
Optical Design Using Excel
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"This book is a handy and practical guide for scientists and engineers who are working in the laser optical system design field. It could also benefit graduate students and industry professionals interested in optics." (Optics & Photonics News, 5 October 2015)More details
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Hiroshi Nakajima, formerly Technical consultant, Hitachi High-Technologies Corporation, Tokyo, Japan (until March 2012).?Nakajima studied Electronics at?Doshisha University, Kyoto, Japan, between 1963 and 1967. Between 1967 and 2012 he worked in a variety of roles at Hitachi High-Technologies Corporation Technical in Japan, from which he is now retired.
Content
Preface i Outline of contents ii Chapter 1 - Geometrical optics 1 1.1 Characteristics of lasers 2 1.2 The three fundamental characteristics of light which form the basis of geometrical optics 3 1.3 Fermat's principle 4 1.4 Principle of reversibility 7 1.5 Paraxial theory using thin lenses 7 1.6 The five Seidel aberrations 15 1.7 The sine condition 21 1.8 Aplanatic lenses 23 1.9 Reflection and transmission 24 Chapter 2 - Examples of simple optical design using paraxial theory 27 2.1 Types of lenses 28 2.2 Applied calculations for simple optical systems 35 2.3 Considerations relating to the design of laser optical systems 42 Chapter 3 - Ray tracing applications of paraxial theory 47 3.1 Deriving the equations for ray tracing using paraxial theory 48 3.2 Problems of ray tracing calculations using paraxial theory 50 Chapter 4 - Two-dimensional ray tracing 53 4.1 Ray tracing for a spherical surface 54 4.2 Ray tracing for a plane surface 56 4.3 Ray tracing for an aspheric surface (using VBA programming) 57 4.4 Ray tracing for an aberration-free lens 60 4.5 Optical path length calculation for an aberration-free lens 62 4.6 Ray tracing for an optical system which is set at a tilt 65 4.7 How to use the ray trace calculation table 68 4.8 A method for generating a ray trace calculation table using a VBA program 73 4.9 Sample ray tracing problems 76 Chapter 5 - Three-dimensional ray tracing 101 5.1 Three-dimensional ray tracing for a spherical surface 102 5.2 Three-dimensional ray tracing for a cylindrical surface 105 5.3 Simulation for two cylindrical lenses which are fixed longitudinally (or laterally) but allowed to rotate slightly around the optical axis 106 5.4 Three-dimensional ray tracing for a plane surface which is perpendicular to the optical axis 108 5.5 Three-dimensional ray tracing for an aberration-free lens 109 5.6 Three-dimensional ray tracing for a lens which is set at a tilt 115 5.7 How to use the three-dimensional ray trace calculation table 121 5.8 Operating instructions for using the ray trace calculation table, while running the VBA program 125 5.9 Three dimensional ray tracing problems 128 Chapter 6 - Mathematical formulae for describing wave motion 137 6.1 Mathematical formulae for describing wave motion 138 6.2 Describing waves with complex exponential functions 142 6.3 Problems relating to wave motion 146 Chapter 7 - Calculations for focusing Gaussian beams 149 7.1 What is a Gaussian beam? 150 7.2 Equations for focusing a Gaussian beam 154 7.3 The M2 (M squared) factor 156 7.4 Sample Gaussian beam focusing problems 159 Chapter 8 - Diffraction: theory and calculations 167 8.1 The concept of diffraction 168 8.2 Diffraction at a slit aperture 170 8.3 Diffraction calculations using numerical integration 171 8.4 Diffraction at a rectangular aperture 173 8.5 Diffraction at a circular aperture 174 8.6 Diffraction wave generated after the incident wave exits a focusing lens 177 8.7 Diffraction calculation problems 178 Chapter 9 - Calculations for Gaussian beam diffraction 183 9.1 The power and the central irradiance of a Gaussian beam 184 9.2 General equations for waves diffracted by an aperture 189 9.3 Diffraction wave equations for a focused beam 191 9.4 Diffraction wave equations for a collimated beam 194 9.5 Diffraction calculation program 197 9.6 Operating instructions for diffraction calculation programs 198 9.7 Gaussian beam diffraction calculation problems 206 Appendix 219 Appendix A Paraxial theory: A detailed account 220 Appendix B A table of refractive indices for BK7 225 Appendix C Equations for plane waves, spherical waves and Gaussian beams 226 Appendix D Numerical integration methods 239 Appendix E Fresnel diffraction and Fraunhofer diffraction 241 Appendix F Wave-front conversion by a lens 245 Appendix G List of Excel calculation files on the companion Website 247 References 249
Index 250
Chapter 1
Geometrical Optics
1.1 Characteristics of Lasers
This book is about optical calculation methods and the principles for applying these methods to actual optical devices. Most of these devices use lasers, so we will begin by briefly examining the characteristics of lasers. The following exposition will be especially beneficial for readers whose understanding of lasers is rather limited.
The term LASER is an acronym for "Light Amplification by Stimulated Emission of Radiation." Lasers have special characteristics that distinguish them from most light-emitting devices: a narrow, low-divergence beam (sharp directivity), and a very narrow wavelength spectrum (monochromaticity). These features of lasers make them ideally suited for the generation of high intensity beams.
The history of lasers goes back about half a century to 1960, when the first working laser was demonstrated. Lasers are now widely used in a variety of fields, including optical storage (e.g., CD drives and DVD drives), fiber-optic communication, manufacturing (especially for cutting, bending, welding, and marking materials), scientific measurement, and medicine. This diversity of application is due to the following four properties of lasers, which give them a commercial and scientific edge over other light-emitting devices.
