Page 40 - Design of Solar Thermal Power Plants
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1.2 BRIEF INTRODUCTION TO SOLAR THERMAL POWER GENERATION  33

               and spillage loss. Based on this, the concentration field layout
               design must consider the causes for these losses and mitigate them
               through a reasonable layout of concentrators to collect more solar
               irradiation through the receivers.
               a. Specular loss. Based on the need for concentrating efficiency,
                 specular reflectance on the reflective surface of the concentrator
                 is normally high, about 0.93e0.94. However, as a heliostat is
                 exposed to atmospheric conditions while functioning,
                 environmental factors such as dust and humidity will contribute
                 to decreases in specular reflectance.
                 Fig. 1.18 shows the measured result of one heliostat in the Beijing
                 Badaling CSP plant, based on which we can see that influences
                 of dust accumulation contribute to a decrease in specular
                 reflectance from 94.6% on Aug. 23, 2011, to 45.5% on Oct. 10,
                 2011. On Oct. 13, 2011, due to rain, the specular reflectance
                 climbed back to 82.1%.
               b. Cosine loss. In order to reflect sun beam onto a fixed target, the
                 surface of the heliostat is not always perpendicular to the
                 incident light and may create certain angles. Cosine loss is
                 generated because of the reduction of the heliostat surface area
                 against the sun beam projected area caused by such an
                 inclination. The value of cosine efficiency is in proportion to the
                 cosine value of the angle between the heliostat surface’s normal
                 direction and incident solar radiation. When arranging
                 heliostats in a concentration field, heliostats must be arranged in
                 areas with the greatest cosine efficiencies possible.
























           FIGURE 1.18  Influence of dust on the reflectance of the heliostat. Provided by the Institute
           of Electrical Engineering, Chinese Academy of Sciences, 2012.
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