<<

n 1.33 sin θ = sin θ = sin 35◦ , air n water 1.00 air   i.e.

◦ θair = 49.7 .

Thus, the height above the horizon is

◦ ◦ θ = 90 θair = 40.3 . (4.7) − Because the is far away from the fisherman and the diver, the fisherman will see the sun at the same angle above the horizon.

4.4 Total Internal Reflection

Suppose that a moves from a medium of n1 to one in which n1 > n2, e.g. -to-air, where n1 = 1.50 and n2 = 1.0003. ◦ If the angle of incidence θ1 = 10 , then by Snell’s law, •

n 1.50 θ = sin−1 1 sin θ = sin−1 sin 10◦ 2 n 1 1.0003  2    = sin−1 (0.2604) = 15.1◦ .

◦ If the angle of incidence is θ1 = 50 , then by Snell’s law, •

n 1.50 θ = sin−1 1 sin θ = sin−1 sin 50◦ 2 n 1 1.0003  2    = sin−1 (1.1487) =??? .

◦ So when θ1 = 50 , we have a problem:

Mathematically: the angle θ2 cannot be computed since sin θ2 > 1. •

142 Physically: the ray is unable to refract through the boundary. Instead, • 100% of the light reflects from the boundary back into the .

This process is known as total internal reflection (TIR).

Figure 8672 shows several rays leaving a point source in a medium with re- fractive index n1.

Figure 86: The and reflection of light rays with increasing angle of incidence.

The medium on the other side of the boundary has n2 < n1. • Crossing the boundary from a medium of higher to lower refractive index • causes the ray to bend away from the .

72Knight, Figure 23.22, page 725

143 Two things happen as the angle θ1 increases: •

– The angle of refraction approaches 90◦.

– The fraction of light that is transmitted decreases, while that of the reflected ray increases.

So in the above case where n1 > n2, there must exist some critical angle,

θc, at which the refracted ray vanishes and the reflected ray becomes 100% for all θ1 θc. ≥

◦ This critical angle corresponds to when θ2 = 90 ; by Snell’s law,

n n θ = sin−1 2 sin 90◦ = sin−1 2 . (4.8) c n n  1   1 

Note: the existence of this critical angle is only true when n1 > n2. If n1 < n2, there is no critical angle, and hence no TIR

So for the above case of a glass/air boundary, if n1 = 1.50 and n2 = 1.0003, then from (4.8),

1.0003 θ = sin−1 = 42◦ . c 1.50  

◦ The fact that θc < 45 for the glass/air boundary has important applications. For example, in (figure 8773):

the are much further apart than your , so the light rays need • to be brought together before exiting the .

Instead of using , binoculars use a pair of on each side – • the light undergoes two TIR and emerges from the .

73Knight, Figure 23.23, page 725

144

Figure 87: The use of total internal reflection in binoculars.

4.4.1 Application of TIR: Fibre

The transmission of light through optical fibres provides arguably the most important application of TIR.

Figure 8874 shows a beam entering one end of a narrow-diameter glass tube. Light ray from laser beam passes easily from air into the glass fibre. • The ray hits the boundary – i.e. inside wall of the tube – at an angle of • ◦ incidence θ1 which approaches 90 .

74Knight, Figure 23.25(a), page 726

145 Figure 88: The use of total internal reflection in an optical fibre.

Since θ1 > θc, the light ray undergoes TIR and remains inside the tube. • The light ray undergoes a series of total internal reflections as it moves • down the fibre.

◦ By the time the ray reaches the end of the fibre, θ1 0 < θc, and the • ≈ ray refracts out of the fibre, and is easily detected.

Practical optical fibres (figure 8975) consist of a glass surrounded by a layer of cladding.

The cladding protects the glass surface from scratches, etc., that can • alter the angle of incidence.

The cladding has a refractive index nclad < ncore, so the light ray under- • goes TIR at the boundary, and remains confined to the tube.

Note: realistically, there is always some of light by the glass tube – no glass is perfectly transparent.

75Knight, Figure 23.25(b), page 726

146