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AGU: Geophysical Research Letters

 

Index Terms

  • Atmospheric Composition and Structure: Aerosols and particles
  • Atmospheric Composition and Structure: Volcanic effects
  • Volcanology: Atmospheric effects
  • Volcanology: Instruments and techniques

Abstract

Dynamics of giant volcanic ash clouds from supervolcanic eruptions

P. G. Baines

University of Melbourne, Department of Civil and Environmental Engineering, Melbourne, Victoria, Australia

University of Bristol, School of Mathematics, Bristol, UK

R. S. J. Sparks

University of Bristol, Department of Earth Sciences, Bristol, UK

The largest explosive volcanic eruptions that have occurred on Earth generated giant ash clouds from rising plumes that spread in the stratosphere around a height of neutral buoyancy, with estimated supply rates that are in the range 1011 to 1013 m3/s. These giant ash clouds are controlled by a balance between gravity and Coriolis forces, forming spinning bodies of nearly fixed proportions after a few hours and are initially insensitive to stratospheric winds. In contrast, volcanic plumes from eruptions with small to intermediate magnitude spread as inertial intrusions under the influence of stratospheric winds, with the Earth's rotation being unimportant. In the largest eruptions the giant spinning ash clouds typically develop diameters greater than 600 km and up to 6000 km in the most powerful super-eruptions, thus explaining why areas of continental size can be covered with volcanic ash. The radial expansion and spinning velocities are calculated at tens of metres per second and increase with eruption intensity. Higher spreading velocities carry larger ash grain sizes to a given radius, so that grain size at a given distance from the source increases with eruption intensity, consistent with geological observations.

Received 13 September 2005; accepted 11 November 2005; published 23 December 2005.

Citation: Baines, P. G., and R. S. J. Sparks (2005), Dynamics of giant volcanic ash clouds from supervolcanic eruptions, Geophys. Res. Lett., 32, L24808, doi:10.1029/2005GL024597.

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