CN206161945U - Novel card formula collimator device - Google Patents
Novel card formula collimator device Download PDFInfo
- Publication number
- CN206161945U CN206161945U CN201621252202.6U CN201621252202U CN206161945U CN 206161945 U CN206161945 U CN 206161945U CN 201621252202 U CN201621252202 U CN 201621252202U CN 206161945 U CN206161945 U CN 206161945U
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- graticle
- mirror
- frame
- telescope
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Abstract
The utility model discloses a novel card formula collimator device, include primary mirror subassembly, secondary mirror subassembly, mirror tube and take the frame graticule, wherein, primary mirror subassembly and secondary mirror subassembly install respectively in mirror tube's both ends, the primary mirror subassembly is kept away from mirror tube's terminal surface facial make -up is equipped with graduation seat connecting plate, and the packing ring has been installed at the middle part of this graduation seat connecting plate, the packing ring is kept away from installed through the graduation panel seat on mirror tube's the terminal surface take the frame graticule, should take the frame graticule to lock by the clamp ring. The utility model discloses can effectively solve ordinary straight tube type collimator relative aperture and the visual field is little, the focus is short, bulky scheduling problem, and it is convenient, small to have an easy operation, convenient outdoor use, and it is high to produce quality control school precision, range of application advantage such as wide.
Description
Technical field
The utility model belongs to optical instrument calibration field, more particularly, to a kind of Novel clamped parallel light tube device.
Background technology
Parallel light tube is the optical instrument for producing collimated light beam, it be Photoelectric Detection, optical system calibration it is important
Equipment.The uniformity that Display Aim Taking on TV Set axle at present in electro-optical system, infrared sight take aim at many optical axises such as axle, laser ranging transmitting optical axis is straight
Connect and determine the degree of accuracy detected to target information with acquisition.
Traditional straight pipe type parallel light tube relative aperture and visual field is little, focal length is short, bulky, it is impossible to fast and accurately school
The uniformity of many optical axises in accurate multispectral electro-optical tracking device, while being unfavorable for that open air uses.
Utility model content
For the disadvantages described above or Improvement requirement of prior art, the utility model is filled there is provided a kind of cassette parallel light tube
Put, wherein by the structure to its key component primary mirror component, secondary mirror assembly and with frame reticule assembly and its concrete setting side
Formula is studied and designed, can effectively solving ordinary straight tubular type parallel light tube relative aperture and visual field are little, focal length is short, bulky
The problems such as, with simple to operation, small volume, facilitate open air to use, product calibration high precision, the advantages of applied range.
For achieving the above object, the utility model proposes a kind of Novel clamped parallel light tube device, including primary mirror component,
Secondary mirror assembly, telescope and band frame graticle, wherein：
The primary mirror component and time mirror assembly are installed in respectively the two ends of the telescope, and the primary mirror component is away from the mirror
Graduation seat connecting plate is equiped with the end face of pipe, in the middle part of the graduation seat connecting plate packing ring is equiped with, the packing ring is away from institute
State and the band frame graticle is equiped with by graduation panel seat on the end face of telescope, the band frame graticle is locked by clamp ring.
As it is further preferred that the primary mirror component include principal reflection mirror, primary frame and core cylinder, wherein：The master is anti-
Penetrate in the middle part of mirror and offer centre bore, it is flush-mounted in the inside of the primary frame, and is compressed by pressing plate；The primary frame is flush-mounted in
One end of the telescope；, horizontal through the centre bore of the principal reflection mirror, and by trim ring and only spiral shell is only tight for the core cylinder.
As it is further preferred that described mirror assembly includes protecgulum, adjusting rod, parallax components and secondary mirror, wherein：
The protecgulum is arranged on the other end of the telescope, and time picture frame is embedded with inside it, and lid is provided with this picture frame；The regulation
Above-mentioned lid is inserted in one end of bar, and the other end is connected with the parallax components；The parallax components include be sequentially connected connecting seat,
Packing ring and time microscope base, wherein, the connecting seat is connected with the adjusting rod, and on described microscope base the secondary mirror is pasted with.
As it is further preferred that the band frame graticle includes graticle housing, two graticle trim rings and graticle,
Wherein, described two graticle trim rings are arranged on the two ends inside the graticle housing, and are threadedly coupled with graticle housing,
The graticle is arranged between two graticle trim rings, and is fitted with the end face of two graticle trim rings, and it is only tight by only spiral shell.
