Convection in a mushy layer along a vertical heated wall

Motivated by the mushy zones of sea ice, volcanoes and icy moons of the outer solar system, we perform a theoretical and numerical study of boundary-layer convection along a vertical heated wall in a bounded ideal mushy region. The mush is comprised of a porous and reactive binary alloy with a mixtu...

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Bibliografski detalji
Glavni autori: Boury, S, Meyer, CR, Vasil, GM, Wells, AJ
Format: Journal article
Jezik:English
Izdano: Cambridge University Press 2021
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author Boury, S
Meyer, CR
Vasil, GM
Wells, AJ
author_facet Boury, S
Meyer, CR
Vasil, GM
Wells, AJ
author_sort Boury, S
collection OXFORD
description Motivated by the mushy zones of sea ice, volcanoes and icy moons of the outer solar system, we perform a theoretical and numerical study of boundary-layer convection along a vertical heated wall in a bounded ideal mushy region. The mush is comprised of a porous and reactive binary alloy with a mixture of saline liquid in a solid matrix, and is studied in the near-eutectic approximation. Here, we demonstrate the existence of four regions and study their behaviour asymptotically. Starting from the bottom of the wall, the four regions are (i) an isotropic corner region; (ii) a buoyancy dominated vertical boundary layer; (iii) an isotropic connection region; and (iv) a horizontal boundary layer at the top boundary with strong gradients of pressure and buoyancy. Scalings from numerical simulations are consistent with the theoretical predictions. Close to the heated wall, the convection in the mushy layer is similar to a rising buoyant plume abruptly stopped at the top, leading to increased pressure and temperature in the upper region, whose impact is discussed as an efficient melting mechanism.
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spelling oxford-uuid:4038a79e-d71d-41da-828e-8c51fc1f9b0b2022-03-26T14:36:44ZConvection in a mushy layer along a vertical heated wallJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:4038a79e-d71d-41da-828e-8c51fc1f9b0bEnglishSymplectic ElementsCambridge University Press2021Boury, SMeyer, CRVasil, GMWells, AJMotivated by the mushy zones of sea ice, volcanoes and icy moons of the outer solar system, we perform a theoretical and numerical study of boundary-layer convection along a vertical heated wall in a bounded ideal mushy region. The mush is comprised of a porous and reactive binary alloy with a mixture of saline liquid in a solid matrix, and is studied in the near-eutectic approximation. Here, we demonstrate the existence of four regions and study their behaviour asymptotically. Starting from the bottom of the wall, the four regions are (i) an isotropic corner region; (ii) a buoyancy dominated vertical boundary layer; (iii) an isotropic connection region; and (iv) a horizontal boundary layer at the top boundary with strong gradients of pressure and buoyancy. Scalings from numerical simulations are consistent with the theoretical predictions. Close to the heated wall, the convection in the mushy layer is similar to a rising buoyant plume abruptly stopped at the top, leading to increased pressure and temperature in the upper region, whose impact is discussed as an efficient melting mechanism.
spellingShingle Boury, S
Meyer, CR
Vasil, GM
Wells, AJ
Convection in a mushy layer along a vertical heated wall
title Convection in a mushy layer along a vertical heated wall
title_full Convection in a mushy layer along a vertical heated wall
title_fullStr Convection in a mushy layer along a vertical heated wall
title_full_unstemmed Convection in a mushy layer along a vertical heated wall
title_short Convection in a mushy layer along a vertical heated wall
title_sort convection in a mushy layer along a vertical heated wall
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AT meyercr convectioninamushylayeralongaverticalheatedwall
AT vasilgm convectioninamushylayeralongaverticalheatedwall
AT wellsaj convectioninamushylayeralongaverticalheatedwall