The optical performance of the solar tower system depends on the specifications of the heliostat and receiver, along with the tower height and the mirror arrangement in the field. In this study, the heliostat field domain is discretized into a grid, and the mirror density denotes the mirror area in each grid element. The receiver aperture is idealized to be the outer surface of a cone situated at the aim point on the tower, and is represented by the tilt angle. The cosine and the attenuation efficiency are calculated based on the grid point location and the aim point. The interception efficiency is predicted by approximating the spread of the image on the receiver aperture plane. The mirror density is used to estimate the shading and the blocking efficiency. An optimization procedure is developed that can distribute a given mirror area optimally to reach the maximum optical efficiency. Detailed parametric analyses facilitated a deeper understanding of optical performance and mirror density distribution with the system parameters. Optical efficiency improvement of 3%-5% can be achieved by optimally tilting the receiver aperture. The heliostat field’s annual optical efficiency and average mirror density increase with the tower height to varying extents depending on the latitude. Results also indicate that, smaller capacity solar tower systems employing a short tower might be more beneficial for higher latitude locations. On the other hand, the combination of a tall tower and a high tilt receiver aperture might be preferable for lower latitude locations.
扫码关注我们
求助内容:
应助结果提醒方式:
