1. Porous Melt Flow in Continental Crust—A Numerical Modeling Study.
- Author
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Maierová, P., Hasalová, P., Schulmann, K., Štípská, P., and Souček, O.
- Subjects
CONTINENTAL crust ,DIAPIRS ,ELECTRIC conductivity ,SEISMIC wave velocity ,ROCK properties ,MELTING - Abstract
In continental crust, rapid melt flow through macroscopic conduits is usually envisaged as the most efficient form of melt transport. In contrast, there is growing evidence that in hot continental crust, grain‐scale to meso‐scale porous melt flow may operate over long distances and over millions of years. Here, we investigate the dynamics of such porous melt flow by means of two‐dimensional thermo‐mechanical numerical models using the code ASPECT. Our models are crustal‐scale and describe the network of pores through which the melt flows by permeability that depends on the spacing of the pores. Our results suggest that assuming realistic material properties, melt can slowly migrate in the hot and thick continental crust through pores with a characteristic spacing of 1 mm or larger. Despite its low velocity (millimeters to centimeters per year), over millions of years, such flow can create large partially molten zones in the middle‐lower crust and significantly affect its thermal state, deformation, and composition. We examined the role of the permeability, melt and solid viscosities, the slope of the melting curve and temperature conditions. We obtained contrasting styles of melt distribution, melt flow, and solid deformation, which can be categorized as melt‐enhanced convection, growth of partially molten diapirs and melt percolation in porosity waves. Our numerical experiments further indicate that grain‐scale porous flow is more likely in rocks where the melt productivity increases slowly with temperature, such as in metaigneous rocks. Plain Language Summary: Continental crust contains a significant proportion of rocks that can melt relatively easily. Geophysical methods that measure, for example, seismic velocities or electric conductivity revealed large partially molten regions in the continental crust. In addition, solidified melt pathways (veins, dykes) are often observed in rocks that were formerly in hot continental interiors. Usually, melt flow through macroscopic pathways is assumed to be the most efficient type of melt transport. However, several geological studies have shown that melt may flow through much finer (microscopic) pores, which form a network along boundaries of rock grains. The question arises, how efficient this microscopic melt flow is, and how it affects the properties of the continents. We address this issue using numerical models. According to our models, microscopic melt flow is very slow—melt moves millimeters to centimeters per year. Despite its low velocity, over millions of years, it forms large partially molten zones, significantly increases the temperature in the crust, changes its composition and softens it. The style of this process varies notably depending on the rock properties and temperature conditions. For example, in some models, kilometer‐sized melt batches move through nearly immobile rock, while in others, melt and rock both move together as a stirred mush. Key Points: Numerical thermo‐mechanical models simulate porous melt flow through hot felsic continental crustMelt can propagate through pores with the spacing of 1 mm or larger with a velocity of millimeters to centimeters per year and form large partially molten zonesStyle of melt flow and solid deformation vary between melt‐enhanced convection, diapirism, and porosity waves depending on model parameters [ABSTRACT FROM AUTHOR]
- Published
- 2023
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