4.6 Article

Accurate interpolation methods for the annual simulation of solar central receiver systems using celestial coordinate system

Journal

SOLAR ENERGY
Volume 213, Issue -, Pages 328-338

Publisher

PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.solener.2020.10.087

Keywords

Solar central receiver system; Annual simulation; Ecliptic coordinate system; Equatorial coordinate system; Celestial coordinate system

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This paper optimizes heliostat field layout for annual energy production, using new methods to reduce simulation points and improve efficiency. By decoupling power computation from irradiation and approximating efficiency based on solar angle, high accuracy is achieved.
Heliostat field layout optimization bases on simulations of the annual energy production. To reduce the computation time of the optimization process, one can try to reduce the number of simulation points of the annual domain, while keeping similar accuracy. For the temporal domain, there exist already different approaches as aggregation of days. To further reduce the number of needed simulation points, in this paper we decouple the power computation from the irradiation, such that we just regard the computation of the power plant efficiency. This time-dependent parameter is transformed into a celestial coordinate system where the solar angle-dependent efficiency will be approximated using suitable multi-dimensional interpolation methods. We distinguish between an accurate approximation of the received annual optical energy and the electrical energy of each moment of a year. These methods are demonstrated for the existing heliostat field layouts PS10 and Gemasolar in Seville, while using realistic weather conditions. With this new approach just around 40 simulation points suffice to reach an accuracy of 99.9% for the received power for smaller power plants as PSIO, and for larger plants as Gemasolar. Compared to a state-of-the-art method, this investigation helps to accelerate the simulation by factor three.

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