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Geological Society, London, Special Publications; 2006; v. 269; p. 47-63;
DOI: 10.1144/GSL.SP.2006.269.01.04
© 2006 Geological Society of London

Large ignimbrite eruptions and volcano-tectonic depressions in the Central Andes: a thermomechanical perspective

Shanaka De Silva1, George Zandt2, Robert Trumbull3, José G. Viramonte4, Guido Salas5 & Néstor Jiménez6

1 Department of Geosciences, Oregon State University, Corvallis, OR 97331 desilva{at}geo.oregonstate.edu
2 Department of Geosciences, University of Arizona, Tucson, AZ, 85721-0077, USA
3 GeoForschungZentrum Potsdam, Telegrafenberg, PB 4.2, 14473, Potsdam, Germany
4 Instituto GEONORTE and CONICET, Universidad Nacional de Salta, Buenos Aires 177, Salta, 4400, Argentina
5 Facultad de Geología, Geofísica y Minas, Universidad de San Agustín, Arequipa, Peru
6 Facultad de Ciencias Geológicas, Universidad Mayor de San Andrés, La Paz, Bolivia

The Neogene ignimbrite flare-up of the Altiplano Puna Volcanic Complex (APVC) of the Central Andes produced one of the best-preserved large silicic volcanic fields on Earth. At least 15 000 km3 of magma erupted as regional-scale ignimbrites between 10 and 1 Ma, from large complex calderas that are typical volcano-tectonic depressions (VTD). Simple Valles-type calderas are absent. Integration of field, geochronological, petrological, geochemical and geophysical data from the APVC within the geodynamic context of the Central Andes suggests a scenario where elevated mantle power input, subsequent crustal melting and assimilation, and development of a crustal-scale intrusive complex lead to the development of APVC. These processes lead to thermal softening of the sub-APVC crust and eventual mechanical failure of the roofs above batholith-scale magma chambers to trigger the massive eruptions. The APVC ignimbrite flare-up and the resulting VTDs are thus the result of the time-integrated impact of intrusion on the mechanical strength of the crust, and should be considered tectonomagmatic phenomena, rather than purely volcanic features. This model requires a change in paradigm about how the largest explosive eruptions may operate.





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