Abstract

The sedimentation rate of volcanic ash through the atmosphere influences its travel distance, with important implications for aviation and health. The fall velocity of a particle depends on its size and density, but also shape, and volcanic ash is not spherical. To capture the sedimentation of ash, atmospheric dispersion models use empirical drag equations calibrated using geometric shape descriptors. However, particle shape data are scarce and there is no standard method of shape measurement. In addition, shape measurements are not always available during an eruption, when dispersion models are used operationally to forecast ash hazard. We assess the variability in the shape of volcanic ash from Icelandic eruptions using X-ray computed tomography. To consider how good different drag equations and shape descriptors are at representing the sedimentation of volcanic ash we compare calculated fall velocities to measured fall velocities of volcanic ash in air in a settling column. We then suggest the best drag equations and shape descriptors for use in atmospheric dispersion models. We find that shape-dependent drag equations produce more accurate results than a spherical approximation. However, accurate drag calculations based on the shape descriptor sphericity, which is a function of surface area, require the imaging resolution to be within the range of 102 - 105 voxels per particle (where a voxel is a volumetric pixel) as surface area is sensitive to imaging resolution. We suggest that the large-scale form of the particle impacts sedimentation more than small-scale surface roughness. Shape descriptors based on ratios between principal axis lengths are more practical as they are less variable among particle size classes and much less sensitive to imaging resolution. Finally, we use particle shape data from this study and literature sources to make recommendations on default values for use with atmospheric dispersion models where no shape data are available.

Highlights

  • Volcanic ash can remain in the atmosphere from minutes to days or longer after a large explosive eruption (Durant et al, 2010); the rate of removal from the atmosphere depends on meteorological processes and particle terminal fall velocity

  • To assess the effectiveness of the shape descriptors in anticipating particle fall velocity, we measure the terminal velocity of selected mm-sized tephra particles in a settling column and compare the results to calculated terminal velocities using empirical drag equations with our measured shape parameters. From this we provide guidance on the best theoretical approach for use in atmospheric dispersion models to represent the sedimentation of volcanic ash particles

  • As shape can be sensitive to imaging resolution, we investigated the impact of voxel size on measured shape factors using X-ray computed tomography (CT) data for 16 individual particles

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Summary

Introduction

Volcanic ash (tephra particles with diameters < 2 mm) can remain in the atmosphere from minutes to days or longer after a large explosive eruption (Durant et al, 2010); the rate of removal from the atmosphere depends on meteorological processes and particle terminal fall velocity. For the Ganser (1993) drag equation, which uses the shape factor sphericity that is very sensitive to imaging resolution, we first recalculate terminal velocity using every value of sphericity obtained from resampling the CT data for the 16 high resolution scans

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