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5.2 Spherochromatism of a Cemented Doublet

139

inside the paraxial focus for d light while the C light focus lies to the outside. This should be evident since the refractive index is progressively greater for C, d, and F light thereby increasing the optical power of the lens ðfl ¼ ðnl 1Þðc1 c2ÞÞ. The longitudinal axial chromatic aberration is given by L0ch ¼ LF0 LC0 (see 5.2.3) and transverse axial chromatic aberration6 is given by L0ch tan u0. A simple converging lens that is uncorrected for aberrations, as shown in Figure 5.1, is said to have undercorrected aberrations. If the sign of an aberration of the optical system is opposite to that of a simple converging lens, the lens system is said to be overcorrected. When a specific aberration is made zero or less than some desired tolerance, the lens system is said to be corrected.

5.2SPHEROCHROMATISM OF A CEMENTED DOUBLET

Consider a cemented doublet objective lens, as illustrated in Figure 5.2. The prescription of this lens, repeated from Section 2.5, is as follows:

r1

¼ 7:3895

c1 ¼ 0:135327

 

 

 

 

 

d1 ¼ 1:05

n1

¼ 1:517

r2

¼ 5:1784

c2

¼ 0:19311

 

 

 

 

 

d2 ¼ 0:40

n2

¼ 1:649

r3

¼ 16:2225

c3

¼ 0:06164

 

 

If we now trace through it a marginal, zonal, and paraxial ray in each of five wavelengths, we obtain Table 5.1, which shows image distances expressed relative to the paraxial focus in D light.

Figure 5.2 A cemented doublet objective.

140

 

 

 

Chromatic Aberration

 

 

Table 5.1

 

 

 

Image Distance versus Wavelength Relative to the Paraxial Focus

 

 

 

 

 

 

 

Wavelength

A0 (0.7665)

C (0.6563)

D (0.5893)

F (0.4861)

g (0.4358)

Crown index

1.51179

1.51461

1.517

1.52262

1.52690

Flint index

1.63754

1.64355

1.649

1.66275

1.67408

Marginal Y ¼ 2

0.0203

0.0100

0.0081

0.0265

0.0588

Zonal Y ¼ 1.4

0.0059

–0.0101

–0.0176

–0.0153

0.0025

Paraxial

0.0327

0.0121

0

–0.0101

–0.0033

 

 

 

 

 

 

These data may be plotted in two ways. First we can plot the longitudinal spherical aberration against aperture, separately in each wavelength (Figure 5.3a); and second, we can plot aberration against wavelength for each zone (Figure 5.3b). The first set of curves represents the chromatic variation of spherical aberration, or “spherochromatism,” and the second set represents the chromatic aberration curves for the three zones. On these curves we notice several specific aberrations.

5.2.1 Spherical Aberration (LA0)

This is given by L0marginal l0paraxial in brightest (D) light. It has the value 0.0081 in this example, and is slightly overcorrected.

5.2.2 Zonal Aberration (LZA0)

This is given by L0zonal l0paraxial in D light. It has the value –0.0175, and is undercorrected. The best compromise between marginal and zonal aberration

for photographic objectives is generally to secure that LA0 þ LZA0 ¼ 0, but for visual systems it is better to have LA0 ¼ 0.

5.2.3 Chromatic Aberration (L0ch)

This

is given by LF0 LC0 , and its magnitude varies from zone to zone

(Figure

5.4) as shown in Table 5.2.

5.2 Spherochromatism of a Cemented Doublet

141

Chromatic focus error

M

g

D

Z

 

F

 

C

 

A

 

 

 

 

 

P

 

 

 

 

–0.024

–0.012

0

0.012

0.024

0.036

0.048

0.06

 

 

 

(a)

 

 

 

 

0.06

 

 

 

 

 

 

 

0.04

 

 

 

 

 

 

 

0.02

 

 

 

 

 

Paraxial

 

 

 

 

 

 

 

 

 

 

Marginal

 

 

 

0.00

 

 

 

 

 

 

Zonal

 

 

 

 

 

 

 

–0.02

 

 

g

F

 

 

D

 

C

 

 

 

A

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

0.40

0.45

0.50

0.55

0.60

0.65

0.70

0.75

0.80

 

 

 

 

 

 

 

 

 

Wavelength

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(b)

 

 

 

 

 

 

 

Figure 5.3 Spherochromatism ( f ¼ 12). (a) Chromatic variation of spherical aberration;

(b) chromatic aberration for three zones.

If no zone is specified, we generally refer to the 0.7 zonal chromatic aberration because zero zonal chromatic aberration is the best compromise for a visual system. Photographic lenses, on the other hand, are generally stopped down somewhat in use, and it is often better to unite the extreme colored foci for about the 0.4 zone instead of the 0.7 zone suggested here.

142

Chromatic Aberration

Y

M

Z

P

 

 

 

 

 

 

 

L

 

 

 

 

 

 

 

 

–0.02

0

0.02

 

ch

 

 

 

Figure 5.4 Variation of chromatic aberration with aperture.

Table 5.2

Chromatic Aberration for Three Zones in the Aperture

Zone

Lch0 ¼ LF0 LC0

Marginal

þ0.0165

0.7 Zonal

–0.0052

Paraxial

–0.0222

 

 

Chromatic aberration can be represented as a power series of the ray height Y:

chromatic aberration ¼ L0ch ¼ a þ bY2 þ cY4 þ . . .

The constant term a is the paraxial or “primary” chromatic aberration. The secondary term bY2 and the tertiary term cY4 represent the variation of chromatic aberration with aperture as shown in Figure 5.4.

5.2.4 Secondary Spectrum

Secondary spectrum is generally expressed as the distance of D focus from the combined C – F focus, taken at the height Y at which the C and F curves intersect. In the example shown later in this section, the C and F curves intersect at about Y ¼ 1.6, and at that height the other wavelengths depart from the combined C and F focus by

Spectrum line

A0

C

D

F

g

Departure of focus

0.005

0

–0.016

0

0.012