Imaging optical system and optical apparatus using the same

Information

  • Patent Grant
  • 6822806
  • Patent Number
    6,822,806
  • Date Filed
    Thursday, February 26, 2004
    20 years ago
  • Date Issued
    Tuesday, November 23, 2004
    20 years ago
Abstract
An imaging optical system has a variable magnification optical system. The variable magnification optical system includes, in order from the object side, a first lens unit with positive refractive power, a second lens unit with positive refractive power, a third lens unit with negative refractive power, a fourth lens unit with positive refractive power, and an aperture stop interposed between the third lens unit and the fourth lens unit. The variable magnification optical system changes an imaging magnification while keeping an object-to-image distance constant. The imaging magnification is changed by varying spacing between the first lens unit and the second lens unit, spacing between the second lens unit and the third lens unit, and spacing between the third lens unit and the fourth lens unit. When the imaging magnification is changed, the imaging optical system satisfies the following conditions in at least one variable magnification state:|En|/L>0.4|Ex|/|L/β|>0.4where En is a distance from a first lens surface on the object side of the variable magnification optical system to the entrance pupil of the imaging optical system, L is the object-to-image distance of the imaging optical system, Ex is a distance from the most image-side lens surface of the variable magnification optical system to the exit pupil of the imaging optical system, and β is the magnification of the entire system of the imaging optical system.
Description




BACKGROUND OF THE INVENTION




1. Field of the Invention




This invention relates to a variable magnification lens which is capable of changing an imaging magnification in accordance with the purpose of use and an optical system which is capable of photographing an image recorded by a film at a magnification most suitable for the film, and to an optical apparatus, such as an image transforming apparatus, using this optical system.




2. Description of Related Art




Imaging optical systems which are designed to be both-side telecentric and to change the imaging magnification have been proposed, for example, by Japanese Patent Kokai No. 2001-27726 and Japanese Patent No. 2731481.




The optical system set forth in Kokai No. 2001-27726 includes, in order from the object side, the first lens unit with positive refractive power, the second lens unit with positive refractive power, the third lens unit with negative refractive power, and is the fourth lens unit with positive refractive power. This optical system is thus constructed to be both-side telecentric and to change the imaging magnification.




The optical system set forth in U.S. Pat. No. 2,731,481 includes, in order from the object side, the first lens unit with positive refractive power, the second lens unit with negative refractive power, and the third lens unit with positive refractive power. This optical system is thus constructed to be both-side telecentric and to change the imaging magnification while keeping an object-to-image distance constant.




SUMMARY OF THE INVENTION




The imaging optical system of the present invention includes a variable magnification optical system comprising, in order from the object side toward the image side, a first lens unit with positive refractive power, a second lens unit with positive refractive power, a third lens unit with negative refractive power, a fourth lens unit with positive refractive power, and an aperture stop interposed between the third lens unit and the fourth lens unit. The variable magnification optical system changes an imaging magnification while keeping an object-to-image distance constant. The imaging magnification is changed by varying spacing between the first lens unit and the second lens unit, spacing between the second lens unit and the third lens unit, and spacing between the third lens unit and the fourth lens unit. When the imaging magnification is changed, the imaging optical system satisfies the following conditions in at least one variable magnification state:






|


En|/L


>0.4








|


Ex|/|L


/β|>0.4






where En is a distance from a first lens surface on the object side of the variable magnification optical system to the entrance pupil of the imaging optical system, L is the object-to-image distance of the imaging optical system, Ex is a distance from the most image-side lens surface of the variable magnification optical system to the exit pupil of the imaging optical system, and β is the magnification of the entire system of the imaging optical system.




The imaging optical system of the present invention preferably satisfies the following conditions:






1.0


<MAXFNO


<8.0











FNO


/Δβ|<5






where MAXFNO is the smallest object-side F-number where the imaging magnification of the imaging optical system is changed, ΔFNO is a difference between the object-side F-number at the minimum magnification and the object-side F-number at the maximum magnification in the entire system of the imaging optical system, and Δβ is a difference between the minimum magnification and the maximum magnification in the entire system of the imaging optical system.




The imaging optical system of the present invention preferably satisfies the following condition:






0.6<|(


R




3




f+R




3




b


)/(


R




3




f−R




3




b


)|<5.0






where R


3


f is the radius of curvature of the most object-side surface of the third lens unit and R


3


b is the radius of curvature of the most image-side surface of the third lens unit.




The imaging optical system of the present invention is preferably constructed so that the most object-side lens of the first lens unit has positive refractive power.




The imaging optical system of the present invention is preferably constructed so that the first lens unit includes, in order from the object side, a lens with positive refractive power, a lens with negative refractive power, and a lens with positive refractive power.




The imaging optical system of the present invention is preferably constructed so that the third lens unit includes at least two meniscus lenses, each with a convex surface directed toward the object side.




The imaging optical system of the present invention is preferably constructed so that the third lens unit includes two meniscus lenses, each with negative refractive power, and one meniscus lens with positive refractive power.




In the present invention, an optical apparatus using the imaging optical system of the present invention is provided.




According to the present invention, the imaging optical system in which even when the imaging magnification is changed, the object-to-image distance remains unchanged and the fluctuation of the F-number is minimized, and the optical apparatus using the imaging optical system can be provided.




These and other features and advantages of the present invention will become apparent from the following detailed description of the preferred embodiments when taken in conjunction with the accompanying drawings.











BRIEF DESCRIPTION OF THE DRAWINGS





FIGS. 1A

,


1


B, and


1


C are sectional views showing optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of a first embodiment of the imaging optical system according to the present invention;





FIGS. 2A

,


2


B, and


2


C are diagrams showing aberration characteristics in focusing at an imaging magnification of 0.4× of the imaging optical system in the first embodiment;





FIGS. 3A

,


3


B, and


3


C are sectional views showing optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of a second embodiment of the imaging optical system according to the present invention;





FIGS. 4A

,


4


B, and


4


C are diagrams showing aberration characteristics in focusing at an imaging magnification of 0.4× of the imaging optical system in the second embodiment;





FIGS. 5A

,


5


B, and


5


C are sectional views showing optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of a third embodiment of the imaging optical system according to the present invention;





FIGS. 6A

,


6


B, and


6


C are diagrams showing aberration characteristics in focusing at an imaging magnification of 0.4× of the imaging optical system in the third embodiment;





FIGS. 7A

,


7


B, and


7


C are sectional views showing optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of a fourth embodiment of the imaging optical system according to the present invention;





FIGS. 8A

,


8


B, and


8


C are diagrams showing aberration characteristics in focusing at an imaging magnification of 0.4× of the imaging optical system in the fourth embodiment;





FIGS. 9A

,


9


B, and


9


C are sectional views showing optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of a fifth embodiment of the imaging optical system according to the present invention;





FIGS. 10A

,


10


B, and


10


C are diagrams showing aberration characteristics in focusing at an imaging magnification of 0.4× of the imaging optical system in the fifth embodiment;





FIGS. 11A

,


11


B, and


11


C are sectional views showing optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of a sixth embodiment of the imaging optical system according to the present invention;





FIGS. 12A

,


12


B, and


12


C are diagrams showing aberration characteristics in focusing at an imaging magnification of 0.4× of the imaging optical system in the sixth embodiment;





FIGS. 13A

,


13


B, and


13


C are sectional views showing optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of a seventh embodiment of the imaging optical system according to the present invention;





FIGS. 14A

,


14


B, and


14


C are diagrams showing aberration characteristics in focusing at an imaging magnification of 0.4× of the imaging optical system in the seventh embodiment;





FIGS. 15A

,


15


B, and


15


C are sectional views showing optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of an eighth embodiment of the imaging optical system according to the present invention;





FIGS. 16A

,


16


B, and


16


C are diagrams showing aberration characteristics in focusing at an imaging magnification of 0.4× of the imaging optical system in the eighth embodiment;





FIGS. 17A

,


17


B, and


17


C are sectional views showing optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of a ninth embodiment of the imaging optical system according to the present invention;





FIGS. 18A

,


18


B, and


18


C are diagrams showing aberration characteristics in focusing at an imaging magnification of 0.4× of the imaging optical system in the ninth embodiment;





FIG. 19

is a conceptual view showing an embodiment of a telecine apparatus using the imaging optical system of the present invention; and





FIG. 20

is a view showing schematically an embodiment of a height measuring apparatus using the imaging optical system of the present invention.











DETAILED DESCRIPTION OF THE PREFERRED EMBODIMENTS




Before undertaking the description of the embodiments, the function and effect of the present invention will be explained.




In the imaging optical system of the present invention, as described above, the variable magnification optical system includes four lens units with positive, positive, negative, and positive refractive powers. Ahead of (or on the object side of) the stop, the first lens unit with positive refractive power, the second lens unit with positive refractive power, and the third lens unit with negative refractive power are arranged so that the whole of these lens units constitutes a lens system with positive refractive power. The fourth lens unit located behind (or on the image side of) the stop constitutes a lens system with positive refractive power. The aperture stop is interposed between the third lens unit and the fourth lens unit.




The imaging optical system of the present invention is designed to change the imaging magnification while keeping the object-to-image distance constant. That is, the imaging optical system of the present invention is an optical system in which a conjugate length is fixed.




The imaging optical system of the present invention is constructed so that when the imaging magnification is changed, the imaging optical system satisfies the following conditions in at least one variable magnification state and is both-side telecentric:






|


En|/L


>0.4  (1)








|


Ex|/|L


/β|>0.4  (2)






where En is a distance from a first lens surface on the object side of the variable magnification optical system to the entrance pupil of the imaging optical system, L is the object-to-image distance of the imaging optical system, Ex is a distance from the most image-side lens surface of the variable magnification optical system to the exit pupil of the imaging optical system, and β is the magnification of the entire system of the imaging optical system.




The imaging optical system of the present invention is constructed so that the stop is located at the focal position of the lens system made up of the first to third lens units lying on the object side of the stop. By this arrangement, the entrance pupil which is the image of the stop is projected at infinity. As a result, the imaging optical system of the present invention constitutes an object-side telecentric optical system.




Further, the imaging optical system of the present invention is constructed so that the stop is located at the focal position of the lens system of the fourth lens unit lying on the image side of the stop. By this arrangement, the exit pupil which is the image of the stop is projected at infinity. As a result, the imaging optical system of the present invention also constitutes an image-side telecentric optical system.




In the imaging optical system of the present invention constructed as mentioned above, the role of a multi-variator is allotted to each of the second lens unit with positive refractive power and the third lens unit with negative refractive power. Whereby, a synthesized focal length of the first to third lens units located on the object side of the stop can be changed.




Still further, the imaging optical system of the present invention is constructed so that the stop is interposed between the third lens unit and the fourth lens unit. The fourth lens unit located on the image side of the stop has no variable magnification function. Even when the imaging magnification is changed, the shift of the position of the stop is suppressed as far as possible so that the position of the stop remains practically unchanged. An arrangement is thus made such that the stop is always located in the proximity of the focal position of the fourth lens unit, and thereby the imaging optical system is capable of changing the imaging magnification while maintaining the telecentric characteristic and the F-number on the exit side.




However, in order to maintain the object-side telecentric characteristic and fix the conjugate length while keeping the F-number constant when the imaging magnification is changed, it is necessary to satisfy conditions described below. First, even in the magnification change, the stop must be located at the synthesized focal position of the first to third lens units lying on the object side of the stop. Second, even in the magnification change, a distance from an object surface to a stop surface must be kept nearly constant.




