The efficiency of an open-cavity tubular solar receiver for a small-scale solar thermal Brayton cycle
•Results show efficiencies of a low-cost stainless steel tubular cavity receiver.•Optimum ratio of 0.0035 is found for receiver aperture area to concentrator area.•Smaller receiver tube and higher mass flow rate increase receiver efficiency.•Larger tube and smaller mass flow rate increase second law...
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| Published in: | Energy conversion and management 2014-08, Vol.84, p.457-470 |
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| Main Authors: | , , |
| Format: | Article |
| Language: | eng |
| Subjects: | |
| Online Access: | Get full text |
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| Summary: | •Results show efficiencies of a low-cost stainless steel tubular cavity receiver.•Optimum ratio of 0.0035 is found for receiver aperture area to concentrator area.•Smaller receiver tube and higher mass flow rate increase receiver efficiency.•Larger tube and smaller mass flow rate increase second law efficiency.•Large-tube receiver performs better in the small-scale solar thermal Brayton cycle.
The first law and second law efficiencies are determined for a stainless steel closed-tube open rectangular cavity solar receiver. It is to be used in a small-scale solar thermal Brayton cycle using a micro-turbine with low compressor pressure ratios. There are many different variables at play to model the air temperature increase of the air running through such a receiver. These variables include concentrator shape, concentrator diameter, concentrator rim angle, concentrator reflectivity, concentrator optical error, solar tracking error, receiver aperture area, receiver material, effect of wind, receiver tube diameter, inlet temperature and mass flow rate through the receiver. All these variables are considered in this paper. The Brayton cycle requires very high receiver surface temperatures in order to be successful. These high temperatures, however, have many disadvantages in terms of heat loss from the receiver, especially radiation heat loss. With the help of ray-tracing software, SolTrace, and receiver modelling techniques, an optimum receiver-to-concentrator-area ratio of A′≈0.0035 was found for a concentrator with 45° rim angle, 10mrad optical error and 1° tracking error. A method to determine the temperature profile and net heat transfer rate along the length of the receiver tube is presented. Receiver efficiencies are shown in terms of mass flow rate, receiver tube diameter, pressure drop, maximum receiver surface temperature and inlet temperature of the working fluid. For a 4.8m diameter parabolic dish, the larger the receiver tube diameter and the smaller the mass flow rate through the receiver, the higher the receiver surface temperature and the less efficient the collector becomes. However, the smaller the receiver tube diameter, the higher the pressure drop through the tube and the smaller the second law efficiency. It was found that the receiver with larger tube diameter would perform better in a solar thermal Brayton cycle. An overall solar-to-heat efficiency of between 45% and 70% is attainable for the solar collector using the open-cavity receiver. |
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| ISSN: | 0196-8904 1879-2227 |