4.3 Article

Geomorphology and structural development of the nested summit crater of Lascar Volcano studied with Terrestrial Laser Scanner data and analogue modelling

Journal

JOURNAL OF VOLCANOLOGY AND GEOTHERMAL RESEARCH
Volume 329, Issue -, Pages 1-12

Publisher

ELSEVIER
DOI: 10.1016/j.jvolgeores.2016.09.018

Keywords

Lascar Volcano; Terrestrial Laser Scanner (TLS); Geomorphology; Nested craters; Sandbox modelling

Funding

  1. Helmholtz Alliance Remote Sensing and Earth System Dynamics (HGF EDA)
  2. TOPOMOD
  3. VOLCAPSE (ERC-COG) [646858]
  4. GFZ
  5. European Research Council (ERC) [646858] Funding Source: European Research Council (ERC)

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Many volcano summits host craters that are partially overlapping. The formation of such nested craters has been commonly interpreted as vent migration. Here, we present an additional mechanism that may explain the geometry of nested craters at volcanoes. Lascar Volcano, the most active volcano of the Central Volcanic Zone in the Chilean Andes, hosts ENE-WSW trending summit craters that are partially overlapping (nested). Details on the evolution and interaction between the different craters remain unclear. To create a robust dataset, Terrestrial Laser Scanner (TLS) data were collected at the summit of Lascar in 2013. The resulting topographic data set, consisting of more than 15 million data points with centimetre sampling, allows visualising almost the complete eastern edifice of the volcano's summit. From the TLS data, a Digital Elevation Model (DEM) and a slope map were generated allowing us to create a lineament map and quantify the observed morphological and structural features. To further improve our understanding, of the processes responsible for the formation of the craters and geomorphology, we designed sandbox analogue models. Results suggest that one of the craters is a 'parasite' crater, formed as a consequence of ongoing activity in the adjacent crater. Our data suggest that the nested craters have all been modified since the last major eruption in 1993, by near surface effects associated with cooling, compaction and gravitational sliding of the crater floor infill. As the active crater deepens, the adjacent inactive crater extends and partially slumps towards the active one. Understanding the structural development of these nested craters is relevant for assessing potential future eruption sites, thus making Lascar a dynamic target for a detailed morphology study. These findings may similarly be applied to other volcanoes, where nested craters have developed. (C) 2016 Elsevier B.V. All rights reserved.

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