Achromatic lens

Chromatic aberration of a single lens causes different wavelengths of light to have differing focal lengths.

An achromatic doublet brings red and blue light to the same focus, and is the earliest example of an achromatic lens.

In an achromatic lens, two wavelengths are brought into the same focus, here red and blue.

An achromatic lens or achromat is a lens that is designed to limit the effects of chromatic and spherical aberration. Achromatic lenses are corrected to bring two wavelengths (typically red and blue) into focus on the same plane.

The most common type of achromat is the achromatic doublet, which is composed of two individual lenses made from glasses with different amounts of dispersion. Typically, one element is a negative (concave) element made out of flint glass such as F2, which has relatively high dispersion, and the other is a positive (convex) element made of crown glass such as BK7, which has lower dispersion. The lens elements are mounted next to each other, often cemented together, and shaped so that the chromatic aberration of one is counterbalanced by that of the other.

In the most common type (shown), the positive power of the crown lens element is not quite equalled by the negative power of the flint lens element. Together they form a weak positive lens that will bring two different wavelengths of light to a common focus. Negative doublets, in which the negative-power element predominates, are also made.

History[]

Theoretical considerations of the feasibility of correcting chromatic aberration were debated in the 18th century following Newton's statement that such a correction was impossible (see History of the telescope). Credit for the invention of the first achromatic doublet is often given to an English barrister and amateur optician named Chester Moore Hall.^[1]^[2] Hall wished to keep his work on the achromatic lenses a secret and contracted the manufacture of the crown and flint lenses to two different opticians, Edward Scarlett and James Mann.^[3]^[4]^[5] They in turn sub-contracted the work to the same person, George Bass. He realized the two components were for the same client and, after fitting the two parts together, noted the achromatic properties. Hall used the achromatic lens to build the first achromatic telescope, but his invention did not become widely known at the time.^[6]

In the late 1750s, Bass mentioned Hall's lenses to John Dollond, who understood their potential and was able to reproduce their design.^[2] Dollond applied for and was granted a patent on the technology in 1758, which led to bitter fights with other opticians over the right to make and sell achromatic doublets.

Dollond's son Peter invented the apochromat, an improvement on the achromat, in 1763.^[2]

Types[]

Several different types of achromat have been devised. They differ in the shape of the included lens elements as well as in the optical properties of their glass (most notably in their optical dispersion or Abbe number).

In the following, R denotes the radius of the spheres that define the optically relevant refracting lens surfaces. By convention, R₁ denotes the first lens surface counted from the object. A doublet lens has four surfaces with radii R₁ to R₄.

Littrow doublet[]

Uses an equiconvex crown glass lens with R₁ = R₂, and a second flint glass lens with R₃ = -R₂. The back of the flint glass lens is flat. A Littrow doublet can produce a ghost image between R₂ and R₃ because the lens surfaces of the two lenses have the same radii.

Fraunhofer doublet (Fraunhofer objective)[]

The first lens has positive refractive power, the second negative. R₁ is set greater than R₂, and R₂ is set close to, but not equal to, R₃. R₄ is usually greater than R₃. In a Fraunhofer doublet, the dissimilar curvatures of R₂ and R₃ are mounted close, but not in contact.^[7] This design yields more degrees of freedom (one more free radius, length of the air space) to correct for optical aberrations.

Clark doublet[]

Early Clark lenses follow the Fraunhofer design. After the late 1860s, they changed to the Littrow design, approximately equiconvex crown, R₁ = R₂, and a flint with R₃ ≃ R₂ and R₄ ≫ R₃. By about 1880, Clark lenses had R₃ set slightly shorter than R₂ to create a focus mismatch between R₂ and R₃, thereby avoiding ghosting caused by reflections within the airspace.^[8]

Oil-spaced doublet[]

The use of oil between the crown and flint eliminates the effect of ghosting, particularly where R₂ = R₃. It can also increase light transmission slightly and reduce the impact of errors in R₂ and R₃.

Steinheil doublet[]

The Steinheil doublet, devised by Carl August von Steinheil, is a flint-first doublet. In contrast to the Fraunhofer doublet, it has a negative lens first followed by a positive lens. It needs stronger curvature than the Fraunhofer doublet.^[9]

Dialyte[]

Dialyte lenses have a wide air space between the two elements. They were originally devised in the 19th century to allow much smaller flint glass elements down stream since flint glass was hard to produce and expensive.^[10] They are also lenses where the elements can not be cemented because R₂ and R₃ have different absolute values.^[11]

Design[]

The first-order design of an achromat involves choosing the overall power $\phi _{\text{sys}}$ of the doublet and the two glasses to use. The choice of glass gives the mean refractive index, often written as $n_{d}$ (for the refractive index at the Fraunhofer "d" spectral line wavelength), and the Abbe number $V$ (for the reciprocal of the glass dispersion). To make the linear dispersion of the system zero, the system must satisfy the equations

{\begin{aligned}\phi _{1}+\phi _{2}&=\phi _{\text{sys}}\\{\frac {\phi _{1}}{V_{1}}}+{\frac {\phi _{2}}{V_{2}}}&=0\ ,\end{aligned}}

where the lens power is $\phi =1/f$ for a lens with focal length $f$ . Solving these two equations for $\phi _{1}$ and $\phi _{2}$ gives

{\frac {\phi _{1}}{\phi _{\text{sys}}}}={\frac {V_{1}}{V_{1}-V_{2}}}\qquad {\text{and}}\qquad {\frac {\phi _{2}}{\phi _{\text{sys}}}}={\frac {-V_{2}}{V_{1}-V_{2}}}\ .

