WO2017200240A1

WO2017200240A1 - Telescope device cradled on glasses frame

Info

Publication number: WO2017200240A1
Application number: PCT/KR2017/004958
Authority: WO
Inventors: 권창민
Original assignee: 아이비케어 주식회사
Priority date: 2016-05-17
Filing date: 2017-05-12
Publication date: 2017-11-23
Also published as: KR101656430B1

Abstract

The present invention relates to a telescope device cradled on a glasses frame, the telescope device comprising: a telescope body; a connector portion formed on the telescope body; a hinge portion formed to be connected to the connector portion; and a glasses frame portion formed such that the hinge portion is coupled thereto, wherein the connector portion has a stop member formed thereon such that the same can rotate about the hinge portion and can stop at a specific location.

Description

Telescope device mounted on spectacle frame

The present invention relates to a telescope device mounted on the spectacle frame, and in more detail, when using the telescope mounted on the spectacle frame, the structure is formed so that the telescope can be rotated by 90 degrees on the spectacle frame so as not to obstruct the view. It relates to a telescope device mounted on the spectacle frame.

In general, the distance that a human can clearly identify objects and the like is only a few tens of meters, so a telescope is used to observe an object located at a distance that cannot be identified by the human eye.

Such a telescope is composed of an objective lens and an eyepiece, and the objective lens is located on the object side to collect light from the object, and the eyepiece is located on the eye side to enlarge the light collected at the focal point of the objective lens. do.

There are many kinds of telescopes such as binoculars, which are widely used for leisure and military use. The binoculars are seen in two-dimensional eyes by looking at the two telescopes, and the three-dimensional image can be easily distinguished from perspective.

That is, the binoculars are to magnify an object at a high magnification so that the object can be enlarged and viewed as if it is seen at a short distance, and an object lens receiving an image of the object, two prisms to refract the image passing through the object lens, and The eyepiece is configured to be an eyepiece which can be magnified and seen through the image passing through the prism.

Such binoculars have a magnification determined according to the number of lenses and the lens distance, and the size of the binoculars is determined.

These binoculars are widely used for leisure in modern times where leisure culture is developed. In particular, binoculars are widely used for watching various sports such as basketball and baseball, as well as traveling for migratory bird watching and beautiful scenery. .

However, conventional conventional binoculars are inconvenient because the user has to hold the hand by hand and look at the object, and especially when using the binoculars for a long time such as watching a game, the fatigue of the hand is accumulated due to the weight of the binoculars. There is considerable difficulty.

[Preceding technical literature]

[Patent Documents]

(Patent Document 1) Korean Utility Model Model No. 20-0192184

The present invention is to provide a telescope device which is mounted on the frame frame is formed so that the user can use the telescope for a long time without holding by hand.

The present invention includes a telescope body, a connector portion formed on the telescope body, a hinge portion formed to be connected to the connector portion, and a spectacle frame formed to be coupled to the hinge portion, the connector portion is rotated about the hinge portion While providing a telescope device mounted to the spectacle frame, characterized in that the stop member is formed so as to stop at a specific position.

The stop member may be a concave groove or a convex protrusion.

It may further include a torsion spring portion formed to fix the telescope body by performing a torsion spring action to a plurality of points of the glasses in a state of being fitted in the torsion groove formed on the side end of the hinge portion.

The telescope body may include a left telescope unit and a right telescope unit, and a gap controller configured to adjust a gap between the left telescope unit and the right telescope unit by using a gear.

The telescope body includes an objective lens unit for receiving light transmitted from a remote object and an eyepiece unit for receiving the light transmitted from the objective lens unit and transmitting the light to a user's eye, wherein the objective lens unit is transmitted from a remote object. A first concave mirror formed to receive light, a plane mirror formed to reflect light transmitted from the first concave mirror, and a second mirror formed to receive light transmitted from the plane mirror and to transmit the light back to the plane mirror It may include a concave mirror.

