Large relative aperture and high precision catadioptric star sensor optical system
A star sensor and relative aperture technology, applied in the field of optical systems, can solve the problems of slow image refresh rate, long integration time, and poor authenticity, so as to reduce the time of dynamic attitude determination, increase the diameter of the entrance pupil, and reduce the adjustment effect of error
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[0037] Such as figure 1 As shown, the front mirror group A with positive refractive power and the rear mirror group B with positive refractive power are respectively set according to the order of light incidence, and the front mirror group A is composed of secondary reflector A-1 and primary reflector A-2 composition, focal length f A '=247.63mm; the rear mirror group B is composed of the first convex-concave lens B-1, the second convex-concave lens B-2, the third convex-concave lens B-3 and the parallel plate glass B-4, the first convex-concave lens B-1, the second convex-concave lens B-2 and the third convex-concave lens B-3 are all spherical lenses with focal length f B '=141.811 mm.
[0038] The air gap between the front mirror group A and the rear mirror group B is 68.034mm.
[0039]The air separation between the secondary mirror A-1 and the primary mirror A-2 is 72mm.
[0040] The air gap between the first lenticular lens B-1 and the second lenticular lens B-2 was 0....
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