2022
DOI: 10.1016/j.jvolgeores.2022.107611
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Real-time tephra-fallout accumulation rates and grain-size distributions using ASHER (ASH collector and sizER) disdrometers

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Cited by 4 publications
(3 citation statements)
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“…The fact that bimodal fallout deposits, such as the one at Llaima (Figure 8), are relatively rare suggests effective particle size segregation occurs near the vent in most cases. On the other hand, hindered settling accounts for reduced particle settling velocity, otherwise explained by non spherical particle shape or the presence of wind (Marchetti et al., 2022). In a broader context, hindered settling is likely to occur in various types of geophysical flows containing particles with Stokes number ≫1, and our experiments suggest that this mechanism can operate at concentrations as low as ∼1 vol.%, which may be surprising.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…The fact that bimodal fallout deposits, such as the one at Llaima (Figure 8), are relatively rare suggests effective particle size segregation occurs near the vent in most cases. On the other hand, hindered settling accounts for reduced particle settling velocity, otherwise explained by non spherical particle shape or the presence of wind (Marchetti et al., 2022). In a broader context, hindered settling is likely to occur in various types of geophysical flows containing particles with Stokes number ≫1, and our experiments suggest that this mechanism can operate at concentrations as low as ∼1 vol.%, which may be surprising.…”
Section: Discussionmentioning
confidence: 99%
“…Instead, if the particles are not suspended, they settle to form a deposit or a dense basal flow controlled by particle‐particle interactions. Experimental and numerical studies revealed that the particle settling velocity may increase (Dey et al., 2019; Wang & Maxey, 1993) or decrease (Dey et al., 2019; Fornari et al., 2016; Nielsen, 1993) depending on the degree of turbulence, and it can be lower (Marchetti et al., 2022) or higher (Del Bello et al., 2017) than predicted theoretically for a single particle depending on the particle size, shape, and concentration. Actual particle settling velocities different from theoretical velocities used in models may be a cause of discrepancies between observed and simulated volcanic fall deposits (Tadini et al., 2020, 2022) and this issue is critical in the context of hazard assessment.…”
Section: Introductionmentioning
confidence: 99%
“…Continuous processing and automation of astrometry data collected by the Gemini Observatory on Mauna Kea (Figure 1) would be helpful for quantifying plume heights. The development and deployment of an automated ash sampling array (Marchetti et al., 2022; Shimano et al., 2013) could provide a continuous record of tephra fall. Time‐constrained tephra records would inform ongoing ash dispersal modeling, provide context for radar and satellite analysis and yield a valuable tephra‐sample data set for petrology and ash morphology analyses.…”
Section: Discussionmentioning
confidence: 99%