In the lens arrangement of positive, negative, and positive refractive powers, if the first lens unit is divided into two lens units with positive and negative refractive powers, the balance between the refractive powers will be destroyed. Consequently, chromatic aberration of magnification and distortion will be increased. As in the present invention, when the first lens unit is divided into two lens units with positive and positive refractive powers and the optical system is constructed with four lens units with positive, positive, negative, and positive refractive powers, the amount of the production of aberration can be minimized.




In the both-side telecentric optical system, even when the magnification is changed, an off-axis ray of light at the position of the stop is nearly parallel to the optical axis. On the image side of the stop, only the fourth lens unit is located, and it is not moved, thus making the focal length constant. Hence, when the magnification is changed, the fluctuation of the image-side F-number is minimized, and it is not necessary to adjust the brightness of a camera even in this case.




When the object-side telecentric optical system is constructed like the imaging optical system of the present invention, the following advantages are obtained. To explain this, a telecine apparatus (a motion picture film scanner) is cited as an example. The telecine apparatus is adapted to digitize the motion picture film. The telecine apparatus is constructed so that the film is illuminated by an illumination optical system and an image is formed by a solid-state image sensor, such as a CCD, through the imaging optical system.




However, when the imaging optical system of the telecine apparatus is constructed to be object-side telecentric like the imaging optical system of the present invention, matching of the pupil of the illumination system with the imaging system is facilitated, and a loss of the amount of light is reduced. Moreover, a change in magnification on an image plane, caused by the disturbance of flatness of the film, can be kept to a minimum.




When the image-side telecentric optical system is constructed like the imaging optical system of the present invention, the following advantages are obtained. To explain this, a so-called multi-imager camera using image sensors in accordance with colors, such as RGB, is cited as an example. In this multi-imager camera, a color separation prism is generally used. This prism has a separation interference film splitting light in accordance with wavelength, namely a dichroic film, on its interface. If the exit pupil is located close to the image plane, the angle of incidence where a chief ray is incident on the interference film will be changed in accordance with the position of an image point on the image. Consequently, the optical path length of film thickness is changed and a color separation characteristic is varied in accordance with a field angle, bringing about different color reproducibility, that is, causing color shading.




However, when the imaging optical system of the multi-imager camera is constructed to be image-side telecentric like the imaging optical system of the present invention, color shading can be suppressed.




Here, for example, it is assumed that the solid-image sensor, such as the CCD, is placed on the image side of the color separation prism. If the exit pupil is located close to the image plane, the chief ray is obliquely incident on a pixel. Thus, off-axis incident light is chiefly blocked by the structure of the CCD to decrease the amount of light, and light other than that to enter an original light-receiving section is incident. This brings about a state where a signal other than original information is output. That is, shading is caused.




However, when the image-side telecentric optical system is constructed like the imaging optical system of the present invention, shading can be suppressed.




The imaging optical system of the present invention is also constructed as the both-side telecentric optical system. Consequently, the imaging magnification can be practically determined by the ratio between the focal length of the lens units located on the object side of the stop and the focal length of the lens unit located on the image side of the stop.




Spacings between individual lens units located on the object side of the stop are changed so that the focal length of the lens units on the object side of the stop is varied. Whereby, the imaging magnification can be changed.




In the imaging optical system of the present invention, the first lens unit has the positive refractive power, and the entrance pupil which is the image of the stop is projected at infinity. In doing so, a chief ray on the object side of the first lens unit is refracted parallel to the optical axis and thereby the object-side telecentric optical system can be realized.




In the imaging optical system of the present invention, the second lens unit has the positive refractive power and the third lens unit has the negative refractive power. By changing the spacing between the second lens unit and the third lens unit, the synthesized focal length of the second and third lens units is varied. That is, the second and third lens units are designed to function as a multi-variator. Thus, the second and third lens units are moved, and thereby the magnification can be optimally adjusted to the size of an object.




When the third lens unit is designed to have the negative refractive power like the imaging optical system of the present invention, the Petzval sum is increased and an optical system which is free of curvature of field can be realized.




The imaging optical system of the present invention is also constructed so that the positive refractive power is imparted to the fourth lens unit and the exit pupil which is the image of the stop is projected at infinity. Thus, the chief ray on the image side of the fourth lens unit is rendered parallel to the optical axis, and thereby the image-side telecentric optical system can be realized.




When the imaging optical system of the present invention provided with the variable magnification function, mentioned above, is used to construct an optical apparatus, the following advantages are obtained. To explain this, for example, the telecine apparatus is cited as described above. The telecine apparatus, in which a video camera is attached to a film photographing device, is constructed so that the film image is converted into a video signal, which is digitized.




On the other hand, motion picture films have a plurality of standards, and the size of the image section of the film varies with each standard. For example, a 35 mm standard film measures 16 (height)×21.95 (width) mm and a European wide film measures 11.9×21.95 mm. In this way, the aspect ratio of the film varies according to the film standard. The dimension of the imaging surface of the CCD, for example, in a ⅔″ CCD solid-state image sensor, is 5.4×9.6 mm. In order to photograph an image through superfine pixels, it is desirable to acquire image information relative to the entire CCD imaging area. For this purpose, it becomes necessary to change the imaging magnification in accordance with the film standard.




However, when the imaging optical system of the present invention is used to construct the optical apparatus, the films of various standards can be digitized, for example, in the telecine apparatus. In this case, even when the imaging magnification is changed, the conjugate length remains unchanged, and the magnification can be varied with little fluctuation in image-side F-number.




For example, when the imaging optical system of the present invention is used to construct the multi-imager camera, color shading caused by the color separation prism and shading of the CCD camera can be suppressed. Moreover, the imaging magnification can be changed, without moving the camera, in accordance with the film standard and the size of the object, and even when the magnification is changed, the adjustment of brightness is unnecessary.




In the imaging optical system of the present invention, in order to obtain further both-side telecentricity, it is favorable that when imaging magnification is changed, the imaging optical system satisfies the following conditions, instead of Conditions (1) and (2), in at least one variable magnification state:






|


En|/L


>0.8  (1′)








|


Ex|/|L


/β|>0.8  (2′)






It is more favorable to satisfy the following conditions:






|


En|/L


>1.6  (1″)








|


Ex|/|L


/β|>1.6  (2″)






In the imaging optical system of the present invention, the F-number is defined by the following conditions:






1.0


<MAXFNO


<8.0  (3)











FNO


/Δβ|<5  (4)






where MAXFNO is the smallest object-side F-number where the imaging magnification of the imaging optical system is changed, ΔFNO is a difference between the object-side F-number at the minimum magnification and the object-side F-number at the maximum magnification in the entire system of the imaging optical system, and Δβ is a difference between the minimum magnification and the maximum magnification in the entire system of the imaging optical system.




Also, the F-number refers to an amount expressing the brightness of the optical system. As the value of the F-number becomes small, a brighter optical system is obtained.




If the F-number is extremely small, the number of lenses must be increased in order to correct aberration. This causes the problem that the overall length of the optical system is increased. On the other hand, an extremely large F-number is not suitable for motion picture photography because of shortage in the amount of light.




However, when the optical system satisfies Condition (3), the F-number is neither extremely small nor large. The above problems that the overall length of the optical system is increased and the F-number is not suitable for motion picture photography can thus be obviated.




If the value of |ΔFNO/Δβ| is extremely large, the fluctuation of the image-side F-number becomes remarkable in the magnification change. As a result, the brightness of the camera must be adjusted. However, when Condition (4) is satisfied, there is no need to adjust the brightness of the camera.




It is desirable to satisfy the following conditions:






2.0


<MAXFNO


<5.6  (3′)











FNO


/Δβ|<3  (4′)






It is more desirable to satisfy the following conditions:






3.0


<MAXFNO


<4.0  (3″)











FNO


/Δβ|<1  (4″)






In the imaging optical system of the present invention, it is desirable that the most object-side lens of the first lens unit has the positive refractive power. When the most object-side lens of the first lens unit is constructed as the positive lens, an off-axis beam of light can be lowered and thus aberration becomes small.




In the imaging optical system of the present invention, it is desirable that the first lens unit includes, in order from the object side, positive, negative, and positive lenses. When the first lens unit is constructed with the positive, negative, and positive lenses, chromatic aberration of magnification and off-axis chromatic aberration can be corrected.




In the imaging optical system of the present invention, it is desirable to satisfy a condition described below. When this condition is satisfied, the fluctuation of off-axis aberration can be kept to a minimum.






0.6<|(


R




3




f+R




3




b


)/(


R




3




f−R




3




b


)|<5.0  (5)






where |(R


3


f+R


3


b)/(R


3


f−R


3


b)| is a virtual shape factor, R


3


f is the radius of curvature of the most object-side surface of the third lens unit and R


3


b is the radius of curvature of the most image-side surface of the third lens unit.




Beyond the upper limit of the virtual shape factor, the radius of curvature of the most object-side surface of the third lens unit approximates that of the most imageside surface of the third lens unit. As such, the refractive power of the third lens unit becomes extremely weak. Consequently, when the imaging magnification is changed, the amount of movement of the third lens unit must be increased. When the amount of movement of the third lens unit is large, the ray height of off-axis light incident on the third lens unit fluctuates. Thus, the fluctuation of off-axis aberration becomes pronounced. Below the lower limit of the virtual shape factor, the refractive power of the third lens unit becomes extremely strong. As a result, the angle of incidence of the off-axis beam on the third lens unit is increased, and the fluctuation of off-axis aberration caused by the movement of the third lens unit becomes heavy.




However, when Condition (5) is satisfied, the refractive power of the third lens unit is neither extremely high nor low, and the above problem that the fluctuation of off-axis aberration is heavy can be obviated.




It is desirable to satisfy the following condition:






1.2<|(


R




3




f+R




3




b


)/(


R




3




f−R




3




b


)|<3.5  (5′)






It is more desirable to satisfy the following condition:






2.0<|(


R




3




f+R




3




b


)/(


R




3




f−R




3




b


)|<3.0  (5″)






In the imaging optical system of the present invention, it is desirable that the third lens unit has at least two meniscus lenses, each with a convex surface directed toward the object side. It is more desirable that the third lens unit has at least three meniscus lenses. More specifically, it is desirable that the third lens unit, for example, has two negative meniscus lenses, each with a convex surface directed toward the object side, and one positive meniscus lens with a convex surface directed toward the object side. Since the third lens unit is located close to the stop, off-axis rays are incident on the lenses of the third lens unit at almost the same angle, irrespective of the angle of view.




However, the meniscus lens in which a convex surface is directed toward the object side, namely the object-side surface has the positive refractive power, has nearly minimum deflection angles with respect to on- and off-axis light beams at individual angles of view, and hence the production of aberration can be prevented.




In accordance with the drawings, the embodiments of the present invention will be described below.




First Embodiment





FIGS. 1A

,


1


B, and


1


C show optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of the first embodiment of the imaging optical system according to the present invention.

FIGS. 2A

,


2


B, and


2


C show aberration characteristics in focusing at an imaging magnification of 0.4× of the imaging optical system in the first embodiment.




The imaging optical system of the first embodiment has a variable magnification optical system Z. In

FIG. 1A

, reference symbol P represents a prism, CG represents a cover glass, and I represents an imaging surface.




The variable magnification optical system Z comprises, in order from the object side toward the image side, a first lens unit G


1


with positive refractive power, a second lens unit G


2


with positive refractive power, a third lens unit G


3


with negative refractive power, an aperture stop S, and a fourth lens unit G


4


with positive refractive power.




The first lens unit G


1


includes, in order from the object side, a biconvex lens L


1




1


, a biconcave lens L


1




2


, and a biconvex lens L


1




3


.




The second lens unit G


2


includes, in order from the object side, a negative meniscus lens L


2




1


with a convex surface directed toward the object side, a biconvex lens L


2




2


, a negative meniscus lens L


2




3


with a concave surface directed toward the object side, and a biconvex lens L


2




4


.




