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Ординатура / Офтальмология / Английские материалы / Lens Design Fundamentals 2nd edition_Kingslake, Johnson_2009.pdf
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11.2 The Petzval Theorem

297

Slope of entering principal ray

Figure 11.6

–30°

–20°

–10°

0

–0.2

0

0.2

–0.2

0

0.2

 

(a)

 

 

(b)

 

10°

20°

30°

Fields of a Protar lens, (a) centered and (b) rear surface tilted clockwise by 6 arcmin.

before and after the last surface was tilted, the effect of the tilt can be readily seen. Briefly, it causes the field to tilt in a counterclockwise direction, the tangential field being tilted and distorted much more than the sagittal field. Limiting ourselves to one field angle, say 17.2 , we find that the tangential field has been tilted by 35.2 arcmin while the sagittal field has been tilted through 13.3 arcmin, both considerably more than the surface tilt that caused the problem. Actually, the effects of a tilt as small as 5 arcmin can generally be detected, and it is customary to try to limit accidental surface tilts in any good lens to about one arcmin.

Surface tilt does more damage to an image than any other manufacturing error, and in assembling a lens it is essential to avoid tilted surfaces at any cost.

11.2 THE PETZVAL THEOREM

From very simple considerations, it is clear that a positive lens ought to have an inward-curving field. The extraaxial or off-axis points on a flat object are further from the lens than the axial point, and consequently their images should be closer to the lens than the axial image, leading at once to an inward-curving field.

298

The Oblique Aberrations

r

Surface

r

r

C l

l

Auxiliary

axis

Lens axis

(

(n′)

n)

Object

Image

Figure 11.7 The Petzval theorem.

The exact amount of this natural field curvature can be calculated by the following argument. Suppose we place a small stop at the center of curvature C of a single spherical refracting surface (Figure 11.7). This will automatically eliminate coma and astigmatism by forcing the oblique light to be refracted along an auxiliary axis as if it were an axial beam. If the stop is small enough to eliminate spherical aberration also, we shall be left with nothing but the basic field curvature that we are trying to evaluate.

It is, of course, obvious that under these conditions an object having the form of a sphere centered about C must be imaged as a sphere also centered about C. If the radii of curvature of object and image are represented by r and r0, then5

r ¼ l r; r0 ¼ l0 r

and since for a single surface n0/l0 n/l ¼ (n0 n)/r, we can readily show that, for one surface,

1

1

 

n0 n

n0r0

 

nr

¼

nn0r

We can now write this expression for every surface in the lens and add them up, but this procedure will be valid only if we can assume that all traces of astigmatism have somehow been eliminated. Nevertheless, for such a lens having k surfaces, we find that

1

1

¼ X

n0 n

nk0 rk0

 

n1r1

nn0r

This expression relates the radius of curvature of the image with the radius of curvature of the object, provided there is no astigmatism present. It is clear,

11.2 The Petzval Theorem

299

then, that the radius of curvature of the image of a plane object with r1 ¼ 1, is given by

1

 

n0

n0 n

(11-5)

rk0

¼

X nn0r

k

 

It should be noted that a positive value of r corresponds to a negative sag, or an inward-curving image. Hence the sag of the curved image of a plane object, in the absence of astigmatism, will be given by

Z0

 

1

h0

2n0

n0 n

(11-6)

¼

 

X nn0r

ptz

2 k

k

 

This is the famous Petzval theorem, and we shall have many occasions to refer to it since it is only possible to design a flat-field lens free from astigmatism by reducing the Petzval sum; thus the Petzval theorem dominates the entire design processes for flat-field photographic lenses.

The quantity under the summation in these different expressions is called the Petzval sum, and the radius of curvature of the image is evidently the reciprocal of the Petzval sum. Another useful term is the Petzval ratio, which is the ratio of the Petzval radius to the focal length of the lens. It is given by

r0=f 0 ¼ 1=f 0 S

where S is the Petzval sum. Note the reciprocal relationship here. A long focal length lens tends to have a small Petzval sum, while the sum is large in a strong lens of short focal length.

11.2.1Relation Between the Petzval Sum and Astigmatism

It can be shown6 that at very small obliquity angles the tangential astigmatism— that is, the longitudinal distance from the Petzval surface to the tangential focal line—is three times as great as the corresponding sagittal astigmatism. Thus, if the astigmatism in any lens can be made zero, the two focal lines will coalesce on the Petzval surface. In all other cases the locus of the tangential foci at various obliquities is called the tangential field of a lens, and similarly for the sagittal field. As the Petzval surface in most simple lenses is inward-curving, it is often possible to flatten the tangential field by the deliberate introduction of overcorrected astigmatism, leaving the sagittal image to fall between the Petzval surface and the tangential image. However, when designing an “anastigmat” having a flat field free from astigmatism, it is necessary to reduce the Petzval sum drastically.

If it is necessary to design a lens having an inward-curving field to meet some customer requirement, the astigmatism can easily be removed and the Petzval

300 The Oblique Aberrations

sum adjusted to give the desired field curvature. On the other hand, if the field must be backward-curving, it is difficult to avoid an excessive amount of overcorrected astigmatism. It is worth noting that in some types of lens, if the Petzval sum is made too small the separation between the astigmatic fields becomes excessively large at intermediate field angles.

