JODAS, © 2001-2006

Telescopes

Refractors
Doublet
Triplet
Reflectors
Catadioptric

Doublet

Introduction
An objective with the crown lens in front is the usual form, originally known as the Fraunhofer objective. The positive crown element of this air-spaced doublet is in front, the negative flint at the rear. The interior radius of curvatures are unequal, and air-space is small (about 2-5 mm).

Optical Schema: Ray Tracing Optical Schema: Telescope Specifications


The Steinheil, or „flint-in-front“, objective is less used because of the greater suscepttibility of the flint glass (less stable than crown glass) to atmospheric attack. The Steinheil objective is also used when offers better correction of aberrations. However, because it has stronger curves, it is seldom used unless necessary.

Optical Schema: Ray Tracing Optical Schema: Telescope Specifications


Design and Optimization
The design of an achromatic refractor doublet is a trial and error process. The designer varies the available degrees of freedom until the aberrations have been reduced to an acceptable level. It is important to work systematically. The design procedure includes four steps. These are: If the aberration or spot size cannot be reduced to an acceptable level, the designer returns to the first step.

To start design select from the pull down menu "Refractor | Doublet". The Achromatic Doublet design and analysis applet appears and you can input/change the general doublet data, such as clear diameter, system focal length, edge thickness of the positive lens and center thickness of the negative lens. For a 200 mm lens the minimum edge thickness for the positive lens and the minimum axial thickness for the negative lens will be around 15 mm. In a positive lens the center thickness is always larger than the edge thickness.

The last input is the glass type selection. This is maybe the most important element of the design whose success depends upon the correct glass selection. The following rules apply to the choice of glass: After all data needed for the design has been input we can start the optimization procedure by pressing the Solve button. This will compute all data, which is necessary for calculation and plotting of the longitudinal spherical aberration, i.e.: Correcting Spherical Aberration
Now we can proceed to the optimization (iterative process) by using the scroll bars for the corresponding six optimization parameters. What do we need to know for the optimization procedure of an achromatic doublet.

For a cemented doublet, the width of the air space (air gap) is zero, and R2=R3. In an air spaced doublet, the air gap between the lenses is typically set to 1 or 2 millimeters. The initial values of the radii of curvatures are not very critical, but it is useful to study some existing designs before starting. We might assume an initial R1 equal to 2/3 of the focal length of the objective. Making R2 and R3 different is an effective tool in reducing spherical aberration. Suppose we set R3/R2 equal to 1.01 for a Fraunhofer design and to 0.99 for a Steinheil type.

After bending the two lenses so that longitudinal spherical aberration is corrected, you will often discover that the red light and the blue light curves are not crossed and we must move the blue curve with respect to the red curve. This is accomplished by giving the first lens a slightly stronger power (i.e. shorter focal length). The lens power factor of the first lens in a Fraunhofer type doublet normally lies between 1.00 and 1.01, while that of the negative first lens of a Steinheil objective lies between 1.01 and 1.02.

In summary, we can see that for a given set of glasses, the design process works by altering only three parameters: The designer works by manipulating these three variables until a satisfactory design solution has been achieved. The final design should be checked then by image quality analysis with some features available from the analysis buttons bar.

Other Optimization Parameters
If the designer cannot reduce the aberrations for a particular combination of glasses, a number of degrees of freedom remain. These are the thicknesses of the elements and the width of the air gap, if there is one. The air space is most useful in controlling spherical aberration. Making the air gap larger can reduce spherochromatism. This approach leads to a design called the Clark objective.

Another reason for selecting a larger lens separation is that the designer can achieve an aplanatic system with equal R2 and R3. This simplifies fabrication because the surfaces can be tested against each other by interference. If the ratio R3/R2 approaches unity as the separation of the elements is increased, then this goal can be achieved.

Unfortunately, a large lens distance has some disadvantages: it is very sensitive to decentering, and lateral color may occur. For this reason, the Clark objective is not often used.

The designer may also opt for a Steinheil objective rather than a Fraunhofer. However, only in exceptional cases can a better design be achieved with the Steinheil form.

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