Joint inversion of receiver functions and surface wave dispersion in the Recôncavo–Tucano basin of NE Brazil: implications for basin formation
SUMMARY The crustal structure of the Recôncavo–Tucano basin, an aborted rift system that developed in NE Brazil during extension related to the opening of the South Atlantic Ocean, has been investigated through local constraints from receiver functions developed at 18 seismic stations in the region....
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Veröffentlicht in: | Geophysical journal international 2022-03, Vol.230 (1), p.317-333 |
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The crustal structure of the Recôncavo–Tucano basin, an aborted rift system that developed in NE Brazil during extension related to the opening of the South Atlantic Ocean, has been investigated through local constraints from receiver functions developed at 18 seismic stations in the region. Gravity modelling has proved unable to unequivocally localize crustal thinning under the basin depocentre and, together with a general lack of sediments from a putative thermal sag phase, this has led to a range of basin formation models invoking either pure or simple shear or a combination of both. In particular, the ‘flexural cantilever’ model has assumed simple shear extension in the upper crust and pure shear extension in the lower crust and mantle, enabling local erosion of the rift flanks after footwall uplift and regional erosion of the thermal sag phase after magmatic underplate of the basin's crust. Our results reveal that the crust is over 40 km thick beneath the Tucano and Recôncavo basins and that it contains a thick (5–8 km) layer of high velocity (Vs > 4.0 km s–1) material below ∼35 km depth. These observations contrast with structure immediately West (São Francisco Craton) and East (Borborema Province) of the basin, for which crustal thicknesses average 42 and 36 km, respectively, lower crustal velocities are below 4.0 km s–1, and local instances of crust as thin as 33.5 km are observed. We propose, in agreement with the ‘flexural cantilever’ model, that the fast velocity layer making the basin's lowermost crust resulted from mafic underplating after stretching and thinning during the syn-rift phase, restoring crustal thickness to pre-rift values (or larger) and providing the necessary buoyancy to trigger regional uplift. Moreover, although not pervasive, instances of thin crust along the footwall could be related to rift flank erosion. We thus conclude that, regardless of the mode of extension in the upper crust, our results favour models of basin formation invoking extension of the lower crust by pure shear. |
doi_str_mv | 10.1093/gji/ggac080 |
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The crustal structure of the Recôncavo–Tucano basin, an aborted rift system that developed in NE Brazil during extension related to the opening of the South Atlantic Ocean, has been investigated through local constraints from receiver functions developed at 18 seismic stations in the region. Gravity modelling has proved unable to unequivocally localize crustal thinning under the basin depocentre and, together with a general lack of sediments from a putative thermal sag phase, this has led to a range of basin formation models invoking either pure or simple shear or a combination of both. In particular, the ‘flexural cantilever’ model has assumed simple shear extension in the upper crust and pure shear extension in the lower crust and mantle, enabling local erosion of the rift flanks after footwall uplift and regional erosion of the thermal sag phase after magmatic underplate of the basin's crust. Our results reveal that the crust is over 40 km thick beneath the Tucano and Recôncavo basins and that it contains a thick (5–8 km) layer of high velocity (Vs > 4.0 km s–1) material below ∼35 km depth. These observations contrast with structure immediately West (São Francisco Craton) and East (Borborema Province) of the basin, for which crustal thicknesses average 42 and 36 km, respectively, lower crustal velocities are below 4.0 km s–1, and local instances of crust as thin as 33.5 km are observed. We propose, in agreement with the ‘flexural cantilever’ model, that the fast velocity layer making the basin's lowermost crust resulted from mafic underplating after stretching and thinning during the syn-rift phase, restoring crustal thickness to pre-rift values (or larger) and providing the necessary buoyancy to trigger regional uplift. Moreover, although not pervasive, instances of thin crust along the footwall could be related to rift flank erosion. We thus conclude that, regardless of the mode of extension in the upper crust, our results favour models of basin formation invoking extension of the lower crust by pure shear.