The third lens unit G


3


includes a positive meniscus lens L


3




1


with a convex surface directed toward the object side, a negative meniscus lens L


3




2


with a convex surface directed toward the object side, and a negative meniscus lens L


3




3


with a convex surface directed toward the object side.




The fourth lens unit G


4


includes a cemented doublet of a biconcave lens L


4




1


and a biconvex lens L


4




2


, a biconcave lens L


4




3


, a biconvex lens L


4




4


, a biconvex lens L


4




5


, and a biconvex lens L


4




6


.




When the magnification is changed from 0.3× to 0.5× in focusing of an infinite object point, the first lens unit G


1


, after being moved once toward the object side, is moved toward the image side, the second lens unit G


2


is moved toward the object side, the third lens unit G


3


is moved toward the image side together with the stop S, and the fourth lens unit G


4


is moved toward the image side so that spacing between the third and fourth lens units G


3


and G


4


is slightly widened. Also, the object-to-image distance in the magnification change is kept constant.




Subsequently, numerical data of optical members constituting the imaging optical system of the first embodiment are shown below. In the numerical data, r


0


, r


1


, r


2


, . . . denote radii of curvature of surfaces of individual optical members shown in this order from the object side; d


0


, d


1


, d


2


, . . . denote thicknesses (mm) of individual optical members or air spacings between them; n


e1


, n


e2


, . . . denote refractive indices of individual optical members at the e line; ν


e1


, ν


e2


, . . . denote Abbe's numbers of individual optical members at the e line. These symbols are also used for the numerical data of other embodiments to be described later.


















Numerical data 1













Image height: 5.783







r


0


= ∞ (object)













d


0


= 50.000













r


1


= ∞ (object surface)













d


1


= D1













r


2


= 189.5313















d


2


= 7.308




n


e2


= 1.48915




ν


e2


= 70.04













r


3


= −117.0877













d


3


= 10.588













r


4


= −6124.8097















d


4


= 6.910




n


e4


= 1.61639




ν


e4


= 44.15













r


5


= 67.5133













d


5


= 12.028













r


6


= 88.2299















d


6


= 8.685




n


e6


= 1.43985




ν


e6


= 94.53













r


7


= −425.3119













d


7


= D7













r


8


= 148.1127















d


8


= 6.000




n


e8


= 1.61639




ν


e8


= 44.15













r


9


= 64.7754













d


9


= 5.355













r


10


= 88.2208















d


10


= 8.016




n


e10


= 1.43985




ν


e10


= 94.53













r


11


= −81.9368













d


11


= 1.062













r


12


= −69.6148















d


12


= 7.000




n


e12


= 1.61639




ν


e12


= 44.15













r


13


= −171.6506













d


13


= 17.627













r


14


= 210.1703















d


14


= 6.814




n


e14


= 1.43985




ν


e14


= 94.53













r


15


= −82.3361













d


15


= D15













r


16


= 40.6305















d


16


= 4.323




n


e16


= 1.69417




ν


e16 = 30.83















r


17


= 250.0598













d


17


= 0.300













r


18


= 25.0517















d


18


= 9.360




n


e18


= 1.72538




ν


e18


= 34.47













r


19


= 21.5375













d


19


= 1.156













r


20


= 41.2143















d


20


= 2.000




n


e20


= 1.72538




ν


e20


= 34.47













r


21


= 15.8016













d


21


= 2.560













r


22


= ∞ (aperture stop)













d


22


= D22













r


23


= −29.2488















d


23


= 2.000




n


e23


= 1.61669




ν


e23


= 44.02













r


24


= 23.4936















d


24


= 7.647




n


e24


= 1.48915




ν


e24


= 70.04













r


25


= −17.8845













d


25


= 3.043













r


26


= −13.7038















d


26


= 1.417




n


e26


= 1.61639




ν


e26


= 44.15













r


27


= 89.8893













d


27


= 4.829













r


28


= 707.1568















d


28


= 8.564




n


e28


= 1.43985




ν


e28


= 94.53













r


29


= −18.1649













d


29


= 0.325













r


30


= 69.4722















d


30


= 5.111




n


e30


= 1.43985




ν


e30


= 94.53













r


31


= −90.8646













d


31


= 0.300













r


32


= 62.9985















d


32


= 4.778




n


e32


= 1.43985




ν


e32


= 94.53













r


33


= −179.4454













d


33


= D33













r


34


= ∞















d


34


= 33.000




n


e34


= 1.61173




ν


e34


= 46.30













r


35


= ∞















d


35


= 13.200




n


e35


= 1.51825




ν


e35


= 63.93













r


36


= ∞













d


36


= 0.500













r


37


= ∞ (imaging surface)













d


37


= 0.000





























Zoom data















0.3×




0.4×




0.5×




















D1




39.880




37.812




44.358







D7




109.204




77.238




48.939







D15




3.000




37.903




60.723







D22




3.552




4.754




6.263







D33




21.051




18.980




16.405





























Parameters of conditions
















Magnification: β




0.3×




0.4×




0.5×




















Entrance pupil position: En




1160.856




20252.775




−1133.552







Object-to-image distance: L




428.492




428.492




428.492







|En|/L




2.709




47.265




2.645







Exit pupil position: Ex




−352.468




−578.834




−1818.976







|Ex|/|L/β|




0.247




0.540




2.123







F-number: FNO




3.500




3.536




3.598














FNO fluctuation: ΔFNO




0.098







|ΔFNO/Δβ|




0.490







Object-side radius of curva-




40.630







ture: R3f







Image-side radius of curva-




15.802







ture: R3b







|(R3f + F3b)/(R3f − R3b)|




2.273















Second Embodiment





FIGS. 3A

,


3


B, and


3


C show optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of the second embodiment of the imaging optical system according to the present invention.

FIGS. 4A

,


4


B, and


4


C show aberration characteristics in focusing at a magnification of 0.4× of the imaging optical system in the second embodiment.




The imaging optical system of the second embodiment has the variable magnification optical system Z.




The variable magnification optical system Z comprises, in order from the object side toward the image side, the first lens unit G


1


with positive refractive power, the second lens unit G


2


with positive refractive power, the third lens unit G


3


with negative refractive power, the aperture stop S, and the fourth lens unit G


4


with positive refractive power.




The first lens unit G


1


includes, in order from the object side, the biconvex lens L


1




1


, a negative meniscus lens L


1




2


′ with a convex surface directed toward the object side, and the biconvex lens L


1




3


.




The second lens unit G


2


, in order from the object side, the negative meniscus lens L


2




1


with a convex surface directed toward the object side, the biconvex lens L


2




2


, the negative meniscus lens L


2




3


with a concave surface directed toward the object side, and the biconvex lens L


2




4


.




The third lens unit G


3


includes the positive meniscus lens L


3




1


with a convex surface directed toward the object side, the negative meniscus lens L


3




2


with a convex surface directed toward the object side, and the negative meniscus lens L


3




3


with a convex surface directed toward the object side.




The fourth lens unit G


4


includes the cemented doublet of the biconcave lens L


4




1


and the biconvex lens L


4




2


, the biconcave lens L


4




3


, the biconvex lens L


4




4


, the biconvex lens L


4




5


, and the biconvex lens L


4




6


.




When the magnification is changed from 0.3× to 0.5× in focusing of the infinite object point, the first lens unit G


1


, after being moved once toward the object side, is moved toward the image side, the second lens unit G


2


is moved toward the object side, the third lens unit G


3


remains fixed together with the stop S, and the fourth lens unit G


4


is moved toward the image side so that the spacing between the third and fourth lens units G


3


and G


4


is slightly widened. Also, the object-to-image distance in the magnification change is kept constant. Subsequently, numerical data of optical members constituting the imaging optical system of the second embodiment are shown below.


















Numerical data 2













Image height: 5.783







r


0


= ∞ (object)













d


0


= 50.000













r


1


= ∞ (object surface)













d


1


= D1













r


2


= 172.4277















d


2


= 6.648




n


e2 = 1.48915






ν


e2


= 70.04













r


3


= −112.2625













d


3


= 7.313













r


4


= 1492.6672















d


4 = 7.985






n


e4 = 1.61639






ν


e4


= 44.15













r


5


= 62.4069













d


5


= 12.125













r


6


= 79.8565















d


6


= 9.415




n


e6


= 1.43985




ν


e6


= 94.53













r


7


= −1585.7009













d


7


= D7













r


8


= 151.8708















d


8


= 6.000




n


e8


= 1.61639




ν


e




8


= 44.15













r


9


= 64.4718













d


9


= 5.384













r


10


= 86.7203















d


10


= 8.163




n


e10


= 14.3985




ν


e10


= 94.53













r


11


= −80.8037













d


11


= 1.049













r


12


= −68.7719















d


12


= 6.410




n


e12


= 1.61639




ν


e12


= 44.15













r


13


= −178.7270













d


13


= 16.603













r


14


= 219.0646















d


14


= 6.722




n


e14


= 1.43985




ν


e14


= 94.53













r


15


= −81.1984













d


15


= D15













r


16


= 40.1465















d


16


= 4.375




n


e16


= 1.69417




ν


e16


= 30.83













r


17


= 229.4681













d


17


= 0.300













r


18


= 24.8118















d


18


= 9.366




n


e18


= 1.72538




ν


e18


= 34.47













r


19


= 21.1952













d


19


= 1.169













r


20


= 40.9998















d


20


= 2.000




n


e20


= 1.72538




ν


e20


= 34.47













r


21


= 15.9793













d


21


= 2.555













r


22


= ∞ (aperature stop)













d


22


= D22













r


23


= −29.1565















d


23


= 2.000




n


e23


= 1.61669




ν


e23


= 44.02













r


24


= 23.6864















d


24


= 7.373




n


e24


= 1.48915




ν


e24


= 70.04













r


25


= −18.0561













d


25


= 3.435













r


26


= −13.7966















d


26


= 1.355




n


e26


= 1.61639




ν


e26


= 44.15













r


27


= 84.7189













d


27


= 4.778













r


28


= 547.3608















d


28


= 8.544




n


e28


= 1.43985




ν


e28


= 94.53













r


29


= −18.0837













d


29


= 0.300













r


30


= 70.0296















d


30


= 5.063




n


e30


= 1.43985




ν


e30


= 94.53













r


31


= −93.9274













d


31


= 0.388













r


32


= 58.3720















d


32


= 4.869




n


e32


= 1.43985




ν


e32


= 94.53













r


33


= −203.9907













d


33


= D33













r


34


= ∞















d


34


= 33.000




n


e34


= 1.61173




ν


e34


= 46.30













r


35 = ∞

















d


35


= 13.200




n


e35


= 1.51825




ν


e35


= 63.93













r


36


= ∞













d


36


= 0.500













r


37


= ∞ (imaging surface)













d


37


= 0.000





























Zoom data















0.3×




0.4×




0.5×




















D1




43.904




39.311




43.788







D7




110.381




79.183




50.950







D15




3.089




38.880




62.637







D22




3.559




5.250




7.195







D33




20.639




18.949




17.003





























Parameters of conditions
















Magnification: β




0.3×




0.4×




0.5×




















Entrance pupil position: En




1124.667




16516.516




−1141.823







Object-to-image distance: L




429.959




429.959




429.959







|En|/L




2.616




38.414




2.656







Exit pupil position: Ex




−351.154




−741.700




24496.963







|Ex|/|L/β|




0.245




0.690




28.488







F-number: FNO




3.500




3.560




3.646














FNO fluctuation: ΔFNO




0.146







|ΔFNO/Δβ|




0.729







Object-side radius of curva-




38.452







ture: R3f







Image-side radius of curva-




17.589







ture: R3b







|(R3f + R3b)/(R3f − R3b)|




2.686















Third Embodiment





FIGS. 5A

,


5


B, and


5


C show optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of the third embodiment of the imaging optical system according to the present invention.

