CFD analysis of solar tower Hybrid Pressurized Air Receiver (HPAR) using a dual-banded radiation model

•A hybrid pressurized air central CSP receiver is modeled using CFD.•Solar irradiation and conjugate heat transfer is included in CFD model.•Receiver geometry is parameterized to enable optimization.•The effect of a glass window to trap thermal re-radiation is investigated.•Dual-band gray radiation is modeled using the Discrete Ordinates model. Solar receivers used for central tower Concentrated Solar Power (CSP) plants use either a surface-based or volumetric heat transfer region. Volumetric receivers are more efficient but require more sophisticated and expensive materials that can withstand the elevated temperatures (in excess of 1000°C). For a solarized gas-turbine application, pressurized air from the compressor is used as heat transfer fluid (HTF) in order to increase both the density and heat capacity of the HTF. If a volumetric receiver is used, it needs to be located in a pressure vessel with a pressurized quartz window located at the aperture of the concentrator. An alternative approach to utilize pressurized air in a pseudo-volumetric fashion is to populate a volumetric region with piped pressurized air. A tubular-type volumetric receiver (named a Hybrid Pressurized Air Receiver (HPAR)) is studied here. The HPAR provides the challenge of enabling maximum heat transfer without causing hot spots on the side of the solar irradiation source. Heat transfer in the HPAR would not be as effective as for a true volumetric receiver because the heat transfer area is limited by the tube wall. The heat transfer to the HTF is however enhanced through mixing generated by external forced convection caused by suction due to a downstream fan in the receiver cavity. In addition, the aperture of the cavity contains a glass windowed louver system, to limit re-radiation losses. A Computational Fluid Dynamics (CFD) model is generated of the solar receiver cavity. The commercial CFD code ANSYS Fluent v14.5 is used to evaluate the heat transfer between the incoming solar flux and the HTF. A numerical validation is performed to illustrate mesh dependency and the choice of turbulence model. The incoming solar irradiation and its absorption, reflection and transmission are modeled using the Discrete Ordinates (DO) radiation model in ANSYS Fluent. An idealized and a solar flux map based on the PS10 field are used as source. For comparison, both a gray (without a glass louver) and a semi-gray two-banded DO approach are used when modeling the absorption of high-wavelength re-