Abstract
Modern parabolic trough solar collectors operated at high temperatures to provide the heat input to Rankine steam power cycles employ evacuated receiver tubes along the collector focal line. High performance is achieved via the use of a selective surface with a high absorptance for incoming short-wave solar radiation and a low emittance for outgoing long-wave infrared radiation, as well as theuse of a hard vacuum to essentially eliminate convective and conductive heat losses. This paper describes a new method that determines receiver overall optical efficiency by exposing a fluid-filled, pre-cooled receiver to one sun outdoors and measuring the slope of the temperature curve at the point where the receiver temperature passes the glass envelope temperature (that is, the point at whichthere is no heat gain or loss from the absorber). This transient test method offers the potential advantages of simplicity, high accuracy, and the use of the actual solar spectrum.
Original language | American English |
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Number of pages | 10 |
State | Published - 2011 |
Event | SolarPACES 2011 - Granada, Spain Duration: 20 Sep 2011 → 23 Sep 2011 |
Conference
Conference | SolarPACES 2011 |
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City | Granada, Spain |
Period | 20/09/11 → 23/09/11 |
NREL Publication Number
- NREL/CP-5500-52466
Keywords
- CSP
- optical efficiency
- optical performance
- parabolic trough
- receiver tube
- solar collectors
- thermal transient test