FIGS. 6A

,


6


B, and


6


C show aberration characteristics in focusing at a magnification of 0.4× of the imaging optical system in the third embodiment.




The imaging optical system of the third embodiment has the variable magnification optical system Z.




The variable magnification optical system Z comprises, in order from the object side toward the image side, the first lens unit G


1


with positive refractive power, the second lens unit G


2


with positive refractive power, the third lens unit G


3


with negative refractive power, the aperture stop S, and the fourth lens unit G


4


with positive refractive power.




The first lens unit G


1


includes, in order from the object side, the biconvex lens L


1




1


, the negative meniscus lens L


1




2


′ with a convex surface directed toward the object side, and a positive meniscus lens L


1




3


′ with a convex surface directed toward the object side.




The second lens unit G


2


, in order from the object side, the negative meniscus lens L


2




1


with a convex surface directed toward the object side, the biconvex lens L


2




2


, the negative meniscus lens L


2




3


with a concave surface directed toward the object side, and the biconvex lens L


2




4


.




The third lens unit G


3


includes the positive meniscus lens L


3




1


with a convex surface directed toward the object side, the negative meniscus lens L


3




2


with a convex surface directed toward the object side, and the negative meniscus lens L


3




3


with a convex surface directed toward the object side.




The fourth lens unit G


4


includes the cemented doublet of the biconcave lens L


4




1


and the biconvex lens L


4




2


, the biconcave lens L


4




3


, the biconvex lens L


4




4


, the biconvex lens L


4




5


, and the biconvex lens L


4




6


.




When the magnification is changed from 0.3× to 0.5× in focusing of the infinite object point, the first lens unit G


1


, after being moved once toward the object side, is moved toward the image side, the second lens unit G


2


is moved toward the object side, the third lens unit G


3


is moved toward the object side together with the stop S so that the spacing between the third and fourth lens units G


3


and G


4


is slightly widened, and the fourth lens unit G


4


remains fixed. Also, the object-to-image distance in the magnification change is kept constant.




Subsequently, numerical data of optical members constituting the imaging optical system of the third embodiment are shown below.


















Numerical data 3













Image height: 5.783







r


0


= ∞ (object)













d


0


= 50.000













r


1


= ∞ (object surface)













d


1


= D1













r


2


= 67.5689















d


2


= 7.816




n


e2


= 1.48915




ν


e2


= 70.04













r


3


= −335.3716













d


3


= 0.300













r


4


= 140.6380















d


4


= 6.025




n


e4


= 1.61639




ν


e4


= 44.15













r


5


= 45.2535













d


5


= 8.810













r


6


= 57.6476















d


6


= 11.963




n


e6


= 1.43985




ν


e6


= 94.53













r


7


= 109.0130













d


7


= D7













r


8


= 140.9050















d


8


= 6.209




n


e8


=1.61639




ν


e8


= 44.15













r


9


= 59.1517













d


9


= 5.421













r


10


= 89.7738















d


10


= 7.460




n


e10


= 1.43985




ν


e10


= 94.53













r


11


= −74.4487













d


11


= 1.335













r


12


= −57.6329















d


12


= 7.000




n


e12


= 1.61639




νe


12


= 44.15













r


13


= −145.4391













d


13


= 15.344













r


14


= 312.0611















d


14


= 8.089




n


e14


= 1.43985




ν


e14


= 94.53













r


15


= −66.7614













d


15


= D15













r


16


= 42.2336















d


16


= 4.331




n


e16


= 1.69417




ν


e16


= 30.83













r


17


= 254.0344













d


17


= 0.300













r


18


= 24.1640















d


18


= 9.326




n


e18


= 1.72538




ν


e18


= 34.47













r


19


= 20.0169













d


19


= 1.206













r


20


= 36.3821















d


20


= 2.000




n


e20


= 1.72538




ν


e20


= 34.47













r


21


= 16.7574













d


21


= 2.601













r


22


= ∞ (aperture stop)













d


22


= D22













r


23


= −26.7471















d


23


= 2.030




n


e23


= 1.61669




ν


e23


= 44.02













r


24


= 24.0157















d


24


= 5.463




n


e24


= 1.48915




ν


e24


= 70.04













r


25


= −17.6590













d


25


= 4.328













r


26


= −13.4729















d


26


= 1.058




n


e26


= 1.61639




ν


e26


= 44.15













r


27


= 93.0104













d


27


= 4.726













r


28


= 913.0291















d


28


= 8.540




n


e28


= 1.43985




ν


e28


= 94.53













r


29


= −17.8834













d


29


= 0.300













r


30


= 81.9603















d


30


= 6.985




n


e30


= 1.43985




ν


e30


= 94.53













r


31


= −64.2115













d


31


= 3.523













r


32


= 60.0466















d


32


= 6.110




n


e32


= 1.43985




ν


e32


= 94.53













r


33


= −318.5459













d


33


= 19.314













r


34


= ∞















d


34


= 33.000




n


e34


= 1.61173




ν


e34


= 46.30













r


35


= ∞















d


35


= 13.200




n


e35


= 1.51825




ν


e35


= 63.93













r


36


= ∞













d


36


= 0.500













r


37


= ∞ (imaging surface)













d


37


= 0.000





























Zoom data















0.3×




0.4×




0.5×




















D1




50.134




38.319




43.946







D7




107.947




77.883




43.657







D15




3.000




42.757




69.242







D22




3.638




5.759




7.874





























Parameters of conditions
















Magnification: β




0.3×




0.4×




0.5×




















Entrance pupil position: En




1271.479




−18393.929




−1095.982







Object-to-image distance: L




429.334




429.334




429.334







|En|/L




2.962




42.843




2.553







Exit pupil position: Ex




−362.746




−906.100




4824.866







|Ex|/|L/β|




0.253




0.844




5.619







F-number: FNO




3.500




3.593




3.687














FNO fluctuation: ΔFNO




0.187







|ΔFNo/Δβ|




0.935







Object-side radius of




42.234







curvature: R3f







Image-side radius of




16.757







curvature: R3b







|(R3f + R3b)/(R3f − R3b)|




2.316















Fourth Embodiment





FIGS. 7A

,


7


B, and


7


C show optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of the fourth embodiment of the imaging optical system according to the present invention.

FIGS. 8A

,


8


B, and


8


C show aberration characteristics in focusing at a magnification of 0.4× of the imaging optical system in the fourth embodiment.




The imaging optical system of the fourth embodiment has the variable magnification optical system Z.




The variable magnification optical system Z comprises, in order from the object side toward the image side, the first lens unit G


1


with positive refractive power, the second lens unit G


2


with positive refractive power, the third lens unit G


3


with negative refractive power, the aperture stop S, and the fourth lens unit G


4


with positive refractive power.




The first lens unit G


1


includes, in order from the object side, the biconvex lens L


1




1


, the negative meniscus lens L


1




2


′ with a convex surface directed toward the object side, and the positive meniscus lens L


1




3


′ with a convex surface directed toward the object side.




The second lens unit G


2


, in order from the object side, the negative meniscus lens L


2




1


with a convex surface directed toward the object side, the biconvex lens L


2




2


, the negative meniscus lens L


2




3


with a concave surface directed toward the object side, and the biconvex lens L


2




4


.




The third lens unit G


3


includes the positive meniscus lens L


3




1


with a convex surface directed toward the object side, the negative meniscus lens L


3




2


with a convex surface directed toward the object side, and the negative meniscus lens L


3




3


with a convex surface directed toward the object side.




The fourth lens unit G


4


includes the cemented doublet of the biconcave lens L


4




1


and the biconvex lens L


4




2


, the biconcave lens L


4




3


, the biconvex lens L


4




4


, the biconvex lens L


4




5


, and the biconvex lens L


4




6


.




When the magnification is changed from 0.3× to 0.5× in focusing of the infinite object point, the first lens unit G


1


is moved toward the image side, the second lens unit G


2


is moved toward the object side, the third lens unit G


3


is moved toward the image side, and the fourth lens unit G


4


is moved toward the image side together with the stop S so that the spacing between the third and fourth lens units G


3


and G


4


is slightly widened. Also, the object-to-image distance in the magnification change is kept constant.




Subsequently, numerical data of optical members constituting the imaging optical system of the fourth embodiment are shown below.


















Numerical data 4













Image height: 5.783







r


0


= ∞ (object)













d


0


= 50.000













r


1


= ∞ (object surface)













d


1


= D1













r


2


= 107.8560















d


2


= 7.337




n


e2


= 1.48915




ν


e2


= 70.04













r


3


= −119.7849













d


3


= 3.971













r


4


= 454.1088















d


4


= 7.857




n


e4


= 1.61639




ν


e4


= 44.15













r


5


= 49.9355













d


5


= 12.309













r


6


= 64.2291















d


6


= 6.018




n


e6


= 1.43985




ν


e6


= 94.53













r


7


= 300.8668













d


7


= D7













r


8


= 126.3256















d


8


= 6.000




n


e8


= 1.61639




ν


e8


= 44.15













r


9


= 56.4062













d


9


= 6.775













r


10


= 81.4055















d


10


= 8.793




n


e10


= 1.43985




ν


e10


= 94.53













r


11


= −83.1434













d


11


= 1.494













r


12


= −63.8486















d


12


= 7.000




n


e12


= 1.61639




ν


e12


= 44.15













r


13


= −133.7944













d


13


= 15.757













r


14


= 330.3809















d


14


= 7.640




n


e14


= 1.43985




ν


e14


= 94.53













r


15


= −69.3107













d


15


= D15













r


16


= 40.1299















d


16


= 4.652




n


e16


= 1.69417




ν


e16


= 30.83













r


17


= 187.3566













d


17


= 0.300













r


18


= 24.6796















d


18


= 9.359




n


e18


= 1.72538




ν


e18


= 34.47













r


19


= 20.3802













d


19


= 1.377













r


20


= 39.2697















d


20


= 2.000




n


e20


= 1.72538




ν


e20


= 34.47













r


21


= 16.0804













d


21


= D21













r


22


= ∞ (aperture stop)













d


22


= 3.575













r


23


= −30.0984















d


23


= 2.000




n


e23


= 1.61669




ν


e23


= 44.02













r


24


= 23.9795















d


24


= 8.757




n


e24


= 1.48915




ν


e24


= 70.04













r


25


= −18.9682













d


25


= 3.837













r


26


= −14.1963















d


26


= 0.817




n


e26


= 1.61639




ν


e26


= 44.15













r


27


= 101.4717













d


27


= 4.565













r


28


= 1012.5847















d


28


= 8.419




n


e28


= 1.43985




ν


e28


= 94.53













r


29


= −18.1103













d


29


= 0.629













r


30


= 69.9749















d


30


= 4.880




n


e30


= 1.43985




ν


e30


= 94.53













r


31


= −123.8898













d


31


= 0.928













r


32


= 61.1846















d


32


= 4.997




n


e32


= 1.43985




ν


e32


= 94.53













r


33


= −136.6736













d


33


= D33













r


34


= ∞















d


34


= 33.000




n


e34


= 1.61173




ν


e34


= 46.30













r


35


= ∞















d


35


= 13.200




n


e35


= 1.51825




ν


e35


= 63.93













r


36


= ∞













d


36


= 0.500













r


37


= ∞ (imaging surface)













d


37


= 0.000





























Zoom data















0.3×




0.4×




0.5×




















D1




38.765




44.451




53.283







D7




117.344




81.410




52.958







D15




3.000




34.932




56.369







D21




2.614




3.787




5.228







D33




21.660




18.803




15.544





























Parameters of conditions
















Magnification: β




0.3×




0.4×




0.5×




















Entrance pupil position: En




1117.828




5171.585




−1158.986







Object-to-image distance: L




432.125




432.125




432.125







|En|/L




2.587




11.968




2.682







Exit pupil position: Ex




−357.630




−357.630




−357.630







|Ex|/|L/β|




0.248




0.331




0.485







F-number: FNO




3.500




3.479




3.414














FNO fluctuation: ΔFNO




−0.046







|ΔFNO/Δβ|




−0.228







Object-side radius of curva-




40.130







ture: R3f







Image-side radius of curva-




16.080







ture: R3b







|(R3f + R3b)/(R3f − R3b)|




2.337















Fifth Embodiment





FIGS. 9A

,


9


B, and


9


C show optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of the fifth embodiment of the imaging optical system according to the present invention.

