File:Puquios Chaos.jpg

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Español: a) From the 31CH road to the southeast (Fig. 3), the boudined, folded and faulted limestones blocks of the Puquios chaos stand out at the forefront. At the top

of the hill, the allochthon IV shows the original succession of volcanic rocks at the base and limestones towards the top that constitute the Cerro Águila strata. b) Erosive contact between the Puquios chaos underlying the Paleogene volcanosedimentary rocks of the Venado Formation. This erosive contact constitutes the western limit of the tectonic unit. c) Configuration of the southeastern part of the study area. The Puquios detachment put into contact the Allochthons IV (Cerro Águila strata) and II (La Ternera Formation). The Puquios chaos is underthrusted by the Triassic rocks of the La Ternera Formation through a late (probably Eocene) reverse fault. d) Contact between the andesitic rocks (down) that comprise the matrix of the Puquios chaos and the calcareous stratified rocks. Acronyms (CA1 and

CA2) are referred to the local geology (Fig. 2b). e) Packstone-grainstone rocks with tractive structures (ripples of probably sinuous crest)
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current23:13, 8 August 2020Thumbnail for version as of 23:13, 8 August 20202,481 × 3,508 (4.18 MB)FSERSA (talk | contribs)Cross-wiki upload from es.wikipedia.org

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