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- A New Implementation of a Fourth-Order CESE Scheme for 3D MHD . . .
This paper is devoted to the description and validation of a new implementation of a fourth-order space–time conservation-element and solution-element (CESE) scheme to numerically solve the time-dependent, three-dimensional (3D) magnetohydrodynamic (MHD) equations
- A projection method for the non-stationary incompressible MHD coupled . . .
In this paper, we introduce a linearized projection scheme for non-stationary incompressible coupled the MHD with heat equations, which buoyancy affects because temperature differences in the flow cannot be neglected
- A high-order CESE scheme with a new divergence-free method for MHD . . .
In this paper, we give a high-order space–time conservation element and solution element (CESE) method with a most compact stencil for magneto-hydrodynamics (MHD) equations This is the first study to extend the second-order CESE scheme to a high order for MHD equations
- Abstract. arXiv:2305. 14820v1 [math. NA] 24 May 2023
memethod for the ideal magnetohydrodynamics (MHD) As a distinctive feature, the method simultaneously preserves two critical physical constraints: a discretely divergence-free (DDF) constraint on the magnetic field and the positivity-preserving (PP) property, which ensures the po
- A CHARGE-CONSERVATIVE FINITE ELEMENT METHOD FOR INDUCTIONLESS MHD . . .
To design such liquid metal blankets, numerical simulations of incompressible MHD play an important role in knowing the characteristics of MHD ows at high Hartmann numbers
- A Novel Fully Decoupled Scheme for the MHD System with Va. . .
In this paper, we first establish a novel first-order, fully decoupled, unconditionally stable time discretization scheme for the MHD system with variable density
- A New MHD Model with a Rotated-hybrid Scheme and Solenoidality . . .
In this paper, the rotated-hybrid scheme is applied for the first time to 3D magnetohydrodynamics (MHD) equations in the finite-volume frame
- ComputationMHD1 - Tsinghua University
MHD provides accurate description of collisional plasmas MHD is often reasonably OK to describe the large-scale phenomenon (even) for collisionless plasmas Computational MHD has been
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