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      • KCI등재

        Impact of Magnetic Field and Second-Order Slip Flow of Casson Liquid with Heat Transfer Subject to Suction/Injection and Convective Boundary Condition

        Aaqib Majeed,Ahmad Zeeshan,Tariq Mahmood,Shafiq Ur Rahman,Imran Khan 한국자기학회 2019 Journal of Magnetics Vol.24 No.1

        The present article is planned theoretically to throw light on non-Newtonian Casson liquid flow and heat transport analysis over an exponentially stretching sheet with second-order velocity slip condition. The analysis of magneto-hydrodynamic (MHD) is an important interdisciplinary field. One of the most imperative applications related to engineering problems is plasma confinement, liquid-metal cooling of nuclear reactors, and electromagnetic casting. The flow here is considered to be electrically conducting. The modelled equations of mass, momentum and energy transport are reduced into the nonlinear ordinary differential equations by employing a similarity approach which are then solved numerically by employing finite difference collocation process (a three-stage Lobatto IIIa scheme). The inspiration of convergence flow parameters on dimensionless velocity, temperature have been discussed graphically. The obtained results confirm that an excellent agreement is achieved for the Newtonian case with those available in the literature. Consequences establish that skin friction rises in the presence of Casson fluid parameter and the Nusselt number show enhancement for second order slip parameter.

      • SCIESCOPUSKCI등재

        Hall Current and Viscous Dissipation Impact on MHD Mixed Convection Flow towards a Porous Exponentially Surface with its Engineering Applications

        Aaqib Majeed,Ahmad Zeeshan,Aqila Shaheen,Mohammed Sh. Alhodaly,Farzan Majeed Noori 한국자기학회 2022 Journal of Magnetics Vol.27 No.2

        Power generators, Hall accelerators, and flight MHD all require high levels of Hall current. The influence of Hall current and viscous dissipation on time-independent hydro-magnetic mixed convective radiative flow across a porous heated surface has thus been investigated using numerical computing and mathematical modeling in the current study. The fluid is electrically conducted and varies exponentially. It is assumed that the wall temperature and elongation rate will vary with specific exponential shapes. A solid uniform magnetic field B0 is employed normally to the surface. The mathematical model of PDEs for incompressible flow is transformed into ODE by applying a numerical technique based on a finite-difference structure which includes a three-stage Lobatto IIIa scheme with the help of MATLAB. The obtained solution depends on the convergence constraints involving the radiation parameter R, magnetic parameter M, porosity parameter Ω, Hall parameter m, buoyancy parameter ε, temperature distribution parameter a, Eckert number Ec, Prandtl number Pr, and convective term bh. Graphs of the velocity and temperature profiles are explained via pertinent parameters. Skin friction factor, and Nusselt number are also evaluated and presented graphically and in tabular form. Results clarify that temperature profile reduces by increasing values of temperature distribution parameter whereas opposite behavior is noted for positive values of the buoyancy parameter.

      • KCI등재

        Numerical Investigations of Radiative Flow of Viscous Fluid Through Porous Medium

        Tasawar Abbas,Bilal Ahmad,Aaqib Majeed,Taseer Muhammad,Muhammad Ismail 한국자기학회 2021 Journal of Magnetics Vol.26 No.3

        This study incorporates the numerical behavior of radiative flow of electrically conductive viscous fluid though porous medium with slip effects. The boundary is supposed to be convective during the flow. The governing nonlinear partial differential equations are transformed into its corresponding ode’s with the help of suitable similarity transformations. Numerical technique is used to solve the system of ordinary differential equations. Effects of pertinent parameters on velocity and fluid temperature are plotted graphically. The velocity of fluid reduces due to opposing force offer by magnetic field whereas temperature rises.

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