FIGS. 10A

,


10


B, and


10


C show aberration characteristics in focusing at a magnification of 0.4× of the imaging optical system in the fifth embodiment.




The imaging optical system of the fifth embodiment has the variable magnification optical system Z.




The variable magnification optical system Z comprises, in order from the object side toward the image side, the first lens unit G


1


with positive refractive power, the second lens unit G


2


with positive refractive power, the third lens unit G


3


with negative refractive power, the aperture stop S, and the fourth lens unit G


4


with positive refractive power.




The first lens unit G


1


includes, in order from the object side, a plano-convex lens L


1




1


′ with a convex surface directed toward the object side and a plane surface directed toward the image side, the negative meniscus lens L


1




2


′ with a convex surface directed toward the object side, and the positive meniscus lens L


1




3


′ with a convex surface directed toward the object side.




The second lens unit G


2


, in order from the object side, the negative meniscus lens L


2




1


with a convex surface directed toward the object side, the biconvex lens L


2




2


, the negative meniscus lens L


2




3


with a concave surface directed toward the object side, and the biconvex lens L


2




4


.




The third lens unit G


3


includes the positive meniscus lens L


3




1


with a convex surface directed toward the object side, the negative meniscus lens L


3




2


with a convex surface directed toward the object side, and the negative meniscus lens L


3




3


with a convex surface directed toward the object side.




The fourth lens unit G


4


includes the cemented doublet of the biconcave lens L


4




1


and the biconvex lens L


4




2


, the biconcave lens L


4




3


, the biconvex lens L


4




4


, the biconvex lens L


4




5


, and the biconvex lens L


4




6


.




When the magnification is changed from 0.3× to 0.5× in focusing of the infinite object point, the first lens unit G


1


, after being moved once toward the object side, is moved toward the image side, the second lens unit G


2


is moved toward the object side, the third lens unit G


3


is moved toward the object side so that the spacing between the third and fourth lens units G


3


and G


4


is slightly widened, and the fourth lens unit G


4


remains fixed together with the stop S. Also, the object-to-image distance in the magnification change is kept constant.




Subsequently, numerical data of optical members constituting the imaging optical system of the fifth embodiment are shown below.


















Numerical data 5













Image height: 5.783







r


0


= ∞ (object)













d


0


= 50.000













r


1


= ∞ (object surface)













d


1


= D1













r


2


= 53.6678















d


2


= 7.850




n


e2


= 1.48915




ν


e2


= 70.04













r


3


= ∞













d


3


= 0.300













r


4


= 74.4381















d


4


= 6.000




n


e4


= 1.61639




ν


e4


= 44.15













r


5


= 34.5362













d


5


= 8.043













r


6


= 39.1043















d


6


= 4.857




n


e6


= 1.43985




ν


e6


= 94.53













r


7


= 52.1576













d


7


= D7













r


8


= 149.0540















d


8


= 6.000




n


e8


= 1.61639




ν


e8


= 44.15













r


9


= 50.6084













d


9


= 6.908













r


10


= 78.4447















d


10


= 9.096




n


e10


= 1.43985




ν


e10


= 94.53













r


11


= −67.1214













d


11


= 1.239













r


12


= −55.5198















d


12


= 7.000




n


e12


= 1.61639




ν


e12


= 44.15













r


13


= −130.4767













d


13


= 17.549













r


14


= 526.4312















d


14


= 10.495




n


e14


= 1.43985




ν


e14


= 94.53













r


15


= −60.7655













d


15


= D15













r


16


= 42.8799















d


16


= 4.607




n


e16


= 1.69417




ν


e16


= 30.83













r


17


= 241.5957













d


17


= 0.300













r


18


= 24.0062















d


18


= 9.266




n


e18


= 1.72538




ν


e18


= 34.47













r


19


= 20.0630













d


19


= 1.423













r


20


= 37.0493















d


20


= 2.000




n


e20


= 1.72538




ν


e20


= 34.47













r


21


= 16.8163













d


21


= D21













r


22


= ∞ (aperture stop)













d


22


= 3.685













r


23


= −27.7248















d


23


= 2.000




n


e23


= 1.61669




ν


e23


= 44.02













r


24


= 25.1231















d


24


= 5.991




n


e24


= 1.48915




ν


e24


= 70.04













r


25


= −18.8837













d


25


= 4.943













r


26


= −14.1386















d


26


= 0.553




n


e26


= 1.61639




ν


e26


= 44.15













r


27


= 103.4372













d


27


= 4.610













r


28


= 946.2142















d


28


= 8.426




n


e28


= 1.43985




ν


e28


= 94.53













r


29


= −18.1453













d


29


= 0.300













r


30


= 79.1515















d


30


= 7.210




n


e30


= 1.43985




ν


e30


= 94.53













r


31


= −65.2376













d


31


= 5.640













r


32


= 63.0290















d


32


= 6.581




n


e32


= 1.43985




ν


e32


= 94.53













r


33


= −291.4522













d


33


= 19.405













r


34


= ∞















d


34


= 33.000




n


e34


= 1.61173




ν


e34


= 46.30













r


35


= ∞















d


35


= 13.200




n


e35


= 1.51825




ν


e35


= 63.93













r


36


= ∞













d


36


= 0.500













r


37


= ∞ (imaging surface)













d


37


= 0.000





























Zoom data















0.3×




0.4×




0.5×




















D1




42.960




38.372




47.817







D7




105.480




70.527




33.769







D15




3.000




40.551




66.211







D21




2.679




4.670




6.322





























Parameters of conditions
















Magnification: β




0.3×




0.4×




0.5×




















Entrance pupil position: En




1295.110




24846.034




−1103.070







Object-to-image distance: L




423.096




423.096




423.096







|En|/L




3.061




58.724




2.607







Exit pupil position: Ex




−366.274




−366.274




−366.274







|Ex|/|L/β|




0.260




0.346




0.433







F-number: FNO




3.500




3.500




3.500














FNO fluctuation: ΔFNO




0.000







|ΔFNO/Δβ|




−0.002







Object-side radius of curva-




42.880







ture: R3f







Image-side radius of curva-




16.816







ture: R3b







|(R3f + R3b)/(R3f − R3b)|




2.290















Sixth Embodiment





FIGS. 11A

,


11


B, and


11


C show optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of the sixth embodiment of the imaging optical system according to the present invention.

FIGS. 12A

,


12


B, and


12


C show aberration characteristics in focusing at a magnification of 0.4× of the imaging optical system in the sixth embodiment.




The imaging optical system of the sixth embodiment has the variable magnification optical system Z.




The variable magnification optical system Z comprises, in order from the object side toward the image side, the first lens unit G


1


with positive refractive power, the second lens unit G


2


with positive refractive power, the third lens unit G


3


with negative refractive power, the aperture stop S, and the fourth lens unit G


4


with positive refractive power.




The first lens unit G


1


includes, in order from the object side, the biconvex lens L


1




1


, the biconcave lens L


1




2


, and the biconvex lens L


1




3


.




The second lens unit G


2


, in order from the object side, the negative meniscus lens L


2




1


with a convex surface directed toward the object side, the biconvex lens L


2




2


, the negative meniscus lens L


2




3


with a concave surface directed toward the object side, and a positive meniscus lens L


2




4


′ with a concave surface directed toward the object side.




The third lens unit G


3


includes the positive meniscus lens L


3




1


with a convex surface directed toward the object side, the negative meniscus lens L


3




2


with a convex surface directed toward the object side, and the negative meniscus lens L


3




3


with a convex surface directed toward the object side.




The fourth lens unit G


4


includes the cemented doublet of the biconcave lens L


4




1


and the biconvex lens L


4




2


, the biconcave lens L


4




3


, the biconvex lens L


4




4


, the biconvex lens L


4




5


, and the biconvex lens L


4




6


.




When the magnification is changed from 0.3× to 0.5× in focusing of the infinite object point, the first lens unit G


1


is moved toward the object side, the second lens unit G


2


is moved toward the object side so that spacing between the first and second lens units G


1


and G


2


is widened, the third lens unit G


3


is moved together with the stop S toward the image side, and the fourth lens unit G


4


is moved toward the image side so that the spacing between the third and fourth lens units G


3


and G


4


is slightly widened. Also, the object-to-image distance in the magnification change is kept constant.




Subsequently, numerical data of optical members constituting the imaging optical system of the sixth embodiment are shown below.


















Numerical data 6













Image height: 5.783







r


0


= ∞ (object)













d


0


= 50.000













r


1


= ∞ (object surface)













d


1


= D1













r


2


= 361.3250















d


2


= 12.000




n


e2


= 1.48915




ν


e2


= 70.04













r


3


= −65.3190













d


3


= 0.300













r


4


= −90.3503















d


4


= 8.000




n


e4


= 1.61639




ν


e4


= 44.15













r


5


= 45.5593













d


5


= 11.355













r


6


= 65.7955















d


6


= 12.000




n


e6


= 1.43985




ν


e6


= 94.53













r


7


= −101.4028













d


7


= D7













r


8


= 113.0032















d


8


= 7.000




n


e8


= 1.61639




ν


e8


= 44.15













r


9


= 53.1618













d


9


= 7.854













r


10


= 84.6315















d


10


= 8.348




n


e10


= 1.43985




ν


e10


= 94.53













r


11


= −82.9242













d


11


= 2.346













r


12


= −51.6817















d


12


= 6.901




n


e12


= 1.61639




ν


e12


= 44.15













r


13


= −78.9538













d


13


= 0.300













r


14


= −746.1406















d


14


= 7.363




n


e14


= 1.43985




ν


e14


= 94.53













r


15


= −54.9986













d


15


= D15













r


16


= 40.2152















d


16


= 4.672




n


e16


= 1.69417




ν


e16


= 30.83













r


17


= 202.9669













d


17


= 0.300













r


18


= 25.2156















d


18


= 9.337




n


e18


= 1.72538




ν


e18


= 34.47













r


19


= 20.5989













d


19


= 1.486













r


20


= 47.2290















d


20


= 2.000




n


e20


= 1.72538




ν


e20


= 34.47













r


21


= 17.1952













d


21


= D21













r


22


= ∞ (aperture stop)













d


22


= 8.090













r


23


= −31.8155















d


23


= 12.000




n


e23


= 1.61669




ν


e23


= 44.02













r


24


= 23.4115















d


24


= 6.316




n


e24


= 1.48915




ν


e24


= 70.04













r


25


= −23.1015













d


25


= 1.525













r


26


= −17.3296















d


26


= 0.137




n


e26


= 1.61639




ν


e26


= 44.15













r


27


= 121.5936













d


27


= 4.365













r


28


= 236.9154















d


28


= 8.477




n


e28


= 1.43985




ν


e28


= 94.53













r


29


= −20.8758













d


29


= 0.300













r


30


= 78.3373















d


30


= 5.274




n


e30


= 1.43985




ν


e30


= 94.53













r


31


= −103.6059













d


31


= 0.983













r


32


= 81.5041















d


32


= 5.879




n


e32


= 1.43985




ν


e32


= 94.53













r


33


= −103.9512













d


33


= D33













r


34


= ∞















d


34


= 33.000




n


e34


= 1.61173




ν


e34


= 46.30













r


35


= ∞















d


35


= 13.200




n


e35


= 1.51825




ν


e35


= 63.93













r


36


= ∞













d


36


= 0.500













r


37


= ∞ (imaging surface)













d


37


= 0.000





























Zoom data















0.3×




0.4×




0.5×




















D1




68.668




51.352




36.703







D7




65.281




56.350




50.311







D15




3.000




32.024




53.396







D21




2.770




2.825




3.398







D33




20.686




17.854




16.597





























Parameters of conditions
















Magnification: β




0.3×




0.4×




0.5×




















Entrance pupil position: En




140.733




198.229




329.610







Object-to-image distance: L




412.012




412.012




412.012







|En|/L




0.342




0.481




0.800







Exit pupil position: Ex




2022.944




2022.944




2022.944







|Ex|/|L/β|




1.473




1.964




2.455







F-number: FNO




3.500




3.511




3.516














FNO fluctuation: ΔFNO




0.016







|ΔFNO/Δβ|




0.082







Object-side radius of curva-




40.215







ture: R3f







Image-side radius of curva-




17.195







ture: R3b







|(R3f + R3b)/(R3f − R3b)|




2.494















Seventh Embodiment





FIGS. 13A

,


13


B, and


13


C show optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of the seventh embodiment of the imaging optical system according to the present invention.

