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Abstract

The 12 to 13 July 2003 andesite lava dome collapse at the Soufrière Hills volcano, Montserrat, provides the first opportunity to document comprehensively both the sub-aerial and submarine sequence of events for an eruption. Numerous pyroclastic flows entered the ocean during the collapse, depositing approximately 90\% of the total material into the submarine environment. During peak collapse conditions, as the main flow penetrated the air\textendashocean interface, phreatic explosions were observed and a surge cloud decoupled from the main flow body to travel 2 to 3 km over the ocean surface before settling. The bulk of the flow was submerged and rapidly mixed with sea water forming a water-saturated mass flow. Efficient sorting and physical differentiation occurred within the flow before initial deposition at 500 m water depth. The coarsest components (\~60\% of the total volume) were deposited proximally from a dense granular flow, while the finer components (\~40\%) were efficiently elutriated into the overlying part of the flow, which evolved into a far-reaching turbidity current.

Year of Publication
2008
Journal
Sedimentology
Volume
55
Number of Pages
617-634
ISBN Number
1365-3091
URL
http://dx.doi.org/10.1111/j.1365-3091.2007.00914.x
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