</description><identifier>ISSN: 0956-540X</identifier><identifier>EISSN: 1365-246X</identifier><identifier>DOI: 10.1093/gji/ggac080</identifier><language>eng</language><publisher>Oxford University Press</publisher><subject>Sciences of the Universe</subject><ispartof>Geophysical journal international, 2022-03, Vol.230 (1), p.317-333</ispartof><rights>The Author(s) 2022. Published by Oxford University Press on behalf of The Royal Astronomical Society. 2022</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-a358t-8cf2988c9a80aeac509fb9e8da66c61cf952197fb20b3d90b3393dcf82c5b7f3</citedby><cites>FETCH-LOGICAL-a358t-8cf2988c9a80aeac509fb9e8da66c61cf952197fb20b3d90b3393dcf82c5b7f3</cites><orcidid>0000-0002-4387-5785 ; 0000-0002-9232-0938</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,1598,27901,27902</link.rule.ids><linktorsrc>$$Uhttps://dx.doi.org/10.1093/gji/ggac080$$EView_record_in_Oxford_University_Press$$FView_record_in_$$GOxford_University_Press</linktorsrc><backlink>$$Uhttps://hal.science/hal-04203773$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Döring, M F</creatorcontrib><creatorcontrib>Julià, J</creatorcontrib><creatorcontrib>Evain, M</creatorcontrib><title>Joint inversion of receiver functions and surface wave dispersion in the Recôncavo–Tucano basin of NE Brazil: implications for basin formation</title><title>Geophysical journal international</title><description>SUMMARY
The crustal structure of the Recôncavo–Tucano basin, an aborted rift system that developed in NE Brazil during extension related to the opening of the South Atlantic Ocean, has been investigated through local constraints from receiver functions developed at 18 seismic stations in the region. Gravity modelling has proved unable to unequivocally localize crustal thinning under the basin depocentre and, together with a general lack of sediments from a putative thermal sag phase, this has led to a range of basin formation models invoking either pure or simple shear or a combination of both. In particular, the ‘flexural cantilever’ model has assumed simple shear extension in the upper crust and pure shear extension in the lower crust and mantle, enabling local erosion of the rift flanks after footwall uplift and regional erosion of the thermal sag phase after magmatic underplate of the basin's crust. Our results reveal that the crust is over 40 km thick beneath the Tucano and Recôncavo basins and that it contains a thick (5–8 km) layer of high velocity (Vs > 4.0 km s–1) material below ∼35 km depth. These observations contrast with structure immediately West (São Francisco Craton) and East (Borborema Province) of the basin, for which crustal thicknesses average 42 and 36 km, respectively, lower crustal velocities are below 4.0 km s–1, and local instances of crust as thin as 33.5 km are observed. We propose, in agreement with the ‘flexural cantilever’ model, that the fast velocity layer making the basin's lowermost crust resulted from mafic underplating after stretching and thinning during the syn-rift phase, restoring crustal thickness to pre-rift values (or larger) and providing the necessary buoyancy to trigger regional uplift. Moreover, although not pervasive, instances of thin crust along the footwall could be related to rift flank erosion. We thus conclude that, regardless of the mode of extension in the upper crust, our results favour models of basin formation invoking extension of the lower crust by pure shear.