Diffraction grating

From Academic Kids

Missing image
A huge diffraction grating.

In optics, a diffraction grating is an array of fine, parallel, equally spaced grooves ("rulings") on a reflecting or transparent substrate.

When photons (electromagnetic energy) encounter a diffraction grating, diffractive and mutual interference effects occur. Photons are reflected or transmitted in discrete directions, called "orders," or "spectral orders."

Because the angle of deviation of the diffracted beam is wavelength-dependent, a diffraction grating separates the incident beam spatially into its constituent wavelength components, i.e., it is dispersive. Each component of the electromagnetic spectrum is sent into a different direction, producing a rainbow of colors. This is visually similar to that produced by a prism, though the mechanism is very different.

The groove dimensions and spacings are on the order of the wavelength in question. In the optical regime, in which the use of diffraction gratings is most common, there are many hundreds, or thousands, of grooves per millimeter.

Order zero corresponds to direct transmission or specular reflection. Higher orders result in deviation of the incident beam from the direction predicted by geometric (ray) optics. With a normal angle of incidence, the angle θ, the deviation of the diffracted ray from the direction predicted by geometric optics, is given by the following equation, where m is the spectral order, λ is the wavelength, and d is the spacing between corresponding parts of adjacent grooves:

<math>\theta = \pm \sin^{-1} \left( {m \lambda \over d} \right)<math>

The spectral orders produced by diffraction gratings may overlap, depending on the spectral content of the incident beam and the number of grooves per unit distance on the grating. The higher the spectral order, the greater the overlap into the next-lower order.

By controlling the cross-sectional shape of the grooves, it is possible to concentrate most of the diffracted energy in the order of interest. This technique is called "blazing."

Originally high resolution diffraction gratings were ruled. The construction of high quality ruling engines was a large undertaking. A later photolithographic technique allows gratings to be created from a holographic interference pattern. Holographic gratings have sinusoidal grooves and so are not as bright, but are preferred in monochromators because they lead to a much lower stray light level than blazed gratings. A copying technique allows high quality replicas to be made from master gratings, this helps to lower costs of gratings.

Another method of producing diffraction gratings uses a photosensitive gel sandwitched between two substrates. A holographic interference pattern exposes the gel which is later developed. These gratings, also called volume phase holograpy (VPH) diffraction gratings have no physical grooves, but instead a periodic modulation of the refractive index within the gel, removing much of the surface scattering effects typically seen in other types of gratings. VPH gratings tend to have higher grating efficiency, and allow for inclusion of complicated patterns into one grating.


Diffraction gratings are often used in monochromators and other optical instruments.

Ordinary pressed CD and DVD media are every-day examples of diffraction gratings and can be used to demonstrate the effect by shining an ordinary laser pointer onto the surface. This is a side effect of their manufacture, as they have a thin layer of aluminium with regular grooves pressed into it in a spiral pattern.

Diffraction gratings are also present in nature. For example, the iridescent colors of peacock feathers, mother-of-pearl, and some insects are caused by very fine regular structures that diffract light, splitting it into its component colors.

Source: adapted from a public domain entry in Federal Standard 1037C.

2. National Optical Astronomy Observatories entry regarding VPH gratings.da:Diffraktivt gitter (optisk) de:Beugungsgitter ja:回折格子 nl:Tralie (natuurkunde) pl:Siatka dyfrakcyjna fr:Rseau de diffraction


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