Telescope anti-shake structure and control method thereof

By adopting the anti-shake structure of driving motors, magnets and gyroscopes in the telescope, combined with the parallelogram principle and real-time signal compensation control, the problem of poor anti-shake effect of the telescope is solved, and the stability of the telescope under intense motion is achieved and the optical axis adjustment is simplified, which is convenient for diversified applications.

CN120255137AInactive Publication Date: 2025-07-04KUNMING PAIDU TRADING CO LTD
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Patent Information

Application Number
CN202510484833.8
Authority / Receiving Office
CN · China
Patent Type
Applications(China)
Current Assignee / Owner
Filing Date
2025-04-17
Publication Date
2025-07-04
Estimated Expiration
Not applicable · inactive patent

AI Technical Summary

Technical Problem

The anti-shake structure of existing telescopes is not effective, and it is easy to shake during use, causing blurred images, making adjustments troublesome.

Method used

Adopt anti-shake structure including the second frame and the first frame, a built-in drive motor and magnet, and jitter signals are collected through gyroscopes and angular velocity sensors, and stable rotation of the prism group or focus mirror group is achieved using the parallelogram principle and magnetic suction connection, and real-time compensation control is performed in combination with the motor control board and the microcontroller processor.

Benefits of technology

It achieves stronger stability of the telescope in the case of intense exercise, simple adjustment of the optical axis, suitable for different anti-shake systems, supports modular design, and is convenient for customized production.

✦ Generated by Eureka AI based on patent content.

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Abstract

The invention relates to the field of telescopes, and discloses an anti-shake structure of a telescope and a control method thereof.The anti-shake structure comprises a second frame and a first frame, driving motors are fixedly connected to the interiors of the second frame and the first frame, magnets are fixedly arranged at the output ends of the driving motors, and a prism set or a focusing lens set is arranged on the outer wall of each magnet; a bearing is rotatably connected in the prism group or the focusing lens group, prism seats or focusing lens seats are fixedly connected to the outer wall of the prism group or the focusing lens group, and a connecting cross beam is fixedly connected between the prism seats or the focusing lens seats. By applying the characteristic that the two sides of the parallelogram are always kept parallel, the optical axes of the two prism sets or the focusing lens sets are accurately ensured to be always parallel by the two prism sets or the focusing lens sets, the optical axis of a single prism set or a single focusing lens set can be independently adjusted, and the effects that the displacement correction of the two prism sets or the focusing lens sets is consistent and the stability is higher are achieved.
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Description

Technical Field

[0001] The present invention relates to the technical field of telescopes, and specifically to an anti-shake structure of a telescope and its control method. Background Art

[0002] A telescope is an optical instrument that collects and focuses light through a combination of lenses or mirrors, making distant objects appear closer, larger, or clearer. When holding a telescope by hand, the shaking of the hand will affect the observation effect. An anti-shake structure can compensate for this shaking, making hand-held observation more stable and comfortable, so an anti-shake structure of a telescope will be used.

[0003] The anti-shake structure of a telescope refers to a special mechanical or electronic system added to the telescope to reduce or eliminate the shaking of the telescope caused by hand tremors or other external factors. In the existing telescope technology, the anti-shake effect of the telescope is not good, and it is easy to cause image blurring due to shaking during use. Summary of the Invention

[0004] Aiming at the deficiencies of the prior art, the present invention provides an anti-shake structure of a telescope and its control method, which solves the problems of poor anti-shake effect and troublesome adjustment during the use of the telescope.

[0005] To achieve the above object, the present invention is realized through the following technical solutions: An anti-shake structure of a telescope includes a second frame and a first frame. Inside both the second frame and the first frame, a driving motor is fixedly connected. The output end of the driving motor is fixedly provided with a magnet. An outer wall of the magnet is provided with a prism group or a focusing lens group. The outer wall of the magnet is arranged on the outer wall of the first frame. Inside the prism group or the focusing lens group, a bearing is rotatably connected. An outer wall of the bearing is fixedly connected inside the second frame. The inside of the first frame is rotatably connected to the outer wall of the bearing. An outer wall of the prism group or the focusing lens group is fixedly connected with a prism seat or a focusing lens seat. The outer wall of the prism seat or the focusing lens seat is arranged inside the second frame. A connecting cross beam is fixedly connected between the prism seats or the focusing lens seats.

