Solar radiation and lower gravitational effects on wave oscillations in heat transfer along magnetic-driven porous cone in the presence of Joule heating
Solar radiation is a very useful form of energy such as heat and current density in gas turbines, nuclear power plants and thermal energy storage. The fundamental source of heat for multiple reactions in the climate, oceans, and ecological system is solar radiation. The current radiative flow model...
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| Format: | Article |
| Language: | English |
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Elsevier
2024-01-01
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| Series: | Case Studies in Thermal Engineering |
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| Online Access: | http://www.sciencedirect.com/science/article/pii/S2214157X23010882 |
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| author | Mohamed Boujelbene Fethi Albouchi Zia Ullah Musaad S. Aldhabani Samirah H. Alsulami Ahmed M. Hassan |
| author_facet | Mohamed Boujelbene Fethi Albouchi Zia Ullah Musaad S. Aldhabani Samirah H. Alsulami Ahmed M. Hassan |
| author_sort | Mohamed Boujelbene |
| collection | DOAJ |
| description | Solar radiation is a very useful form of energy such as heat and current density in gas turbines, nuclear power plants and thermal energy storage. The fundamental source of heat for multiple reactions in the climate, oceans, and ecological system is solar radiation. The current radiative flow model has significant applications in nuclear power generation, radioactive reactor cooling mechanisms, heating boilers, recycling of underground radioactive materials, fabrication of glass-fiber material and thermal textiles. The significance of study to reduce excessive heating by using magnetized surface. The main goal of current research is to report the Joule heating effect on heat and magnetic flux along the magnetic-driven porous cone under solar radiations and lower gravitational region. The novelty of this work is to explore wave oscillations in heat and magnetic flux with solar radiations under lower gravitational region. The Joule heating is applied to control the thermal boundary layer along gravity-driven cone. The coupled mathematical model is changed into non-dimensional form for physical parameters. The steady and oscillatory parts are obtained by using Stokes conditions. For smooth programming in FORTRAN computing tool, the primitive variables are used. The efficient finite difference scheme is used to plot the numerical findings with Gaussian elimination technique. The impact of governing parameters involved in the problem on wave oscillations of magnetic flux and heat transmission are drafted physically and numerically. It is noted that the fluid velocity enhances with significant amplitude as lower gravity and solar radiation increases along porous cone. It is found that wave oscillations of heat and magnetic flux increases as magnetic Prandtl number enhances under lower gravitational region. |
| first_indexed | 2024-03-08T14:36:17Z |
| format | Article |
| id | doaj.art-7d149c74ea5346d98f160409d1cb12f3 |
| institution | Directory Open Access Journal |
| issn | 2214-157X |
| language | English |
| last_indexed | 2024-03-08T14:36:17Z |
| publishDate | 2024-01-01 |
| publisher | Elsevier |
| record_format | Article |
| series | Case Studies in Thermal Engineering |
| spelling | doaj.art-7d149c74ea5346d98f160409d1cb12f32024-01-12T04:56:22ZengElsevierCase Studies in Thermal Engineering2214-157X2024-01-0153103782Solar radiation and lower gravitational effects on wave oscillations in heat transfer along magnetic-driven porous cone in the presence of Joule heatingMohamed Boujelbene0Fethi Albouchi1Zia Ullah2Musaad S. Aldhabani3Samirah H. Alsulami4Ahmed M. Hassan5Industrial Engineering Department, College of Engineering, University of Ha'il, Kingdom of Saudi ArabiaFaculty of Science and Arts (Mohail Asir Campus-Males), King Khalid University, Abha, Kingdom of Saudi ArabiaDepartment of Mathematics and Statistics, The University of Lahore, Sargodha-Campus, 40100, Sargodha, Pakistan; Corresponding author.Department of Mathematics, Faculty of Science, University of Tabuk, P.O.Box 741, Tabuk, 71491, Kingdom of Saudi ArabiaDepartment of Mathematics, Faculty of Science, University of Jeddah, Jeddah, 21959, P.O.Box 34, Kingdom of Saudi ArabiaFaculty of Engineering, Future University in Egypt, New Cario, 11835, EgyptSolar radiation is a very useful form of energy such as heat and current density in gas turbines, nuclear power plants and thermal energy storage. The fundamental source of heat for multiple reactions in the climate, oceans, and ecological system is solar radiation. The current radiative flow model has significant applications in nuclear power generation, radioactive reactor cooling mechanisms, heating boilers, recycling of underground radioactive materials, fabrication of glass-fiber material and thermal textiles. The significance of study to reduce excessive heating by using magnetized surface. The main goal of current research is to report the Joule heating effect on heat and magnetic flux along the magnetic-driven porous cone under solar radiations and lower gravitational region. The novelty of this work is to explore wave oscillations in heat and magnetic flux with solar radiations under lower gravitational region. The Joule heating is applied to control the thermal boundary layer along gravity-driven cone. The coupled mathematical model is changed into non-dimensional form for physical parameters. The steady and oscillatory parts are obtained by using Stokes conditions. For smooth programming in FORTRAN computing tool, the primitive variables are used. The efficient finite difference scheme is used to plot the numerical findings with Gaussian elimination technique. The impact of governing parameters involved in the problem on wave oscillations of magnetic flux and heat transmission are drafted physically and numerically. It is noted that the fluid velocity enhances with significant amplitude as lower gravity and solar radiation increases along porous cone. It is found that wave oscillations of heat and magnetic flux increases as magnetic Prandtl number enhances under lower gravitational region.http://www.sciencedirect.com/science/article/pii/S2214157X23010882Joule heatingLower gravitational regionMagnetic fluxOscillatory heat transferMagnetohydrodynamicPorous medium |
| spellingShingle | Mohamed Boujelbene Fethi Albouchi Zia Ullah Musaad S. Aldhabani Samirah H. Alsulami Ahmed M. Hassan Solar radiation and lower gravitational effects on wave oscillations in heat transfer along magnetic-driven porous cone in the presence of Joule heating Case Studies in Thermal Engineering Joule heating Lower gravitational region Magnetic flux Oscillatory heat transfer Magnetohydrodynamic Porous medium |
| title | Solar radiation and lower gravitational effects on wave oscillations in heat transfer along magnetic-driven porous cone in the presence of Joule heating |
| title_full | Solar radiation and lower gravitational effects on wave oscillations in heat transfer along magnetic-driven porous cone in the presence of Joule heating |
| title_fullStr | Solar radiation and lower gravitational effects on wave oscillations in heat transfer along magnetic-driven porous cone in the presence of Joule heating |
| title_full_unstemmed | Solar radiation and lower gravitational effects on wave oscillations in heat transfer along magnetic-driven porous cone in the presence of Joule heating |
| title_short | Solar radiation and lower gravitational effects on wave oscillations in heat transfer along magnetic-driven porous cone in the presence of Joule heating |
| title_sort | solar radiation and lower gravitational effects on wave oscillations in heat transfer along magnetic driven porous cone in the presence of joule heating |
| topic | Joule heating Lower gravitational region Magnetic flux Oscillatory heat transfer Magnetohydrodynamic Porous medium |
| url | http://www.sciencedirect.com/science/article/pii/S2214157X23010882 |
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