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Optics Express

Optics Express

  • Editor: Michael Duncan
  • Vol. 14, Iss. 11 — May. 29, 2006
  • pp: 4687–4694
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On the chromatic aberration of microlenses

Patrick Ruffieux, Toralf Scharf, Hans Peter Herzig, Reinhard Völkel, and Kenneth J. Weible  »View Author Affiliations


Optics Express, Vol. 14, Issue 11, pp. 4687-4694 (2006)
http://dx.doi.org/10.1364/OE.14.004687


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Abstract

The optical properties of plano-convex refractive microlenses with low Fresnel Number (typically FN <10) are investigated. It turns out that diffraction effects at the lens aperture limit the range of the effective focal length. The upper limit of the focal length is determined by the diffraction pattern of a pinhole with equal diameter. In addition achromatic microlenses can be realized because refraction and diffraction have opposing effects on the focal length. Gaussian beam propagation method has been used for simulation. The presented results are of relevance for applications, where microlenses with small apertures and long focal lengths are used, for example, Shack Hartmann wavefront sensors or confocal microscopes.

© 2006 Optical Society of America

1. Introduction

The refractive index of any transparent material is function of the wavelength. Therefore, a lens made in one single material shows different positions of focus at each wavelength. The difference in position of these focal points is known as the longitudinal primary chromatic aberration [1

1. D. Malacara and Z. Malacara, Handbook of lens design, (Dekker, New York, 1994).

]. To correct this aberration, achromatic lenses are usually manufactured using two lenses of different material having different Abbe numbers combined to form a doublet or even triplet [1

1. D. Malacara and Z. Malacara, Handbook of lens design, (Dekker, New York, 1994).

]. This method uses the different dispersion curves of the materials to obtain, at two well separated wavelengths, the same focal length with small variations for the other wavelengths in between. By their small dimensions microlenses can have low Fresnel number and then exhibit strong diffractive effects on the position and the shape of their focal point as it has been extensively studied in literature (focal shift [2

2. Y. Li and E. Wolf, “Focal shifts in diffracted converging spherical waves,” Opt. Commun. 39, 211 (1981). [CrossRef]

] [3

3. Y. Li and H. Platzer, “An experimental investigation of diffraction patterns in low Fresnel-number focusing systems,” Optica Acta 30, 1621 (1983). [CrossRef]

] [4

4. W. Wang, A. T. Friberg, and E. Wolf, “Structure of focused fields in systems with large Fresnel numbers,” J. Opt. Soc. Am. A. 12, 1947 (1995). [CrossRef]

]). We show here that for such lenses a range for the radius of curvature (ROC) can be found where microlenses show an achromatic behavior. Firstly we focus our study on the position of the peak irradiance (Zp) for different microlenses diameters as function of ROC. The focal length is increased by increasing the ROC. However at a certain value for ROC, the focal length cannot be further increased. The limit is fixed by the position of the peak irradiance of the light diffracted by an aperture equal to the lens diameter. Secondly we study the position of the peak irradiance at different wavelengths. We observe two phenomena influencing Zp. One is the focal shift due to diffraction and the second is the chromatic aberration due to the material dispersion. Because these two phenomena have opposing influence on Zp, a choice for the ROC can be found where Zp is the same at two wavelengths. This property could be used to design achromatic lenses in one single material.

2. Basic considerations

The focal length f E of a plano-convex refractive lens is derived from the radius of curvature ROC and the refractive index n of the lens material

fE=ROC(n1).
(1)

The refractive index is a function of the wavelength λ, whereas n(λ2)<n(λ1) for λ21. The longitudinal primary chromatic aberration, corresponds to a chromatic shift of the focal length, f E2)>f E1) for λ21, [1

1. D. Malacara and Z. Malacara, Handbook of lens design, (Dekker, New York, 1994).

]. The Fresnel number FN of a lens with a lens diameter Ø=2ρ is defined by

FN=ρ2λfE.
(2)

For large Fresnel numbers FN≫1, geometric optics is well suitable to derive the focal length of a microlens. For low Fresnel numbers, the focal length is shifted towards the lens due to the influence of the diffraction at the lens stop. A Gaussian beam decomposition algorithm [5

5. J. Arnaud, “Representation of Gaussian beams by complex rays,” Appl. Opt. 24, (1985). [CrossRef] [PubMed]

] is used for the comprehensive analysis of the refractive and diffractive properties of the microlenses.