[0006] Preferably, the driving motor is installed inside the first frame and the driving motor is installed inside the second frame.

[0007] Preferably, a gyroscope and an angular velocity sensor are arranged on an outer wall of the prism group or the focusing lens group, and the gyroscope and the angular velocity sensor are used to collect shaking signals on the X-axis and the Y-axis.

[0008] Preferably, an outer wall of the gyroscope and the angular velocity sensor is electrically connected to a motor control board, and the inside of the motor control board is electrically connected to an outer wall of the driving motor.

[0009] Preferably, the outer wall of the motor control board is installed inside the second frame, and the motor control board is connected to the gyroscope and the angular velocity sensor by wiring, so that the entire circuit part is dispersed.

[0010] Preferably, the driving motor and the magnet are magnetically connected to adsorb the prism group or the focusing lens group, thereby driving the prism group or the focusing lens group to rotate.

[0011] Preferably, the driving motor pushes a group of prism groups or focusing lens groups to rotate, thereby driving the second group of prism groups or focusing lens groups to rotate. The first frame is pushed to rotate in the Y-axis direction by the driving motor, driving the rotation of the two prism seats or focusing lens seats in the Y-axis direction, so that the X-axis direction and the Y-axis direction can work independently.

[0012] Preferably, the prism seat or the focusing lens seat is installed inside the first frame, and the prism seats or the focusing lens seats are rigidly connected by the parallelogram principle.

[0013] Preferably, the prism group or the focusing lens group is supported and fixed by bearings to ensure synchronous movement in the X-axis direction inside the first frame.

[0014] A control method for the anti-shake structure of a telescope, used for the anti-shake structure of a telescope, the method comprising the following steps: S1. Power on and calibrate the zero position; S2. The gyroscope and the angular velocity sensor collect jitter signals, and the jitter signals include direction and angular acceleration; S3. The MCU compares the zero position with the newly collected signal according to a preset threshold, and after processing and calculation, sends a motion execution signal to the driving motor: S3.1 If it exceeds the set threshold, return to S1 again; S3.2 Execute downward within the set threshold range; S4. The driving motor executes the motion instruction to drive the component to move; S5. The gyroscope and the angular velocity sensor collect signals in real time, and return to the calibrated zero position until the moving component is detected, and send an instruction; S6. The driving motor parks and returns to S2 again.

[0015] Working principle: When the telescope module is jittered during use, gyroscopes and acceleration sensors on the prism base or the focusing lens base collect jitter signals on the X-axis and Y-axis. The gyroscopes are connected to the single-chip microcomputer processor circuit board, the single-chip microcomputer circuit board is connected to the motor control board, and the motor control board is connected to two driving motors. The gyroscopes and acceleration sensors transmit the real-time jitter signals to the single-chip microcomputer for processing. After calculation, the single-chip microcomputer outputs control signals to the motor control board, and the motor control board controls the movement of the driving motors. When the driving motors drive the prism group or the focusing lens back to the calibrated position before jitter, the gyroscopes will collect signals and return to the original position, and the entire system recalibrates the initial position. The gyroscopes and acceleration sensors collect the direction, angle, and acceleration of the jitter signals, and the single-chip microcomputer calculates the numerical value of the motor compensation according to the data. Through the control of this closed-loop system, the movement of the telescope module is corrected in real time, ensuring that it still has good anti-shake function under intense movement conditions; Through the linkage drive adopted in the structure, this anti-shake module can be used not only in the prism anti-shake system, including roof prisms, Abbe prisms, and Porro prisms, but also in the focusing lens anti-shake system. It can be achieved simply by replacing the prism base or the focusing lens base, achieving a modular product design, facilitating the use in different aspects, and also providing convenience for the diversified customized production of products.

