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Topic 6: Optical Systems Aim: To apply the image formation theory to - PDF document

I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N Topic 6: Optical Systems Aim: To apply the image formation theory to basic real optical sys- tems and how they are designed. Contents: 1. Basic Design


  1. I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N Topic 6: Optical Systems Aim: To apply the image formation theory to basic real optical sys- tems and how they are designed. Contents: 1. Basic Design Criteria. 2. Available lens types and materials. 3. Ray Tracing 4. Evaluation of ray tracing. O P T I C D S E G I R L O P P U A P D S Real Systems -1- Autumn Term C E P I S A Y R H T P M f E o N T

  2. I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N Design Criteria Aim of Lens Design is to form a system that has “sufficiently good” performance in a given geometry. There are no universal solutions, but a range of good solutions have been developed over the last 100 years. Before you start designing a system you need consider: � Numeric Aperture (or F No ). � Field angle. � Range of wavelength (mono or poly chromatic). � Location on object and image planes. � Quality needed. � Cost and complexity allowable. Use this information to look-up the “Type of Lens” you will need. (Don’t want to use a 7 element lens when a 2 element will do). The aim of lens design is to cancel the aberrations with combinations of lenses, mirrors and (perhaps) holograms. O P T I C D S E G I R L O P P U A P D S Real Systems -2- Autumn Term C E P I S A Y R H T P M f E o N T

  3. I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N System Types 90 180 Fisheye 60 120 50 Retro-Focus 100 Angulon 30 60 Tessar Double Gauss 30 15 Landscape Triplet Split Triplet 10 Petzval 20 Half Field Angle Full Field Angle 8 16 Schmidt- 10 5 Cassegrian Schmidt 8 4 5 4 2 Ritchey-Chretien Microscope 3 Objective 2 1 Cassegrian 1 0.5 Optical Disk Objective Achromatic Doublet Parabola na 0.2 0.1 0.05 1.0 0.02 0.5 Fno 25 15 10 5 1.5 1 3 2 0.8 0.5 Diagram of system types for various ranges of F No and Field Angle , (from Modern Lens Design , WJ Smith, Academic Press) O P T I C D S E G I R L O P P U A P D S Real Systems -3- Autumn Term C E P I S A Y R H T P M f E o N T

  4. I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N Lens Types and Materials. 95% of optical surface are spherical and 99% of optical systems are “on-axis” (cylinderically symmertic). Why? 1. Spherical surface are easy to make by polishing. 2. Design with spherical surfaces well developed. 3. On-axis easy to design and make. Spherical Surface Lenses Spherical Dome Mass produce spherical surfaces, convex surfaces on a “dome”, con- cave on a “depression”. Accurate surfaces, but less control on lens thickness. O P T I C D S E G I R L O P P U A P D S Real Systems -4- Autumn Term C E P I S A Y R H T P M f E o N T

  5. I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N Other Types Other surfaces possible, these include Reflective Surfaces: 1. No dispersion, (any wavelength). 2. Folded or “off-axis” optical systems. 3. Results in “short” system. 4. Relatively expensive. 5. Easy(ish) to make very large (4 m diameter mirrors have been made). 6. Mixed reflective/refractive system. Secondary Mirror Small spherical optics Glass Window Film Plane Primary Mirror Long focal length “mirror” type camera lens, (1000 mm). Two mirrors, (usually slightly aspheric). Used extensively in large telescopes. O P T I C D S E G I R L O P P U A P D S Real Systems -5- Autumn Term C E P I S A Y R H T P M f E o N T

  6. I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N Aspheric Surfaces: 1. Molded glass light collection systems (in projectors). 2. Individual polishing or diamond machining. Both “one-off” man- ufacture, so expensive. 3. Used to deduce number of elements where weight or light effi- cency is essential. 4. Plastic molded surfaces. Plastic not ideal optical material. Aspheric Condensor To Screen Slide Projector Lens Spherical Mirror (Multi element Spherical) Spherical Singlet Projector system has one aspherical surface to correct SA in the con- densor. O P T I C D S E G I R L O P P U A P D S Real Systems -6- Autumn Term C E P I S A Y R H T P M f E o N T

