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Laser Tracking on the CD Scaled Views of a Compact Disc

Laser Tracking on the CD Scaled Views of a Compact Disc

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= and =<br />

The transmissi<strong>on</strong> coefficients are<br />

= and<br />

=<br />

Note that <strong>the</strong>se coefficients are fracti<strong>on</strong>al amplitudes, and must be squared to get fracti<strong>on</strong>al<br />

intensities for reflecti<strong>on</strong> and transmissi<strong>on</strong>.<br />

You can choose values <strong>of</strong> parameters which will give transmissi<strong>on</strong> coefficients greater than 1, and<br />

that would appear to violate c<strong>on</strong>servati<strong>on</strong> <strong>of</strong> energy. (For example, try light incident from a medium<br />

<strong>of</strong> n 1 =1.5 up<strong>on</strong> a medium <strong>of</strong> n 2 =1.0 with an angle <strong>of</strong> incidence <strong>of</strong> 30°.) But <strong>the</strong> square <strong>of</strong> <strong>the</strong><br />

transmissi<strong>on</strong> coefficient gives <strong>the</strong> transmitted energy flux per unit area (intensity), and <strong>the</strong> area <strong>of</strong><br />

<strong>the</strong> transmitted beam is smaller in <strong>the</strong> refracted beam than in <strong>the</strong> incident beam if <strong>the</strong> index <strong>of</strong><br />

refracti<strong>on</strong> is less than that <strong>of</strong> <strong>the</strong> incident medium. When you take <strong>the</strong> intensity times <strong>the</strong> area for<br />

both <strong>the</strong> reflected and refracted beams, <strong>the</strong> total energy flux must equal that in <strong>the</strong> incident beam.<br />

For fur<strong>the</strong>r details, see Jenkins and White.<br />

Checking out c<strong>on</strong>servati<strong>on</strong> <strong>of</strong> energy in this situati<strong>on</strong> leads to <strong>the</strong> relati<strong>on</strong>ship<br />

which applies to both <strong>the</strong> parallel and perpendicular cases.<br />

Parallel case: Reflected % and transmitted %.<br />

Perpendicular case: Reflected % and transmitted %.<br />

Blue Sky<br />

The blue color <strong>of</strong> <strong>the</strong> sky is caused by <strong>the</strong> scattering <strong>of</strong> sunlight <strong>of</strong>f <strong>the</strong> molecules <strong>of</strong> <strong>the</strong><br />

atmosphere. This scattering, called Rayleigh scattering, is more effective at short wavelengths (<strong>the</strong><br />

blue end <strong>of</strong> <strong>the</strong> visible spectrum). Therefore <strong>the</strong> light scattered down to <strong>the</strong> earth at a large angle<br />

with respect to <strong>the</strong> directi<strong>on</strong> <strong>of</strong> <strong>the</strong> sun's light is predominantly in <strong>the</strong> blue end <strong>of</strong> <strong>the</strong> spectrum.

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