Effects produced by the present invention are as follows.

The user who uses the glasses can mount the telescope device according to the size of the glasses they are using.

And since the person using the glasses does not have to carry the telescope device by hand, the convenience of use is improved.

In addition, the present invention has a short length of the telescope body, even when the telescope body is mounted on the glasses, the effect that the glasses do not peel off well.

According to the present invention, a user who does not use glasses can attach a telescope to an eyeglass frame without eyeglasses, so that the trouble of having to observe the telescope when necessary while holding the telescope directly in his hand is prevented.

1 is a plan view (a), a front view (b) and a side view (c) illustrating a case where a telescope device mounted on an eyeglass frame according to the present invention is mounted on large glasses.

2 is a plan view (a), a front view (b) and a side view (c) illustrating a case where the telescope device mounted on the spectacle frame of the present invention is mounted on the medium sized glasses.

3 is a plan view (a), a front view (b) and a side view (c) illustrating a case where the telescope device mounted on the spectacle frame of the present invention is mounted on small glasses.

4 is an enlarged exploded view in which the portion A of FIG. 1 is enlarged and disassembled.

5 (a) is a case where the telescope device is located in front of the eyeglasses, and FIG. 5 (b) is a case where the telescope device is rotated 90 degrees and positioned in front of the eyeglasses.

6A is a schematic cross-sectional view showing the inside of the telescope body of the present invention, and FIG. 6B is a schematic cross-sectional view showing the inside of the conventional telescope body.

Figure 7 is a schematic orthogonal perspective view showing a structure capable of adjusting the distance between the two telescopes formed on the telescope body of the telescope device mounted on the spectacle frame of the present invention.

FIG. 8 is a schematic orthogonal view showing a state in which the distance between both telescopes is increased to the maximum in FIG. 7.

9 is a front view and a plan view showing a state in which the telescope device mounted on the spectacle frame is mounted on the spectacle frame.

FIG. 10 is a side view for explaining a position change of the telescope apparatus in FIG. 9. FIG.

Hereinafter, exemplary embodiments of the present invention will be described in detail with reference to the accompanying drawings. However, the accompanying drawings are only described in order to more easily disclose the contents of the present invention, but the scope of the present invention is not limited to the scope of the accompanying drawings that will be readily available to those of ordinary skill in the art. You will know.

In the description of the present embodiment, the same components and the same reference numerals are used for the same configuration, and additional description thereof will be omitted.

Also, the terminology used herein is for the purpose of describing particular embodiments only and is not intended to be limiting of the invention. Singular expressions include plural expressions unless the context clearly indicates otherwise. In this application, the terms "comprise" or "have" are intended to indicate that there is a feature, number, step, operation, component, part, or combination thereof described in the specification, and one or more other features. It is to be understood that the present invention does not exclude the possibility of the presence or the addition of numbers, steps, operations, components, components, or a combination thereof.

1 is a plan view (a), a front view (b) and a side view (c) illustrating a case in which the telescope device mounted on the spectacle frame of the present invention is mounted on large glasses, and FIG. 2 is a telescope apparatus mounted on the spectacle frame of the present invention. A plan view (a) and a front view (b) and a side view (c) showing the case where the glasses are mounted on the medium size glasses, and FIG. 3 is a plan view (a) showing the case where the telescope device mounted on the glasses frame of the present invention is mounted on the small glasses. ), Front view (b) and side view (c).

The telescope device 100 mounted on the spectacle frame of the present invention is divided into a first embodiment mounted on the spectacles of the person using the glasses and a second embodiment mounted on the spectacle frame without the glasses of the person who does not use the glasses. 3 is a case of the first embodiment in which the telescope is mounted on the spectacles of the person using the spectacles.

