On the modelling of rotational effects in the lower convective region of the sun

Abstract

The purpose of this work is to study effects of differential rotation in the lower convective region of the Sun. Similar to MHD case; the governing equations are separated in variables, allowing numerical integration in this layer. This algorithm facilitates solutions of more complicated systems, with less computing time. Two different known rotation profiles are used in order to fit the model. The fitting procedure is accomplished by making use of sphericity and density shape parameters related to the rotation profiles. It is also shown that the most important feature of rotation is to break the spherical symmetric distribution of density in this layer. As in the MHD effects found before, differential rotation changes considerably the density of the reference model for both cases.

MHD and Thermal Radiation Effects on Rotating Fluid Past a Moving Vertical Plate with Heat and Mass Transfer in the Presence of Chemical Reaction, OHMIC Heating

“…Cavus and Karafistan [8] studied the effects of differential rotation in the lower convective region of the Sun, Ch Kesavaiah et.al. [7] has effects of the chemical reaction and radiation absorption on an unsteady MHD convective heat and mass transfer flow past a semi-infinite vertical permeable moving plate embedded in a porous medium with heat source and suction, Bhavana et.al [12] investigated the Soret effect on free convective unsteady MHD flow over a vertical plate with heat source. However, MHD effects on a moving infinite vertical plate in a rotating fluid with mass transfer in the presence of thermal radiation is not studied in the literature.…”