2016
DOI: 10.1016/j.jvolgeores.2016.01.016
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An expansion–coalescence model to track gas bubble populations in magmas

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Cited by 13 publications
(7 citation statements)
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“…Because bubble diffusion is typically negligibly small, bubble walls can only approach when a particular mechanism leads to differential bubble rise velocities or by bubble growth. In magmas with a sufficiently separated bubble flow, two neighbouring bubbles of different size can approach each other vertically due to the differential buoyancy velocities (Manga and Stone, 1994;Lovejoy et al, 2004). In magmas with a dispersed bubble flow, in contrast, the relative position of bubble centres remains fixed; thus, bubble coalescence is controlled by the bubble expansion rate caused by the ascent of the overall magma column (or affected magma parcel).…”
Section: Bubble Motion and Bubble Coalescencementioning
confidence: 99%
“…Because bubble diffusion is typically negligibly small, bubble walls can only approach when a particular mechanism leads to differential bubble rise velocities or by bubble growth. In magmas with a sufficiently separated bubble flow, two neighbouring bubbles of different size can approach each other vertically due to the differential buoyancy velocities (Manga and Stone, 1994;Lovejoy et al, 2004). In magmas with a dispersed bubble flow, in contrast, the relative position of bubble centres remains fixed; thus, bubble coalescence is controlled by the bubble expansion rate caused by the ascent of the overall magma column (or affected magma parcel).…”
Section: Bubble Motion and Bubble Coalescencementioning
confidence: 99%
“…Mesoscopic models represent intermediate models that describe, through a set of mesoscale variables, the microphysics of the system. The formulation of population balance requires adequate closure models for the microphysics that can be developed with the aid of experimental (Mancini et al, 2016) and DNS investigations (Marchisio and Fox, 2013). The inclusion of Lagrangian tracers will result in a more detailed description, with respect to multi-fluid models, of the microphysics that determine the macroscopic properties driving the dynamics.…”
Section: Discussionmentioning
confidence: 99%
“…Bubbles typically vary in size following a power law (Cashman and Marsh, 1988;Blower et al, 2003) and in shape from spherical to ellipsoidal (Rust et al, 2003;Moitra et al, 2013). While models based on polydisperse bubble size distributions are available (Sahagian and Proussevitch, 1998;Huber et al, 2013;Mancini et al, 2016), a common starting point to analyse the temporal evolution of 25 the bubbles is nevertheless the assumption of a monodisperse size distribution of spherical bubbles (Prousevitch et al, 1993;Lensky et al, 2004).…”
Section: Gas Bubbles In Magmatic Meltmentioning
confidence: 99%