The wavelets shown were emitted as each point on the wavefront struck the mirror. Huygens’s principle applied to a straight wavefront striking a mirror. The wavelets closer to the left have had time to travel farther, producing a wavefront traveling in the direction shown. As the wavefront strikes the mirror, wavelets are first emitted from the left part of the mirror and then the right. In addition, we will see that Huygens’s principle tells us how and where light rays interfere.įigure 3 shows how a mirror reflects an incoming wave at an angle equal to the incident angle, verifying the law of reflection. We will find it useful not only in describing how light waves propagate, but also in explaining the laws of reflection and refraction. Huygens’s principle works for all types of waves, including water waves, sound waves, and light waves. The new wavefront is a line tangent to the wavelets and is where we would expect the wave to be a time t later. These are drawn at a time t later, so that they have moved a distance s = vt. Each point on the wavefront emits a semicircular wave that moves at the propagation speed v. A wavefront is the long edge that moves, for example, the crest or the trough. The new wavefront is a line tangent to the wavelets.įigure 2 shows how Huygens’s principle is applied. Each point on the wavefront emits a semicircular wavelet that moves a distance. Huygens’s principle applied to a straight wavefront. The new wavefront is a line tangent to all of the wavelets. Starting from some known position, Huygens’s principle states that:Įvery point on a wavefront is a source of wavelets that spread out in the forward direction at the same speed as the wave itself. The Dutch scientist Christiaan Huygens (1629–1695) developed a useful technique for determining in detail how and where waves propagate. The direction of propagation is perpendicular to the wavefronts (or wave crests) and is represented by an arrow like a ray. A transverse wave, such as an electromagnetic wave like light, as viewed from above and from the side. The view from above is perhaps the most useful in developing concepts about wave optics. The side view would be a graph of the electric or magnetic field. From above, we view the wavefronts (or wave crests) as we would by looking down on the ocean waves. A light wave can be imagined to propagate like this, although we do not actually see it wiggling through space.
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