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Physics for Geologists, Second edition

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Optics 45<br />

know whether the light was at B or B1. The principle of reciprocity requires<br />

that light travelling in the reverse directions traverses the same paths. (Do<br />

not <strong>for</strong>get that light is going out from the point in all directions, but we only<br />

see that which arrives first.)<br />

In Figure 4.3, the light travels from a plane source AA1. When the ray from<br />

A reaches the interface at B, the remainder of the plane wave front BC still<br />

has some distance to travel in air while the ray at B continues in the other<br />

medium. The frequency of the plane wave remains the same, but its speed<br />

changes, so its wavelength also changes. In the time taken <strong>for</strong> the incident<br />

ray to travel from B' to C', the refracted ray travels a shorter distance (in<br />

this case) from B to C, and the direction of the wave front is altered. The<br />

refracted wave is parallel to CC1.<br />

When the incident light is in the medium with larger refractive index,<br />

smaller speed ci < c, (Figure 4.2(b)), the angle of refraction is larger than<br />

the angle of incidence. As the angle of incidence increases, so the angle of<br />

refraction increases until the refracted ray is in the plane of contact between<br />

the two media and the angle of refraction is 90". This angle of incidence is<br />

called the critical angle, i,, and at any angle of incidence greater than i, the<br />

ray is totally reflected. You can see this when diving. Looking upwards, you<br />

can see things above the surface; but there is an angle i, from the vertical<br />

greater than which the surface appears as a mirror - which indeed it is. Snell's<br />

law tells us that i, = sin-' ci/c, where ci is the speed of light in the denser<br />

medium and c, that in air. This is the inverse of the relationship that gives<br />

the refractive index, so i, = sin-' (lln). For water with a refractive index<br />

of 1.333, the critical angle is about 48.6". For very precise work we would<br />

have to take into account that the speed of light, c, is not quite the same in<br />

air as in a vacuum (the refractive index of air is 1.0002).<br />

Snell's Law applies to the reflection and refraction of sound and seismic<br />

waves as well (see page 107).<br />

Copyright 2002 by Richard E. Chapman<br />

Figure 4.3 Huygen's geometric construction of the refraction path, in section.<br />

When the wave-front AA' reaches BB', it begins to be refracted. The<br />

velocity in the lower medium is less than that in the above, so the<br />

wave only travels the distance BC in the time it takes the wave at B'<br />

to reach C'.

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