CN100504493C - Zoom lens and electronic image pickup apparatus using the same - Google Patents

Zoom lens and electronic image pickup apparatus using the same Download PDF

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Publication number
CN100504493C
CN100504493C CNB2007101534383A CN200710153438A CN100504493C CN 100504493 C CN100504493 C CN 100504493C CN B2007101534383 A CNB2007101534383 A CN B2007101534383A CN 200710153438 A CN200710153438 A CN 200710153438A CN 100504493 C CN100504493 C CN 100504493C
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lens
lens combination
combination
object side
negative
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CN101149466A (en
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左部校之
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Olympus Corp
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Olympus Imaging Corp
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Abstract

The present invention provides zoom lens system and electronic image pickup apparatus using the same. A zoom lens system comprises a first lens unit having a positive refractive power, a second lens unit having a negative refractive power and a third lens unit having a positive refractive power, and during zooming from a wide-angle end to a telephoto end, a space between a first lens (G1)unit and a second lens unit (G2) and a space between the second lens unit (G2) and a third lens unit (G3) are changed, the space between the first lens unit (G1)and the second lens unit (G2) is enlarged in the telephoto end as compared with the wide-angle end, and the space between the second lens unit (G2)and the third lens unit (G3)is narrowed in the telephoto end as compared with the wide-angle end.

Description

Zoom lens and use the electronic image pickup device of this zoom lens
The patent No. that the present invention requires on September 19th, 2006 to submit to is that the Jap.P. of 2006-252569 and the patent No. of submission on October 25th, 2006 are the right of priority of the Jap.P. of 2006-290117, and by reference foregoing is incorporated among the application.
Technical field
The present invention relates to zoom lens and use the electronic image pickup device of this zoom lens.
Background technology
In recent years, replace silver film camera (silver halide film camera), the digital camera that uses ccd image sensor (CCD image sensor) and the such electro-photographic element of CMOS type imageing sensor (CMOS typeimage sensor) to take subject becomes main flow.And then it has plurality of classes with the high-performance type from business in small-sized popular such scope widely.
The user of popular digital camera wishes can both enjoy in various scenes easily whenever and wherever possible to take enjoyment.Therefore, small-sized commodity, particularly be easy to put into the pocket etc. of clothes and bag and portable, thickness direction size the digital camera of thin type be subjected to people and welcome.
On the other hand, the change multiple proportions of the digital camera of compact generally is about 3 times, but further requires to compare in the past the more camera of hypermutation multiple proportions.
As the zoom lens that is easy to keep than the hypermutation multiple proportions, the known zoom lens that following type is arranged: have the 1st lens combination of positive refractive power, the 2nd lens combination of negative refractive power and the 3rd lens combination of positive refractive power from object side.
On the other hand, because the size of thickness direction is mainly determined by the size of lens barrel in the camera size, so in order to realize the slimming of camera, it is effective making the lens barrel slimming.
Recently, mostly be and under the user mode of camera, make lens barrel stretch out, make when carrying in the camera body it to be accommodated in so-called Collapsible lens barrel in the camera body.Therefore, require to have considered the zoom lens of the slimming of the lens barrel when flexible.
Following zoom lens is disclosed in 2005-No. 242116 communiques of TOHKEMY, 2005-No. 326743 communiques of TOHKEMY, 2006-No. 78979 communiques of TOHKEMY and 2005-No. 148420 communiques of TOHKEMY: constitute the 1st lens combination by 2 or 3 lens, the 2nd lens combination is carried out the aberration correction and the miniaturization of the 2nd lens combination thus by carry out the symmetrical beam power configuration of negative lens, positive lens, negative lens successively from object side.
In above-mentioned conventional art, move because make aperture diaphragm (aperture stop) be independent of each lens combination, thus help aberration correction etc., but the structure of lens barrel is complicated.
And in above-mentioned conventional art, in wide-angle side, separately very big distance disposes aperture diaphragm from the 3rd lens combination to object side.Therefore, the light height of the off-axis ray by the 3rd lens combination uprises.Thus, the 3rd lens combination is whole maximizes.
And, when the 1st lens combination is 3 lens, be unfavorable for the radially miniaturization of the thickness when flexible of zoom lens.
And the face of the object side of the 2nd lens combination is that convex surface is towards object side.Under the situation of this structure, the thickness thickening of the 2nd lens combination self even make the 1st lens combination near the 2nd lens combination, also causes interference easily, miniaturization and hypermutation multiple proportionsization when being unfavorable for stretching.
And, because keep off the 2nd lens combination in wide-angle side the 1st lens combination, so in order to ensure the visual angle, the radially increase of the 1st lens combination.The 1st lens combination is made of 3 lens and then more is unfavorable for miniaturization.
Summary of the invention
One object of the present invention is to provide a kind of zoom lens, helps the miniaturization of the 3rd lens combination, simultaneously by research the 1st lens combination and the 2nd lens combination, the miniaturization when being easy to stretch, guarantees visual angle and optical property.
Another object of the present invention is to provide a kind of zoom lens, reduce the lens number of the 1st lens combination and the 2nd lens combination, reduce the thickness of the 2nd lens combination, thereby be easy to reduce the distance with the 1st lens combination, guarantee miniaturization and become multiple proportions, be easy to guarantee optical property simultaneously.
Another purpose of the present invention is to provide a kind of zoom lens, by studying each lens combination etc., is easier to guarantee miniaturization, aberration performance and becomes multiple proportions.
Another purpose of the present invention is to provide the electronic image pickup device that is easy to realize miniaturization with this zoom lens.
In the 1st side, zoom lens of the present invention has successively from object side: the 1st lens combination of positive refractive power; The 2nd lens combination of negative refractive power; And the 3rd lens combination of positive refractive power,
From wide-angle side when telescope end becomes times,
Interval between interval between described the 1st lens combination and described the 2nd lens combination and described the 2nd lens combination and described the 3rd lens combination changes,
With respect to wide-angle side, the interval between described the 1st lens combination and described the 2nd lens combination broadens at telescope end,
With respect to wide-angle side, the interval between described the 2nd lens combination and described the 3rd lens combination narrows down at telescope end,
Described zoom lens has when described change times and the constant aperture diaphragm of relative position of described the 3rd lens combination,
Described the 1st lens combination has positive lens, and the total lens number in described the 1st lens combination is below 2,
Described the 2nd lens combination has successively from object side: at the object side negative lens that has concave surface as side, positive lens and picture side negative lens, the total lens number in described the 2nd lens combination is 3,
Described object side negative lens in described the 2nd lens combination and described positive lens dispose across the airspace on optical axis,
The described zoom lens formula that meets the following conditions:
—1.70<R 2n1r/f 2<—0.70 (1A)
Wherein, R 2n1rBe the paraxial radius-of-curvature of the picture side of the object side negative lens in the 2nd lens combination, f 2It is the focal length of the 2nd lens combination.
And electronic image pickup device of the present invention has: zoom lens of the present invention; And the electro-photographic element, it is configured in the picture side of described zoom lens, will be converted to electric signal by the optical image that described zoom lens forms.
With the claim of being added, other features and advantages of the present invention will become obvious in the embodiment of following detailed description in conjunction with the accompanying drawings.
Description of drawings
The present invention can become clearer and more definite from following detailed description that provides and accompanying drawing, but just provides with the form of example, can not limit the present invention.
Figure 1A～1C is the sectional view of the infintie object point that comprises the embodiment 1 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 1A is the sectional view of wide-angle side, Figure 1B is the sectional view of intermediateness, and Fig. 1 C is the sectional view of telescope end.
Fig. 2 A～2C is the sectional view of the infintie object point that comprises the embodiment 2 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Fig. 2 A is the sectional view of wide-angle side, Fig. 2 B is the sectional view of intermediateness, and Fig. 2 C is the sectional view of telescope end.
Fig. 3 A～3C is the sectional view of the infintie object point that comprises the embodiment 3 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Fig. 3 A is the sectional view of wide-angle side, Fig. 3 B is the sectional view of intermediateness, and Fig. 3 C is the sectional view of telescope end.
Fig. 4 A～4C is the sectional view of the infintie object point that comprises the embodiment 4 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Fig. 4 A is the sectional view of wide-angle side, Fig. 4 B is the sectional view of intermediateness, and Fig. 4 C is the sectional view of telescope end.
Fig. 5 A～5C is the sectional view of the infintie object point that comprises the embodiment 5 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Fig. 5 A is the sectional view of wide-angle side, Fig. 5 B is the sectional view of intermediateness, and Fig. 5 C is the sectional view of telescope end.
Fig. 6 A～6C is the sectional view of the infintie object point that comprises the embodiment 6 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Fig. 6 A is the sectional view of wide-angle side, Fig. 6 B is the sectional view of intermediateness, and Fig. 6 C is the sectional view of telescope end.
Fig. 7 A～7C is the sectional view of the infintie object point that comprises the embodiment 7 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Fig. 7 A is the sectional view of wide-angle side, Fig. 7 B is the sectional view of intermediateness, and Fig. 7 C is the sectional view of telescope end.
Fig. 8 A～8C is the sectional view of the infintie object point that comprises the embodiment 8 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Fig. 8 A is the sectional view of wide-angle side, Fig. 8 B is the sectional view of intermediateness, and Fig. 8 C is the sectional view of telescope end.
Fig. 9 A～9C is the sectional view of the infintie object point that comprises the embodiment 9 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Fig. 9 A is the sectional view of wide-angle side, Fig. 9 B is the sectional view of intermediateness, and Fig. 9 C is the sectional view of telescope end.
Figure 10 A～10C is the sectional view of the infintie object point that comprises the embodiment 10 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 10 A is the sectional view of wide-angle side, Figure 10 B is the sectional view of intermediateness, and Figure 10 C is the sectional view of telescope end.
Figure 11 A～11C is the sectional view of the infintie object point that comprises the embodiment 11 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 11 A is the sectional view of wide-angle side, Figure 11 B is the sectional view of intermediateness, and Figure 11 C is the sectional view of telescope end.
Figure 12 A～12C is the sectional view of the infintie object point that comprises the embodiment 12 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 12 A is the sectional view of wide-angle side, Figure 12 B is the sectional view of intermediateness, and Figure 12 C is the sectional view of telescope end.
Figure 13 A～13C is the sectional view of the infintie object point that comprises the embodiment 13 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 13 A is the sectional view of wide-angle side, Figure 13 B is the sectional view of intermediateness, and Figure 13 C is the sectional view of telescope end.
Figure 14 A～14C is the sectional view of the infintie object point that comprises the embodiment 14 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 14 A is the sectional view of wide-angle side, Figure 14 B is the sectional view of intermediateness, and Figure 14 C is the sectional view of telescope end.
Figure 15 A～15C is the sectional view of the infintie object point that comprises the embodiment 15 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 15 A is the sectional view of wide-angle side, Figure 15 B is the sectional view of intermediateness, and Figure 15 C is the sectional view of telescope end.
Figure 16 A～16C is the sectional view of the infintie object point that comprises the embodiment 16 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 16 A is the sectional view of wide-angle side, Figure 16 B is the sectional view of intermediateness, and Figure 16 C is the sectional view of telescope end.
Figure 17 A～17C is the sectional view of the infintie object point that comprises the embodiment 17 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 17 A is the sectional view of wide-angle side, Figure 17 B is the sectional view of intermediateness, and Figure 17 C is the sectional view of telescope end.
Figure 18 A～18C is the sectional view of the infintie object point that comprises the embodiment 18 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 18 A is the sectional view of wide-angle side, Figure 18 B is the sectional view of intermediateness, and Figure 18 C is the sectional view of telescope end.
Figure 19 A～19C is the sectional view of the infintie object point that comprises the embodiment 19 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 19 A is the sectional view of wide-angle side, Figure 19 B is the sectional view of intermediateness, and Figure 19 C is the sectional view of telescope end.
Figure 20 A～20C is the sectional view of the infintie object point that comprises the embodiment 20 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 20 A is the sectional view of wide-angle side, Figure 20 B is the sectional view of intermediateness, and Figure 20 C is the sectional view of telescope end.
Figure 21 A～21C is the sectional view of the infintie object point that comprises the embodiment 21 of the zoom lens of the present invention optical axis of (focused at infinity) when focusing on, Figure 21 A is the sectional view of wide-angle side, Figure 21 B is the sectional view of intermediateness, and Figure 21 C is the sectional view of telescope end.
Figure 22 A～22C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 1 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 22 A represents the state of wide-angle side, Figure 22 B represents the state of intermediateness, and Figure 22 C represents the state of telescope end.
Figure 23 A～23C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 2 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 23 A represents the state of wide-angle side, Figure 23 B represents the state of intermediateness, and Figure 23 C represents the state of telescope end.
Figure 24 A～24C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 3 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 24 A represents the state of wide-angle side, Figure 24 B represents the state of intermediateness, and Figure 24 C represents the state of telescope end.
Figure 25 A～25C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 4 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 25 A represents the state of wide-angle side, Figure 25 B represents the state of intermediateness, and Figure 25 C represents the state of telescope end.
Figure 26 A～26C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 5 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 26 A represents the state of wide-angle side, Figure 26 B represents the state of intermediateness, and Figure 26 C represents the state of telescope end.
Figure 27 A～27C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 6 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 27 A represents the state of wide-angle side, Figure 27 B represents the state of intermediateness, and Figure 27 C represents the state of telescope end.
Figure 28 A～28C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 7 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 28 A represents the state of wide-angle side, Figure 28 B represents the state of intermediateness, and Figure 28 C represents the state of telescope end.
Figure 29 A～29C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 8 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 29 A represents the state of wide-angle side, Figure 29 B represents the state of intermediateness, and Figure 29 C represents the state of telescope end.
Figure 30 A～30C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 9 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 30 A represents the state of wide-angle side, Figure 30 B represents the state of intermediateness, and Figure 30 C represents the state of telescope end.
Figure 31 A～31C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 10 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 31 A represents the state of wide-angle side, Figure 31 B represents the state of intermediateness, and Figure 31 C represents the state of telescope end.
Figure 32 A～32C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 11 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 32 A represents the state of wide-angle side, Figure 32 B represents the state of intermediateness, and Figure 32 C represents the state of telescope end.
Figure 33 A～33C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 12 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 33 A represents the state of wide-angle side, Figure 33 B represents the state of intermediateness, and Figure 33 C represents the state of telescope end.
Figure 34 A～34C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 13 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 34 A represents the state of wide-angle side, Figure 34 B represents the state of intermediateness, and Figure 34 C represents the state of telescope end.
Figure 35 A～35C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 14 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 35 A represents the state of wide-angle side, Figure 35 B represents the state of intermediateness, and Figure 35 C represents the state of telescope end.
Figure 36 A～36C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 15 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 36 A represents the state of wide-angle side, Figure 36 B represents the state of intermediateness, and Figure 36 C represents the state of telescope end.
Figure 37 A～37C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 16 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 37 A represents the state of wide-angle side, Figure 37 B represents the state of intermediateness, and Figure 37 C represents the state of telescope end.
Figure 38 A～38C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 17 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 38 A represents the state of wide-angle side, Figure 38 B represents the state of intermediateness, and Figure 38 C represents the state of telescope end.
Figure 39 A～39C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 18 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 39 A represents the state of wide-angle side, Figure 39 B represents the state of intermediateness, and Figure 39 C represents the state of telescope end.
Figure 40 A～40C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 19 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 40 A represents the state of wide-angle side, Figure 40 B represents the state of intermediateness, and Figure 40 C represents the state of telescope end.
Figure 41 A～41C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 20 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 41 A represents the state of wide-angle side, Figure 41 B represents the state of intermediateness, and Figure 41 C represents the state of telescope end.
Figure 42 A～42C is the aberration diagram of the spherical aberration (SA) of the infintie object point of the embodiment 21 of expression zoom lens of the present invention when focusing on, astigmatism (FC), distortion aberration (DT), ratio chromatism, (CC), Figure 42 A represents the state of wide-angle side, Figure 42 B represents the state of intermediateness, and Figure 42 C represents the state of telescope end.
Figure 43 is the figure that is used to illustrate the definition of aspheric surface departure.
Figure 44 is the figure of the key concept when being used to illustrate the distortion that electricity proofreaies and correct picture.
Figure 45 is the figure that is used to illustrate the implication of subject half angle of view.
Figure 46 is the place ahead stereographic map of outward appearance of the embodiment of expression digital camera of the present invention.
Figure 47 is the rear view of the digital camera of Figure 46.
Figure 48 is the figure of inner structure that schematically shows the digital camera of Figure 46.
Figure 49 is the block diagram of major part of internal circuit of the digital camera of Figure 46.
Embodiment
As mentioned above, in the 1st side, zoom lens of the present invention has successively from object side: the 1st lens combination of positive refractive power; The 2nd lens combination of negative refractive power; And the 3rd lens combination of positive refractive power,
From wide-angle side when telescope end becomes times,
Interval between interval between described the 1st lens combination and described the 2nd lens combination and described the 2nd lens combination and described the 3rd lens combination changes,
With respect to wide-angle side, the interval between described the 1st lens combination and described the 2nd lens combination broadens at telescope end,
With respect to wide-angle side, the interval between described the 2nd lens combination and described the 3rd lens combination narrows down at telescope end,
Described zoom lens has when described change times and the constant aperture diaphragm of relative position of described the 3rd lens combination,
Described the 1st lens combination has positive lens, and the total lens number in described the 1st lens combination is below 2,
Described the 2nd lens combination has successively from object side: at the object side negative lens that has concave surface as side, positive lens and picture side negative lens, the total lens number in described the 2nd lens combination is 3,
Described object side negative lens in described the 2nd lens combination and described positive lens dispose across the airspace on optical axis,
The described zoom lens formula that meets the following conditions:
—1.70<R 2n1r/f 2<—0.70 (1A)
Wherein, R 2n1rBe the paraxial radius-of-curvature of the picture side of the object side negative lens in the 2nd lens combination, f 2It is the focal length of the 2nd lens combination.
In the 1st side, zoom lens constitutes, and has successively from object side: the 1st lens combination of positive refractive power; The 2nd lens combination of negative refractive power; And the 3rd lens combination of positive refractive power, from wide-angle side when telescope end becomes times, interval between described the 1st lens combination and described the 2nd lens combination and the interval between described the 2nd lens combination and described the 3rd lens combination are changed, with respect to wide-angle side, interval between described the 1st lens combination and described the 2nd lens combination broadens at telescope end, with respect to wide-angle side, the interval between described the 2nd lens combination and described the 3rd lens combination narrows down at telescope end.
By adopting this structure, the 2nd lens combination and the 3rd lens combination are effectively shared become burden doubly, guarantee to become multiple proportions, and the aberration change that is easy to when becoming times suppresses lessly.
And the 1st lens combination is made of the lens below 2, and the 2nd lens combination is made of 3 lens, by such utilization seldom the lens of sheet number constitute, be easy to suppress the thickness of zoom lens when flexible.And, also be easy to reduce wide-angle side from the object side of the 1st lens combination the distance to entrance pupil, and be easy to carry out the miniaturization of the radial dimension of zoom lens.
And 2 negative lenses of configuration are shared the negative power of the 2nd lens combination, thereby are easy to suppress aberration in the 2nd lens combination.And by have the such configuration of negative lens, positive lens and negative lens successively from object side, the symmetry of lens arrangement is good, becomes the structure that can efficiently carry out aberration correction in the 2nd lens combination.
And above-mentioned zoom lens has aperture diaphragm, and the 3rd lens combination concerns constant with the position of aperture diaphragm when becoming times.Thus, prevent that the light height of the off-axis ray by the 3rd lens combination from uprising, be easy to suppress the radial dimension and the axle wall thickness of the 3rd lens combination less, help miniaturization.And, even guarantee refractive power in the 3rd lens combination, the aberration change when also being easy to suppress to become times.
When disposing aperture diaphragm like this, meet the following conditions (1A), be easier to carry out miniaturization and these both sides of aberration balancing by making the 2nd lens combination.
—1.70<R 2n1r/f 2<—0.70 (1A)
Wherein, R 2n1rBe the paraxial radius-of-curvature of the picture side of the object side negative lens in the 2nd lens combination, f 2It is the focal length of the 2nd lens combination.
The paraxial radius-of-curvature of the picture side of the object side negative lens in condition (1A) restriction the 2nd lens combination.R 2n1r/ f 2The upper limit-0.70 that is not higher than condition (1A) helps reducing the curvature (increase radius-of-curvature) of picture side concave surface of negative lens of the object side of the 2nd lens combination, and suppresses the refraction angle of the off-axis ray on this face.Thus, being particularly conducive to the outer coma of axle that is reduced in wide-angle side produces.
And, by reducing the curvature of this concave surface, can reduce to be easy to increase the sag (sag) of this concave surface of curvature, also be easy to suppress the thickness of the 2nd lens combination.Miniaturization when thus, helping stretching.
R 2n1r/ f 2Be not less than lower limit-1.70, guarantee the curvature of the picture side concave surface of object side negative lens by appropriateness, and the appropriate effect of guaranteeing to make the off-axis ray refraction, in wide-angle side, can be suppressed at respect to off-axis ray under the very big state of the angle of optical axis by in the 2nd lens combination.Aberration change when thus, being easy to suppress to become times.
And then the 3rd lens combination of preferred zoom lens is below 3 to the lens number as side.
By this structure, the slimming when helping stretching and the simplification of Zoom lens structure.
If zoom lens is constituted as 3 groups of zoom lens, then can simplify the mechanism that lens are moved.
Zoom lens is constituted as 4 groups of zoom lens, and establish the 4th lens combination when being positive refractive power, preferably make the 4th lens combination have function away from exit pupil.And, if for to make the 4th lens combination move the structure of focusing, the visual angle change when then being easy to suppress to focus.If utilize a slice positive lens to constitute the 4th lens combination, the miniaturization when then also helping stretching etc.
And, zoom lens is constituted as 5 groups of zoom lens, and to establish the 4th lens combination be negative refractive power, establish the 5th lens combination when being positive refractive power, as the power configuration symmetry of the lens combination of zoom lens integral body, the change of astigmatism is preferred when being easy to suppress to become times.
The 2nd lens combination meet the following conditions (2A), (3A), miniaturization and aberration balancing better aspect be preferred.
0<SF 2n1<1.25 (2A)
—0.32<f 2/R 2pf<0.5 (3A)
Wherein, SF 2n1By SF 2n1=(R 2n1f+ R 2n1r)/(R 2n1f-R 2n1r) define R 2n1fBe the paraxial radius-of-curvature of the object side of the object side negative lens in the 2nd lens combination, R 2n1rBe the paraxial radius-of-curvature of the picture side of the object side negative lens in the 2nd lens combination, R 2pfIt is the paraxial radius-of-curvature of the object side of the positive lens in the 2nd lens combination.
Condition (2A) be used to guarantee the 2nd lens combination the object side negative lens focal power and in miniaturization with guarantee the condition that averages out between the performance.
By making SF 2n1Be not higher than the upper limit 1.25 of condition (2A),, be easy to guarantee the negative power of negative lens yet even reduce the curvature of picture side.Thus, be easy to reduce the front and back variable quantity at interval of the 2nd lens combination, also help the miniaturization of lens picture frame.And, be easy to guarantee to make the effect of light refraction in the object side, reduce the light height of the 1st lens combination, help miniaturization radially.And, be easy to reduce the thickness of the 2nd lens combination on optical axis.
