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

Active Publication Date: 2017-07-14
CHANGCHUN INST OF OPTICS FINE MECHANICS & PHYSICS CHINESE ACAD OF SCI
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Problems solved by technology

[0003] In order to solve the problems in the prior art that the incident light energy received by the image detector per unit time is small, the integration time is long when the motion imaging is fixed, and the image refresh rate is slow; the adaptive spectral range is narrow; the imaging distortion is large and the authenticity is poor. Provide a high-precision catadioptric star sensor optical system with large relative aperture, large entrance pupil area, small deviation of the energy center of mass of the entire field of view, and low distortion. Reduce the integration time of the image detector of the star sensor, meet the requirements of fast attitude determination of the star sensor, expand the application range of the optical system of the star sensor, and overcome the defect of the low performance index of the existing technology of the transmissive star sensor

Method used

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  • Large relative aperture and high precision catadioptric star sensor optical system
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  • Large relative aperture and high precision catadioptric star sensor optical system

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Embodiment

[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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Abstract

The optical system of large relative aperture and high-precision catadioptric star sensor belongs to the field of optical system technology. In order to overcome the problems existing in the prior art, the optical system sets the front group with positive focal power and the focal power of The positive rear group, the front mirror group is composed of a secondary reflector and a primary reflector; the rear mirror group is composed of a first convex-concave lens, a second convex-concave lens, a third convex-concave lens and parallel flat glass, and the first The convex-concave lens, the second convex-concave lens and the third convex-concave lens are all spherical lenses; the air interval between the secondary reflector and the first convex-concave lens is 68.034, and the air interval between the secondary reflector and the main reflector is 72mm, the air gap between the first convex-concave lens and the second convex-concave lens is 0.5mm, the air gap between the second convex-concave lens and the third convex-concave lens is 2.013mm, and the air gap between the third convex-concave lens and the parallel flat glass The interval is 7.328mm.

Description

technical field [0001] The invention relates to a catadioptric star sensor optical system, which belongs to the technical field of optical systems. Background technique [0002] Star sensors have a variety of imaging models according to the wavelength range and detector type used. Their performance indicators are quite different. Most of them adopt the transmission type of full transmission lens. The focal length of the system is generally 20mm-60mm, and the effective entrance pupil diameter is generally 10mm-50mm. The incident light energy received by the image detector per unit time is less, and the motion imaging Attitude-time integration time is long, the image refresh rate is slow; the adaptive spectral range is narrow; imaging distortion is large, and the authenticity is poor. Contents of the invention [0003] In order to solve the problems in the prior art that the incident light energy received by the image detector per unit time is small, the integration time is...

Claims

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Application Information

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Patent Type & Authority Patents(China)
IPC IPC(8): G01C21/02
CPCG01C21/02
Inventor 刘伟奇吕博张大亮姜珊康玉思
Owner CHANGCHUN INST OF OPTICS FINE MECHANICS & PHYSICS CHINESE ACAD OF SCI
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