[0016] The present invention provides an anti-shake structure of a telescope and its control method. It has the following beneficial effects: 1. By applying the characteristic that the two sides of a parallelogram always remain parallel, the present invention enables the two prism bases or focusing lens bases to accurately ensure that the optical axes of the two prism groups or focusing lens groups are always parallel. The optical axis of a single prism group or focusing lens group can be adjusted separately, achieving the effect of ensuring consistent displacement correction of the two prism groups or focusing lens groups, with stronger stability. The structure is simple, making the optical axis calibration easier.

[0017] 2. Through the linkage drive, the present invention can be used not only in the prism anti-shake system but also in the focusing lens anti-shake system. It can be achieved simply by replacing the prism base or the focusing lens base, achieving a modular product design, facilitating the use in different aspects, and providing convenience for the diversified customized production of products. BRIEF DESCRIPTION OF THE DRAWINGS

[0018] Figure 1 is a three-dimensional view of the present invention; Figure 2 is a partial structural schematic diagram of the bearing of the present invention; Figure 3 is a partial structural schematic diagram of the bearing of the present invention; Figure 4 is a partial structural schematic diagram of the prism base or the focusing lens base of the present invention; Figure 5Schematic diagram of the partial structure of the prism group or focusing lens group of the present invention; Figure 6 Schematic cross-sectional view of the internal structure of the present invention; Figure 7 Front view of the present invention; Figure 8 Schematic cross-sectional view of the internal structure of the present invention; Figure 9 Schematic cross-sectional view of the internal structure of the present invention; Figure 10 Flow chart of the present invention.

[0019] Wherein, 1, driving motor; 2, second frame; 3, first frame; 4, prism group or focusing lens group; 5, magnet; 6, bearing; 7, prism seat or focusing lens seat; 8, connecting cross beam; 9, motor control board; 10, gyroscope and angular velocity sensor. Specific embodiments

[0020] Next, the technical solutions of the present invention will be clearly and completely described in conjunction with the accompanying drawings of the present invention. Obviously, the described embodiments are only a part of the embodiments of the present invention, rather than all the embodiments. Based on the embodiments of the present invention, all other embodiments obtained by those of ordinary skill in the art without creative efforts shall fall within the protection scope of the present invention.

[0021] Please refer to the attached Figure 1 - attached Figure 9 , the embodiment of the present invention provides an anti-shake structure for a telescope, including a second frame 2 and a first frame 3. Driving motors 1 are fixedly connected inside both the second frame 2 and the first frame 3. A magnet 5 is fixedly arranged at the output end of the driving motor 1. A prism group or focusing lens group 4 is arranged on the outer wall of the magnet 5. The outer wall of the magnet 5 is arranged on the outer wall of the first frame 3. A bearing 6 is rotatably connected inside the prism group or focusing lens group 4. The outer wall of the bearing 6 is fixedly connected inside the second frame 2. The inside of the first frame 3 is rotatably connected to the outer wall of the bearing 6. A prism seat or focusing lens seat 7 is fixedly connected to the outer wall of the prism group or focusing lens group 4. The outer wall of the prism seat or focusing lens seat 7 is arranged inside the second frame 2. A connecting cross beam 8 is fixedly connected between the prism seats or focusing lens seats 7; Specifically, the first frame 3 and the second frame 2 play a role in supporting and fixing both the driving motor 1 in the X-axis direction and the driving motor 1 in the Y-axis direction. Through the driving effect of the driving motor 1, the magnet 5 can be driven to rotate. The magnet 5 in the X-axis direction and the magnet 5 in the Y-axis direction respectively play a role in fixing the prism group or the focusing lens group 4 and the first frame 3, and can respectively drive the prism group or the focusing lens group 4 and the first frame 3 to rotate. When the driving motor 1 in the X-axis direction starts, it can drive a group of prism groups or focusing lens groups 4 to rotate and drive the other group of prism groups or focusing lens groups 4 to rotate synchronously through the connecting cross beam 8. The magnetic connection can avoid the gaps in the assembly of parts and achieve higher precision. The bearing 6 plays a role in supporting the prism group or the focusing lens group 4, enabling the prism group or the focusing lens group 4 to rotate stably. Through the parallelogram principle between the two prism seats or focusing lens seats 7, the prism groups or focusing lens groups 4 on both sides can always maintain the characteristic of being parallel, enabling the two prism seats or focusing lens seats 7 to accurately ensure that the optical axes of the two prism groups or focusing lens groups 4 are always parallel. The linkage of the two prism seats or focusing lens seats 7 ensures that the movement corrections of the two prism groups or focusing lens groups 4 are always consistent, with stronger stability, a simple structure, and also making the optical axis calibration simpler.

