Passive radial supporting mechanism for primary mirror of optical telescope based on kinetic equilibrium

A radial support and kinematics technology, used in telescopes, optics, optical components, etc., can solve the problems of unsuitability, unfavorable telescope rigidity, large stress and deformation of the main mirror, and improve the number of support points, the principle is clear, and the reduction The effect of stress

A radial support and kinematics technology, used in telescopes, optics, optical components, etc., can solve the problems of unsuitability, unfavorable telescope rigidity, large stress and deformation of the main mirror, and improve the number of support points, the principle is clear, and the reduction The effect of stress

CN102508347BInactive Publication Date: 2014-06-18CHANGCHUN INST OF OPTICS FINE MECHANICS & PHYSICS CHINESE ACAD OF SCI

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  • Passive radial supporting mechanism for primary mirror of optical telescope based on kinetic equilibrium
  • Passive radial supporting mechanism for primary mirror of optical telescope based on kinetic equilibrium
  • Passive radial supporting mechanism for primary mirror of optical telescope based on kinetic equilibrium

Examples

Experimental program
Comparison scheme
Effect test

Embodiment 1

[0024] Such as figure 2 As shown, the passive radial support mechanism of the optical telescope primary mirror based on kinematic balance of the present invention includes a primary mirror chamber 2, three first-stage connecting rods 3 evenly distributed around the primary mirror 1, and three second-stage connecting rods 4 and three third-stage connecting rods 5; one end of the first-stage connecting rod 3 is hinged with the edge of the primary mirror chamber 2, and the other end is simultaneously hinged with the second-stage connecting rod 4 and the third-stage connecting rod 5, and the second-stage The other ends of the connecting rod 4 and the third connecting rod 5 are hinged to the edge of the primary mirror 1; and there is an angle θ between the second connecting rod 4 and the third connecting rod 5 .

[0025] The joints of the first-stage connecting rod 3 and the second-stage connecting rod 4 and the third-stage connecting rod 5 adopt a spherical hinge structure, and t...

Embodiment 2

[0027] Such as image 3 , 4 As shown, the passive radial support mechanism of the optical telescope primary mirror based on kinematic balance of the present invention includes a primary mirror chamber 2, six first-stage connecting rods 3 evenly distributed around the primary mirror 1, and six second-stage connecting rods 4 and six third-stage connecting rods 5; one end of the first-stage connecting rod 3 is hinged with the edge of the primary mirror chamber 2, and the other end is hinged with the second-stage connecting rod 4 and the third-stage connecting rod 5 at the same time, and the second-stage The other ends of the connecting rod 4 and the third connecting rod 5 are hinged to the edge of the primary mirror 1; the second connecting rod 4 and the third connecting rod 5 are respectively tangent to the edge of the primary mirror 1.

[0028] The first-stage connecting rod 3, the second-stage connecting rod 4, and the third-stage connecting rod 5 are all made of spring steel...

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Abstract

The invention relates to a passive radial supporting mechanism for a primary mirror of an optical telescope based on kinetic equilibrium. One end of a first-stage connecting rod of the mechanism is hinged with the rim of a primary mirror chamber, and the other end of the first-stage connecting rod is hinged with a second-stage connecting rod and a third-stage connecting rod at the same time; the other end of the second-stage connecting rod and the other end of the third-stage connecting rod are hinged with the rim of the primary mirror; and an included angle theta is formed between the second-stage connecting rod and the third-stage connecting rod. By a kinetic equilibrium system, the radial direction of the primary mirror is not restrained by an over-restraining characteristic, so that a stable equilibrium state is realized; when temperature is changed, the whole radial supporting system does micro motion in accord with a kinetic rule by using the change of the geometric size caused by thermal deformation of a connecting rod mechanism, so that stress caused by the thermal deformation among the primary mirror, the radial supporting mechanism and the primary mirror chamber is counteracted; therefore, the passive radial supporting mechanism is suitable for supporting primary mirrors made of materials with large thermal expansion coefficients and primary mirrors working under a relatively severe working environment.

Description

technical field [0001] The invention relates to a radial support mechanism for a primary mirror of an optical telescope, in particular to a radial passive support mechanism for a primary mirror of a 1-2 meter optical telescope based on kinematic balance. Background technique [0002] The primary mirror of an optical telescope needs to maintain an accurate position and a good surface shape of the primary mirror under working conditions. The mirror support mechanism includes an axial support system and a radial support system. It is usually designed based on the principle of rigid body statics, and is realized by applying a reasonable amount of support force at an appropriate position on the back and side of the primary mirror. The support mechanism is mainly responsible for maintaining the surface shape and position accuracy of the mirror. The radial support structure also needs to offset the stress and deformation of the mirror caused by the temperature change of the working...

Claims

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Application Information

Patent Timeline
18 Jun 2014
Publication
CN102508347B
IPC
G02B7/00; G02B23/00
Inventors
吴小霞; 杨飞