SF 2n1Be not less than the lower limit 0 of condition (2A), help having very strong negative power to suppress, and be suppressed at the curvature of the image and the distortion aberration of wide-angle side the mask of object side.
And when satisfying condition (1A), the generation of the aberration of the picture side of the negative lens of object side reduces.Thus, the positive lens about the 2nd lens combination, satisfy condition (3A) helps more suitably carrying out the balance of aberration.
By making f 2/ R 2pfBe not less than the lower limit-0.32 of condition (3A), can become very strong positive light coke by the mortifier body side surface, help the 2nd lens combination negative power guarantee correction with coma.
f 2/ R 2pfWhen not being higher than the upper limit 0.5 of condition (3A), guarantee the focal power of positive lens, can guarantee to proofread and correct the function of the aberration that object side and picture side negative lens produce, be easy to suppress coma and spherical aberration by appropriateness.
In addition, when condition (1A) is as described below, further preferred.
—1.30<R 2n1r/f 2<—0.74 (1A)’
When meeting the following conditions, be more preferably.
—0.85<R 2n1r/f 2<—0.78 (1A)”
When condition (2A) is as described below, further preferred.
0.35<SF 2n1<1.15 (2A)’
When meeting the following conditions, be more preferably.
0.70<SF 2n1<1.05 (2A)”
When condition (3A) is as described below, further preferred.
—0.21<f 2/R 2pf<0.3 (3A)’
When meeting the following conditions, be more preferably.
—0.1<f 2/R 2pf<0.1 (3A)”
Also can only limit the lower limit of above-mentioned condition or only limit higher limit.Each condition later on too.
The positive lens of the 2nd lens combination preferably meet the following conditions (4A), (5A).This is the refractive index condition relevant with Abbe number with the positive lens of the 2nd lens combination.
1.84<n d2p<2.20 (4A)
13.0<v d2p<30.0 (5A)
Wherein, n D2pBe the refractive index of the positive lens of the 2nd lens combination with respect to the d line, v D2pIt is the Abbe number of the positive lens of the 2nd lens combination.
By making n D2pThe upper limit 2.20 that is not higher than condition (4A), the production of material and acquired good is beneficial to and reduces cost.
By making n D2pBe not less than the lower limit 1.84 of condition (4A),, also can reduce the curvature absolute value of lens face, be easy to suppress the generation of spherical aberration and coma even guarantee focal power.
Condition (5A) is with chromatic aberration correction, particularly proofreaies and correct relevant condition with axle ratio chromatism, outward.In order in this lens combination, to proofread and correct the aberration that produces by big negative power well, preferably in suitable scope, positive lens is used the bigger material of dispersivity (color dispersion).
v D2pThe upper limit 30.0 that is not higher than condition (5A) helps guaranteeing disperseing, and proofreaies and correct the aberration that negative lens produces.
v D2pBe not less than the lower limit 13.0 of condition (5A), help suppressing the chromatic dispersion of short wavelength side, suppress the aberration of the short wavelength side of this positive lens generation, suppress the generation of side spectrum.
Further preferred when as described below.
1.87<n d2p<2.15 (4A)’
15.0<v d2p<26.0 (5A)’
Be more preferably when as described below.
1.90<n d2p<2.12 (4A)”
17.0<v d2p<21.0 (5A)”
In order further to reduce the generation of the aberration in the 2nd lens combination, when the shape that is set at the positive lens of the 2nd lens combination satisfies following conditional, be more preferably.
0.45<SF 2p<1.80 (6A)
Wherein, SF 2pBy SF 2p=(R 2pf+ R 2pr)/(R 2pf-R 2pr) define R 2pfBe the paraxial radius-of-curvature of the object side of the positive lens in the 2nd lens combination, R 2prIt is the paraxial radius-of-curvature of the picture side of the positive lens in the 2nd lens combination.
By making SF 2pBe no more than the upper limit 1.80 and the lower limit 0.45 of condition (6A), be easy to the generation that balance suppresses spherical aberration and coma well.
Further preferred when as described below.
0.55<SF 2p<1.6 (6A)’
Be more preferably when meeting the following conditions.
0.6<SF 2p<1.3 (6A)”
The material of the negative lens of the object side of the 2nd lens combination preferably meets the following conditions.
1.78<n d2n1<2.20 (7A)
35<v d2n1<50 (8A)
Wherein, n D2n1Be the refractive index of the object side negative lens of the 2nd lens combination with respect to the d line, v D2n1It is the Abbe number of the object side negative lens of the 2nd lens combination.
By making n D2n1The upper limit 2.20 that is not higher than condition (7A), the production of material and acquired good helps reducing cost.n D2n1When being not less than the lower limit 1.78 of condition (7A), reduce the curvature absolute value of lens face when guaranteeing refractive power, be easy to suppress coma and curvature of the image in wide-angle side.
v D2n1When not being higher than the upper limit 50 of condition (8A), help guaranteeing material acquired of high index of refraction.v D2n1When being not less than the lower limit 35 of condition (8A), appropriateness suppresses chromatic dispersion, helps suppressing aberration.
Further preferred when as described below.
1.79<n d2n1<1.95 (7A)’
37<v d2n1<47 (8A)’
Be more preferably when meeting the following conditions.
1.80<n d2n1<1.90 (7A)”
40<v d2n1<43 (8A)”
About the 2nd lens combination as the negative lens of side, also can preestablish optimal material.Particularly, preferably meet the following conditions.
1.78<n d2n2<2.00 (9A)
35<v d2n2<50 (10A)
Wherein, n D2n2Be the refractive index of the picture side negative lens of the 2nd lens combination with respect to the d line, v D2n2It is the Abbe number of the picture side negative lens of the 2nd lens combination.
n D2n2When not being higher than the upper limit 2.00 of condition (9A), the production of material and acquired good helps reducing cost.n D2n2When being not less than the lower limit 1.78 of condition (9A),, also can reduce the curvature absolute value of lens face, be easy to suppress the generation of spherical aberration and coma even guarantee refractive power.
v D2n2When not being higher than the upper limit 50 of condition (10A), help improving the acquired of the high material of refractive index.By making v D2n2Be not less than the lower limit 35 of condition (10A), suppress chromatic dispersion, help correcting chromatic aberration.
Further preferred when as described below.
1.79<n d2n2<1.95 (9A)’
38<v d2n2<48 (10A)’
Be more preferably when meeting the following conditions.
1.80<n d2n2<1.90 (9A)”
40<v d2n2<47 (10A)”
Shape about this negative lens preferably meets the following conditions.
—3.0<SF 2n2<—0.6 (11A)
Wherein, SF 2n2By SF 2n2=(R 2n2f+ R 2n2r)/(R 2n2f-R 2n2r) define R 2n2F is the paraxial radius-of-curvature of the object side of the picture side negative lens in the 2nd lens combination, R 2n2rIt is the paraxial radius-of-curvature of the picture side of the picture side negative lens in the 2nd lens combination.
SF 2n2The upper limit-0.6 o'clock that is not higher than condition (11A) helps suppressing the undercorrection of curvature of the image.Be not less than lower limit-3.0 o'clock, appropriateness reduces the curvature absolute value of two lens faces, is easy to suppress the generation of spherical aberration and coma.
Further preferred when as described below.
—2.6<SF 2n2<—0.9 (11A)’
Be more preferably when meeting the following conditions.
—2.1<SF 2n2<—1.1 (11A)”
And in order to carry out good aberration correction, the positive lens of the 2nd lens combination preferably meets the following conditions.
—3.0<f 2p/f 2<—1.0 (12A)
Wherein, f 2pIt is the focal length of the positive lens of the 2nd lens combination.
f 2p/ f 2The upper limit-1.0 o'clock that is not higher than condition (12A) suppresses the focal power of positive lens by appropriateness, is easy to suppress the undercorrection of curvature of the image.Be not less than lower limit-3.0 o'clock, guarantee the focal power of positive lens, help proofreading and correct spherical aberration and coma that the negative lens of the 2nd lens combination produces by appropriateness.In any case, surpass bound and all be difficult to guarantee the good optical performance.
Further preferred when as described below.
—2.8<f 2p/f 2<—1.4 (12A)’
Be more preferably when meeting the following conditions.
—2.6<f 2p/f 2<—1.8 (12A)”
And, for the generation that further suppresses aberration and obtain the good optical performance, also can be at least one lens face configuration aspheric surface in the object side negative lens of the 2nd lens combination.And, also can dispose aspheric surface on the two sides.To proofreading and correct coma and curvature of the image is effective.
At this moment, preferably meet the following conditions.
0.002<(ASP 2n1f+|ASP 2n1r|)/f w<0.10 (13A)
—0.06<(ASP 2n1r—ASP 2n1f)/f w<0.06 (13B)
Wherein, ASP 2n1fBe the aspheric surface departure (aspherical displacement) of lens face of object side of the object side negative lens of the 2nd lens combination, ASP 2n1rBe the aspheric surface departure of lens face of picture side of the object side negative lens of the 2nd lens combination, f wFocal length for the zoom lens of wide-angle side.Here, aspheric surface departure ASP as shown in figure 43, at the sphere that will have the vertex of surface identical and have a radius-of-curvature identical during as benchmark sphere RS with the paraxial radius of curvature R of this lens face with the summit P of lens face LS, on the position of the maximum light height of incidence Yw of the wide-angle side in this lens face, be distance when measuring, will be made as plus sign in the situation that picture side direction (right among the figure) is measured from the benchmark sphere to this lens face with optical axis L c parallel direction.Aspheric surface departure when lens face is sphere or plane is 0.
By making (ASP 2n1f+ | ASP 2n1r|)/f wBe not less than the lower limit 0.002 of condition (13A), be easy to guarantee aspheric aberration correction effect, be easy to the barrel distortion aberration (barreltype distortion) that suppresses superfluous.By making it not be higher than the upper limit 0.10, can suppress the degree of aspheric change of shape, be easy to suppress the harmful effect of decectration aberration and superfluous coma are proofreaied and correct.
By making (ASP 2n1r-ASP 2n1f)/f wThe upper limit 0.06 that is not higher than condition (13B) is easy to suppress the correction surplus of curvature of the image.By making it be not less than lower limit-0.06, be easy to suppress the undercorrection of curvature of the image.All be effective to obtaining the good optical performance in any case.
Further preferred when as described below.
—0.059<(ASP 2n1r—ASP 2n1f)/f w<0.04 (13B)’
Be more preferably when meeting the following conditions.
—0.055<(ASP 2n1r—ASP 2n1f)/f w<0.015 (13B)”
And then, the aspheric surface that the object side of the object side negative lens of the 2nd lens combination also can increase along with the increase with optical axis distance for refractive power.
In addition, the refractive power increase means that negative refractive power reduces or positive refractive power increases.
By such shape, help proofreading and correct the off-axis aberration of wide-angle side.
And then, the object side negative lens of preferred the 2nd lens combination is a double-concave negative lens, the object side of double-concave negative lens is the aspheric surface that negative refractive power reduces along with the increase with optical axis distance, double-concave negative lens be the aspheric surface (embodiment 1～10) that negative refractive power increases along with the increase with optical axis distance as the side.
By such shape, when guaranteeing the negative power of core, peripheral part of lens, help proofreading and correct the outer coma of axle of wide-angle side, help guaranteeing of visual angle.And, also help the slimming of the 2nd lens combination integral body.
The 2nd lens combination as the negative lens of side be aspheric surface as the side time, be effective to the correction of spherical aberration and coma.At this moment, preferably meet the following conditions.
—0.09<(ASP 2n2r—ASP 2n2f)/f w<—0.003 (14A)
Wherein, ASP 2n2fBe the aspheric surface departure of lens face of object side of the picture side negative lens of the 2nd lens combination, ASP 2n2rBe the aspheric surface departure of lens face of picture side of the picture side negative lens of the 2nd lens combination, f wFocal length for the zoom lens total system of wide-angle side.Aspheric surface departure when lens face is sphere or plane is 0.
(ASP 2n2r-ASP 2n2f)/f wThe upper limit-0.003 o'clock that is not higher than condition (14A) is easy to suppress the correction surplus of curvature of the image.Be not less than lower limit-0.09 o'clock, help correcting spherical aberration and coma.All be effective to obtaining the good optical performance in any case.
Further preferred when as described below.
—0.07<(ASP 2n2r—ASP 2n2f)/f w<—0.005 (14A)’
Be more preferably when meeting the following conditions.
—0.05<(ASP 2n2r—ASP 2n2f)/f w<—0.015 (14A)”
And then, preferred the 2nd lens combination be convex surface towards the negative meniscus lens of picture side as the side negative lens, the face as side of negative meniscus lens is the aspheric surface that positive refractive power strengthens along with the increase with optical axis distance.
By this structure, help carrying out well the spherical aberration of the 2nd lens combination and the correction of outer each aberration of axle.
The positive lens of the 2nd lens combination and also can also can engaging as the negative lens of side for not engaging simple lens independent of each other.Utilize the degree of freedom of aberration correction of air surface of contact big when not engaging.On the other hand, help chromatic aberration correction during joint, and, can relax the qualification rate that causes because of eccentric relatively optical performance degradation and worsen, relate to the reduction of cost.
And the 1st lens combination has positive lens and negative lens, is preferred aspect aberration.
Especially, the 1st lens combination also can be arranged in order negative lens and positive lens from object side.Like this, when considering the total of the 1st lens combination and the 2nd lens combination, become the good structure of symmetry that is followed successively by negative lens, positive lens, negative lens, positive lens and negative lens from object side.Particularly can effectively eliminate the aberration of synthetic lens combination (the composite lens system) generation that constitutes by the 1st lens combination and the 2nd lens combination in wide-angle side.And, because the rear side principal point position of the 1st lens combination is near the picture side, so effectively guarantee to become multiple proportions.
The negative lens of the 1st lens combination and positive lens utilization do not engage and lens composition independent of each other when constituting, and utilize the air lens that form between two lens, can proofread and correct the coma of telescope end especially well.
At this moment, the interval between two lens preferably meets the following conditions.
0.0≤L 1np/L 1<0.2 (15A)
Wherein, L 1npBe the negative lens and the interval of positive lens on optical axis of the 1st lens combination, L 1It is the gross thickness on the optical axis of the 1st lens combination.
L 1np/ L 1When surpassing the upper limit 0.2 of condition (15A), the off-axis ray height of the lens by object side uprises, and the lens effective diameter increases, and is difficult to realize miniaturization radially.Can not surpass lower limit 0.0.
Further preferred when as described below.
0.0≤L 1np/L 1<0.16 (15A)’
Be more preferably when meeting the following conditions.
0.0≤L 1np/L 1<0.12 (15A)”
And the negative lens of the 1st lens combination and positive lens also can engage.Can proofread and correct the ratio chromatism, of wide-angle side and the axle of telescope end well and go up aberration.And, can relax the qualification rate that causes because of eccentric relatively performance degradation and worsen, relate to the reduction of cost.
When the 1st lens combination is made of a slice positive lens, help miniaturization and cost degradation.
In order to realize the slimming of lens barrel, preferred the 3rd lens combination is made of the lens below 3.
Preferred especially the 3rd lens combination constitutes by be followed successively by these 3 lens of positive lens, positive lens and negative lens from object side.By making two lens disperse the focal power of positive lens and using negative lens, help correcting spherical aberration, coma and aberration.And, because principal point is near object side, so help the hypermutation multiple proportionsization.
And, preferably on optical axis, engage the 2nd positive lens and the negative lens from object side of the 3rd lens combination.By engaging positive lens and negative lens, can carry out the correction of a last aberration more effectively.And, by make two lens disperse the focal power of positive lens and make positive lens and negative lens for engaging lens, thereby can prevent from assembling procedure, to produce, by the deterioration of the lens eccentric relatively optical property that causes each other, relate to the raising of qualification rate and the reduction of cost.
Aspheric surface in the 3rd lens combination more than the configuration one side is effective to the correction of spherical aberration and coma.Especially, when the positive lens of the object side of the 3rd lens combination is the lens of both-sided aspherical, help the correction of each aberration.When on the multi-disc lens, disposing aspheric surface, increase the eccentric relatively optical performance degradation that causes of lens easily, but by the two sides that makes a slice lens is aspheric surface, can suppress the eccentric relatively optical performance degradation that cause of lens less, and correcting spherical aberration and coma more well.
Focal power about the 2nd lens combination preferably meets the following conditions.
0.20<|f 2/f t|<0.325 (16A)
Wherein, f tFocal length for the zoom lens of telescope end.
| f 2/ f t| when not being higher than the upper limit 0.325 of condition (16A), be used for the amount of movement of zoom, then help the miniaturization of lens barrel if guarantee focal power and inhibition.When being not less than lower limit 0.20,, can easily carry out aberration correction by suppressing refractive power.
Further preferred when as described below.
0.25<|f 2/f t|<0.320 (16A)’
Be more preferably when meeting the following conditions.
0.29<|f 2/f t|<0.315 (16A)”
From the viewpoint of the balance between miniaturization and the optical property, the focal power of the 1st lens combination is set at meets the following conditions, be preferred.
0.7<f 1/f t<1.8 (17A)
Wherein, f 1Be the focal length of the 1st lens combination, f tFocal length for the zoom lens of telescope end.
f 1/ f tWhen not being higher than the upper limit 1.8 of condition (17A),, be easy to reduce the total length of zoom lens, be easy to realize miniaturization by guaranteeing the focal power of the 1st lens combination.When being not less than lower limit 0.7,, then be easy to suppress the spherical aberration and the coma of telescope end if appropriateness suppresses focal power.
Further preferred when as described below.
1.0<f 1/f t<1.7 (17A)’
Be more preferably when meeting the following conditions.
1.3<f 1/f t<1.6 (17A)”
Focal power about the 3rd lens combination preferably meets the following conditions.
0.25<f 3/f t<0.50 (18A)
Wherein, f 3Be the focal length of the 3rd lens combination, f tFocal length for the zoom lens of telescope end.
f 3/ f tWhen not being higher than the upper limit 0.50 of condition (18A),, helping shortening the zoom lens total length and guarantee to become multiple proportions by guaranteeing focal power.When being not less than lower limit 0.25,, help aberration correction by suppressing refractive power.
Further preferred when as described below.
0.30<f 3/f t<0.40 (18A)’
Be more preferably when meeting the following conditions.
0.34<f 3/f t<0.38 (18A)”
Zoom lens is the structure with the 4th lens combination of positive refractive power, and integral body is when being 4 groups of zoom lens, and the focal power about the 4th lens combination preferably meets the following conditions.
0.40<f 4/f t<1.0 (19A)
Wherein, f 4Be the focal length of the 4th lens combination, f tFocal length for the zoom lens of telescope end.
f 4/ f tWhen not being higher than the upper limit 1.0 of condition (19A),, help guaranteeing to make the effect of off-axis ray refraction by guaranteeing the focal power of the 4th lens combination.Can reduce to incide the ccd image sensor (CCD image sensor) that is configured in image planes and the angle of the light on the CMOS type imageing sensor electro-photographic elements such as (CMOS typeimage sensor), be easy to suppress the generation of shade (deficiency in light quantity) of the brightness in image planes corner.When being not less than lower limit 0.40,, then be easy to suppress the undercorrection of curvature of the image if appropriateness suppresses the focal power of the 4th lens combination.And, the 4th lens combination is moved when focusing, be easy to suppress the change of curvature of the image.
Further preferred when as described below.
0.50<f 4/f t<0.80 (19A)’
Be more preferably when meeting the following conditions.
0.62<f 4/f t<0.66 (19A)”
The 4th lens combination also can be formed by plastic material.In the 4th lens combination, the exit pupil position configuration is gone up in position, can bring into play making light incide effect on ccd image sensor (CCD image sensor) and the CMOS type imageing sensor electro-photographic elements such as (CMOS type image sensor) efficiently.In order to realize this effect, when being set in the focal power of the 4th lens combination in the such scope of above-mentioned condition (19A), because do not need bigger focal power, so can use the low material of this refractive index of plastic lens to constitute.When the 4th lens combination is used plastic lens, suppress cost lower, more cheap zoom lens can be provided.
In addition, in order to keep performance and to realize the hypermutation multiple proportions, each lens combination given become doubly effect efficiently, and preferred balance aberration correction well in whole change times zone.
Constitute at zoom lens under the situation of 4 groups of zoom lens, preferably constitute from wide-angle side when telescope end becomes times, the 1st lens combination, the 2nd lens combination, the 3rd lens combination and the 4th lens combination move respectively, so that the interval between the 1st lens combination and the 2nd lens combination broadens, interval between the 2nd lens combination and the 3rd lens combination narrows down, and the interval between the 3rd lens combination and the 4th lens combination broadens.
Like this, move, be easy to become doubly when keeping aberration balancing, help the hypermutation multiple proportionsization by making all lens combination.And, move by making aperture diaphragm, can effectively proofread and correct ratio chromatism, and distortion aberration, not only have effect, and can suitably control entrance pupil position and exit pupil position at aspect of performance.
Therefore, the angle that will incide the light on ccd image sensor (CCD image sensor) and the CMOS type imageing sensor (CMOS type image sensor) etc. remains on suitable scope, can prevent the generation of the shade (deficiency in light quantity) of the brightness in image planes corner, be applicable to the camera head that uses the electro-photographic element.
And, preferably constitute from wide-angle side when telescope end becomes times, the 1st lens combination moves, and is positioned at object side so that compare wide-angle side at telescope end, the 2nd lens combination moves, the 3rd lens combination only moves to object side, the 4th lens combination moves.Help guaranteeing to become multiple proportions when reducing the total length of zoom lens of wide-angle side.
At this moment, the 1st lens combination can only move to object side, also can move along the protruding rail mark as side.
The 2nd lens combination can also can move along the protruding rail mark as side only to the picture side shifting.
The 3rd lens combination preferably only moves to object side.
The 4th lens combination can only move to object side, also can be only to the picture side shifting.Perhaps, also can move or move along the protruding rail mark along the protruding rail mark at object side as side.
Preferred configuration aperture diaphragm and shutter unit between the 2nd lens combination and the 3rd lens combination, shutter unit is mobile integratedly with the 3rd lens combination when becoming times.Entrance pupil is positioned at from object side observes on the very near position, and can make exit pupil away from image planes.And because between the 2nd lens combination and the 3rd lens combination be the low position of height of off-axis ray, shutter unit can not maximize the wasted space in the time of can reducing aperture diaphragm and shutter unit are moved.
And zoom lens preferably meets the following conditions.
3.8<f t/f w<15.0 (21A)
Wherein, f wBe the focal length of the zoom lens of wide-angle side, f tFocal length for the zoom lens of telescope end.
f t/ f wWhen not being higher than the upper limit 15.0 of condition (21A), be easy to guarantee optical property.When being not less than lower limit 3.8, can guarantee to become multiple proportions.
Further preferred when as described below.
4.2<f t/f w<10.0 (21A)’
Be more preferably when meeting the following conditions.
