The primary image reflected from the field-stop of solar Gregory telescopes is used for automatic guiding. This new system avoids temporal varying influences from the bending of the telescope tube by the main mirror's gravity and from offsets between the telescope and a separate guiding refractor. The required stiffness of the guider mechanics and the small areas of the sensors demand small f-numbers for the guider optics, which cause problems with the image quality and with heat.
Problems also arise from the imaging of the pinhole in the telescope's field stop.
The corresponding lack of image information at that location can be reduced numerically by Fourier methods much more effectively than with profile centering methods. Several types of such guiders are tested, a final equipment, now installed at the Gregory telescopes at Tenerife and at Locarno, is described.