JPS6132655B2 - - Google Patents
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- Publication number
- JPS6132655B2 JPS6132655B2 JP56157009A JP15700981A JPS6132655B2 JP S6132655 B2 JPS6132655 B2 JP S6132655B2 JP 56157009 A JP56157009 A JP 56157009A JP 15700981 A JP15700981 A JP 15700981A JP S6132655 B2 JPS6132655 B2 JP S6132655B2
- Authority
- JP
- Japan
- Prior art keywords
- lens
- positive
- negative
- lenses
- focal length
- Prior art date
- Legal status (The legal status is an assumption and is not a legal conclusion. Google has not performed a legal analysis and makes no representation as to the accuracy of the status listed.)
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Classifications
-
- G—PHYSICS
- G02—OPTICS
- G02B—OPTICAL ELEMENTS, SYSTEMS OR APPARATUS
- G02B13/00—Optical objectives specially designed for the purposes specified below
- G02B13/18—Optical objectives specially designed for the purposes specified below with lenses having one or more non-spherical faces, e.g. for reducing geometrical aberration
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- Physics & Mathematics (AREA)
- General Physics & Mathematics (AREA)
- Optics & Photonics (AREA)
- Lenses (AREA)
Description
本発明は、画角が75゜程度でFナンバーは
F1.4と明るく、かつ極めて性能の優秀なるコン
パクトな広角写真レンズを提供せんとするもので
ある。
従来より、画角75゜程度の一眼レフカメラ用広
角写真レンズについては、主にレトロフオーカス
タイプで多くのものが公知となつているが、Fナ
ンバーがF1.4という大口径比のものは極めて例
が少ない。その理由は、大口径比に伴つて、単に
球面収差を補正するのみならず、十分な周辺光量
の確保、並びに増大するコマフレアーの補正など
数多くの問題を解決しつつ、コンパクトにレンズ
系をまとめるということが極めて難しいという点
にある。
特にコマフレアーは、画像のコントラストを低
下させるだけではなく、夜景撮影等で点光源ある
いはそれに近い光源を撮影した場合、著しく画質
を損なうなどの欠点をもたらす為、十分補正され
るべきものであるが、従来の例では満足すべきも
のは無かつた。
本発明は以上の点に着目し、非球面レンズを導
入することによつて、前記コマフレアーを十分に
補正し、なおかつ周辺光量を十分に確保した上で
残る諸収差をも良好に除き、大口径にして極めて
性能良好なる広角写真レンズを達成し得たもので
ある。
以下、本発明について詳述する。
本発明は、物体側より順に、正レンズの第1レ
ンズ、共に負メニスカスレンズである第2レンズ
と第3レンズ、及び正メニスカスレンズの第4レ
ンズの4枚構成で全体として負の屈折力を有する
第1群と、共に正レンズである第5レンズと第6
レンズ、負レンズの第7レンズ、負レンズの第8
レンズと正レンズの第9レンズとの貼合せレン
ズ、及び正レンズの第10レンズの6枚構成で全体
として正の屈折力を有する第2群とから成り、両
群が絞りをはさんで配置されるレンズ系であつ
て、前記第9レンズまたは第10レンズの内、何れ
か一方のレンズの像側の面を非球面とし、該非球
面の頂点(極)を原点として光軸方向にy軸、光
軸と垂直方向にx軸をとつて非球面の方程式を一
般的にy=f(x)とおいたとき、f(x)の2
次導関数
f″(x)=d2y/dx2
の符号が有効径内の端付近において負から正へ変
化する場所が一ケ所存在することを特徴とする大
口径比で性能の極めて良好な広角写真レンズであ
る。
非球面レンズを導入する目的としては、球面収
差の補正、歪曲収差の補正、コマ収差の補正等が
考えられる。一般に、レトロフオーカス型レンズ
においては、負屈折力を持つ前群で負の歪曲収差
が大きく発生し、この負の歪曲収差は全系のコン
パクト化をおしすすめると更に悪化する傾向にあ
る。そこで、従来の非球面レンズ使用の例では、
この歪曲収差の補正を主目的にしたものが多く見
受けられる。