4.5<f t/f w<6 (21A)”
Then, in the 2nd side, zoom lens of the present invention has successively from object side: the 1st lens combination of positive refractive power; The 2nd lens combination of negative refractive power; And the 3rd lens combination of positive refractive power,
From wide-angle side when telescope end becomes times,
Interval between interval between described the 1st lens combination and described the 2nd lens combination and described the 2nd lens combination and described the 3rd lens combination changes,
With respect to wide-angle side, the interval between described the 1st lens combination and described the 2nd lens combination broadens at telescope end,
With respect to wide-angle side, the interval between described the 2nd lens combination and described the 3rd lens combination narrows down at telescope end,
Described the 1st lens combination comprises positive lens, and the total lens number in described the 1st lens combination is below 2,
Described the 2nd lens combination has successively from object side: the object side negative lens of concave-concave shape, positive lens and these 3 lens of picture side negative lens, and the total lens number in described the 2nd lens combination is 3,
Described positive lens be convex surface as the side as side, littler as the absolute value of the paraxial radius-of-curvature of side than the absolute value of the paraxial radius-of-curvature of object side,
Described object side negative lens in described the 2nd lens combination and described positive lens dispose across the airspace on optical axis,
The described zoom lens formula that meets the following conditions:
0<f 2/R 2n1f<0.4 (1B)
—1.6<SF 2air<—0.5 (2B)
Wherein, R 2n1fBe the paraxial radius-of-curvature of the object side of the object side negative lens in the 2nd lens combination, f 2Be the focal length of the 2nd lens combination, SF 2airBy SF 2air=(R 2n1r+ R 2p1f)/(R 2n1r-R 2p1f) define R 2n1rBe the paraxial radius-of-curvature as the side of the object side negative lens of the 2nd lens combination, R 2p1fIt is the paraxial radius-of-curvature of object side of the positive lens of the 2nd lens combination.
In the 2nd side, zoom lens constitutes, and has successively from object side: the 1st lens combination of positive refractive power; The 2nd lens combination of negative refractive power; And the 3rd lens combination of positive refractive power, from wide-angle side when telescope end becomes times, interval between described the 1st lens combination and described the 2nd lens combination and the interval between described the 2nd lens combination and described the 3rd lens combination are changed, with respect to wide-angle side, interval between described the 1st lens combination and described the 2nd lens combination broadens at telescope end, with respect to wide-angle side, the interval between described the 2nd lens combination and described the 3rd lens combination narrows down at telescope end.
By this structure, the 2nd lens combination and the 3rd lens combination are effectively shared become burden doubly, guarantee to become multiple proportions, and the aberration change that is easy to when becoming times suppresses lessly.
And the 1st lens combination is made of the lens below 2, and the 2nd lens combination is made of 3 lens, by such utilization seldom the lens of sheet number constitute, be easy to suppress the thickness of zoom lens when flexible.And, also be easy to reduce wide-angle side from the object side of the 1st lens combination the distance to entrance pupil, and be easy to carry out the miniaturization of the radial dimension of zoom lens.
And 2 negative lenses of configuration are shared the negative power of the 2nd lens combination, thereby are easy to suppress aberration in the 2nd lens combination.And by have the such configuration of negative lens, positive lens and negative lens successively from object side, the symmetry of lens arrangement is good, becomes the structure that can efficiently carry out aberration correction in the 2nd lens combination.
And above-mentioned zoom lens is that the object side and the picture side of the object side negative lens of the 2nd lens combination all is concave surface.
By this shape, the generation that suppresses the spherical aberration of telescope end is easy to guarantee the negative power of the 2nd lens combination simultaneously, and, be easy to suppress the thickness of the 2nd lens combination on optical axis.
And, the positive lens of the 2nd lens combination be convex surface as the side as side, and the absolute value of radius-of-curvature of picture side is littler than the absolute value of the radius-of-curvature of object side.And the object side negative lens and the positive lens of the 2nd lens combination dispose across the airspace on optical axis.By such formation, guarantee the positive refractive power of unique positive lens of the 2nd lens combination, the principal point of the 2nd lens combination helps guaranteeing to become multiple proportions near object simultaneously.And, be easy to keep the double-concave negative lens of object side and the aberration balancing between the picture negative lens of side.
In the 2nd side, zoom lens further meets the following conditions.
0.0<f 2/R 2n1f<0.4 (1B)
—1.6<SF 2air<—0.5 (2B)
Wherein, R 2n1fBe the paraxial radius-of-curvature of the object side of the object side negative lens in the 2nd lens combination, f 2Be the focal length of the 2nd lens combination, SF 2airBy SF 2air=(R 2n1r+ R 2pf)/(R 2n1r-R 2pf) define R 2n1rBe the paraxial radius-of-curvature as the side of the object side negative lens of the 2nd lens combination, R 2pfIt is the paraxial radius-of-curvature of object side of the positive lens of the 2nd lens combination.
The object side of the object side negative lens of the 2nd lens combination is when object side is concave shape, and total length can be shortened more near the 1st lens combination in the principal point position of the 2nd lens combination, or the multiplying power that increases the 2nd lens combination increases the change multiple proportions.At this moment, (1B) preferably satisfies condition.
By making f 2/ R 2n1fBe not less than the lower limit 0.0 of condition (1B), be easy to obtain the effect of the principal point position of the 2nd lens combination, help the miniaturization and the hypermutation multiple proportionsization of total length near the 1st lens combination.
f 2/ R 2n1fWhen not being higher than the upper limit 0.4 of condition (1B), suppress the curvature of this face, be easy to be suppressed at the correction surplus of the curvature of the image of wide-angle side especially by appropriateness.
When satisfying condition (1B), the negative power of the 2nd lens combination strengthens easily.So, for the negative power with the 2nd lens combination remains on suitable scope, and be easy to keep the aberration situation well, (2B) preferably satisfies condition.
SF 2airThe upper limit-0.5 o'clock that is not higher than condition (2B), appropriateness suppresses the negative power of the 2nd lens combination, helps suppressing the generation of each aberration.Be easy to suppress the correction surplus of curvature of the image especially.
SF 2airBe not less than the lower limit-1.6 o'clock of condition (2B),, then can reduce refraction angle poor of the upside light (upper ray) of an outer light beam and downside light (lowerray) if suppress the curvature of the object side of positive lens.Thus, preferred appropriateness suppresses the generation of the coma of telescope end, suppresses the surplus of the aberration amount of positive lens with respect to the aberration amount of negative lens generation.
When condition (1B) is as described below, further preferred.
0.005<f 2/R 2n1f<0.3 (1B)’
Be more preferably when meeting the following conditions.
0.01<f 2/R 2n1f<0.2 (1B)”
When condition (2B) is as described below, further preferred.
—1.4<SF 2air<—0.7 (2B)’
Be more preferably when meeting the following conditions.
—1.2<SF 2air<—0.9 (2B)”
And then the 3rd lens combination of preferred zoom lens is below 3 to the lens number as side.
The slimming when helping stretching and the simplification of Zoom lens structure.
If zoom lens is made as 3 groups of zoom lens, then can simplifies the mechanism that lens are moved.
Zoom lens is constituted as 4 groups of zoom lens, and establish the 4th lens combination when being positive refractive power, preferably make the 4th lens combination have function away from exit pupil.And, if for to make the 4th lens combination move the structure of focusing, the visual angle change when then being easy to suppress to focus.If utilize a slice positive lens to constitute the 4th lens combination, the miniaturization when then also helping stretching etc.
And, zoom lens is constituted as 5 groups of zoom lens, and to establish the 4th lens combination be negative refractive power, establish the 5th lens combination when being positive refractive power, as the power configuration symmetry of the lens combination of zoom lens integral body, the change of astigmatism is preferred when being easy to suppress to become times.
And, when the face of the both sides in the space of the 1st lens combination and the 2nd lens combination clamping meets the following conditions, be easy to realize better miniaturization and aberration balancing.
0.00<(1/R 2n1f—1/R 1r)·f 2<0.40 (3B)
Wherein, R 2n1fBe the paraxial radius-of-curvature of the object side of the object side negative lens in the 2nd lens combination, R 1rBe the 1st lens combination as the paraxial radius-of-curvature of the picture side of the lens of side.
This condition is in order to be easy to keep the aberration balancing from the wide-angle side to the telescope end, and limits the condition of difference of the curvature of the lens face before and after the space of the 1st lens combination and the 2nd lens combination clamping.
By (1/R 2n1f-1/R 1r) f 2Be not less than the lower limit 0.00 of condition (3B), be easy to make the outer lens face of the axle of the 1st lens combination and the 2nd lens combination approaching in wide-angle side, so, help guaranteeing curvature poor of two lens faces and the curvature of the image of correction wide-angle side.
By (1/R 2n1f-1/R 1r) f 2The upper limit 0.40 that is not higher than condition (3B) helps guaranteeing the focal power of the 1st lens combination, the spherical aberration that helps proofreading and correct telescope end.
Further preferred when as described below.
0.03<(1/R 2n1—1/R 1r)·f 2<0.30 (3B)’
Be more preferably when meeting the following conditions.
0.07<(1/R 2n1—1/R 1r)·f 2<0.20 (3B)”
Also can only limit the lower limit of above-mentioned condition or only limit higher limit.Each condition later on too.
The positive lens of the 2nd lens combination preferably satisfy condition (4A), (5A).This is the refractive index condition relevant with Abbe number with the positive lens of the 2nd lens combination.
1.84<n d2p<2.20 (4A)
13.0<v d2p<30.0 (5A)
Wherein, n D2pBe the refractive index of the positive lens of the 2nd lens combination with respect to the d line, v D2pIt is the Abbe number of the positive lens of the 2nd lens combination.
The implication of these conditions was as illustrating.
Further preferred when as described below.
1.87<n d2p<2.15 (4A)’
15.0<v d2p<26.0 (5A)’
Be more preferably when as described below.
1.90n d2p<2.12 (4A)”
17.0v d2p<21.0 (5A)”
In order further to reduce the generation of the aberration in the 2nd lens combination, when the shape that is set at the positive lens of the 2nd lens combination satisfies following conditional, be more preferably.
0.45<SF 2p<1.80 (6A)
Wherein, SF 2pBy SF 2p=(R 2pf+ R 2pr)/(R 2pf-R 2pr) define R 2pfBe the paraxial radius-of-curvature of the object side of the positive lens in the 2nd lens combination, R 2prIt is the paraxial radius-of-curvature of the picture side of the positive lens in the 2nd lens combination.
The implication of this condition was as illustrating.
Further preferred when as described below.
0.55<SF 2p<1.6 (6A)’
Be more preferably when meeting the following conditions.
0.6<SF 2p<1.3 (6A)”
The material of the negative lens of the object side of the 2nd lens combination preferably meets the following conditions.
1.78<n d2n1<2.20 (7A)
35<v d2n1<50 (8A)
Wherein, n D2n1Be the refractive index of the object side negative lens of the 2nd lens combination with respect to the d line, v D2n1It is the Abbe number of the object side negative lens of the 2nd lens combination.
The implication of these conditions was as illustrating.
Further preferred when as described below.
1.79<n d2n1<1.95 (7A)’
37v d2n1<47 (8A)’
Be more preferably when meeting the following conditions.
1.80<n d2n1<1.90 (7A)”
40<v d2n1<43 (8A)”
About the 2nd lens combination as the negative lens of side, also can preestablish optimal material.Particularly, preferably meet the following conditions.
1.78<n d2n2<2.00 (9A)
35<v d2n2<50 (10A)
Wherein, n D2n2Be the refractive index of the picture side negative lens of the 2nd lens combination with respect to the d line, v D2n2It is the Abbe number of the picture side negative lens of the 2nd lens combination.
The implication of these conditions was as illustrating.
Further preferred when as described below.
1.79n d2n2<1.95 (9A)’
38v d2n2<48 (10A)’
Be more preferably when meeting the following conditions.
1.80n d2n2<1.90 (9A)”
40<v d2n2<47 (10A)”
Shape about this negative lens preferably meets the following conditions.
—3.0<SF 2n2<—0.6 (11A)
Wherein, SF 2n2By SF 2n2=(R 2n2f+ R 2n2r)/(R 2n2f-R 2n2r) define R 2n2fBe the paraxial radius-of-curvature of the object side of the picture side negative lens in the 2nd lens combination, R 2n2rIt is the paraxial radius-of-curvature of the picture side of the picture side negative lens in the 2nd lens combination.
The implication of this condition was as illustrating.
Further preferred when as described below.
—2.6<SF 2n2<—0.9 (11A)’
Be more preferably when meeting the following conditions.
—2.1<SF 2n2<—1.1 (11A)”
And, in order to carry out good aberration correction, the positive lens of the 2nd lens combination formula that preferably meets the following conditions.
—3.0<f 2p/f 2<—1.0 (12A)
Wherein, f 2pIt is the focal length of the positive lens of the 2nd lens combination.
The implication of this condition was as illustrating.
Further preferred when as described below.
—2.8<f 2p/f 2<—1.4 (12A)’
Be more preferably when meeting the following conditions.
—2.6<f 2p/f 2<—1.8 (12A)”
And, for the generation that further suppresses aberration and obtain the good optical performance, also can be at least one lens face configuration aspheric surface in the object side negative lens of the 2nd lens combination.And, also can dispose aspheric surface on the two sides.To proofreading and correct coma and curvature of the image is effective.
At this moment, preferably meet the following conditions.
0.002<(ASP 2n1f+|ASP 2n1r|)/f w<0.10 (13A)
—0.06<(ASP 2n1r—ASP 2n1f)/f w<0.06 (13B)
Wherein, ASP 2n1fBe the aspheric surface departure (aspherical displacement) of lens face of object side of the object side negative lens of the 2nd lens combination, ASP 2n1rBe the aspheric surface departure of lens face of picture side of the object side negative lens of the 2nd lens combination, f wFocal length for the zoom lens of wide-angle side.The aspheric surface departure as shown in figure 43, at the sphere that will have the vertex of surface identical and have a radius-of-curvature identical during as the benchmark sphere with the paraxial radius-of-curvature of this lens face with the summit of lens face, on the position of the maximum light height of incidence of the wide-angle side in this lens face, be distance when measuring, will be made as plus sign in the situation that picture side direction (right among the figure) is measured from the benchmark sphere to this lens face with the optical axis parallel direction.Aspheric surface departure when lens face is sphere or plane is 0.
The implication of these conditions was as illustrating.
Further preferred when as described below.
—0.055<(ASP 2n1r—ASP 2n1f)/f w<0.04 (13B)’
Be more preferably when meeting the following conditions.
—0.059<(ASP 2n1r—ASP 2n1f)/f w<0.015 (13B)”
And then, the object side of the object side negative lens in the 2nd lens combination also can for refractive power along with the aspheric surface that increases away from optical axis.
In addition, the refractive power increase means that negative refractive power reduces or positive refractive power increases.
By such shape, help proofreading and correct the off-axis aberration of wide-angle side.
And then, the object side negative lens of preferred the 2nd lens combination is a double-concave negative lens, the object side of double-concave negative lens is the aspheric surface that negative refractive power reduces along with the increase with optical axis distance, double-concave negative lens be the aspheric surface (embodiment 1～10) that negative refractive power increases along with the increase with optical axis distance as the side.
By such shape, when guaranteeing the negative power of core, peripheral part of lens, help proofreading and correct the outer coma of axle of wide-angle side, help guaranteeing the visual angle.And, also help the slimming of the 2nd lens combination integral body.
The 2nd lens combination as the negative lens of side be aspheric surface as the side time, be effective to the correction of spherical aberration and coma.At this moment, preferably meet the following conditions.
—0.09<(ASP 2n2r—ASP 2n2f)/f w<—0.003 (14A)
Wherein, ASP 2n2fBe the aspheric surface departure of lens face of object side of the picture side negative lens of the 2nd lens combination, ASP 2n2rBe the aspheric surface departure of lens face of picture side of the picture side negative lens of the 2nd lens combination, f wBe the system-wide focal length of the zoom lens of wide-angle side.Aspheric surface departure when lens face is sphere or plane is 0.
The implication of this condition is such as already explained.
Further preferred when as described below.
—0.07<(ASP 2n2r—ASP 2n2f)/f w<—0.005 (14A)’
Be more preferably when meeting the following conditions.
—0.05<(ASP 2n2r—ASP 2n2f)/f w<—0.015 (14A)”
And then, preferred the 2nd lens combination be convex surface towards the negative meniscus lens of picture side as the side negative lens, the face as side of negative meniscus lens is that positive refractive power is along with the aspheric surface that strengthens away from optical axis.
By this structure, help carrying out well the spherical aberration of the 2nd lens combination and the correction of outer each aberration of axle.
The positive lens of the 2nd lens combination and also can also can engaging as the negative lens of side for not engaging simple lens independent of each other.Utilize the degree of freedom of aberration correction of air surface of contact big when not engaging.On the other hand, help chromatic aberration correction during joint, and, can relax the qualification rate that causes because of eccentric relatively optical performance degradation and worsen, relate to the reduction of cost.
And the 1st lens combination has positive lens and negative lens, is preferred aspect aberration.
Especially, the 1st lens combination also can be arranged in order negative lens and positive lens from object side.Like this, when considering the total of the 1st lens combination and the 2nd lens combination, become the good structure of symmetry that is followed successively by negative lens, positive lens, negative lens, positive lens and negative lens from object side.Particularly can effectively eliminate the aberration that the synthetic lens combination that is made of the 1st lens combination and the 2nd lens combination in wide-angle side produces.And, because the rear side principal point position of the 1st lens combination is near the picture side, so effectively guarantee to become multiple proportions.
The negative lens of the 1st lens combination and positive lens utilization do not engage and lens composition independent of each other when constituting, and utilize the air lens that form between two lens, can proofread and correct the coma of telescope end especially well.
At this moment, the interval between two lens preferably meets the following conditions.
0.0≤L 1np/L 1<0.2 (15A)
Wherein, L 1npBe the negative lens and the interval of positive lens on optical axis of the 1st lens combination, L 1It is the gross thickness on the optical axis of the 1st lens combination.
The implication of this condition was as illustrating.
Further preferred when as described below.
0.0≤L 1np/L 1<0.16 (15A)’
Be more preferably when meeting the following conditions.
0.0≤L 1np/L 1<0.12 (15A)”
And the negative lens of the 1st lens combination and positive lens also can engage.Can proofread and correct the ratio chromatism, of wide-angle side and the axle of telescope end well and go up aberration.And, can relax the qualification rate that causes because of eccentric relatively performance degradation and worsen, relate to the reduction of cost.
When the 1st lens combination is made of a slice positive lens, help miniaturization and cost degradation.
In order to realize the slimming of lens barrel, preferred the 3rd lens combination is made of the lens below 3.
Preferred especially the 3rd lens combination constitutes by be followed successively by these 3 lens of positive lens, positive lens and negative lens from object side.By making two lens disperse the focal power of positive lens and using negative lens, help correcting spherical aberration, coma and aberration.And, because principal point is near object side, so help the hypermutation multiple proportionsization.
And, preferably on optical axis, engage the 2nd positive lens and the negative lens from object side of the 3rd lens combination.By engaging positive lens and negative lens, can carry out the correction of a last aberration more effectively.And, by make two lens disperse the focal power of positive lens and make positive lens and negative lens for engaging lens, can prevent from assembling procedure, to produce, by the deterioration of the lens eccentric relatively optical property that causes each other, relate to the raising of qualification rate and the reduction of cost.
Aspheric surface in the 3rd lens combination more than the configuration one side is effective to the correction of spherical aberration and coma.Especially, when the positive lens of the object side of the 3rd lens combination is the lens of both-sided aspherical, help the correction of each aberration.When on the multi-disc lens, disposing aspheric surface, increase the eccentric relatively optical performance degradation that causes of lens easily, but by the two sides that makes a slice lens is aspheric surface, can suppress the eccentric relatively optical performance degradation that cause of lens less, and correcting spherical aberration and coma more well.
Focal power about the 2nd lens combination preferably meets the following conditions.
0.20<|f 2/f t|<0.325 (16A)
Wherein, f tFocal length for the zoom lens of telescope end.
The implication of this condition was as illustrating.
Further preferred when as described below.
0.25<|f 2/f t|<0.320 (16A)’
Be more preferably when meeting the following conditions.
0.29<|f 2/f t|<0.315 (16A)”
From the viewpoint of the balance between miniaturization and the optical property, the focal power of the 1st lens combination is set to meet the following conditions be preferred.
0.7<f 1/f t<1.8 (17A)
Wherein, f 1Be the focal length of the 1st lens combination, f tFocal length for the zoom lens of telescope end.
The implication of this condition was as illustrating.
Further preferred when as described below.
1.0<f 1/f t<1.7 (17A)’
Be more preferably when meeting the following conditions.
1.3<f 1/f t<1.6 (17A)”
Focal power about the 3rd lens combination preferably meets the following conditions.
0.25<f 3/f t<0.50 (18A)
Wherein, f 3Be the focal length of the 3rd lens combination, f tFocal length for the zoom lens of telescope end.
The implication of this condition was as illustrating.
Further preferred when as described below.
0.30<f 3/f t<0.40 (18A)’
Be more preferably when meeting the following conditions.
0.34<f 3/f t<0.38 (18A)”
Zoom lens is the structure with the 4th lens combination of positive refractive power, and integral body is when being 4 groups of zoom lens, and the focal power about the 4th lens combination preferably meets the following conditions.
0.40<f 4/f t<1.0 (19A)
Wherein, f 4Be the focal length of the 4th lens combination, f tFocal length for the zoom lens of telescope end.
The implication of this condition was as illustrating.
Further preferred when as described below.
0.50<f 4/f t<0.80 (19A)’
Be more preferably when meeting the following conditions.
0.62<f 4/f t<0.66 (19A)”
The 4th lens combination also can be formed by plastic material.In the 4th lens combination, the exit pupil position configuration is gone up in position, can bring into play making light incide effect on ccd image sensor (CCD image sensor) and the CMOS type imageing sensor electro-photographic elements such as (CMOS type image sensor) efficiently.In order to realize this effect, when being set in the focal power of the 4th lens combination in the such scope of above-mentioned condition (19A), because do not need bigger focal power, so can use the low material of this refractive index of plastic lens to constitute.When the 4th lens combination is used plastic lens, suppress cost lower, more cheap zoom lens can be provided.
In addition, in order to keep performance and to realize the hypermutation multiple proportions, each lens combination given become doubly effect efficiently, and preferred balance aberration correction well in whole change times zone.
Constitute at zoom lens under the situation of 4 groups of zoom lens, preferably constitute from wide-angle side when telescope end becomes times, the 1st lens combination, the 2nd lens combination, the 3rd lens combination and the 4th lens combination move respectively, so that the interval between the 1st lens combination and the 2nd lens combination broadens, interval between the 2nd lens combination and the 3rd lens combination narrows down, and the interval between the 3rd lens combination and the 4th lens combination broadens.
Like this, move, be easy to become doubly when keeping aberration balancing, help the hypermutation multiple proportionsization by making all lens combination.And, move by making aperture diaphragm, can effectively proofread and correct ratio chromatism, and distortion aberration, not only have effect, and can suitably control entrance pupil position and exit pupil position at aspect of performance.
