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Airflow change and exergy analysis due to the installation of various types of partitions in the collector of a solar chimney power plant

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An Erratum to this article was published on 04 August 2023

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Abstract

Interest in renewable energy is rapidly growing due to the increase in energy demand, environmental pollution, and depletion of fossil fuels worldwide. One of these sources is solar chimney power plant, which utilizes solar energy to generate electrical energy at a relatively low operating cost. Solar chimneys also do not require cooling, indicating that water resources are not wasted, and they are expected to be widely used in developing countries with abundant solar radiation. This study involved installing a solar chimney with a height of 3 m and a diameter of 3 m for the collector. The experimental results were verified by performing numerical work using ANSYS Fluent, under the scenario that no partition was present in the collector. The exergy efficiencies with I- and C-type partitions were compared with the case without partition. The result showed that the exergy efficiencies were 7.05 % and 7.12 % for the I- and C-type partitions, respectively, and they were higher than the previous 6.44 % for no partition. This study confirmed that the power generation exergy efficiency can be increased by installing partitions in existing solar chimney power plants.

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Abbreviations

A abs :

Surface area of the absorbing plate (m2)

A chimney :

Cross-sectional area of the chimney (m2)

EX heat :

Exergy generated by the solar collector

EX rad :

Exergy for solar radiation

Gr :

Grashof number

g :

Gravitational acceleration (m/s2)

h :

Enthalpy (J/kg)

I :

Radiation intensity of the black body

:

Mass flow rate (kg/s)

P :

Power (W)

Pr :

Prandtl number

q u :

Amount of heat

Ra :

Rayleigh number

S :

Entropy (J/K)

T ds :

Dead state temperature (K)

T h :

Average temperature in the collector (K)

T s :

Surface temperature of the absorber (K)

h out :

Enthalpy of the air (J/kg)

h DS :

Dead state enthalpy (J/kg)

S out :

Entropy of the air (J/K)

S ds :

Dead state entropy (J/K)

U air :

Air flow velocity at the chimney inlet (m/s)

X :

Characteristic length (m)

α :

Thermal diffusion coefficient

α λ :

Spectral absorption coefficient

β :

Coefficient of thermal expansion

ϑ :

Kinematic viscosity

λ :

Wavelength

μ :

Coefficient of dynamic viscosity

ρ air :

Air density at the chimney inlet

σ s :

Scattering coefficient

ψ chimney :

Efficiency of the chimney

ψ net :

Total efficiency of the system

ψsol :

Efficiency of the solar collector

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Acknowledgments

This work was supported by the National Research Foundation of Korea grant funded by the Korean Government (MSIT) (Nos. 2021R1F1A1061409 and 2021M3H4A3A02099204).

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Correspondence to Jeong-Heon Shin or Jung Hwan Seo.

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Jeong-Heon Shin is currently an Assistant Professor at the Department of Mechanical and System Design Engineering, Hongik University. He received his Ph.D. degree in Mechanical Engineering from the University of Texas, Austin. His research interest fields are heat and fluid flow in nano- and micro-channels and renewable energy systems.

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Kang, H.G., So, H.S., Lee, H.W. et al. Airflow change and exergy analysis due to the installation of various types of partitions in the collector of a solar chimney power plant. J Mech Sci Technol 37, 3807–3816 (2023). https://doi.org/10.1007/s12206-023-0643-y

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