Velocity structure beneath the southern Puna plateau: evidence for delamination
- Autores
- Calixto, Frank J.; Sandvol, Eric; Kay, Suzanne; Mulcahy, Patrick; Heit, Benjamin; Yuan, Xiaohui; Coira, Beatriz Lidia Luisa; Comte, Diana; Alvarado, Patricia Monica
- Año de publicación
- 2013
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The high elevation of the southern Puna plateau, the widespread melting of its crust, the gap in intermediate depth seismicity and the recent eruptions of ignimbrite complexes can be explained by delamination of the lithospheric mantle beneath it. To test this hypothesis, an array consisting of 73 broad band and short period seismic stations was deployed in the region for a period of 2 years starting in 2007. We inverted the data using the two plane wave approach and obtained 1-D and 3-D Rayleigh wave phase velocities. Our dispersion curve shows that at short periods (<70 s) the phase velocities are slightly higher than those of the Tibetan plateau and lower than those of the Anatolian plateau. At periods of 100–140 s we observe a low velocity zone that might be remnant hot asthenosphere below a flat slab (7–10 Ma). We estimate the average continental lithosphere thickness for the region to be between 100 and 130 km. Our three-dimensional Rayleigh wave phase velocities show a high velocity anomaly at low frequencies (0.007, 0.008, and 0.009 Hz) slightly to the north of Cerro Galan. This would be consistent with the hypothesis of delamination in which a piece of lithosphere has detached and caused upwelling of hot asthenosphere, which in turn caused widespread alkaline-collision related volcanism. This interpretation is also corroborated by our shear wave velocity model, where a high velocity anomaly beneath the northern edge of Cerro Galan at 130 km depth is interpreted as the delaminated block on top of the subducting Nazca slab.
Fil: Calixto, Frank J.. University of Missouri; Estados Unidos
Fil: Sandvol, Eric. University of Missouri; Estados Unidos
Fil: Kay, Suzanne. Cornell University; Estados Unidos
Fil: Mulcahy, Patrick. Cornell University; Estados Unidos
Fil: Heit, Benjamin. Helmholtz-Centre Potsdam. Deutsches GeoForschungsZentrum; Alemania
Fil: Yuan, Xiaohui. Helmholtz-Centre Potsdam. Deutsches GeoForschungsZentrum; Alemania
Fil: Coira, Beatriz Lidia Luisa. Universidad Nacional de Jujuy. Instituto de Geología Minera; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Comte, Diana. Universidad de Chile; Chile
Fil: Alvarado, Patricia Monica. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina - Materia
-
Velocity Structure beneath
Southern Puna Plateau
Evidence for Delamination - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/25419
Ver los metadatos del registro completo
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spelling |
Velocity structure beneath the southern Puna plateau: evidence for delaminationCalixto, Frank J.Sandvol, EricKay, SuzanneMulcahy, PatrickHeit, BenjaminYuan, XiaohuiCoira, Beatriz Lidia LuisaComte, DianaAlvarado, Patricia MonicaVelocity Structure beneathSouthern Puna PlateauEvidence for Delaminationhttps://purl.org/becyt/ford/1.5https://purl.org/becyt/ford/1The high elevation of the southern Puna plateau, the widespread melting of its crust, the gap in intermediate depth seismicity and the recent eruptions of ignimbrite complexes can be explained by delamination of the lithospheric mantle beneath it. To test this hypothesis, an array consisting of 73 broad band and short period seismic stations was deployed in the region for a period of 2 years starting in 2007. We inverted the data using the two plane wave approach and obtained 1-D and 3-D Rayleigh wave phase velocities. Our dispersion curve shows that at short periods (<70 s) the phase velocities are slightly higher than those of the Tibetan plateau and lower than those of the Anatolian plateau. At periods of 100–140 s we observe a low velocity zone that might be remnant hot asthenosphere below a flat slab (7–10 Ma). We estimate the average continental lithosphere thickness for the region to be between 100 and 130 km. Our three-dimensional Rayleigh wave phase velocities show a high velocity anomaly at low frequencies (0.007, 0.008, and 0.009 Hz) slightly to the north of Cerro Galan. This would