Numerical simulations of highly non-linear coupled full MHD equations in spherical geometry

被引:10
作者
Sekhar, T. V. S. [1 ]
Sivakumar, R. [2 ]
Kumar, T. V. R. Ravi [3 ]
Vimala, S. [1 ]
机构
[1] Pondicherry Engn Coll, Dept Math, Pondicherry 605014, India
[2] Pondicherry Univ, Dept Phys, Pondicherry 605014, India
[3] Kakinada Inst Engn & Technol, Dept Math, Kakinada 533461, India
关键词
Spherical geometry; Full MHD equations; Magnetic Reynolds number; Lorentz force; Control of flow separation; Finite differences; REAR STAGNATION POINT; CONDUCTING FLUID; REYNOLDS-NUMBER; MAGNETIC-FIELD; FLOW; CYLINDER; DRAG; WAKE;
D O I
10.1016/j.ijnonlinmec.2011.10.005
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
Numerical simulations have been performed to solve highly non-linear coupled full MHD equations in spherical polar coordinates. The control of flow separation behind a sphere using Lorentz forces is investigated at moderate magnetic Reynolds numbers. An external magnetic field is applied in the direction of the steady, viscous and electrically conducting flow such that it is aligned at large distances from the sphere. The governing equations are coupled non-linear Navier-Stokes and non-linear Maxwell's equations. The parameters that governs the flow are Reynolds number Re, magnetic Reynolds number R-m and Alfven number beta. The finite difference method combined with multigrid technique is used to solve the full MHD equations which are expressed in vorticity, stream function and magnetic stream function form. All the non-linearities in the momentum equation due to Lorentz force are handled effectively. It is found that the separation for highly conducting fluids can be suppressed with low magnetic fields. The drag coefficient is found to decrease for beta <= 1 and then increase. The results agree with experimental results. (C) 2011 Elsevier Ltd. All rights reserved.
引用
收藏
页码:599 / 615
页数:17
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