1992
DOI: 10.1007/bf00569939
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Cooling of tephra during fallout from eruption columns

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Cited by 100 publications
(56 citation statements)
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“…Vesicle shapes formed during ascent within the conduit may be modified after fragmentation by bubble growth (e.g., Thomas and Sparks 1992;Kaminsky and Jaupart 1997) and shape relaxation due to capillary forces (e.g., Klug and Cashman 1996). However, for silicic and for microlite-rich basaltic magmas, post-fragmentation bubble growth should be of limited extent, due to permeable outgassing (e.g., Rust and Cashmann 2011;Gonnermann and Houghton 2012).…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…Vesicle shapes formed during ascent within the conduit may be modified after fragmentation by bubble growth (e.g., Thomas and Sparks 1992;Kaminsky and Jaupart 1997) and shape relaxation due to capillary forces (e.g., Klug and Cashman 1996). However, for silicic and for microlite-rich basaltic magmas, post-fragmentation bubble growth should be of limited extent, due to permeable outgassing (e.g., Rust and Cashmann 2011;Gonnermann and Houghton 2012).…”
Section: Resultsmentioning
confidence: 99%
“…Moreover, the characteristic time scale for shape relaxation, τ relaxation , would need to be much shorter than the characteristic quenching time, τ quenching . To evaluate the effect of post-fragmentation shape relaxation, we estimate τ quenching ∼ 100 s for centimeter-size pyroclasts following the approach of Thomas and Sparks (1992). For Vulcanian, Plinian, ultraplinian, and basaltic Plinian eruptions, τ relaxation = ηR/σ ∼ 10 3 to 10 5 s τ quenching (assuming that the viscosity in the case of the basaltic Plinian magmas accounts for the effect of microlites).…”
Section: Resultsmentioning
confidence: 99%
“…After expelling up to 0.5 km 3 of dacite (~0.25 km 3 DRE) and 0.35 km 3 of andesite (~0.17 km 3 DRE), the eruptive regime dramatically increased, three orders of magnitude in volume, and generated deposits that completely covered the northeast part of Umnak Island. Most likely, the pyroclastic current deposits are responsible for the charred vegetation buried underneath the fall deposits because the fall deposits were not hot enough to char vegetation when they were deposited (Thomas and Sparks 1992). The pyroclastic deposits, however, were not hot enough to cause welding or scoria oxidation, which suggests that their temperature was between 200 and 600 °C (Riehle 1973).…”
Section: Eruption Dynamicsmentioning
confidence: 99%
“…In order to achieve this the Roza fountains needed to be high (>> 504 1 km) and sedimentation from the fountains needed to be enhanced by fallout of coarse, hot 505 pyroclasts from the lower parts of associated convecting plumes of potentially Subplinian to Plinian 506 intensity (e.g., Thomas and Sparks, 1992 linked to bubble rise and coalescence, degassing processes and melt rheology driven by microlite 535 crystallisation (Houghton and Gonnermann, 2008). An in-depth discussion of the parameters 536 controlling more vigorously explosive phases of the Roza eruption is beyond the scope of this paper 537 and will be dealt with in a future publication.…”
Section: Fountain and Eruption Dynamics 476mentioning
confidence: 99%