Download Handbook of Optics by Michael Bass, Carolyn MacDonald, Guifang Li, Casimer M. PDF
By Michael Bass, Carolyn MacDonald, Guifang Li, Casimer M. DeCusatis, Virendra N. Mahajan
V. 1. Geometrical and actual optics, polarized mild, elements and tools -- v. four. Optical homes of fabrics, nonlinear optics, quantum optics -- v. five. Atmospheric optics, modulators, fiber optics, X-ray and neutron optic
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Optical fiber technology is truly an interdisciplinary field, incorporating aspects of solid-state physics, material science, and electrical engineering, among others. In the section on fiber optics, we introduce the fundamentals of optical fibers and cable assemblies, optical connectors, light sources, detectors, and related components. Assembly of the building blocks into optical networks required discussion of the unique requirements of digital versus analog links and telecommunication versus data communication networks.
2 is representative of the most common instrument configuration in use. The source is fixed in position. The sample is rotated to the desired incident angle, and the receiver is rotated about the sample in the plane of incidence. Although dozens of instruments have been built following this general design, other configurations are in use. For example, the source and receiver may be fixed and the sample rotated so that the scatter pattern moves past the receiver. This is easier mechanically than moving the receiver at the end of an arm, but complicates analysis because the incident angle and the observation angle change simultaneously.
The aperture at the front of the receiver determines the solid angle over which scatter is gathered. Any light entering this aperture that originates from within the FOV will reach the detector and become part of the signal. This includes instrument signature contributions scattered through small angles by the source optics. It will also include light scattered by the receiver lens so that it appears to come from the sample. The configuration in Fig. 3a can be used to obtain near specular measurements by bringing a small receiver aperture close to the focused specular beam.