3. Plano-convex refractive microlens

A plane wave with constant intensity profile illuminates a plano-convex refractive microlens as shown in Fig. 1. An aperture blocks the light outside the microlens.

Fig. 1. Model of a plano-convex microlens illuminated by a plane wave.

As an example, a microlens with diameter Ø=635 µm, ROC=2.03 mm, made of fused silica with n (633 nm)=1.456 has been chosen. From paraxial geometric optics, the focal length is f E=4.45 mm. The Fresnel number of the lens is FN=35.7. As shown in Fig. 2, diffraction analysis [5

5. J. Arnaud, “Representation of Gaussian beams by complex rays,” Appl. Opt. 24, (1985). [CrossRef] [PubMed]

] predicts a position of the peak irradiance Zp at 4.36 mm. The difference between the position of the peak irradiance Zp derived from diffraction theory and the focal length f E obtained from geometrical optics is defined as focal shift δ [6

6. U. Vokinger, R. Dändliker, P. Blattner, and H. P. Herzig, “Unconventional treatment of focal shift,” Opt. Commun. 157, 218–224 (1998). [CrossRef]

]:

δ=ZpfE.
(3)

In the example of a microlens with a Fresnel number FN=35.7. A focal shift of δ=-0.09 mm, corresponding to 2% mismatch is observed. This shows a good agreement between geometrical optics and diffraction theory for microlenses with large Fresnel numbers.

Fig. 2. Intensity (a.u.) distribution behind a microlens of Ø=635 µm, ROC=2.03 mm, illuminated by a plane wave at 633 nm. The lens stands in the x,y plan while z corresponds to the propagating axis.

Figure 3 shows the intensity distribution of a microlens with a Fresnel number FN=6.29. A focal shift of δ=-6.23 mm, corresponding to 11% mismatch is observed.

Fig. 3. Intensity (a.u.) distribution behind a microlens of Ø=635 µm and ROC=25.2 mm illuminated by a plane wave at 633 nm. The lens stands in the x,y plan while z corresponds to the propagating axis.

Figure 4 shows the intensity distribution of a microlens with a Fresnel number FN=0.3. A focal shift of δ=-416.86 mm, corresponding to 75% mismatch is observed.

Fig. 4. Intensity (a.u.) distribution behind a microlens of Ø=635 µm, ROC=252 mm, illuminated by a plane wave at 633 nm. The lens stands in the x,y plan while z corresponds to the propagating axis.

Figure 5 shows the intensity distribution behind a pinhole with same diameter. A pinhole with no refractive power corresponds to a microlens with ROC=∞.

Fig. 5. Intensity (a.u.) distribution behind an aperture of Ø=635 µm illuminated by a plane wave at 633 nm. The lens stands in the x,y plan while z corresponds to the propagating axis.

The observed peak irradiance position Zp=162.93 mm is the maximum obtainable focus spot position for a microlens of Ø=635 µm diameter.

4. Refractive and diffractive regime

These phenomena are now analyzed for different microlens diameters illuminated by a plane wave at 633 nm.

Fig. 6. ROC [mm] versus position of peak irradiance for six diameters of microlenses illuminated by a plane wave at 633nm.

Figure 6 shows Zp function of ROC for different microlens diameters. For low ROC (typically ROC <1 mm for Ø=635 µm microlens) the peak irradiance corresponds to the focal length obtained by Eq. (1). For increasing values of ROC, the peak irradiance converges to a maximum value Zp max illustrated by vertical dash lines in Fig. 6. This value corresponds to the peak irradiance position obtained for a pinhole with no optical power, i.e. ROC=∞. To check the validity of the present approach, the values of Zp max obtained by the Gaussian beam decomposition algorithm are now compared to the values derived from the Rayleigh-Sommerfeld integral.

