In this paper, we derive the post-Newtonian equations of the ideal magnetohydrodynamics. To do so, we use the

modern approach to post-Newtonian theory, where the harmonic gauge is used instead of the standard post...

parameters due to last stages of the accretion-flow condition. To resolve the magnetohydrodynamical equations, we were inspired by previous sets of solutions, since the magnetofluid equations are just the same as the fluid ones in the case of vanishing...

We solved the set of two-dimensional magnetohydrodynamic (MHD) equations for optically thin black hole accretion flows incorporating the toroidal component of the magnetic field. Following global and local MHD simulations of black hole accretion...

We have studied the structure of hot accretion flow bathed in a general large-scale magnetic field. We

have considered magnetic parameters βr,ϕ,z[= c2 r,ϕ,z/(2c2 s )], where c2 r,ϕ,z are the Alfvén sound speeds in ...

Control of wake structure may lead to a reduction in the unsteady forces and vibrations in

the marine structures. In this paper, the finite-volume method (FVM) is used to simulate the flow around

two-dimensional ...

We investigate the properties of a hot accretion flow bathed in a poloidal magnetic field. We consider an axisymmetric viscous-resistive flow in the steady-state configuration. We assume that the dominant mechanism of ...

The effect of a uniform magnetic field on the

formation of drops of specific size has been investigated numerically

in a T-shaped microchannel. Previous researches indicated that the

drop sizes of ...

Purpose: The analysis of the flow field and heat transfer around a tube row or tube banks wrapped with porous layer have many related engineering applications. Examples include the reactor safety analysis, combustion, ...