Patent Application
20060245050
This application is based upon and claims the benefit of priority from prior Japanese Patent Application No. 2005-115972, filed Apr. 13, 2005, the entire contents of which are incorporated herein by reference.
1. Field of the Invention
The present invention relates to an imaging device.
2. Description of the Related Art
A conventional CCD mounting structure will be described with reference to
The sensor shield is for covering the CCD to shield it from light so that unwanted external light will not enter the CCD. The dustproof member is for causing the space between the cover glass and LPF to be a shielded space where fine dust in air will not enter.
Japanese Patent No. 3034995 discloses a CCD mounting structure. The CCD mounting structure comprises a CCD with an optical receiver covered with a cover glass, a holder on which the CCD is mounted, an LPF which faces the opening of the holder and opposes the optical receiver, and a dustproof light-shielding member which is interposed between the LPF and CCD. The dustproof light-shielding member, which is made of an elastic, opaque material, has an opening which allows external light to pass, an inner bank provided around the opening, an outer bank provided outside the inner bank, and a fitting portion into which a rear end of the LPF is to be fitted. The inner bank is brought into contact with the cover glass, and the outer bank with a package of the CCD. The holder is configured to have a recess to house the LPF and a projecting ridge surrounding it slightly outside the recess and to hold the fitting portion of the dustproof light-shielding member between the projecting ridge and LPF.
The above invention, which is aimed at overall downsizing, weight reduction, and cost reduction, adds a light-shielding function for the CCD to the dustproof member of the CCD to eliminate a light-shielding shield member, and a positioning function for the LPF and dustproof member to decrease the number of assembly steps.
The dustproof light-shielding member has the fitting portion that can fix the LPF, to facilitate positioning of the LPF and dustproof light-shielding member. On that surface of the dustproof light-shielding member which is to come into contact with the CCD, bank-like steps are formed around a lid cover and a package that covers the CCD. This improves the contact to improve the light-shielding properties and dustproof properties.
Japanese Pat. Appln. KOKAI Publication No. 6-85221 discloses a solid-state imaging device using a laminated ceramic package. This solid-state imaging device includes a light-shielding plate which covers a solid-state imager except for a portion above an effective pixel region in order to prevent any unwanted light or bright light from being received by the solid-state imager and suppresses flare of the image. From the viewpoint of improving the productivity, a CERDIP type solid-state imaging device may be possible in which a lead frame is clamped by filling a space between a ceramic base and a lid with an adhesive. However, this apparatus does not include a layer to place the light-shielding plate. Therefore, it is difficult to arrange the light-shielding plate above the solid-state imager accurately.
As a solution to readily arrange the light-shielding plate above the solid-state imager, the light-shielding plate is directly mounted on the base through support pieces. With this structure, the light-shielding plate can be attached highly accurately with reference to the upper surface of the base. Therefore, the gap between the solid-state imager and light-shielding plate can be set accurately. If the light-shielding plate and the support pieces are molded integrally, the light-shielding plate can be attached readily. With this application, the cost can be reduced while maintaining the light-shielding properties. Consequently, the degrees of freedom in selection of the package increase.
According to an aspect of the invention, there is provided an imaging device comprising an imager including an optical receiver, an optical element located on an optical path extending to the optical receiver, a substrate to which the imager is fixed, a casing which covers the imager and the optical element, and a dustproof light-shielding member interposed between the imager and the optical element. The dustproof light-shielding member includes an opening which allows light to pass, and a fitting portion formed like a recess in which the imager is to be fitted. The dustproof light-shielding member is held between the imager and the optical element to form a sealed space, protecting a space between the imager and the optical element against dust.
Advantages of the invention will be set forth in the description which follows, and in part will be obvious from the description, or may be learned by practice of the invention. Advantages of the invention may be realized and obtained by means of the instrumentalities and combinations particularly pointed out hereinafter.
The accompanying drawings, which are incorporated in and constitute a part of the specification, illustrate embodiments of the invention, and together with the general description given above and the detailed description of the embodiments given below, serve to explain the principles of the invention.
The embodiments of the present invention will be described with reference to the accompanying drawing.
As shown in
As shown in
As shown in
For example, the optical element 10 is a low-pass filter which blocks a signal having a wavelength lower than a predetermined frequency and is placed on the dustproof light-shielding member 7. The optical element 10 is so arranged as to oppose the optical receiver 2.
The casing 11 formed like a recess is fixed to the substrate 6 with screws, packaging the CCD 1 fixed to the substrate 6, the dustproof light-shielding member 7 arranged to cover the CCD 1 like a lid, and the optical element 10 arranged to ride on the dustproof light-shielding member 7. The casing 11 has an opening 12 which allows light entering the CCD 1 to pass. The opening 12 has such a size that it does not come into contact with the light ray L.
