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Empirical investigation of friction weakening of terrestrial and Martian landslides using discrete element models
Understanding what controls the travelling distance of large landslides has been the topic of considerable debate. By combining observation and experimental data with depth-averaged continuum modelling of landslides and generated seismic waves, it was empirically observed that lower effective fricti...
Autores principales: | , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Springer Berlin Heidelberg
2019
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6529039/ https://www.ncbi.nlm.nih.gov/pubmed/31178675 http://dx.doi.org/10.1007/s10346-019-01140-8 |
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author | Borykov, Timur Mège, Daniel Mangeney, Anne Richard, Patrick Gurgurewicz, Joanna Lucas, Antoine |
author_facet | Borykov, Timur Mège, Daniel Mangeney, Anne Richard, Patrick Gurgurewicz, Joanna Lucas, Antoine |
author_sort | Borykov, Timur |
collection | PubMed |
description | Understanding what controls the travelling distance of large landslides has been the topic of considerable debate. By combining observation and experimental data with depth-averaged continuum modelling of landslides and generated seismic waves, it was empirically observed that lower effective friction had to be taken into account in the models to reproduce the dynamics and runout distance of larger volume landslides. Moreover, such simulation and observation results are compatible with a friction weakening with velocity as observed in earthquake mechanics. We investigate here as to whether similar empirical reduced friction should be put into discrete element models (DEM) to reproduce observed runout of large landslides on Earth and on Mars. First we show that, in the investigated parameter range and for a given volume, the runout distance simulated by 3D DEM is not much affected by the number (i.e. size) of grains once this number attains ~ 8000. We then calibrate the model on laboratory experiments and simulate other experiments of granular flows on inclined planes, making it possible for the first time to reproduce the observed effect of initial volume and aspect ratio on runout distances. In particular, the normalised runout distance starts to depend on the volume involved only above a critical slope angle > 16–19°, as observed experimentally. Finally, based on field data (volume, topography, deposit), we simulate a series of landslides on simplified inclined topography. The empirical friction coefficient, calibrated to reproduce the observed runout for each landslide, is shown to decrease with increasing landslide volume (or velocity), going down to values as low as 0.1–0.2. No distinguishable difference is observed between the behaviour of terrestrial and Martian landslides. ELECTRONIC SUPPLEMENTARY MATERIAL: The online version of this article (10.1007/s10346-019-01140-8) contains supplementary material, which is available to authorized users. |
format | Online Article Text |
id | pubmed-6529039 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2019 |
publisher | Springer Berlin Heidelberg |
record_format | MEDLINE/PubMed |
spelling | pubmed-65290392019-06-07 Empirical investigation of friction weakening of terrestrial and Martian landslides using discrete element models Borykov, Timur Mège, Daniel Mangeney, Anne Richard, Patrick Gurgurewicz, Joanna Lucas, Antoine Landslides Original Paper Understanding what controls the travelling distance of large landslides has been the topic of considerable debate. By combining observation and experimental data with depth-averaged continuum modelling of landslides and generated seismic waves, it was empirically observed that lower effective friction had to be taken into account in the models to reproduce the dynamics and runout distance of larger volume landslides. Moreover, such simulation and observation results are compatible with a friction weakening with velocity as observed in earthquake mechanics. We investigate here as to whether similar empirical reduced friction should be put into discrete element models (DEM) to reproduce observed runout of large landslides on Earth and on Mars. First we show that, in the investigated parameter range and for a given volume, the runout distance simulated by 3D DEM is not much affected by the number (i.e. size) of grains once this number attains ~ 8000. We then calibrate the model on laboratory experiments and simulate other experiments of granular flows on inclined planes, making it possible for the first time to reproduce the observed effect of initial volume and aspect ratio on runout distances. In particular, the normalised runout distance starts to depend on the volume involved only above a critical slope angle > 16–19°, as observed experimentally. Finally, based on field data (volume, topography, deposit), we simulate a series of landslides on simplified inclined topography. The empirical friction coefficient, calibrated to reproduce the observed runout for each landslide, is shown to decrease with increasing landslide volume (or velocity), going down to values as low as 0.1–0.2. No distinguishable difference is observed between the behaviour of terrestrial and Martian landslides. ELECTRONIC SUPPLEMENTARY MATERIAL: The online version of this article (10.1007/s10346-019-01140-8) contains supplementary material, which is available to authorized users. Springer Berlin Heidelberg 2019-03-01 2019 /pmc/articles/PMC6529039/ /pubmed/31178675 http://dx.doi.org/10.1007/s10346-019-01140-8 Text en © The Author(s) 2019 OpenAccessThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. |
spellingShingle | Original Paper Borykov, Timur Mège, Daniel Mangeney, Anne Richard, Patrick Gurgurewicz, Joanna Lucas, Antoine Empirical investigation of friction weakening of terrestrial and Martian landslides using discrete element models |
title | Empirical investigation of friction weakening of terrestrial and Martian landslides using discrete element models |
title_full | Empirical investigation of friction weakening of terrestrial and Martian landslides using discrete element models |
title_fullStr | Empirical investigation of friction weakening of terrestrial and Martian landslides using discrete element models |
title_full_unstemmed | Empirical investigation of friction weakening of terrestrial and Martian landslides using discrete element models |
title_short | Empirical investigation of friction weakening of terrestrial and Martian landslides using discrete element models |
title_sort | empirical investigation of friction weakening of terrestrial and martian landslides using discrete element models |
topic | Original Paper |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6529039/ https://www.ncbi.nlm.nih.gov/pubmed/31178675 http://dx.doi.org/10.1007/s10346-019-01140-8 |
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