2009
DOI: 10.1029/2008jb005946
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Shape and volume change of pressurized ellipsoidal cavities from deformation and seismic data

Abstract: 1] We present exact expressions for the volume change of a pressurized ellipsoidal cavity in an infinite homogeneous elastic medium. The expressions can be used as approximate solutions also for a homogeneous half-space. We show that previously published widely used expressions are correct for spheres but underestimate the ratio of the volume change to the product of pressure and volume in any other case. We discuss the capability to infer the shape of a single ellipsoidal cavity from far-field deformation mea… Show more

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Cited by 90 publications
(118 citation statements)
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“…The ratio of the extruded magma volume to the deflation volume (Rv) is 1.8 ± 0.5. The value is affected not only by the magma compressibility (Rivelta and Segall, 2008) but also by the shape of the magma reservoir (Amoruso and Crescentini, 2009). Rivalta and Segall (2008) pointed out that the ratio should be greater than one if the magma within the reservoir is compressible.…”
Section: Discussionmentioning
confidence: 99%
“…The ratio of the extruded magma volume to the deflation volume (Rv) is 1.8 ± 0.5. The value is affected not only by the magma compressibility (Rivelta and Segall, 2008) but also by the shape of the magma reservoir (Amoruso and Crescentini, 2009). Rivalta and Segall (2008) pointed out that the ratio should be greater than one if the magma within the reservoir is compressible.…”
Section: Discussionmentioning
confidence: 99%
“…For a spherical chamber in an elastic full-space, b ch = 3/4m where m is the shear modulus of the elastic medium [McTigue, 1987]; however, this result does not hold for nonspherical shapes [Amoruso and Crescentini, 2009]. Using the finite element method we numerically compute b ch for chambers with aspect ratios w ranging from 0.05 to 20 in an elastic half-space with n = 0.25 and m = 20 GPa.…”
Section: Magma Chambermentioning
confidence: 99%
“…Penny-shaped cracks (left) become highly compressible, while vertical pipe-like chambers (right) become only somewhat more compressible than the sphere. Analytical expressions and results from Amoruso and Crescentini [2009] are shown for a sphere, penny-shaped crack (with n = 0.25), and highly elongate vertical prolate ellipsoid (all in elastic full-spaces); the latter two are end-member cases so their horizontal position on the axes is approximate. Analytical approximations fail most significantly with shallow penny-shaped chambers.…”
Section: Numerical Solutionmentioning
confidence: 99%
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“…Source depth depends on a range of factors relating to buoyancy, magma composition, stress conditions and pre-existing structural features (e.g., Chaussard & Amelung, 2014), as well as conditions that promote the amalgamation of lenses of melt and volatiles in a mush system to form larger bodies of eruptible magma (e.g., Cashman et al, 2017). We do not discuss estimations of volume change here, because it is strongly dependent on the reservoir or intrusion compressibility, which is very poorly constrained, and depends on both magma and exsolved gas compressibilities as well as source geometry and material properties of the surrounding rock (e.g., Rivalta and Segall, 2008;Amoruso and Crescentini, 2009;McCormick Kilbride et al, 2016). Modelled source depth is recorded for some deformation episodes by both VOTW and COMET, and we build on this by including further preferred deformation source depths from publications (including any estimation of uncertainty provided).…”
Section: Derived Deformation Source Parametersmentioning
confidence: 99%