A width 13a of a recess 13 of the casing 11 is larger than a width 10a of the optical element 10 by 0.5 mm to 1 mm. A width 13b of the recess 13 is larger than a width 10b of the optical element 10 by 0.5 mm to 1 mm. A depth 13c of the recess 13 is slightly smaller than a height 14 from the upper surface of the substrate 6 to the upper surface of the optical element 10.
In this imaging device, light from an object passes through the opening 12, is transmitted through the optical element 10, passes through the opening 9, is transmitted through the cover glass 5, and is focused to form an image on the optical receiver 2. In order to prevent image deterioration caused by diffused reflection or the like, the dustproof light-shielding member 7 effectively shields portions other than the optical receiver 2, such as the lead frames 3 or the bonding wires 4, from light.
In the assembly, the CCD 1 and dustproof light-shielding member 7 are fitted at the fitting portion 8, eliminating the need for position adjustment of the optical receiver 2 and opening 9 after the mounting, which facilitates the assembly. This can prevent the factors of image deterioration, such as diffused reflection or eclipse of the light ray L caused by misalignment. Spacing wide between the widths 10a and 10b of the optical element 10 and the widths 13a and 13b of the recess 13 of the casing 11 further facilitates the assembly.
The optical element 10 is urged by the casing 11, squeezing the dustproof light-shielding member 7 to form a sealed space 19 between the CCD 1 and optical element 10. The dustproof light-shielding member 7 has a sufficient thickness to be squeezed.
The formation of the sealed space 19 protects the space between the CCD 1 and optical element 10 against dust. Thus, any unwanted material such as dust will not enter between the optical element 10 and optical receiver 2. Since no unwanted material is reflected in the image, image deterioration can be prevented.
As shown in
The dustproof light-shielding member 21 has an opening 22 which allows light to pass. The opening 22 has such a size that it does not come into contact with a light ray L having a maximum width of the light that can be received by an optical receiver 2. The dustproof light-shielding member 21 also has a projection 23 projecting toward the CCD 1 and surrounding the opening 22 continuously with adjacent to it. A distal end 23a of the projection 23 has a rounded or angled shape. For example, an optical element 10 is a low-pass filter which blocks a signal having a wavelength lower than a predetermined frequency. The optical element 10 is placed on the projection 23 of the dustproof light-shielding member 21 and so arranged as to oppose the optical receiver 2 of the CCD 1.
A casing 11 is so arranged as to cover the CCD 1 fixed to a substrate 6, the dustproof light-shielding member 21 arranged to cover the CCD 1 like a lid, and the optical element 10 arranged to ride on the dustproof light-shielding member 21, and is fixed to the substrate 6 with screws. The casing 11 has an opening 12 which allows light to pass. The opening 12 is sufficiently larger than the opening 22 of the dustproof light-shielding member 21 and smaller than the outer diameter of the optical element 10.
A width 13a of a recess 13 of the casing 11 is larger than a width 10a of the optical element 10 by 0.5 mm to 1 mm. A width 13b of the recess 13 is larger than a width 10b of the optical element 10 by 0.5 mm to 1 mm. A depth 13c of the recess 13 is slightly smaller than a height 14 from the upper surface of the substrate 6 to the upper surface of the optical element 10.
In this imaging device, light from an object passes through the opening 12, is transmitted through the optical element 10, passes through the opening 22, is transmitted through a cover glass 5, and is focused to form an image on the optical receiver 2. In order to prevent image deterioration caused by diffused reflection or the like, the dustproof light-shielding member 21 effectively shields portions other than the optical receiver 2, such as the lead frames 3 or the bonding wires 4, from light.
In the assembly, the CCD 1 and dustproof light-shielding member 21 are fitted at the fitting portion 8, eliminating the need for position adjustment of the optical receiver 2 and opening 22 after the mounting, which facilitates the assembly. This can prevent the factors of image deterioration, such as diffused reflection or eclipse of the light ray L caused by misalignment. Spacing wide between the widths 10a and 10b of the optical element 10 and the widths 13a and 13b of the recess 13 of the casing 11 further facilitates the assembly.
The optical element 10 is urged by the casing 11, slightly squeezing the projection 23 of the dustproof light-shielding member 21 to form a sealed space 19 between the CCD 1 and optical element 10. The projection 23 supports the optical element 10 with its distal end 23a by line contact. Accordingly, the force required for squeezing the projection 23 may be smaller than the force required for urging it by surface contact. The presence of the projection 23 allows thickness reduction of the other portions, leading to cost reduction.
The formation of the sealed space 19 protects the space between the CCD 1 and optical element 10 against dust. Thus, any unwanted material such as dust will not enter between the optical element 10 and optical receiver 2. Since no unwanted material is reflected in the image, image deterioration can be prevented.