- 1. Monochromaticity: Radiation that has a very narrow frequency band (or wavelength band) is said to possess the property of monochromaticity. Because the band is so narrow, the radiation can be regarded as having a single frequency (or alternatively, a single wavelength). Laser light typically has a very narrow frequency band (or wavelength band), which makes it an ideal example of the property of monochromaticity. Sunlight, by contrast, has a very broad band spectrum, with multiple frequencies and wavelengths.
- 2. Beam directivity: The term directivity, when used in relation to lasers, refers to the directional properties of the electromagnetic radiation they emit. A laser beam exhibits a very sharp (narrow) directivity, allowing it to propagate in a straight line with almost no expansion. By contrast, normal light sources such as flashlights and car headlights have broader directivity than lasers, so their beams cannot travel as far.
- 3. Coherence: If split laser beams which were emitted from the same source are superimposed, a fringe pattern will appear. This fringe pattern is never observed in an isolated beam. We refer to this phenomenon as interference caused by the wave characteristics of light. If these two beams traveling onto the same plane are superimposed while they are in phase (with their crests and troughs lined up), the resultant beam will appear brighter, but if these waves are superimposed with a 180° phase difference (i.e., if crests and troughs are superimposed), the beam will appear dark and the resultant amplitude will be zero. A laser can easily generate interference patterns because of its coherence (uniformity of phase). Sunlight cannot readily generate interference patterns, due to its incoherence: because its coherence time and coherence length are very short, and the phases of the superimposed waves will not come into phase very easily. Sunlight will only exhibit coherence over a very short interval both of time and space.
- 4. High concentration of energy (high intensity): A sheet of paper can be burnt simply by focusing sunlight on it, using a convex lens. A laser is much more concentrated: it can even weld two pieces of steel together. This is not merely due to the high power of the laser, but also because of the extremely high intensity of the laser beam, where the light energy is narrowly focused. It is relatively easy to concentrate a laser beam on a small target. A high intensity beam can be generated very easily using a laser.
All of these characteristics of lasers can best be summed up by the word "coherent." A laser is both temporally coherent and spatially coherent. What this means is that a laser has a uniform phase over time at an arbitrary point in space, and it also has a uniform phase in space at an arbitrary point in time. Thus a laser has a uniform phase both in time and in space. A laser radiates a single-wavelength (more precisely, a very narrow wavelength spectrum) beam with a constant phase and it can propagate in a specific direction. An electric light, by contrast, radiates a multitude of different wavelengths at various phases and in all directions. Thus it is both spatially and temporally incoherent.
1.2 The Three Fundamental Characteristics of Light Which Form the Basis of Geometrical Optics
To understand geometrical optics, which is the most basic form of optics, we need to first study the fundamental characteristics of light - including light emitted by lasers. The following properties of light are confirmed by everyday experience:
- 1. Light rays travel in straight lines in a uniform medium.
- 2. Light rays are independent of one another.
- 3. Light rays can be reflected and refracted: they change their direction at a boundary between different media, in accordance with the laws of reflection and refraction.
The whole science of geometrical optics can be derived from these three characteristics of light.
1.2.1 Light Rays Travel in Straight Lines
Many common optical phenomena attest to the fact that light rays travel in straight lines. For instance, when the sun is shining outdoors, a tree casts a shadow whose shape is identical with its own. Without using any lenses, we can construct a pinhole camera that can capture the image of an object, simply by making a pinhole in one of the walls of a black box as shown in Figure 1.1.
Figure 1.1 Pinhole camera
1.2.2 Light Rays Act Independently of One Another
Figure 1.2 illustrates the independent action of light rays using the example of three spotlights whose light is of different colors: red, blue, and green. When we irradiate the same area on a white sheet of paper with these three spotlights, we perceive the light as "white." However, if we replace the paper with a mirror, and then project the reflected light onto another sheet of paper, the three separate beams of light reappear in their original colors of red, blue, and green. The fact that these three beams reappear in their original colors demonstrates that light rays coming from different sources act independently of one another after being reflected by the mirror. Likewise, the fact that the light from the three spotlights appears white when they are all focused on the same area of paper can be explained in terms of the constituent light wavelengths (red, blue, and green) reaching our eyes and acting on our retinas independently. It is the superposition of waves which causes us to perceive them as white.
Figure 1.2 Independent action of light rays
1.2.3 Reflection of Light Rays
As shown in Figure 1.3a, when a light ray is reflected by a mirror at the point of incidence O, we can define the normal as an imaginary line through point O perpendicular to the mirror. The reflected ray will lie in the same plane as the incident ray and the normal to the mirror surface, and the angle of reflection will be the same as the angle of incidence. We are all familiar with this phenomenon from everyday experience. It can be described by the following equation:
1.1Figure 1.3 (a) Reflection of a light ray and (b) refraction of a light ray
1.2.4 Refraction of Light Rays
An object lying in a tub of water appears to be at a shallower depth than it actually is. This phenomenon can be explained by the refraction of light at the interface between the water and the air. As shown in Figure 1.3b, when a ray is refracted at a boundary plane between different media, the relationship between the angle of incidence and angle of refraction can be described by the following equation (Snell's law):
1.2where
n1 = Refractive index in medium 1 n2 = Refractive index in medium 2 ?i = Angle of incidence ?t = Angle of refraction.1.3 Fermat's Principle
The law of rectilinear propagation and the law of reflection and refraction of light rays can both be derived from Fermat's principle, as explained below [1].
- i. The velocity of light is inversely proportional to the refractive index of the medium in which light propagates. (In other words, light travels more slowly in a medium having a higher refractive index.)
The velocity of light in a vacuum is a constant, c:
1.3The velocity of light v in a medium having refractive index n is:
1.4In optical calculations, the optical path length L is defined as follows:
1.5where L0 = physical length traversed by light in the...
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