1989
DOI: 10.1017/s0022112089001680
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Solitary waves in magma dynamics

Abstract: We investigate the stability of the one-dimensional solitary waves solutions of the equations proposed by McKenzie to model the ascent of melts in the Earth interior. We show that for small porosity and two-dimensional horizontal disturbances with long wavelength, these solitary waves are unstable. We also exhibit two-and threedimensional solitary-wave solutions of the McKenzie equations.

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Cited by 76 publications
(90 citation statements)
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References 14 publications
(16 reference statements)
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“…To test the code, a constant viscosity matrix was set up with a 2D solitary wave initial condition and periodic boundary conditions, and allowed to evolve. As expected, the wave moved without changing form, with a velocity that agreed with that found theoreticany by Barcilon and Lovera [1989] (Fig. la).…”
Section: Gravity Controlled Flowsupporting
confidence: 87%
“…To test the code, a constant viscosity matrix was set up with a 2D solitary wave initial condition and periodic boundary conditions, and allowed to evolve. As expected, the wave moved without changing form, with a velocity that agreed with that found theoreticany by Barcilon and Lovera [1989] (Fig. la).…”
Section: Gravity Controlled Flowsupporting
confidence: 87%
“…Early work on solitary wave solutions in viscous media emphasized distinctions between one-dimensional and multidimensional solutions that are important for the small amplitude waves that initiate in the viscous scenario [Barcilon and Richter, 1986;Barcilon and Lovera, 1989]. The simulations here demonstrate that extraordinary amplitudes may be achieved by waves in a decompaction weakening matrix.…”
Section: Speed and Amplitudementioning
confidence: 64%
“…Note the introduction of the solid matrix velocity v s , as well as the matrix shear and bulk viscosities η , ζ , which arise due to matrix compressibility and depend on the porosity as described below. For nondimensionalization, we follow the scalings described in Spiegelman (1993a) (a similar reduction was performed in Scott & Stevenson (1984; Barcilon & Richter (1986); Barcilon & Lovera (1989)). This requires the introduction of the natural length scale of matrix compaction δ and the natural velocity scale of melt percolation w 0 proposed by McKenzie (1984), which for a background porosity φ 0 are defined as…”
Section: Magma Geophysicsmentioning
confidence: 99%