In general, by the contemplated above technical scheme of the utility model possess compared with prior art, mainly with
Under technological merit：
1. the utility model by the structure to key component primary mirror component, secondary mirror assembly and with frame reticule assembly and its
Concrete set-up mode is studied and designed, and Novel clamped parallel light tube device is obtained, with simple to operation, volume
It is little, facilitate open air to use, product calibration high precision, the advantages of applied range.
2. the utility model adopts reflective optical system, can ultraviolet to infrared broadband operated within range, and
No color differnece, without thermalization, compact conformation, various wavelength light imagings all unanimously overlap, and system axial distance can be reduced to
Originally the 1/3 of focal length, solves the problems, such as that the little focal length of ordinary straight tubular type parallel light tube relative aperture and visual field is short bulky.
Description of the drawings
Fig. 1 is the sectional view of the cassette parallel light tube device of the utility model embodiment；
Fig. 2 is the stereogram of the cassette parallel light tube device of the utility model embodiment；
Fig. 3 is the primary mirror assemble cross-section of the utility model embodiment；
Fig. 4 is the secondary mirror assemble cross-section of the utility model embodiment；
Fig. 5 is the band frame graticle sectional view of the utility model embodiment；
Fig. 6 is the optical system diagram of the cassette parallel light tube device of the utility model embodiment.
Specific embodiment
In order that the purpose of this utility model, technical scheme and advantage become more apparent, below in conjunction with accompanying drawing and enforcement
Example, is further elaborated to the utility model.It should be appreciated that specific embodiment described herein is only to explain
The utility model, is not used to limit the utility model.Additionally, institute in the utility model disclosed below each embodiment
As long as the technical characteristic being related to does not constitute each other conflict and just can be mutually combined.
As shown in figure 1, a kind of Novel clamped parallel light tube device that the utility model embodiment is provided, it includes primary mirror group
Part 1, secondary mirror assembly 2, band frame graticle 3 and telescope 4, when using, light is first passed around with the graticle 3-3 in frame graticle 3,
Then outgoing directional light after the principal reflection mirror 1-1 Jing secondary mirror 2-1 in time mirror assembly 2 and in primary mirror component 1 reflects, and mirror
Pipe 4 is used to install fixed primary mirror component 1, secondary mirror assembly 2 and band frame graticle 3.By cooperating for above-mentioned all parts, can
The correction of the light axis consistencies such as the infrared, white light of photoelectric comprehensive product is realized, while infrared light supply target can also be produced, with behaviour
Make simple and convenient, small volume facilitates open air to use, product calibration high precision, the advantages of applied range.
Below more specific detail will be one by one carried out to each component.
Used as the primary mirror component 1 of one of key component, it is installed in one end (right-hand member of Fig. 1) of telescope 4, and it is away from telescope
(i.e. the right-hand member of Fig. 1) is equiped with graduation seat connecting plate 9 on 4 end face, and the middle part of the graduation seat connecting plate 9 is equiped with the first pad
Circle 7, (i.e. the right-hand member of Fig. 1) is equiped with graduation panel seat 8, the first packing ring 7 and graduation on end face of first packing ring 7 away from telescope 4
Panel seat 8 is fixed on graduation seat connecting plate 9, and band frame graticle 3 is equiped with graduation panel seat 8.
As shown in figure 3, primary mirror component 1 includes principal reflection mirror 1-1, primary frame 1-2 and core cylinder 1-3, wherein：Primary frame 1-2
It is flush-mounted in one end (right-hand member of Fig. 1) of telescope 4；Principal reflection mirror 1-1 is flush-mounted in the inside of primary frame 1-2, during its middle part offers
Heart hole, and compressed by pressing plate 1-6, pressing plate 1-6 is provided with altogether three pieces；Core cylinder 1-3 horizontal through principal reflection mirror 1-1 centre bore,
And stop tight by trim ring 1-4 and only spiral shell.Specifically, as shown in figure 3, by core cylinder 1-3 from left to right through the center of principal reflection mirror 1-1
Hole, is equiped with packing ring 1-5 between its left end and principal reflection mirror 1-1, packing ring is equally equiped between its right-hand member and principal reflection mirror 1-1
1-5, is then threaded into trim ring 1-4 in its right-hand member, and by stopping spiral shell that trim ring 1-4 is only tight.Specifically, graduation seat connection
The outer end installing framed 5 of plate 9, the frame 5 is fixed to above primary frame 1-2 in primary mirror component 1.