Therefore, the angle that will incide the light on ccd image sensor (CCD image sensor) and the CMOS type imageing sensor (CMOS type image sensor) etc. remains on suitable scope, can prevent the generation of the shade (deficiency in light quantity) of the brightness in image planes corner, be applicable to the camera head that uses the electro-photographic element.
And, preferably constitute from wide-angle side when telescope end becomes times, the 1st lens combination moves, and is positioned at object side so that compare wide-angle side at telescope end, the 2nd lens combination moves, the 3rd lens combination only moves to object side, the 4th lens combination moves.Help guaranteeing to become multiple proportions when reducing the total length of zoom lens of wide-angle side.
At this moment, the 1st lens combination can only move to object side, also can move along the protruding rail mark as side.
The 2nd lens combination can also can move along the protruding rail mark as side only to the picture side shifting.
The 3rd lens combination preferably only moves to object side.
The 4th lens combination can only move to object side, also can be only to the picture side shifting.Perhaps, also can move or move along the protruding rail mark along the protruding rail mark at object side as side.
Preferred configuration aperture diaphragm and shutter unit between the 2nd lens combination and the 3rd lens combination, shutter unit is mobile integratedly with the 3rd lens combination when becoming times.Entrance pupil is positioned at from object side observes on the very near position, and can make exit pupil away from image planes.And because between the 2nd lens combination and the 3rd lens combination be the low position of height of off-axis ray, shutter unit can not maximize the wasted space in the time of can reducing aperture diaphragm and shutter unit are moved.
And zoom lens preferably meets the following conditions.
3.8<f t/f w<15.0 (21A)
Wherein, f wBe the focal length of the zoom lens of wide-angle side, f tFocal length for the zoom lens of telescope end.
The implication of this condition was as illustrating.
Further preferred when as described below.
4.2<f t/f w<10.0 (21A)’
Be more preferably when meeting the following conditions.
4.5<f t/f w<6 (21A)”
And electronic image pickup device of the present invention has: zoom lens of the present invention; And the electro-photographic element, it is configured in the picture side of described zoom lens, will be converted to electric signal by the optical image that described zoom lens forms.
And this electronic image pickup device preferably meets the following conditions.
0.70<I m/f w<1.00 (20A)
Wherein, I mBe maximum image height, f wFocal length for the zoom lens of wide-angle side.
I m/ f wWhen not being higher than the upper limit 1.00 of condition (20A), the photography visual angle can be not excessive, so help reducing the generation of barrel distortion aberration.When being not less than lower limit 0.70, can bring into play the advantage of small-sized, the wide-angleization of zoom lens of the present invention.
Further preferred when as described below.
0.72<I m/f w<0.90 (20A)’
Be more preferably when meeting the following conditions.
0.74<I m/f w<0.77 (20A)”
Then, embodiment is described.
Figure 1A～21C is the sectional view of the infintie object point that comprises embodiment 1～21 optical axis when focusing on.Wherein, Figure 1A, 2A, 3A... are the sectional views of wide-angle side, and Figure 1B, 2B, 3B... are the sectional views of intermediateness, and Fig. 1 C, 2C, 3C... are the sectional views of telescope end.In Figure 1A～Figure 21 C, the 1st lens combination is represented with G1, the 2nd lens combination is represented with G2, aperture diaphragm represents that with S the 3rd lens combination represents that with G3 the 4th lens combination is represented with G4, the 5th lens combination is represented with G5, optical low-pass filter represents that with F the cloche of electro-photographic element represents that with C image planes are represented with 1.In addition, in order to remove infrared light, for example also can directly implement the infrared cut of light plated film on the surface of optical low-pass filter F.Perhaps, also can dispose the IR-cut absorbing filter in addition.
Shown in Figure 1A～1C, embodiment 1 has the 1st lens combination G1, the 2nd lens combination G2, the aperture diaphragm S of negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power of positive refractive power successively from object side.From wide-angle side during to the telescope end zoom, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move along the protruding rail mark at object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 by be followed successively by double-concave negative lens from object side, convex surface constitutes towards the negative meniscus lens as side towards positive meniscus shaped lens and the convex surface as side, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the face of the object side of the two sides of the biconvex positive lens of the face of the picture side of the two sides of the double-concave negative lens of the 2nd lens combination G2, negative meniscus lens, the 3rd lens combination G3 and the biconvex positive lens of the 4th lens combination G4.
Shown in Fig. 2 A～2C, embodiment 2 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move along the protruding rail mark at object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 by be followed successively by double-concave negative lens from object side, convex surface constitutes towards the negative meniscus lens as side towards positive meniscus shaped lens and the convex surface as side, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the face of the object side of the two sides of the biconvex positive lens of the face of the picture side of the two sides of the double-concave negative lens of the 2nd lens combination G2, negative meniscus lens, the 3rd lens combination G3 and the biconvex positive lens of the 4th lens combination G4.
Shown in Fig. 3 A～3C, embodiment 3 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move along the protruding rail mark at object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 by be followed successively by double-concave negative lens from object side, convex surface constitutes towards the negative meniscus lens as side towards positive meniscus shaped lens and the convex surface as side, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the face of the object side of the two sides of the biconvex positive lens of the face of the picture side of the two sides of the double-concave negative lens of the 2nd lens combination G2, negative meniscus lens, the 3rd lens combination G3 and the biconvex positive lens of the 4th lens combination G4.
Shown in Fig. 4 A～4C, embodiment 4 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move along the protruding rail mark at object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 is by being followed successively by double-concave negative lens, convex surface from object side towards constituting towards the joint lens as the negative meniscus lens of side as the positive meniscus shaped lens of side and convex surface, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the two sides of the double-concave negative lens of the 2nd lens combination G2, engage lens as the face of the object side of the biconvex positive lens of the two sides of the biconvex positive lens of the face of side, the 3rd lens combination G3 and the 4th lens combination G4.
Shown in Fig. 5 A～5C, embodiment 5 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move along the protruding rail mark at object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes by be followed successively by the negative meniscus lens and the biconvex positive lens of convex surface towards object side from object side, the 2nd lens combination G2 is by being followed successively by double-concave negative lens, convex surface from object side towards constituting towards the joint lens as the negative meniscus lens of side as the positive meniscus shaped lens of side and convex surface, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the two sides of the double-concave negative lens of the 2nd lens combination G2, engage lens as the face of the object side of the biconvex positive lens of the two sides of the biconvex positive lens of the face of side, the 3rd lens combination G3 and the 4th lens combination G4.
Shown in Fig. 6 A～6C, embodiment 6 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move along the protruding rail mark at object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 by be followed successively by double-concave negative lens from object side, convex surface constitutes towards the negative meniscus lens as side towards positive meniscus shaped lens and the convex surface as side, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the face of the object side of the two sides of the biconvex positive lens of the face of the picture side of the two sides of the double-concave negative lens of the 2nd lens combination G2, negative meniscus lens, the 3rd lens combination G3 and the biconvex positive lens of the 4th lens combination G4.
Shown in Fig. 7 A～7C, embodiment 7 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move along the protruding rail mark at object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 by be followed successively by double-concave negative lens from object side, convex surface constitutes towards the negative meniscus lens as side towards positive meniscus shaped lens and the convex surface as side, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the face of the object side of the two sides of the biconvex positive lens of the face of the picture side of the two sides of the double-concave negative lens of the 2nd lens combination G2, negative meniscus lens, the 3rd lens combination G3 and the biconvex positive lens of the 4th lens combination G4.
Shown in Fig. 8 A～8C, embodiment 8 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move along the protruding rail mark at object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 is by being followed successively by double-concave negative lens, convex surface from object side towards constituting towards the joint lens as the negative meniscus lens of side as the positive meniscus shaped lens of side and convex surface, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the two sides of the double-concave negative lens of the 2nd lens combination G2, engage lens as the face of the object side of the biconvex positive lens of the two sides of the biconvex positive lens of the face of side, the 3rd lens combination G3 and the 4th lens combination G4.
Shown in Fig. 9 A～9C, embodiment 9 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move along the protruding rail mark at object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 is by being followed successively by double-concave negative lens, convex surface from object side towards constituting towards the joint lens as the negative meniscus lens of side as the positive meniscus shaped lens of side and convex surface, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the two sides of the double-concave negative lens of the 2nd lens combination G2, engage lens as the face of the object side of the biconvex positive lens of the two sides of the biconvex positive lens of the face of side, the 3rd lens combination G3 and the 4th lens combination G4.
Shown in Figure 10 A～10C, embodiment 10 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 is moving along the protruding rail mark as side, more close a little as side in intermediateness than the position of wide-angle side, at telescope end than the more close object side in the position of wide-angle side, when the interval between the 2nd lens combination G2 and the 1st lens combination G1 broadens to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, the 4th lens combination G4 from the wide-angle side to the intermediateness and the interval between the 3rd lens combination G3 move to object side when broadening, from middle state to the telescope end almost fixed.
The 1st lens combination G1 constitutes towards the joint lens of the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 constitutes towards the negative meniscus lens as side by be followed successively by double-concave negative lens, biconvex positive lens and convex surface from object side, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the face of the object side of the two sides of the biconvex positive lens of the face of the picture side of the two sides of the double-concave negative lens of the 2nd lens combination G2, negative meniscus lens, the 3rd lens combination G3 and the biconvex positive lens of the 4th lens combination G4.
Shown in Figure 11 A～11C, embodiment 11 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move along the protruding rail mark at object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 by be followed successively by double-concave negative lens from object side, convex surface constitutes towards the negative meniscus lens as side towards positive meniscus shaped lens and the convex surface as side, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the face of the object side of the two sides of the biconvex positive lens of the face of the object side of the two sides of the double-concave negative lens of the 2nd lens combination G2, negative meniscus lens, the 3rd lens combination G3 and the biconvex positive lens of the 4th lens combination G4.
Shown in Figure 12 A～12C, embodiment 12 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move along the protruding rail mark at object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 by be followed successively by double-concave negative lens from object side, convex surface constitutes towards the negative meniscus lens as side towards positive meniscus shaped lens and the convex surface as side, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the face of the object side of the two sides of the biconvex positive lens of the two sides of the two sides of the double-concave negative lens of the 2nd lens combination G2, negative meniscus lens, the 3rd lens combination G3 and the biconvex positive lens of the 4th lens combination G4.
Shown in Figure 13 A～13C, embodiment 13 is made of the 2nd lens combination G2, aperture diaphragm S, the 3rd lens combination G3 of positive refractive power, the 4th lens combination G4 of negative refractive power and the 5th lens combination G5 of positive refractive power of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, interval between the 4th lens combination G4 and the 3rd lens combination G3 temporarily broadens and moves to object side when then narrowing down, and moves to object side when the interval between the 5th lens combination G5 and the 4th lens combination G4 broadens.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 is by being followed successively by double-concave negative lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of picture side towards the positive meniscus shaped lens and the convex surface of picture side, the 3rd lens combination G3 is made of a slice biconvex positive lens, the 4th lens combination G4 constitutes towards the joint lens of the negative meniscus lens of object side by be followed successively by the positive meniscus shaped lens and the convex surface of convex surface towards object side from object side, and the 5th lens combination G5 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the two sides of the double-concave negative lens of the 2nd lens combination G2, engage lens as the face of the object side of the biconvex positive lens of the two sides of the biconvex positive lens of the face of side, the 3rd lens combination G3 and the 5th lens combination G5.
Shown in Figure 14 A～14C, embodiment 14 is made of the 2nd lens combination G2, aperture diaphragm S, the 3rd lens combination G3 of positive refractive power, the 4th lens combination G4 of negative refractive power and the 5th lens combination G5 of positive refractive power of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, interval between the 4th lens combination G4 and the 3rd lens combination G3 temporarily broadens and moves to object side when then narrowing down, move along the protruding rail mark at object side when the interval between the 5th lens combination G5 and the 4th lens combination G4 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 is by being followed successively by double-concave negative lens from object side, convex surface constitutes towards the negative meniscus lens of picture side towards the positive meniscus shaped lens and the convex surface of picture side, the 3rd lens combination G3 is made of a slice biconvex positive lens, the 4th lens combination G4 constitutes towards the joint lens of the negative meniscus lens of object side by be followed successively by the positive meniscus shaped lens and the convex surface of convex surface towards object side from object side, and the 5th lens combination G5 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the face of the object side of the two sides of the biconvex positive lens of the face of the object side of the two sides of the double-concave negative lens of the 2nd lens combination G2, negative meniscus lens, the 3rd lens combination G3 and the biconvex positive lens of the 5th lens combination G5.
Shown in Figure 15 A～15C, embodiment 15 is made of the 2nd lens combination G2, aperture diaphragm S, the 3rd lens combination G3 of positive refractive power, the 4th lens combination G4 of negative refractive power and the 5th lens combination G5 of positive refractive power of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, the 2nd lens combination G2 is moving along the protruding rail mark as side, at telescope end than the more close picture side in the position of wide-angle side.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, interval between the 4th lens combination G4 and the 3rd lens combination G3 temporarily broadens and moves to object side when then narrowing down, move along the protruding rail mark at object side when the interval between the 5th lens combination G5 and the 4th lens combination G4 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes by be followed successively by the negative meniscus lens and the biconvex positive lens of convex surface towards object side from object side, the 2nd lens combination G2 is by being followed successively by double-concave negative lens, convex surface from object side towards constituting towards the joint lens as the negative meniscus lens of side as the positive meniscus shaped lens of side and convex surface, the 3rd lens combination G3 is made of a slice biconvex positive lens, the 4th lens combination G4 constitutes towards the joint lens of the negative meniscus lens of object side by be followed successively by the positive meniscus shaped lens and the convex surface of convex surface towards object side from object side, and the 5th lens combination G5 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the two sides of the double-concave negative lens of the 2nd lens combination G2, engage lens as the face of the object side of the biconvex positive lens of the two sides of the biconvex positive lens of the face of side, the 3rd lens combination G3 and the 5th lens combination G5.
Shown in Figure 16 A～16C, embodiment 16 is made of the 2nd lens combination G2, aperture diaphragm S, the 3rd lens combination G3 of positive refractive power, the 4th lens combination G4 of negative refractive power and the 5th lens combination G5 of positive refractive power of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 is moving along the protruding rail mark as side, in intermediateness than the position of wide-angle side a little near the picture side, at telescope end than the more close object side in the position of wide-angle side.The 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move along the protruding rail mark at object side integratedly, more close a little as side at telescope end than the position of intermediateness, than the more close object side in the position of wide-angle side, interval between the 4th lens combination G4 and the 3rd lens combination G3 temporarily broadens and moves along the protruding rail mark at object side when then narrowing down, more close a little as side at telescope end than the position of intermediateness, than the more close object side in the position of wide-angle side, interval between the 5th lens combination G5 and the 4th lens combination G4 temporarily broadens and moves along the protruding rail mark at object side when then narrowing down a little, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the joint lens of the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 is by being followed successively by double-concave negative lens from object side, convex surface constitutes towards the negative meniscus lens of picture side towards the positive meniscus shaped lens and the convex surface of picture side, the 3rd lens combination G3 is made of a slice biconvex positive lens, the 4th lens combination G4 constitutes towards the joint lens of the negative meniscus lens of object side by be followed successively by the positive meniscus shaped lens and the convex surface of convex surface towards object side from object side, and the 5th lens combination G5 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the face of the object side of the two sides of the biconvex positive lens of the face of the picture side of the two sides of the double-concave negative lens of the 2nd lens combination G2, negative meniscus lens, the 3rd lens combination G3 and the biconvex positive lens of the 5th lens combination G5.
Shown in Figure 17 A～17C, embodiment 17 is made of the 2nd lens combination G2, aperture diaphragm S, the 3rd lens combination G3 of positive refractive power, the 4th lens combination G4 of negative refractive power and the 5th lens combination G5 of positive refractive power of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, interval between the 4th lens combination G4 and the 3rd lens combination G3 temporarily broadens and moves to object side when then narrowing down, move along the protruding rail mark at object side when the interval between the 5th lens combination G5 and the 4th lens combination G4 broadens, at telescope end than the position of wide-angle side a little near object side.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 is by being followed successively by double-concave negative lens from object side, convex surface constitutes towards the negative meniscus lens of picture side towards the positive meniscus shaped lens and the convex surface of picture side, the 3rd lens combination G3 is made of a slice biconvex positive lens, the 4th lens combination G4 constitutes towards the joint lens of the negative meniscus lens of object side by be followed successively by the positive meniscus shaped lens and the convex surface of convex surface towards object side from object side, and the 5th lens combination G5 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the face of the object side of the two sides of the biconvex positive lens of the face of the picture side of the two sides of the double-concave negative lens of the 2nd lens combination G2, negative meniscus lens, the 3rd lens combination G3 and the biconvex positive lens of the 5th lens combination G5.
Shown in Figure 18 A～18C, embodiment 18 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move to object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens.
The 1st lens combination G1 is made of the positive meniscus shaped lens of a slice convex surface towards object side, the 2nd lens combination G2 constitutes towards the negative meniscus lens as side by be followed successively by double-concave negative lens, biconvex positive lens and convex surface from object side, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of towards the positive meniscus shaped lens as side a slice convex surface.
Below eight faces use aspheric surfaces: the face of the object side of the two sides of the face of the two sides of the double-concave negative lens of the two sides of the positive meniscus shaped lens of the 1st lens combination G1, the 2nd lens combination G2, the picture side of negative meniscus lens, the biconvex positive lens of the 3rd lens combination G3 and the positive meniscus shaped lens of the 4th lens combination G4.
Shown in Figure 19 A～19C, embodiment 19 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, move to object side when the interval between the 4th lens combination G4 and the 3rd lens combination G3 broadens.
The 1st lens combination G1 is made of the positive meniscus shaped lens of a slice convex surface towards object side, the 2nd lens combination G2 constitutes by be followed successively by double-concave negative lens, biconvex positive lens and double-concave negative lens from object side, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of towards the positive meniscus shaped lens as side a slice convex surface.
Below eight faces use aspheric surfaces: the two sides of the double-concave negative lens of the object side of the two sides of the positive meniscus shaped lens of the 1st lens combination G1, the 2nd lens combination G2, as the face of the object side of the positive meniscus shaped lens of the two sides of the biconvex positive lens of the face of the picture side of the double-concave negative lens of side, the 3rd lens combination G3 and the 4th lens combination G4.
Shown in Figure 20 A～20C, embodiment 20 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side respectively independently, and the interval between the 3rd lens combination G3 and the aperture diaphragm S narrows down from the wide-angle side to the intermediateness, broaden to telescope end from middle state, move to object side simultaneously.When broadening, the interval between the 4th lens combination G4 and the 3rd lens combination G3 moves to object side a little.
The 1st lens combination G1 constitutes by be followed successively by the negative meniscus lens and the biconvex positive lens of convex surface towards object side from object side, the 2nd lens combination G2 is made of the joint lens that are followed successively by double-concave negative lens, biconvex positive lens and double-concave negative lens from object side, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below six faces use aspheric surfaces: the two sides of the double-concave negative lens of the 2nd lens combination G2, engage lens as the face of the object side of the biconvex positive lens of the two sides of the biconvex positive lens of the face of side, the 3rd lens combination G3 and the 4th lens combination G4.
Shown in Figure 21 A～21C, embodiment 21 is made of the 2nd lens combination G2, the aperture diaphragm S of the 1st lens combination G1 that is followed successively by positive refractive power from object side, negative refractive power, the 3rd lens combination G3 of positive refractive power and the 4th lens combination G4 of positive refractive power, from wide-angle side when telescope end becomes times, the 1st lens combination G1 moves to object side, and the 2nd lens combination G2 is to the picture side shifting.Aperture diaphragm S and the 3rd lens combination G3 move to object side integratedly, the 4th lens combination G4 from the wide-angle side to the intermediateness and the interval between the 3rd lens combination G3 move to object side when broadening, from middle state to the telescope end almost fixed.
The 1st lens combination G1 constitutes towards the positive meniscus shaped lens of object side by be followed successively by the negative meniscus lens and the convex surface of convex surface towards object side from object side, the 2nd lens combination G2 constitutes towards the negative meniscus lens as side by be followed successively by negative meniscus lens, biconvex positive lens and the convex surface of convex surface towards object side from object side, the 3rd lens combination G3 by be followed successively by the biconvex positive lens from object side, convex surface constitutes towards the joint lens of the negative meniscus lens of object side towards the positive meniscus shaped lens and the convex surface of object side, the 4th lens combination G4 is made of a slice biconvex positive lens.
Below five faces use aspheric surfaces: the face of the picture side of the negative meniscus lens of the object side of the 2nd lens combination G2, as the face of the object side of the biconvex positive lens of the two sides of the biconvex positive lens of the face of the picture side of the negative meniscus lens of side, the 3rd lens combination G3 and the 4th lens combination G4.
The numeric data of each embodiment is shown below, and except above-mentioned symbol, f is the focal length of zoom lens, F NoBe the F value, 2 ω are the visual angle, and WE is a wide-angle side, and ST is an intermediateness, and TE is a telescope end, r 1, r 2... be the paraxial radius-of-curvature of each lens face, d 1, d 2... be the interval between each lens face, n D1, n D2... be the refractive index of the d line of each lens, v D1, v D2... be the Abbe number of each lens.The symbol of radius-of-curvature back (AS) represents that this face is an aspheric surface, represents that (S) this face is the aperture diaphragm face, represents that (I) this face is image planes.In addition, be that x axle (direct of travel of establishing light for just), optical axis and aspheric intersection point are initial point, direction by initial point and light shaft positive cross is in the coordinate system of y axle establishing optical axis, aspherical shape is as shown in the formula expression.
x＝(y 2/r)/[1+{1-(K+1)(y/r) 2} 1/2]
+A 4y 4+A 6y 6+A 8y 8+A 10y 10
Wherein, r is paraxial radius-of-curvature, and K is the circular cone coefficient, A 4, A 6, A 8, A 10Be respectively 4 times, 6 times, 8 times, 10 times asphericity coefficient.