[Modification to Second Embodiment]
As shown in
The dustproof light-shielding member 31 has an opening 32 which allows light to pass. The opening 32 has such a size that it does not come into contact with a light ray L having a maximum width of the light that can be received by an optical receiver 2. The dustproof light-shielding member 31 also has a projection 33 projecting toward the CCD 1 and surrounding the opening 32 continuously. The projection 33 is located outside the opening 32 to be spaced apart from it by several mm. A distal end 33a of the projection 33 has a rounded or angled shape. For example, an optical element 10 is a low-pass filter which blocks a signal having a wavelength lower than a predetermined frequency. The optical element 10 is placed on the projection 33 of the dustproof light-shielding member 31 and so arranged as to oppose the optical receiver 2 of the CCD 1.
A casing 11 is so arranged as to cover the CCD 1 fixed to a substrate 6, the dustproof light-shielding member 31 arranged to cover the CCD 1 like a lid, and the optical element 10 arranged to ride on the dustproof light-shielding member 31, and is fixed to the substrate 6 with screws. The casing 11 has an opening 12 which allows light to pass. The opening 12 is sufficiently larger than the opening 32 of the dustproof light-shielding member 31 and smaller than the outer diameter of the optical element 10.
A width 13a of a recess 13 of the casing 11 is larger than a width 10a of the optical element 10 by 0.5 mm to 1 mm. A width 13b of the recess 13 is larger than a width 10b of the optical element 10 by 0.5 mm to 1 mm. A depth 13c of the recess 13 is slightly smaller than a height 14 from the upper surface of the substrate 6 to the upper surface of the optical element 10.
In this imaging device, light from an object passes through the opening 12, is transmitted through the optical element 10, passes through the opening 22, is transmitted through a cover glass 5, and is focused to form an image on the optical receiver 2. In order to prevent image deterioration caused by diffused reflection or the like, the dustproof light-shielding member 31 effectively shields portions other than the optical receiver 2, such as the lead frames 3 or the bonding wires 4, from light.
In the assembly, the CCD 1 and dustproof light-shielding member 31 are fitted at the fitting portion 8, eliminating the need for position adjustment of the optical receiver 2 and opening 32 after the mounting, which facilitates the assembly. This can prevent the factors of image deterioration, such as diffused reflection or eclipse of the light ray L caused by misalignment. Spacing wide between the widths 10a and 10b of the optical element 10 and the widths 13a and 13b of the recess 13 of the casing 11 further facilitates the assembly.
The optical element 10 is urged by the casing 11, slightly squeezing the projection 33 of the dustproof light-shielding member 31 to form a sealed space 19 between the CCD 1 and optical element 10. The projection 33 supports the optical element 10 with its distal end 33a by line contact. Accordingly, the force required for squeezing the projection 33 may be smaller than the force required for urging it by surface contact. The presence of the projection 33 allows thickness reduction of the other portions, leading to cost reduction.
The projection 33 is formed outside the opening 32 to be spaced apart from it by several mm, allowing the opening area of the opening 32 to be smaller than the area of the opening 22 while maintaining the light ray L. Thus, unnecessary portions other than the optical receiver 2, such as the lead frames 3 or the bonding wires 4, can be shielded from light more reliably.
The formation of the sealed space 19 protects the space between the CCD 1 and optical element 10 against dust. Thus, any unwanted material such as dust will not enter between the optical element 10 and optical receiver 2. Since no unwanted material is reflected in the image, image deterioration can be prevented.
As shown in
The dustproof light-shielding member 41 has an opening 42 which allows light to pass. The opening 42 has such a size that it does not come into contact with a light ray L having a maximum width of the light that can be received by an optical receiver 2. An inner wall 42a of the opening 42 is slanted so as to expand radially from a CCD 1 side toward an optical element 10 side. The dustproof light-shielding member 41 also has a projection 43 projecting toward the CCD 1 and surrounding the opening 42 continuously. The projection 43 is located outside the opening 42 to be spaced apart from it by several mm. A distal end 43a of the projection 43 has a rounded or angled shape. For example, the optical element 10 is a low-pass filter which blocks a signal having a wavelength lower than a predetermined frequency. The optical element 10 is placed on the projection 43 of the dustproof light-shielding member 41 and so arranged as to oppose the optical receiver 2 of the CCD 1.
A casing 44 is so arranged as to cover the CCD 1 fixed to a substrate 6, the dustproof light-shielding member 41 arranged to cover the CCD 1 like a lid, and the optical element 10 arranged to ride on the dustproof light-shielding member 41, and is fixed to the substrate 6 with screws. The casing 44 has an opening 45 which allows light to pass. The opening 45 is sufficiently larger than the opening 42 of the dustproof light-shielding member 41 and smaller than the outer diameter of the optical element 10. An inner wall 45a of the opening 45 is slanted so as to expand from the CCD 1 side toward the optical element 10 side.
A width 13a of a recess 13 of the casing 44 is larger than a width 10a of the optical element 10 by 0.5 mm to 1 mm. A width 13b of the recess 13 is larger than a width 10b of the optical element 10 by 0.5 mm to 1 mm. A depth 13c of the recess 13 is slightly smaller than a height 14 from the upper surface of the substrate 6 to the upper surface of the optical element 10.
