Bulletin of Volcanology

, 81:25 | Cite as

Investigation of surge-derived pyroclastic flow formation by numerical modelling of the 25 June 1997 dome collapse at Soufrière Hills Volcano, Montserrat

  • Valentin GueugneauEmail author
  • Karim Kelfoun
  • Timothy Druitt
Research Article


Deposits from ash-cloud surges associated with dome collapse can, under certain conditions, be remobilised to form surge-derived pyroclastic flows (SDPFs). Using numerical modelling, we reproduce the emplacement of these flows and investigate the conditions that favour their genesis. We use the new version of the numerical model VolcFlow, which simulates the two components of a pyroclastic flow: the basal avalanche and the overriding ash-cloud surge. The basal avalanche (primary block-and-ash flows and SDPFs) are simulated using three previously published rheological laws: plastic, frictional and frictional velocity-weakening rheologies. Applied to the 25 June 1997 dome collapse at Soufrière Hills Volcano, the models reproduce to different degrees the deposit footprints formed by the block-and-ash flows, the ash-cloud surges and the SDPFs. In the plastic model, SDPFs occur if the ash-cloud surge deposit exceeds a threshold thickness that allows it to remobilise and flow. In the frictional models, SDPFs occur only if ash-cloud surge deposition takes place on a slope exceeding the friction angle of the ash. Results also highlight that SDPFs appeared so clearly in 1997 at Montserrat due to a combination of topographic factors: (i) a bend in the Mosquito Ghaut drainage that allowed the ash-cloud surges to detach, (ii) a depositional area on the watershed between the eastern and western drainage channels and (iii) a network of tributaries that drained all the remobilised mass into Dyer’s River to form a single, large SDPF. Our model could be a promising tool for the future forecasting of hazards posed by surge-derived pyroclastic flows.


Pyroclastic flows Soufrière Hills Volcano Dome collapse Numerical modelling Rheology Volcanic hazards 



We are very grateful to Dr. Adam Stinton and the Montserrat Volcano Observatory for providing the digital elevation model of Montserrat Island and also Dr. Anne Mangeney for discussions about seismic waves.

Funding information

The development of the numerical code was funded by the Domerapi—ANR (French Agence Nationale de la Recherche) Project (ANR-12-BS06-0012). This research was (partly) supported by the French Government Laboratory of Excellence initiative no. ANR-10-LABX-0006, the Région Auvergne and the European Regional Development Fund. This is Laboratory of Excellence ClerVolc contribution number 336.

Supplementary material

445_2019_1284_MOESM1_ESM.docx (2 mb)
ESM 1 (DOCX 2072 kb)
445_2019_1284_MOESM2_ESM.avi (121.5 mb)
ESM 2 (AVI 124404 kb)


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Copyright information

© International Association of Volcanology & Chemistry of the Earth's Interior 2019

Authors and Affiliations

  1. 1.CNRS, IRD, OPGC, Laboratoire Magmas et VolcansUniversité Clermont AuvergneClermont-FerrandFrance

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