[0022] Please refer to the attached Figure 1 - attached Figure 5 , the driving motor 1 is installed inside the first frame 3, and the driving motor 1 is installed inside the second frame 2; Specifically, the first frame 3 plays a role in fixing the driving motor 1 in the X-axis direction, can drive a group of prism seats or focusing lens seats 7 to move and drive the second group of prism seats or focusing lens seats 7 to move synchronously through the connecting cross beam 8. The second frame 2 plays a role in fixing the driving motor 1 in the Y-axis direction, and can drive the first frame 3 to drive the two prism groups or focusing lens groups 4 to move synchronously in the Y-axis direction.

[0023] Please refer to the attached Figure 1 - attached Figure 7 , a gyroscope and an angular velocity sensor 10 are arranged on the outer wall of the prism group or the focusing lens group 4, and the gyroscope and the angular velocity sensor 10 are used to collect the jitter signals of the X-axis and the Y-axis; Specifically, the gyroscope and the angular velocity sensor 10 can be installed on a group of prism groups or focusing lens groups 4 to collect the jitter signals of the X-axis and the Y-axis, or the gyroscope and the angular velocity sensor 10 can be installed on both groups of prism groups or focusing lens groups 4, which can be used to compare the two sets of data.

[0024] Please refer to the attached Figure 1 - attached Figure 7 , the outer wall of the gyroscope and the angular velocity sensor 10 is electrically connected to a motor control board 9, and the inside of the motor control board 9 is electrically connected to the outer wall of the driving motor 1; Specifically, the gyroscope and angular velocity sensor 10 are connected to the single-chip microcomputer processor circuit board, and the single-chip microcomputer processor circuit board is connected to the motor control board 9. By controlling the drive motor 1 through the motor control board 9, the control of the prism group or the focusing lens group 4 can be realized. The gyroscope and angular velocity sensor 10 can collect real-time jitter signals and transmit the signals to the single-chip microcomputer for processing. After calculation, the single-chip microcomputer outputs a control signal to the motor control board 9. The motor control board 9 controls the movement of the drive motor 1. When the drive motor 1 drives the prism group or the focusing lens group 4 back to the calibrated position before jitter, the signals collected by the gyroscope and angular velocity sensor 10 return to their original positions, and the single-chip microcomputer calculates the compensation value of the drive motor 1 based on the data.

[0025] Please refer to the appendix Figure 1 - appendix Figure 7 The outer wall of the motor control board 9 is installed inside the second frame 2. The motor control board 9 and the gyroscope and angular velocity sensor 10 are connected by wiring, so that the entire circuit part is dispersed. Specifically, the second frame 2 plays a role in supporting and fixing the motor control board 9. By connecting the motor control board 9 and the gyroscope and angular velocity sensor 10 by wiring, the entire circuit can be dispersed, which can ensure better heat dissipation performance of the telescope under high-frequency movement.