Embodiment 1
r 1＝19.996 d 1＝0.80 n d1＝1.92286 v d1＝18.90
r 2＝15.394 d 2＝0.26
r 3＝17.278 d 3＝3.11 n d2＝1.76802 v d2＝49.24
r 4=534.344 d 4=variable
r 5＝-58.703(AS) d 5＝0.82 n d3＝1.88300 v d3＝40.76
r 6＝5.969(AS) d 6＝2.65
r 7＝-431.058 d 7＝1.95 n d4＝2.00170 v d4＝20.64
r 8＝-14.597 d 8＝0.07
r 9＝-13.708 d 9＝0.67 n d5＝1.81600 v d5＝46.62
r 10=-67.948 (AS) d 10=variable
r 11＝∞(S) d 11＝0.10
r 12＝5.491(AS) d 12＝2.70 n d6＝1.58913 v d6＝61.14
r 13＝-11.075(AS) d 13＝0.10
r 14＝5.503 d 14＝1.38 n d7＝1.59201 v d7＝67.02
r 15＝13.913 d 15＝0.80 n d8＝2.00069 v d8＝25.46
r 16=3.463 d 16=variable
r 17＝19.919(AS) d 17＝2.07 n d9＝1.74330 v d9＝49.33
r 18=-25.922 d 18=variable
r 19＝∞ d 19＝0.40 n d10＝1.54771 v d10＝62.84
r 20＝∞ d 20＝0.50
r 21＝∞ d 21＝0.50 n d11＝1.51633 v d11＝64.14
r 22＝∞ d 22＝0.36
r 23＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝1.99104×10 -4 A 6＝-8.59909×10 -6 A 8＝2.01071×10 -7
A 10＝-1.73584×10 -9
The 6th
K＝0.000
A 4＝7.61962×10 -5 A 6＝2.30339×10 -5 A 8＝-1.98717×10 -6
A 10＝4.99512×10 -8
The 10th
K＝10.849
A 4＝-2.64668×10 -4 A 6＝-1.16671×10 -6 A 8＝-1.29451×10 -7
A 10＝0
The 12nd
K＝-0.000
A 4＝-9.20803×10 -4 A 6＝7.90503×10 -6 A 8＝-4.58612×10 -6
A 10＝5.46733×10 -7
The 13rd
K＝0.000
A 4＝5.31169×10 -4 A 6＝2.85804×10 -5 A 8＝-8.58478×10 -6
A 10＝9.90563×10 -7
The 17th
K＝0.000
A 4＝-2.06640×10 -6 A 6＝1.19043×10 -5 A 8＝-4.13589×10 -7
A 10＝6.77582×10 -9
The zoom data ' (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
FNO 3.10 4.58 4.91
2ω(°) 80.14 35.47 17.64
d 4 0.73 4.49 13.26
d 10 10.82 3.67 0.68
d 16 2.75 8.58 9.99
d 18 2.83 3.05 2.97
Embodiment 2
r 1＝23.279 d 1＝0.80 n d1＝1.92286 v d1＝18.90
r 2＝16.155 d 2＝0.18
r 3＝17.729 d 3＝3.05 n d2＝1.85719 v d2＝43.01
r 4=577.289 d 4=variable
r 5＝-57.796(AS) d 5＝0.80 n d 3＝1.83481 v d3＝42.71
r 6＝5.963(AS) d 6＝2.79
r 7＝-136.071 d 7＝1.78 n d4＝1.94595 v d4＝17.98
r 8＝-16.198 d 8＝0.09
r 9＝-14.697 d 9＝0.68 n d5＝1.83481 v d5＝42.71
r 10=44.810 (AS) d 10=variable
r 11＝∞(S) d 11＝0.10
r 12＝5.548(AS) d 12＝2.70 n d6＝1.58913 v d6＝61.14
r 13＝-10.984(AS) d 13＝0.10
r 14＝5.510 d 14＝1.36 n d7＝1.59201 v d7＝67.02
r 15＝13.333 d 15＝0.80 n d8＝2.00069 v d8＝25.46
r 16=3.476 d 16=variable
r 17＝19.243(AS) d 17＝2.07 n d9＝1.74330 v d9＝49.33
r 18=-28.285 d 18=variable
r 19＝∞ d 19＝0.40 n d10＝1.54771 v d10＝62.84
r 20＝∞ d 20＝0.50
r 21＝∞ d 21＝0.50 n d11＝1.51633 v d11＝64.14
r 22＝∞ d 22＝0.36
r 23＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝1.91532×10 -4 A 6＝-6.16585×10 -6 A 8＝9.93129×10 -8
A 10＝-6.19551×10 -10
The 6th
K＝0.000
A 4＝8.56780×10 -5 A 6＝2.37196×10 -5 A 8＝-1.32112×10 -6
A 10＝1.29769×10 -8
The 10th
K＝5.360
A 4＝-2.35672×10 -4 A 6＝-2.32986×10 -6 A 8＝3.46565×10 -8
A 10＝0
The 12nd
K＝-0.000
A 4＝-9.12531×10 -4 A 6＝-2.10029×10 -6 A 8＝-2.33162×10 -6
A 10＝3.38870×10 -7
The 13rd
K＝0.000
A 4＝5.13813×10 -4 A 6＝9.30700×10 -6 A 8＝-3.76459×10 -6
A 10＝5.20840×10 -7
The 17th
K＝0.000
A 4＝1.55240×10 -5 A 6＝1.05486×10 -5 A 8＝-3.44689×10 -7
A 10＝5.43477×10 -9
The zoom data, (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.11 4.54 4.94
2ω(°) 80.14 35.40 17.62
d 4 0.73 4.73 13.26
d 10 10.87 3.73 0.66
d 16 2.77 8.48 10.09
d 18 2.86 3.06 2.97
Embodiment 3
r 1＝24.343 d 1＝0.80 n d1＝1.92286 v d1＝18.90
r 2＝16.189 d 2＝0.16
r 3＝17.639 d 3＝3.05 n d2＝1.88300 v d2＝40.76
r 4=598.304 d 4=variable
r 5＝-58.725(AS) d 5＝0.82 n d3＝1.88300 v d3＝40.76
r 6＝6.041(AS) d 6＝2.60
r 7＝407.018 d 7＝2.01 n d4＝2.00170 v d4＝20.64
r 8＝-14.787 d 8＝0.08
r 9=-13.762 d 9＝0.68 n d5＝1.83481 v d5＝42.71
r 10=-88.096 (AS) d 10=variable
r 11＝∞(S) d 11＝0.10
r 12＝5.462(AS) d 12＝2.70 n d6＝1.58913 v d6＝61.14
r 13＝-11.013(AS) d 13＝0.10
r 14＝5.530 d 14＝1.36 n d7＝1.59201 v d7＝67.02
r 15＝13.426 d 15＝0.80 n d8＝2.00069 v d8＝25.46
r 16=3.443 d 16=variable
r 17＝19.462(AS) d 17＝2.07 n d9＝1.74330 v d9＝49.33
r 18=-27.222 d 18=variable
r 19＝∞ d 19＝0.40 n d10＝1.54771 v d10＝62.84
r 20＝∞ d 20＝0.50
r 21＝∞ d 21＝0.50 n d11＝1.51633 v d11＝64.14
r 22＝∞ d 22＝0.36
r 23＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝1.78466×10 -4 A 6＝-8.17272×10 -6 A 8＝2.01295×10 -7
A 10＝-1.77746×10 -9
The 6th
K＝0.000
A 4＝5.13913×10 -5 A 6＝2.24397×10 -5 A 8＝-1.94651×10 -6
A 10＝5.11678×10 -8
The 10th
K＝11.427
A 4＝-2.56902×10 -4 A 6＝-1.57604×10 -6 A 8＝-1.15551×10 -7
A 10＝0
The 12nd
K＝-0.000
A 4＝-9.39293×10 -4 A 6＝-5.83997×10 -6 A 8＝-2.22901×10 -6
A 10＝3.45022×10 -7
The 13rd
K＝0.000
A 4＝5.38804×10 -4 A 6＝3.49744×10 -6 A 8＝-2.93189×10 -6
A 10＝4.74550×10 -7
The 17th
K＝0.000
A 4＝2.27544×10 -5 A 6＝1.04163×10 -5 A 8＝-3.36814×10 -7
A 10＝5.32127×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.11 4.62 4.92
2ω(°) 80.16 35.55 17.62
d 4 0.73 4.28 13.31
d 10 10.93 3.71 0.72
d 16 2.76 8.74 9.98
d 18 2.84 3.04 2.97
Embodiment 4
r 1＝20.367 d 1＝0.80 n d1＝1.92286 v d1＝18.90
r 2＝15.608 d 2＝0.29
r 3＝17.741 d 3＝3.14 n d2＝1.76802 v d2＝49.24
r 4=3497.716 d 4=variable
r 5＝-45.639(AS) d 5＝0.80 n d3＝1.83481 v d3＝42.71
r 6＝5.950(AS) d 6＝2.73
r 7＝-255.106 d 7＝1.84 n d4＝1.92286 v d4＝18.90
r 8＝-15.843 d 8＝0.68 n d5＝1.83481 v d5＝42.71
r 9=-58.807 (AS) d 9=variable
r 10＝∞(S) d 10＝0.10
r 11＝5.586(AS) d 11＝2.70 n d6＝1.5913 v d6＝61.14
r 12＝-11.262(AS) d 12＝0.10
r 13＝5.436 d 13＝1.38 n d7＝1.59201 v d7＝67.02
r 14＝13.074 d 14＝0.80 n d8＝2.00069 v d8＝25.46
r 15=3.469 d 15=variable
r 16＝19.614(AS) d 16＝2.07 n d9＝1.74330 v d9＝49.33
r 17=-26.892 d 17=variable
r 18＝∞ d 18＝0.40 n d10＝1.54771 v d10＝62.84
r 19＝∞ d 19＝0.50
r 20＝∞ d 20＝0.50 n d11＝1.51633 v d11＝64.14
r 21＝∞ d 21＝0.36
r 22＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝2.17672×10 -4 A 6＝-5.32946×10 -6 A 8＝7.95875×10 -8
A 10＝-5.34232×10 -10
The 6th
K＝0.000
A 4＝1.20203×10 -4 A 6＝2.54566×10 -5 A 8＝-1.22695×10 -6
A 10＝2.02973×10 -8
The 9th
K＝19.659
A 4＝-2.47017×10 -4 A 6＝-1.58699×10 -6 A 8＝-1.04315×10 -7
A 10＝0
The 11st
K＝-0.000
A 4＝-8.71078×10 -4 A 6＝-4.22508×10 -7 A 8＝-1.92565×10 -6
A 10＝3.14754×10 -7
The 12nd
K＝0.000
A 4＝5.15823×10 -4 A 6＝1.00484×10 -5 A 8＝-2.82400×10 -6
A 10＝4.47946×10 -7
The 16th
K＝0.000
A 4＝6.80361×10 -6 A 6＝1.09868×10 -5 A 8＝-3.72817×10 -7
A 10＝5.90895×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.05 4.41 4.82
2ω(°) 80.12 35.18 17.61
d 4 0.72 5.37 13.24
d 9 10.83 3.84 0.65
d 15 2.75 8.06 10.08
d 17 2.86 3.05 2.97
Embodiment 5
r 1＝25.173 d 1＝0.80 n d1＝1.92286 v d1＝18.90
r 2＝16.537 d 2＝0.20
r 3＝18.252 d 3＝3.06 n d2＝1.88300 v d2＝40.76
r 4=-4161.584 d 4=variable
r 5＝-44.093(AS) d 5＝0.80 n d3＝1.83481 v d3＝42.71
r 6＝6.129(AS) d 6＝2.67
r 7＝-897.611 d 7＝1.86 n d4＝1.92286 v d4＝18.90
r 8＝-16.194 d 8＝0.68 n d5＝1.83481 v d5＝42.71
r 9=-75.584 (AS) d 9=variable
r 10＝∞(S) d 10＝0.10
r 11＝5.515(AS) d 11＝2.70 n d6＝1.58913 v d6＝61.14
r 12＝-10.975(AS) d 12＝0.10
r 13＝5.494 d 13＝1.36 n d7＝1.59201 v d7＝67.02
r 14＝12.850 d 14＝0.80 n d8＝2.00069 v d8＝25.46
r 15=3.429 d 15=variable
r 16＝19.614(AS) d 16＝2.07 n d9＝1.74330 v d9＝49.33
r 17=-27.158 d 17=variable
r 18＝∞ d 18＝0.40 n d10＝1.54771 v d10＝62.84
r 19＝∞ d 19＝0.50
r 20＝∞ d 20＝0.50 n d11＝1.51633 v d11＝64.14
r 21＝∞ d 21＝0.36
r 22＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝2.01152×10 -4 A 6＝-5.53549×10 -6 A 8＝1.09307×10 -7
A 10＝-9.22389×10 -10
The 6th
K＝0.000
A 4＝1.24289×10 -4 A 6＝2.52204×10 -5 A 8＝-1.55015×10 -6
A 10＝3.87174×10 -8
The 9th
K＝15.880
A 4＝-2.56363×10 -4 A 6＝3.83459×10 -7 A 8＝-1.74921×10 -7
A 10＝0
The 11st
K＝-0.000
A 4＝-9.56239×10 -4 A 6＝-9.52999×10 -6 A 8＝-3.92591×10 -7
A 10＝1.39818×10 -7
The 12nd
K＝0.000
A 4＝4.88481×10 -4 A 6＝-6.29539×10 -6 A 8＝4.03797×10 -7
A 10＝1.15552×10 -7
The 16th
K＝0.000
A 4＝3.74250×10 -5 A 6＝1.03247×10 -5 A 8＝-3.43630×10 -7
A 10＝5.32503×10 -9
The zoom data ' (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.10 4.44 4.96
2ω(°)80.15 35.27 17.62
d 4 0.72 5.21 13.32
d 9 11.01 3.94 0.73
d 15 2.77 8.18 10.05
d 17 2.83 3.00 2.97
Embodiment 6
r 1＝23.739 d 1＝0.81 n d1＝1.94595 v d1＝17.98
r 2＝16.355 d 2＝0.21
r 3＝18.106 d 3＝3.01 n d2＝1.88300 v d2＝40.76
r 4=846.562 d 4=variable
r 5＝-52.113(AS) d 5＝0.82 n d3＝1.88300 v d3＝40.76
r 6＝6.190(AS) d 6＝2.65
r 7＝-235.098 d 7＝1.86 n d4＝1.94595 v d4＝17.98
r 8＝-15.562 d 8＝0.09
r 9＝-14.315 d 9＝0.80 n d5＝1.88300 v d5＝40.76
r 10=-41.886 (AS) d 10=variable
r 11＝(S) d 11＝0.10
r 12＝5.555(AS) d 12＝2.70 n d6＝1.58913 v d6＝61.14
r 13＝-10.974(AS) d 13＝0.10
r 14＝5.438 d 14＝1.38 n d7＝1.59201 v d7＝67.02.
r 15＝13.503 d 15＝0.80 n d8＝2.00069 v d8＝25.46
r 16=3.433 d 16=variable
r 17＝18.727(AS) d 17＝2.07 n d9＝1.74330 v d9＝49.33
r 18=-29.343 d 18=variable
r 19＝∞ d 19＝0.40 n d10＝1.54771 v d10＝62.84
r 20＝∞ d 20＝0.50
r 21＝∞ d 21＝0.50 n d11＝1.51633 v d11＝64.14
r 22＝∞ d 22＝0.37
r 23＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝2.02790×10 -4 A 6＝-6.36728×10 -6 A 8＝1.15320×10 -7
A 10＝-8.37226×10 -10
The 6th
K＝0.000
A 4＝8.20642×10 -5 A 6＝2.47151×10 -G A 8＝-1.53936×10 -6
A 10＝2.64133×10 -8
The 10th
K＝6.008
A 4＝-2.06900×10 -4 A 6＝-2.13247×10 -6 A 8＝1.58746×10 -8
A 10＝0
The 12nd
K＝-0.000
A 4＝-9.21086×10 -4 A 6＝-6.31048×10 -6 A 8＝-1.81135×10 -6
A 10＝2.67397×10 -7
The 13rd
K＝0.000
A 4＝4.87773×10 -4 A 6＝3.10768×10 -6 A 8＝-2.75976×10 -6
A 10＝3.94656×10 -7
The 17th
K＝0.000
A 4＝2.23802×10 -5 A 6＝1.07437×10 -5 A 8＝-3.4S358×10 -7
A 10＝5.42112×10 -9
The zoom data ' (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.12 4.57 4.94
2ω(°) 80.163 5.42 17.62
d 4 0.72 4.78 13.23
d 10 10.77 3.71 0.66
d 16 2.77 8.47 10.05
d 18 2.85 3.06 2.96
Embodiment 7
r 1＝23.679 d 1＝0.81 n d1＝1.94595 v d1＝17.98
r 2＝16.309 d 2＝0.20
r 3＝17.975 d 3＝3.03 n d2＝1.88300 v d2＝40.76
r 4=652.312 d 4=variable
r 5＝-57.513(AS) d 5＝0.82 n d3＝1.88300 v d3＝40.76
r 6＝6.169(AS) d 6＝2.64
r 7＝-172.005 d 7＝1.92 n d4＝2.10227 v d4＝17.10
r 8＝-18.412 d 8＝0.11
r 9＝-15.586 d 9＝0.80 n d5＝1.88300 v d5＝40.76
r 10=-47.805 (AS) d 10=variable
r 11＝∞(S) d 11＝0.10
r 12＝5.447(AS) d 12＝2.70 n d6＝1.58913 v d6＝61.14
r 13＝＝-10.900(AS) d 13＝0.10
r 14＝5.577 d 14＝1.35 n d7＝1.59201 v d7＝67.02
r 15＝13.324 d 15＝0.80 n d8＝2.00069 v d8＝25.46
r 16=3.452 d 16=variable
r 17＝19.617(AS) d 17＝2.07 n d9＝1.74330 v d9＝49.33
r 18=-26.823 d 18=variable
r 19＝∞ d 19＝0.40 n d10＝1.54771 v d10＝62.84
r 20＝∞ d 20＝0.50
r 21＝∞ d 21＝0.50 n d11＝1.51633 v d11＝64.14
r 22＝∞ d 22＝0.36
r 23＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝2.08796×10 -4 A 6＝-7.65961×10 -6 A 8＝1.42959×10 -7
A 10＝-1.03287×10 -9
The 6th
K＝0.000
A 4＝9.25739×10 -5 A 6＝2.37928×10 -5 A 8＝-1.56581×10 -6
A 10＝2.33770×10 -8
The 10th
K＝13.662
A 4＝-2.04807×10 -4 A 6＝-2.93679×10 -6 A 8＝7.51268×10 -8
A 10＝0
The 12nd
K＝-0.000
A 4＝-9.47047×10 -4 A 6＝-9.73137×10 -6 A 8＝-9.44664×10 -7
A 10＝2.30496×10 -7
The 13rd
K＝0.000
A 4＝5.55221×10 -4 A 6＝-3.16660×10 -6 A 8＝-3.51784×10 -7
A 10＝2.04855×10 -7
The 17th
K＝0.000
A 4＝2.11262×10 -5 A 6＝1.08100×10 -5 A 8＝-3.55468×10 -7
A 10＝5.58942×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.11 4.57 4.91
2ω(°) 80.18 35.47 17.61
d 4 0.72 4.59 13.25
d 10 10.75 3.70 0.68
d 16 2.76 8.58 9.98
d 18 2.86 3.06 2.97
Embodiment 8
r 1＝23.572 d 1＝0.81 n d1＝1.94595 v d1＝17.98
r 2＝16.325 d 2＝0.19
r 3＝17.924 d 3＝3.08 n d2＝1.88300 v d2＝40.76
r 4=481.040 d 4=variable
r 5＝-63.672(AS) d 5＝0.82 n d3＝1.88300 v d3＝40.76
r 6＝6.059(AS) d 6＝2.72
r 7＝-238.294 d 7＝1.87 n d4＝2.10227 v d4＝17.10
r 8＝-19.462 d 8＝0.80 n d5＝1.88300 v d5＝40.76
r 9=-90.854 (AS) d 9=variable
r 10＝∞(S) d 10＝0.10
r 11＝5.548(AS) d 11＝2.70 n d6＝1.5S913 v d6＝61.14
r 12＝-11.217(AS) d 12＝0.10
r 13＝5.502 d 13＝1.39 n d7＝1.59201 v d7＝67.02
r 14＝13.285 d 14＝0.80 n d8＝2.00069 v d8＝25.46
r 15=3.476 d 15=variable
r 16＝19.903(AS) d 16＝2.07 n d9＝1.74330 v d9＝49.33
r 17=-26.017 d 17=variable
r 18＝∞ d 18＝0.40 n d10＝1.54771 v d10＝62.84
r 19＝∞ d 19＝0.50
r 20＝∞ d 20＝0.50 n d11＝1.51633 v d11＝64.14
r 21＝∞ d 21＝0.36
r 22＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝2.11173×10 -4 A 6＝-8.21005×10 -6 A 8＝1.62208×10 -7
A 10＝-1.25817×10 -9
The 6th
K＝0.000
A 4＝1.55260×10 -4 A 6＝2.35459×10 -5 A 8＝-1.47843×10 -6
A 10＝2.40340×10 -8
The 9th
K＝13.988
A 4＝-2.46764×10 -4 A 6＝-3.00682×10 -6 A 8＝1.43307×10 -8
A 10＝0
The 11st
K＝-0.000
A 4＝-8.70152×10 -4 A 6＝2.07452×10 -6 A 8＝-2.51898×10 -8
A 10＝3.52050×10 -7
The 12nd
K＝0.000
A 4＝5.43211×10 -4 A 6＝1.77046×10 -5 A 8＝-4.53251×10 -6
A 10＝5.84184×10 -7
The 16th
K＝0.000
A 4＝1.55829×10 -5 A 6＝1.00684×10 -5 A 8＝-3.25292×10 -7
A 10＝5.11814×10 -9
The zoom data | (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.03 4.45 4.73
2ω(°) 80.16 35.27 17.59
d 4 0.72 5.02 13.27
d 9 10.82 3.84 0.72
d 15 2.75 8.31 9.95
d 17 2.86 3.04 2.97
Embodiment 9
r 1＝21.524 d 1＝0.80 n d1＝1.92286 v d1＝18.90
r 2＝15.990 d 2＝0.25
r 3＝18.038 d 3＝3.04 n d2＝1.80400 v d2＝46.57
r 4=1821.002 d 4=variable
r 5＝-46.956(AS) d 5＝0.79 n d3＝1.80610 v d3＝40.92
r 6＝5.863(AS) d 6＝2.76
r 7＝-178.037 d 7＝1.90 n d4＝1.92286 v d4＝18.90
r 8＝-14.340 d 8＝0.67 n d5＝1.80610 v d5＝40.92
r 9=-72.767 (AS) d 9=variable
r 10＝∞(S) d 10＝0.10
r 11＝5.470(AS) d 11＝2.70 n d6＝1.58913 v d6＝61.14
r 12＝-11.162(AS) d 12＝0.10
r 13＝5.576 d 13＝1.36 n d7＝1.59201 v d7＝67.02
r 14＝13.756 d 14＝0.80 n d8＝2.00069 v d8＝25.46
r 15=3.493 d 15=variable
r 16＝19.520(AS) d 16＝2.07 n d9＝1.74330 v d9＝49.33
r 17=-27.248 d 17=variable
r 18＝∞ d 18＝0.40 n d10＝1.54771 v d10＝62.84
r 19＝∞ d 19＝0.50
r 20＝∞ d 20＝0.50 n d11＝1.51633 v d11＝64.14
r 21＝∞ d 21＝0.36
r 22＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝2.34682×10 -4 A 6＝-7.08038×10 -6 A 8＝1.25390×10 -7
A 10＝-9.36786×10 -10
The 6th
K＝0000
A 4＝1.52904×10 -4 A 6＝2.55798×10 -5 A 8＝-1.41637×10 -6
A 10＝2.87416×10 -8
The 9th
K＝4.725
A 4＝-2.74195×10 -4 A 6＝-1.46147×10 -6 A 8＝-1.44866×10 -7
A 10＝0
The 11st
K＝-0.000
A 4＝-9.07011×10 -4 A 6＝6.10900×10 -6 A 8＝-3.38866×10 -6
A 10＝4.78449×10 -7
The 12nd
K＝0.000