The scalar field U(r,z) at the point P is given by [7

7. J. W. Goodman, Introduction to Fourier Optics, 2nd ed., (MacGraw-Hill, New York, 1968), Chap. 4, pp. 63–69.

],

U(r,z)=1iλΣA0(r0)exp(ikR)Rcos(θ)dS,
(4)

where Σ is the surface limited by the aperture in z0=0. For a plane wave diffracted at the circular aperture and propagating along the optical axis we have A 0(r0)=A 0 and R=z2+r02 with r 0=|r 0|. Furthermore, for paraxial approximation we assume that cos(θ)≈1. Substituting these relations into Eq. (4) and introducing polar co-ordinates yields to

U(r=0,z)=A0iλφ=02πr0=0ρ0exp(ikz2+r20)z2+r20r0dr0dϕ,
(5)

where ρ 0 is the radius of the limiting aperture at z0=0. Integrating Eq. (5) and approximating the square root in the phase by the first two terms of the Taylor series yields to

I(r=0,z)=(2A0sin(kρ204z))2,
(6)

describing the intensity distribution along the optical axis. The maximum intensity is found by setting the derivative of Eq. (6) equal to zero,

dI(r=0,z)dz=A0kρ02sin(kρ202z)1z2=0,
(7)

which implies that kρ022z=π. The position of peak irradiance of an aperture obtained by the Rayleigh-Sommerfeld integral is

Zp=ρ02λ.
(8)

The peak irradiance positions Zp of pinholes with Ø=2ρ0 diameters obtained from Rayleigh-Sommerfeld, are shown as dashed lines in Fig. 6. The Gaussian beam decomposition algorithm corresponds well to the Rayleigh-Sommerfeld approach.

5. Achromaticity

Fig. 7. ROC versus position of peak irradiance Zp for microlenses of Ø=635 µm illuminated by a plane wave at two different wavelengths.

In the refractive domain, the peak irradiance Zp respectively the focal length f E is inversely proportional to the refractive index n(λ). The dispersion curve of a material approximated by the Cauchy Formula [1

1. D. Malacara and Z. Malacara, Handbook of lens design, (Dekker, New York, 1994).

] Eq. (9),

n=C0+C1λ2+C2λ4,
(9)

leads to a decreasing refractive index for increasing wavelengths. In the refractive regime, the position of the peak irradiance (Zp) is equal to the focal length given by Eq. (1).

Figure 8 shows the peak irradiance position function of ROC at different wavelengths λ. The longitudinal primary chromatic aberration δλ is the difference of the peak irradiance positions for different wavelengths δλ=Zp1) - Zp2), expressed along the optical axis [1

1. D. Malacara and Z. Malacara, Handbook of lens design, (Dekker, New York, 1994).

]. In classical optics, an achromatic lens is designed to have the same focal length for two well separated wavelengths, i.e. δλ=0.

Fig. 8. ROC versus position of peak irradiance Zp for a microlens of Ø=635 µm, illuminated by a plane wave at four different wavelengths. The crossings between two curves corresponding to achromatic microlenses are shown with circles.

In Fig. 8, we observe that for each pair of wavelengths the different graphs are crossing in one point. From the UV to the IR a value for ROC is found where the longitudinal chromatic aberrations are zero for two different wavelengths. For our example of a microlens with diameter Ø=635 µm, the peak radiance at 248 nm and 1550 nm are equal zp(248 nm)=zp(1550 nm)=21.7mm for ROC=10.8 mm, Fig. 7.

Fig. 9. Relative variations on Zp calibrated at 550 nm for five microlenses of Ø=635 µm for five ROC, illuminated by a plane wave at different wavelengths.

To investigate an achromatic design for a microlens we fix a diameter. Then to allow comparisons a wavelength of reference fixing Zp is required. It is now possible to plot the relative variations of this Zp against the wavelength of a defined spectrum. For example, Fig. 9 shows the variations as function of the wavelength of Zp expressed in percent of the Zp calibrated at 550 nm. This is done for different ROC while for each lens Zp at 550 nm is taken to normalize. The effect of diffraction appears when ROC increases. Correction of chromatic aberrations is possible for curve shapes that show a maximum in the desired wavelengths region. It would seem that small curvature (large radius of curvature) of the plot at the maximum would lead to small chromatic aberration in Fig. 9. Curves for ROC=20.2 mm (FN=4), 12.6 mm (FN=6) and 10.1 mm (FN=8) in Fig. 9 show a maximum. Note, that the FN are calculated at 550 nm. The maximum shifts to shorter wavelengths for increasing ROC. The microlens with a ROC fixed to 10.1 mm shows less than 1 ‰ variation on Zp from 530 nm to 690 nm. For comparison the microlens with ROC=2 mm is not influenced by diffraction effects and shows more than 8 ‰ variations on Zp inside the same range. For this wavelengths range we see from Fig. 9 that the lens with ROC=10.1 mm represents an optimum design for a lens of 635 µm diameter. The position of the peak irradiance is 21.5 mm.