In this imaging device, light from an object passes through the opening 45, is transmitted through the optical element 10, passes through the opening 42, is transmitted through a cover glass 5, and is focused to form an image on the optical receiver 2. In order to prevent image deterioration caused by diffused reflection or the like, the dustproof light-shielding member 41 effectively shields portions other than the optical receiver 2, such as the lead frames 3 or the bonding wires 4, from light.
In the assembly, the CCD 1 and dustproof light-shielding member 41 are fitted at the fitting portion 8, eliminating the need for position adjustment of the optical receiver 2 and opening 42 after the mounting, which facilitates the assembly. This can prevent the factors of image deterioration, such as diffused reflection or eclipse of the light ray L caused by misalignment. Spacing wide between the widths 10a and 10b of the optical element 10 and the widths 13a and 13b of the recess 13 of the casing 11 further facilitates the assembly.
The optical element 10 is urged by the casing 44, slightly squeezing the projection 43 of the dustproof light-shielding member 41 to form a sealed space 19 between the CCD 1 and optical element 10. The projection 43 supports the optical element 10 with its distal end 43a by line contact. Accordingly, the force required for squeezing the projection 43 may be smaller than the force required for urging it by surface contact. The presence of the projection 43 allows thickness reduction of the other portions, leading to cost reduction.
The projection 43 is formed outside the opening 42 to be spaced apart from it by several mm, allowing the area of the opening 42 to be smaller than the area of the opening 22 while maintaining the light ray L. Thus, unnecessary portions other than the optical receiver 2, such as the lead frames 3 or the bonding wires 4, can be shielded from light more reliably. The slant inner walls 42a and 45a of the openings 42 and 45 allow further reduction of the opening areas to be smaller than the opening area shown in
The formation of the sealed space 19 protects the space between the CCD 1 and optical element 10 against dust. Thus, any unwanted material such as dust will not enter between the optical element 10 and optical receiver 2. Since no unwanted material is reflected in the image, image deterioration can be prevented.
[Modification to Third Embodiment]
This embodiment is a modification of part of the dustproof light-shielding member 41 of the third embodiment. Hence, this embodiment will be described with reference to
A dustproof light-shielding member 41 formed of an elastic member is mounted on a CCD 1 so as to cover it like a lid. The dustproof light-shielding member 41 has a fitting portion 8 formed like a recess in which the CCD 1 is to be fitted. A fitting length 8a is larger than a length 1a of the side surface of the CCD 1 by approximately 0 mm to 0.2 mm. A fitting length 8b is larger than a length 1b of the side surface of the CCD 1 by approximately 0 mm to 0.2 mm.
The dustproof light-shielding member 41 has an opening 42 which allows light to pass. The opening 42 has such a size that it does not come into contact with a light ray L having a maximum width of the light that can be received by an optical receiver 2. An inner wall 42a of the opening 42 is slanted so as to expand radially from a CCD 1 side toward an optical element 10 side. The dustproof light-shielding member 41 also has a projection 43 projecting toward the CCD 1 and surrounding the opening 42 continuously. The projection 43 is located outside the opening 42 to be spaced apart from it by several mm. A distal end 43a of the projection 43 has a rounded or angled shape. For example, the optical element 10 is a low-pass filter which blocks a signal having a wavelength lower than a predetermined frequency. The optical element 10 is placed on the projection 43 of the dustproof light-shielding member 41 and so arranged as to oppose the optical receiver 2 of the CCD 1.
The surface of that inner wall of the dustproof light-shielding member 41 which is surrounded by the optical element 10, CCD 1, and dustproof light-shielding member 41 is subjected to a surface roughening process with a roughness of 0 to 200.
A casing 44 is so arranged as to cover the CCD 1 fixed to a substrate 6, the dustproof light-shielding member 41 arranged to cover the CCD 1 like a lid, and the optical element 10 arranged to ride on the dustproof light-shielding member 41, and is fixed to the substrate 6 with screws. The casing 44 has an opening 45 which allows light to pass. The opening 45 is sufficiently larger than the opening 42 of the dustproof light-shielding member 41 and smaller than the outer diameter of the optical element 10. An inner wall 45a of the opening 45 is slanted so as to expand from the CCD 1 side toward the optical element 10 side.
A width 13a of a recess 13 of the casing 44 is larger than a width 10a of the optical element 10 by 0.5 mm to 1 mm. A width 13b of the recess 13 is larger than a width 10b of the optical element 10 by 0.5 mm to 1 mm. A depth 13c of the recess 13 is slightly smaller than a height 14 from the upper surface of the substrate 6 to the upper surface of the optical element 10.
