Abstract: A solar collection antenna has a large aperture reflective dish which is mounted on a dish support fame. When the dish is pointed at the sun, it reflects received solar radiation into a zone of concentration, at which either a solar energy receiver or a secondary reflector (supported by an ancillary support) is located. To track the sun, the dish is rotated about a first axis which is transverse the dish aperture and a second, orthogonal axis (which intersects the first axis). The center of mass of the combination of the dish, its support frame, the solar energy receiver or secondary reflector and the ancillary support is relatively close to the lower edge of the dish, and lies substantially on the transverse axis of rotation, at the point where the first and second axes intersect (or almost intersect). The dish aperture is chosen so that the dish experiences balanced wind loading about its transverse axis of rotation.

Abstract: A dish antenna framework is constructed from tetrahedral strut assemblies. Each assembly is made up of six struts joined at their ends to four nodes. The nodes also constitute dish mounting points for the dish on the dish antenna framework. These points are located on the envelope of the dish. The framework supported on base frame is rotated about the vertical axis using a movable hydraulic ram arrangement wherein a ram cylinder is attached by an arm to the base frame to be rotated, a ram piston is removably attached to anchor members fixed to a platform. Rotation is effected by expanding and contracting the hydraulic ram. The ram is guided between anchor members by guiding means.