FIGS. 14A

,


14


B, and


14


C show aberration characteristics in focusing at a magnification of 0.4× of the imaging optical system in the seventh embodiment.




The imaging optical system of the seventh embodiment has the variable magnification optical system Z. In

FIG. 13A

, reference symbol GL designates a plane-parallel plate and P


1


and P


2


designate prisms.




The variable magnification optical system Z comprises, in order from the object side toward the image side, the first lens unit G


1


with positive refractive power, the second lens unit G


2


with positive refractive power, the third lens unit G


3


with negative refractive power, the aperture stop S, and the fourth lens unit G


4


with positive refractive power.




The first lens unit G


1


includes, in order from the object side, the biconvex lens L


1




1


, the negative meniscus lens L


1




2


′ with a convex surface directed toward the object side, and the positive meniscus lens L


1




3


′ with a convex surface directed toward the object side.




The second lens unit G


2


, in order from the object side, the negative meniscus lens L


2




1


with a convex surface directed toward the object side, the biconvex lens L


2




2


, the negative meniscus lens L


2




3


with a concave surface directed toward the object side, and the biconvex lens L


2




4


.




The third lens unit G


3


includes the positive meniscus lens L


3




1


with a convex surface directed toward the object side, the negative meniscus lens L


3




2


with a convex surface directed toward the object side, and the negative meniscus lens L


3




3


with a convex surface directed toward the object side.




The fourth lens unit G


4


includes the cemented doublet of the biconcave lens L


4




1


and the biconvex lens L


4




2


, the biconcave lens L


4




3


, a positive meniscus lens L


4




4


′ with a concave surface directed toward the object side, the biconvex lens L


4




5


, and the biconvex lens L


4




6


.




When the magnification is changed from 0.3× to 0.5× in focusing of the infinite object point, the first lens unit G


1


is moved toward the object side, the second lens unit G


2


is moved toward the object side so that the spacing between the first and second lens units G


1


and G


2


is narrowed, the third lens unit G


3


is moved together with the stop S toward the image side, and the fourth lens unit G


4


is moved toward the image side so that the spacing between the third and fourth lens units G


3


and G


4


is slightly widened. Also, the object-to-image distance in the magnification change is kept constant.




Subsequently, numerical data of optical members constituting the imaging optical system of the seventh embodiment are shown below.















Numerical data 7






Image height: 5.783


























r


0


= ∞ (object)










d


0


= 51.000






r


1


= ∞ (object surface)







d


1


= 9.260




n


e1


= 1.51825




ν


e1


= 63.93






r


2


= ∞







d


2


= 2.740






r


3


= ∞







d


3


= 35.000






r


4


= ∞







d


4


= 60.000




n


e4


= 1.51825




ν


e4


= 63.93






r


5


= ∞







d


5


= D5






r


6


= 206.3131







d


6


= 6.508




n


e6


= 1.48915




ν


e6


= 70.04






r


7


= −156.0897







d


7


= 15.114






r


8


= 130.1657







d


8


= 8.000




n


e8


= 1.61639




ν


e8


= 44.15






r


9


= 61.3830







d


9


= 1.693






r


10


= 80.8720







d


10


= 12.000




n


e10


= 1.43985




ν


e10


= 94.53






r


11


= 232.8980







d


11


= D11






r


12


= 672.7620







d


12


= 6.836




n


e12


= 1.61639




ν


e12


= 44.15






r


13


= 82.8549







d


13


= 2.818






r


14


= 110.5678







d


14


= 9.282




n


e14


= 1.43985




ν


e14


= 94.53






r


15


= −65.4332







d


15


= 0.300






r


16


= −67.0268







d


16


= 6.107




n


e16


= 1.61639




ν


e16


= 44.15






r


17


= −156.9702







d


17


= 50.171






r


18


= 160.2358







d


18


= 10.874




n


e18


= 1.43985




ν


e18


= 94.53






r


19


= −98.7058







d


19


= D19






r


20


= 37.4259







d


20


= 5.034




n


e20


= 1.69417




ν


e20


= 30.83






r


21


= 212.9113







d


21


= 0.300






r


22


= 22.9775







d


22


= 8.363




n


e22


= 1.72538




ν


e22


= 34.47






r


23


= 18.2286







d


23


= 1.827






r


24


= 101.2051







d


24


= 2.247




n


e24


= 1.72538




ν


e24


= 34.47






r


25


= 17.6992







d


25


= 2.554






r


26


= ∞ (aperture stop)







d


26


= D26






r


27


= −55.3149







d


27


= 2.589




n


e27


= 1.61669




ν


e27


= 44.02






r


28


= 20.3875







d


28


= 11.136




n


e28


= 1.48915




ν


e28


= 70.04






r


29


= −22.7793







d


29


= 2.967






r


30


= −17.4070







d


30


= 2.255




n


e30


= 1.61639




ν


e30


= 44.15






r


31


= 660.0000







d


31


= 5.164






r


32


= −361.4116







d


32


= 9.280




n


e32


= 1.43985




ν


e32


= 94.53






r


33


= −21.6618







d


33


= 0.300






r


34


= 57.4166







d


34


= 5.104




n


e34


= 1.43985




ν


e34


= 94.53






r


35


= −177.5066







d


35


= 0.350






r


36


= 61.7155







d


36


= 4.849




n


e36


= 1.43985




ν


e36


= 94.53






r


37


= −672.7620







d


37


= D37






r


38


= ∞







d


38


= 33.000




n


e38


= 1.61173




ν


e38


= 46.30






r


39


= ∞







d


39


= 13.200




n


e39


= 1.51825




ν


e39


= 63.93






r


40


= ∞







d


40


= 0.500






r


41


= ∞ (imaging surface)







d


41


= 0.000

























Zoom data















0.3x




0.4x




0.5x




















D5




32.142




28.009




24.962







D11




58.194




27.683




8.473







D19




3.000




39.963




64.634







D26




3.340




5.440




7.048







D37




23.777




19.357




15.336


























Parameters of conditions













Magnification β:















0.3x




0.4x




0.5x


















Entrance pupil position: En




1215.330




17052.978




−1195.682






Object-to-image distance: L




467.675




467.675




467.675






|En|/L




2.599




36.463




2.557






Exit pupil position: Ex




−361.027




−890.944




−13016.681






|Ex|/|L/β|




0.232




0.762




13.916






F-number: FNO




3.500




3.517




3.556












FNO fluctuation: ΔFNO




0.056






|ΔFNO/Δβ|




0.280






Object-side radius of




37.426






curvature: R3f






Image-side radius of




17.699






curvature: R3b






|(R3f + R3b)/(R3f − R3b)|




2.794














Eighth Embodiment





FIGS. 15A

,


15


B, and


15


C show optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of the eighth embodiment of the imaging optical system according to the present invention.

FIGS. 16A

,


16


B, and


16


C show aberration characteristics in focusing at a magnification of 0.4× of the imaging optical system in the eighth embodiment. The imaging optical system of the eighth embodiment has the variable magnification optical system Z.




The variable magnification optical system Z comprises, in order from the object side toward the image side, the first lens unit G


1


with positive refractive power, the second lens unit G


2


with positive refractive power, the third lens unit G


3


with negative refractive power, the aperture stop S, and the fourth lens unit G


4


with positive refractive power.




The first lens unit G


1


includes, in order from the object side, a positive meniscus lens L


1




1


″ with a concave surface directed toward the object side, the negative meniscus lens L


1




2


′ with a concave surface directed toward the object side, and the biconvex lens L


1




3


.




The second lens unit G


2


, in order from the object side, the negative meniscus lens L


2




1


with a convex surface directed toward the object side, the biconvex lens L


2




2


, the negative meniscus lens L


2




3


with a concave surface directed toward the object side, the positive meniscus lens L


2




4


′ with a concave surface directed toward the object side, and a positive meniscus lens L


2




5


with a convex surface directed toward the object side.




The third lens unit G


3


includes a biconvex lens L


3




1


′, the negative meniscus lens L


3




2


with a convex surface directed toward the object side, and the negative meniscus lens L


3




3


with a convex surface directed toward the object side.




The fourth lens unit G


4


includes a negative meniscus lens L


4




1


′ with a convex surface directed toward the object side, a positive meniscus lens L


4




2


′ with a concave surface directed toward the object side, a negative meniscus lens L


4




3


′ with a concave surface directed toward the object side, the positive meniscus lens L


4




4


′ with a concave surface directed toward the object side, the biconvex lens L


4




5


, and a positive meniscus lens L


4




6


′ with a convex surface directed toward the object side. When the magnification is changed from 0.3× to 0.5× in focusing of the infinite object point, the first lens unit G


1


is moved toward the object side, the second lens unit G


2


is moved toward the object side so that the spacing between the first and second lens units G


1


and G


2


is widened, the third lens unit G


3


is moved together with the stop S toward the object side so that the spacing between the second and third lens units G


2


and G


3


is slightly widened, and the fourth lens unit G


4


, after being slightly moved once toward the image side, is slightly moved toward the object side. Also, the object-to-image distance in the magnification change is kept constant.




Subsequently, numerical data of optical members constituting the imaging optical system of the eighth embodiment are shown below.















