Wind speed effect on the flow field and heat transfer around a parabolic trough solar collector

•Large Eddy Simulations to study fluid flow and heat transfer on a PTC are performed.•Drag and lift forces were shown to be independent on the Reynolds number.•Nusselt number is highly dependent on the pitch angle.•Heat losses from the HCE are overestimated compared to literature’s correlations.•Mai...

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Veröffentlicht in:Applied energy 2014-10, Vol.130, p.200-211
Hauptverfasser: Hachicha, A.A., Rodríguez, I., Oliva, A.
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Oliva, A.
description •Large Eddy Simulations to study fluid flow and heat transfer on a PTC are performed.•Drag and lift forces were shown to be independent on the Reynolds number.•Nusselt number is highly dependent on the pitch angle.•Heat losses from the HCE are overestimated compared to literature’s correlations.•Main frequencies affecting the stability of the PTC structure are determined. Parabolic trough solar collectors are currently one of the most mature and prominent solar technology for the production of electricity. These systems are usually located in an open terrain where strong winds may be found, and could affect their stability and optical performance, as well as the heat exchange between the solar receiver and the ambient air. In this context, a wind flow analysis around a parabolic trough solar collector under real working conditions is performed. A numerical aerodynamic and heat transfer study based on Large Eddy Simulations is carried out to characterise the wind loads and heat transfer coefficients. After the study carried out by the authors in an earlier work (Hachicha et al. 2013) at ReW1=3.9×105, computations are performed at a higher Reynolds number of ReW2=1×106, and for various pitch angles. The effects of wind speed and pitch angle on the averaged and instantaneous flow are assessed. The aerodynamic coefficients are calculated around the solar collector and validated with measurements performed in wind tunnel tests. The variation of the heat transfer coefficient around the heat collector element with the Reynolds number is presented and compared to the circular cylinder in cross-flow. The unsteady flow is studied for three pitch angles: θ=0°,θ=45° and θ=90° and different structures and recirculation regions are identified. A spectral analysis around the parabola and its receiver is also carried out in order to detect the most relevant frequencies related to the vortex shedding mechanism which affects the stability of the collector.
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Parabolic trough solar collectors are currently one of the most mature and prominent solar technology for the production of electricity. These systems are usually located in an open terrain where strong winds may be found, and could affect their stability and optical performance, as well as the heat exchange between the solar receiver and the ambient air. In this context, a wind flow analysis around a parabolic trough solar collector under real working conditions is performed. A numerical aerodynamic and heat transfer study based on Large Eddy Simulations is carried out to characterise the wind loads and heat transfer coefficients. After the study carried out by the authors in an earlier work (Hachicha et al. 2013) at ReW1=3.9×105, computations are performed at a higher Reynolds number of ReW2=1×106, and for various pitch angles. The effects of wind speed and pitch angle on the averaged and instantaneous flow are assessed. The aerodynamic coefficients are calculated around the solar collector and validated with measurements performed in wind tunnel tests. The variation of the heat transfer coefficient around the heat collector element with the Reynolds number is presented and compared to the circular cylinder in cross-flow. The unsteady flow is studied for three pitch angles: θ=0°,θ=45° and θ=90° and different structures and recirculation regions are identified. 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Parabolic trough solar collectors are currently one of the most mature and prominent solar technology for the production of electricity. These systems are usually located in an open terrain where strong winds may be found, and could affect their stability and optical performance, as well as the heat exchange between the solar receiver and the ambient air. In this context, a wind flow analysis around a parabolic trough solar collector under real working conditions is performed. A numerical aerodynamic and heat transfer study based on Large Eddy Simulations is carried out to characterise the wind loads and heat transfer coefficients. After the study carried out by the authors in an earlier work (Hachicha et al. 2013) at ReW1=3.9×105, computations are performed at a higher Reynolds number of ReW2=1×106, and for various pitch angles. The effects of wind speed and pitch angle on the averaged and instantaneous flow are assessed. 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subjects Applied sciences
Calor
Dinàmica de fluids
Energia solar tèrmica
Energia tèrmica solar
Energies
Energy
Energy. Thermal use of fuels
Exact sciences and technology
Fluid dynamics
Heat
Heat transfer
Heat transfer coefficient
Large Eddy Simulations
Natural energy
Parabolic trough solar collector
PTC stability
Solar collectors
Solar energy
Solar thermal conversion
Solar thermal energy
Theoretical studies. Data and constants. Metering
Transmission
Transmissió
Turbulence
Turbulència
Wind speed effect
Àrees temàtiques de la UPC
title Wind speed effect on the flow field and heat transfer around a parabolic trough solar collector
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