The telescope device 100 mounted on the spectacle frame according to the present invention includes a telescope body 110, a connector portion 130 formed on the telescope body 110, and a hinge portion 150 connected to the connector portion 130. ) And the left torsion spring part formed to fix the telescope body 110 by performing a torsion spring action at three points of the glasses while being fitted in the torsion grooves 152 formed at both ends of the hinge part 150, respectively. 170 and the right torsion spring portion 190.

The left torsion spring unit 170 may include a left upper mounting member 172 mounted on an upper portion of the left eyeglasses 210 and a first left lower mounting member 174 mounted on two lower points of the left eyeglasses 210. And a second left lower mounting member 176.

The right torsion spring unit 190 may include a right upper mounting member 192 mounted on an upper portion of the right eyeglass 230, a first right lower mounting member 194 mounted on two lower points of the right eyeglass 230. And a second right lower mounting member 196.

The left upper mounting member 172, the first left lower mounting member 174, the second left lower mounting member 176, the right upper mounting member 192, the first right lower mounting member 194 and the second right side The lower mounting member 196 is generally made of thin and hard iron or plastic to form the torsion spring, but the contact portion contacting the eyeglasses is formed of a soft material such as rubber to prevent damage to the eyeglasses.

The left upper mounting member 172 extends from the torsion groove 152 of the hinge portion 150 to the upper portion of the left eyeglasses 210 and is then bent 90 degrees to form the opposite side of the left eyeglasses 210, and then left upper contact. Portion 302 abuts the surface of left eyeglasses 210.

The first left lower mounting member 174 extends while contacting one surface of the left eyeglasses 210 from the torsion groove 152 of the hinge part 150 to the lower side of the left eyeglasses 210 and then bend 90 degrees to the left. After extending to the opposite side of the eyeglasses 210, the first lower left contact portion 304 abuts the surface of the left eyeglasses 210.

In addition, the second left lower mounting member 176 is bent 90 degrees after extending from the torsion groove 152 of the hinge part 150 to the lower side of the left eyeglasses 210 while contacting one surface of the left eyeglasses 210. After extending to the opposite side of the left eyeglasses 210, the second lower left contacting portion 306 abuts the surface of the left eyeglasses 210 adjacent to the first left lower contacting portion 304.

The right upper mounting member 192 is formed to face the left upper mounting member 172 and the hinge portion 150 as a center, and the first right lower mounting member 194 is formed with the first left lower mounting member 174. The hinge 150 is formed to face the center, and the second right lower mounting member 196 is formed to face the second left lower mounting member 176 and the hinge 150.

When the user's glasses are large as shown in FIG. 1, the first lower left contact portion 304 and the second left lower contact portion 306 contact the median height of the eyeglasses, and the user's glasses have a medium degree as shown in FIG. 2. In the case of the size, the first lower left contact portion 304 and the second lower left contact portion 306 are in contact with the lower than the median height of the eyeglass ball, the first left when the user's glasses are small as shown in FIG. The lower contact portion 304 and the second left lower contact portion 306 contact the bottom of the eyeglasses.

Through the structure as described above, the present invention has the effect that the user using the glasses can be mounted to the telescope device according to the size of the glasses in use.

The present invention is formed in a structure that can rotate 90 degrees upward when the telescope device is not mounted on the spectacles of the person using the glasses.

That is, the present invention is formed in a substantially cylindrical shape in which the concave groove 135 is formed at a 90-degree interval in the connector 130 formed on the upper portion of the telescope body 110 as shown in FIG. The convex protrusion 155 to be engaged with the concave groove 135 includes a central rod portion 157 formed at an interval of 90 degrees.

If necessary, convex protrusions may be formed in the connector 130 at intervals of 90 degrees, and concave grooves may be formed in the hinge portion 150 at intervals of 90 degrees.

The concave groove 135 and the convex protrusion 155 are stop members formed so that the connector 130 can be stopped at a specific position while being rotated about the hinge 150.