Used as the secondary mirror assembly 2 of one of another key component, it is installed in the other end (left end of Fig. 1) of telescope 4, such as schemes
Shown in 4, secondary mirror assembly 2 includes protecgulum 2-9, adjusting rod 2-4, parallax components and secondary mirror 2-1, wherein：Protecgulum 2-9 is arranged on
The other end (left end of Fig. 1) of telescope 4, is embedded with time picture frame 2-3 inside it, lid 2-7 is provided with this picture frame 2-3；It is described
One end (left end of Fig. 4) of adjusting rod 2-4 is inserted in above-mentioned lid 2-7, and the other end (right-hand member of Fig. 4) is connected with parallax components and (has
Body is connected with the connecting seat 2-8 in parallax components by screw thread)；Connecting seat 2-8 that the parallax components include being sequentially connected, the
Two packing ring 2-2 and time microscope base 2-6, secondary mirror 2-1 is pasted with secondary microscope base 2-6 by glue, secondary mirror 2-1 and master
SMIS cylinder 1-3 is relative for mirror assembly 1.For the ease of the fixed installation of adjusting rod 2-4, on lid 2-7 gland 2-5 is fixed with.
Used as the band frame graticle 3 of one of another key component, it is locked on graduation panel seat 8 by clamp ring 6, such as Fig. 5
Shown, it includes graticle housing 3-1, two graticle trim ring 3-2 and graticle 3-3, wherein, two graticle trim ring 3-2
Two ends inside graticle housing 3-1, and be threadedly coupled with graticle housing 3-1, graticle 3-3 is arranged on two points
Draw between plate trim ring 3-2, and fit with the end face of two graticle trim ring 3-2, it is only tight by only spiral shell.
Additionally, the installation for the ease of whole parallel light tube device is fixed, the outside of telescope 4 is provided with support 10.
The utility model when in use, cassette parallel light tube is placed on firm platform, twists off graticle clamp ring 6,
Graticle 3-3 required for selecting is loaded on cassette parallel light tube afterbody, then puts at the rear (the right of Fig. 1) of graticle 3-3
Black matrix gripper shoe is put, black matrix is placed in black matrix gripper shoe, finally connect black matrix power supply, adjust black matrix to temperature required.
The optical system diagram of cassette parallel light tube device of the present utility model is illustrated in figure 6, when using, light Jing first
Graticle 3-3 is crossed, then the outgoing directional light Jing after secondary mirror 2-1, principal reflection mirror 1-1 reflections.
As it will be easily appreciated by one skilled in the art that preferred embodiment of the present utility model is the foregoing is only, not
To limit the utility model, all any modifications made within spirit of the present utility model and principle, equivalent and change
Enter, should be included within protection domain of the present utility model.
Claims (4)
1. a kind of Novel clamped parallel light tube device, it is characterised in that including primary mirror component (1), secondary mirror assembly (2), band frame point
Plate (3) and telescope (4) are drawn, wherein：
The primary mirror component (1) and time mirror assembly (2) are installed in respectively the two ends of the telescope (4), and the primary mirror component (1) is remote
Graduation seat connecting plate (9) is equiped with the end face of the telescope (4), is equiped with the middle part of graduation seat connecting plate (9)
One packing ring (7), first packing ring (7) is equiped with the band away from the end face of the telescope (4) by graduation panel seat (8)
Frame graticle (3), band frame graticle (3) is locked by clamp ring (6).
2. Novel clamped parallel light tube device as claimed in claim 1, it is characterised in that the primary mirror component (1) is including master
Speculum (1-1), primary frame (1-2) and core cylinder (1-3), wherein：Centre bore is offered in the middle part of the principal reflection mirror (1-1),
It is flush-mounted in the inside of the primary frame (1-2), and is compressed by pressing plate (1-6)；The primary frame (1-2) is flush-mounted in the telescope
(4) one end；, horizontal through the centre bore of the principal reflection mirror (1-1), and by trim ring and only spiral shell is only tight for the core cylinder (1-3).
3. Novel clamped parallel light tube device as claimed in claim 2, it is characterised in that described mirror assembly (2) is including front
Lid (2-9), adjusting rod (2-4), parallax components and secondary mirror (2-1), wherein：The protecgulum (2-9) is arranged on the telescope
(4) the other end, is embedded with time picture frame (2-3) inside it, on this picture frame (2-3) lid (2-7) is provided with；The adjusting rod
(2-4) above-mentioned lid (2-7) is inserted in one end, and the other end is connected with the parallax components；The parallax components include being sequentially connected
Connecting seat (2-8), second packing ring (2-2) and time microscope base (2-6), wherein, the connecting seat (2-8) and the adjusting rod (2-
4) it is connected, on described microscope base (2-6) secondary mirror (2-1) is pasted with.