6. Conclusion

It is well known from geometric optics that increasing the focal length of any lens leads to increase its ROC. This is the case for lenses having large values of FN≫1. By comparison, microlenses by their small diameters impose small value for ROC and then short focal length. When designing a microlens with large ROC, diffraction at the lens aperture may severely dominate the optical properties of the microlens and limit the range of the effective focal length. The upper limit of the focal length is determined by the diffraction pattern of a pinhole with equal diameter. Moreover refraction and diffraction have opposing influence on the position of the peak irradiance when changing the wavelength of illumination. Diffraction at the lens stop can be used to correct chromatic aberration introduced from the dispersion of the lens material. For microlenses with low Fresnel numbers (FN<10), achromatic designs can be realized in one single material.

References

1.

D. Malacara and Z. Malacara, Handbook of lens design, (Dekker, New York, 1994).

2.

Y. Li and E. Wolf, “Focal shifts in diffracted converging spherical waves,” Opt. Commun. 39, 211 (1981). [CrossRef]

3.

Y. Li and H. Platzer, “An experimental investigation of diffraction patterns in low Fresnel-number focusing systems,” Optica Acta 30, 1621 (1983). [CrossRef]

4.

W. Wang, A. T. Friberg, and E. Wolf, “Structure of focused fields in systems with large Fresnel numbers,” J. Opt. Soc. Am. A. 12, 1947 (1995). [CrossRef]

5.

J. Arnaud, “Representation of Gaussian beams by complex rays,” Appl. Opt. 24, (1985). [CrossRef] [PubMed]

6.

U. Vokinger, R. Dändliker, P. Blattner, and H. P. Herzig, “Unconventional treatment of focal shift,” Opt. Commun. 157, 218–224 (1998). [CrossRef]

7.

J. W. Goodman, Introduction to Fourier Optics, 2nd ed., (MacGraw-Hill, New York, 1968), Chap. 4, pp. 63–69.

OCIS Codes
(130.0130) Integrated optics : Integrated optics

ToC Category:
Integrated Optics

History
Original Manuscript: March 30, 2006
Revised Manuscript: May 9, 2006
Manuscript Accepted: May 10, 2006
Published: May 29, 2006

Virtual Issues
Vol. 1, Iss. 6 Virtual Journal for Biomedical Optics

Citation
Patrick Ruffieux, Toralf Scharf, Hans Peter Herzig, Reinhard Völkel, and Kenneth J. Weible, "On the chromatic aberration of microlenses," Opt. Express 14, 4687-4694 (2006)
http://www.opticsinfobase.org/oe/abstract.cfm?URI=oe-14-11-4687


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References

  1. D. Malacara, and Z. Malacara, Handbook of lens design, (Dekker, New York, 1994).
  2. Y. Li, and E. Wolf, "Focal shifts in diffracted converging spherical waves," Opt. Commun. 39,211 (1981). [CrossRef]
  3. Y. Li, and H. Platzer, "An experimental investigation of diffraction patterns in low Fresnel-number focusing systems," Optica Acta 30,1621 (1983). [CrossRef]
  4. W. Wang, A. T. Friberg, E. Wolf, "Structure of focused fields in systems with large Fresnel numbers," J. Opt. Soc. Am. A. 12,1947 (1995). [CrossRef]
  5. J. Arnaud, "Representation of Gaussian beams by complex rays," Appl. Opt. 24, (1985). [CrossRef] [PubMed]
  6. U. Vokinger, R. Dändliker, P. Blattner, and H. P. Herzig, "Unconventional treatment of focal shift," Opt. Commun. 157,218-224 (1998). [CrossRef]
  7. J. W. Goodman, Introduction to Fourier Optics, 2nd ed., (MacGraw-Hill, New York, 1968), Chap. 4, pp. 63-69.

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