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Magmatic gas percolation through the old lava dome of El Misti volcano.
Moussallam, Yves; Peters, Nial; Masias, Pablo; Apaza, Fredy; Barnie, Talfan; Ian Schipper, C; Curtis, Aaron; Tamburello, Giancarlo; Aiuppa, Alessandro; Bani, Philipson; Giudice, Gaetano; Pieri, David; Davies, Ashley Gerard; Oppenheimer, Clive.
Afiliação
  • Moussallam Y; 1Department of Geography, University of Cambridge, Downing Place, Cambridge, CB2 3EN UK.
  • Peters N; 1Department of Geography, University of Cambridge, Downing Place, Cambridge, CB2 3EN UK.
  • Masias P; Observatorio Vulcanológico del Ingemmet (OVI), Arequipa, Peru.
  • Apaza F; Observatorio Vulcanológico del Ingemmet (OVI), Arequipa, Peru.
  • Barnie T; Nordic Volcanological Center, Institute of Earth Sciences, Sturlugata 7 - Askja, 101, Reykjavik, Iceland.
  • Ian Schipper C; 4School of Geography, Environment and Earth Sciences, Victoria University of Wellington, PO Box 600, Wellington, 6140 New Zealand.
  • Curtis A; 5Jet Propulsion Laboratory-California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 USA.
  • Tamburello G; 6Istituto nazionale di geofisica e vulcanologia, sezione di Bologna, Bologna, Italy.
  • Aiuppa A; 7Dipartimento DiSTeM, Università di Palermo, Via archirafi 36, 90146 Palermo, Italy.
  • Bani P; 8Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Palermo Via La Malfa, 153, 90146 Palermo, Italy.
  • Giudice G; 9Université Clermont Auvergne, CNRS, IRD, OPGC, Laboratoire Magmas et Volcans, F-63000 Clermont-Ferrand, France.
  • Pieri D; 8Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Palermo Via La Malfa, 153, 90146 Palermo, Italy.
  • Davies AG; 5Jet Propulsion Laboratory-California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 USA.
  • Oppenheimer C; 5Jet Propulsion Laboratory-California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 USA.
Bull Volcanol ; 79(6): 46, 2017.
Article em En | MEDLINE | ID: mdl-32025076
ABSTRACT
The proximity of the major city of Arequipa to El Misti has focused attention on the hazards posed by the active volcano. Since its last major eruption in the fifteenth century, El Misti has experienced a series of modest phreatic eruptions and fluctuating fumarolic activity. Here, we present the first measurements of the compositions of gas emitted from the lava dome in the summit crater. The gas composition is found to be fairly dry with a H2O/SO2 molar ratio of 32 ± 3, a CO2/SO2 molar ratio of 2.7 ± 0.2, a H2S/SO2 molar ratio of 0.23 ± 0.02 and a H2/SO2 molar ratio of 0.012 ± 0.002. This magmatic gas signature with minimal evidence of hydrothermal or wall rock interaction points to a shallow magma source that is efficiently outgassing through a permeable conduit and lava dome. Field and satellite observations show no evolution of the lava dome over the last decade, indicating sustained outgassing through an established fracture network. This stability could be disrupted if dome permeability were to be reduced by annealing or occlusion of outgassing pathways. Continued monitoring of gas composition and flux at El Misti will be essential to determine the evolution of hazard potential at this dangerous volcano.
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Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2017 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2017 Tipo de documento: Article