Laser Tracking on the CD Scaled Views of a Compact Disc

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which applies to both the parallel and perpendicular cases. Parallel case: Reflected % and transmitted %. Perpendicular case: Reflected % and transmitted %. Reflection and Transmission Internal Reflection Fresnel's equations describe the reflection and transmission of electromagnetic waves at an interface. That is, they give the reflection and transmission coefficients for waves parallel and perpendicular to the plane of incidence. For a dielectric medium where Snell's Law can be used to relate the incident and transmitted angles, Fresnel's Equations can be stated in terms of the angles of incidence and transmission. For light from a medium of index = incident upon a medium of index = at an angle = ° the angle of transmission is = ° Fresnel's equations give the reflection coefficients:
= and = The transmission coefficients are = and = Note that these coefficients are fractional amplitudes, and must be squared to get fractional intensities for reflection and transmission. You can choose values of parameters which will give transmission coefficients greater than 1, and that would appear to violate conservation of energy. (For example, try light incident from a medium of n 1 =1.5 upon a medium of n 2 =1.0 with an angle of incidence of 30°.) But the square of the transmission coefficient gives the transmitted energy flux per unit area (intensity), and the area of the transmitted beam is smaller in the refracted beam than in the incident beam if the index of refraction is less than that of the incident medium. When you take the intensity times the area for both the reflected and refracted beams, the total energy flux must equal that in the incident beam. For further details, see Jenkins and White. Checking out conservation of energy in this situation leads to the relationship which applies to both the parallel and perpendicular cases. Parallel case: Reflected % and transmitted %. Perpendicular case: Reflected % and transmitted %. Blue Sky The blue color of the sky is caused by the scattering of sunlight off the molecules of the atmosphere. This scattering, called Rayleigh scattering, is more effective at short wavelengths (the blue end of the visible spectrum). Therefore the light scattered down to the earth at a large angle with respect to the direction of the sun's light is predominantly in the blue end of the spectrum.
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Laser Tracking on the CD Scaled Views of a Compact Disc

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