これに対し、本発明においては、まず第1レン
ズを正レンズとすることによつて歪曲収差を補正
し、さらに第2群を対称的な構造とすることによ
り歪曲収差の発生を極力抑えるなど、根本的に歪
曲収差の残りにくい光学系を構成している。また
第2、第3レンズを共に負メニスカスレンズとし
て、入射光束に対してコンセントリツクな構造を
与えて、諸収差の発生を抑えながら十分な負の屈
折力を持たせ、さらに第4レンズを正メニスカス
レンズとして球面収差、色収差の補正を図り、第
1群全体として強い負屈折力を持ちながら諸収差
の発生しにくい構造をとつている。
また第2群では、第5レンズ、第6レンズと2
枚の正レンズを配して強い正の屈折力を与え、第
7レンズは負レンズとして球面収差ならびに非点
収差の補正を図つている。負レンズの第8レンズ
と正レンズの第9レンズは貼合せレンズとして非
点収差、像面彎曲、色収差を補正し、最後に正レ
ンズの第10レンズを配して球面収差、コマ収差の
補正を図つている。また前述したごとく第2群全
体を対称的な構造として歪曲収差の発生を抑えて
いる。
以上のように、第1、第2各群共に諸収差の発
生を極力抑えながら強い屈折力を与え得る構造と
して、コンパクトにして性能の高い光学系の下地
を作つた上で、本発明の一つの特徴は第9レンズ
または第10レンズの内の何れか一方のレンズの像
側の面を非球面とする点にある。
本発明における非球面使用の一つの大きな目的
は、大口径比の広角レンズで特に大きく発生する
コマフレアーを補正することである。前述のごと
く、基本的に諸収差のの発生しにくい光学系構造
を採つているので、コマフレアーを抑える為に非
球面を非常に効果的に用いることができる。
非球面は、一般に製作が難しく、コストも高く
なるので、少ない面数で効果的に用いるのが望ま
しい。本発明においては、像側から数えて第1番
目または第2番目の正レンズであるところの第9
レンズまたは第10レンズの像側の面に非球面を用
いることが、コマフレアーの除去に対して最も効
果的であることを見出した。
また非球面の頂点(極)を原点として光軸方向
にy軸、光軸と垂直方向にx軸をとつて非球面の
方程式を一般的にy=f(x)とおいたとき、f
(x)の2次関数
f″(x)=d2y/dx2
の符号が実施例1、2のx、f(x)、f″(x)
の表の中で数値を開示したごとく有効径内の端付
近において負から正へ変化する場所が一ケ所存在
するという条件は、非球面の形状に関するもので
ある。これは言い換えれば、非球面曲線が有効径
内において変曲点を持つということであるが、こ
のような非球面形状を用いると、コマフレアーの
除去に極めて効果的であるということに加え、レ
ンズ系を構成する非球面以外の他の要素との収差
補正の負担の分担を適切に行うことができる。
以上のような構成によつて大口径比にして極め
て性能の良好な広角写真レンズが達成できるが、
本発明は更に条件を付与することにより、より一
層コンパクトにして性能の優秀なる大口径比写真
レンズが実現される。即ち
(1) 1.2f<|f123|<2.0f、f123<0
(2) 0.4f<D6<0.9f
(3) 1.0f<f<1.6f
(4) 2f<L<3f
(5) 5f<f1<12f
(6) NP>1.7
ここでf123は第1レンズから第3レンズまでの合
成焦点距離、fは全系の焦点距離、D6は第3レ
ンズと第4レンズとの空気間隔、fは第2群の
焦点距離、Lはレンズ全長、f1は第1レンズの焦
点距離、NPは第5レンズと第6レンズの屈折率
の平均値である。
を満足することである。
条件(1)から(4)までは、一眼レフカメラ用レンズ
としてカメラボデー内のミラーと機械的に干渉し
ない様に必要なバツクフオーカスを確保すると共
に、レンズ全系をコンパクトに保ちかつ高い性能
を維持する為の条件である。
まず条件(1)は第1レンズから第3レンズまでの
レンズ群の屈折力に関する。条件(1)の下限を超え
ると、屈折力は増し、コンパクト化に対しては有
利となるが、負の球面収差、コマ収差、歪曲収差
等の諸収差が大きく発生し、もはや良好な性能を
維持することが困難となる。また条件(1)の上限を
超えると、屈折力が減り、収差補正の面では有利
となるが、全長の増大を招きコンパクト化の意図
に反する。
条件(2)は第3レンズ及び第4レンズ間の空気間
隔に関する。条件(2)の下限を超えると、該空気間
隔は短くなり過ぎ、必要なバツクフオーカスの確
保が困難となる。また条件(2)の上限を超えると、
第1レンズから第3レンズ群までのレンズ群で発
生した負の球面収差、色収差等を第4レンズにて
補正することが困難となる。
条件(3)は第2群の屈折力に関する。第2群は第
1群で発散した光束を収束させる役割を持ち、か
つ大口径比の光束が通過するので、諸収差の発生
を抑えつつ全系のコンパクト化を図る為には、そ
の屈折力の決定がポイントとなる。条件(3)の下限
を超えると、第2群の屈折力が大きくなり過ぎ
て、正の球面収差、像面彎曲、色収差が発生し、
良好な性能の維持が難しくなる。また条件(3)の上
限を超えると、第2群の屈折力がゆるくなり過
ぎ、収差補正の面では有利であるが、コンパクト
性が達成されない。
条件(4)はレンズ全長に関する。条件(4)の下限を
超えると、各レンズ群の屈折力が強くなり、諸収
差が発生し良好な収差補正が得られない。また条
件(4)の上限を超えると、必要な周辺光量の確保の
為に前玉径を大きくする必要を生じ、コンパクト
化の意図に反する。