Many decades ago, lens designers taught that the tangential astigmatic field should be flattened to obtain the smallest spot size.7,8,9 This can be easily under-

stood by considering Eqs. (4-6) and (4-7) and assuming that all aberration coefficients are zero other than primary astigmatism ðs3Þ and Petzval ðs4Þ. The sagittal and tangential astigmatic ray errors in the paraxial image plane are

2

sin y

 

2

cos y, respectively. Three basic cases to

ðs3 þ s4ÞrH

and ð3s3 þ s4ÞrH

 

contemplate are a flat sagittal field, a flat tangential field, and equally balanced fields about the paraxial image plane. For a flat sagittal field, s3 þ s4 ¼ 0 or s3 ¼ s4, which means that the residual tangential astigmatism in the paraxial image plane is 3s3 þ s4 ¼ 2s4. When the tangential field is flat, 3s3 þ s4 ¼ 0, which implies that s3 ¼ s4=3 and the residual sagittal astigmatism is 2s4=3. When the errors are balanced, the tangential astigmatism is equal to the negative of the sagittal astigmatism, or s3 ¼ s4=2.

In the balance-fields case, the values of the residual sagittal and tangential astigmatism are observed each to be smaller than the residual values of the prior two cases. This might lead one to select this condition as the optimal minimum spot size10; however, such a conclusion is erroneous.11 It is a general practice by lens designers to adjust the astigmatic surfaces such that the tangential field is flat and then adjust the position of the image plane to the location of the smallest blur at the edge of the field. The definition of the imagery is relatively uniform over the whole image area. In a balanced-field case, the image definition is quite superior in the central region of the image to that of the flat tangential field case, and inferior in the outer portions of the imagery.12 As B. K. Johnson stated, “It therefore depends much on the requirements for which the lens is to be used, as to which criterion is to be adopted.”

11.2.2 Methods for Reducing the Petzval Sum

There are several methods by which the Petzval sum can be reduced, and one or more of these appear in every type of photographic objective. These methods can also be applied to a wide variety of optical systems.

A Thick Meniscus

If we have a single lens in which both radii of curvature are equal and of the same sign, the Petzval sum will be zero, while the lens power is proportional to the thickness. Cemented interfaces in such a lens have very little effect on the

11.2 The Petzval Theorem

301

Petzval sum. This property has been used in many symmetrical lenses such as the Dagor and Orthostigmat.

Separated Thin Elements

In a system containing several widely separated thin elements, the Petzval sum is given by

X

Ptz ¼ f=n (11-7)

where f is the power of an element. If there is about as much negative as positive power in such a system, the Petzval sum can be made as small as desired. This property has been used in many lenses of the dialyte type (see Section 13.2).

Negative Lens Field Flattener

An interesting special case is that in which a negative lens element is placed at or near an image plane, as illustrated in Figure 11.8. This element has little or no effect on the focal length or the aberrations, but it contributes its full power to the Petzval sum. (See Section 11.7.4.)

Conversely, if it is necessary to insert a positive lens in an image plane to act as a field lens, then this lens has a large adverse effect on the Petzval sum. For this reason it is almost impossible to reduce the Petzval sum in a long periscope having several internal images and field lenses. However, by using photographic-type lenses as field lenses it is sometimes possible to reduce the sum appreciably.

It should be noted that in a lens having a long central air space, the Petzval sum is increased if both components are positive (as in the Petzval portrait lens) because the rear component acts partly as a positive field lens. On the other hand, if the rear component is negative (as in a telephoto), then the Petzval

Figure 11.8 Negative lens element is placed at or near an image plane.

302

The Oblique Aberrations

sum is reduced, and in an extreme telephoto it may actually become negative, requiring some degree of undercorrected astigmatism to offset it.

A Concentric Lens Field Flattener

The preceding field flattener has several inherent problems that may make it difficult or impossible to use. There are situations where a field flattener needs to be remote from the image plane—for example, an infrared detector array located inside a vacuum dewar. Rosin13 described the use of a concentric lens centered about the focus of diverging or converging axial rays as illustrated in Figure 11.9. Since any of these axial rays are incident normal to the lens surfaces, the position of the image does not change with the introduction of this lens nor does it change the image size.

It can be shown that aberration contributions of this lens have the following characteristics.

. Zero spherical aberration

. Zero tangential and sagittal coma

. Zero axial color

. Zero lateral color

. Distortion is unchanged

. Sagittal field curvature is unaffected

. Tangential field curvature can be independently controlled

The tangential field contribution is proportional to ðR2 R1Þ NN 1 , which means that the effect cause is based on the thickness of the lens and the distance to its center of curvature. Higher-order aberrations will generally remain corrected for spherical aberration, axial color, distortion, sagittal coma, sagittal field curvature, spherochromatism, zonal spherical aberration, and sagittal

r2

r1

Air

Glass

Air

 

Figure 11.9 Concentric lens used to flatten tangential field.

