Abstract
Thermal transport of nanofluid natural convection in a wavy porous enclosure exposed to an external and uniform magnetic source is investigated numerically. Numerous pertinent factors in terms of Darcy (Da = 10−4–10−2), Hartmann (Ha = 0–40), Rayleigh (Ra = 104–107), Prandtl (Pr = 0.71–7) and undulation (n = 3) numbers, in addition to wave amplitudes (A = 0.025–0.1) and particle volume concentration (\(\phi\) = 0, 2 and 4%) have been investigated. The Brinkmann–Forchheimer extended Darcy model is utilized, and the governing equations are solved by employing our own finite difference ADI-based program. Code accuracy was successfully validated with the open literature. The results revealed that for Ra > 105 and Da < 10−3, the magnetic field does not play a substantial role in the convective thermal energy, while at high Ha and low Ra, the intensity of conduction increases. The surface waviness and Darcy number both have significant effects on the heat transfer suppression if insulation is desired. Furthermore, a critical value of Ra = 105 is observed whereby the mean Nusselt number decreases despite particle volume concentration, particularly at high Hartmann values.
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The datasets during and/or analyzed during the current study available from the corresponding author on reasonable request.
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The implemented CFD code during the current study available from the corresponding author on reasonable request.
Abbreviations
- A:
-
Amplitude of the wavy surface
- B o :
-
External magnetic field, Tesla
- C p :
-
Specific heat transfer, \( {\text{J}}{\text{kg}}^{-1}\,{\text{K}}^{-1} \)
- Da :
-
Darcy number
- g :
-
Gravitational acceleration, \( {\text{m}}\,{\text{s}}^{-2} \)
- Ha :
-
Hartmann number
- k :
-
Thermal conductivity, \( {\text{W}} {\text{m}}^{-1}\,{\text{K}}^{-1} \)
- K :
-
Porous media permeability, \( {\text{m}}^{2} \)
- L :
-
Length and height of the enclosure, \( {\text{m}} \)
- n :
-
Undulation number
- Nu x :
-
Local Nusselt number
- Nu m :
-
Mean Nusselt number
- p :
-
Pressure, \( Pa \)
- P :
-
Dimensionless pressure
- Pr :
-
Prandtl number
- Ra :
-
Rayleigh number
- T :
-
Temperature, \( \text{K} \)
- u, v :
-
Velocity components in x, y directions, \( {\text{m}}\,{\text{s}}^{-1} \)
- U, V :
-
Dimensionless velocity components
- x, y :
-
Cartesian coordinates, \( {\text{m}} \)
- X, Y :
-
Dimensionless coordinates, \( {\text{m}} \)
- \( \alpha \) :
-
Thermal diffusivity, \( {\text{m}}^{2}\,{\text{s}}^{-1}\)
- \( \beta \) :
-
Thermal expansion coefficient, \( {{\text{K}}^{-1}} \)
- \( \phi \) :
-
Nanoparticles volume fraction
- \( \mu \) :
-
Dynamic viscosity, \( \text{Pa s} \)
- \( \upsilon \) :
-
Kinematic viscosity, \( {\text{m}}^{2}\,{\text{s}}^{-1} \)
- \( \omega \) :
-
Dimensionless vorticity
- \( \varepsilon \) :
-
Porosity
- \( \theta \) :
-
Dimensionless temperature
- \( \rho \) :
-
Density, \( {\text{kg}}\,{\text{m}}^{-3} \)
- \( \sigma \) :
-
Electrical conductivity, \( {\text{S}}\,{\text{m}}^{-1} \)
- \( \psi \) :
-
Dimensionless stream function
- c:
-
Cold
- bf:
-
Fluid
- h:
-
Hot
- m:
-
Mean
- nf:
-
Nanofluid
- p:
-
Particles
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All authors contributed to the study conception and design. Material preparation, data collection and analysis were performed by [Hudhaifa Hamzah], [Ahmed Albojamal], [Besir Sahin], and [Kambiz Vafai].
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Hamzah, H., Albojamal, A., Sahin, B. et al. Thermal management of transverse magnetic source effects on nanofluid natural convection in a wavy porous enclosure. J Therm Anal Calorim 143, 2851–2865 (2021). https://doi.org/10.1007/s10973-020-10246-4
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DOI: https://doi.org/10.1007/s10973-020-10246-4