Star sensor on-orbit calibration method based on star angular distance subtraction
A technology of star sensor and calibration method, which is applied in the field of astronomical navigation and can solve the problems of time-consuming
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[0078] The detailed content of the present invention and its specific implementation will be further described below in conjunction with the accompanying drawings.
[0079] 1. Establish star distance subtraction model:
[0080] At present, the star sensor calibration mostly uses the angular distance as the calibration reference, and the focal length of the star sensor is f , w and v are the direction vectors of the star in the star sensor coordinate system and the celestial coordinate system respectively, and the star i The center coordinates of the projected point in the star sensor imaging plane coordinate system are ( x i ,y i ),but
[0081] (1)
[0082] (2)
[0083] in,( x 0 ,y 0 ) principal point coordinates, α i and δ i Respectively represent the first i right ascension and declination of the star; assuming that there are i , j Two stars, according to the invariant principle of star angular distance orthogonal transformation, without considering...
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