DWDM

Chapter 2 - Optical Components

2
OPTICAL COMPONENTS

 

2.1 INTRODUCTION

DWDM systems require specialized optical and photonic components that are based on light-matter and light-matter-light interactions as well as on the propagation properties of light. The optical components deployed in communications systems provide an equivalent functionality of their electrical or electronic counterparts. Such components are transformers (Fourier lens), transmitters, receivers, filters, modulators, amplifiers, add-drop multiplexers, cross-connect, couplers, and so on. In this chapter we provide a thorough description of the critical optical components that are used in the design of DWDM systems.

2.1.1 Geometrical Optics

The earliest optical components used for scientific and commercial purposes were lenses and mirrors. Ancient mathematicians, geometers, and astronomers, such as Apollonios of Perga (3rd c. B.C.), Diocles of Carystos (3rd c. B.C.), Eudoxos of Cnidos (5th-4th c. B.C.), Hipparchos of Nicaea (2nd c. B.C.), Zenodoros of Athens (ca. 3rd-2nd c. B.C.) and others, studied the propagation and reflectivity of light and developed the theory of spherics; they also discovered the focusing imperfection of spherical mirrors and corrected them with parabolic mirrors. In the centuries that followed, these and new theories along with the development of purer glass and tribology made it possible to manufacture better lenses in various shapes and sizes, which led to the development of reading glasses, microscopes, telescopes, and other scientific optical instruments. Depending on curvature, lenses are distinguished as plano-convex, convex-convex, plano-concave, concave-concave, convex-concave (or meniscus), and cylindrical (Fig. 2.1), as well as other specialized shapes.

Figure 2.1 Types of lenses (shown cross-section perpendicular to axis).

Instruments rarely consist of a single lens; they typically, consist of lens systems. Lens systems, depending on the function they perform, may be comprised of one or more lens types. Thus, telescope or microscope eyepieces differ from telescope objectives in lens size and composition. Thus, some lenses utilize a large area (aperture), whereas others use only that portion that is near their axis. Some lens systems are complex in order to correct image distortions caused by lens imperfections and by interaction of lens material with light such as spherical aberration, astigmatism, coma, pincushion (positive) or barrel (negative) distortion, lateral color aberration, dichroism, and so on. All these aberration types degrade either the quality and/or the power level of the optical signal. Consequently, image distortion-free lens systems have been for many years a serious design effort that has led a number of notable lens arrangements such as for example the Gauss, the Tessar, the Petzval, the Dogmar/Aviar, the Augulon/Biogon, and others.

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