The objective of this work is to analyze the impact magneto-hydrodynamics flow across a stretching layer in existing magnetic sector. classifying boundary equations are converted set non-linear by taking advantage similarity structures. transformed scheme mathematically resolved homotopy analysis method. Results measured numerically and plotted graphically for velocity temperature distribution....

We review the main properties of shell models for magnetohydrodynamic (MHD) turbulence. After a brief account on shell models with nearest neighbour interactions, the paper focuses on the most recent results concerning dynamical properties and intermittency of a model which is a generalization to MHD of the Gledzer-Yamada-Okhitani (GOY) model for hydrodynamic. Applications to astrophysical prob...

Examinations of the magnetohydrodynamic (MHD) equations across a bow shock are presented. These equations are written in the familiar Rankine–Hugoniot set, and an exact solution to this set is given which involves the upstream magnetosonic Mach number, plasma , polytropic index, and B v , as a function of position along the shock surface. The asymptotic Mach cone angle of the shock surface is a...

The study of the problem of Magneto Hydrodynamic viscous flow due to a shrinking sheet of Micropolar fluids has been solved numerically by using SOR method with Simpson (1/3) Rule. The similarity transformations have been used to reduce the highly nonlinear partial differential equations of motion to ordinary differential equations. The resulting equations are then integrated by using appropria...

Heating from active galactic nuclei (AGN) is thought to stabilize cool-core clusters, limiting star formation and cooling flows. We employ radiative magneto-hydrodynamic (MHD) simulations model light AGN jet feedback with different accretion modes (Bondi-Hoyle-Lyttleton cold accretion) in an idealised Perseus-like cluster. Independent of the probed model, efficiency, density resolution, cluster...

This communication deals with the properties of heat source/sink in a magneto-hydrodynamic flow of a non-Newtonian fluid immersed in a porous medium. Shrinking phenomenon along with the permeability of the wall is considered. Mathematical modelling is performed to convert the considered physical process into set of coupled nonlinear mathematical equations. Suitable transformations are invoked t...

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