In this imaging device, light from an object passes through the opening 45, is transmitted through the optical element 10, passes through the opening 42, is transmitted through a cover glass 5, and is focused to form an image on the optical receiver 2. In order to prevent image deterioration caused by diffused reflection or the like, the dustproof light-shielding member 41 effectively shields portions other than the optical receiver 2, such as the lead frames 3 or the bonding wires 4, from light.
In the assembly, the CCD 1 and dustproof light-shielding member 41 are fitted at the fitting portion 8, eliminating the need for position adjustment of the optical receiver 2 and opening 42 after the mounting, which facilitates the assembly. This can prevent the factors of image deterioration, such as diffused reflection or eclipse of the light ray L caused by misalignment. Spacing wide between the widths 10a and 10b of the optical element 10 and the widths 13a and 13b of the recess 13 of the casing 11 further facilitates the assembly.
The optical element 10 is urged by the casing 44, slightly squeezing the projection 43 of the dustproof light-shielding member 41 to form a sealed space 19 between the CCD 1 and optical element 10. The projection 43 supports the optical element 10 with its distal end 43a by line contact. Accordingly, the force required for squeezing the projection 43 may be smaller than the force required for urging it by surface contact. The presence of the projection 43 allows thickness reduction of the other portions, leading to cost reduction.
The projection 43 is formed outside the opening 42 to be spaced apart from it by several mm, allowing the area of the opening 42 to be smaller than the area of the opening 22 while maintaining the light ray L. Thus, unnecessary portions other than the optical receiver 2, such as the lead frames 3 or the bonding wires 4, can be shielded from light more reliably. The slant inner walls 42a and 45a of the openings 42 and 45 allow further reduction of the opening areas to be smaller than the opening area of the opening 32 shown in
The inner wall 42a of the opening 42 of the dustproof light-shielding member 41, an inner wall 43b of the projection 43 of the dustproof light-shielding member 41, and a portion between the inner walls 42a and 43b are subjected to a surface roughening process, serving as antireflective portions to prevent stray light, diffused reflection, and the like between the optical element 10 and optical receiver 2.
The formation of the sealed space 19 protects the space between the CCD 1 and optical element 10 against dust. Thus, any unwanted material such as dust will not enter between the optical element 10 and optical receiver 2. Since no unwanted material is reflected in the image, image deterioration can be prevented.
As shown in
The dustproof light-shielding member 51 has an opening 42 which allows light to pass. The opening 42 has such a size that it does not come into contact with a light ray L having a maximum width of the light that can be received by an optical receiver 2. An inner wall 42a of the opening 42 is slanted so as to expand radially from a CCD 1 side toward an optical element 10 side. The dustproof light-shielding member 51 also has a projection 52 projecting toward the CCD 1 and surrounding the opening 42 continuously. The projection 52 is located outside the opening 42 to be spaced apart from it by several mm. A distal end 52a of the projection 52 has a rounded or angled shape. The upper surface of the projection 52 is slanted with respect to the light-receiving surface of the optical receiver 2. For example, an optical element 10 is a low-pass filter which blocks a signal having a wavelength lower than a predetermined frequency. The optical element 10 is placed on the projection 52 of the dustproof light-shielding member 51 and so arranged as to oppose the optical receiver 2 of the CCD 1. The inner wall of that portion of the dustproof light-shielding member 51 which is surrounded by the optical element 10, CCD 1, and dustproof light-shielding member 51 is subjected to a surface roughening process with a roughness of 0 to 200.
A casing 53 is so arranged as to cover the CCD 1 fixed to a substrate 6, the dustproof light-shielding member 51 arranged to cover the CCD 1 like a lid, and the optical element 10 supported aslant by the projection 52 of the dustproof light-shielding member 51, and is fixed to the substrate 6 with screws. The casing 53 has an opening 54 which allows light to pass. The opening 54 is sufficiently larger than the opening 42 of the dustproof light-shielding member 51 and smaller than the outer diameter of the optical element 10. An inner wall 54a of the opening 54 is slanted so as to expand from a CCD 1 side toward an optical element 10 side.
A width 13a of a recess 13 of the casing 53 is larger than a width 10a of the optical element 10 by 0.5 mm to 1 mm. A width 13b of the recess 13 is larger than a width 10b of the optical element 10 by 0.5 mm to 1 mm. A depth 13c of the recess 13 is slightly smaller than a height 14 from the upper surface of the substrate 6 to the upper surface of the optical element 10.
A surface 56 of the recess 13 of the casing 53 which urges the optical element 10 is parallel to the slant upper surface of the projection 52.
In this imaging device, light from an object passes through the opening 54, is transmitted through the optical element 10, passes through the opening 42, is transmitted through a cover glass 5, and is focused to form an image on the optical receiver 2. In order to prevent image deterioration caused by diffused reflection or the like, the dustproof light-shielding member 51 effectively shields portions other than the optical receiver 2, such as the lead frames 3 or the bonding wires 4, from light.
