Short term forecasting of explosions at Ubinas volcano, Perú
Descripción del Articulo
Most seismic eruption forerunners are described using Volcano‐Tectonic earthquakes, seismic energy release, deformation rates or seismic noise analyses. Using the seismic data recorded at Ubinas volcano (Perú) between 2006 and 2008, we explore the time evolution of the Long Period (LP) seismicity ra...
Autores: | , , , , , , |
---|---|
Formato: | artículo |
Fecha de Publicación: | 2011 |
Institución: | Instituto Geofísico del Perú |
Repositorio: | IGP-Institucional |
Lenguaje: | inglés |
OAI Identifier: | oai:repositorio.igp.gob.pe:20.500.12816/3041 |
Enlace del recurso: | http://hdl.handle.net/20.500.12816/3041 https://doi.org/10.1029/2010JB008180 |
Nivel de acceso: | acceso abierto |
Materia: | Long Period Ubinas Explosion Forecasting Seismicity Volcano http://purl.org/pe-repo/ocde/ford#1.05.00 http://purl.org/pe-repo/ocde/ford#1.05.04 http://purl.org/pe-repo/ocde/ford#1.05.07 |
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dc.title.es_ES.fl_str_mv |
Short term forecasting of explosions at Ubinas volcano, Perú |
title |
Short term forecasting of explosions at Ubinas volcano, Perú |
spellingShingle |
Short term forecasting of explosions at Ubinas volcano, Perú Traversa, P. Long Period Ubinas Explosion Forecasting Seismicity Volcano http://purl.org/pe-repo/ocde/ford#1.05.00 http://purl.org/pe-repo/ocde/ford#1.05.04 http://purl.org/pe-repo/ocde/ford#1.05.07 |
title_short |
Short term forecasting of explosions at Ubinas volcano, Perú |
title_full |
Short term forecasting of explosions at Ubinas volcano, Perú |
title_fullStr |
Short term forecasting of explosions at Ubinas volcano, Perú |
title_full_unstemmed |
Short term forecasting of explosions at Ubinas volcano, Perú |
title_sort |
Short term forecasting of explosions at Ubinas volcano, Perú |
author |
Traversa, P. |
author_facet |
Traversa, P. Lengliné, O. Macedo Sánchez, Orlando Efraín Metaxian, J. P. Grasso, J. R. Inza Callupe, Lamberto Adolfo Taipe, Edu |
author_role |
author |
author2 |
Lengliné, O. Macedo Sánchez, Orlando Efraín Metaxian, J. P. Grasso, J. R. Inza Callupe, Lamberto Adolfo Taipe, Edu |
author2_role |
author author author author author author |
dc.contributor.author.fl_str_mv |
Traversa, P. Lengliné, O. Macedo Sánchez, Orlando Efraín Metaxian, J. P. Grasso, J. R. Inza Callupe, Lamberto Adolfo Taipe, Edu |
dc.subject.es_ES.fl_str_mv |
Long Period Ubinas Explosion Forecasting Seismicity Volcano |
topic |
Long Period Ubinas Explosion Forecasting Seismicity Volcano http://purl.org/pe-repo/ocde/ford#1.05.00 http://purl.org/pe-repo/ocde/ford#1.05.04 http://purl.org/pe-repo/ocde/ford#1.05.07 |
dc.subject.ocde.es_ES.fl_str_mv |
http://purl.org/pe-repo/ocde/ford#1.05.00 http://purl.org/pe-repo/ocde/ford#1.05.04 http://purl.org/pe-repo/ocde/ford#1.05.07 |
description |
Most seismic eruption forerunners are described using Volcano‐Tectonic earthquakes, seismic energy release, deformation rates or seismic noise analyses. Using the seismic data recorded at Ubinas volcano (Perú) between 2006 and 2008, we explore the time evolution of the Long Period (LP) seismicity rate prior to 143 explosions. We resolve an average acceleration of the LP rate above the background level during the 2–3 hours preceding the explosion onset. Such an average pattern, which emerges when stacking over LP time series, is robust and stable over all the 2006–2008 period, for which data is available. This accelerating pattern is also recovered when conditioning the LP rate on the occurrence of an other LP event, rather than on the explosion time. It supports a common mechanism for the generation of explosions and LP events, the magma conduit pressure increase being the most probable candidate. The average LP rate acceleration toward an explosion is highly significant prior to the higher energy explosions, supposedly the ones associated with the larger pressure increases. The dramatic decay of the LP activity following explosions, still reinforce the strong relationship between these two processes. We test and we quantify the retrospective forecasting power of these LP rate patterns to predict Ubinas explosions. The prediction quality of the forecasts (e.g. for 17% of alarm time, we predict 63% of Ubinas explosions, with 58% of false alarms) is evaluated using error diagrams. The prediction results are stable and the prediction algorithm validated, i.e. its performance is better than the random guess. |
publishDate |
2011 |
dc.date.accessioned.none.fl_str_mv |
2018-09-21T15:59:21Z |
dc.date.available.none.fl_str_mv |
2018-09-21T15:59:21Z |
dc.date.issued.fl_str_mv |
2011-11 |
dc.type.es_ES.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
dc.identifier.citation.es_ES.fl_str_mv |
Traversa, P., Lengliné, O., Macedo, O., Metaxian, J. P., Grasso, J. R., Inza, A., & Taipe, E. (2011). Short term forecasting of explosions at Ubinas volcano, Perú.==$Journal of Geophysical Research: Solid Earth, 116$==(B11), B11301. https://doi.org/10.1029/2010JB008180 |
dc.identifier.govdoc.none.fl_str_mv |
index-oti2018 |
dc.identifier.uri.none.fl_str_mv |
http://hdl.handle.net/20.500.12816/3041 |
dc.identifier.journal.es_ES.fl_str_mv |
Journal of Geophysical Research: Solid Earth |
dc.identifier.doi.es_ES.fl_str_mv |
https://doi.org/10.1029/2010JB008180 |
identifier_str_mv |
