Computational analysis of radiative heat transfer and free convective flow over a vertical wavy surface with Lorentz forces
In several engineering systems, wavy surfaces are utilized to enhance thermal distribution such as heat exchangers and aerodynamics and drag control. However, when radiative heat transfer, heat generation and magnetic fields are considered, velocity and thermal distribution become more difficult, making it significant to understand their combined influences for improved heat transfer. Therefore, this problem focuses on the flow rate, isotherms, streamlines and thermal distrib
Researchers have computationally analyzed fluid flow and heat transfer over a vertical wavy surface, considering factors like radiative heat transfer, heat generation, and magnetic fields. This study aimed to understand the complex interactions influencing velocity and thermal distribution in such systems. The team employed the Spectral Quasi-Linearization Method (SQLM) in Wolfram Mathematica to solve the governing equations, validating their approach against prior studies to ensure accuracy.
The findings indicate that increased radiation-conduction parameters lead to enhanced thermal distribution within the boundary layer. Conversely, a higher amplitude of waviness in the surface was observed to decrease fluid velocity.
Understanding these complex thermal and fluid dynamics is crucial for optimizing the performance of engineering systems that utilize wavy surfaces for improved heat distribution and drag control.
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