A 4＝5.63212×10 -4 A 6＝2.36073×10 -5 A 8＝-6.03623×10 -6
A 10＝8.08280×10 -7
The 16th
K＝0.000
A 4＝1.27541×10 -5 A 6＝1.11474×10 -5 A 8＝-3.87618×10 -7
A 10＝6.24145×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.11 4.45 4.93
2ω(°) 80.13 35.19 17.61
d 4 0.72 5.33 13.27
d 9 10.94 3.89 0.69
d 15 2.76 8.08 10.07
d 17 2.86 3.05 2.97
Embodiment 10
r 1＝21.929 d 1＝0.81 n d1＝1.94595 v d1＝17.98
r 2＝15.886 d 2＝3.02 n d2＝1.83481 v d2＝42.71
r 3=87.110 d 3=variable
r 4＝-603.712(AS) d 4＝0.82 n d3＝1.8S300 v d3＝40.76
r 5＝5.962(AS) d5＝2.72
r 6＝108.526 d 6＝1.76 n d4＝2.10227 v d4＝17.10
r 7＝-23.243 d 7＝0.16
r 8＝-17.863 d 8＝0.80 n d5＝1.88300 v d5＝40.76
r 9=-201.302 (AS) d 9=variable
r 10＝∞(S) d 10＝0.10
r 11＝5.737(AS) d 11＝2.70 r d6＝1.58913 v d6＝61.14
r 12＝-10.526(AS) d 12＝0.10
r 13＝5.184 d 13＝1.42 n d7＝1.59201 v d7＝67.02
r 14＝12.685 d 14＝0.80 n d8＝2.00069 v d8＝25.46
r 15=3.389 d 15=variable
r 16＝28.421(AS) d 16＝2.07 n d9＝1.74330 v d9＝49.33
r 17=-19.743 d 17=variable
r 18＝∞ d 18＝0.40 n d10＝1.54771 v d10＝62.84
r 19＝∞ d 19＝0.50
r 20＝∞ d 20＝0.50 n d11＝1.51633 v d11＝64.14
r 21＝∞ d 21＝0.35
r 22＝∞(I)
Asphericity coefficient
The 4th
K＝0.000
A 4＝1.17638×10 -4 A 6＝-1.87398×10 -6 A 8＝-1.21415×10 -8
A 10＝3.25687×10 -10
The 5th
K＝0.000
A 4＝9.74365×10 -5 A 6＝1.86507×10 -5 A 8＝-6.27883×10 -7
A 10＝-6.71787×10 -9
The 9th
K＝300.320
A 4＝-2.68737×10 -4 A 6＝-2.18216×10 -8 A 8＝-4.79877×10 -8
A 10＝0
The 11st
K＝-0.000
A 4＝-9.41932×10 -4 A 6＝-1.82332×10 -5 A 8＝9.47875×10 -7
A 10＝1.96272×10 -7
The 12nd
K＝0.000
A 4＝4.34113×10 -4 A 6＝-1.86904×10 -5 A 8＝-3.97394×10 -7
A 10＝1.70317×10 -7
The 16th
K＝0.000
A 4＝2.98825×10 -5 A 6＝7.00636×10 -6 A 8＝-2.06857×10 -7
A 10＝3.08660×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.03 4.93 4.99
2ω(°) 80.21 36.18 17.76
d 8 0.74 0.99 13.31
d 9 11.18 3.27. 0.898
d 15 2.71 9.95 10.21
d 17 2.64 2.99 2.99
Embodiment 11
r 1＝19.964 d 1＝0.80 n d1＝1.92286 v d1＝18.90
r 2＝15.354 d 2＝0.22
r 3＝16.981 d 3＝3.10 n d2＝1.76802 v d2＝49.24
r 4=321.532 d 4=variable
r 5＝-79.400(AS) d 5＝0.82 n d3＝1.88300 v d3＝40.76
r 6＝6.026(AS) d 6＝2.65
r 7＝-512.296 d 7＝2.00 n d4＝2.00170 v d4＝20.64
r 8＝-14.190 d 8＝0.13
r 9＝-10.837(AS) d 9＝0.67 n d5＝1.81600 v d5＝46.62
r 10=-38.820 d 10=variable
r 11＝∞(S) d 11＝0.10
r 12＝5.567(AS) d 12＝2.70 n d6＝1.58913 v d6＝61.14
r 13＝-10.835(AS) d 13＝0.10
r 14＝5.426 d 14＝1.39 n d7＝1.59201 v d7＝67.02
r 15＝13.374 d 15＝0.80 n d8＝2.00069 v ds＝25.46
r 16=3.434 d 16=variable
r 17＝21.181(AS) d 17＝2.07 n d9＝1.74330 v d9＝49.33
r 18=-23.592 d 18=variable
r 19＝∞ d 19＝0.40 n d10＝1.54771 v d10＝62.84
r 20＝∞ d 20＝0.50
r 21＝∞ d 21＝0.50 n d11＝1.51633 v d11＝64.14
r 22＝∞ d 22＝0.36
r 23＝∞(I)
Aspheric surface system
The 5th
K＝0.000
A 4＝1.81913×10 -4 A 6＝-7.45514×10 -6 A 8＝1.16696×10 -7
A 10＝-6.24258×10 -10
The 6th
K＝0.000
A 4＝3.02384×10 -5 A 6＝2.11070×10 -5 A 8＝-1.27196×10 -6
A 10＝4.98377×10 -9
The 9th
K＝-0.063
A 4＝2.66985×10 -4 A 6＝5.08873×10 -6 A 8＝-1.46937×10 -7
A 10＝0
The 12nd
K＝-0.000
A 4＝-9.20807×10 -4 A 6＝-4.91248×10 -6 A 8＝-3.02284×10 -6
A 10＝3.84485×10 -7
The 13rd
K＝0.000
A 4＝5.02906×10 -4 A 6＝7.33058×10 -6 A 8＝-5.38763×10 -6
A 10＝6.41876×10 -7
The 17th
K＝0.000
A 4＝2.80646×10 -6 A 6＝1.03678×10 -5 A 8＝-3.21345×10 -7
A 10＝4.86255×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.09 4.69 4.91
2ω(°) 80.15 35.68 17.65
d 4 0.73 3.65 13.26
d 10 10.76 3.56 0.77
d 16 2.74 9.08 10.01
d 18 2.81 3.04 2.97
Embodiment 12
r 1＝20.035 d 1＝0.80 n d1＝1.92286 v d1＝18.90
r 2＝15.388 d 2＝0.21
r 3＝16.987 d 3＝3.10 n d2＝1.76802 v d2＝49.24
r 4=322.739 d 4=variable
r 5＝-67.042(AS) d 5＝0.82 n d3＝1.88300 v d2＝40.76
r 6＝6.104(AS) d 6＝2.63
r 7＝-553.055 d 7＝2.02 n d4＝2.00170 v d4＝20.64
r 8＝-14.110 d 8＝0.17
r 9＝-11.468(AS) d 9＝0.67 n d5＝1.81600 v d5＝46.62
r 10=-48.428 (AS) d 10=variable
r 11＝∞(S) d 11＝0.10
r 12＝5.592(AS) d 12＝2.70 n d6＝1.58913 v d6＝61.14
r 13＝-10.777(AS) d 13＝0.10
r 14＝5.381 d 14＝1.39 n d7＝1.59201 v d7＝67.02
r 15＝13.633 d 15＝0.80 n d8＝2.00069 v d8＝25.46
r 16=3.428 d 16=variable
r 17＝21.377(AS) d 17＝2.07 n d9＝1.74330 v d9＝49.33
r 18=-23.467 d 18=variable
r 19＝∞ d 19＝0.40 n d10＝1.54771 v d10＝62.84
r 20＝∞ d 20＝0.50
r 21＝∞ d 21＝0.50 n d11＝1.51633 v d11＝64.14
r 22＝∞ d 22＝0.36
r 23＝∞(I)
Asphericity coefficient
The 5th
K＝0.000.
A 4＝2.02227×10 -4 A 6＝-8.03922×10 -6 A 8＝1.51641×10 -7
A 10＝-1.06462×10 -9
The 6th
K＝0.000
A 4＝3.98938×10 -5 A 6＝1.96692×10 -5 A 8＝-1.68354×10 -6
A 10＝2.76679×10 -8
The 9th
K＝-0.063
A 4＝2.07247×10 -5 A 6＝-3.77371×10 -6 A 8＝2.63786×10 -7
A 10＝0
The 10th
K＝-0.897
A 4＝-2.19314×10 4 A 6＝-5.31018×10 -6 A 8＝3.15789×10 -7
A 10＝0
The 12nd
K＝-0.000
A 4＝-9.35871×10 -4 A 6＝-1.13973×10 -5 A 8＝-7.24228×10 -7
A 10＝1.19444×10 -7
The 13rd
K＝0.000
A 4＝4.83658×10 -4 A 6＝-9.01954××10 -6 A 8＝1.55326×10 -7
A 10＝4.11169×10 -8
The 17th
K＝0.000
A 4＝8.51281×10 -6 A 6＝9.83773×10 -6 A 8＝-3.17684×10 -7
A 10＝5.22025×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.09 4.69 4.92
2ω(°)80.14 35.67 17.64
d 4 0.73 3.64 13.26
d 10 10.77 3.56 0.77
d 16 2.74 9.08 10.02
d 18 2.80 3.03 2.97
Embodiment 13
r 1＝24.847 d 1＝0.80 n d1＝1.94595 v d1＝17.98
r 2＝16.542 d 2＝0.29
r 3＝18.208 d 3＝3.02 n d2＝1.88300 v d2＝40.76
r 4=3582.698 d 4=variable
r 5＝-43.179(AS) d 5＝0.79 n d3＝1.80610 v d3＝40.92
r 6＝5.891(AS) d 6＝2.64
r 7＝-157590.062 d 7＝1.91 n d4＝1.94595 v d4＝17.98
r 8＝-15.395 d 8＝0.67 n d5＝1.80610 v d5＝40.92
r 9=-175.340 (AS) d 9=variable
r 10＝∞(S) d 10＝0.10
r 11＝5.417(AS) d 11＝2.70 n d6＝1.58913 v d6＝61.14
r 12=-10.144 (AS) d 12=variable
r 13＝5.942 d 13＝1.42 n d7＝1.59201 v d7＝67.02
r 14＝24.078 d 14＝0.80 n d8＝2.00069 v d8＝25.46
r 15=3.618 d 15=variable
r 16＝17.723(AS) d 16＝2.07 n d9＝1.74330 v d9＝49.33
r 17=-30.024 d 17=variable
r 18＝∞ d 18＝0.40 n d10＝1.54771 v d10＝62.84
r 19＝∞ d 19＝0.50
r 20＝∞ d 20＝0.50 n d11＝1.51633 v d11＝64.14
r 21＝∞ d 21＝0.36
r 22＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝2.41650×10 -4 A 6＝-7.80486×10 -6 A 8＝1.53963×10 -7
A 10＝-1.21087×10 -9
The 6th
K＝0.000
A 4＝1.85981×10 -4 A 6＝2.55754×10 -5 A 8＝-1.92596×10 -6
A 10＝3.81224×10 -8
The 9th
K＝-4.077
A 4＝-3.33609×10 -4 A 6＝6.19746×10 -6 A 8＝-2.40693×10 -7
A 10＝4.21649×10 -10
The 11st
K＝-0.000
A 4＝-1.00640×10 -3 A 6＝2.89626×10 -5 A 8＝-5.10096×10 -6
A 10＝7.01287×10 -7
The 12nd
K＝0.000
A 4＝6.92460×10 -4 A 6＝4.80286×10 -5 A 8＝-9.42465×10 -6
A 10＝1.22823×10 -6
The 16th
K＝0.000
A 4＝3.67077×10 -5 A 6＝1.07760×10 -5 A 8＝-3.84914×10 -7
A 10＝6.38037×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 12.00 24.28
F NO 3.23 4.54 5.07
2ω(°) 80.19 35.07 17.60
d 4 0.71 5.09 13.51
d 9 10.96 3.46 0.85
d 12 0.20 0.57 0.40
d 15 2.75 7.12 9.46
d 17 2.80 2.94 2.96
Embodiment 14
r 1＝19.959 d 1＝0.80 n d1＝1.92286 v d1＝18.90
r 2＝15.153 d 2＝0.19
r 3＝16.567 d 3＝3.19 n d2＝1.76802 v d2＝49.24
r 4=328.834 d 4=variable
r 5＝-66.705(AS) d 5＝0.82 n d3＝1.88300 v 63＝40.76
r 6＝6.014(AS) d 6＝2.67
r 7＝-97.974 d 7＝1.95 n d4＝2.00170 v d4＝20.64
r 8＝-12.905 d 8＝0.12
r 9＝-10.476(AS) d 9＝0.67 n d5＝1.81600 v d5＝46.62
10=-36.471 d 10=variable |
r 11＝∞(S) d 11＝0.10
r 12＝5.598(AS) d 12＝2.70 n d6＝1.58913 v d6＝61.14
r 13=-10.200 (AS) d 13=variable
r 14＝5.893 d 14＝1.42 n d7＝1.59201 v d7＝67.02
r 15＝20.687 d 15＝0.80 n d8＝2.00069 v d8＝25.46
r 16=3.680 d 16=variable |
r 17＝18.589(AS) d 17＝2.07 n d9＝1.74330 v d9＝49.33
r 18=-26.724 d 18=variable
r 19＝∞ d 19＝0.40 n d10＝1.54771 v d10＝62.84
r 20＝∞ d 20＝0.50
r 21＝∞ d 21＝0.50 n d11＝1.51633 v d11＝64.14
r 22＝∞ d 22＝0.36
r 23＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝1.92323×10 -4 A 6＝-4.86162×10 -6 A 8＝5.55922×10 -8
A 10＝-2.22548×10 -10
The 6th
K＝0.000
A 4＝9.52228×10 -5 A 6＝2.45561×10 -5 A 8＝-1.19859×10 -6
A 10＝6.02161×10 -9
The 9th
K＝0.020
A 4＝3.06753×10 -4 A 6＝-6.37184×10 -7 A 8＝2.66117×10 -8
A 10＝0
The 12nd
K＝-0.000
A 4＝-9.26843×10 -4 A 6＝3.04592×10 -5 A 8＝-6.90151×10 -6
A 10＝7.46676×10 -7
The 13rd
K＝0.000
A 4＝6.28294×10 -4 A 6＝5.21648×10 -6 A 8＝-1.31953×10 -5
A 10＝1.46113×10 -6
The 17th
K＝0.000
A 4＝-6.81284×10 -6 A 6＝1.02822×10 -5 A 8＝-3.09403×10 -7
A 10＝4.47496×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.13 4.50 4.92
2ω(°) 80.23 35.24 17.60
d 4 0.72 4.62 13.21
d 10 10.56 3.30 0.78
d 13 0.23 0.57 0.43
d 16 2.76 7.67 9.68
d 18 2.86 3.00 2.96
Embodiment 15
r 1＝25.601 d 1＝0.80 n d1＝1.92286 v d1＝18.90
r 2＝16.493 d 2＝0.20
r 3＝18.075 d 3＝3.23 n d2＝1.88300 v d2＝40.76
r 4=-1234.242 d 4=variable
r 5＝-40.268(AS) d 5＝0.80 n d3＝1.83481 v d3＝42.71
r 6＝6.022(AS) d 6＝2.62
r 7＝-407.214 d 7＝1.83 n d4＝1.92286 v d4＝18.90
r 8＝-15.866 d 8＝0.68 n d5＝1.83481 v d5＝42.71
r 9=-66.674 (AS) d 9=variable
r 10＝∞(S) d 10＝0.10
r 11＝5.520(AS) d 11＝2.70 n d6＝1.58913 v d6＝61.14
r 12=-9.949 (AS) d 12=variable
r 13＝6.163 d 13＝1.35 n d7＝1.59201 v d7＝67.02
r 14＝18.256 d 14＝0.80 n d8＝2.00069 v d8＝25.46
r 15=3.675 d 15=variable
r 16＝15.963(AS) d 16＝2.07 n d9＝1.74330 v d9＝49.33
r 17=-38.145 d 17=variable
r 18＝∞ d 18＝0.40 n d10＝1.54771 v d10＝62.84
r 19＝∞ d 19＝0.50
r 20＝∞ d 20＝0.50 n d11＝1.51633 v d11＝64.14
r 21＝∞ d 21＝0.37
r 22＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝2.05163×10 -4 A 6＝-3.37326×10 -6 A 8＝4.45283×10 -8
A 10＝-3.62203×10 -10
The 6th
K＝0.000
A 4＝1.47479×10 -4 A 6＝2.72737×10 -5 A 8＝-1.43607×10 -6
A 10＝3.29097×10 -8
The 9th
K＝17.341
A 4＝-2.82382×10 -4 A 6＝3.16842×10 -6 A 8＝-2.28861×10 -7
A 10＝0
The 11st
K＝-0.000
A 4＝-1.03741×10 -3 A 6＝2.15062×10 -5 A 8＝-6.81878×10 -6
A 10＝7.72131×10 -7
The 12nd
K＝0.000
A 4＝5.90361×10 -4 A 6＝4.12917×10 -5 A 8＝-1.28212×10 -5
A 10＝1.50309×10 -6
The 16th
K＝0.000
A 4＝2.50156×10 -5 A 6＝1.12904×10 -5 A 8＝-3.91013×10 -7
A 10＝6.07074×10 -9
The zoom data ' (∞)
WE ST TE
f(mm) 5.06 12.00 24.29
F NO 3.13 4.24 4.94
2ω(°) 80.27 34.6 817.58
d 4 0.71 6.26 13.33
d 9 10.81 3.63 0.72
d 12 0.27 0.57 0.42
d 15 2.76 6.65 9.78
d 17 2.83 3.00 2.96
Embodiment 16
r 1＝21.193 d 1＝0.81 n d1＝1.94595 v d1＝17.98
r 2＝15.192 d 2＝3.09 n d2＝1.83481 v d2＝42.71
r 3=81.748 d 3=variable
r 4＝-603.712(AS) d 4＝0.82 n d3＝1.88300 v d3＝40.76
r 5＝5.982(AS) d 5＝2.78
r 6＝-237.176 d 6＝1.71 n d4＝2.10227 v d4＝17.10
r 7＝-18.101 d 7＝0.09
r 8＝-15.997 d 8＝0.80 n d5＝1.88300 v d5＝40.76
r 9=-168.381 (AS) d 9=variable |
r 10＝∞(S) d 10＝0.10
r 11＝5.812(AS) d 11＝2.70 n d6＝1.58913 v d6＝61.14
r 12=-10.295 (AS) d 12=variable |
r 13＝5.387 d 13＝1.54 n d7＝1.59201 v d7＝67.02
r 14＝19.283 d 14＝0.80 n d8＝2.00069 v d8＝25.46
r 15=3.554 d 15=variable
r 16＝24.991(AS) d 16＝2.07 n d9＝1.74330 v d9＝49.33
r 17=-19.483 d 17=variable |
r 18＝∞ d 18＝0.40 n d10＝1.54771 v d10＝62.84
r 19＝∞ d 19＝0.50
r 20＝∞ d 20＝0.50 n d11＝1.51633 v d11＝64.14
r 21＝∞ d 21＝0.35
r 22＝∞(I)
Asphericity coefficient
The 4th
K＝0.000
A 4＝1.21970×10 -4 A 6＝-1.08084×10 -6 A 8＝-1.14600×10 -8
A 10＝1.97222×10 -10
The 5th
K＝0.000
A 4＝1.75555×10 -4 A 6＝2.16172×10 -5 A 8＝-8.70023×10 -7
A 10＝1.24313×10 -8
The 9th
K＝410.383
A 4＝-2.79644×10 -4 A 6＝4.80703×10 -6 A 8＝-2.06609×10 -7
A 10＝0
The 11st
K＝-0.000
A 4＝-8..72572×10 -4 A 6＝1.99478×10 -5 A 8＝-4.51334×10 -6
A 10＝5.24324×10 -7
The 12nd
K＝0.000
A 4＝5.50797×10 -4 A 6＝2.74834×10 -5 A 8＝-6.52190×10 -6
A 10＝7.69571×10 -7
The 16th
K＝0.000
A 4＝1.78974×10 -6 A 6＝7.85039×10 -6 A 8＝-2.65852×10 -7
A 10＝4.28825×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.08 4.93 4.91
2ω(°) 80.33 36.11 17.66
d 3 0.74 1.00 13.34
d 9 10.94 3.05 0.89
d 12 0.16 0.57 0.55
d 15 2.75 9.30 9.26
d 17 2.70 3.00 2.99
Embodiment 17
r 1＝24.005 d 1＝0.80 n d1＝1.92286 v d1＝18.90
r 2＝15.730 d 2＝0.18
r 3＝16.798 d 3＝3.12 n d2＝1.88300 v d2＝40.76
r 4=320.063 d 4=variable
r 5＝-63.961(AS) d 5＝0.80 n d3＝1.83481 v d3＝42.71
r 6＝5.769(AS) d 6＝2.79
r 7＝-110.876 d 7＝1.74 n d4＝1.94595 v d4＝17.98
r 8＝-15.935 d 8＝0.08
r 9＝-14.478 d 9＝0.68 n d5＝1.83481 v d5＝42.71
r 10=-43.168 (AS) d 10=variable
r 11＝∞(S) d 11＝0.10
r 12＝5.627(AS) d 12＝2.70 n d6＝1.58913 v d6＝61.14
r 13=-9.958 (AS) d 13=variable
r 14＝6.057 d 14＝1.36 n d7＝1.59201 v d7＝67.02
r 15＝18.994 d 15＝0.80 n d8＝2.00069 v d8＝25.46
r 16=3.702 d 16=variable
r 17＝16.931(AS) d 17＝2.07 n d9＝1.74330 v d9＝49.33
r 18=-33.088 d 18=variable
r 19＝∞ d 19＝0.40 n d10＝1.54771 v d10＝62.84
r 20＝∞ d 20＝0.50
r 21＝∞ d 21＝0.50 n d11＝1.51633 v d11＝64.14
r 22＝∞ d 22＝0.37
r 23＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝2.20322×10 -4 A 6＝-8.05410×10 -6 A 8＝1.50663×10 -7
A 10＝-1.08544×10 -9
The 6th
K＝0.000
A 4＝1.19766×10 -4 A 6＝2.71353×10 -5 A 8＝-1.79261×10 -6
A 10＝2.50985×10 -8
The 10th
K＝4.763
A 4＝-2.60503×10 -4 A 6＝-1.23050×10 -6 A 8＝2.35967×10 -8
A 10＝0
The 12nd
K＝-0.000
A 4＝-9.80569×10- 4 A 6＝1.94848×10 -5 A 8＝-5.98539×10 -6
A 10＝6.24092×10 -7
The 13rd
K＝0.000
A 4＝5.74317×10 -4 A 6＝3.99276×10 -5 A 8＝-1.14945×10 -5
A 10＝1.22736×10 -6
The 17th
K＝0.000
A 4＝8.72792×10 -7 A 6＝1.10477×10 -5 A 8＝-3.58880×10 -7
A 10＝5.71191×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.14 4.56 4.90
2ω(°) 80.18 35.40 17.59
d 4 0.73 4.26 13.29
d 10 10.70 3.25 0.68
d 13 0.29 0.58 0.46
d 16 2.76 7.98 9.63
d 18 2.86 3.05 2.96
Embodiment 18
r 1＝17.636(AS) d 1＝3.46 n d1＝1.49700 v d1＝81.54
r 2=1651.373 (AS) d 2=variable
r 3＝-89.845(AS) d 3＝0.82 n d2＝1.88300 v d2＝40.76
r 4＝6.252(AS) d 4=2.41
r 5＝36.538 d 5＝2.14 n d3＝1.94595 v d3＝17.98
r 6＝-20.686 d 6＝0.20
r 7＝-15.473 d 7＝0.70 n d4＝1.88300 v d4＝40.76
r 8=-705.490 (AS) d 8=variable
r 9＝∞(S) d 9＝0.10
r 10＝5.371(AS) d 10＝2.70 n d5＝1.58913 v d5＝61.14
r 11＝-12.630(AS) d 11＝0.10
r 12＝4.840 d 12＝1.30 n d6＝1.59201 v d6＝67.02
r 13＝8.993 d 13＝0.80 n d7＝2.00170 v d7＝20.64
r 14=3.169 d 14=variable
r 15＝-175.389(AS) d 15＝2.05 n d8＝2.00170 v d8＝20.64
r 16=-15.339 d 16=variable
r 17＝∞ d 17＝0.40 n d9＝1.54771 v d9＝62.84
r 18＝∞ d 18＝0.50
r 19＝∞ d 19＝0.50 n d10＝1.51633 v d10＝64.14
r 20＝∞ d 20＝0.36
r 21＝∞(I)
Asphericity coefficient.