</description><subject>Sciences of the Universe</subject><issn>0956-540X</issn><issn>1365-246X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNp9kD9OwzAYxS0EEqUwcQFPSAiF2nGS2mxQFQqqQEIdukVfHLt1lcaVnRTBxBUQV-EG3ISTkLYRI8v35-n33vAQOqXkkhLBerOF6c1mIAkne6hDWRIHYZRM91GHiDgJ4ohMD9GR9wtCaEQj3kEfD9aUFTblWjlvbImtxk5JZZof67qUVSN6DGWOfe00SIVfYK1wbvyqdZgSV3OFn5X8_iolrO3P--ekllBanIE328jHIb5x8GaKK2yWq8JI2OVq61qouZZb8RgdaCi8Oml3F01uh5PBKBg_3d0PrscBsJhXAZc6FJxLAZyAAhkToTOheA5JIhMqtYhDKvo6C0nGctEMJlguNQ9lnPU166LzXewcinTlzBLca2rBpKPrcbrRSBQS1u-zNW3Yix0rnfXeKf1noCTdFJ82xadt8Q19tqNtvfoX_AVycYmS</recordid><startdate>20220324</startdate><enddate>20220324</enddate><creator>Döring, M F</creator><creator>Julià, J</creator><creator>Evain, M</creator><general>Oxford University Press</general><general>Oxford University Press (OUP)</general><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><scope>VOOES</scope><orcidid>https://orcid.org/0000-0002-4387-5785</orcidid><orcidid>https://orcid.org/0000-0002-9232-0938</orcidid></search><sort><creationdate>20220324</creationdate><title>Joint inversion of receiver functions and surface wave dispersion in the Recôncavo–Tucano basin of NE Brazil: implications for basin formation</title><author>Döring, M F ; Julià, J ; Evain, M</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a358t-8cf2988c9a80aeac509fb9e8da66c61cf952197fb20b3d90b3393dcf82c5b7f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Sciences of the Universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Döring, M F</creatorcontrib><creatorcontrib>Julià, J</creatorcontrib><creatorcontrib>Evain, M</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><jtitle>Geophysical journal international</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Döring, M F</au><au>Julià, J</au><au>Evain, M</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Joint inversion of receiver functions and surface wave dispersion in the Recôncavo–Tucano basin of NE Brazil: implications for basin formation</atitle><jtitle>Geophysical journal international</jtitle><date>2022-03-24</date><risdate>2022</risdate><volume>230</volume><issue>1</issue><spage>317</spage><epage>333</epage><pages>317-333</pages><issn>0956-540X</issn><eissn>1365-246X</eissn><abstract>SUMMARY
The crustal structure of the Recôncavo–Tucano basin, an aborted rift system that developed in NE Brazil during extension related to the opening of the South Atlantic Ocean, has been investigated through local constraints from receiver functions developed at 18 seismic stations in the region. Gravity modelling has proved unable to unequivocally localize crustal thinning under the basin depocentre and, together with a general lack of sediments from a putative thermal sag phase, this has led to a range of basin formation models invoking either pure or simple shear or a combination of both. In particular, the ‘flexural cantilever’ model has assumed simple shear extension in the upper crust and pure shear extension in the lower crust and mantle, enabling local erosion of the rift flanks after footwall uplift and regional erosion of the thermal sag phase after magmatic underplate of the basin's crust. Our results reveal that the crust is over 40 km thick beneath the Tucano and Recôncavo basins and that it contains a thick (5–8 km) layer of high velocity (Vs > 4.0 km s–1) material below ∼35 km depth. These observations contrast with structure immediately West (São Francisco Craton) and East (Borborema Province) of the basin, for which crustal thicknesses average 42 and 36 km, respectively, lower crustal velocities are below 4.0 km s–1, and local instances of crust as thin as 33.5 km are observed. We propose, in agreement with the ‘flexural cantilever’ model, that the fast velocity layer making the basin's lowermost crust resulted from mafic underplating after stretching and thinning during the syn-rift phase, restoring crustal thickness to pre-rift values (or larger) and providing the necessary buoyancy to trigger regional uplift. Moreover, although not pervasive, instances of thin crust along the footwall could be related to rift flank erosion. We thus conclude that, regardless of the mode of extension in the upper crust, our results favour models of basin formation invoking extension of the lower crust by pure shear.</abstract><pub>Oxford University Press</pub><doi>10.1093/gji/ggac080</doi><tpages>17</tpages><orcidid>https://orcid.org/0000-0002-4387-5785</orcidid><orcidid>https://orcid.org/0000-0002-9232-0938</orcidid><oa>free_for_read</oa></addata></record> |
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title | Joint inversion of receiver functions and surface wave dispersion in the Recôncavo–Tucano basin of NE Brazil: implications for basin formation |
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