Page 251 - Design of Solar Thermal Power Plants
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234              4. DESIGN OF THE CONCENTRATION SYSTEM

            4.2.3 Brief Introduction to the Toroidal Heliostat
               A toroid, also known as a toroidal surface, has two symmetric sections
            perpendicular to each other, namely the tangential and sagittal sections;
            the arcs of these two sections have different curvature radii and therefore
            are nonrotational symmetric curved surfaces.
               For a fixed incident angle q, the value of the tangential curvature radius
            of the toroidal surface is:

                                    R t ¼ 2f t ¼ 2L=cos q 0
            and the sagittal curvature radius is:

                                    R s ¼ 2f s ¼ 2L cos q 0
               Then according to Eqs. (4.1) and (4.2), the beam spot on a focal plane
            with toroidal surface slant distance L has the minimum area, no astigma-
            tism, and a diameter of bL, from which the minimum value of the spot size
            of the spherical mirror appears when q ¼ 0 , and the toroidal surface can


            shift the minimum value of the spot diameter from q ¼ 0 to q ¼ q 0 .
               In reality, the surface shape of the heliostat is fixed, whereas the inci-
            dent angle q of the solar beam varies over time. Therefore, in order to
            determine the surface shape of the toroidal surface, an appropriate q 0
            shall be selected, which is referred to as the designed incident angle of the
            toroidal surface. Once the slant distance L and designed incident angle q 0
            have been determined, the surface shape of the toroidal surface can be
            determined accordingly.
               R. Zaibel et al. proposed the astigmatic-corrected target-aligned
            heliostat with a fixed rotation axis pointing to the target position in
            1995, which combines a toroidal surface with a two-axis tracking mode
            with a fixed rotation axis pointing to the target position so that during
            whole-day sun tracking and solar concentrating by the heliostat, the
            incident plane of the solar beam at the mirror surface center (including
            normal and incident solar beam at the mirror surface center) always
            coincides with the tangential plane of the mirror surface (including the
            principal optic axis of the mirror surface and the normal direction of
            the mirror surface center). In this case, further optimization design of the
            heliostat mirror surface shape is feasible, and the corresponding method
            for optimization is also simple, thus making practical application of the
            toroidal heliostat feasible. Figs. 4.5 and 4.8 display a two-axis tracking
            heliostat with a fixed rotation axis pointing to the target position. The
            fixed axis points to the center of the receiver aperture; the slave rotation-
            axis is fixed to the heliostat frame and is perpendicular to the fixed axis.
            The design method for the surface shape of an astigmatism-corrected
            toroidal heliostat uses the variation range of incident angle q of the
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