Since $\phi _{2}=-\phi _{1}V_{2}/V_{1}$ , and the Abbe numbers are positive-valued, the power of the second element in the doublet is negative when the first element is positive.

Further color correction[]

Focus error for four types of lens, over the visible and near infrared spectrum.

Lens designs more complex than achromatic can improve the precision of color images by bringing more wavelengths into exact focus, but require more expensive types of glass, and more careful shaping and spacing of the combination of simple lenses:

apochromatic lenses: bring three wavelengths into a common focus and requires costly materials
superachromatic lenses: bring four wavelengths into focus and must be manufactured with even more expensive fluoride glass and to considerably tighter tolerances

In theory, the process can continue indefinitely: Compound lenses used in cameras typically have six or more simple lenses (e.g. double-Gauss lens); several of those lenses can be made with different types of glass, with slightly altered curvatures, in order to bring more colors into focus. The constraint is extra manufacturing cost, and diminishing returns of improved image for the effort.

References[]

^ Daumas, Maurice, Scientific Instruments of the Seventeenth and Eighteenth Centuries and Their Makers, Portman Books, London 1989 ISBN 978-0-7134-0727-3
^ ^a ^b ^c Watson, Fred (2007). Stargazer: the life and times of the telescope. Allen & Unwin. pp. 140–55. ISBN 978-1-74175-383-7.
^ Fred Hoyle, Astronomy; A history of man's investigation of the universe, Rathbone Books, 1962, LCCN 62-14108
^ J. A. B. "Peter Dollond answers Jesse Ramsden". Sphaera 8. Museum of the History of Science, Oxford. Retrieved November 27, 2017. – A review of the events of the invention of the achromatic doublet with emphasis on the roles of Hall, Bass, John Dollond and others.
^ Dokland, Terje; Ng, Mary Mah-Lee (2006). Techniques in microscopy for biomedical applications. p. 23. ISBN 981-256-434-9.
^ "Chester Moor Hall". Encyclopædia Britannica. Retrieved 16 February 2019.
^ Wolfe, William L. (2007). Optics Made Clear: The Nature of Light and how We Use it. Press monograph. Vol. 163 (illustrated ed.). SPIE. p. 38. ISBN 9780819463074.
^ Warner, Deborah Jean; Ariail, Robert B. (1995). Alvan Clark & Sons, Artists In Optics (2nd ed.). Willmann-Bell. p. 174.
^ Kidger, M.J. (2002) Fundamental Optical Design. SPIE Press, Bellingham, WA, pp. 174ff
^ Peter L. Manly (1995). Unusual Telescopes. Cambridge University Press. p. 55. ISBN 978-0-521-48393-3.
^ Fred A. Carson, Basic optics and optical instruments, page AJ-4

External links[]

Media related to Achromatic lenses at Wikimedia Commons

[daumas-1] Daumas, Maurice, Scientific Instruments of the Seventeenth and Eighteenth Centuries and Their Makers, Portman Books, London 1989 ISBN 978-0-7134-0727-3

[Stargazer-2] Watson, Fred (2007). Stargazer: the life and times of the telescope. Allen & Unwin. pp. 140–55. ISBN 978-1-74175-383-7.

[3] Fred Hoyle, Astronomy; A history of man's investigation of the universe, Rathbone Books, 1962, LCCN 62-14108

[Dollond-4] J. A. B. "Peter Dollond answers Jesse Ramsden". Sphaera 8. Museum of the History of Science, Oxford. Retrieved November 27, 2017. – A review of the events of the invention of the achromatic doublet with emphasis on the roles of Hall, Bass, John Dollond and others.

[5] Dokland, Terje; Ng, Mary Mah-Lee (2006). Techniques in microscopy for biomedical applications. p. 23. ISBN 981-256-434-9.

[6] "Chester Moor Hall". Encyclopædia Britannica. Retrieved 16 February 2019.

[7] Wolfe, William L. (2007). Optics Made Clear: The Nature of Light and how We Use it. Press monograph. Vol. 163 (illustrated ed.). SPIE. p. 38. ISBN 9780819463074.

[8] Warner, Deborah Jean; Ariail, Robert B. (1995). Alvan Clark & Sons, Artists In Optics (2nd ed.). Willmann-Bell. p. 174.

[9] Kidger, M.J. (2002) Fundamental Optical Design. SPIE Press, Bellingham, WA, pp. 174ff

[10] Peter L. Manly (1995). Unusual Telescopes. Cambridge University Press. p. 55. ISBN 978-0-521-48393-3.

[11] Fred A. Carson, Basic optics and optical instruments, page AJ-4

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