2022
DOI: 10.5194/egusphere-egu22-12185
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The permeability of loose magma mush

Abstract: <div><strong><strong>Large-volume rhyolitic eruptions are characteristically crystal-poor yet are thought to originate from crystal rich magma mush bodies. This contradiction is explained by the interstitial melt being extracted prior to the eruption, generating large volumes of crystal-poor magmas. The timescale for melt extraction is inversely correlated to the permeability of the mush, defined by the shape of the crystals. Yet, existing approaches for estimating the… Show more

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Cited by 2 publications
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“…Also shown are the data from Bretagne et al. (2023) for cuboid simulations, and the model (Equation 4) with C = 5 and for a best fit value of C = 4.01. For comparison, we also show hard sphere simulations from Vasseur et al.…”
Section: Results and Analysismentioning
confidence: 99%
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“…Also shown are the data from Bretagne et al. (2023) for cuboid simulations, and the model (Equation 4) with C = 5 and for a best fit value of C = 4.01. For comparison, we also show hard sphere simulations from Vasseur et al.…”
Section: Results and Analysismentioning
confidence: 99%
“…We perform this minimization using all data (including the numerical cuboid data from Bretagne et al. (2023) or with each data set individually (Table 2, Figure 3b) and show the result with the best‐fit C for the combination of the fudge and sugar crystals (i.e., C = 4.01 ± 0.24). Zoomed in, the data fall closer to the model using C = 4.01 (Figure 3b).…”
Section: Results and Analysismentioning
confidence: 99%
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