Numerical data 8






Image height: 5.783


























r


0


= ∞ (object)










d


0


= 51.000






r


1


= ∞ (object surface)







d


1


= 9.260




n


e1


= 1.51825




ν


e1


= 63.93






r


2


= ∞







d


2


= 2.740






r


3


= ∞







d


3


= 35.000






r


4


= ∞







d


4


= 60.000




n


e4


= 1.51825




ν


e4


= 63.93






r


5


= ∞







d


5


= D5






r


6


= −218.393







d


6


= 11.966




n


e6


= 1.48915




ν


e6


= 70.04






r


7


= −59.981







d


7


= 0.724






r


8


= −58.074







d


8


= 8.000




n


e8


= 1.61639




ν


e8


= 44.15






r


9


= −192.015







d


9


= 0.300






r


10


= 453.258







d


10


= 11.399




n


e10


= 1.43985




ν


e10


= 94.53






r


11


= −95.008







d


11


= D11






r


12


= 111.240







d


12


= 6.982




n


e12


= 1.61639




ν


e12


= 44.15






r


13


= 49.021







d


13


= 0.808






r


14


= 52.125







d


14


= 6.307




n


e14


= 1.43985




ν


e14


= 94.53






r


15


= −602.409







d


15


= 3.345






r


16


= −51.702







d


16


= 7.000




n


e16


= 1.61639




ν


e16


= 44.15






r


17


= −123.131







d


17


= 0.300






r


18


= −267.367







d


18


= 5.244




n


e18


= 1.43985




ν


e18


= 94.53






r


19


= −59.230







d


19


= 0.300






r


20


= 62.890







d


20


= 5.562




n


e20


= 1.43985




ν


e20


= 94.53






r


21


= 208.855







d


21


= D21






r


22


= 109.670







d


22


= 4.560




n


e22


= 1.67765




ν


e22


= 31.84






r


23


= −261.555







d


23


= 4.236






r


24


= 27.656







d


24


= 9.660




n


e24


= 1.83945




ν


e24


= 42.47






r


25


= 22.416







d


25


= 3.719






r


26


= 591.785







d


26


= 2.000




n


e26


= 1.83945




ν


e26


= 42.47






r


27


= 32.027







d


27


= 2.504






r


28


= ∞ (aperture stop)







d


28


= D28






r


29


= 235.972







d


29


= 3.058




n


e29


= 1.61639




ν


e29


= 44.15






r


30


= 39.062







d


30


= 3.236






r


31


= −23.495







d


31


= 6.117




n


e31


= 1.43985




ν


e31


= 94.53






r


32


= −17.821







d


32


= 0.300






r


33


= −18.080







d


33


= 4.802




n


e33


= 1.61639




ν


e33


= 44.15






r


34


= −31.126







d


34


= 0.300






r


35


= −67.557







d


35


= 4.329




n


e35


= 1.43985




ν


e35


= 94.53






r


36


= −32.513







d


36


= 0.300






r


37


= 81.623







d


37


= 4.159




n


e37


= 1.43985




ν


e37


= 94.53






r


38


= −357.038







d


38


= 0.484






r


39


= 34.763







d


39


= 5.000




n


e39


= 1.43985




ν


e39


= 94.53






r


40


= 244.020







d


40


= D40






r


41


= ∞







d


41


= 33.000




n


e41


= 1.61173




ν


e41


= 46.30






r


42


= ∞







d


42


= 13.200




n


e42


= 1.51825




ν


e42


= 63.93






r


43


= ∞







d


43


= 0.500






r


44


= ∞ (imaging surface)







d


44


= 0

























Zoom data















0.3x




0.4x




0.5x




















D5




193.324




142.895




90.403







D11




3.000




43.660




80.930







D21




3.160




6.077




8.978







D28




20.516




27.628




34.649







D40




11.289




11.032




16.330


























Parameters of conditions













Magnification β:















0.3x




0.4x




0.5x


















Entrance pupil position: En




89.768




209.179




450.391






Object-to-image distance: L




562.991




562.991




562.991






|En|/L




0.159




0.372




0.800






Exit pupil position: Ex




−355.985




−5834.634




634.502






|Ex|/|L/β|




0.190




4.145




0.564






F-number: FNO




3.500




3.789




4.037












FNO fluctuation: ΔFNO




0.537






|ΔFNO/Δβ|




2.685






Object-side radius of




109.670






curvature: R3f






Image-side radius of




32.027






curvature: R3b






|(R3f + R3b)/(R3f − R3b)|




1.825














Ninth Embodiment





FIGS. 17A

,


17


B, and


17


C show optical arrangements, developed along the optical axis, at magnifications of 0.3×, 0.4×, and 0.5×, respectively, of the ninth embodiment of the imaging optical system according to the present invention.

FIGS. 18A

,


18


B, and


18


C show aberration characteristics in focusing at a magnification of 0.4× of the imaging optical system in the ninth embodiment.




The imaging optical system of the ninth embodiment has the variable magnification optical system Z.




The variable magnification optical system Z comprises, in order from the object side toward the image side, the first lens unit G


1


with positive refractive power, the second lens unit G


2


with positive refractive power, the third lens unit G


3


with negative refractive power, the aperture stop S, and the fourth lens unit G


4


with positive refractive power.




The first lens unit G


1


includes, in order from the object side, the positive meniscus lens L


1




1


″ with a concave surface directed toward the object side, the negative meniscus lens L


1




2


′ with a concave surface directed toward the object side, and a positive meniscus lens L


1




3


″ with a concave surface directed toward the object side.




The second lens unit G


2


, in order from the object side, the negative meniscus lens L


2




1


with a convex surface directed toward the object side, the biconvex lens L


2




2


, the negative meniscus lens L


2




3


with a concave surface directed toward the object side, the biconvex lens L


2




4


, and a biconvex lens L


2




5


′.




The third lens unit G


3


includes the biconvex lens L


3




1


, the negative meniscus lens L


3




2


with a convex surface directed toward the object side, and the negative meniscus lens L


3




3


with a convex surface directed toward the object side.




The fourth lens unit G


4


includes a negative meniscus lens L


4




4


″ with a concave surface directed toward the object side, the positive meniscus lens L


4




2


′ with a concave surface directed toward the object side, the negative meniscus lens L


4




3


′ with a concave surface directed toward the object side, the positive meniscus lens L


4




4


′ with a concave surface directed toward the object side, the biconvex lens L


4




5


, and the biconvex lens L


4




6


.




When the magnification is changed from 0.3× to 0.5× in focusing of the infinite object point, the first lens unit G


1


is moved toward the object side, the second lens unit G


2


is moved toward the object side so that the spacing between the first and second lens units G


1


and G


2


is widened, the third lens unit G


3


is moved together with the stop S toward the object side so that the spacing between the second and third lens units G


2


and G


3


is widened, and the fourth lens unit G


4


, after being slightly moved once toward the image side, is slightly moved toward the object side. Also, the object-to-image distance in the magnification change is kept constant.




Subsequently, numerical data of optical members constituting the imaging optical system of the ninth embodiment are shown below.















Numerical data 9






Image height: 5.783


























r


0


= ∞ (object)










d


0


= 21.000






r


1


= ∞ (object)







d


1


= 26.161






r


2


= ∞ (object surface)







d


2


= D2






r


3


= −153.3010







d


3


= 12.000




n


e3


= 1.48915




ν


e3


= 70.04






r


4


= −56.0044







d


4


= 6.782






r


5


= −42.5771







d


5


= 8.000




n


e5


= 1.61639




ν


e5


= 44.15






r


6


= −173.4981







d


6


= 15.255






r


7


= −454.5776







d


7


= 12.000




n


e7


= 1.43985




ν


e7


= 94.53






r


8


= −54.2450







d


8


= D8






r


9


= 74.1238







d


9


= 7.000




n


e9


= 1.61639




ν


e9


= 44.15






r


10


= 47.9620







d


10


= 0.782






r


11


= 50.6461







d


11


= 6.639




n


e11


= 1.43985




ν


e11


= 94.53






r


12


= −395.4325







d


12


= 2.526






r


13


= −67.4730







d


13


= 6.000




n


e13


= 1.61639




ν


e13


= 44.15






r


14


= −489.0704







d


14


= 0.300






r


15


= 162.7339







d


15


= 5.252




n


e15


= 1.43985




ν


e15


= 94.53






r


16


= −122.6735







d


16


= 0.300






r


17


= 377.7299







d


17


= 4.142




n


e17


= 1.43985




ν


e17


= 94.53






r


18


= −202.1041







d


18


= D18






r


19


= 108.3047







d


19


= 4.106




n


e19


= 1.67765




ν


e19


= 31.84






r


20


= −192.0405







d


20


= 0.454






r


21


= 25.9085







d


21


= 9.623




n


e21


= 1.83945




ν


e21


= 42.47






r


22


= 24.8614







d


22


= 2.939






r


23


= 50.8391







d


23


= 2.000




n


e23


= 1.83945




ν


e23


= 42.47






r


24


= 18.5107







d


24


= 3.223






r


25


= ∞ (aperture stop)







d


25


= D25






r


26


= −23.8975







d


26


= 8.198




n


e26


= 1.61639




ν


e26


= 44.15






r


27


= −142.2318







d


27


= 1.569






r


28


= −27.6769







d


28


= 12.000




n


e28


= 1.43985




ν


e28


= 94.53






r


29


= −15.4629







d


29


= 0.617






r


30


= −15.4255







d


30


= 2.000




n


e30


= 1.61639




ν


e30


= 44.15






r


31


= −31.9175







d


31


= 0.300






r


32


= −193.4359







d


32


= 5.561




n


e32


= 1.43985




ν


e32


= 94.53






r


33


= −30.6965







d


33


= 0.300






r


34


= 190.3831







d


34


= 4.818




n


e34


= 1.43985




ν


e34


= 94.53






r


35


= −61.6979







d


35


= 0.300






r


36


= 63.1906







d


36


= 4.652




n


e36


= 1.43985




ν


e36


= 94.53






r


37


= −264.7349







d


37


= D37






r


38


= ∞







d


38


= 33.000




n


e38


= 1.61173




ν


e38


= 46.30






r


39


= ∞







d


39


= 13.200




n


e39


= 1.51825




ν


e39


= 63.93






r


40


= ∞







d


40


= 0.500






r


41


= ∞ (imaging surface)







d


41


= 0.000

























Zoom data















0.3x




0.4x




0.5x




















D2




131.948




109.433




66.283







D8




3.000




7.576




32.565







D18




3.338




20.375




31.678







D25




6.470




11.057




13.774







D37




16.892




13.207




17.349


























Parameters of conditions













Magnification β:















0.3x




0.4x




0.5x


















Entrance pupil position: En




104.859




165.265




302.380






Object-to-image distance: L




405.147




405.147




405.147






|En|/L




0.259




0.408




0.746






Exit pupil position: Ex




−368.020




2564.601




598.424






|Ex|/|L/β|




0.273




2.532




0.739






F-number: FNO




3.500




3.725




3.839












FNO fluctuation: ΔFNO




0.339






|ΔFNO/Δβ|




1.693






Object-side radius of




108.305






curvature: R3f






Image-side radius of




18.511






curvature: R3b






|(R3f + R3b)/(R3f − R3b)|




1.412














Subsequently, parameter values of the conditions in the above embodiments and whether the arrangements of the embodiments satisfy the requirements of the present invention are summarized in Tables 1 through 3.
















TABLE 1











First




Second




Third







embodiment




embodiment




embodiment





























Object-side tele-




2.71




2.62




2.96







centricity |En|/L (β =







0.3)







Object-side tele-




47.27




38.41




42.84







centricity |En|/L (β =







0.4)







Object-side tele-




2.65




2.66




2.55







centricity |En|/L (β =







0.5)







Image-side tele-




0.25




0.25




0.25







centricity |En|/|L/β|







(β = 0.3)







Image-side tele-




0.54




0.69




0.84







centricity |En|/|L/β|







(β = 0.4)







Image-side tele-




2.12




28.49




5.62







centricity |En|/|L/β|







(β = 0.5)







Conditions (1), (2)






















Conditions (1′), (2′)






















Conditions (1″), (2″)






















Difference between




0.00000




0.00002




0.00000







object-to-image







distances at 0.3× and







0.5×







Smallest object-side




3.5




3.5




3.5







F-number, MAXFNO







|ΔFNO/Δβ|




0.49




0.729




0.935







Conditions (3), (4)






















Conditions (3′), (4′)






















Conditions (3″), (4″)






















Lens arrangement of






















1st lens unit; positive







Lens arrangement of






















1st lens unit; positive,







negative







Lens arrangement of






















1st lens unit; positive,







negative, positive







Virtual shape factor of




2.27




2.69




2.32







3rd lens unit







|(R3f + R3b)/(R3f −







R3b)|







Condition (5)






















Condition (5′)






















Condition (5″)






















3rd lens unit: at least






















two meniscus lenses,







each with a convex







surface directed







toward the object side







3rd lens unit: at least






















three meniscus lenses,







each with a convex







surface directed







toward the object side

















Note:







∘ indicates that the condition is satisfied and x indicates that







the condition is not satisfied.