条件(5)は第1レンズの屈折力に関する。条件(5)
の上限を超えると、第1レンズの屈折力が減つ
て、負の歪曲収差を補正する役割がなくなり、第
2レンズ群に補正の負担が加わり、ひいては非球
面部にも負担が及び、良好な収差補正が困難とな
る。また条件(5)の下限を超えると、第1レンズの
屈折力が強くなり過ぎるが、第1群は全体として
負の屈折力を有するので、正の屈折力を有する第
1レンズが強くなり過ぎると、負レンズであると
ころの第2、第3レンズの屈折力も相応に強くな
らざるを得ず、収差補正の面で不利となる。
条件(6)は第5レンズ及び第6レンズの屈折率に
関する。この条件は第2群において悪化しがちな
球面収差を補正し、かつペツツバール和を改善し
て像面彎曲、非点収差を除く為に必要な条件であ
る。
以下、本発明の実施例のデータを記載する。こ
こでfは焦点距離、Rはレンズの曲率半径、Dは
レンズ厚またはレンズ間隔、Nは屈折率、νはア
ツベ数である。
実施例 1
The present invention has an angle of view of about 75 degrees and an F number of
The objective is to provide a compact wide-angle photographic lens that is bright at F1.4 and has extremely excellent performance. Conventionally, many wide-angle photographic lenses for single-lens reflex cameras with an angle of view of about 75° have been known, mainly retrofocus types, but those with a large aperture ratio with an F number of F1.4 have been known. There are extremely few examples. The reason for this is that with a large aperture ratio, it is not only necessary to correct spherical aberration, but also to solve a number of problems such as securing sufficient peripheral illumination and correcting the increasing coma flare, while also making the lens system compact. The point is that it is extremely difficult. In particular, coma flare not only reduces the contrast of the image, but also causes drawbacks such as a significant loss of image quality when shooting a point light source or a light source close to it, such as when shooting night scenes, so it should be adequately corrected. , the conventional examples were not satisfactory. The present invention has focused on the above points, and by introducing an aspherical lens, the coma flare can be sufficiently corrected, and even after securing a sufficient amount of peripheral light, remaining various aberrations can be favorably removed, and a large amount can be achieved. We have achieved a wide-angle photographic lens with extremely good performance considering its aperture. The present invention will be explained in detail below. The present invention has a four-lens configuration in which, in order from the object side, the first lens is a positive lens, the second and third lenses are both negative meniscus lenses, and the fourth lens is a positive meniscus lens, and has a negative refractive power as a whole. a fifth lens and a sixth lens, both of which are positive lenses.
