The application discloses an atmospheric
coherence length measurement self-adaptive pointing tracking method and
system, belongs to the technical field of atmospheric optical measurement instruments, and solves the technical problems of low recognition and alignment efficiency, weak self-adaptive
adaptation capability, insufficient anti-interference performance and poor
system cooperation in the prior art. A star camera is used to collect a starry
sky area image of a target star area; after the image is analyzed and a
celestial body measurement parameter is obtained, a turntable is finely adjusted so that the target star is on a
target surface of a main mirror camera;
exposure time and
gain of the main mirror camera are adjusted; two light spots of the target star are automatically adjusted to be centered on a field center of the main mirror camera; a target star image is collected; an atmospheric
coherence length value is calculated in real time; whether the atmospheric
coherence length value is empty or an abnormal value is determined at a
fixed interval; if yes, the turntable automatically points to a next target star; and if not, an atmospheric coherence
length measurement task is continuously executed. The application is used for realizing fast alignment and stable tracking of a
beacon light source in a weak light environment at night.