Heat transfer in a fluidized bed tubular solar receiver. On-sun experimental investigation

Using particles as heat transfer fluid in a solar receiver is an attractive way to increase the global efficiency of solar power plants. In the case of the particle-in-tube solar receiver concept, the fluidized particles circulate vertically in tubes thanks to a controlled pressure gradient and an additional air injection. Experiments are conducted with olivine particles in a one-tube mock-up at the 1 MW CNRS solar furnace (France). The tube of high aspect ratio (more than 3 m height over 48 mm internal diameter) is irradiated along a 1-m height with several solar flux configurations that correspond to realistic operation conditions of a solar thermal power plant. The novelties of this paper lie in extending the operating parameters compared to earlier studies and in linking the fluidization regimes to wall heat transfer. Slugging, turbulent fluidization and fast fluidization regimes are detected within the receiver tube. It is shown that the system can tolerate high solar flux densities, up to 800 kW/m(2). The system proves to be highly controllable and flexible with respect to particle mass flux variation and transient operations. Particle temperature increase ranges from 100 to 650 degrees C depending on the particle mass flux. Maximum thermal efficiency and particle outlet temperature of respectively similar to 60 % and 680 degrees C are obtained, proving that this technology can be combined with highly efficient thermodynamic cycles. Global wall-to-particle heat transfer coefficient varies strongly with particle mass flux. It reaches a quasi-plateau above 15 kg/(m(2)s) with a mean value of 1000 +/- 200 W/(m(2)K) and peaks data up to 1500 W/(m(2)K). A dimensionless heat transfer index is derived to account for the effects of the particle mass flux on the experimental results. It highlights that both increasing the temperature and working in the turbulent fluidization regime result in the increase of the heat transfer between the tube walls and the particles.

Automated summary

Using particles as heat transfer fluid in solar receivers can improve the efficiency of solar power plants. In this study, olivine particles were used in a one-tube mock-up to investigate the fluidization regimes and wall heat transfer. The experiments demonstrated that the system could tolerate high solar flux densities and showed high controllability and flexibility. The particle temperature increase and wall-to-particle heat transfer coefficient were found to be influenced by the particle mass flux.