lens, negative lens 7th lens, negative lens 8th lens
Consists of a second group that has positive refractive power as a whole and consists of six elements: a bonded lens with a positive 9th lens, and a positive 10th lens, and both groups are arranged with an aperture in between. A lens system in which the image side surface of either the ninth lens or the tenth lens is an aspherical surface, and the y-axis is aligned in the optical axis direction with the apex (pole) of the aspherical surface as the origin. , when the x-axis is taken perpendicular to the optical axis and the equation of an aspherical surface is generally set as y=f(x), then 2 of f(x)
Extremely good performance with a large aperture ratio characterized by the fact that there is one place where the sign of the order derivative f″(x)=d 2 y/dx 2 changes from negative to positive near the end of the effective diameter. It is a wide-angle photographic lens. Possible purposes for introducing an aspherical lens include correction of spherical aberration, correction of distortion aberration, correction of coma aberration, etc. In general, retrofocus lenses have negative refractive power. A large amount of negative distortion occurs in the front group, and this negative distortion tends to worsen as the entire system is made more compact.Therefore, in the conventional example of using an aspherical lens,
There are many devices whose main purpose is to correct this distortion aberration. In contrast, in the present invention, distortion is corrected by first making the first lens a positive lens, and furthermore, by making the second lens group symmetrical, the occurrence of distortion is suppressed as much as possible. The optical system is fundamentally resistant to residual distortion. In addition, the second and third lenses are both negative meniscus lenses, giving a concentric structure to the incident light beam, suppressing the occurrence of various aberrations, and providing sufficient negative refractive power. As a meniscus lens, spherical aberration and chromatic aberration are corrected, and the first group as a whole has a strong negative refractive power, yet has a structure that makes it difficult for various aberrations to occur. In addition, in the second group, the fifth lens, the sixth lens and the second
Two positive lenses are arranged to provide strong positive refractive power, and the seventh lens is used as a negative lens to correct spherical aberration and astigmatism. The 8th negative lens and the 9th positive lens are used as a bonded lens to correct astigmatism, field curvature, and chromatic aberration, and finally the 10th positive lens is placed to correct spherical aberration and coma aberration. We are trying to Furthermore, as described above, the entire second group has a symmetrical structure to suppress the occurrence of distortion. As described above, the first and second groups have a structure that can provide strong refractive power while minimizing the occurrence of various aberrations, and have created the basis for a compact and high-performance optical system. One feature is that the image side surface of either the ninth lens or the tenth lens is an aspherical surface. One of the major purposes of using an aspherical surface in the present invention is to correct coma flare, which occurs particularly large in wide-angle lenses with large aperture ratios. As mentioned above, since the optical system structure is basically such that various aberrations are difficult to occur, aspheric surfaces can be used very effectively to suppress coma flare. Since aspherical surfaces are generally difficult to manufacture and expensive, it is desirable to use them effectively with a small number of surfaces. In the present invention, the ninth positive lens is the first or second positive lens counting from the image side.
It has been found that using an aspheric surface on the image side surface of the lens or the tenth lens is most effective in removing coma flare. In addition, when the apex (pole) of the aspheric surface is the origin, the y axis is in the optical axis direction, and the x axis is perpendicular to the optical axis, and the equation of the aspheric surface is generally y = f (x), f
The quadratic function of (x) f″(x)=d 2 y/dx The sign of 2 is x, f(x), f″(x) in Examples 1 and 2
The condition that there is one place near the end of the effective diameter where the value changes from negative to positive, as disclosed in the table above, is related to the shape of the aspheric surface. In other words, the aspherical curve has an inflection point within the effective diameter, but using such an aspherical shape is extremely effective in eliminating coma flare, as well as The burden of aberration correction can be appropriately shared with other elements other than the aspherical surface constituting the system. With the above configuration, it is possible to achieve a wide-angle photographic lens with extremely good performance at a large aperture ratio.
By further adding conditions to the present invention, it is possible to realize a large aperture ratio photographic lens that is even more compact and has excellent performance. That is, (1) 1.2f<|f 123 |<2.0f, f 123 <0 (2) 0.4f<D 6 <0.9f (3) 1.0f<f<1.6f (4) 2f<L<3f (5) ) 5f<f 1 <12f (6) N P >1.7 Here, f 123 is the composite focal length from the first lens to the third lens, f is the focal length of the entire system, and D 6 is the third and fourth lenses. f is the focal length of the second group, L is the total length of the lens, f 1 is the focal length of the first lens, and N P is the average value of the refractive index of the fifth lens and the sixth lens. It is to satisfy the following. Conditions (1) to (4) are to ensure the necessary back focus to avoid mechanical interference with the mirror inside the camera body as a lens for single-lens reflex cameras, and to keep the entire lens system compact and maintain high performance. This is a condition for doing so. First, condition (1) relates to the refractive power of the lens group from the first lens to the third lens. If the lower limit of condition (1) is exceeded, the refractive power will increase and it will be advantageous for compactness, but various aberrations such as negative spherical aberration, coma aberration, and distortion will occur, making it no longer possible to achieve good performance. It becomes difficult to maintain. If the upper limit of condition (1) is exceeded, the refractive power decreases, which is advantageous in terms of aberration correction, but increases the overall length, which goes against the intention of compactness. Condition (2) relates to the air gap between the third lens and the fourth lens. If the lower limit of condition (2) is exceeded, the air interval becomes too short and it becomes difficult to secure the necessary back focus. Also, if the upper limit of condition (2) is exceeded,
It becomes difficult for the fourth lens to correct negative spherical aberration, chromatic aberration, etc. generated in the lens groups from the first lens to the third lens group. Condition (3) relates to the refractive power of the second group. The second group has the role of converging the light beam diverged by the first group, and the light beam with a large aperture ratio passes through it, so in order to minimize the occurrence of various aberrations and make the entire system compact, its refractive power is required. The key point is to decide. If the lower limit of condition (3) is exceeded, the refractive power of the second group becomes too large, causing positive spherical aberration, curvature of field, and chromatic aberration.