In the assembly, the CCD 1 and dustproof light-shielding member 51 are fitted at the fitting portion 8, eliminating the need for position adjustment of the optical receiver 2 and opening 42 after the mounting, which facilitates the assembly. This can prevent the factors of image deterioration, such as diffused reflection or eclipse of the light ray L caused by misalignment. Spacing wide between the widths 10a and 10b of the optical element 10 and the widths 13a and 13b of the recess 13 of the casing 53 further facilitates the assembly.
The optical element 10 is urged by the casing 53, slightly squeezing the projection 52 of the dustproof light-shielding member 51 to form a sealed space 19 between the CCD 1 and optical element 10. The projection 52 supports the optical element 10 with its distal end 52a by line contact. Accordingly, the force required for squeezing the projection 52 may be smaller than the force required for urging it by surface contact. The presence of the projection 52 allows thickness reduction of the other portions, leading to cost reduction.
The projection 52 is formed outside the opening 42 to be spaced apart from it by several mm, allowing the area of the opening 42 to be smaller than the area of the opening 22 of
The inner wall 42a of the opening 42 of the dustproof light-shielding member 41, an inner wall 52b of the projection 52 of the dustproof light-shielding member 41, and a portion between the inner walls 42a and 52b are subjected to a surface roughening process, serving as antireflective portions to prevent stray light, diffused reflection, and the like between the optical element 10 and optical receiver 2.
Light from the object passes through the opening 54 of the casing 53, is transmitted through the optical element 10, passes through the opening 42 of the dustproof light-shielding member 51, is transmitted through the cover glass 5, and reaches the optical receiver 2. At this time, the light passing through the cover glass 5 is partly reflected by the light-receiving surface of the optical receiver 2, and passes through the cover glass 5 again to reach the optical element 10. Part of the light reaching the optical element 10 is reflected by the optical element 10 and reaches the optical receiver 2 again. This repetitive reflection at the same position is called spot flare that considerably degrades the image. The optical element 10 is mounted aslant with respect to the optical receiver 2, reflecting the light to be reflected by the optical element 10 aslant with respect to the light-receiving surface of the optical receiver 2, which prevents repetitive reflection at the same position, so that the light eventually goes outside the visual field and hits the inner wall of the casing 53 or the like to disappear. Accordingly, spot flare can be decreased.
The formation of the sealed space 19 protects the space between the CCD 1 and optical element 10 against dust. Thus, any unwanted material such as dust will not enter between the optical element 10 and optical receiver 2. Since no unwanted material is reflected in the image, image deterioration can be prevented.
As shown in
A dustproof light-shielding member 63 formed of an elastic member is mounted on the CCD 1 so as to cover it like a lid. As shown in
The dustproof light-shielding member 63 has an opening 42 which allows light to pass. The opening 42 has such a size that it does not come into contact with a light ray L having a maximum width of the light that can be received by an optical receiver 2. An inner wall 42a of the opening 42 is slanted so as to expand radially from a CCD 1 side toward an optical element 10 side. The dustproof light-shielding member 63 also has a projection 52 projecting toward the CCD 1 and surrounding the opening 42 continuously. The projection 52 is located outside the opening 42 to be spaced apart from it by several mm. A distal end 52a of the projection 52 has a rounded or angled shape. The upper surface of the projection 52 is slanted with respect to the light-receiving surface of the optical receiver 2. For example, an optical element 10 is a low-pass filter which blocks a signal having a wavelength lower than a predetermined frequency. The optical element 10 is placed on the projection 52 of the dustproof light-shielding member 63 and so arranged as to oppose the optical receiver 2 of the CCD 1. The inner wall of that portion of the dustproof light-shielding member 63 which is surrounded by the optical element 10, CCD 1, and dustproof light-shielding member 63 is subjected to a surface roughening process with a roughness of 0 to 200.
A casing 53 is so arranged as to cover the CCD 1 fixed to a substrate 6, the dustproof light-shielding member 63 arranged to cover the CCD 1 like a lid, and the optical element 10 supported aslant by the projection 52 of the dustproof light-shielding member 63, and is fixed to the substrate 6 with screws. The casing 53 has an opening 54 which allows light to pass. The opening 54 is sufficiently larger than the opening 42 of the dustproof light-shielding member 63 and smaller than the outer diameter of the optical element 10. An inner wall 54a of the opening 54 is slanted so as to expand from a CCD 1 side toward an optical element 10 side.
A width 13a of a recess 13 of the casing 53 is larger than a width 10a of the optical element 10 by 0.5 mm to 1 mm. A width 13b of the recess 13 is larger than a width 10b of the optical element 10 by 0.5 mm to 1 mm. A depth 13c of the recess 13 is slightly smaller than a height 14 from the upper surface of the substrate 6 to the upper surface of the optical element 10.
A surface 56 of the recess 13 of the casing 53 which urges the optical element 10 is parallel to the slant upper surface of the projection 52.
