Deep-seated gravitational slope deformations in Sierra Nevada, Spain: insights from InSAR, geomorphic and stability analyses
- 1University of Granada, Granada, Spain (jpgalve@ugr.es)
- 2University of Alicante, Alicante, Spain
- 3University of Milano-Bicocca, Milan, Italy
- 4University of Cantabria, Santander, Spain
- 5University of Urbino "Carlo Bo", Urbino, Italy
- 6National Center-Geological and Mining Institute of Spain from the Spanish Research Council (CN IGME-CSIC), Granada, Spain
Sierra Nevada (Spain) is a mountain range thoroughly studied from a geological-geomorphological perspective due to its anomalously high local relief and the ongoing debate about its origin and geological structure. From the standpoint of slope dynamics, several studies have carried out, but it was not until last year that deep-seated gravitational slope deformations (DSGSDs) were described in this mountain range. Their recognition was facilitated by synergizing geomorphological assessments with data from two well-established techniques: Differential Synthetic Aperture Radar Interferometry (DInSAR) and Landscape Analysis using the normalized channel steepness index (ksn), a geomorphic index commonly used to outline landscape perturbations in tectonically-active mountain ranges. Systematic evaluation of ksn anomalies along rivers illuminated key DSGSD sectors that were studied in detail. This approach resulted in a novel inventory of 17 DSGSDs in the southwestern sector of the range, providing an initial figure of the widespread occurrence of large DSGSDs in Sierra Nevada.
In a second phase, we conducted a detailed study of two slopes affected by DSGSDs in the Poqueira catchment, which provided new insights into Sierra Nevada’s DSGSDs. There, we characterized slope deformations by detailed morpho-structural mapping supported by fieldwork and interpretation of optical and LiDAR-derived imagery, resulting in morpho-structural maps and interpretative cross-sections. Collected data allowed setting up a series of 2DFEM multistage elasto-plastic models, parametrized by laboratory data and field rock mass assessment and validated with field evidence and DInSAR data. The studied cases are characterized by multiple nested landslides that become increasingly shallow, deformed, and active towards the valley. The geometry and kinematics of DSGSDs seem to be partially influenced by the orientation of foliation, indicating rock mass anisotropy, with dip slopes mainly exhibiting translational movements and anti-dip slopes demonstrating prevalence of rotational motions. We tested our initial hypothesis that these slope instabilities in the region were initiated because the development of fluvial incision, favored by the active tectonics and uplifting of the range. Preliminary findings of our analyses suggest that fluvial incision was a key trigger of DSGSDs in Sierra Nevada, but not the only one. Model simulations emphasize that, in addition to fluvial incision, rock mass anisotropy and long-term seismic activity played a crucial role in the onset and accumulation of large deformations of high slopes across the region, favoring the occurrence of significant mass movements. Considering this, rough estimates regarding the timing of incision and seismic activity suggest that initial DSGSD onset took place over a timescale of 104-105 years.
How to cite: Galve, J. P., Reyes-Carmona, C., Agliardi, F., Cannarozzi, M., Pérez-Peña, J. V., Moreno-Sánchez, M., Alfonso-Jorde, D., Ballesteros, D., Torre, D., Azañón, J. M., and Mateos, R. M.: Deep-seated gravitational slope deformations in Sierra Nevada, Spain: insights from InSAR, geomorphic and stability analyses, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-10312, https://doi.org/10.5194/egusphere-egu24-10312, 2024.