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Physics for Geologists, Second edition

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48 Optics<br />

only the light oscillating normal to the plane of incidence is reflected; the<br />

rest is refracted and partly polarized in the plane of incidence. If the incident<br />

light is polarized in the plane of incidence, none is reflected and the refracted<br />

light is polarized in the plane of incidence. If it is polarized normal to the<br />

plane of incidence, it is partly reflected at all angles of incidence and the<br />

refracted light remains polarized normal to the plane of incidence.<br />

Fresnel's reflection <strong>for</strong>mulae <strong>for</strong> the proportion of light reflected at various<br />

angles of incidence are, - tan (i - r)/ tan (i +Y) <strong>for</strong> light polarized in the plane<br />

of incidence, and - sin (i - r)/ sin (i + Y) <strong>for</strong> light polarized normal to the<br />

plane of incidence. These proportions are in terms of amplitudes of the light.<br />

When the incident light is polarized in the plane of incidence and the angle of<br />

incidence is Brewster's angle (i+r = 90°), no light is reflected. The coefficient<br />

of reflection is the ratio of the intensity of the reflected light to the intensity<br />

of the incident light, and the intensity is proportional to the square of the<br />

amplitude. So the coefficients of reflection are, <strong>for</strong> light polarized in the plane<br />

of incidence, tan2 (i - r)/ tan2 (i + r), and <strong>for</strong> light polarized normal to the<br />

plane of incidence, sin2 (i - r)/ sin2 (i + r). For unpolarized light, there is<br />

another <strong>for</strong>mula due to Fresnel:<br />

The coefficient of reflection <strong>for</strong> normal incident light on a transparent surface<br />

can be derived from these <strong>for</strong>mulae and is given by<br />

where n is the refractive index. The derivation uses the fact that when the<br />

angles i and r or (i - r) and (i + r) are very small, sin2 (i - r)/ sin2 (i + r) =<br />

tan2 (i - r)/ tan2 (i + r) x (i - ~ )~/(i + Y ) = ~ (n - ~ )~/(n + I )~.<br />

The blue sky is partly polarized, most strongly polarized at right angles<br />

to the direction of the Sun. This can be verified by looking at the blue sky<br />

through a polaroidTM filter (or one lens of polaroidTM sunglasses) and rotating<br />

it. The amount of light passing through the lens will vary in different<br />

parts of the sky and with different orientations of the polaroidTM filter. The<br />

Vikings knew this and used the polarizing mineral cordierite <strong>for</strong> navigation<br />

(even on a cloudy day, the position of the Sun can be estimated to 13", it is<br />

said). Bees can also detect polarized light and use it <strong>for</strong> navigation.<br />

We cannot distinguish the directions of vibration of light without assistance.<br />

If we pass ordinary light through a crystal of tourmaline that has been<br />

cut parallel to its principal axis, and then let it pass through another similar<br />

crystal, we find that the light emerging from the first crystal is polarized<br />

parallel to its axis. We use the second crystal to analyse the light emerging<br />

from the first, which we call the polarizer.<br />

Copyright 2002 by Richard E. Chapman

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