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Large-eddy simulation of magnetohydrodynamic turbulence [PDF]

Computer Physics Communications, 2002
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Muller, Wolf-Christian, Carati, Daniele
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Lattice kinetic simulation of nonisothermal magnetohydrodynamics

Physical Review E, 2010
In this paper, a lattice kinetic algorithm is presented to simulate nonisothermal magnetohydrodynamics in the low-Mach number incompressible limit. The flow and thermal fields are described by two separate distribution functions through respective scalar kinetic equations and the magnetic field is governed by a vector distribution function through a ...
Dipankar, Chatterjee, Sakir, Amiroudine
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Global magnetohydrodynamic simulations on multiple GPUs

Computer Physics Communications, 2014
Abstract Global magnetohydrodynamic (MHD) models play the major role in investigating the solar wind–magnetosphere interaction. However, the huge computation requirement in global MHD simulations is also the main problem that needs to be solved. With the recent development of modern graphics processing units (GPUs) and the Compute Unified Device ...
Un-Hong Wong, Hon-Cheng Wong, Yonghui Ma
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Maintaining Pressure Positivity in Magnetohydrodynamic Simulations

Journal of Computational Physics, 1999
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Balsara, Dinshaw S., Spicer, Daniel
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Implementation of the CIP algorithm to magnetohydrodynamic simulations

Computer Physics Communications, 2008
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Yosuke Matsumoto, Kanako Seki
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Lattice Boltzmann model for simulation of magnetohydrodynamics

Physical Review Letters, 1991
A numerical method, based on a discrete Boltzmann equation, is presented for solving the equations of magnetohydrodynamics (MHD). The algorithm provides advantages similar to the cellular automaton method in that it is local and easily adapted to parallel computing environments.
, Chen, , Chen, , Martnez, , Matthaeus
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Global magnetohydrodynamic simulations of the magnetosphere

IEEE Transactions on Plasma Science, 1989
The authors demonstrate the use of a global MHD (magnetohydrodynamic) simulations to study the magnetospheric configuration by reviewing some of the results obtained from the Ogino model. The authors start by considering the steady-state configuration of the magnetosphere in the absence of an IMF (interplanetary magnetic field), and then demonstrate ...
R.J. Walker, T. Ogino
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Three-dimensional Magnetohydrodynamical Simulations of the Morphology of Head–Tail Radio Galaxies Based on the Magnetic Tower Jet Model

Astrophysical Journal, 2017
The distinctive morphology of head–tail radio galaxies reveals strong interactions between the radio jets and their intra-cluster environment, the general consensus on the morphology origin of head–tail sources is that radio jets are bent by violent ...
Hui Li, Zhaoming Gan
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Numerical Simulation of Magnetohydrodynamic Flows

Journal of Spacecraft and Rockets, 2004
The development of a versatile computational tool for the solution of turbulent magnetohydrodynamic flows is presented. The flow solver can simulate the full magnetohydrodynamic equations or simplified equations based on the low magnetic Reynolds number approximation. Both laminar and turbulent flows are investigated. The Baldwin‐Lomax turbulence model
Jean-Francois Dietiker, Klaus A. Hoffmann   +1 more
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Magnetohydrodynamic Pump Work Simulation

2018 International Russian Automation Conference (RusAutoCon), 2018
Magnetohydrodynamic pump (MHD-pump) is used for high-temperature metal fusions delivery. Herewith, it does not get in contact with a fusion itself, does not have mobile elements and is not vulnerable to consumption. But its low efficiency and absence of a dose delivery system restrict its usage in other spheres.
Ivan Martynovich, Artem Avdeev, Alexey Drobotov   +2 more
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