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Effects on Chilean Vertical Reference Frame due to the Maule Earthquake co-seismic and post-seismic effects
Indexado
WoS WOS:000418972300003
Scopus SCOPUS_ID:85042202248
DOI 10.1016/J.JOG.2017.07.006
Año 2017
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



The Maule Earthquake (M-w = 8.8) of February 27, 2010 is among the strongest earthquakes that occurred in recent years throughout the world. The crustal deformation caused by this earthquake has been widely studied using GNSS, InSAR and gravity observations. However, there is currently no estimation of the possible vertical deformations produced by co-seismic and post-seismic effects in segments of the Chilean Vertical Reference Frame (CHVRF). In this paper, we present an estimation of co-seismic and post-seismic deformations on the CHVRF using an indirect approach based on GNSS and Gravity Recovery and Climate Experiment (GRACE) data as well as by applying a trajectory model. GNSS time series were used from 10 continuous GNSS stations in the period from 2007 to 2015, as well as 28 GNSS temporary stations realized before and after the earthquake, and 34 vertical deformation vectors in the region most affected by the earthquake. We considered a set of 147 monthly solutions of spherical harmonic gravity field that were expanded up to degree, as well as order 96 of the GRACE mission provided by Center for Space Research, University of Texas at Austin (UT-CSR) process center. The magnitude of vertical deformation was estimated in part of the Chilean vertical network due to the co-seismic and post-seismic effects. Once we evaluated the hydrological effect, natural and artificial jumps, and the effect of glacial isostatic adjustment in GNSS and GRACE time series, the maximum values associated to co- and post-seismic deformations on orthometric height were found to be similar to -34 cm and 5 cm, respectively. Overall, the deformation caused by the Maule earthquake in orthometric heights is almost entirely explained by the variation in the ellipsoidal heights (over 85% in co-seismic jump); however, coseismic jump in the geoid reached -3.3 mm, and could influence the maintenance of a modern vertical reference network in a medium to long term. We evaluated the consistency for a segment of the CHVRF after the earthquake and recommended precautions for using the CHVRF in the region.

Revista



Revista ISSN
Journal Of Geodynamics 0264-3707

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Disciplinas de Investigación



WOS
Geochemistry & Geophysics
Scopus
Earth Surface Processes
Geophysics
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 MONTECINO-CASTRO, HENRY DIVERTH Hombre UNIV FED PARANA - Brasil
Universidad de Concepción - Chile
Universidade Federal do Paraná - Brasil
2 de Freitas, S. R. C. Hombre UNIV FED PARANA - Brasil
Universidade Federal do Paraná - Brasil
3 BAEZ-SOTO, JUAN CARLOS Hombre Universidad de Chile - Chile
4 Ferreira, Vagner G. Hombre Hohai Univ - China
Hohai University - China

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Origen de Citas Identificadas



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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 27.27 %
Citas No-identificadas: 72.73 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 27.27 %
Citas No-identificadas: 72.73 %

Financiamiento



Fuente
National Natural Science Foundation of China
CNPq
Conselho Nacional de Desenvolvimento Científico e Tecnológico
University of Concepcion (UdeC)

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Agradecimientos



Agradecimiento
Author Henry Montecino would like to thank the PhD scholarship granted by the University of Concepcion (UdeC). The author Silvio de Freitas thanks CNPq (Grant process N. 306936/2015-1). Vagner Ferreira acknowledges the partial support provided by the National Natural Science Foundation of China through a grant No. 42574001. The authors thank the CSR, GFZ and JPL processing centers for providing monthly solutions of the gravity field, the Earth Science Division of NASA for the distribution of GLDAS, the CAP projects, IGS, and BKG and the Universidad de Chile for providing the GPS observations used here. We thank Professor Irhia Artemieva (Editor-in-Chief) and the two anonymous reviewers for their constructive comments that helped us to improve the quality of this manuscript.
Author Henry Montecino would like to thank the PhD scholarship granted by the University of Concepción (UdeC). The author Silvio de Freitas thanks CNPq (Grant process N. 306936/2015-1). Vagner Ferreira acknowledges the partial support provided by the National Natural Science Foundation of China through a grant No. 42574001. The authors thank the CSR, GFZ and JPL processing centers for providing monthly solutions of the gravity field, the Earth Science Division of NASA for the distribution of GLDAS, the CAP projects, IGS, and BKG and the Universidad de Chile for providing the GPS observations used here. We thank Professor Irina Artemieva (Editor-in-Chief) and the two anonymous reviewers for their constructive comments that helped us to improve the quality of this manuscript.

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