In this imaging device, light from an object passes through the opening 54, is transmitted through the optical element 10, passes through the opening 42, is transmitted through a cover glass 5, and is focused to form an image on the optical receiver 2. In order to prevent image deterioration caused by diffused reflection or the like, the dustproof light-shielding member 63 effectively shields portions other than the optical receiver 2, such as the lead frames 3 or the bonding wires 4, from light.
In the assembly, the CCD 1 and dustproof light-shielding member 63 are fitted at the fitting portion 8, eliminating the need for position adjustment of the optical receiver 2 and opening 42 after the mounting, which facilitates the assembly. This can prevent the factors of image deterioration, such as diffused reflection or eclipse of the light ray L caused by misalignment. Spacing wide between the widths 10a and 10b of the optical element 10 and the widths 13a and 13b of the recess 13 of the casing 53 further facilitates the assembly.
The optical element 10 is urged by the casing 53, slightly squeezing the projection 52 of the dustproof light-shielding member 63 to form a sealed space 19 between the CCD 1 and optical element 10. The projection 52 supports the optical element 10 with its distal end 52a by line contact. Accordingly, the force required for squeezing the projection 52 may be smaller than the force required for urging it by surface contact. The presence of the projection 52 allows thickness reduction of the other portions, leading to cost reduction.
The projection 52 is formed outside the opening 42 to be spaced apart from it by several mm, allowing the area of the opening 42 to be smaller than the area of the opening 22 of
The inner wall 42a of the opening 42 of the dustproof light-shielding member 63, an inner wall 52b of the projection 52 of the dustproof light-shielding member 63, and a portion between the inner walls 42a and 52b are subjected to a surface roughening process, serving as antireflective portions to prevent stray light, diffused reflection, and the like between the optical element 10 and optical receiver 2.
Light from the object passes through the opening 54 of the casing 53, is transmitted through the optical element 10, passes through the opening 42 of the dustproof light-shielding member 63, is transmitted through the cover glass 5, and reaches the optical receiver 2. At this time, the light passing through the cover glass 5 is partly reflected by the light-receiving surface of the optical receiver 2, and passes through the cover glass 5 again to reach the optical element 10. Part of the light reaching the optical element 10 is reflected by the optical element 10 and reaches the optical receiver 2 again. This repetitive reflection at the same position is called spot flare that considerably degrades the image. The optical element 10 is mounted aslant with respect to the optical receiver 2, reflecting the light to be reflected by the optical element 10 aslant with respect to the light-receiving surface of the optical receiver 2, which prevents repetitive reflection at the same position, so that the light eventually goes outside the visual field and hits the inner wall of the casing 53 or the like to disappear. Accordingly, spot flare can be decreased.
The formation of the sealed space 19 protects the space between the CCD 1 and optical element 10 against dust. Thus, any unwanted material such as dust will not enter between the optical element 10 and optical receiver 2. Since no unwanted material is reflected in the image, image deterioration can be prevented.
The heat dissipation plate 61 has larger thermal conductivity than the optical element 10. Heat generated by the CCD 1 is conducted from the bottom surface of the CCD 1 to the heat dissipation plate 61 and dissipated. Heat generated in the upper and side surfaces of the CCD 1 is conducted from the dustproof light-shielding member 63 in tight contact with the side and upper surfaces of the CCD 1, to the heat dissipation plate 61 and dissipated. Hence, the CCD 1 can be cooled efficiently. As a result, thermal noise can be decreased.
As shown in
A dustproof light-shielding member 75 made of a heat-insulating material is mounted on the CCD 1 so as to cover it like a lid. As the heat-insulating material, for example, polypropylene is employed. As shown in
The dustproof light-shielding member 75 has an opening 42 which allows light to pass. The opening 42 has such a size that it does not come into contact with a light ray L having a maximum width of the light that can be received by an optical receiver 2. An inner wall 42a of the opening 42 is slanted so as to expand radially from a CCD 1 side toward an optical element 10 side. The dustproof light-shielding member 75 also has a projection 52 projecting toward the CCD 1 and surrounding the opening 42 continuously. The projection 52 is located outside the opening 42 to be spaced apart from it by several mm. A distal end 52a of the projection 52 has a rounded or angled shape. The upper surface of the projection 52 is slanted with respect to the light-receiving surface of the optical receiver 2. For example, an optical element 10 is a low-pass filter which blocks a signal having a wavelength lower than a predetermined frequency. The optical element 10 is placed on the projection 52 of the dustproof light-shielding member 75 and so arranged as to oppose the optical receiver 2 of the CCD 1. The inner wall of that portion of the dustproof light-shielding member 75 which is surrounded by the optical element 10, CCD 1, and dustproof light-shielding member 75 is subjected to a surface roughening process with a roughness of 0 to 200.
