A Numerical Investigation of an Artificially Roughened Solar Air Heater
Abstract
:1. Introduction
2. Numerical Simulations
- The flow is fully developed, turbulent, steady, and 2-dimensional.
- Regardless of the temperature, the wall of the duct, the absorbing plate, and the roughness material all have a constant thermal conductivity.
- The roughness material, as well as the duct wall and absorbing plate, are all composed of a homogeneous and isotropic material.
- Air is considered to be incompressible for SAHs, as density fluctuation is low.
- The model’s fluid contact walls have a no-slip boundary condition.
- Heat losses through radiation and other means are negligible.
2.1. Numerical Model
2.2. Governing Equation
2.3. Boundary Conditions
2.4. Selection and Validation of the Model
2.5. Solution Method
2.6. Data Reduction
3. Result and Discussion
3.1. Effect of Grid Density
3.2. Effect of Re
3.3. Effect of RRP
3.4. Effect of RRH
3.5. Thermohydraulic Performance Parameter (THPP)
3.6. Validation of Results
4. Conclusions
- This study demonstrated that the RNG k-ε turbulence model predicted results that were in close agreement with the experimental results, thus providing confidence in the numerical predictions based on this model. Using the RNG k-ε model, the Nur data deviates from Equation (6) by 2.58 percent.
- There is an increase in the average Nur with an increase in the Re. The Nur was found to reach a maximum value of 139.65 at an Re of 18,000 for an RRP of 5 and an RRH of 0.06.
- The maximum Nur enhancement for a roughened duct was found to be 2.76 times that of a smooth duct with an RRP of 5 and an RRH of 0.06 at an Re of 18,000.
- There is a decrease in the average fr with an increase in the Re. The fr was found to reach a maximum value of 0.0309 at an Re of 3800 for an RRP of 5 and an RRH of 0.06.
- The maximum fr enhancement for a roughened duct was found to be 3.07 times that of a smooth duct with an RRP of 5 and an RRH of 0.06 at an Re of 3800.
- A semi-circular rib roughness with an RRP = 10 and RRH = 0.06 at an Re of 15,000 was found to provide the best THPP, of 1.98, which can be effectively utilized for the purpose of enhancing heat transfer.
- Finally, it was found that semi-circular ribs which have rib pitch = 20 mm and a rib height = 2 mm can be applied in an SAH to enhance heat transfer.
Author Contributions
Funding
Data Availability Statement
Acknowledgments
Conflicts of Interest
Nomenclature
CFD | Computational fluid dynamics |
Cp | Specific heat of air, J/kg K |
D | Equivalent or hydraulic diameter of duct, mm |
e | Rib height, mm |
Gk | Generation of turbulence kinetic energy, m2/s2 |
H | Depth of duct, mm |
h | Heat transfer coefficient, W/m2 K |
k | Thermal conductivity of air, W/m K |
L | Length of duct, mm |
L1 | Inlet length of duct, mm |
L2 | Test length of duct, mm |
L3 | Outlet length of duct, mm |
P | Pitch, mm |
q | Heat flux, W/m2 |
RNG | Renormalization group |
RRH | Relative roughness height |
RRP | Relative roughness pitch |
SAH | Solar air heater |
TDR | Turbulence dissipation rate |
THPP | Thermo-hydraulic performance parameter |
TI | Turbulence intensity |
TKE | Turbulence kinetic energy |
v | Velocity of air in the duct, m/s |
W | Width of duct, mm |
ΔP | Pressure drop, Pa |
Dimensionless parameters | |
e/D | Relative roughness height |
e+ | Roughness Reynolds number |
f | Friction factor |
G | Heat transfer function |
I | Turbulence intensity |
Nu | Nusselt number |
P/e | Relative roughness pitch |
Pr | Prandtl number |
R | Roughness function |
