JODAS, © 2001-2006

Telescopes

Refractors
Doublet
Triplet
Reflectors
Catadioptric

Triplet

Introduction
After Fraunhofer and Steinheil objectives, the triplet is thethird type of objective commonly used in refracting telescopes. This is a photo-visual objective. The use of three different glasses permits a considerable reduction of chromatic difference of focus over a given spectral range to be obteined. This objective is almost equally good for photographic and visual wavelengths, and at one time was popular for astronomical use at apertures up to about 12“.

Additionally, triplet refractors can be designed to work at focal ratios between f/6 and f/10, as compared with the f/15 focal ratio of a conventional doublet. A triplet corrected for three colors is called an apochromat, whereas a triplet corrected for four colors is termed a superachromat (by Max Herzberger). The first element is biconvex, the second biconcave, and the third element biconvex.

The steep curves of the centre component, making centering difficult, and the early use of unstable varieties of flint glass, have detracted, however, from the value of these lenses.

Optical Schema: Ray Tracing Optical Schema: Telescope Specifications


Design and Optimization
The designing a triplet is nearly the same as designing a doublet. But there are some important differences. When designing a triplet, the choice of a proper glass combination is very important, so much so that it is the coice of glass, and not the design process, that is the most time-consuming part of making a new design.

With a triplet, the number of design parameters is higher than with a doublet. The additional parameters are the curvature ratio R5/R4 and the lens power ratio F3/F2. Because there are more ways to achieve very low spherical aberration and OSC with apochromatic color correction, designing a triplet is considerably more complex than designing a doublet.

In general a suitable combination of glasses for a triplet consists of: A combination of glasses suitable for a triplet will form a wide triangle in the P-V diagram. The larger the area of this triangle is, the easier the design will be. Such combination of glasses consists BK7, KzFS1 and BaFN10. Other combination use the same BK7, KzFS1 glasses, but the BaFN10, a relatively inexpensive glass is replaced by the considerably more expensive glass TiF2. Under no circumstances can these glasses lie on a straight line in the P-V diagram. If this were the case, the elements would have to have very high powers, which would hinder the correction of the aberrations. In principle, there are numerous possible combinations of glass for an apochromat (for an objective to be corrected for three colors, such as blue, green and red).

When we require that the lens bring four colors to a common focus (violet, blue, green and red), the three glasses must satisfy an additional condition. It can be shown mathematically that when four colors are to be corrected, the three glasses in the P-P (Pec-Pge) diagram will lie on a straight line. This is the case for the combination that includes TiF2. The glass combination with BaFN10 glass does not satisfy the straight line condition and with this combination only three color can be brought into a common focus.

In the design of a broken triplet, we use the variables R1, R3/R2 and R5/R4 to correct spherical aberration and coma, while lens power ratios F2/F1 and F3/F2 are used to minimize the influence of spherochromatism. We start with changing the values of R3/R2 and R5/R4 for one starting value of R1 (default value is 1.04 of the triplet focal length). Through trial and error, we determine what particular combination of both variables gives the smallest LA and OSC. We repeat the procedure for other values of R1 until the best values of LA and OSC are obtained. During the first trials, the three desired colors generally do not focus at a common point on the LA-curves. As soon as the value of LA has been sufficiently decreased, we vary slightly the powers of the first and second lens with respect to the third lens.After several trials, the colors are made to coincide and intersect somewhere between to 70% and 100% zone. After correcting spherochromatism, we continue to optimize LA and OSC.

Designing cemented and immersion objectives is difficult because the airgraps are fixed at zero and both curvature ratios are fixed at unity. Only R1 and the lens power are free parameters. In this case all other radii depend on the chosen value of R1. Often it is not possible to correct LA and OSC sufficiently with R1 alone and we must vary with F2/F1 and F3/F2 to achieve a good design.

Applet Tag: Note: Relation between index number and color:
Keywords: telescope optical design optics optician software freeware source code excel visual basic applications java scripts applets cgi borland turbo pascal delphi kylix c++ builder dos windows linux susse redhat astronomy ray trace raytrace raytracing spot diagram aberration seidel third order spherical coma astigmatism distortion chromatism spherochromatism opd optical path diference encircled ensquared fft psf mtf otf optimization optimize global local merit function damped least square dlsq lsq tolerance layout telescope refractor objective doublet achromatic aplanatic cemented broken airspaced fraunhofer steinheil clark triplet christen glass schott hoya hikari ohara sumita corning gost lzos reflector mirror sphere ellipsoid prolate oblate paraboloid hyperboloid toroid mangin one mirror newtonian dob dobson dobsonian two mirror cassegrain gregorian ritchey-chretien dall-kirkham pressmann-camichel schwarzschild three mirror loveday picht catadioptric camera maksutov schmidt baker wright sigler gregory simak rumak relay wright lurie houghton loveday tct tilted brachyt shiefspiegler yolo off-axis stevick stevick-paul brunn kutter buchroeder herschel focal corrector extender reducer flattener plate lens menisc meniscus barlow ross winn bird brixner eyepices huygenian abbe ramsden kellner erfle plössl ploessl könig koenig ortoscopic amateur astronomer telescope maker atm atm's modas jodas eodas ivan krastev oslo zemax sigma vob code v optix optalix lensview winlens asap synopsis raycad opticad optikwerks winlens winspot optec optica opticalc lensview atmos dboptic opus autoray ados kdp roadrunner aberrator test startest grid terebizh ronchi mosby null inverse wire foucault knife edge millues-lacroix sinnott texerau book article magazine journal letters atmj atmlj sky & telescope skywatch amateurastronomy coelum applied optics josa sterne und weltraum starobserver