[0026] Please refer to the appendix Figure 1 - appendix Figure 9 The drive motor 1 is magnetically connected to the magnet 5 to adsorb the prism group or the focusing lens group 4, thereby driving the prism group or the focusing lens group 4 to rotate. Specifically, by starting the drive motor 1, the magnet 5 can be driven to rotate, and the prism group or the focusing lens group 4 can be rotated by the adsorption of the magnet 5.

[0027] Please refer to the appendix Figure 1 - appendix Figure 9 The drive motor 1 pushes a group of prism groups or focusing lens groups 4 to rotate, thereby driving the second group of prism groups or focusing lens groups 4 to rotate. The first frame 3 is pushed to rotate in the Y-axis direction by the drive motor 1, driving the rotation of the two prism seats or focusing lens seats 7 in the Y-axis direction, so that the X-axis direction and the Y-axis direction can work independently. Specifically, the drive of the drive motor 1 can make the two prism groups or focusing lens groups 4 rotate in the X-axis direction, and the drive of the drive motor 1 on the other side can make the two prism seats or focusing lens seats 7 rotate in the Y-axis direction, thereby realizing independent work in the X-axis direction and the Y-axis direction.

[0028] Please refer to the appendix Figure 1 - appendix Figure 9 The prism seat or the focusing lens seat 7 is installed inside the first frame 3, and the prism seats or the focusing lens seats 7 are rigidly connected by the parallelogram principle. Specifically, the first frame 3 supports the prism base or the focusing lens base 7. Through the connecting cross beam 8 between the two groups of prism bases or focusing lens bases 7, when the first frame 3 rotates under the driving action of the driving motor 1, the prism base or the focusing lens base 7 can be driven to be adjusted, and the stability between the two groups of prism bases or focusing lens bases 7 can be ensured through the connecting cross beam 8.

[0029] Please refer to the appendix Figure 1 - appendix Figure 3 , the prism group or the focusing lens group 4 is supported and fixed by the bearing 6 to ensure synchronous movement in the X-axis direction inside the first frame 3; Specifically, through the supporting action of the bearing 6 on the prism group or the focusing lens group 4, the stable adjustment of the prism group or the focusing lens group 4 can be ensured, and the prism group or the focusing lens group 4 can be rotated synchronously inside the first frame 3.

[0030] Please refer to the appendix Figure 10 , a control method for the anti-shake structure of a telescope, which is used for the anti-shake structure of a telescope, and the method includes the following steps: S1. Power on and calibrate the zero position; S2. The gyroscope and the angular velocity sensor 10 collect jitter signals, and the jitter signals include direction and angular acceleration; S3. The MCU compares the zero position with the newly collected signal according to the preset threshold, and after processing and calculation, sends a motion execution signal to the driving motor 1: S3.1 If it exceeds the set threshold, return to S1 again; S3.2 Execute downward within the set threshold range; S4. The driving motor 1 executes the motion instruction to drive the component to move; S5. The gyroscope and the angular velocity sensor 10 collect signals in real time, and return to the calibrated zero position until the moving component is detected, and an instruction is issued; S6. The driving motor 1 parks and returns to S2 again; Specifically, when the driving motor 1 drives the prism group or the focusing lens group 4 back to the position calibrated before jitter, the gyroscope and the angular velocity sensor 10 collect signals. When it exceeds the set threshold, it will return to the original position, and then the entire system recalibrates the initial position. When the gyroscope and the angular velocity sensor 10 collect jitter signals within the set threshold, the single-chip microcomputer calculates the compensation value of the driving motor 1 according to the data, and then can execute the motion instruction, and then drive the prism group or the focusing lens group 4 to rotate, and correct the motion of the anti-shake module in real time. Through the control of this closed-loop system, it can be ensured that a good anti-shake function is still available in the case of intense movement.

[0031] Although embodiments of the present invention have been shown and described, it will be understood by those of ordinary skill in the art that various changes, modifications, substitutions and variations can be made to these embodiments without departing from the principles and spirit of the present invention, and the scope of the present invention is defined by the appended claims and their equivalents.

