Title
Magmatic gas percolation through the old lava dome of El Misti volcano
Date Issued
01 June 2017
Access level
open access
Resource Type
journal article
Author(s)
Moussallam Y.
Peters N.
Barnie T.
Ian Schipper C.
Curtis A.
Tamburello G.
Aiuppa A.
Bani P.
Giudice G.
Pieri D.
Davies A.G.
Oppenheimer C.
Publisher(s)
Springer Verlag
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.
Volume
79
Issue
6
Language
English
OCDE Knowledge area
Geología
Vulcanología
Subjects
Scopus EID
2-s2.0-85019729861
Source
Bulletin of Volcanology
ISSN of the container
02588900
Sponsor(s)
This research was conducted as part of the ‘Trail By Fire’ expedition (PI: Y. Moussallam). The project was supported by the Royal Geographical Society (with the Institute of British Geographers) with the Land Rover Bursary; the Deep Carbon Observatory DECADE Initiative; Santander, Ocean Optics; Crowcon; Air Liquide; Thermo Fisher Scientific; Cactus Outdoor; Turbo Ace and Team Black Sheep. We thank Jean-loup Guyot, Sebastien Carretier, Rose-Marie Ojeda, Pablo Samaniego and Jean-Luc Lepennec together with IRD South-America personnel for all their logistical help. We are extremely grateful to Marco Rivera and all OVI personnel for their help and support. YM acknowledges support from the Scripps Institution of Oceanography Postdoctoral Fellowship program. A.A and G.T acknowledge the ERC grant no. 305377 (BRIDGE). CIS acknowledges a research start-up grant from Victoria University of Wellington. C.O. is supported by the NERC Centre for the Observation and Modelling of Earthquakes, Volcanoes and Tectonics. The Earth Observing-1 (EO-1) spacecraft is managed by NASA’s Goddard Space Flight Center, Greenbelt, Maryland, USA. We thank Daniel Tran, Steve Chien and Joshua Doubleday (all JPL) and Stuart Frye (GSFC) for their assistance in acquiring EO-1 data. We are very grateful to James White, Patrick Allard and an anonymous reviewer for comments which significantly improved the quality of this manuscript.
Sources of information:
Directorio de Producción Científica
Scopus