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 ...

Abstract— The Plasma resistivity has been measured in the

edge plasma of IR-T1 tokamak. To achive the edge plasma

properties ( Te and ne ) using I-V characteristics of

movable single langmuir probe. ...

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 investigate the effect of self gravity on the equilibrium structure of a thick non rotating disk around a central object by the self similar method. We introduce three dimensionless variables Csg, Ct & Ck that indicate ...

MHD or Magnetic hydro dynamics of an open cavity with three different depths is investigated numerically

in this paper. The SIMPLE algorithm is utilized in order to solve the equations of conservation of

momentum and energy...

Dynamics of clumps within a magnetized advection-dominated accretion flow is investigated

by solving the collisionless Boltzmann equation and considering the drag force due to the

relative velocity between ...

The existence of outflow and magnetic fields in the inner region of hot

accretion flows has been confirmed by observations and numerical magnetohydrodynamic

(MHD) simulations. We present self-similar solutions for radiatively...

The combined impact of rotation and magnetic fields on oscillations of stellar fluids is still

not well known theoretically. It mixes Alfv´en and inertial waves. Neutron stars are a place

where both effects ...

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 ...