A new optical-thermal model for a linear Fresnel solar reflector is presented.
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Solar radiation transfer and energy conversion processes are simulated integrally.
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Yearly optical efficiency of 60.1%–44.7% from the equator to N50° is revealed.
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Heat transfer characteristics and thermal performance of the receiver are analyzed.
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Radiation loss from tubes is found to be dominant and contributes around 81%–87%.
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