Author/Authors :
F. Arqueros a، نويسنده , , *، نويسنده , , A. Jim enez a، نويسنده , , A. Valverde b، نويسنده ,
Abstract :
A novel procedure for the optical characterization of solar concentrators is presented. The method is based on
recording at night the light of a star reflected by the mirror. Images of the mirror taken from its focal region allow the
reconstruction of the slope map. The application of this technique for the in situ characterization of heliostats is
particularly simple and at very low cost. Results on first tests carried out with a heliostat of the CESA-I field at the
Plataforma Solar de Almeria have shown the feasibility of this technique. Uncertainties in the reconstructed slopes of
about 1.0 mrad have been estimated.
2003 Elsevier Ltd. All rights reserved.