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Materials for the Science of Information
Technology are provided on-line, at no cost to the user, in the hope of
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Overview and Objectives
Optical fibers, also called fiber optics, are currently the primary conduit
of digital information. Telephone lines, cable TV lines, and computer
networks all take advantage of fibers' capacity to quickly carry large
amounts of information. Optical fibers make use of the physics principles
of reflection and refraction. This module first explains reflection and
refraction, then uses them to explain how optical fibers work.
Upon finishing this module, students should be able to
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State and apply the Law of Reflection. |
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Define the index of refraction for a medium, and use
it to calculate the speed and wavelength of light in that medium. |
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State, explain, and apply Snell's Law. |
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Define and calculate the critical angle for the interface
of two media. |
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Describe the basic structure and types of optical fiber
and explain how a fiber is able to guide light. |
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Define and calculate characteristics of step-index optical
fibers, such as numerical aperture and cut-off angle. |
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Prerequisites
Before starting this module, students should
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Be familiar with the concepts of wavelength, frequency,
and wave speed and how they relate to each other. (The
Physics Classroom Overview) |
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Be comfortable performing basic algebraic operations.
( Algebra.com
[Click on 'Lesson' to get a quick overview]) |
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Understand geometry and trigonometry as applied to right
triangles. (Wolfram Geometry
and Trigonometry) |
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Have familiarity with metric units of length and metric
prefixes. (Metric
Units and Conversions) |
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Technology
Requirements
In order to use this module, your browser should
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Recognize Unicode Greek letters: αβγ should
be alpha, beta, and gamma. (This will not work on older browsers such as
Netscape 4.) If you have difficulty viewing these, we have some
older versions of
materials available that use Symbol font for Greek letters: abg
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Have the Shockwave plugin. (Want to check? This
page contains a Shockwave animation of refraction.) (Download
Shockwave) |
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Display animated gifs. (Want to check? This
page contains an animated gif of reflection.) |
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Recognize Bookman Old
Style and
Comic Sans MS fonts
(these are Microsoft fonts and optional - purely aesthetic). |
To view the Guest Lecture,
you also need
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Internet Explorer on a PC and Windows Media Player.
(Apologies to the Mac users and anti-Microsoft purists,
but the video is in Microsoft Producer format and won't play in other environments.) |
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A reasonably fast connection to the Internet.
(Dial-up should work, but the buffering is sketchy and
can take a really long time. It can also lead to periodic
pauses in the playback. If you are forced to use dial-up, we recommend
letting the video download for some time before you play it. |
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Copyright
© 1999-2006 Doris Jeanne Wagner and Rensselaer Polytechnic Institute.
All Rights Reserved.