Maintaining good performance becomes difficult. If the upper limit of condition (3) is exceeded, the refractive power of the second group becomes too loose, which is advantageous in terms of aberration correction, but compactness cannot be achieved. Condition (4) relates to the total length of the lens. If the lower limit of condition (4) is exceeded, the refractive power of each lens group becomes strong, various aberrations occur, and good aberration correction cannot be obtained. Moreover, if the upper limit of condition (4) is exceeded, it becomes necessary to increase the diameter of the front lens in order to secure the necessary amount of peripheral light, which goes against the intention of compactness. Condition (5) relates to the refractive power of the first lens. Condition (5)
If the upper limit of It becomes difficult to correct aberrations. If the lower limit of condition (5) is exceeded, the refractive power of the first lens becomes too strong, but since the first group as a whole has negative refractive power, the first lens, which has positive refractive power, becomes too strong. In this case, the refractive power of the second and third lenses, which are negative lenses, must also be correspondingly strong, which is disadvantageous in terms of aberration correction. Condition (6) relates to the refractive index of the fifth lens and the sixth lens. This condition is necessary to correct spherical aberration, which tends to worsen in the second group, and to improve Petzval's sum to eliminate field curvature and astigmatism. Below, data of examples of the present invention will be described. Here, f is the focal length, R is the radius of curvature of the lens, D is the lens thickness or distance between the lenses, N is the refractive index, and ν is the Abbe number. Example 1
【表】【table】
【表】 実施例 2【table】 Example 2
【表】【table】
第1図、第3図は各々実施例1、2のレンズ
図、第2図、第4図は各々実施例1、2の収差
図、第5図、第6図は各々実施例1、2のコマ収
差図である。
Figures 1 and 3 are lens diagrams of Examples 1 and 2, respectively, Figures 2 and 4 are aberration diagrams of Examples 1 and 2, respectively, and Figures 5 and 6 are lens diagrams of Examples 1 and 2, respectively. FIG.
Claims (1)
に負メニスカスレンズである第2レンズと第3レ
ンズ、及び正メニスカスレンズの第4レンズの4
枚構成で、全体として負の屈折力を有する第1群
と、共に正レンズである第5レンズと第6レン
ズ、負レンズの第7レンズ、負レンズの第8レン
ズと正レンズの第9レンズとの貼合せレンズ、及
び正レンズの第10レンズの6枚構成で、全体とし
て正の屈折力を有する第2群とから成り、両群が
絞りをはさんで配置されるレンズ系であつて、前
記第9レンズまたは第10レンズの内、何れか一方
のレンズの像側の面を非球面とし、該非球面の頂
点(極)を頂点として光軸方向にy軸、光軸と垂
直方向にx軸をとつて非球面の方程式を一般的に
y=f(x)とおいたとき、f(x)の2次導関
数f″(x)=d2y/dx2の符号が有効径内の端付
近におい て負から正へ変化する場所が一ケ所存在すること
を特徴とし、かつ次の諸条件を満足して構成した
ことを特徴とする非球面を用いた大口径比広角写
真レンズ。 (1) 1.2f<|f123|<2.0f、f123<0 (2) 0.4f<D6<0.9f (3) 1.0f<f<1.6f (4) 2f<L<3f (5) 5f<f1<12f (6) NP>1.7 ここで、f123は第1レンズから第3レンズまで
の合成焦点距離、fは全系の焦点距離、D6は第
3レンズと第4レンズとの空気間隔、fは第2
群の焦点距離、Lはレンズ全長、f1は第1レンズ
の焦点距離、NPは第5レンズと第6レンズの屈
折率の平均値である。[Claims] 1. In order from the object side, the first lens is a positive lens, the second and third lenses are both negative meniscus lenses, and the fourth lens is a positive meniscus lens.
