4.6 Article

Topographic precursors and geological structures of deep-seated catastrophic landslides caused by Typhoon Talas

Journal

GEOMORPHOLOGY
Volume 201, Issue -, Pages 479-493

Publisher

ELSEVIER
DOI: 10.1016/j.geomorph.2013.07.020

Keywords

Deep-seated catastrophic landslide; Gravitational slope deformation; High-resolution DEM; Scarp; Pre-failure displacement

Funding

  1. Japanese Ministry of Education, Culture, Sports, Science and Technology
  2. Grants-in-Aid for Scientific Research [23310126] Funding Source: KAKEN

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Typhoon Talas crossed the Japanese Islands between 2 and 5 September 2011, causing more than 70 deep-seated catastrophic landslides in a Jurassic to Paleogene-lower Miocene accretion complex. Detailed examination of the topographic features of 10 large landslides before the event, recorded on 1-m DEMs based on airborne laser scanner surveys, showed that all landslides had small scarps near their future crowns prior to the slide, and one landslide had linear depressions along its future crown as precursor topographic features. These scarps and linear depressions were caused by gravitational slope deformation that preceded the catastrophic failure. Although the scarps may have been enlarged by degradation, their sizes relative to the whole slopes suggest that minimal slope deformation had occurred in the period immediately before the catastrophic failure. The scarp ratio, defined as the ratio of length of a scarp to that of the whole slope both measured along the slope line, ranged from 5% to 21%. Careful examination of aerial photographs from another four large landslides, for which no high-resolution DEMs were available, suggested that they also developed scarps at their heads beforehand. Twelve of the 14 landslides we surveyed in the field had sliding surfaces with wedge-shaped discontinuities that consisted of faults and bedding, suggesting that the buildup of pore pressure occurs readily on wedge-shaped discontinuities in a gravitationally deformed rock body. Most of the faults were undulatory and were probably thrust faults that formed during accretion. Other types of gravitational deformation were also active: e.g., flexural toppling and buckling were observed to have preceded one landslide. (C) 2013 Elsevier B.V. All rights reserved.

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