TABLE 2











Fourth




Fifth




Sixth







embodiment




embodiment




embodiment





























Object-side tele-




2.59




3.06




0.34







centricity |En|/L (β =







0.3)







Object-side tele-




11.97




58.72




0.48







centricity |En|/L (β =







0.4)







Object-side tele-




2.68




2.61




0.80







centricity |En|/L (β =







0.5)







Image-side tele-




0.25




0.26




1.47







centricity |En|/|L/β|







(β = 0.3)







Image-side tele-




0.33




0.35




1.96







centricity |En|/|L/β|







(β = 0.4)







Image-side tele-




0.41




0.43




2.46







centricity |En|/|L/β|







(β = 0.5)







Conditions (1), (2)






















Conditions (1′), (2′)




x




x












Conditions (1″), (2″)




x




x




x







Difference between




0.00000




0.00000




0.00000







object-to-image







distances at 0.3× and







0.5×







Smallest object-side




3.45




3.5




3.5







F-number, MAXFNO







|ΔFNO/Δβ|




0.228




0.002




0.082







Conditions (3), (4)






















Conditions (3′), (4′)






















Conditions (3″), (4″)






















Lens arrangement of






















1st lens unit; positive







Lens arrangement of






















1st lens unit; positive,







negative







Lens arrangement of






















1st lens unit; positive,







negative, positive







Virtual shape factor of




2.34




2.29




2.494







3rd lens unit |(R3f +







R3b)/(R3f − R3b)|







Condition (5)






















Condition (5′)






















Condition (5″)






















3rd lens unit: at least






















two meniscus lenses,







each with a convex







surface directed







toward the object side







3rd lens unit: at least






















three meniscus lenses,







each with a convex







surface directed







toward the object side

















Note:







∘ indicates that the condition is satisfied and x indicates that the







condition is not satisfied.























TABLE 3











Seventh




Eighth




Ninth







embodiment




embodiment




embodiment



























Object-side telecentricity




2.60




0.16




0.26






|En|/L






(β = 0.3)






Object-side telecentricity




36.46




0.37




0.41






|En|/L






(β = 0.4)






Object-side telecentricity




2.56




0.80




0.75






|En|/L






(β = 0.5)






Image-side telecentricity




0.23




0.19




0.27






|En|/L/β|






(β = 0.3)






Image-side telecentricity




0.76




4.15




2.53






|En|/L/β|






(β = 0.4)






Image-side telecentricity




13.92




0.56




0.74






|En|/L/β|






(β = 0.5)






Conditions (1), (2)





















Conditions (1′), (2′)









x




x






Conditions (1′′), (2′′)









x




x






Difference between




0.00000




0.00000




0.00000






object-to-image distances at






0.3x and 0.5x






Smallest object-side




3.51




3.5




3.5






F-number, MAXFNO






|ΔFNO/Δβ|




0.304




2.685




1.693






Conditions (3), (4)





















Conditions (3′), (4′)





















Conditions (3′′), (4′′)









x




x






Lens arrangement of 1st





















lens unit; positive






Lens arrangement of 1st





















lens unit; positive, negative






Lens arrangement of 1st





















lens unit; positive,






negative, positive






Virtual shape factor of 3rd




2.69




1.83




1.41






lens unit






|(R3f + R3b)/(R3f − R3b)|






Condition (5)





















Condition (5′)





















Condition (5′′)









x




x






3rd lens unit: at least two





















meniscus lenses, each with a






convex surface directed






toward the object side






3rd lens unit: at least three









x




x






meniscus lenses, each with a






convex surface directed






toward the object side











Note: O indicates that the condition is satisfied and x indicates that the condition is not satisfied.













The imaging optical system of the present invention described above can be used in an optical apparatus such as a motion picture film scanner (a telecine apparatus) or a height measuring apparatus. Embodiments of such apparatuses are described below.





FIG. 19

shows an embodiment of the telecine apparatus using the imaging optical system of the present invention. This telecine apparatus includes a light source


11


for projecting a motion picture, a motion picture film


14


wound on reels


12


and


13


, an imaging optical system


15


, such as that disclosed by each embodiment in the present invention, and a CCD camera


16


. In the figure, the specific arrangement of the imaging optical system


15


is omitted.




In the telecine apparatus of this embodiment constructed as mentioned above, light emitted from the light source


11


is projected on the motion picture film


14


, and projected light is imaged by the CCD camera


16


through the imaging optical system


15


. In the imaging optical system


15


, the magnification can be changed so that the image information of the motion picture film


14


is imaged over the entire imaging area of the CCD camera


16


in accordance with the size of the motion picture film


14


.




According to the telecine apparatus of the embodiment, the imaging optical system


15


is both-side telecentric so that even when the imaging magnification is changed, the conjugate length remains unchanged. Therefore, there is no need to adjust the positions of individual members. Since the fluctuation of the image-side F-number is minimized and a loss of the amount of light is reduced, the adjustment of brightness is unnecessary. Moreover, a change in magnification on an image plane, caused by the disturbance of flatness of an object to be photographed, such as the film, can be kept to a minimum.





FIG. 20

shows an embodiment of the height measuring apparatus using the imaging optical system of the present invention. In this embodiment, the imaging optical system is used as a confocal optical system.




The height measuring apparatus of the embodiment includes a light source


21


, a polarization beam splitter


22


, a disk


23


provided with a plurality of pinholes, a quarter-wave plate


24


, a confocal optical system


25


constructed like the imaging optical system disclosed by each embodiment in the present invention, an XYZ stage


26


, an imaging lens


27


, an image sensor


28


, a motor


29


driving the disk


23


, a stage driving mechanism


30


driving the XYZ stage


26


, a sensor driving mechanism


31


driving the image sensor


28


, and a computer


32


controlling the drive of the motor


29


, the stage driving mechanism


30


, and the sensor driving mechanism


31


.




In the height measuring apparatus of the embodiment constructed as mentioned above, a p or s component of linear polarization, of light emitted from the light source


21


, is reflected by the polarization beam splitter


22


, passes through the pinhole provided on the disk


23


, and suffers a phase shift of 45° through the quarterwave plate


24


to irradiate a certain point of a specimen


33


placed on the XYZ stage


26


through the confocal optical system


25


. Light reflected by the specimen


33


passes through the confocal optical system


25


, suffers a phase shift of 45° through the quarter-wave plate


24


, passes through the spot on the disk


23


, is transmitted through the polarization beam splitter


22


, and is imaged by the image sensor


28


through the imaging lens


27


. By driving the motor


29


through the computer


32


, the entire surface of the specimen


33


can be scanned. In this case, the position where the intensity of light of a confocal image of the specimen


33


imaged by the image sensor


28


becomes ultimate is found while shifting the driving mechanism


30


or


31


along the optical axis. Whereby, the height of the specimen is detected.




The magnification of the confocal optical system


25


can also be changed in accordance with the size of the specimen


33


.




In this height measuring apparatus also, the confocal optical system


25


is both-side telecentric so that even when the magnification is changed, the conjugate length remains unchanged. Therefore, there is no need to adjust the positions of individual members. Since the fluctuation of the image-side F-number is minimized and a loss of the amount of light is reduced, the adjustment of brightness is unnecessary.



Claims
  • 1. An imaging optical system including a variable magnification optical system, the variable magnification optical system comprising, in order from an object side toward an image side:a first lens unit with positive refractive power; a second lens unit with positive refractive power; a third lens unit with negative refractive power; a fourth lens unit with positive refractive power, and an aperture stop interposed between the third lens unit and the fourth lens unit, wherein the variable magnification optical system changes an imaging magnification while keeping a distance between an object and an image constant in the imaging optical system, the imaging magnification is changed by varying spacing between the first lens unit and the second lens unit, spacing between the second lens unit and the third lens unit, and spacing between the third lens unit and the fourth lens unit, and when the imaging magnification is changed, the imaging optical system satisfies the following conditions in at least one variable magnification state: |En|/L>0.4 |Ex|/|L/β|>0.4  where En is a distance from a first lens surface on the object side of the variable magnification optical system to an entrance pupil of the imaging optical system, L is the distance between the object and the image in the imaging optical system, Ex is a distance from a most image-side lens surface of the variable magnification optical system to an exit pupil of the imaging optical system, and β is a magnification of an entire system of the imaging optical system.
  • 2. An imaging optical system according to claim 1, further satisfying the following conditions: 1.0<MAXFNO<8.0|ΔFNO/Δβ|<5 where MAXFNO is a smallest object-side F-number where the imaging magnification of the imaging optical system is changed, ΔFNO is a difference between the object-side F-number at a minimum magnification and the object-side F-number at a maximum magnification in the entire system of the imaging optical system, and Δβ is a difference between the minimum magnification and the maximum magnification in the entire system of the imaging optical system.
  • 3. An imaging optical system according to claim 1, further satisfying the following condition:0.6<|(R3f+R3b)/(R3f−R3b)|<5.0 where R3f is a radius of curvature of a most object-side surface of the third lens unit and R3b is a radius of curvature of a most image-side surface of the third lens unit.
  • 4. An imaging optical system according to claim 1, wherein a most object-side lens of the first lens unit has positive refractive power.
  • 5. An imaging optical system according to claim 1, wherein the first lens unit includes, in order from the object side, a lens with positive refractive power, a lens with negative refractive power, and a lens with positive refractive power.
  • 6. An imaging optical system according to claim 1, wherein the third lens unit includes at least two meniscus lenses, each with a convex surface directed toward the object side.
  • 7. An imaging optical system according to claim 1, wherein the third lens unit includes two meniscus lenses, each with negative refractive power, and one meniscus lens with positive refractive power.
  • 8. An optical apparatus having an imaging optical system, the imaging optical system including a variable magnification optical system, the variable magnification optical system comprising, in order from an object side toward an image side:a first lens unit with positive refractive power; a second lens unit with positive refractive power; a third lens unit with negative refractive power; a fourth lens unit with positive refractive power, and an aperture stop interposed between the third lens unit and the fourth lens unit, wherein the variable magnification optical system changes an imaging magnification while keeping a distance between an object and an image constant in the imaging optical system, the imaging magnification is changed by varying spacing between the first lens unit and the second lens unit, spacing between the second lens unit and the third lens unit, and spacing between the third lens unit and the fourth lens unit, and when the imaging magnification is changed, the imaging optical system satisfies the following conditions in at least one variable magnification state: |En|/L>0.4 |Ex|/|L/β|>0.4  where En is a distance from a first lens surface on the object side of the variable magnification optical system to an entrance pupil of the imaging optical system, L is the distance between the object and the image in the imaging optical system, Ex is a distance from a most image-side lens surface of the variable magnification optical system to an exit pupil of the imaging optical system, and β is a magnification of an entire system of the imaging optical system.
Priority Claims (1)
Number Date Country Kind
2003-056596 Mar 2003 JP
US Referenced Citations (4)
Number Name Date Kind
5414561 Wakimoto et al. May 1995 A
5825546 Matsui Oct 1998 A
6614539 Shimizu Sep 2003 B1
20040105020 Iwasawa Jun 2004 A1
Non-Patent Literature Citations (1)
Entry
T. Hayashi and Z. Wakimoto, Design of Both Side Telecentric Zoom Lens, Lecture No. 7, Lecture draft collection of Optics Symposium, 17TH, 1992.