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Disentangling factors controlling earthquake-triggered soft-sediment deformation in lakes
Indexado
WoS WOS:000830837300001
Scopus SCOPUS_ID:85134250713
DOI 10.1016/J.SEDGEO.2022.106200
Año 2022
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



In-situ soft sediment deformation structures (SSDS) are commonly used as paleoseismic indicators in marine and lacustrine sedimentary records. Earthquake-related shear can deform sediment in the shallow subsurface through Kelvin-Helmholtz instability. The SSDS related to Kelvin-Helmholtz instability have been used to quan-tify shaking strength of past earthquakes. However, the relative importance of i) lithology and physical proper-ties, ii) potential basal shear surfaces (e.g. clastic deposits), iii) slope angle, and iv) seismic shaking strength (e.g. peak ground acceleration) for deformation related to Kelvin-Helmholtz instability remains poorly studied. Lake Rinihue (south-central Chile) is chosen as a natural laboratory for disentangling the effect of the aforemen-tioned factors because i) the sediment composition of background sediment varies downcore and ii) volcanogenic clastic deposits are abundant within the sedimentary sequence. A previous study at lake Rinihue identified 25 SSDS intervals induced by historical earthquakes of varying rupture extent in 17 sediment cores taken at slope angles ranging from-0.2 degrees to-4.9 degrees (i.e. 16 slope sites and 1 basin site). Our study shows that defor-mation mostly occurs directly above volcanogenic deposits (i.e. 72 % of SSDS intervals), suggesting that volcanogenic deposits promote earthquake-induced deformation by strain softening, liquefaction or water film formation. Deformation thickness of SSDS increases with higher slope angles (i.e. strong positive correlation). Ad-ditionally, deformation thickness commonly corresponds to the stratigraphic depth of the youngest preceding volcanogenic deposit, but for steeper slope angles stratigraphically older volcanogenic deposits can function as basal shear surface. Therefore, we suggest that deformation thickness is primarily regulated by gravitational stress (i.e. slope angle) and secondarily by the stratigraphic depth of volcanogenic deposits. The earthquakes related to strongest shaking caused almost exclusively SSDS with highest deformation degrees (i.e. folds and intraclast breccia) as well as largest spatial extent of SSDS, resulting in highest numbers of related SSDS in the investigated cores. Thinner SSDS have higher deformation degrees at a given shaking strength, as seismically -induced shear energy acts more effectively on thinner deforming sequences. Therefore, we suggest that deforma-tion degree is primarily controlled by shaking strength and secondarily modulated by the thickness of the deforming sequences. We infer that deformation thickness is not a reliable indicator of paleoseismic shaking strength as this relies on many preconditioning factors independent of shaking strength. On the other hand, deformation degree can be a good proxy for shaking strength also in settings with varying lithotypes and intercalated clastic event deposits, provided multiple cores are studied to avoid under-or overestimation of paleoseismic shaking strength. (c) 2022 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http:// creativecommons.org/licenses/by/4.0/).

Revista



Revista ISSN
Sedimentary Geology 0037-0738

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Disciplinas de Investigación



WOS
Geology
Scopus
Geology
Stratigraphy
SciELO
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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 Molenaar, A. Mujer Univ Innsbruck - Austria
Universität Innsbruck - Austria
2 Van Daele, M. Hombre Univ Ghent - Bélgica
Universiteit Gent - Bélgica
3 Huang, Jyh Jaan Steven - Univ Innsbruck - Austria
Natl Taiwan Univ - Taiwán
Universität Innsbruck - Austria
Institute of Oceanography, National Taiwan University - Taiwán
4 Strasser, Michael Hombre Univ Innsbruck - Austria
Universität Innsbruck - Austria
5 Fiers, Géraldine Mujer Univ Ghent - Bélgica
Universiteit Gent - Bélgica
6 PINO-ESPINOZA, MARIELA CONSTANZA Hombre Universidad Austral de Chile - Chile
7 URRUTIA-PEREZ, ROBERTO ENRIQUE Hombre Universidad de Concepción - Chile
8 Moernaut, J. Hombre Univ Innsbruck - Austria
Universität Innsbruck - Austria