be consistent with the hypothesis of delamination in which a piece of lithosphere has detached and caused upwelling of hot asthenosphere, which in turn caused widespread alkaline-collision related volcanism. This interpretation is also corroborated by our shear wave velocity model, where a high velocity anomaly beneath the northern edge of Cerro Galan at 130 km depth is interpreted as the delaminated block on top of the subducting Nazca slab.Fil: Calixto, Frank J.. University of Missouri; Estados UnidosFil: Sandvol, Eric. University of Missouri; Estados UnidosFil: Kay, Suzanne. Cornell University; Estados UnidosFil: Mulcahy, Patrick. Cornell University; Estados UnidosFil: Heit, Benjamin. Helmholtz-Centre Potsdam. Deutsches GeoForschungsZentrum; AlemaniaFil: Yuan, Xiaohui. Helmholtz-Centre Potsdam. Deutsches GeoForschungsZentrum; AlemaniaFil: Coira, Beatriz Lidia Luisa. Universidad Nacional de Jujuy. Instituto de Geología Minera; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Comte, Diana. Universidad de Chile; ChileFil: Alvarado, Patricia Monica. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaAmerican Geophysical Union2013-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/25419Calixto, Frank J.; Sandvol, Eric; Kay, Suzanne; Mulcahy, Patrick; Heit, Benjamin; et al.; Velocity structure beneath the southern Puna plateau: evidence for delamination; American Geophysical Union; Geochemistry Geophysics Geosystems; 14; 10; 10-2013; 4292-43051525-2027CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1002/ggge.20266/abstractinfo:eu-repo/semantics/altIdentifier/doi/10.1002/ggge.20266info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:39:05Zoai:ri.conicet.gov.ar:11336/25419instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:39:05.949CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Velocity structure beneath the southern Puna plateau: evidence for delamination |
title |
Velocity structure beneath the southern Puna plateau: evidence for delamination |
spellingShingle |
Velocity structure beneath the southern Puna plateau: evidence for delamination Calixto, Frank J. Velocity Structure beneath Southern Puna Plateau Evidence for Delamination |
title_short |
Velocity structure beneath the southern Puna plateau: evidence for delamination |
title_full |
Velocity structure beneath the southern Puna plateau: evidence for delamination |
title_fullStr |
Velocity structure beneath the southern Puna plateau: evidence for delamination |
title_full_unstemmed |
Velocity structure beneath the southern Puna plateau: evidence for delamination |
title_sort |
Velocity structure beneath the southern Puna plateau: evidence for delamination |
dc.creator.none.fl_str_mv |
Calixto, Frank J. Sandvol, Eric Kay, Suzanne Mulcahy, Patrick Heit, Benjamin Yuan, Xiaohui Coira, Beatriz Lidia Luisa Comte, Diana Alvarado, Patricia Monica |
author |
Calixto, Frank J. |
author_facet |
Calixto, Frank J. Sandvol, Eric Kay, Suzanne Mulcahy, Patrick Heit, Benjamin Yuan, Xiaohui Coira, Beatriz Lidia Luisa Comte, Diana Alvarado, Patricia Monica |
author_role |
author |
author2 |
Sandvol, Eric Kay, Suzanne Mulcahy, Patrick Heit, Benjamin Yuan, Xiaohui Coira, Beatriz Lidia Luisa Comte, Diana Alvarado, Patricia Monica |
author2_role |
author author author author author author author author |
dc.subject.none.fl_str_mv |
Velocity Structure beneath Southern Puna Plateau Evidence for Delamination |
topic |
Velocity Structure beneath Southern Puna Plateau Evidence for Delamination |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.5 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The high elevation of the southern Puna plateau, the widespread melting of its crust, the gap in intermediate depth seismicity and the recent eruptions of ignimbrite complexes can be explained by delamination of the lithospheric mantle beneath it. To test this hypothesis, an array consisting of 73 broad band and short period seismic stations was deployed in the region for a period of 2 years starting in 2007. We inverted the data using the two plane wave approach and obtained 1-D and 3-D Rayleigh wave phase velocities. Our dispersion curve shows that at short periods (<70 s) the phase velocities are slightly higher than those of the Tibetan plateau and lower than