  7. I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N Diffractive Optics: 1. Fresnel lens: Cheap and easy to make, but poor optical quality. Good to large light collection systems (OHP). 2. Holographic Optics: Monochromatic light only, difficult to mass produce. Specilist applications. Imaging Optics To Screen Slide Slide Table Fresnel Lens Lamp (smallish) Spherical Mirror The OHP has a Fresnel (diffractive) condensor to collect light, but all other components are conventional glass spherical surfaces. O P T I C D S E G I R L O P P U A P D S Real Systems -7- Autumn Term C E P I S A Y R H T P M f E o N T

  8. I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N Optical Materials Two basic optical measures of material performance: = Refractive index at Sodium d-line n d and Abbe Number (also know as V -number), given by � 1 = n d V d n f � n c where n f Refractive index at Hydrogen f-line ! n c Refractive index at Hydrogen c-line ! where lines are at: Na d-line 587nm (Y ellow) ! H f-line 486nm (Blue/green) ! H c-line 656nm (Red) ! Available materials have: 1 : 4 ! 2 : 2 = n d 80 ! 20 = V d most common glass is borosilicate crown (Schotts BK7), with = 1 : 51680 & = 64 : 29 n d V d Many hundreds of optical glasses and plastics made with vast range of n d and V d values. O P T I C D S E G I R L O P P U A P D S Real Systems -8- Autumn Term C E P I S A Y R H T P M f E o N T

  9. I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N Glass Plot Scatter plot of Refractive Index agaisnt Abbe Number Note: Low Abbe Number means high dispersion, so most high re- fractive index glasses have high dispersion. O P T I C D S E G I R L O P P U A P D S Real Systems -9- Autumn Term C E P I S A Y R H T P M f E o N T

  10. I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N Glass Properties: � Good optical quality, easy to polish spherical surfaces. � Vast range of n and V values available. � Thermally stable. Ignore expansion in almost all systems. � Optical coatings easy. � Many factory made components. Problems: range of problems selecting glass type, obvious ones are: � Relatively easily broken. � Heavy especially high n glasses that contain lead. � Some high n glasses are “coloured”, or unstable. � Factor of 1:300 (1:1000) in cost of raw material. � Aspheric surface very difficult and expensive. � Thickness of lens difficult to control in manufacture. Almost all high quality optical systems use glass optics. O P T I C D S E G I R L O P P U A P D S Real Systems -10- Autumn Term C E P I S A Y R H T P M f E o N T

  11. I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N Optical Plastics Plastic lenses look very attractive since: � Easy to make in large numbers. � Low cost of raw material. � Aspheric surfaces easy, (once mold is made). � Light and almost unbreakable. � Lens thickness easy to control. � Dye material to produce colour filters. However the range of problems are rather sever, being � Very limited range of n d and V d . � Soft surface, and coatings difficult. � High thermal expansion ( � 8 that of glass) and Refractive index � 100 that of glass.) is temperature dependant, ( > � Expensive is small numbers due to cost of mold. � Doublets not possible (thermal expansion problems.) Useful for “low tech” optics only, spectical lenses, low-cost cameras, magnifiers. = 1 : 67 and V d = 32 just available in 1997. New plastics with n d O P T I C D S E G I R L O P P U A P D S Real Systems -11- Autumn Term C E P I S A Y R H T P M f E o N T

  12. I V N E U R S E I H T Modern Optics Y T O H F G R E U D B I N Other Materials Most glasses opaque outwith 350 ! 1300nm , so have to use other materials. Ultraviolet: Fused quartz, calcium or lithium floride. Relatively few materials, expensive and difficult to shape. Also tend to be birefrin- gent, and “cloudy”. Mainly used in spectrometer optics and UV mi- croscope objectives. � 2 µ m , beyound that Infrared: Limited range of glass transparent to > 1 : 5 µm ). Also need to use Germanium or Silicon (both transparent Sodium Chloride (Salt) possible. Thermal IR ( 10 µm ) of major importance. Mainly used diamond turned � 4 and no aspheric germanium lenses. Very high refractive index n good optical coatings so large reflection problems. Very expensive. O P T I C D S E G I R L O P P U A P D S Real Systems -12- Autumn Term C E P I S A Y R H T P M f E o N T

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