Radiative non-coaxial rotating flow for viscous fluid over accelerated disk with MHD and porosity effects

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...

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Main Authors: Wan Nura’in Nabilah Noranuar, Ahmad Qushairi Mohamad, Lim, Yeou Jiann, Sharidan Shafie, Ling, Dennis Chuang Ching
Format: Article
Language:English
Published: Penerbit Universiti Kebangsaan Malaysia 2022
Online Access:http://journalarticle.ukm.my/20471/1/25.pdf
http://journalarticle.ukm.my/20471/
https://www.ukm.my/jsm/malay_journals/jilid51bil8_2022/KandunganJilid51Bil8_2022.html
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Institution: Universiti Kebangsaan Malaysia
Language: English
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spelling my-ukm.journal.204712022-11-10T07:40:08Z http://journalarticle.ukm.my/20471/ Radiative non-coaxial rotating flow for viscous fluid over accelerated disk with MHD and porosity effects Wan Nura’in Nabilah Noranuar, Ahmad Qushairi Mohamad, Lim, Yeou Jiann Sharidan Shafie, Ling, Dennis Chuang Ching 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. Penerbit Universiti Kebangsaan Malaysia 2022-08 Article PeerReviewed application/pdf en http://journalarticle.ukm.my/20471/1/25.pdf Wan Nura’in Nabilah Noranuar, and Ahmad Qushairi Mohamad, and Lim, Yeou Jiann and Sharidan Shafie, and Ling, Dennis Chuang Ching (2022) Radiative non-coaxial rotating flow for viscous fluid over accelerated disk with MHD and porosity effects. Sains Malaysiana, 51 (8). pp. 2669-2680. ISSN 0126-6039 https://www.ukm.my/jsm/malay_journals/jilid51bil8_2022/KandunganJilid51Bil8_2022.html
institution Universiti Kebangsaan Malaysia
building Tun Sri Lanang Library
collection Institutional Repository
continent Asia
country Malaysia
content_provider Universiti Kebangsaan Malaysia
content_source UKM Journal Article Repository
url_provider http://journalarticle.ukm.my/
language English
description 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.
format Article
author Wan Nura’in Nabilah Noranuar,
Ahmad Qushairi Mohamad,
Lim, Yeou Jiann
Sharidan Shafie,
Ling, Dennis Chuang Ching
spellingShingle Wan Nura’in Nabilah Noranuar,
Ahmad Qushairi Mohamad,
Lim, Yeou Jiann
Sharidan Shafie,
Ling, Dennis Chuang Ching
Radiative non-coaxial rotating flow for viscous fluid over accelerated disk with MHD and porosity effects
author_facet Wan Nura’in Nabilah Noranuar,
Ahmad Qushairi Mohamad,
Lim, Yeou Jiann
Sharidan Shafie,
Ling, Dennis Chuang Ching
author_sort Wan Nura’in Nabilah Noranuar,
title Radiative non-coaxial rotating flow for viscous fluid over accelerated disk with MHD and porosity effects
title_short Radiative non-coaxial rotating flow for viscous fluid over accelerated disk with MHD and porosity effects
title_full Radiative non-coaxial rotating flow for viscous fluid over accelerated disk with MHD and porosity effects
title_fullStr Radiative non-coaxial rotating flow for viscous fluid over accelerated disk with MHD and porosity effects
title_full_unstemmed Radiative non-coaxial rotating flow for viscous fluid over accelerated disk with MHD and porosity effects
title_sort radiative non-coaxial rotating flow for viscous fluid over accelerated disk with mhd and porosity effects
publisher Penerbit Universiti Kebangsaan Malaysia
publishDate 2022
url http://journalarticle.ukm.my/20471/1/25.pdf
http://journalarticle.ukm.my/20471/
https://www.ukm.my/jsm/malay_journals/jilid51bil8_2022/KandunganJilid51Bil8_2022.html
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