Abstract The transport of waves and turbulence beyond the photosphere is central to coronal heating problem. Turbulence in quiet solar corona has been modeled on basis nearly incompressible magnetohydrodynamic (NI MHD) theory describe low-frequency open magnetic field regions. It describes evolution coupled majority quasi-2D minority slab component, driven by carpet advected a subsonic, sub-Alf...

In this paper, the Ritz-Galerkin method in Bernstein polynomial basis is applied for solving the nonlinear problem of the magnetohydrodynamic (MHD) flow of third grade fluid between the two plates. The properties of the Bernstein  polynomials together with the Ritz-Galerkin method are used to reduce the solution of the MHD Couette flow of non-Newtonian fluid in a porous medium to the solution o...

The meshless local radial point interpolation (MLRPI) method is applied to examine the magnetohydrodynamic (MHD) ow of third grade uid in a porous medium. The uid saturates the porous space between the two boundaries. Several limiting cases of fundamental ows can be obtained as the special cases of present analysis. The variations of pertinent parameters are addressed.