In addition, an outer rod portion 159 having an enlarged diameter is formed at both sides of the central rod portion 157, and the left torsion groove 152a is formed inside the outer rod portion 159. A right torsion groove 152b is formed, a part of the left torsion spring unit 170 is fixed to the left torsion groove 152a, and a part of the right torsion spring unit 190 is fixed to the right torsion groove 152b. .

According to the present invention, when a user who uses glasses uses a telescope, the user can observe a large magnified object using a telescope device as shown in FIG. 5 (a), and when the telescope is not used, the hinge part is not used. The connector 130 may be rotated 90 degrees about 150 to raise the telescope body 110 upward.

Through this, the present invention has the effect that the convenience of use is improved because the person using the glasses do not need to carry the telescope device by hand when necessary while carrying the telescope device separately.

The inside of the telescope body 110 of the present invention receives an object lens unit 112 that receives light from a remote object and a light transmitted from the object lens unit 112 as shown in FIG. Eyepiece portion 122 for delivering to the eye.

The objective lens unit 112 includes a first mirror 114 that first receives the light transmitted from a remote object, a plane mirror 116 that reflects the light transmitted from the first cone mirror 114, and And a second concave mirror 118 that receives the light transmitted from the planar mirror 116 and delivers the light back to the planar mirror 116.

In the planar mirror 116, the portion of the light transmitted from the first concave mirror 114 and the portion of the light reflected from the second concave mirror 118 are different.

The light transmitted from the second concave mirror 118 is transmitted to the eyepiece part 122 via the planar mirror 116.

The eyepiece 122 may include a first one-sided convex lens 124 having a convex portion formed by a user's eye, and a second one-sided convex lens 126 having a convex portion opposed to the first one-sided convex lens 124. And the two one-side voltaic lenses are positioned facing the convex portions of each other.

The light transmitted from the planar mirror 116 transmits light to the user's eyes through the first one side convex lens 124 and the second one side convex lens 126.

On the contrary, in the conventional telescope body 11, as shown in FIG. 6 (b), the objective lens unit 12 has the first concave mirror 14, the second concave mirror 18, and the intermediate lens 19 without the reflection mirror. Include.

Therefore, the second concave mirror 18 should be formed to face the first concave mirror 14, and should have a predetermined distance so as to properly receive and reflect the light reflected from the first concave mirror 14, In order to properly refract the light reflected by the second concave mirror 18 from the intermediate lens 19 to be delivered to the eyepiece 22, a constant separation distance between the intermediate lens 19 and the eyepiece 22 is also provided. Should be placed.

Therefore, the conventional telescope body 11 has a problem that the length of the barrel is long, the present invention omits the intermediate lens 19, the plane between the first concave mirror 114 and the second concave mirror 118 The mirror 116 is formed to reduce the distance between the conventional first concave mirror 14 and the second concave mirror 18 by half to reduce the length of the barrel of the telescope body 110.

Through this, the present invention has a short length of the telescope body 110, even when the telescope body 110 is mounted on the glasses, the glasses are not peeled off well in the future.

FIG. 7 is a schematic orthogonal view showing a structure capable of adjusting the distance between two telescopes formed in the telescope body of the telescope device mounted on the spectacle frame of the present invention, and FIG. 8 is a state in which the distance between the two telescopes is maximized in FIG. 7. It is a schematic orthographic view which shows.

The telescope body 110 of the telescope device 100 mounted on the spectacle frame of the present invention is spaced between the left telescope 110a and the right telescope 110b, and between the left telescope 110a and the right telescope 110b. It includes a spacing control unit 350 is formed to adjust.

One side is fixed to the left telescope unit 110a and the other side is fixed to the left length adjusting member 360, the rack gear is formed at the bottom side, and the other side is fixed to the upper side of the right telescope unit 110b. And a pinion gear 380 formed between the left length adjusting member 370 and the left length adjusting member 360 and the right length adjusting member 370.

The center of the pinion gear 380 is located at the center between the left telescope unit 110a and the right telescope unit 110b, and is extended by a knob (not shown) that can be adjusted by the user.