Re | Reynolds number |
St | Stanton number |
W/H | Duct aspect ratio |
Greek symbols | |
α | Angle of attack, degree |
αk | Inverse effective turbulent Prandtl numbers for k |
αε | Inverse effective turbulent Prandtl numbers for ε |
Γ | Molecular thermal diffusivity, m2/s |
δ | Transition sub-layer thickness, m |
ε | Turbulence dissipation rate, m2/s3 |
κ | Turbulence kinetic energy, m2/s2 |
μ | Dynamic viscosity, Ns/m2 |
μeff | Effective turbulent viscosity, Ns/m2 |
μt | Turbulent viscosity, Ns/m2 |
ρ | Density of air, kg/m3 |
ω | Specific dissipation rate, 1/s |
Subscripts | |
r | Rough |
s | Smooth |
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L1 | L2 | L3 | W | H | D | e | P |
---|---|---|---|---|---|---|---|
245 | 280 | 115 | 100 | 20 | 33.33 | 1, 1.5, 2 | 10, 15, 20, 25 |
Parameters | Values |
---|---|
q | 1000 W/m2 |
Re | 3800–18,000 (6 values) |
Pr | 0.71 |
RRP | 5–16.67 (12 values) |
RRH | 0.03–0.06 (3 values) |
Properties | Air | Aluminum |
---|---|---|
ρ (kg/m3) | 1.225 | 2719 |
Cp (J/kg K) | 1006.43 | 871 |
μ (Ns/m2) | 1.7894 × 10−5 | - |
k (W/m K) | 0.0242 | 202.4 |
Element Size (mm) | Number of Nodes | Number of Elements | Nur | % Difference | fr | % Difference |
---|---|---|---|---|---|---|
0.5 | 45,728 | 44,473 | 72.6 | - | 0.01410 | - |
0.4 | 70,058 | 68,524 | 74.5 | 2.58 | 0.01453 | 3.00 |
0.35 | 86,249 | 84,622 | 75.23 | 0.98 | 0.01468 | 1.03 |
0.3 | 114,070 | 112,226 | 75.7 | 0.62 | 0.01482 | 0.95 |
0.2 | 242,305 | 242,106 | 75.93 | 0.30 | 0.01490 | 0.54 |
S. No. | Investigators | Optimal RRP |
---|---|---|
1 | Prasad and Mullick [7] | 12.7 |
2 | Verma and Prasad [39] | 10 |
3 | Gupta et al. [40] | 10 |
4 | Aharwal et al. [41] | 8 |
5 | Varun et al. [42] | 8 |
6 | Ebrahim Momin et al. [43] | 10 |
7 | Hans et al. [44] | 8 |
8 | Singh, Chander, and Saini [12] | 8 |
9 | Prasad [45] | 10 |
10 | Karwa and Chitoshiya [46] | 10.63 |
11 | Kumar et al. [47] | 8 |
12 | Saini and Saini [48] | 10 |
13 | Sethi et al. [49] | 10 |
14 | Yadav et al. [50] | 12 |
15 | Layek et al. [51] | 10 |
16 | Singh et al. [52] | 8 |
17 | Alam et al. [53] | 8 |
18 | Maithani and Saini [54] | 10 |
19 | Bharadwaj et al. [55] | 12 |
20 | Yadav and Sharma [56] | 10 |
21 | Kumar and Layek [57] | 8 |
22 | Sahu et al. [58] | 8 |
23 | Kashyap et al. [59] | 10 |
24 | Kumar and Prasad [60] | 10 |
25 | Present numerical study | 10 |
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Yadav, A.S.; Alam, T.; Gupta, G.; Saxena, R.; Gupta, N.K.; Allamraju, K.V.; Kumar, R.; Sharma, N.; Sharma, A.; Pandey, U.; et al. A Numerical Investigation of an Artificially Roughened Solar Air Heater. Energies 2022, 15, 8045. https://doi.org/10.3390/en15218045
Yadav AS, Alam T, Gupta G, Saxena R, Gupta NK, Allamraju KV, Kumar R, Sharma N, Sharma A, Pandey U, et al. A Numerical Investigation of an Artificially Roughened Solar Air Heater. Energies. 2022; 15(21):8045. https://doi.org/10.3390/en15218045
Chicago/Turabian StyleYadav, Anil Singh, Tabish Alam, Gaurav Gupta, Rajiv Saxena, Naveen Kumar Gupta, K. Viswanath Allamraju, Rahul Kumar, Neeraj Sharma, Abhishek Sharma, Utkarsh Pandey, and et al. 2022. "A Numerical Investigation of an Artificially Roughened Solar Air Heater" Energies 15, no. 21: 8045. https://doi.org/10.3390/en15218045
APA StyleYadav, A. S., Alam, T., Gupta, G., Saxena, R., Gupta, N. K., Allamraju, K. V., Kumar, R., Sharma, N., Sharma, A., Pandey, U., & Agrawal, Y. (2022). A Numerical Investigation of an Artificially Roughened Solar Air Heater. Energies, 15(21), 8045. https://doi.org/10.3390/en15218045