2015
DOI: 10.1016/j.apm.2014.10.007
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Numerical analysis of Backward-Euler discretization for simplified magnetohydrodynamic flows

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Cited by 24 publications
(17 citation statements)
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“…The stability analysis of partitioned methods for MHD at small magnetic Reynolds number is presented by Layton et al in [3]. Numerical analysis of finite element method with Crank-Nicolson discretization [4] and Backward-Euler discretization [5] are performed by Yuksel et. al.…”
Section: Introductionmentioning
confidence: 99%
“…The stability analysis of partitioned methods for MHD at small magnetic Reynolds number is presented by Layton et al in [3]. Numerical analysis of finite element method with Crank-Nicolson discretization [4] and Backward-Euler discretization [5] are performed by Yuksel et. al.…”
Section: Introductionmentioning
confidence: 99%
“…By applying the idea of Lagrange multiplier to magnetic subproblem, semi-implicit Euler scheme and nodal-based FEMs were studied by Prohl (2008) and Wacker et al (2016), respectively. The backward-Euler scheme was investigated by Yuksel and Isik (2014). We refer the reader to Layton et al (2014) and Ravindran (2008) for more efficient fully discrete schemes for evolutionary MHD equations.…”
Section: Introductionmentioning
confidence: 99%
“…In most terrestrial applications, such as the liquid metal, the magnetic Reynolds number of MHD flows is small. In this article, we study the following MHD equations at small magnetic Reynolds numbers, which are also called simplified MHD equations or reduced MHD equations, see, for example, [2,3,[14][15][16]…”
Section: Introductionmentioning
confidence: 99%
“…In most terrestrial applications, such as the liquid metal, the magnetic Reynolds number of MHD flows is small. In this article, we study the following MHD equations at small magnetic Reynolds numbers, which are also called simplified MHD equations or reduced MHD equations, see, for example, . Given a bounded, Lipschitz domain Ω d ( d = 2 or 3 ) , body force f , magnetic B , and time T > 0 , find fluid velocity u : Ω × [ 0 , T ] d , pressure p : Ω × [ 0 , T ] , and electric potential ϕ : Ω × [ 0 , T ] satisfy left 1 N ( boldu t + u · u ) 1 M 2 Δ u + p = f + B × ϕ + ( u × B ) × B , left · u = 0 , left Δ ϕ = · ( u × B ) , with the homogeneous Dirichlet boundary conditions and the initial condition left u = 0 on Ω × [ 0 , T ] , left …”
Section: Introductionmentioning
confidence: 99%
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