ECEN 4616/5616 2/4/2013 Dispersion and Achromats Zemax’s “Glass Map”: The index of refraction of glasses is traditionally taken at three wavelengths (for use in the visible). These are the Fraunhofer lines for hydrogen and helium ( a nearby line from mercury was used before helium became widely available). These were convenient, because they spanned the visible spectrum and could be duplicated with great precision in any well-equipped laboratory. F (hydrogen) 486nm d (helium) 588 nm C (hydrogen) 656 nm pg. 1 ECEN 4616/5616 2/4/2013 In the “glass map”, the index of refraction is the index at the d line (nd), and the ‘Abbe Number’ (often called the “V-number” by those who aren’t sure how to pronounce “Abbe”) is: n 1 Vd d nF nC The significance of this value follows from the calculation of the chromatic variation of power for a thin lens. 1 1 Power at d: K d nd 1 nd 1C R1 R2 Power at F: nF 1C Power at C: nC 1C Consider: K F K C nF 1C nC 1C nF nC 1 nd 1C Kd nd 1 Vd Hence: K K F KC d Vd From the image equation, we have: 1 1 1 1 K F , and KC lF lF lC lC 1 1 K K F KC d lF lC Vd So, the change in power is proportional to the power divided by the Abbe number. (It can also be shown that change in magnification with wavelength – transverse K chromatic aberration – is also proportional to d . Vd Hence, chromatic aberration (longitudinal and transverse) will be corrected (paraxially) if we use two lenses whos ratios sum to zero: K1 K 2 0 V1 V2 where the K’s are implicitly calculated at the d wavelength. For two thin lenses in contact, K K1 K2 . Solving these two equations, we get: VK VK K1 1 and K 2 2 V1 V2 V1 V2 So, we can create a compound lens without (to first order) chromatic aberration by combining a positive and negative lens made with glasses that have different V-numbers. pg. 2 ECEN 4616/5616 2/4/2013 (Note that, since all V-numbers are positive, the first equation can only be satisfied if the powers are one positive and one negative.) Equivalent V-Number: Suppose we design a doublet with a non-zero change in chromatic focal power: K K1 K 2 K K . Since, from K F K C d , we can define V , we can say the K V1 V2 Vd K1 K 2 . Hence we can produce a the effective V-number of our doublet is V K1 K 2 V1 V2 compound lens with an effective V-number that wouldn’t be available from a single glass. This can prove useful in correcting optical instruments with widely separated elements such as microscope and telescopes – the eyepiece can be designed to correct the chromatic aberrations of the objective, for instance, allowing more freedom to design the objective’s performance. pg. 3