those of the Anatolian plateau. At periods of 100–140 s we observe a low velocity zone that might be remnant hot asthenosphere below a flat slab (7–10 Ma). We estimate the average continental lithosphere thickness for the region to be between 100 and 130 km. Our three-dimensional Rayleigh wave phase velocities show a high velocity anomaly at low frequencies (0.007, 0.008, and 0.009 Hz) slightly to the north of Cerro Galan. This would be consistent with the hypothesis of delamination in which a piece of lithosphere has detached and caused upwelling of hot asthenosphere, which in turn caused widespread alkaline-collision related volcanism. This interpretation is also corroborated by our shear wave velocity model, where a high velocity anomaly beneath the northern edge of Cerro Galan at 130 km depth is interpreted as the delaminated block on top of the subducting Nazca slab. Fil: Calixto, Frank J.. University of Missouri; Estados Unidos Fil: Sandvol, Eric. University of Missouri; Estados Unidos Fil: Kay, Suzanne. Cornell University; Estados Unidos Fil: Mulcahy, Patrick. Cornell University; Estados Unidos Fil: Heit, Benjamin. Helmholtz-Centre Potsdam. Deutsches GeoForschungsZentrum; Alemania Fil: Yuan, Xiaohui. Helmholtz-Centre Potsdam. Deutsches GeoForschungsZentrum; Alemania Fil: Coira, Beatriz Lidia Luisa. Universidad Nacional de Jujuy. Instituto de Geología Minera; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Comte, Diana. Universidad de Chile; Chile Fil: Alvarado, Patricia Monica. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina |
description |
The high elevation of the southern Puna plateau, the widespread melting of its crust, the gap in intermediate depth seismicity and the recent eruptions of ignimbrite complexes can be explained by delamination of the lithospheric mantle beneath it. To test this hypothesis, an array consisting of 73 broad band and short period seismic stations was deployed in the region for a period of 2 years starting in 2007. We inverted the data using the two plane wave approach and obtained 1-D and 3-D Rayleigh wave phase velocities. Our dispersion curve shows that at short periods (<70 s) the phase velocities are slightly higher than those of the Tibetan plateau and lower than those of the Anatolian plateau. At periods of 100–140 s we observe a low velocity zone that might be remnant hot asthenosphere below a flat slab (7–10 Ma). We estimate the average continental lithosphere thickness for the region to be between 100 and 130 km. Our three-dimensional Rayleigh wave phase velocities show a high velocity anomaly at low frequencies (0.007, 0.008, and 0.009 Hz) slightly to the north of Cerro Galan. This would be consistent with the hypothesis of delamination in which a piece of lithosphere has detached and caused upwelling of hot asthenosphere, which in turn caused widespread alkaline-collision related volcanism. This interpretation is also corroborated by our shear wave velocity model, where a high velocity anomaly beneath the northern edge of Cerro Galan at 130 km depth is interpreted as the delaminated block on top of the subducting Nazca slab. |
publishDate |
2013 |
dc.date.none.fl_str_mv |
2013-10 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/25419 Calixto, Frank J.; Sandvol, Eric; Kay, Suzanne; Mulcahy, Patrick; Heit, Benjamin; et al.; Velocity structure beneath the southern Puna plateau: evidence for delamination; American Geophysical Union; Geochemistry Geophysics Geosystems; 14; 10; 10-2013; 4292-4305 1525-2027 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/25419 |
identifier_str_mv |
Calixto, Frank J.; Sandvol, Eric; Kay, Suzanne; Mulcahy, Patrick; Heit, Benjamin; et al.; Velocity structure beneath the southern Puna plateau: evidence for delamination; American Geophysical Union; Geochemistry Geophysics Geosystems; 14; 10; 10-2013; 4292-4305 1525-2027 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1002/ggge.20266/abstract info:eu-repo/semantics/altIdentifier/doi/10.1002/ggge.20266 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
American Geophysical Union |
publisher.none.fl_str_mv |
American Geophysical Union |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844614415599534080 |
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13.070432 |