The 1st
K＝-0.000
A 4＝-9.36696×10 -21 A 6＝-3.07965×10 7 A 8＝1.40121×10 -9
A 10＝8.27669×10 -11
The 2nd
K＝-0.000
A 4＝1.06767×10 -5 A 6＝-7.16715×10 -7 A 8＝1.70324×10 -8
A 10＝-3.34505×10 -11
The 3rd
K＝0.000
A 4＝4.52338×10 -5 A 6＝1.74362×10 -6 A 8＝-8.20880×10 -8
A 10＝1.09382×10 -9
The 4th
K＝0.000
A 4＝-5.26435×10 -5 A 6＝9.38403×10 -6 A 8＝-4.26308×10 -7
A 10＝1.16873×10 -8
The 8th
K＝-3.680
A 4＝-2.58689×10 -4 A 6＝7.09681×10 -6 A 8＝-7.55479×10 -7
A 10＝1.66474×10 -8
The 10th
K＝-0.000
A 4＝-8.26225×10 -4 A 6＝2.42650×10 -5 A 8＝-2.03186×10 -6
A 10＝2.44772×10 -7
The 11st
K＝0.000
A 4＝6.51537×10 -4 A 6＝4.56976×10 -5 A 8＝-3.58200×10 -6
A 10＝4.02796×10 -7
The 15th
K＝0.000
A 4＝8.11366×10 -8 A 6＝1.01901×10 -5 A 8＝-3.84282×10 -7
A 10＝5.33610×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 11.98 24.29
F NO 3.03 4.41 5.05
2ω(°) 81.54 36.13 18.37
d 2 0.72 4.69 12.81
d 8 11.55 4.15 0.93
d 14 2.78 7.77 10.07
d 16 2.78 2.99 3.33
Embodiment 19
r 1＝15.057(AS) d 1＝3.36 n d1＝1.43875 v d1＝94.93
r 2=16740.605 (AS) d 2=variable
r 3＝-109.482(AS) d 3＝0.82 n d2＝1.88300 v d2＝40.76
r 4＝5.865(AS) d 4＝2.48
r 5＝29.434 d 5＝2.25 n d3＝1.94595 v d3＝17.98
r 6＝-21.699 d 6＝0.26
r 7＝-15.455 d 7＝0.70 n d4＝1.88300 v d4＝40.76
r 8=61494.611 (AS) d 8=variable
r 9＝∞(S) d 9＝0.10
r 10＝5.519(AS) d 10＝2.70 n d5＝1.58913 v d5＝61.14
r 11＝-12.178(AS) d 11＝0.10
r 12＝4.874 d 12＝1.36 n d6＝1.59201 v d6＝67.02
r 13＝9.784 d 13＝0.80 n d7＝2.00170 v d7＝20.64
r 14=3.227 d 14=variable
r 15＝-455.052(AS) d 15＝2.04 n d8＝2.00170 v d8＝20.64
r 16=-15.796 d 16=variable
r 17＝∞ d 17＝0.40 n d9＝1.54771 v d9＝62.84
r 18＝∞ d 18＝0.50
r 19＝∞ d 19＝0.50 n d10＝1.51633 v d10＝64.14
r 20＝∞ d 20＝0.36
r 21＝∞(I)
Asphericity coefficient
The 1st
K＝-0.000
A 4＝-9.36696×10 -21 A 6＝-2.82322×10 -7 A 8＝-3.32314×10 -9
A 10＝9.80939×10 -11
The 2nd
K＝-0.000
A 4＝2.03046×10 -5 A 6＝-8.63339×10 -7 A 8＝1.39119×10 -8
A 10＝-2.72606×10 -11
The 3rd
K＝0.000
A 4＝1.45879×10 -4 A 6＝-7.06884×10 -6 A 8＝1.23121×10 -7
A 10＝-5.62979×10 -10
The 4th
K＝0.000
A 4＝-5.29316×10 -5 A 6＝3.56817×10 -6 A 8＝1.11723×10 -6
A 10＝1.49013×10 -8
The 8th
K＝-3.680
A 4＝-2.43119×10 -4 A 6＝1.50423×10 -6 A 8＝-8.73464×10 -8
A 10＝2.80319×10 -9
The 10th
K＝-0.000
A 4＝-7.77230×10 -4 A 6＝1.47499×10 -5 A 8＝-1.23145×10 -6
A 10＝1.55776×10 -7
The 11st
K＝0.000
A 4＝6.35918×10 -4 A 6＝3.49158×10 -5 A 8＝-2.91520×10 -6
A 10＝2.80196×10 -7
The 15th
K＝0.000
A 4＝4.02871×10 -5 A 6＝1.18379×10 -5 A 8＝-4.08960×10 -7
A 10＝5.70846×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 11.98 24.29
F NO 3.11 4.53 5.05
2ω(°) 81.61 36.13 18.35
d 2 0.72 4.72 12.77
d 8 11.25 4.14 0.96
d 14 2.79 7.94 9.79
d 16 2.84 2.99 3.34
Embodiment 20
r 1＝24.617 d 1＝0.80 n d1＝1.94595 v d1＝17.98
r 2＝16.485 d 2＝0.34
r 3＝18.513 d 3＝3.03 n d2＝1.88300 v d2＝40.76
r 4=-1350.827 d 4=variable
r 5＝-39.777(AS) d 5＝0.79 n d3＝1.80610 v d3＝40.92
r 6＝5.736(AS) d 6＝2.50
r 7＝46.539 d 7＝1.93 n d4＝1.94595 v d4＝17.98
r 8＝-22.674 d 8＝0.64 n d5＝1.80610 v d5＝40.92
r 9=177.436 (AS) d 9=variable
r 10=∞ (S) d 10=variable
r 11＝5.325(AS) d 11＝2.70 n d6＝1.58913 v d6＝61.14
r 12＝-9.884(AS) d 12＝0.10
r 13＝6.305 d 13＝1.41 n d7＝1.59201 v d7＝67.02
r 14＝18.239 d 14＝0.80 n d8＝2.00069 v d8＝25.46
r 15=3.616 d 15=variable
r 16＝17.024(AS) d 16＝2.07 n d9＝1.74330 v d9＝49.33
r 17=34.757 d 17=variable
r 18＝∞ d 18＝0.40 n d10＝1.54771 v d10＝62.84
r 19＝∞ d 19＝0.50
r 20＝∞ d 20＝050 n d11＝1.51633 v d11＝64.14
r 21＝∞ d 21＝0.37
r 22＝∞(I)
Asphericity coefficient
The 5th
K＝0.000
A 4＝2.65294×10 -4 A 6＝-4.86067×10 -6 A 8＝-4.95916×10 -8
A 10＝1.45582×10 9
The 6th
K＝0.000
A 4＝1.22290×10 -4 A 6＝3.07865×10 -5 A 8＝-1.23246×10 -6
A 10＝-2.75048×10 -8
The 9th
K＝-4.077
A 4＝-3.44903×10 -4 A 6＝4.47305×10 -6 A 8＝-7.49149×10 -7
A 10＝2.89043×10 -8
The 11st
K＝-0.000
A 4＝-1.06943×10 -3 A 6＝1.88431×10 -5 A 8＝-3.97910×10 -6
A 10＝3.05632×10 -7
The 12nd
K＝0.000
A 4＝7.51908×10 -4 A 6＝1.59771×10 -5 A 8＝-2.43151×10 -6
A 10＝2.99982×10 -7
The 16th
K＝0.000
A 4＝2.22601×10 -5 A 6＝1.31566×10 -5 A 8＝-4.73811×10 -7
A 10＝7.81341×10 -9
Zoom data (∞)
WE ST TE
f(mm) 5.06 12.01 24.28
F NO 3.07 4.72 5.05
2ω(°) 80.13 35.38 17.61
d 4 0.71 4.88 13.53
d 9 9.86 4.07 0.85
d 10 1.54 0.22 0.28
d 15 2.73 8.32 9.66
d 17 2.75 2.95 2.96
Embodiment 21
r 1＝21.541 d 1＝0.81 n d1＝1.94595 v d1＝17.98
r 2＝15.611 d 2＝0.24
r 3＝15.754 d 3＝3.00 n d2＝1.83481 v d2＝42.71
r 4=86.752 d 4=variable
r 5＝689.472 d 5＝0.82 n d3＝1.88300 v d3＝40.76
r 6＝5.858(AS) d 6＝2.64
r 7＝187.160 d 7＝1.74 n d4＝2.10227 v d4＝17.10
r 8＝-20.892 d 8＝0.11
r 9＝-17.292 d 9＝0.80 n d5＝1.88300 v d5＝40.76
r 10=-218.644 (AS) d 10=variable
r 11＝∞(S) d 11＝0.10
r 12＝5.786(AS) d 12＝2.70 n d6＝1.58913 v d6＝61.14
r 13＝-10.671(AS) d 13＝0.10
r 14＝5.093 d 14＝1.45 n d7＝1.59201 v d7＝67.02
r 15＝13.011 d 15＝0.80 n d8＝2.00069 v d8＝25.46
r 16=3.389 d 16=variable
r 17＝26.835(AS) d 17＝2.07 n d9＝1.74330 v d9＝49.33
r 18=-20.472 d 18=variable
r 19＝∞ d 19＝0.40 n d10＝1.54771 v d10＝62.84
r 20＝∞ d 20＝0.50
r 21＝∞ d 21＝0.50 n d11＝1.51633 v d11＝64.14
r 22＝∞ d 22＝0.35
r 23＝∞(I)
Asphericity coefficient
The 6th
K＝0.000
A 4＝-8.01634×10 -6 A 6＝1.74636×10 -5 A 8＝-9.27328×10 -7
A 10＝8.36328×10 -9
The 10th
K＝335.081
A 4＝-2.97735×10 -4 A 6＝3.50224×10 -6 A 8＝-1.54842×10 -7
A 10＝0
The 12nd
K＝-0.000
A 4＝-9.17134×10 -4 A 6＝1.14404×10 -5 A 8＝-5.40338×10 -6
A 10＝5.59156×10 -7
The 13rd
K＝0.000
A 4＝4.20917×10 -4 A 6＝2.06348×10 -5 A 8＝-7.89133×10 -6
A 10＝8.16743×10 -7
The 17th
K＝0.000
A 4＝4.79555×10 -5 A 6＝7.02757×10 -6 A 8＝-2.32832×10 -7
A 10＝3.87420×10 -9
The zoom data | (∞)
WE ST TE
f(mm) 5.06 12.01 24.29
F NO 3.08 5.02 5.05
2ω(°) 80.75 36.31 17.82
d 4 0.74 0.99 13.33
d 10 11.11 3.28 0.91
d 16 2.72 9.93 10.06
d 18 2.60 2.99 2.99
Aberration diagram when Figure 22～Figure 42 represents respectively that the infintie object point of the foregoing description 1～21 focuses on.
In these aberration diagrams, (a) spherical aberration, astigmatism, distortion aberration and the ratio chromatism, of expression wide-angle side, (b) spherical aberration, astigmatism, distortion aberration and the ratio chromatism, of expression intermediateness, (c) spherical aberration, astigmatism, distortion aberration and the ratio chromatism, of expression telescope end.Among each figure, " FIY " represents maximum image height.
The value of the condition in the various embodiments described above then, is shown.
Embodiment 1 2 3 4 5 6 7
(1A) -0.794 -0.789 -0.798 -0.788 -0.804 -0.823 -0.822
(2A) 0.815 0.813 0.813 0.769 0.756 0.788 0.806
(3A) 0.017 0.056 -0.019 0.030 0.008 0.032 0.044
(4A) 2.0017 1.94595 2.0017 1.92286 1.92286 1.94595 2.10226
(5A) 20.6 18.0 20.6 18.9 18.9 18.0 17.1
(6A) 1.070 1.270 0.930 1.132 1.037 1.142 11240
(7A) 1.8830 1.8348 1.8830 1.8348 1.8348 1.8830 1.8830
(8A) 40.8 42.7 40.8 42.7 42.7 40.8 40.8
(9A) 1.8160 1.8348 1.8348 1.8348 1.8348 1.8880 1.8830
(10A) 46.6 42.7 42.7 42.7 42.7 40.8 40.8
(11A) -1.505 -1.976 -1.370 -1.738 -1.545 -2.038 1.967
(12A) 2.001 2.553 1.885 2.416 2.341 2.334 .2.477
(13A) 0.029 0.030 0.027 0.052 0.054 0.036 0.028
(13B) -0.007 -0.008 -0.006 -0.004 -0.001 -0.008 -0.008
(14A) -0.025 -0.021 -0.025 -0.025 -0.025 -0.019 -0.019
(15A) 0.008 0.005 0.005 0.009 0.006 0.006 0.006
(16A) 0.310 0.311 0.312 0.311 0.314 0.309 0.309
(17A) 1.383 1.383 1.380 1.385 1.385 1.367 1.367
(18A) 0.370 0.372 0.371 0.371 0.371 0.371 0.370
(19A) 0.636 0.646 0.641 0.640 0.643 0.645 0.640
(20A) 0.759 0.759 0.759 0.759 0.759 0.759 0.759
(21A) 4.800 4.800 4.800 4.799 4.800 4.801 4.800
(IB) 0.128 0.131 0.129 0.165 0.173 0.144 0.130
(2B) -0.973 -0.916 -1.030 -0.954 -0.986 -0.949 -0.931
(3B) 0.142 0.144 0.142 0.168 0.171 0.153 0.142
Embodiment 8 9 10 11 12 13 14
(1A) -0.807 -0.773 -0.787 -0.809 -0.819 -0.794 -0.836
(2A) 0.826 0.778 0.980 0.859 0.833 0.760 0.835
(3A) 0.032 0.043 -0.070 0.015 0.013 0.000 0.073
(4A) 2.10226 1.92286 2.10226 2.0017 2.0017 1.94595 2.0017
(5A) 17.1 18.9 17.1 20.6 20.6 17.98 20.64
(6A) 1.178 1.175 0.647 1.057 1.052 1.000 1.303
(7A) 1.8830 1.8061 1.8830 1.8830 1.8830 1.8061 1.8830
(8A) 40.8 40.8 40.8 40.8 40.92 40.76
(9A) 1.8830 1.8061 1.8830 1.8160 1.8160 1.8061 1.816
(10A) 40.8 40.9 40.8 46.6 46.6 40.92 46.62
(11A) -1.545 -1.491 -1.195 -1.775 -1.621 -1.193 -1.806
(12A) 2.548 2.215 2.307 1.953 1.936 2.195 2.038
(13A) 0.035 0.053 0.027 0.013 0.020 0.047 0.033
(13B) 0.001 -0.001 -0.001 -0.013 -0.020 -0.010 -0.008
(14A) -0.022 -0.028 -0.022 -0.026 -0.019 -0.021 -0.022
(15A) 0.006 0.008 0.000 0.006 0.006 0.008 0.006
(16A) 0.309 0.312 0.312 0.306 0.307 0.305 0.296
(17A) 1.371 1.386 1.501 1.393 1.396 1.394 1.376
(18A) 0.370 0.372 0.356 0.366 0.366 0.264 0.270
(19A) 0.637 0.642 0.657 0.631 0.632 — —
(20A) 0.759 0.759 0.759 0.759 0.759 0.759 0.759
(21A) 4.799 4.799 4.798 4.800 4.800 4.800 4.800
(1B) 0.118 0.162 0.013 0.094 0.111 0.172 0.108
(2B) -0.950 -0.936 -1.116 -0.977 -0.978 -1.000 -0.884
(3B) 0.134 0.166 0.100 0.117 0.134 0.174 0.130
Embodiment 15 16 17 18 19 20 21
(1A) -0.810 -0.830 -0.786 -0.824 -0.796 -0.751 -0.777
(2A) 0.740 0.980 0.835 0.870 0.898 0.748 1.017
(3A) 0.018 0.030 0.066 -0.208 -0.250 -0.164 -0.040
(4A) 1.92286 2.10226 1.94595 1.94595 1.94595 1.94595 2.10226
(5A) 18.90 17.10 17.98 17.98 17.98 17.98 17.1
(6A) 1.081 1.165 1.336 0.277 0.151 0.345 0.799
(7A) 1.83481 1.883 1.83481 1.883 1.883 1.8061 1.8830
(8A) 42.71 40.76 42.71 40.76 40.76 40.92 40.8
(9A) 1.83481 1.883 1.83481 1.8830 1.8830 1.8061 1.8830
(10A) 42.71 40.76 42.71 40.76 40.76 40.92 40.8
(11A) -1.625 -1.210 -2.009 -1.045 -0.999 -0.773 -1.172
(12A) 2.400 2.458 2.657 1.874 1.831 2.140 2.271
(13A) 0.061 0.050 0.031 0.025 0.051 0.034 0.003
(13B) -0.004 0.008 -0.008 -0.010 -0.051 -0.034 0.003
(14A) -0-022 -0.018 -0.020 -0.022 -0.017 -0.025 -0.020
(15A) 0.006 0.000 0.005 — — 0.010 0.007
(16A) 0.306 0.297 0.302 0.313 0.303 0.314 0.311
(17A) 1.376 1.467 1.370 1.476 1.414 1.382 1.484
(18A) 0.265 0.277 0.269 0.349 0.351 0.370 0.354
(19A) — — — 0.687 0.671 0.644 0.655
(20A) 0.758 0.759 0.759 0.759 0.760 0.759 0.759
(21A) 4.797 4.800 4.800 4.802 4.804 4.798 4.799
(1B) 0.185 0.012 0.115 0.084 0.067 0.192
(2B) -0.971 -0.951 -0.901 -1.413 -1.498 -1.281
(3B) 0.179 0.100 0.138 0.089 0.068 0.186
Each embodiment also can be following structure.
In order not need light, except aperture diaphragm S, also can dispose the hot spot aperture by ghost image and hot spot etc.Can be configured between object side, the 1st lens combination G1 and the 2nd lens combination G2 of the 1st lens combination G1, between the 2nd lens combination G2 and the 3rd lens combination G3, between the 3rd lens combination G3 and the 4th lens combination G4, from the 4th lens combination G4 to the image planes I, between the 4th lens combination G4 and the 5th lens combination G5, from the 5th lens combination G5 to any position the image planes I.And, can constitute by members of frame to come also miscellaneous part can be set by hot spot light.And, also can be at the directly printing of the surface of lens, application, adhering and sealing pad etc.And, any shapes such as scope that the shape of its opening can be circle, ellipse, rectangle, polygon, function curve surrounded.And, not only by harmful light beam, can also be by the light beams such as coma hot spot of image planes periphery.
And, each lens is prevented to reflect plated film, also can alleviate ghost image and hot spot.If multicoating then can effectively alleviate ghost image and hot spot, be preferred.And, also can on lens face, cloche etc., implement the IR-cut plated film.
But,, generally on the air surface of contact of lens, implement to prevent to reflect plated film (anti-reflection coating) in order to prevent the generation of ghost image and hot spot.On the other hand, on the composition surface that engages lens, the refractive index of the refractive index ratio air of adhesives is high a lot.Therefore, become identical with the individual layer plated film or to be lower than the situation of reflectivity of individual layer plated film a lot, the situation of implementing to prevent to reflect plated film by force is few.
But, if on the composition surface, initiatively implement to prevent to reflect plated film, can also alleviate ghost image and hot spot, can obtain more preferable image.Particularly the material of high index of refraction is popularized recently, because the effect of aberration correction aspect is fine, so be used for camera optical system, still high-index material is used as when engaging lens more, can not ignore the reflection on the composition surface.In this case, it is effective especially to implement to prevent to reflect plated film in advance on the composition surface.
Effective using method of composition surface plated film is disclosed in Japanese kokai publication hei 2-27301 number, TOHKEMY 2001-324676 number, TOHKEMY 2005-92115 number, USP 7116482 etc.In these documents, narrated the plated film that is provided with on the composition surface of the joint lens in the 1st lens combination of (positive-lead type) zoom lens of just going ahead of the rest especially, about the composition surface in the 1st lens combination of positive light coke of the present invention, get final product according to disclosed such enforcement of these documents.As the material of employed plated film, according to as the refractive index of the lens of substrate and the refractive index of adhesives, suitably the selective refraction rate is than higher Ta 2O 5, TiO 2, Nb 2O 5, ZrO 2, HfO 2, CeO 2, SnO 2, In 2O 3, ZnO, Y 2O 3Deng, the MgF that refractive index ratio is lower 2, SiO 2, Al 2O 3Deng, be set at the thickness that satisfies phase condition and get final product.
The plated film of the air surface of contact of lens equally also can be with the composition surface plated film as multicoating.By Coating Materials and the thickness of appropriate combination more than 2 layers or 2 layers, can carry out the control of the further reduction of reflectivity and the dichroism/angular characteristics of reflectivity etc. etc.And,, also can carry out the composition surface plated film according to same thought about the lens composition surface beyond the 1st lens combination.
And, preferably utilize the 4th lens combination G4 or the 5th lens combination G5 to focus.When utilizing the 4th lens combination G4 or the 5th lens combination G5 to focus, because lens weight saving, so few to the load of the drive system of motor etc.And then total length does not change during focusing, and can be at lens picture frame internal configurations driving motor, so help the miniaturization of picture frame.As mentioned above, though preferred the 4th lens combination G4 focuses or the 5th lens combination G5 focuses, also can utilize the 1st lens combination G1, the 2nd lens combination G2, the 3rd lens combination G3 to focus.And, also can move a plurality of lens combination and focus.And, can extract lens combination integral body out and focus, a part of lens that also can extract out or be selected in the lens combination are focused.
