A model for steady flows of magma-volatile mixtures
Marco Belan, Enzo Cataldo

TL;DR
This paper introduces a versatile one-dimensional steady flow model for magma-volatile mixtures in vertical ducts, useful for understanding volcanic eruptions on Earth and planetary bodies, with an implementation that allows flexible hypothesis testing.
Contribution
It presents a symbolic, user-friendly code for modeling steady magma-volatile flows, incorporating an inverse problem approach and applying it to planetary and terrestrial scenarios.
Findings
Realistic eruption descriptions for Earth and Io
Versatile symbolic code for flow analysis
Insights into conduit shapes and flow properties
Abstract
A general one-dimensional model for the steady adiabatic motion of liquid-volatile mixtures in vertical ducts with varying cross-section is presented. The liquid contains a dissolved part of the volatile and is assumed to be incompressible and in thermomechanical equilibrium with a perfect gas phase, which is generated by the exsolution of the same volatile. An inverse problem approach is used -- the pressure along the duct is set as an input datum, and the other physical quantities are obtained as output. This fluid-dynamic model is intended as an approximate description of magma-volatile mixture flows of interest to geophysics and planetary sciences. It is implemented as a symbolic code, where each line stands for an analytic expression, whether algebraic or differential, which is managed by the software kernel independently of the numerical value of each variable. The code is…
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Taxonomy
TopicsAstro and Planetary Science · Planetary Science and Exploration · Methane Hydrates and Related Phenomena
