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The effects of variable viscosity and thermal conductivity on mhd flow due to a point sink.
(2011-10-13)
A theoretical investigation of the influence of variable viscosity and thermal conductivity on the
MHD boundary layer flow due to a point sink is presented. Both the fluid viscosity and thermal
conductivity are assumed ...
Exploring various flux vector splittings for the magneto hydrodynamic system
(Elsevier, 2016)
In this paper we explore flux vector splittings for the MHD system of equations. Our approach follows the strategy that was initially put forward in Toro and Vazquez-Cendon (2012) [55]. We split the flux vector into an ...
Magnetic fields in protoplanetary discs: from MHD simulations to ALMA observations
(Oxford University Press, 2017-01)
Magnetic fields significantly influence the evolution of protoplanetary discs and the formation of planets, following the predictions of numerous magnetohydrodynamic (MHD) simulations. However, these predictions are yet ...
Study of fractal features of magnetized plasma through an MHD shell model
(American Institute of Physics, 2017)
A magnetohydrodynamic (MHD) shell model is used to describe the dissipative events which take place in magnetized plasmas. A scatter plot box-counting fractal dimension D is calculated for the time series of the magnetic ...
Study of the fractality of magnetized plasma using an MHD shell model driven by solar wind data
(American Institute of Physics Inc., 2018)
An MHD shell model is used to describe the dissipative events that take place in magnetized plasmas. We analyze the activity of the time series of the magnetic energy dissipation rate obtained in the MHD shell model, which ...
Two-fluid simulations of the magnetic field evolution in neutron star cores in the weak-coupling regime
(Oxford University Press, 2020)
In a previous paper, we reported simulations of the evolution of the magnetic field in neutron star (NS) cores through ambipolar diffusion, taking the neutrons as a motionless uniform background. However, in real NSs, ...
On magnetic equilibria in barotropic stars
(IOP PUBLISHING, 2015)
Upper main-sequence stars, white dwarfs, and neutron stars are known to possess stable, large-scale magnetic fields. Numerical works have confirmed that stable magnetohydrodynamic equilibria can exist in non-barotropic, ...