What happens when a pyroclastic flow enters the water: numerical modelling of an offshore pyroclastic turbidite

Peter James Rowley, Dave Waltham, Andrew Hogg, Fukashi Maeno, Stuart McLean, Stephen Sparks, Peter Talling, Jessica Trofimovs, Sebastian Watt

    Research output: Contribution to conferencePoster

    Abstract

    Tis work explores whether the dispersal of material as a pyroclastic flow enters the ocean can be modelled as a turbidity current, and hence elucidate the inititaion, propagation and deposition conditions during these poorly understood events. We simulate the main pulse of the 2003 dome collapse at Soufrière Hills, Montserrat, which propagated down the far valley, into the ocean. The extensive dataset includes vibrocore sediment samples of the submarine deposit, high resolution bathymetry (Figure 1), duration estimates from seismometers,and descriptions of the terrestrial portion of flow and deposit.Our work assumes a debris-type flow travelled descended the proximal flank of Montserrat, elutriating the finer frraction which propagated as a turbulent density current across thebasin

    1
    Original languageEnglish
    Publication statusPublished - 2013
    EventIAVCEI General Assembly - Kagoshima, Japan
    Duration: 20 Jul 201324 Jul 2013

    Conference

    ConferenceIAVCEI General Assembly
    Country/TerritoryJapan
    CityKagoshima
    Period20/07/1324/07/13

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    • IAVCEI General Assembly

      Peter Rowley (Speaker)

      2013

      Activity: Participating in or organising an event typesParticipation in conference

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