TY  - JOUR
N2  - An analytical solution to analyze the effects of radiation, magnetic, and permeability in an accelerating non-coaxial rotation phenomenon is not yet reported in the previous studies. Therefore, a radiative mixed convection flow for non-coaxial rotating MHD viscous fluid in a porous medium past an accelerated disk is studied. The fluid motion in this problem is induced by two sources which are rotating and buoyancy force. The dimensional coupled differential equations subjected to initial and accelerated boundary conditions are transformed to the dimensionless equations by utilizing appropriate dimensionless variables. The Laplace transform technique is applied to generate the closed form analytical solution for this problem. The impacts of Prandtl number, Grashof number, radiation, magnetic, porosity, and accelerated parameters on the temperature and velocity fields are illustrated graphically. The velocity and temperature profiles satisfy both the initial and boundary conditions, and the present results are found in accordance to the published work. The velocity is improved with the assistance of acceleration, radiation and porosity, while the implementation of magnetic field causes the opposite effect. Increasing radiation leads to the growth of the thermal boundary layer as well as reducing the heat transmission rate. This result can significantly contribute to the designing of heating systems because the imposition of radiation able to sustain an environment for a specific temperature. The obtained analytical solution can be used to check the correctness of the solution obtained from the numerical and experimental studies. © 2022 Penerbit Universiti Kebangsaan Malaysia. All rights reserved.
IS  - 8
ID  - scholars16495
KW  - heat transfer; Laplace transform; magnetic field; permeability; porosity; radiative forcing; viscoelastic fluid; viscous flow
Y1  - 2022///
A1  - Noranuar, W.N.N.
A1  - Mohamad, A.Q.
A1  - Jiann, L.Y.
A1  - Shafie, S.
A1  - Ching, D.L.C.
JF  - Sains Malaysiana
UR  - https://www.scopus.com/inward/record.uri?eid=2-s2.0-85140321614&doi=10.17576%2fjsm-2022-5108-25&partnerID=40&md5=0456716e4a7012d059e40df53a1b76b3
VL  - 51
AV  - none
N1  - cited By 0
SP  - 2669
TI  - Radiative Non-Coaxial Rotating Flow for Viscous Fluid over Accelerated Disk with MHD and Porosity Effects Aliran Beradiasi yang Berputar Tidak Sepaksi bagi Bendalir Likat Melepasi Cakera Bergerak dengan Kesan Magnetohidrodinamik dan Keliangan
PB  - Penerbit Universiti Kebangsaan Malaysia
SN  - 01266039
EP  - 2680
ER  -