The application belongs to the technical field of large
radio telescope, and provides a kind of spherical
radio telescope active reflecting
surface shape adjusting method and
system, first, the reference spherical
radius and focal ratio are obtained, the coordinate
system is updated, and the ideal parabolic surface of the observed
celestial body is determined;Then, the coordinates of each node under the original coordinate
system and the
azimuth and elevation of the measured
celestial body are obtained, and the position coordinates of each node under the new coordinate system are obtained through rotation transformation;The center of the ideal parabolic surface aperture is calculated, and the to-be-adjusted node is determined in combination with the reference spherical
radius;Finally, the sum of the square of the distance between the coordinates of all to-be-adjusted nodes in the radial direction of the working parabolic surface and the ideal parabolic surface is minimized as the target, the target coordinates of all to-be-adjusted nodes are determined, and the extension amount of the top end of the
actuator is calculated, so that the working parabolic surface is as close as possible to the ideal parabolic surface, to obtain the best receiving effect of the electromagnetic wave of the
celestial body reflected by the reflecting surface.