Claims

1. An anti-shake structure for a telescope, comprising a second frame (2) and a first frame (3), characterized in that: A driving motor (1) is fixedly connected inside both the second frame (2) and the first frame (3). A magnet (5) is fixedly arranged at the output end of the driving motor (1). A prism group or a focusing lens group (4) is arranged on the outer wall of the magnet (5). The outer wall of the magnet (5) is arranged on the outer wall of the first frame (3). A bearing (6) is rotatably connected inside the prism group or the focusing lens group (4). The outer wall of the bearing (6) is fixedly connected inside the second frame (2). The inside of the first frame (3) is rotatably connected to the outer wall of the bearing (6). A prism base or a focusing lens base (7) is fixedly connected to the outer wall of the prism group or the focusing lens group (4). The outer wall of the prism base or the focusing lens base (7) is arranged inside the second frame (2). A connecting cross beam (8) is fixedly connected between the prism bases or the focusing lens bases (7).

2. The anti-shake structure of a telescope according to claim 1, characterized in that: The driving motor (1) is installed inside the first frame (3), and the driving motor (1) is installed inside the second frame (2).

3. The anti-shake structure of a telescope according to claim 1, wherein: A gyroscope and an angular velocity sensor (10) are arranged on the outer wall of the prism group or the focusing lens group (4). The gyroscope and the angular velocity sensor (10) are used to collect jitter signals in the X-axis and Y-axis directions.

4. The anti-shake structure of a telescope according to claim 3, wherein: The outer wall of the gyroscope and the angular velocity sensor (10) is electrically connected to a motor control board (9). The inside of the motor control board (9) is electrically connected to the outer wall of the driving motor (1).

5. The anti-shake structure of a telescope according to claim 4, characterized in that: The outer wall of the motor control board (9) is installed inside the second frame (2). The motor control board (9) and the gyroscope and the angular velocity sensor (10) are connected by wiring, so that the entire circuit part is dispersed.

6. The anti-shake structure of a telescope according to claim 1, characterized in that: The driving motor (1) and the magnet (5) are magnetically connected to adsorb the prism group or the focusing lens group (4), thereby driving the prism group or the focusing lens group (4) to rotate.

7. The anti-shake structure of a telescope according to claim 1, wherein: The driving motor (1) drives a group of prism groups or focusing lens groups (4) to rotate, thereby driving the second group of prism groups or focusing lens groups (4) to rotate. The first frame (3) is driven to rotate in the Y-axis direction by the driving motor (1), driving the two prism bases or focusing lens bases (7) to rotate in the Y-axis direction, so that the X-axis direction and the Y-axis direction can work independently.

8. The anti-shake structure of a telescope according to claim 1, wherein: The prism base or the focusing lens base (7) is installed inside the first frame (3). The prism bases or the focusing lens bases (7) are rigidly connected by the parallelogram principle.

9. The anti-shake structure of a telescope according to claim 1, characterized in that: The prism group or the focusing lens group (4) is supported and fixed by the bearing (6) to ensure synchronous movement in the X-axis direction inside the first frame (3).

10. A control method for an anti-shake structure of a telescope, characterized in that: For an anti-shake structure of a telescope according to any one of claims 1-9, the method includes the following steps: S1. Power on and calibrate the zero position; S2. The gyroscope and the angular velocity sensor (10) collect jitter signals, and the jitter signals include direction and angular acceleration; S3. The MCU compares the zero position with the newly collected signal according to a preset threshold, and after processing and calculation, sends a motion execution signal to the driving motor (1): S3.1 If it exceeds the set threshold, return to S1 again; S3.2 Execute downward within the set threshold range; S4. The driving motor (1) executes the motion instruction to drive the component to move; S5. The gyroscope and angular velocity sensor (10) collect signals in real time, issue an instruction until the moving part returns to the calibrated zero position when detected. S6. The drive motor (1) parks and returns to S2 again.