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Understanding caldera structure and development: An overview of analogue models compared to natural calderas
Institution:1. Dipartimento di Scienze della Terra e Geoambientali, Via Orabona 4, 70125, Bari, Italy;2. Istituto Nazionale di Geofisica e Vulcanologia, Via Donato Creti 12, 40128, Bologna, Italy;1. Institute of Geological Sciences, University of Bern, Baltzerstrasse 1 & 3, CH 3012, Bern, Switzerland;2. Geodynamics Team, Geological Survey of Norway, 7491, Trondheim, Norway;3. The Centre for Earth Evolution and Dynamics, University of Oslo, PO Box 1048, Blindern, 0316, Oslo, Norway;4. Department of Geology, University of Toronto, 22 Russell St., M5S 3B1, Toronto, Ontario, Canada;5. Hans Ramberg Tectonic Laboratory, Department of Earth Sciences, Uppsala University, Villavägen, S-75326, Uppsala, Sweden;6. IFP Energies Nouvelles, 1 et 4 avenue de Bois Préau, F-92500, Rueil Malmaison, Cedex, France;7. NEXT – Natural and Experimental Tectonics Research Group, Department of Physics and Earth Sciences “Macedonio Melloni”, University of Parma, Via G. Usberti 157/A, I-43100, Parma, Italy;8. Universidad Nacional Autonoma de Mexico, Centro de Geociencias, Blvd Juriquilla 3001, Juriquilla, Queretaro, 76230, Mexico;9. Department of Geosciences, National Taiwan University, 1 Roosevelt Road Section 4, Taipei, 106, Taiwan;10. Departamento de Ciencias Geológicas, Universidad de Buenos Aires, Pabellón II, Ciudad Universitaria, C1428EHA, Buenos Aires, Argentina;11. Department of Geology, University of Toronto, 22 Russell St., Toronto, Ontario, M5S 3B1, Canada;12. Department of Geological and Environmental Sciences, Stanford University, Braun Hall 215, Stanford, CA, 94305-2115, USA;13. Departamento de Geologia, Universidade Federal de Ouro Preto, Morro do Cruzeiro s/n, 35, 400-000, Ouro Preto, Minas Gerais, Brazil;14. Université Lille-Nord de France, Laboratoire Géosystèmes, FRE CNRS 3298, 59655, Villeneuve d’Ascq, Cedex, France;15. Department of Earth and Planetary Sciences, Rutgers University, 610 Taylor Road, Piscataway, NJ, 08854-8066, USA;p. Department of Geological and Environmental Sciences, Braun Hall 233, Stanford University, Stanford, CA, 94305-2115, USA;q. Department of Geosciences, National Taiwan University, 1 Roosevelt Road, Taipei, 106, Taiwan;r. Laboratoire Géosciences et Environnement Cergy, Université de Cergy-Pontoise, 5 Mail Gay-Lussac, Neuville-sur-Oise, 95031, Cergy-Pontoise, Cedex, France;s. School of Earth, Atmosphere and Environment, Monash University, Melbourne, Victoria, 3800, Australia;t. Helmholtz-Centre Potsdam, GFZ German Research Centre for Geosciences, Telegrafenberg, D-14473, Potsdam, Germany;u. Department of Civil Engineering, Queen''s University, Kingston, Ontario, K7L 3N6, Canada;v. Université Lille, UMR 8187, LOG, Laboratoire d’Océanologie et de Géosciences, F 59000, Lille, France;w. Department of Civil and Earth Resources Engineering, Kyoto University, Kyoto, 615-8540, Japan;1. Geological Survey of Japan, AIST, 1-1-1 Higashi, Tsukuba, Ibaraki 305-8567, Japan;2. Dip. Scienze Geologiche Roma Tre, Largo S. L. Murialdo 1, 00146, Roma, Italy
Abstract:Understanding the structure and development of calderas is crucial for predicting their behaviour during periods of unrest and to plan geothermal and ore exploitation. Geological data, including that from analysis of deeply eroded examples, allow the overall surface setting of calderas to be defined, whereas deep drillings and geophysical investigations provide insights on their subsurface structure. Collation of this information from calderas worldwide has resulted in the recent literature in five main caldera types (downsag, piston, funnel, piecemeal, trapdoor), being viewed as end-members. Despite its importance, such a classification does not adequately examine: (a) the structure of calderas (particularly the nature of the caldera's bounding faults); and (b) how this is achieved (including the genetic relationships among the five caldera types). Various sets of analogue models, specifically devoted to study caldera architecture and development, have been recently performed, under different conditions (apparatus, materials, scaling parameters, stress conditions).The first part of this study reviews these experiments, which induce collapse as a result of underpressure or overpressure within the chamber analogue. The experiments simulating overpressure display consistent results, but the experimental depressions require an exceptional amount of doming, seldom observed in nature, to form; therefore, these experiments are not appropriate to understand the structure and formation of most natural calderas. The experiments simulating underpressure reveal a consistent scenario for caldera structure and development, regardless of their different boundary conditions. These show that complete collapse proceeds through four main stages, proportional to the amount of subsidence, progressively characterized by: (1) downsag; (2) reverse ring fault; (3) peripheral downsag; (4) peripheral normal ring fault.The second part of this study verifies the possibility that these latter calderas constitute a suitable analogue to nature and consists of a comprehensive comparison of the underpressure experiments to natural calderas. This shows that all the experimental structures, as well as their progressive development, are commonly observed at natural calderas, highlighting a consistency between models and nature. As the shallow structure of experimental calderas corresponds to a precise architecture at depth, it provides a unique key to infer the deeper structure of natural calderas: recognizing diagnostic surface features within a caldera will thus allow it to be categorized within a precise structural and evolutionary context. The general relationship between the evolutionary stage of a caldera and its d/s (diameter/subsidence) ratio allows such a quantification, with stage 1 calderas characterized by d/s > 40, stage 2 by 18 < d/s < 40, stage 3 by 14 < d/s < 18 and stage 4 by d/s < 14. The consistency between experiments and nature suggests that, in principle, the d/s ratio may permit to evaluate the overall structure and evolutionary stage of a caldera even when its surface structure is poorly known. The volume of erupted magma associated with caldera collapse is poorly dependent on the d/s ratio or evolutionary stage; however, the location of sin- and post-collapse volcanism may depend not only upon the amount of collapse, but also on the roof aspect ratio. As the regional tectonic control is concerned, the experiments explain the ellipticity of a part of natural calderas elongated parallel to the regional extension; the control of pre-existing structures may explain the elongation of elliptic calderas oblique or parallel to the regional structures.The four stages adequately explain the architecture and development of the established caldera end-members along a continuum, where one or more end-members (downsag, piston, funnel, piecemeal, trapdoor) may correspond to a specific stage. While such a continuum is controlled by progressive subsidence, specific collapse geometries will result from secondary contributory factors (roof aspect ratio, collapse symmetry, pre-existing faults). These considerations allow proposing an original classification of calderas, incorporating their structural and genetic features.
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