A casing 53 is so arranged as to cover the CCD 1 fixed to the substrate 71, the dustproof light-shielding member 75 arranged to cover the CCD 1 like a lid, and the optical element 10 supported aslant by the projection 52 of the dustproof light-shielding member 75, and is fixed to the substrate 71 with screws. The casing 53 has an opening 54 which allows light to pass. The opening 54 is sufficiently larger than the opening 42 of the dustproof light-shielding member 75 and smaller than the outer diameter of the optical element 10. An inner wall 54a of the opening 54 is slanted so as to expand from a CCD 1 side toward an optical element 10 side.
A width 13a of a recess 13 of the casing 53 is larger than a width 10a of the optical element 10 by 0.5 mm to 1 mm. A width 13b of the recess 13 is larger than a width 10b of the optical element 10 by 0.5 mm to 1 mm. A depth 13c of the recess 13 is slightly smaller than a height 14 from the upper surface of the substrate 6 to the upper surface of the optical element 10.
A surface 56 of the recess 13 of the casing 53 which urges the optical element 10 is parallel to the slant upper surface of the projection 52.
In this imaging device, light from an object passes through the opening 54, is transmitted through the optical element 10, passes through the opening 42, is transmitted through a cover glass 5, and is focused to form an image on the optical receiver 2. In order to prevent image deterioration caused by diffused reflection or the like, the dustproof light-shielding member 75 effectively shields portions other than the optical receiver 2, such as the lead frames 3 or the bonding wires 4, from light.
In the assembly, the CCD 1 and dustproof light-shielding member 75 are fitted at the fitting portion 8, eliminating the need for position adjustment of the optical receiver 2 and opening 42 after the mounting, which facilitates the assembly. This can prevent the factors of image deterioration, such as diffused reflection or eclipse of the light ray L caused by misalignment. Spacing wide between the widths 10a and 10b of the optical element 10 and the widths 13a and 13b of the recess 13 of the casing 53 further facilitates the assembly.
The optical element 10 is urged by the casing 53, slightly squeezing the projection 52 of the dustproof light-shielding member 75 to form a sealed space 19 between the CCD 1 and optical element 10. The projection 52 supports the optical element 10 with its distal end 52a by line contact. Accordingly, the force required for squeezing the projection 52 may be smaller than the force required for urging it by surface contact. The presence of the projection 52 allows thickness reduction of the other portions, leading to cost reduction.
The projection 52 is formed outside the opening 42 to be spaced apart from it by several mm, allowing the area of the opening 42 to be smaller than the area of the opening 22 of
The inner wall 42a of the opening 42 of the dustproof light-shielding member 75, an inner wall 52b of the projection 52 of the dustproof light-shielding member 75, and a portion between the inner walls 42a and 52b are subjected to a surface roughening process, serving as antireflective portions to prevent stray light, diffused reflection, and the like between the optical element 10 and optical receiver 2.
Light from the object passes through the opening 54 of the casing 53, is transmitted through the optical element 10, passes through the opening 42 of the dustproof light-shielding member 75, is transmitted through the cover glass 5, and reaches the optical receiver 2. At this time, the light passing through the cover glass 5 is partly reflected by the light-receiving surface of the optical receiver 2, and passes through the cover glass 5 again to reach the optical element 10. Part of the light reaching the optical element 10 is reflected by the optical element 10 and reaches the optical receiver 2 again. This repetitive reflection at the same position is called spot flare that considerably degrades the image. The optical element 10 is mounted aslant with respect to the optical receiver 2, reflecting the light to be reflected by the optical element 10 aslant with respect to the light-receiving surface of the optical receiver 2, which prevents repetitive reflection at the same position, so that the light eventually goes outside the visual field and hits the inner wall of the casing 53 or the like to disappear. Accordingly, spot flare can be decreased.
The formation of the sealed space 19 protects the space between the CCD 1 and optical element 10 against dust. Thus, any unwanted material such as dust will not enter between the optical element 10 and optical receiver 2. Since no unwanted material is reflected in the image, image deterioration can be prevented.
The Peltier element 74 cools the CCD 1 through the cooling plate 73. The dustproof light-shielding member 75 made of the heat-insulating material seals the CCD 1. Thus, external heat will not readily flow into the CCD 1, and the CCD 1 can be cooled efficiently. As a result, thermal noise can be decreased. Also, the imaging device can be formed compact at a low cost in comparison to an imaging device to which a fan, a fin, or the like is provided for cooling.
So far the embodiments of the present invention have been described with reference to the accompanying drawing. However, the present invention is not limited to these embodiments, and various changes and modifications may be made without departing from the spirit of the invention.
Additional advantages and modifications will readily occur to those skilled in the art. Therefore, the invention in its broader aspects is not limited to the specific details and representative embodiments shown and described herein. Accordingly, various modifications may be made without departing from the spirit or scope of the general inventive concept as defined by the appended claims and their equivalents.
| Number | Date | Country | Kind |
|---|---|---|---|
| 2005-115972 | Apr 2005 | JP | national |
