西安交通大学：翅片型熔盐吸热器在下一代塔式光热电站中的光-热耦合特性研究

Fig. 7. Optical processes in the heliostat and receiver. (left)

Fig. 20. Preliminary design of the fin-like receiver. (right)

Fig. 16. η at different DNI, Tambient = 15°C, ts = 12:00. (Left)

Fig. 17. The variation of η with the wind speed, Tambient = 15 °C, DNI = 982 W· m ², ts = 12:00. (Right)

Fig. 18. Solar flux distributions at noon of three typical days under the same receiver diameter.

　　原文链接： https://www.sciencedirect.com/science/article/pii/S0306261920305912