When the user rotates the knob, the pinion gear 380 is rotated and the distance between the left telescope 110a and the right telescope 110b may be spaced apart as shown in FIG. 8 to the maximum.

According to the present invention, the distance between the left telescope 110a and the right telescope 110b may be adjusted through the spacing controller 350 so that the center of the left telescope 110a may be adjusted to the position of both eyes of the user. The front of the left eye, and the center of the right telescope 110b may be in front of the right eye.

9 is a front view and a plan view showing a state in which the telescope device mounted on the spectacle frame is mounted on the spectacle frame, and FIG. 10 is a side view for explaining a position change of the telescope apparatus in FIG. 9.

The second embodiment of the telescope device 100 mounted on the spectacle frame of the present invention is formed to be mounted on the spectacle frame without the spectacle frame for the user who does not use the spectacle frame.

That is, the second embodiment of the telescope device 100 mounted on the spectacle frame of the present invention is connected to the telescope body 110, the connector 130 formed on the telescope body 110, the connector 130 is connected The hinge portion 150 and the eyeglass frame portion 410 to which the hinge portion 150 is coupled.

The coupling structure between the connector unit 130 and the hinge unit 150 is the same as described with reference to FIGS. 4 and 5, and the connector unit 130 is rotatable 90 degrees about the rotation unit.

In addition, the eyeglass frame 410 has a structure in which the eyeglasses are mounted.

When the user observes a distant object by using the telescope device 100 mounted on the spectacle frame as shown in (a) of FIG. 10, the user moves the telescope body 110 of the telescope device upward as shown in (b) of FIG. 10. Rotate 90 degrees and see with the naked eye.

Through this, the second embodiment of the present invention, when a user who does not use glasses to have a telescope in his hand to observe the telescope if necessary, and if you do not observe the telescope to escape from the hassle of having to hold it again by hand Therefore, the effect can be easily observed with the naked eye or telescope without having to hold it by hand.

As described above, the embodiments of the present invention have been described, and the fact that the present invention can be embodied in other specific forms without departing from the spirit or scope of the present invention can be embodied by those skilled in the art. It is self-evident to. Therefore, the above-described embodiments should be regarded as illustrative rather than restrictive, and thus, the present invention is not limited to the above description and may be modified within the scope of the appended claims and their equivalents.

[Description of the code]

100: telescope device 110: telescope body

112: objective lens portion 122: eyepiece portion

130: connector portion 150: hinge portion

152: torsion groove 157: center rod

170: left torsion spring portion 190: right torsion spring portion

304: first lower left contact portion 306: second left lower contact portion

350: spacing adjuster 380: pinion gear

Claims

With the telescope body,

A connector portion formed on the telescope body,

A hinge portion formed to be connected to the connector portion, and

It includes a spectacle frame formed to be coupled to the hinge,

The connector portion is formed with a stop member so as to rotate around the hinge portion to stop at a specific position,

The telescope body,

An objective lens unit receiving light transmitted from a distant object, and an eyepiece unit receiving light transmitted from the object lens unit and transmitting the light to the user's eyes,

The objective lens unit,

A first concave mirror formed to receive light transmitted from a distant object, a flat mirror formed to reflect light transmitted from the first concave mirror, and light received from the flat mirror to the flat mirror again Telescope device mounted to the frame, characterized in that it comprises a second concave mirror formed to transmit.
The method according to claim 1,

The stop member is a telescope device mounted to the frame, characterized in that the concave groove or convex protrusions.
The method according to claim 1,

And a torsion spring unit which is formed to fix the telescope body by performing a torsion spring action at a plurality of points of the glasses in a state of being fitted in the torsion groove formed at the side end of the hinge portion.
The method according to claim 3,

The telescope body is

Left telescope and right telescope, and

Telescope device mounted to the spectacle frame, characterized in that it comprises a gap adjusting portion formed to adjust the gap between the left telescope and the right telescope using a gear.