Energy stability of magnetohydrodynamic flow in channels and ducts

Fuente: arXiv
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Autori principali: Boeck, Thomas, Brynjell-Rahkola, Mattias, Duguet, Yohann
Natura: Preprint
Pubblicazione: 2024
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author Boeck, Thomas
Brynjell-Rahkola, Mattias
Duguet, Yohann
author_facet Boeck, Thomas
Brynjell-Rahkola, Mattias
Duguet, Yohann
contents We study the energy stability of pressure-driven laminar magnetohydrodynamic flow in a rectangular duct with transverse homogeneous magnetic field and electrically insulating walls. For sufficiently strong fields, the laminar velocity distribution has a uniform core and convex Hartmann and Shercliff boundary layers on the walls perpendicular and parallel to the magnetic field. The problem is discretized by a double expansion in Chebyshev polynomials in the cross-stream coordinates. The linear eigenvalue problem for the critical Reynolds number depends on the streamwise wavenumber, Hartmann number and the aspect ratio. We consider the limits of small and large aspect ratios in order to compare with stability models based on one-dimensional base flows. For large aspect ratios we find good numerical agreement with results based on the quasi-two-dimensional approximation. The lift-up mechanism dominates in the limit of zero streamwise wavenumber and provides a linear dependence between the critical Reynolds and Hartmann number in the duct. The duct results for small aspect ratio converge to Orr's original energy stability result for spanwise uniform perturbations imposed on the plane Poiseuille base flow. We also examine different possible symmetries of eigenmodes as well as the purely hydrodynamic case in the duct geometry.
format Preprint
id arxiv_https___arxiv_org_abs_2404_08802
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Energy stability of magnetohydrodynamic flow in channels and ducts
Boeck, Thomas
Brynjell-Rahkola, Mattias
Duguet, Yohann
Fluid Dynamics
We study the energy stability of pressure-driven laminar magnetohydrodynamic flow in a rectangular duct with transverse homogeneous magnetic field and electrically insulating walls. For sufficiently strong fields, the laminar velocity distribution has a uniform core and convex Hartmann and Shercliff boundary layers on the walls perpendicular and parallel to the magnetic field. The problem is discretized by a double expansion in Chebyshev polynomials in the cross-stream coordinates. The linear eigenvalue problem for the critical Reynolds number depends on the streamwise wavenumber, Hartmann number and the aspect ratio. We consider the limits of small and large aspect ratios in order to compare with stability models based on one-dimensional base flows. For large aspect ratios we find good numerical agreement with results based on the quasi-two-dimensional approximation. The lift-up mechanism dominates in the limit of zero streamwise wavenumber and provides a linear dependence between the critical Reynolds and Hartmann number in the duct. The duct results for small aspect ratio converge to Orr's original energy stability result for spanwise uniform perturbations imposed on the plane Poiseuille base flow. We also examine different possible symmetries of eigenmodes as well as the purely hydrodynamic case in the duct geometry.
title Energy stability of magnetohydrodynamic flow in channels and ducts
topic Fluid Dynamics
url https://arxiv.org/abs/2404.08802