11.2 The Petzval Theorem

303

oblique spherical aberration. In cases where the stop is significantly distant from the lens, certain higher-order aberrations can become bothersome, namely, tangential coma, lateral color, tangential field curvature, and tangential oblique spherical aberration. In addition to these possible limitations, the lens curvatures toward the image plane may restrict the size of the field due to the geometric size of the field flattener lens. It should be noted that since these lens aberrations are all about zero, spatial positioning of this lens does not need to be nearly as precise as a lens contributing large amounts of aberrations.

The concentric field flattener lens was independently discovered14 and successfully employed, beginning in 1968, to enhance the performance of a variety of thermal infrared optical systems having low f-numbers and moderate fields- of-view. However, the exact concentricity and positioning of the lenses were deviated from the above lens specifications to mitigate potential ghost images that could be formed at the image plane due to reflections from surfaces R1 and R2 when centered on the axial image point. In some cases, this nearly concentric field flattener was used as the dewar window. The amount of aberrations induced by breaking exact concentricity and positioning can be reasonably small while still providing predominate control of the tangential field curvature.

Mann used a concentric field flattener in a 3:1 infrared zoom lens and significantly reduced the field curvature over the zoom range, and generally achieved balanced astigmatic fields (see Section 11.2.1).15 His design technique for the field flattener was to first design the zoom lens and then to place a flat plate where the dewar window was to be located. He then allowed the computer program to vary the curvatures, and somewhat the flattener’s thickness, which naturally became near concentric about the axial image. The final system was near diffraction-limited.

Figure 11.10 illustrates a typical configuration shown by Rosin where the concentric field flattener is located in the image space of a Petzval-type lens. In this case, he followed a design procedure of reducing the Petzval and sagittal field curvatures while rather ignoring the tangential field curvature as shown in

r1

r2

Figure 11.10 Concentric lens behind Petzval lens.

304

 

 

 

 

 

 

The Oblique Aberrations

 

 

 

Focal plane

 

P S

 

T

 

 

 

 

 

 

 

 

P,S,T

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(a)

(b)

Figure 11.11 Flattening of tangential field using concentric lens where lens was designed to have flat sagittal field. (a) Initial design with flat sagittal field; (b) Tangential field bought into coincidence with the sagittal and Petzval curvatures using the concentric field flattener.

Figure 11.11a. With the introduction of the concentric field flattener lens, the tangential (T) field curvature was brought into coincidence with the Petzval (P) and sagittal (S) field curvatures as depicted in Figure 11.11b. A substantial improvement in resolution uniformity and contrast over the field of view was obtained. An alternative location for the concentric lens is to place it between the front and rear elements. In this case, the radii of the concentric lens are centered at the focus location of the front element.

A concentric field flattener lens may be introduced in other than the image space of a lens; however, this can shift the spatial location of the image plane. Another form of the concentric field flattener can be realized by considering a solid glass plate placed in image space, as illustrated in Figure 11.12a, which has been shown in Sections 3.4.4 and 6.4 to shift the image location and introduce aberrations.16 A concentric air lens17 is now formed by removal of the middle section of the glass plate—that is, a plano-concave lens followed by a convex-plano lens as illustrated in Figure 11.12b. The internal surface curvatures are centered on the image location that would occur should the glass plate have contained the image. The design of a lens being combined with this concentric field flattener element should include the aberrations resulting from a glass plate having a thickness equal to the distance between the plano surfaces of the concentric field flattener lens. The air concentric field flattener lens has a manufacturing advantage over the form shown in Figure 11.9 since it is more difficult to colocate the centers of the surfaces of a concentric lens element.

Another field flattener approach18 uses a concentric shell centered about the stop (convex toward the image). The beam passing through this lens has the chief ray always perpendicular to the surfaces of the shell so its induced

11.2 The Petzval Theorem

305

(a)

Glass plate

 

r1

(b)

 

Air lens

r2

Figure 11.12 (a) Image shift caused by glass plate. (b) Creation of concentric air lens from the glass plate.

aberrations are constant as a function of field angle. As it does have some negative power, the shell affects the Petzval sum. It also shifts the image somewhat.

PROBLEM: For a concentric field flattener lens, show that spherical aberration, tangential and sagittal coma, axial color, and lateral color are zero, and that distortion and sagittal field curvature are unaffected.

PROBLEM: Consider the field diagrams shown in Figure 11.11 and explain the astigmatic aberrations depicted in both using Seidel aberration coefficients (s3 and s4).

A New-Achromat Combination

By 1886, Abbe and Schott in Jena, Germany, had developed barium crown glasses having just the required property to reduce the Petzval sum, and these glasses were immediately adopted by Schroder in 1888 in his Ross Concentric lens.19 These glasses provided the sought after method for controlling the Petzval sum by using a crown glass of low dispersion and high refractive index in combination with a flint glass of higher dispersion and a low refractive index. This is precisely opposite to the choice of glasses used in telescope doublets and other ordinary achromats. Lenses of this type are therefore known as “new achromats.” They have been used in the Protar (Section 14.4) and many other types of photographic objectives.