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Research Article |
1 Institut de Physique du Globe de Paris & CNRS, Case 89, 4 Place Jussieu, F-75252 Paris Cedex 05, France
2 Department of Earth Sciences, Wills Memorial Building, University of Bristol, Queen's Road, Bristol BS8 1RJ, UK
3 National Oceanography Centre, Waterfront Campus, European Way, Southampton SO14 3ZH, UK
*Corresponding author (e-mail: lefriant{at}ipgp.jussieu.fr)
Soufrière Hills volcano, Montserrat, has been erupting since 1995. During the current eruption, a large part of the material produced by the volcano has been transported into the sea, modifying the morphology of the submarine flanks of the volcano. We present a unique set of swath bathymetric data collected offshore from Montserrat in 1999, 2002 and 2005. From 1999 to 2002, pyroclastic flows associated with numerous dome collapses entered the sea to produce 100 Mm3 deposit. From 2002 to 2005, the 290 Mm3 submarine deposit is mainly from the 12–13 July 2003 collapse. These data allow us to estimate that, by May 2005, at least 482 Mm3 of material had been deposited on the sea floor since 1995. We compare on-land characteristics and volumes of dome collapse events with the submarine deposits and propose a new analysis of their emplacement on the submarine flanks of the volcano. The deposition mechanism shows a slope dependence, with the maximum thickness of deposit before the break in the slope, probably because of the type of the dense granular flow involved. We conclude that from 1995 to 2005 more than 75% of the erupted volume entered the sea.
