Deposits from dome-collapse and fountain-collapse pyroclastic flows at Soufrière Hills Volcano, Montserrat

Author:

Cole P. D.1,Calder E. S.2,Sparks R. S. J.2,Clarke A. B.3,Druitt T. H.4,Young S. R.5,Herd R. A.6,Harford C. L.2,Norton G. E.6

Affiliation:

1. Centre for Volcanic Studies, University of LutonPark Square, Luton, LU1 3JU, UK (Paul.Cole@luton.ac.uk)

2. Department of Earth Sciences, University of BristolQueens Road, Bristol, BS8 1 RJ. UK

3. Department of Geosciences, Penn State University503 Deike Building, University Park, PA 16802 2714, USA

4. Department des Sciences de la Terre (UMR 6524 et CNRS), Université Blaise Pascal63038 Clermont Ferrand, France

5. British Geological Survey, Murchison HouseWest Mains Road, Edinburgh, EH9 3LA, UK

6. British Geological SurveyKeyworth, Nottingham, NG12 5GG, UK (Paul.Cole@luton.ac.uk)

Abstract

abstractPyroclastic flows were formed at Soufrière Hills Volcano by lava-dome collapse and by fountain collapse associated with Vulcanian explosions. Major episodes of dome collapse, lasting tens of minutes to a few hours, followed escalating patterns of progressively larger flows with longer runouts. Block-and-ash flow deposit volumes range from <0.1 to 25 x 106 m3 with runouts of 1-7 km. The flows formed coarse-grained block-and-ash flow deposits, with associated fine-grained pyroclastic surge deposits and ashfall deposits. Small flows commonly formed lobate channelized deposits. Large block-and-ash flows in unconfined areas produced sheet-like deposits with tapering margins. the development of pyroclastic surges was variable depending on topography and dome pore pressure. Pyroclastic surge deposits commonly had a lower layer poor in fine ash that was formed at the current front and an upper layer rich in fine ash. Block-and-ash flows were erosive, producing striated and scoured bedrock surfaces and forming channels, many metres deep, in earlier deposits. Abundant accidental material was incorporated. Pyroclastic flow deposits formed by fountain collapse were pumiceous, with narrow sinuous, lobate morphologies and well developed levees and snouts. Two coastal fans formed where pyroclastic flows entered the sea. Their seaward extent was limited by a submarine slope break.

Publisher

Geological Society of London

Subject

Geology

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