The present invention discloses a method for solving the fixed
image rotation of a
telescope based on three-point coordinates. The specific steps are as follows: first,
record the current target miss amount coordinate O and the target miss amount coordinates P and Q after adding control amounts to the two directions of the fast mirror respectively. Then, the coordinates O and P are used to determine the quadrant position of the direction of the X direction and the fixed
image rotation angle, and the coordinates O, P, and Q are used to determine the polarities A1 and A2 of the miss amount error, and then the polarities K1 and K4 of the
rotation matrix are determined by judging the positive and negative signs of the cosine values after the
image rotation angle is converted into radians. Finally, a control amount is added to one of the directions to judge the direction of its own direction and the influence on the other direction, and at the same time, the polarities K2 and K3 of the
rotation matrix are determined in combination with the sine value after the image rotation angle is converted into radians, thereby obtaining a complete image rotation solution formula. The method of the present invention has fast calculation speed, is easy to implement, and has stable performance. The fixed image rotation angle can be obtained only through three-point coordinates, and all polarities of the miss amount error and the
rotation matrix can be derived.