And, can alleviate the shade (deficiency in light quantity) of the brightness of picture periphery by the micro lens of mobile CCD.For example can change the design of the micro lens of CCD according to the incident angle of the light in each image height.And, also can proofread and correct reduction by Flame Image Process as the brightness of periphery.
And, also can have a mind to utilize optical system to produce the distortion aberration, after shooting, carry out Flame Image Process and send a telegram here correcting deformed.This Flame Image Process is called the figure adjustment of image distortion aberration, and its key concept is described.
As shown in figure 44, consider intersection point with optical axis L c and shooting face be the center, with the circle of the tangent radius R (image height R) in the long limit of effective shooting face ES.Fix the multiplying power of each point on the circumference of this circle, with each point on this circumference as correction reference.And, the each point on the circumference of any radius r (ω) (image height r (ω)) is in addition roughly moved along the radiation direction, making it with radius r ' and (ω) mode is concentric circles and moves, the distortion aberration of calibrating optical picture thus.For example, in Figure 44, make the radius r arbitrarily of the inboard of the circle that is positioned at radius R 1Some P on the circumference (ω) 1Center towards circle moves to radius r 1' some P on (ω) the circumference 2And, make the radius r arbitrarily in the outside of the circle that is positioned at radius R 2Some Q on the circumference (ω) 1Move to radius r towards direction away from round center 2' some Q on (ω) the circumference 2Here, r ' (ω) can followingly represent.
r’(ω)＝α·f·tanω (0≦α≦1)
Wherein, ω is the subject half angle of view, and f is the focal length of imaging optical system (being zoom lens among the present invention).Here, as shown in figure 45, the subject half angle of view is from the chief ray CR of the object point O angle with respect to optical axis L c, and this object point O is corresponding with the picture point M that (ω) forms on the position of height at the center r ' on the described shooting face of distance.
Here, the corresponding ideal height of point of establishing on the circumference with described radius R (image height R) is Y, then
α＝R/Y＝R/(f·tanω)
Desirable optical system is with respect to optical axis rotation symmetry.Therefore, also produce the distortion aberration symmetrically with respect to the optical axis rotation.The distortion aberration that optics is produced carries out electric timing, as mentioned above, thinks if can proofread and correct by having utilized with respect to the symmetric method of optical axis, and be favourable aspect data volume and the operand then.
, when utilizing the electro-photographic element to take, because the sampling of the pixel of imaging apparatus, optical image can not show with continuous amount.Therefore, the fenestra of the above-mentioned radius R depicted of imagination on the optical image only pixel on the shooting face of electro-photographic element, be arranged in radially, be not round accurately strictly.That is, in the shape correction of the image of giving as the aggregate of the data that obtain by discrete coordinate points (pixel of electro-photographic element), the actual circle that does not have above-mentioned this fixedly multiplying power.So, preferably use according to each pixel (coordinate (X i, Y j)) determine the coordinate (X of mobile destination i', Y j') method.In addition, a plurality of pixels are at a coordinate (X i', Y j') the position on can be mobile the time, obtain the mean value of the value that each pixel has, as being positioned at coordinate (X i', Y j') the data of locational pixel.And, for the position that does not have mobile point, use the data that have several pixels on every side of data because pixel moves to carry out interpolation, make the data of this position thus.
For in the electronic image pickup device that especially has zoom lens, because the foozle of optical system and electro-photographic element etc., it is on the circumference at center and the correction when being asymmetric of the circle that is depicted in the above-mentioned radius R on the optical image that the point that should fix the multiplying power on the above-mentioned optical image is not present in the optical axis, and this method is effective.
In the electronic image pickup device that carries out this correction, also can constitute for calculation correction amount r ' (ω)-r (ω), and will represent the data of the relation between subject half angle of view ω and the image height r, or represent the data of the relation between actual image height r and desirable image height r ' and the α, be recorded on the recording medium that is built in the electronic image pickup device.
In addition, for the light quantity that do not make the image behind the distortion correction at the two ends of its short side direction wretched insufficiency, preferred described radius R meets the following conditions.
0≦R≦0.6L s
Wherein, L sBond length for effective shooting face.
The preferred described radius R formula that meets the following conditions.
0.3L s≦R≦0.6L s
And then, make described radius R with roughly consistent with the tangent radius of a circle in the long limit of effective shooting face be best.
In addition, near radius R=0, be on the optical axis near fixedly multiplying power carry out timing, the zone of radial drawing increases.Therefore, unfavorable a bit aspect pixel count, even but can guarantee that the zoom lens wide-angleization also can realize the effect of miniaturization.
In addition, in the above description, narrated correction to a distortion in images, but the focal length variations of zoom lens, and the state of the distortion that is comprised in the image also changes with the variation of focal length.Therefore, preferably with between the maximal value (telescope end) of focal length and the minimum value (wide-angle side), proofread and correct needed focal length interval, be divided into several focal area and come correcting distorted.For example, near the telescope end in each focal area of being cut apart (state of focal length maximum in each zone), set correcting value, roughly satisfied to obtain
r’(ω)＝α·f·tanω
The correction result, can use the distortion of this correcting value correcting image in this interval.But, under this situation, the wide-angle side in each focal area of being cut apart (state of focal length minimum in each zone), the remaining barrel distortion aberration that has to a certain degree in the resulting image.When increasing the quantity of focal area for fear of this situation, the data quantitative change that should be recorded in the recording medium for correction is many.So, for each focal area of being cut apart in the telescope end one or more focal lengths different with wide-angle side, precompute one or more coefficients.Determine that according to simulation or the actual measurement result of camera head of using this coefficient gets final product.And, also can near the telescope end in described each focal area of cutting apart, calculate roughly and satisfy
r’(ω)＝α·f·tanω
Correction result's correcting value, according to each focal length this correcting value be multiply by described coefficient, determine the correcting value of the state of this focal length.
But, when not having distortion in the picture that obtains at imaging infinity object,
f＝y/tanω
Set up.Wherein, y is the height (image height) of picture point apart from optical axis, and f is the focal length of imaging system (being zoom lens among the present invention), and ω is the subject half angle of view.
When having the barrel distortion aberration in the imaging system, then
f>y/tanω
That is, when the focal distance f of imaging system and image height y were constant, the value of ω increased.
The embodiment of the electronic image pickup device of having used zoom lens of the present invention then, is described.
Figure 46～Figure 49 is the concept map of the structure of expression digital camera that zoom lens of the present invention is assembled as photographic optical system.Figure 46 is the place ahead stereographic map of the outward appearance of expression digital camera, and Figure 47 is the rear view of digital camera, and Figure 48 is the constructed profile of the inner structure of expression digital camera.State when wherein, Figure 46 and Figure 48 represent photographic optical system non-flexible.Digital camera 40 comprises: be positioned at the photographic optical system 41 of photographing with on the light path 42; Be positioned at the finder optical system 43 on the view finder usefulness light path 44; Shutter release button 45; Flashlamp 46; LCD monitor 47; Focal length change button 61 and setting alternation switch 62 etc. when photographic optical system 41 is stretched, by sliding closure 60, cover photographic optical system 41, finder optical system 43 and flashlamp 46 with cover 60.And when opening cover 60 camera settings being photography state, photographic optical system 41 becomes the non-flexible state of Figure 48, when pushing the shutter release button 45 of camera 40 tops configuration, with its interlock, photographs by photographic optical system 41.In this embodiment, use the zoom lens shown in Figure 1A, but also can use certain embodiment of zoom lens.By photographic optical system 41, go up formation object picture at the shooting face (photoelectric conversion surface) of CCD 49 via low-pass filter F that has implemented wave band restriction plated film and cloche C.The object picture of being accepted by this CCD 49 is via processing unit 51, is presented on the LCD monitor 47 that the camera back side is provided with as electronic image.And this processing unit 51 is connected with record cell 52, can write down captured electronic image.In addition, this record cell 52 and processing unit 51 can be provided with separately also and can be wholely set.As record cell, can use the storer that is built in the digital camera and HDD (Hard Disk Drive: hard disk drive), also can use the HDD that can on digital camera, plug, storage card, DVD etc.
And then, at view finder configuration view finder objective lens optical system 53 on the light path 44.View finder is the varifocal optical systems that are made of upright (image erecting) prism system 55 of picture and a plurality of lens combination (being 3 groups) with objective lens optical system 53 among the figure, this is made of prism 55a, 55b, 55c as upright prism system 55, and view finder changes linkedly with the zoom lens that objective lens optical system 53 constitutes its focal length and photographic optical system 41.The object that forms with objective lens optical system 53 by this view finder looks like to be formed on the picture field frame 57 of upright prism system 55.Dispose the eyepiece optical system 59 that upright picture is directed to observer's eyeball E in this exiting side as upright prism system 55.Exiting side at eyepiece optical system 59 disposes cap assembly 50.
Figure 49 is the structured flowchart of internal circuit of the major part of above-mentioned digital camera 40.In addition, in the following description, above-mentioned processing unit 51 for example is made of CDS/ADC portion 24, primary memory 17 and image processing part 18 etc., and storage unit 52 for example is made of storage medium portion 19 grades.
As shown in figure 49, digital camera 40 has: operating portion 12; The control part 13 that is connected with this operating portion 12; The shooting driving circuit 16, primary memory 17, image processing part 18, storage medium portion 19, display part 20 and the set information memory section 21 that connect via bus 14,15 at the control signal output ends mouth of this control part 13.
Above-mentioned primary memory 17, image processing part 18, storage medium portion 19, display part 20 and set information memory section 21 constitute, can carry out inputing or outputing of data mutually via bus 22, and, on shooting driving circuit 16, be connected with CCD49 and CDS/ADC portion 24.
Operating portion 12 is following circuit: it has various load buttons and switches such as shutter release button, camera settings alternation switch, focal length change button, will be delivered to control part from the event information of outside (camera user) input via these load buttons and switch.Control part 13 for example is central arithmetic processing apparatus (central processing unit), be following circuit: it is built-in with not shown program storage, according to institute's program stored in this program storage, receive the directive command that the camera user is imported, control figure camera 40 integral body via operating portion 12.
The object picture that ccd image sensor 49 is accepted by photographic optical system 41 formation.Ccd image sensor 49 is following imaging apparatuss: it is by shooting driving circuit 16 drive controlling, according to each pixel the light quantity of object picture is converted to electric signal, outputs to CDS/ADC portion 24.
CDS/ADC portion 24 is following circuit: amplify from the electric signal of ccd image sensor 49 outputs, and carry out analog/digital conversion, (the bare data are hereinafter referred to as the RAW data with only having carried out image raw data after this amplification and the digital conversion.) output to primary memory 17.
Primary memory 17 is the buffers that are made of for example SDRAM etc., is the above-mentioned RAW memory of data device of interim storage from 24 outputs of CDS/ADC portion.Image processing part 18 is following circuit: it is read and is stored in the RAW data in the primary memory 17 or is stored in RAW data in the storage medium portion 19, according to the specified image quality parameter of control part 13, electrically comprise the distortion aberration correction in interior various Flame Image Process.
Storage medium portion 19 for example is the control circuit of " the card type that is made of flash memory etc. or the pluggable recording medium of excellent type are installed, and record keeping the RAW data that transmit from primary memory 17 and image processing part 18 to carry out the device of the view data after the Flame Image Process in the flash memory of these card types or excellent type ".
Display part 20 has LCD monitor 47 and the circuit of display image and actions menu etc. on this LCD monitor 47.
Set information memory section 21 has: the ROM portion that stores various image quality parameters in advance; The RAM portion that be stored in from the image quality parameter that this ROM portion reads, passes through the selected image quality parameter of input operation of operating portion 12; And the circuit that the input and output of these storeies are controlled.
Like this visual angle of the wide-angle side of the photographic optical system 41 of the digital camera 40 of Gou Chenging wide, small-sized, have the hypermutation multiple proportions and whole change doubly in the zone imaging performance stablize.And, can be implemented in the wide-angle side and the quick focusing action of the side of looking in the distance.
The present invention is not only applicable to the above-mentioned this so-called small digital camera that general subject is taken, and can also be applicable to the monitor camera that needs wide viewing angle and the camera of lens-interchangeable.
The embodiment of above-mentioned zoom lens helps to realize simultaneously the miniaturization of camera and wide-angleization, hypermutation multiple proportionsization, so under the situation that does not influence the camera portability, satisfied the user and wished to photograph the zone than wider in the past expectation.More specifically, be suitable for the slimming of lens barrel when flexible, half angle of view has the wide viewing angle about 39 °, can guarantee the hypermutation multiple proportions about 5 times.And, can keep the image quality that forms by zoom lens well, and be suitable for using with electro-photographic elements combination such as CCD and CMOS.
More than describe the present invention, but can carry out various changes obviously.These change should not be considered as departing from the spirit and scope of the invention.Scope of the present invention should be limited by the equivalent on claim and the legal sense thereof.All conspicuous for those skilled in the art changes all are encompassed within the scope of claim.

Claims (36)

1. zoom lens, it has successively from object side:
The 1st lens combination of positive refractive power;
The 2nd lens combination of negative refractive power; And
The 3rd lens combination of positive refractive power,
From wide-angle side when telescope end becomes times,
Interval between interval between described the 1st lens combination and described the 2nd lens combination and described the 2nd lens combination and described the 3rd lens combination changes,
With respect to wide-angle side, the interval between described the 1st lens combination and described the 2nd lens combination broadens at telescope end,
With respect to wide-angle side, the interval between described the 2nd lens combination and described the 3rd lens combination narrows down at telescope end,
Described zoom lens has when described change times and the constant aperture diaphragm of relative position of described the 3rd lens combination,
Described the 1st lens combination has positive lens, and the total lens number in described the 1st lens combination is below 2,
Described the 2nd lens combination has successively from object side: at the object side negative lens that has concave surface as side, positive lens and picture side negative lens, the total lens number in described the 2nd lens combination is 3,
Described object side negative lens in described the 2nd lens combination and described positive lens dispose across the airspace on optical axis,
Formula meets the following conditions:
—1.70<R 2n1r/f 2<—0.70 (1A)
Wherein, R 2n1rBe the paraxial radius-of-curvature of the picture side of the object side negative lens in the 2nd lens combination, f 2It is the focal length of the 2nd lens combination.
2. zoom lens according to claim 1,
Described zoom lens is 4 groups of zoom lens that possess the 4th lens combination, and the 4th lens combination has positive refractive power.
3. zoom lens according to claim 1,
Described zoom lens is 4 groups of zoom lens with the 4th lens combination, and the 4th lens combination only is made of a slice positive lens.
4. zoom lens according to claim 1,
Described zoom lens is 5 groups of zoom lens with the 4th lens combination and the 5th lens combination, and the lens number of the 4th lens combination and the 5th lens combination is 3, and the 4th lens combination has negative refractive power, and the 5th lens combination has positive refractive power.
5. zoom lens according to claim 1, formula meets the following conditions:
0<SF 2n1<1.25 (2A)
—0.32<f 2/R 2pf<0.5 (3A)
Wherein, SF 2n1By SF 2n1=(R 2n1f+ R 2n1r)/(R 2n1f-R 2n1r) define R 2n1fBe the paraxial radius-of-curvature of the object side of the object side negative lens in the 2nd lens combination, R 2n1rBe the paraxial radius-of-curvature of the picture side of the object side negative lens in the 2nd lens combination, R 2pfIt is the paraxial radius-of-curvature of the object side of the positive lens in the 2nd lens combination.
6. zoom lens according to claim 1, formula meets the following conditions:
1.84<n d2p<2.20 (4A)
13.0<v d2p<30.0 (5A)
Wherein, n D2pBe the refractive index of the positive lens of the 2nd lens combination with respect to the d line, v D2pIt is the Abbe number of the positive lens of the 2nd lens combination.
7. zoom lens according to claim 1, formula meets the following conditions:
0.45<SF 2p<1.80 (6A)
Wherein, SF 2pBy SF 2p=(R 2pf+ R 2pr)/(R 2pf-R 2pr) define R 2pfBe the paraxial radius-of-curvature of the object side of the positive lens in the 2nd lens combination, R 2prIt is the paraxial radius-of-curvature of the picture side of the positive lens in the 2nd lens combination.
8. zoom lens according to claim 1, formula meets the following conditions:
1.78<n d2n1<2.20 (7A)
35<v d2n1<50 (8A)
Wherein, n D2n1Be the refractive index of the object side negative lens of the 2nd lens combination with respect to the d line, v D2n1It is the Abbe number of the object side negative lens of the 2nd lens combination.
9. zoom lens according to claim 1, formula meets the following conditions:
1.78<n d2n2<2.00 (9A)
35<v d2n2<50 (10A)
Wherein, n D2n2Be the refractive index of the picture side negative lens of the 2nd lens combination with respect to the d line, v D2n2It is the Abbe number of the picture side negative lens of the 2nd lens combination.
10. zoom lens according to claim 1, formula meets the following conditions:
—3.0<SF 2n2<—0.6 (11A)
Wherein, SF 2n2By SF 2n2=(R 2n2f+ R 2n2r)/(R 2n2f-R 2n2r) define R 2n2fBe the paraxial radius-of-curvature of the object side of the picture side negative lens in the 2nd lens combination, R 2n2rIt is the paraxial radius-of-curvature of the picture side of the picture side negative lens in the 2nd lens combination.
11. zoom lens according to claim 1, formula meets the following conditions:
—3.0<f 2p/f 2<—1.0 (12A)
Wherein, f 2pIt is the focal length of the positive lens of the 2nd lens combination.
12. zoom lens according to claim 1,
At least one lens face in the described object side negative lens of described the 2nd lens combination is an aspheric surface, and formula meets the following conditions:
0.002<(ASP 2n1f+|ASP 2n1r|)/f w<0.10 (13A)
—0.06<(ASP 2n1r—ASP 2n1f)/f w<0.06 (13B)
Wherein, ASP 2n1fBe the aspheric surface departure of lens face of object side of the object side negative lens of the 2nd lens combination, ASP 2n1rBe the aspheric surface departure of lens face of picture side of the object side negative lens of the 2nd lens combination, f wFocal length for the zoom lens of wide-angle side.
13. zoom lens according to claim 12,
The object side of the described object side negative lens in described the 2nd lens combination is the aspheric surface that refractive power increases along with the increase with optical axis distance.
14. zoom lens according to claim 13,
Described object side negative lens in described the 2nd lens combination is a double-concave negative lens,
The object side of described double-concave negative lens is the aspheric surface that negative refractive power reduces along with the increase with optical axis distance,
Described double-concave negative lens be the aspheric surface that negative refractive power increases along with the increase with optical axis distance as the side.
15. zoom lens according to claim 1,
The described lens face as side as the side negative lens in described the 2nd lens combination is an aspheric surface, satisfies following conditional:
—0.09<(ASP 2n2r—ASP 2n2f)/f w<—0.003 (14A)
Wherein, ASP 2n2fBe the aspheric surface departure of lens face of object side of the picture side negative lens of the 2nd lens combination, ASP 2n2rBe the aspheric surface departure of lens face of picture side of the picture side negative lens of the 2nd lens combination, f wFocal length for the zoom lens total system of wide-angle side.
16. zoom lens according to claim 15,
The described picture side negative lens of described the 2nd lens combination is the negative meniscus lens of convex surface towards the picture side,
The face as side of described negative meniscus lens is the aspheric surface that positive refractive power strengthens along with the increase with optical axis distance.
17. zoom lens according to claim 1,
The described positive lens of described the 2nd lens combination and describedly be respectively simple lens as the side negative lens.
18. zoom lens according to claim 1,
The described positive lens of described the 2nd lens combination and describedly be engaged as the side negative lens.
19. zoom lens according to claim 1,
Described the 1st lens combination has described positive lens and negative lens.
20. zoom lens according to claim 19,
Described the 1st lens combination constitutes by be followed successively by these 2 lens of described negative lens and described positive lens from object side, and the total lens number in described the 1st lens combination is 2.
21. zoom lens according to claim 20,
The described negative lens and the described positive lens of described the 1st lens combination are respectively simple lens.
22. zoom lens according to claim 21,
The described negative lens of described the 1st lens combination and the interval between the described positive lens formula that meets the following conditions:
0.0≤L 1np/L 1<0.2 (15A)
Wherein, L 1npBe the negative lens and the interval of positive lens on optical axis of the 1st lens combination, L 1It is the gross thickness on the optical axis of the 1st lens combination.
23. zoom lens according to claim 22,
The described negative lens and the described positive lens of described the 1st lens combination are engaged.
24. zoom lens according to claim 1,
The lens that comprise in described the 1st lens combination only are described positive lens.
25. zoom lens according to claim 1,
Total lens number in described the 3rd lens combination is below 3.
26. zoom lens according to claim 25,
Described the 3rd lens combination constitutes by be followed successively by these 3 lens of positive lens, positive lens and negative lens from object side.
27. zoom lens according to claim 1, formula meets the following conditions:
0.20<|f 2/f t|<0.325 (16A)
Wherein, f tFocal length for the zoom lens of telescope end.
28. zoom lens according to claim 1, formula meets the following conditions:
0.7<f 1/f t<1.8 (17A)
Wherein, f 1Be the focal length of the 1st lens combination, f tFocal length for the zoom lens of telescope end.
29. zoom lens according to claim 1, formula meets the following conditions:
0.25<f 3/f t<0.50 (18A)
Wherein, f 3Be the focal length of the 3rd lens combination, f tFocal length for the zoom lens of telescope end.
30. zoom lens according to claim 2, formula meets the following conditions:
0.40<f 4/f t<1.0 (19A)
Wherein, f 4Be the focal length of the 4th lens combination, f tFocal length for the zoom lens of telescope end.
31. zoom lens according to claim 2,
From wide-angle side when telescope end becomes times, described the 1st lens combination, described the 2nd lens combination, described the 3rd lens combination and described the 4th lens combination move, so that the interval between described the 1st lens combination and described the 2nd lens combination broadens, interval between described the 2nd lens combination and described the 3rd lens combination narrows down, and the interval between described the 3rd lens combination and described the 4th lens combination broadens.
32. zoom lens according to claim 31,
From wide-angle side when telescope end becomes times, described the 1st lens combination moves, and makes it compare wide-angle side and is positioned at object side at telescope end, described the 2nd lens combination moves, described the 3rd lens combination only moves to object side, described the 4th lens combination moves.
33. zoom lens according to claim 1, formula meets the following conditions:
3.8<f t/f w<15.0 (21A)
Wherein, f wBe the focal length of the zoom lens of wide-angle side, f tFocal length for the zoom lens of telescope end.
34. an electronic image pickup device, it has:
The zoom lens of claim 1; And
The electro-photographic element, it is configured in the picture side of described zoom lens, will be converted to electric signal by the optical image that described zoom lens forms.
35. electronic image pickup device according to claim 34, formula meets the following conditions:
0.70<I m/f w<1.00 (20A)
Wherein, I mBe maximum image height, f wFocal length for the zoom lens of wide-angle side.
CNB2007101534383A 2006-09-19 2007-09-19 Zoom lens and electronic image pickup apparatus using the same Expired - Fee Related CN100504493C (en)

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CN101556369A (en) 2009-10-14
JP2008076493A (en) 2008-04-03

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