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Financiamiento



Fuente
Austrian Science Fund (FWF)
Austrian Science Fund
Fonds Wetenschappelijk Onderzoek
Research Foundation Flanders (FWO)
Universität Innsbruck
Nachwuchsforderung 2016 of the University of Innsbruck
Medizinische Universität Innsbruck

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Agradecimientos



Agradecimiento
The Austrian Science Fund (FWF): project P30285-N34 and P34504-N; and Nachwuchsforderung 2016 of the University of Innsbruck funded the contribution of Ariana Molenaar and Jasper Moernaut.Maarten Van Daele was funded by the Research Foundation Flanders(FWO; project 1523315N and 12D6817N) and Roberto Urrutia by project ANID/FONDAP/15130015. We thank Rik Achten from Ghent University Hospital for allowing access to the medical CT scanner as well as Wolfgang Recheis and Markus Erhardt from the Medical University Innsbruck. Thomas Vandorpe, Koen De Rycker, Robert Brummer, Alejandro Pena, Cristian Araya and Daniel Martinez Olguin are thanked for their logistical and technical support during the Chilean fieldwork. We are grateful to Sebastien Bertrand for showing us how to do biogenicsilica measurements. We thank Marcel Ortler and Samuel Barrett for providing the initial python script used for K-means clustering of XRF data. We are grateful to Ivana Stiperski and Alsbeta Medvedova for advice on Kelvin-Helmholtz instability. We thank Ian Alsop and an anonymous reviewer for their valuable feedback, which allowed us to greatly improve the manuscript.
The Austrian Science Fund (FWF): project P30285-N34 and P34504-N; and Nachwuchsförderung 2016 of the University of Innsbruck funded the contribution of Ariana Molenaar and Jasper Moernaut. Maarten Van Daele was funded by the Research Foundation Flanders (FWO; project 1523315N and 12D6817N) and Roberto Urrutia by project ANID/FONDAP/15130015. We thank Rik Achten from Ghent University Hospital for allowing access to the medical CT scanner as well as Wolfgang Recheis and Markus Erhardt from the Medical University Innsbruck. Thomas Vandorpe, Koen De Rycker, Robert Brümmer, Alejandro Peña, Cristian Araya and Daniel Martínez Olguín are thanked for their logistical and technical support during the Chilean fieldwork. We are grateful to Sebastien Bertrand for showing us how to do biogenic silica measurements. We thank Marcel Ortler and Samuel Barrett for providing the initial python script used for K-means clustering of XRF data. We are grateful to Ivana Stiperski and Alsbeta Medvedova for advice on Kelvin-Helmholtz instability. We thank Ian Alsop and an anonymous reviewer for their valuable feedback, which allowed us to greatly improve the manuscript.
The Austrian Science Fund (FWF): project P30285-N34 and P34504-N; and Nachwuchsförderung 2016 of the University of Innsbruck funded the contribution of Ariana Molenaar and Jasper Moernaut. Maarten Van Daele was funded by the Research Foundation Flanders (FWO; project 1523315N and 12D6817N) and Roberto Urrutia by project ANID/FONDAP/15130015. We thank Rik Achten from Ghent University Hospital for allowing access to the medical CT scanner as well as Wolfgang Recheis and Markus Erhardt from the Medical University Innsbruck. Thomas Vandorpe, Koen De Rycker, Robert Brümmer, Alejandro Peña, Cristian Araya and Daniel Martínez Olguín are thanked for their logistical and technical support during the Chilean fieldwork. We are grateful to Sebastien Bertrand for showing us how to do biogenic silica measurements. We thank Marcel Ortler and Samuel Barrett for providing the initial python script used for K-means clustering of XRF data. We are grateful to Ivana Stiperski and Alsbeta Medvedova for advice on Kelvin-Helmholtz instability. We thank Ian Alsop and an anonymous reviewer for their valuable feedback, which allowed us to greatly improve the manuscript.

Muestra la fuente de financiamiento declarada en la publicación.