Hamamatsu News 3 / 2019

News 2019 Vol. 3 13 and the receiver, which limits the efficiency of energy collection. In modern, high power STPs, the heliostat-receiver distance may exceed 1 kilometer, so the solar extinction caused by local parameters such as humidity or particle concentration (i.e. dust) has to be considered when assessing STP performance. Established methods to analyze solar extinction aim to determine the transmission or scattering coefficients at the local site. There are signi­ ficant drawbacks to using these methods, including the comparably small measurement volume, or the requirement to use monochrome light sources. Deriving the solar extinction, as it is occurring in STPs, from such measurements would therefore require extrapolation in spatial and spectral dimensions, which can create large errors. A new method proposed by Ballestrin et al. employs scientific cameras (ORCA-Flash4.0) as detectors to measure solar extinction. By using the solar signal and a broadband detector, spectral extrapolation can be avoided, yielding more accurate measurements of solar extinction. A simplified diagram of the measurement setup is shown in figure 2. Taking simultaneous images of a Lambertian target (a target with uni­ form scattering properties, as determined in [Ballestrin 2018]) with two cameras at different distances, the solar extinction can be derived by the following formula: With I 2 being the intensity observed by camera 2 and I 1 by camera 1, the areas observed on the target are identical for both cameras. By knowing the distance ‘D’ between both cameras, the extinction coefficient can be determined using the Beer-Lambert law. From this coefficient, solar extinction can be obtained for each particular heliostat receiver distance applying the law. In the system developed at PSA, the distance ‘D’ is 742 m which is representative in a low extinction environment such as PSA. Experimental preconditions for employing this method are the avail­ ability of Lambertian targets of high homogeneity and diffusivity, as well as highly linear cameras. It is desirable to use this method in the process of determining appro­ priate locations for STPs, as well as during operation, to include the effect of solar extinction into the routine assessment of efficiency (see figure 3). The method has been applied over one year at Plataforma Solar de Almería, Spain. The results in figure 4 indicate that the solar extinction reached its minimum value and minimum variability during the winter months, while the absolute extinction and its variability peaked during the summer months [Ballestrin 2019]. Conclusion Solar tower plants rely on a conceptually simple method of energy gen­ eration. However, maximizing their performance and thereby providing an efficient method of energy generation is contingent upon having knowledge of important parameters. In this report, two studies by Ballestrin et al., were presented which involve the determination of solar attenuation in STPs. In another study, Ballestrin et al., showed how scientific cameras can be employed to monitor the solar irradia­ tion on the receiver during operation [Ballestrin 2019]. Both methods employed ORCA-Flash4.0 cameras as spatially resolved light detectors, thereby mitigating geometric effects present in commonly employed point detectors. The ORCA-Flash4.0 was the camera of choice for these experiments, as it delivers good linearity and uniformity. References „ „ Zhang, H. L., et al. “Concentrated solar power plants: Review and design methodology.” Renewable and Sustainable Energy Reviews 22 (2013): 466-481. „ „ Ballestrín, J., et al. “Solar extinction measurement system based on digital cameras. Application to solar tower plants.” Renewable Energy 125 (2018): 648-654. „ „ Ballestrín, J., et al. “One year of solar extinction measurements at Plataforma Solar de Almería. Application to solar tower plants.” Renewable Energy 136 (2019): 1002-1011. „ „ Ballestrín, J., et al. “Diagnosis of a Lambertian target in solar context.” Measurement 119 (2018): 265-269. „ „ Ballestrín, J., et al. “Simplifying the measurement of high solar irradiance on receivers. Application to solar tower plants.” Renewable Energy 138 (2019): 551-561. Figure 2: A Lambertian target, consisting of a white part of high solar reflectance and a black part of high solar absorbance is observed by 2 cameras simultaneously from different distances. The white part of the target serves as the signal source, while the black part serves as a dark reference to consider the effect of scattered light into the measurement distance. Both cameras observe the same area on the target. Camera 2 D Figure 4: Solar extinction measured using the described method at Plataforma Solar de Almería over one year Maximum Average Minimum September February July November April August December May October March January June Extinction (%) 14 13 12 11 10 9 8 7 6 5 4 3 2 1 0 Camera 1 Lambertian target Extinction(%) = 100(1– ) I 1 I 2

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