Traversa, P., Lengliné, O., Macedo, O., Metaxian, J. P., Grasso, J. R., Inza, A., & Taipe, E. (2011). Short term forecasting of explosions at Ubinas volcano, Perú.==$Journal of Geophysical Research: Solid Earth, 116$==(B11), B11301. https://doi.org/10.1029/2010JB008180 index-oti2018 Journal of Geophysical Research: Solid Earth |
url |
http://hdl.handle.net/20.500.12816/3041 https://doi.org/10.1029/2010JB008180 |
dc.language.iso.es_ES.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.none.fl_str_mv |
urn:issn:2169-9313 |
dc.rights.es_ES.fl_str_mv |
info:eu-repo/semantics/openAccess |
dc.rights.uri.es_ES.fl_str_mv |
https://creativecommons.org/licences/by/4.0/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licences/by/4.0/ |
dc.format.es_ES.fl_str_mv |
application/pdf |
dc.coverage.spatial.none.fl_str_mv |
Ubinas, Volcán (Moquegua, Perú) |
dc.publisher.es_ES.fl_str_mv |
American Geophysical Union |
dc.source.none.fl_str_mv |
reponame:IGP-Institucional instname:Instituto Geofísico del Perú instacron:IGP |
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Instituto Geofísico del Perú |
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IGP |
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IGP |
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IGP-Institucional |
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Traversa, P.Lengliné, O.Macedo Sánchez, Orlando EfraínMetaxian, J. P.Grasso, J. R.Inza Callupe, Lamberto AdolfoTaipe, EduUbinas, Volcán (Moquegua, Perú)2018-09-21T15:59:21Z2018-09-21T15:59:21Z2011-11Traversa, P., Lengliné, O., Macedo, O., Metaxian, J. P., Grasso, J. R., Inza, A., & Taipe, E. (2011). Short term forecasting of explosions at Ubinas volcano, Perú.==$Journal of Geophysical Research: Solid Earth, 116$==(B11), B11301. https://doi.org/10.1029/2010JB008180index-oti2018http://hdl.handle.net/20.500.12816/3041Journal of Geophysical Research: Solid Earthhttps://doi.org/10.1029/2010JB008180Most seismic eruption forerunners are described using Volcano‐Tectonic earthquakes, seismic energy release, deformation rates or seismic noise analyses. Using the seismic data recorded at Ubinas volcano (Perú) between 2006 and 2008, we explore the time evolution of the Long Period (LP) seismicity rate prior to 143 explosions. We resolve an average acceleration of the LP rate above the background level during the 2–3 hours preceding the explosion onset. Such an average pattern, which emerges when stacking over LP time series, is robust and stable over all the 2006–2008 period, for which data is available. This accelerating pattern is also recovered when conditioning the LP rate on the occurrence of an other LP event, rather than on the explosion time. It supports a common mechanism for the generation of explosions and LP events, the magma conduit pressure increase being the most probable candidate. The average LP rate acceleration toward an explosion is highly significant prior to the higher energy explosions, supposedly the ones associated with the larger pressure increases. The dramatic decay of the LP activity following explosions, still reinforce the strong relationship between these two processes. We test and we quantify the retrospective forecasting power of these LP rate patterns to predict Ubinas explosions. The prediction quality of the forecasts (e.g. for 17% of alarm time, we predict 63% of Ubinas explosions, with 58% of false alarms) is evaluated using error diagrams. The prediction results are stable and the prediction algorithm validated, i.e. its performance is better than the random guess.Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:2169-9313info:eu-repo/semantics/openAccesshttps://creativecommons.org/licences/by/4.0/Long PeriodUbinasExplosionForecastingSeismicityVolcanohttp://purl.org/pe-repo/ocde/ford#1.05.00http://purl.org/pe-repo/ocde/ford#1.05.04http://purl.org/pe-repo/ocde/ford#1.05.07Short term forecasting of explosions at Ubinas volcano, Perúinfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALtraversa2011.pdftraversa2011.pdfapplication/pdf1516590https://repositorio.igp.gob.pe/bitstreams/f604fd0f-4df0-4dc8-9985-bd754f8015e9/download2bee1bc5bf28ca01d329afef3a809e7eMD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/368859d7-d4f0-491a-aec4-1e0a19324052/download8a4605be74aa9ea9d79846c1fba20a33MD52THUMBNAILtraversa2011.pdf.jpgtraversa2011.pdf.jpgIM Thumbnailimage/jpeg103654https://repositorio.igp.gob.pe/bitstreams/d3d40108-d6a4-45c8-abc1-24b2d5989df8/download41f392e027ae8218a25c0c0914b13545MD53TEXTtraversa2011.pdf.txttraversa2011.pdf.txtExtracted texttext/plain63524https://repositorio.igp.gob.pe/bitstreams/e4d574a2-c3f0-4e35-a24e-2aea501f8a16/download11454ac02391b4a4ca38cd4585094059MD5420.500.12816/3041oai:repositorio.igp.gob.pe:20.500.12816/30412020-12-15 15:16:34.266https://creativecommons.org/licences/by/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico del Perudspace-help@myu.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 |
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La información contenida en este registro es de entera responsabilidad de la institución que gestiona el repositorio institucional donde esta contenido este documento o set de datos. El CONCYTEC no se hace responsable por los contenidos (publicaciones y/o datos) accesibles a través del Repositorio Nacional Digital de Ciencia, Tecnología e Innovación de Acceso Abierto (ALICIA).