The first group has a negative refractive power as a whole, the fifth and sixth lenses are both positive lenses, the seventh lens is a negative lens, the eighth lens is a negative lens, and the ninth lens is a positive lens. It is a lens system consisting of a 6-element lens, a 10th lens which is a positive lens, and a 2nd group having positive refractive power as a whole, and both groups are arranged with an aperture in between. , the image-side surface of either the ninth lens or the tenth lens is an aspherical surface, and the apex (pole) of the aspherical surface is the y-axis in the optical axis direction, and the optical axis is perpendicular to the aspherical surface. When the equation of an aspheric surface is generally taken as y = f (x) with the x axis taken, the sign of the second derivative of f (x) f'' (x) = d 2 y/dx 2 is within the effective diameter. A large aperture ratio wide-angle photographic lens using an aspherical surface, characterized in that there is one place near the edge of which changes from negative to positive, and configured to satisfy the following conditions. ( 1) 1.2f<|f 123 |<2.0f, f 123 <0 (2) 0.4f<D 6 <0.9f (3) 1.0f<f<1.6f (4) 2f<L<3f (5) 5f <f 1 <12f (6) N P >1.7 Here, f 123 is the combined focal length from the first lens to the third lens, f is the focal length of the entire system, and D 6 is the combined focal length of the third and fourth lenses. air spacing, f is the second
The focal length of the group, L is the total length of the lens, f 1 is the focal length of the first lens, and N P is the average value of the refractive index of the fifth lens and the sixth lens.
Priority Applications (1)
| Application Number | Priority Date | Filing Date | Title |
|---|---|---|---|
| JP15700981A JPS5858516A (en) | 1981-10-02 | 1981-10-02 | High-aperture ratio wide angle photographic lens using aspherical surface |
Applications Claiming Priority (1)
| Application Number | Priority Date | Filing Date | Title |
|---|---|---|---|
| JP15700981A JPS5858516A (en) | 1981-10-02 | 1981-10-02 | High-aperture ratio wide angle photographic lens using aspherical surface |
Publications (2)
| Publication Number | Publication Date |
|---|---|
| JPS5858516A JPS5858516A (en) | 1983-04-07 |
| JPS6132655B2 true JPS6132655B2 (en) | 1986-07-28 |
Family
ID=15640179
Family Applications (1)
| Application Number | Title | Priority Date | Filing Date |
|---|---|---|---|
| JP15700981A Granted JPS5858516A (en) | 1981-10-02 | 1981-10-02 | High-aperture ratio wide angle photographic lens using aspherical surface |
Country Status (1)
| Country | Link |
|---|---|
| JP (1) | JPS5858516A (en) |
Cited By (1)
| Publication number | Priority date | Publication date | Assignee | Title |
|---|---|---|---|---|
| JPS6330685U (en) * | 1986-08-12 | 1988-02-29 |
Family Cites Families (8)
| Publication number | Priority date | Publication date | Assignee | Title |
|---|---|---|---|---|
| JPS5232365B2 (en) * | 1972-06-15 | 1977-08-20 | ||
| JPS5510049B2 (en) * | 1972-07-04 | 1980-03-13 | ||
| JPS5832682B2 (en) * | 1975-10-29 | 1983-07-14 | 株式会社ニコン | Koukakuzu-Murrenskei |
| JPS594682B2 (en) * | 1976-05-10 | 1984-01-31 | 旭光学工業株式会社 | Zoom lens system |
| JPS594683B2 (en) * | 1976-09-22 | 1984-01-31 | 旭光学工業株式会社 | Small and bright wide zoom lens |
| JPS53135658A (en) * | 1977-04-30 | 1978-11-27 | Asahi Optical Co Ltd | Zoom lens including ultraawide lens |
| JPS5415733A (en) * | 1977-06-10 | 1979-02-05 | Asahi Optical Co Ltd | Lowwmagnification variableeangleelens system |
| JPS5560911A (en) * | 1978-11-01 | 1980-05-08 | Mamiya Koki Kk | Wide angle zoom lens |
-
1981
- 1981-10-02 JP JP15700981A patent/JPS5858516A/en active Granted
Cited By (1)
| Publication number | Priority date | Publication date | Assignee | Title |
|---|---|---|---|---|
| JPS6330685U (en) * | 1986-08-12 | 1988-02-29 |
Also Published As
| Publication number | Publication date |
|---|---|
| JPS5858516A (en) | 1983-04-07 |
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