Download Applied Optics and Optical Design, Parts One and Two by Conrady A PDF

By Conrady A

This booklet offers a whole approach of optical layout. It leads the reader step-by-step from the basic options of geometrical and actual optics as much as the purpose the place they could layout less complicated optical platforms with no relief. half One covers all traditional ray-tracing tools, including the entire conception of basic aberration and as a lot of upper aberration as is required for the layout of telescopes, low-power microscopes, and straightforward optical platforms. half deals systematic examine and layout of essentially all kinds of optical platforms. This vintage paintings continues to be the one specific remedy of topic for useful dressmaker.
Content:
• entrance topic
• Preface
• desk of Contents
•Part I• creation
1. primary Equations
2. round Aberration
three. actual point of Optical pictures
four. Chromatic Aberration
five. layout of Achromatic Object-Glasses
6. Extra-Axial Image-Points
7. The Optical Sine Theorem
eight. Trigonometrical Tracing of indirect Pencils
nine. common idea of excellent Optical structures
10. traditional Eyepieces
Appendix
•Part II entrance subject
• Editor's Preface
eleven. extra suggestions by way of the Thin-Lens process
12. Optical course variations
thirteen. Optical direction transformations at an Axial Image-Point
14. Optical Tolerances
15. Chromatic Aberration as an OPD
sixteen. The Matching precept and the layout of Microscope pursuits
17. basic Aberrations of indirect Pencils
18. Analytical ideas for easy platforms with distant cease
19. Symmetrical Photographic pursuits
20. Unsymmetrical Photographic pursuits
Appendices
Index

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Additional info for Applied Optics and Optical Design, Parts One and Two

Example text

U'2 = dl . N . u2 and this form of the equation enables us to determine the longitudinal magnification for any centred system, in close analogy with the same stage in the development of the theorem of Lagrange. For a first surface we shall have dl{ . N{ . u{2 = dl; . N l . u l 2, and for a second surface dl; . N; . u? = dl 2 • N 2 . u~. Obviously the axial image dt{ by the first surface acts as the axial object for the second, therefore dl{ ::::: d12; and as N{ ::::: N 2 and u{ ::::: U 2 by the fundamental conventions, the left of the first equation is identical with the right of the second; hence FUNDAMENTAL EQUATIONS 45 and it is evident that these arguments can be repeated any number of times, thus [19] leading to the general theorem of longitudinal magnification dl k .

For particularly erratic computers equation (7) supplies also by far the safest and surest check against errors caused by applying the refractive indices wrongly in the main calculation; such computers (who may be excellent designers in spite of their liability to numerical mistakes) will therefore be wise to adopt (7) instead of the simpler check depending on (6) as a regular part of their computing formulae. When (7) is used the V' for closing the standard calculation and for computing (5)** is of course determined as the starting value of V plus twice the value of t (1 - 1') obtained from (7) ; as in all optical calculations, the sign of all the quantities must be carefully watched.

Every computer therefore should be extremely careful in putting in the given quantities. Our optical formulae provide an ugly trap in this respect in the introduction of the refractive index which enters only once, namely in obtaining sin l' from sin I by equation (2). No one would doubt for a moment that the introduction of a wrong value of NfN' would necessarily lead to a wrong result which would nevertheless satisfy any check that could be applied to it, simply because the result so obtained is the right one for the indices actually used.

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