4. Novel clamped parallel light tube device as claimed in claim 3, it is characterised in that band frame graticle (3) includes
Graticle housing (3-1), two graticle trim rings (3-2) and graticle (3-3), wherein, described two graticle trim rings (3-2)
Installed in the internal two ends of the graticle housing (3-1), and it is threadedly coupled with graticle housing (3-1), the graticle (3-
3) between two graticle trim rings (3-2), and fit with the end face of two graticle trim rings (3-2), it is stopped by only spiral shell
Tightly.
Priority Applications (1)
| Application Number | Priority Date | Filing Date | Title |
|---|---|---|---|
| CN201621252202.6U CN206161945U (en) | 2016-11-16 | 2016-11-16 | Novel card formula collimator device |
Applications Claiming Priority (1)
| Application Number | Priority Date | Filing Date | Title |
|---|---|---|---|
| CN201621252202.6U CN206161945U (en) | 2016-11-16 | 2016-11-16 | Novel card formula collimator device |
Publications (1)
| Publication Number | Publication Date |
|---|---|
| CN206161945U true CN206161945U (en) | 2017-05-10 |
Family
ID=58660628
Family Applications (1)
| Application Number | Title | Priority Date | Filing Date |
|---|---|---|---|
| CN201621252202.6U Active CN206161945U (en) | 2016-11-16 | 2016-11-16 | Novel card formula collimator device |
Country Status (1)
| Country | Link |
|---|---|
| CN (1) | CN206161945U (en) |
Cited By (7)
| Publication number | Priority date | Publication date | Assignee | Title |
|---|---|---|---|---|
| CN107037566A (en) * | 2017-05-24 | 2017-08-11 | 北京空间机电研究所 | A kind of segmented secondary mirror high stability supporting construction |
| CN107577028A (en) * | 2017-09-20 | 2018-01-12 | 长春理工大学 | A kind of multi-purpose laser communication optics antenna system |
| CN108241198A (en) * | 2018-02-07 | 2018-07-03 | 中国科学院光电研究院 | The main secondary mirror supporting structure of coaxial spaces camera |
| CN110955015A (en) * | 2019-12-19 | 2020-04-03 | 中国科学院长春光学精密机械与物理研究所 | Wide-temperature-adaptability collimator reflector supporting structure |
| CN111164491A (en) * | 2017-10-11 | 2020-05-15 | 科磊股份有限公司 | Lens design for spectroscopic ellipsometer or reflectometer |
| CN112882185A (en) * | 2021-01-22 | 2021-06-01 | 西安应用光学研究所 | Glue joint fixing structure and fixing method suitable for adjustable lens group of reflecting system |
| CN113296284A (en) * | 2021-04-14 | 2021-08-24 | 三河市蓝思泰克光电科技有限公司 | Ultra-low temperature collimator device under vacuum environment |
-
2016
- 2016-11-16 CN CN201621252202.6U patent/CN206161945U/en active Active
Cited By (9)
| Publication number | Priority date | Publication date | Assignee | Title |
|---|---|---|---|---|
| CN107037566A (en) * | 2017-05-24 | 2017-08-11 | 北京空间机电研究所 | A kind of segmented secondary mirror high stability supporting construction |
| CN107577028A (en) * | 2017-09-20 | 2018-01-12 | 长春理工大学 | A kind of multi-purpose laser communication optics antenna system |
| CN107577028B (en) * | 2017-09-20 | 2020-03-24 | 长春理工大学 | Multipurpose laser communication optical antenna system |
| CN111164491A (en) * | 2017-10-11 | 2020-05-15 | 科磊股份有限公司 | Lens design for spectroscopic ellipsometer or reflectometer |
| CN108241198A (en) * | 2018-02-07 | 2018-07-03 | 中国科学院光电研究院 | The main secondary mirror supporting structure of coaxial spaces camera |
| CN110955015A (en) * | 2019-12-19 | 2020-04-03 | 中国科学院长春光学精密机械与物理研究所 | Wide-temperature-adaptability collimator reflector supporting structure |
| CN112882185A (en) * | 2021-01-22 | 2021-06-01 | 西安应用光学研究所 | Glue joint fixing structure and fixing method suitable for adjustable lens group of reflecting system |
| CN112882185B (en) * | 2021-01-22 | 2023-03-03 | 西安应用光学研究所 | Glue joint fixing structure and fixing method suitable for adjustable lens group of reflection system |
| CN113296284A (en) * | 2021-04-14 | 2021-08-24 | 三河市蓝思泰克光电科技有限公司 | Ultra-low temperature collimator device under vacuum environment |
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