schwartz, Stéphane</creatorcontrib><creatorcontrib>Langlais, Mickaël</creatorcontrib><creatorcontrib>Nomade, Jérôme</creatorcontrib><creatorcontrib>Guéguen, Philippe</creatorcontrib><title>Analysis of the Spatiotemporal Evolution of the Maurienne Swarm (French Alps) Based on Earthquake Clustering</title><title>Earth and space science (Hoboken, N.J.)</title><description>Between August 2017 and March 2019, an intense seismic swarm was recorded in the Maurienne valley in the north of the Belledonne massif (Western French Alps). In order to study the spatiotemporal evolution of the Maurienne swarm, we created a high‐resolution catalog based on template matching, double‐difference relocation, and moment magnitudes. The catalog includes 71,064 events with a maximum moment magnitude of 3.5 and a magnitude of completeness of 0.7. The seismic activity is interpreted as the reactivation of an N80 strike‐slip fault system called Fond de France. Moreover, earthquake relocation reveals the presence of a shallower fault system with the same strike, but opposite dip direction and smaller size. The presence of two distinct fault systems may explain the observed variation of the b‐value with depth. The seismicity migrated asymmetrically in all directions during the course of about 15 months. Shorter migrations lasting 2–3 days are also observed. The different migration patterns suggest that the swarm is driven by several mechanisms, possibly pore‐pressure diffusion, aseismic slip, and earthquake interactions.
Key Points
We use template matching, double‐difference relocations, and moment magnitudes to create a high‐resolution catalog of the Maurienne swarm
At least two conjugate fault systems with opposite dip directions were reactivated during the swarm
The complex migration of seismicity suggests that the swarm may be driven both by pore‐pressure diffusion and by earthquake interactions</description><subject>Earth Sciences</subject><subject>Earthquakes</subject><subject>Fault lines</subject><subject>Geology</subject><subject>Relocation</subject><subject>Sciences of the Universe</subject><subject>Seismic activity</subject><subject>Tectonics</subject><issn>2333-5084</issn><issn>2333-5084</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>24P</sourceid><sourceid>PIMPY</sourceid><sourceid>DOA</sourceid><recordid>eNp9kU1r3DAQhk1ooSHJLT9AkEsD3XT0Za-P7uI0gS09bHMWY3uc9VZrOZKdsP8-2rot6aW6jHjn4WGYSZJLDjccRP5ZgOBlASAgz06SUyGlXGhYqndv_h-SixB2AMCFTkGo08QWPdpD6AJzLRu3xDYDjp0baT84j5aVz85OMej_9L_h5Dvq-0i-oN-zj7ee-nrLCjuEa_YFAzUs0iX6cfs04U9iKzuFkXzXP54n71u0gS5-17Pk4bb8sbpbrL9_vV8V6wVqSPUizTS0vFJVXoNINa9SIk68oQoyoSTmSNg0udYaqopLTJei0VmmFUGeI6_kWXI_exuHOzP4bo_-YBx25lfg_KOJ43W1JUOka6EahQq5ylFXIqvkEjS2gtr4out6dm3R_qO6K9bmmIHMtJQCnnlkr2Z28O5pojCanZt8XHAwIo3zQqbUkfo0U7V3IXhq_2o5mOMpzdtTRlzM-Etn6fBf1pSbjeCCa_kKCCGddw</recordid><startdate>202207</startdate><enddate>202207</enddate><creator>Minetto, Riccardo</creator><creator>Helmstetter, Agnès</creator><creator>Schwartz, Stéphane</creator><creator>Langlais, Mickaël</creator><creator>Nomade, Jérôme</creator><creator>Guéguen, Philippe</creator><general>John Wiley & Sons, Inc</general><general>American Geophysical Union/Wiley</general><general>American Geophysical Union (AGU)</general><scope>24P</scope><scope>WIN</scope><scope>AAYXX</scope><scope>CITATION</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>HCIFZ</scope><scope>PCBAR</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>1XC</scope><scope>VOOES</scope><scope>DOA</scope><orcidid>https://orcid.org/0000-0003-3072-4635</orcidid><orcidid>https://orcid.org/0000-0001-7942-7071</orcidid><orcidid>https://orcid.org/0000-0002-6797-5190</orcidid><orcidid>https://orcid.org/0000-0003-0597-8289</orcidid><orcidid>https://orcid.org/0000-0003-2211-5960</orcidid><orcidid>https://orcid.org/0000-0001-6362-0694</orcidid></search><sort><creationdate>202207</creationdate><title>Analysis of the Spatiotemporal Evolution of the Maurienne Swarm (French Alps) Based on Earthquake Clustering</title><author>Minetto, Riccardo ; Helmstetter, Agnès ; Schwartz, Stéphane ; Langlais, Mickaël ; Nomade, Jérôme ; Guéguen, Philippe</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a5065-6750f1b4b9c02651b6ee1e1deb07243a9aeadd95550bb13a682d57754e099a1b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Earth Sciences</topic><topic>Earthquakes</topic><topic>Fault lines</topic><topic>Geology</topic><topic>Relocation</topic><topic>Sciences of the Universe</topic><topic>Seismic activity</topic><topic>Tectonics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Minetto, Riccardo</creatorcontrib><creatorcontrib>Helmstetter, Agnès</creatorcontrib><creatorcontrib>Schwartz, Stéphane</creatorcontrib><creatorcontrib>Langlais, Mickaël</creatorcontrib><creatorcontrib>Nomade, Jérôme</creatorcontrib><creatorcontrib>Guéguen, Philippe</creatorcontrib><collection>Wiley-Blackwell Open Access Collection</collection><collection>Wiley Journals</collection><collection>CrossRef</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>Proquest Central</collection><collection>ProQuest Natural Science Collection</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>Earth, Atmospheric & Aquatic 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 China</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><collection>Directory of Open Access Journals</collection><jtitle>Earth and space science (Hoboken, N.J.)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Minetto, Riccardo</au><au>Helmstetter, Agnès</au><au>Schwartz, Stéphane</au><au>Langlais, Mickaël</au><au>Nomade, Jérôme</au><au>Guéguen, Philippe</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Analysis of the Spatiotemporal Evolution of the Maurienne Swarm (French Alps) Based on Earthquake Clustering</atitle><jtitle>Earth and space science (Hoboken, N.J.)</jtitle><date>2022-07</date><risdate>2022</risdate><volume>9</volume><issue>7</issue><epage>n/a</epage><issn>2333-5084</issn><eissn>2333-5084</eissn><abstract>Between August 2017 and March 2019, an intense seismic swarm was recorded in the Maurienne valley in the north of the Belledonne massif (Western French Alps). In order to study the spatiotemporal evolution of the Maurienne swarm, we created a high‐resolution catalog based on template matching, double‐difference relocation, and moment magnitudes. The catalog includes 71,064 events with a maximum moment magnitude of 3.5 and a magnitude of completeness of 0.7. The seismic activity is interpreted as the reactivation of an N80 strike‐slip fault system called Fond de France. Moreover, earthquake relocation reveals the presence of a shallower fault system with the same strike, but opposite dip direction and smaller size. The presence of two distinct fault systems may explain the observed variation of the b‐value with depth. The seismicity migrated asymmetrically in all directions during the course of about 15 months. Shorter migrations lasting 2–3 days are also observed. The different migration patterns suggest that the swarm is driven by several mechanisms, possibly pore‐pressure diffusion, aseismic slip, and earthquake interactions.
Key Points
We use template matching, double‐difference relocations, and moment magnitudes to create a high‐resolution catalog of the Maurienne swarm
At least two conjugate fault systems with opposite dip directions were reactivated during the swarm
The complex migration of seismicity suggests that the swarm may be driven both by pore‐pressure diffusion and by earthquake interactions</abstract><cop>Hoboken</cop><pub>John Wiley & Sons, Inc</pub><doi>10.1029/2021EA002097</doi><tpages>19</tpages><orcidid>https://orcid.org/0000-0003-3072-4635</orcidid><orcidid>https://orcid.org/0000-0001-7942-7071</orcidid><orcidid>https://orcid.org/0000-0002-6797-5190</orcidid><orcidid>https://orcid.org/0000-0003-0597-8289</orcidid><orcidid>https://orcid.org/0000-0003-2211-5960</orcidid><orcidid>https://orcid.org/0000-0001-6362-0694</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Earth Sciences Earthquakes Fault lines Geology Relocation Sciences of the Universe Seismic activity Tectonics |
title | Analysis of the Spatiotemporal Evolution of the Maurienne Swarm (French Alps) Based on Earthquake Clustering |
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