An air-based corrugated cavity-receiver for solar parabolic trough concentrators
•We analyze a novel tubular cavity-receiver for solar parabolic trough collectors.•Four-fold solar concentration ratio is reached compared to conventional receivers.•Efficient operation at up to 500°C is possible.•The pumping power requirement is found to be acceptably low. A tubular cavity-receiver...
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Veröffentlicht in: | Applied energy 2015-01, Vol.138, p.337-345 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | •We analyze a novel tubular cavity-receiver for solar parabolic trough collectors.•Four-fold solar concentration ratio is reached compared to conventional receivers.•Efficient operation at up to 500°C is possible.•The pumping power requirement is found to be acceptably low.
A tubular cavity-receiver that uses air as the heat transfer fluid is evaluated numerically using a validated heat transfer model. The receiver is designed for use on a large-span (9m net concentrator aperture width) solar parabolic trough concentrator. Through the combination of a parabolic primary concentrator with a nonimaging secondary concentrator, the collector reaches a solar concentration ratio of 97.5. Four different receiver configurations are considered, with smooth or V-corrugated absorber tube and single- or double-glazed aperture window. The collector’s performance is characterized by its optical efficiency and heat loss. The optical efficiency is determined with the Monte Carlo ray-tracing method. Radiative heat exchange inside the receiver is calculated with the net radiation method. The 2D steady-state energy equation, which couples conductive, convective, and radiative heat transfer, is solved for the solid domains of the receiver cross-section, using finite-volume techniques. Simulations for Sevilla/Spain at the summer solstice at solar noon (direct normal solar irradiance: 847Wm−2, solar incidence angle: 13.9°) yield collector efficiencies between 60% and 65% at a heat transfer fluid temperature of 125°C and between 37% and 42% at 500°C, depending on the receiver configuration. The optical losses amount to more than 30% of the incident solar radiation and constitute the largest source of energy loss. For a 200m long collector module operated between 300 and 500°C, the isentropic pumping power required to pump the HTF through the receiver is between 11 and 17kW. |
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ISSN: | 0306-2619 1872-9118 |
DOI: | 10.1016/j.apenergy.2014.10.050 |